8/19/13

MirmanHodgmanSchaal Sandwich-To-Go Tour

MirmanHodgmanSchaal Sandwich-To-Go Tour:
Eugene Mirman, John Hodgman, and Kristen Schaal
Team Up For Six-City Tour This October
Tickets on sale Friday, August 23 at 12pm

[August 19, 2013, New York, NY] – Comedians Eugene Mirman, John Hodgman, and Kristen Schaal will take to the road this October as they set off on their “MirmanHodgmanSchaal Sandwich-To-Go Tour” presented by AEG Live.  The tour will stop at six cities in six days, starting with the Keswick Theatre in Glenside, PA on October 15 and wrapping up at the Ohio Theatre in Cleveland, OH on October 20.

“John and Kristen are two of my favorite people to watch do comedy, travel with, and hopefully, if I play my cards right, cuddle with,” says Mirman of the tour.

The trio has shared the stage and the screen with Mirman and Schaal as regulars on the HBO series Flight of the Conchords, and Schaal and Hodgman as contributors on Comedy Central’s The Daily Show with Jon Stewart.  Currently Mirman and Schaal voice the characters “Gene” and “Louise” on Fox’s hit animated series Bob’s Burgers.  Hodgman also recently starred in his own Netflix special John Hodgman: Ragnarok.

“The MirmanHodgmanSchaal sandwich shall soon be among the most famous sandwiches in the United States,” says Hodgman.  “Much more famous than the Beef on Weck and Croque-Monsieur, but not as famous as the French Dip. GODDAMN YOU FRENCH DIP. STOP HOGGING THE LIMELIGHT.”

Adds Schaal: “Mirman, Hodgman and I have wanted to do this tour for awhile. We are so thrilled that it’s finally happening! Comedy connoisseurs! Come whet your appetites on this delicate, yet robust, and slightly aged sandwich of us! Your city, plus the three of us together will probably only happen once in all our lifetimes.”

Tickets for the “MirmanHodgmanSchaal Sandwich-To-Go Tour” will go on sale on Friday, August 23 at 12pm and will be available at AXS.com, Ticketmaster.com, or the venue box office.

The pre-sale password is “cheese”.

Oct 15             Glenside, PA               Keswick Theatre

Oct 16             Washington, DC         Lisner Auditorium

Oct 17             Royal Oak, MI            Royal Oak Music Theatre

Oct 18             Milwaukee, WI           Pabst Theater

Oct 19             Chicago, IL                 Vic Theatre

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Comments

  1. Marty says:

    I am so excited! This will be the second year in a row I get to see you and Kristen Schall for my birthday.

    August 19th, 2013 at 5:23 pm (#)

  2. Meghan says:

    No West Coast?? :(

    August 19th, 2013 at 7:46 pm (#)

  3. Amy says:

    Please come to Seattle!

    August 19th, 2013 at 7:46 pm (#)

  4. Natalie says:

    You guys should come down to Atlanta!

    August 19th, 2013 at 7:49 pm (#)

  5. Jim says:

    Texas is actually quite lovely in October. So we’ll see you in Dallas for the just-added seventh stop. Right? Right!

    August 19th, 2013 at 7:54 pm (#)

  6. Ross says:

    Let me throw in a second vote for Seattle :)

    August 19th, 2013 at 8:13 pm (#)

  7. Elliot says:

    Given modern technology, the Rocky Mountains aren’t as difficult to cross as you might think.

    August 19th, 2013 at 9:13 pm (#)

  8. @RedChesterfield says:

    Will there be bootlegs?

    August 19th, 2013 at 11:36 pm (#)

  9. Shane says:

    Third vote for Seattle! :D

    August 19th, 2013 at 11:46 pm (#)

  10. Sean Doanldson says:

    Please come to Toronto Ontario Canada!!

    August 20th, 2013 at 2:38 am (#)

  11. andrea says:

    ATLANTAAAAAAAAAA

    August 20th, 2013 at 4:21 am (#)

  12. Suzie says:

    Please record this and sell it to me. Or come to Portland, OR.

    August 20th, 2013 at 4:21 am (#)

  13. Rick Urban says:

    Please come to Atlanta!

    August 20th, 2013 at 4:05 pm (#)

  14. Janet says:

    Raleigh, NC !!!!!

    August 21st, 2013 at 7:41 pm (#)

  15. davebo says:

    I’ll be there AND I’ll be square!

    August 22nd, 2013 at 3:55 am (#)

  16. TJ says:

    There’s not even a show I can drive too… Lots of Fans here in Oklahoma. Head out here somewhere. Just make sure your tour bus driver is sober, or you might get arrested like 2 Chains did last night. Maybe try 1 chain. See if that works.

    August 22nd, 2013 at 7:26 pm (#)

  17. Kayla says:

    Atlanta, please!

    August 22nd, 2013 at 8:10 pm (#)

  18. Chris says:

    Lordy lordy! I wish it was coming to Portland, OR.

    August 22nd, 2013 at 9:31 pm (#)

  19. John Hodgman graces Lisner Auditorium in October | NerDC.net says:

    [...] out more at http://eugenemirman.com. Like this:Like Loading… Posted by: Robert B // Events, Happenings, Live Performance, News [...]

    August 23rd, 2013 at 11:56 am (#)

  20. Tony says:

    Yes! Portland! We love you.

    August 23rd, 2013 at 5:02 pm (#)

  21. Beth says:

    Los Angeles needs you!!!

    August 24th, 2013 at 12:35 am (#)

  22. jsb says:

    “Whet” your appetites. Not wet.

    August 26th, 2013 at 12:16 pm (#)

  23. cooper says:

    ATLANTA! plzkthxbai

    August 29th, 2013 at 8:11 pm (#)

  24. jan says:

    EUGENE PLEASE COME TO DENVER!

    September 11th, 2013 at 12:42 am (#)

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  27. Tracy says:

    What the hell, Mirman?!? You cancelled my show in beautiful, sunny Cleveland, City of the Gods and Rock n’ Roll. I tell you, sir, it shall not be so glorious the next time we meet. I shall train my rabbit to bite your ankles and steal your carrots. Then you shall never see the magnificence of Cleveland again! I still have to go, though, because my hotel tickets are non-refundable. I will probably end up seeing Sweeney Todd in a regional theatre production. Bah, Sweeney Todd!

    October 16th, 2013 at 12:15 pm (#)

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    September 20th, 2014 at 8:25 pm (#)

  273. Moncler 2014 says:

    The Arab Spring has also had a very significant impact on the United States’ relations in the region. The State Department is having now to build new relationships with a whole new generation of power brokers. One thing we can say for sure, this seismic shift is going to put pressure on and complicate U.S. support for Israel.Thirteen eligible men bid farewell to the Bachelor mansion and said hello to Atlantic City, N.J., Monday night to embark on the around-the-world portion of their quest to woo Bachelorette Desiree Hartsock.

    September 20th, 2014 at 8:25 pm (#)

  274. Supra TK Society For Hombre Supra TK Society For says:

    STORY WRITTEN FOR & USED WITH PERMISSIONPosted: October 6, 2006NASA managers met Thursday and agreed to relax a self-imposed post-Columbia daylight launch constraint, clearing the way for the shuttle Discovery’s liftoff Dec. 7, around 9:38 p.m. EST, on a complex space station assembly mission. It will be the first night shuttle launch since 2002.But agency managers attending a program requirements change board meeting reserved the option of requiring daylight launches for flights with external fuel tanks featuring significant design changes.One such proposed change is a modification of the tank’s so-called ice-frost ramps, aerodynamically shaped foam insulation used to prevent pre-launch ice buildups on fittings that support external pressurization lines and a cable tray.NASA and contractor engineers have been working on a redesign to reduce the amount of foam used to make the ice-frost ramps and thus minimize the possibility of debris shedding during ascent. But the ramps performed well during the past two missions and some engineers now favor leaving the design alone.Another meeting to discuss the topic is planned for early November.The ice-frost ramps are made up of foam poured into molds and then shaped by hand. Because the ramps are built up on top of already existing foam, engineers believed they were susceptible to temperature-induced cracks that could lead to in-flight debris shedding.The ramps were officially classified as “probable-catastrophic” prior to the last two shuttle missions. That means if no changes were made, one could expect a 50-50 chance of a catastrophic failure over the 100-flight design life of a space shuttle.Before mission STS-121 last July, NASA Administrator Mike Griffin said he did not agree with the probable-catastrophic designation and Discovery was cleared for flight as is. Likewise, Atlantis was cleared for launch last month on mission STS-115 with the understanding that a new ice-frost ramp design would be implemented as soon as possible.As it turned out, no significant ice-frost ramp damage or foam shedding was seen during the last two flights. An ongoing engineering analysis, based in part on in-flight video of the tank, indicates what foam does separate in flight comes off after the tank is out of the dangerous lower regions of the atmosphere.Going into Discovery’s flight last July, the odds of a catastrophic IFR failure were believed to be between 1-in-75 and 1-in-100. The odds currently are believed to be in the neighborhood of 1-in-575 or better, according to a senior manager familiar with the ongoing analysis. As such, the ramps likely will not be classified as probable-catastrophic for Discovery’s upcoming flight in December.At the Kennedy Space Center, meanwhile, engineers are assessing options for fixing a radiator panel mounted on the inside of the shuttle Atlantis’ right-side payload bay door. The panel apparently was damaged when a piece of space debris or a micrometeoroid slammed into the radiator, presumably during the shuttle’s flight last month, blasting .108-inch-wide hole in the upper surface and destroying the aluminum honeycomb material below before exiting the other side.The impact did not threaten the crew and the damage can be repaired. But it illustrates the danger posed by micrometeoroid/orbital debris (MMOD) and the reason why NASA considers such strikes a high risk. The odds of a catastrophic impact-related entry failure range between 1-in-210 to 1-in-350, depending on whether the astronauts inspect the ship in orbit prior to re-entry.At orbital velocities, even tiny pieces of debris pose a serious threat. An aluminum sphere just .4 inches across moving at 10 kilometers per second, or 22,370 mph, carries the same impact energy as a bowling ball moving at 300 mph.A preliminary engineering analysis shows the impact in question was one of the most significant instances of MMOD damage in shuttle history, second only to a cargo bay door impact during shuttle mission STS-72 in 1996.The shuttle’s 60-foot-long payload bay doors each feature four radiator panels that are exposed to space once the doors are opened in orbit. The forward two radiator panels measure about one inch thick, feature Freon coolant tubes positioned about 1.9 inches apart and can pivot to radiate from both sides. The aft panels are fixed and only radiate from one side. They measure a half inch thick and feature coolant tubes separated by about 5 inches. The interior of the panels is made up of an aluminum honeycomb material.The impact on Atlantis’s right-side, or starboard, radiator was found roughly midway between two coolant lines on panel No. 4. The object blasted a .108-inch-wide hole and presumably broke apart on impact. The resulting spray of debris created a cone-shaped damage cavity immediately below the face plate, destroying the honeycomb interior to the full half-inch depth of the panel. The lower face sheet was pushed out in two places. A .26-inch crack and a .03-inch-wide exit hole were found.As part of NASA’s post-Columbia safety protocols, the shuttle and space station fly in an orientation that protects the shuttle’s critical wing leading edge panels from direct, worst-case impacts in the line of flight. In addition, the astronauts now carry out detailed inspections of the shuttle’s heat shield after reaching orbit and again before re-entry to make sure no MMOD impacts occurred during the course of the mission.Areas of the shuttle that are not critical for re-entry are not inspected and the damage to Atlantis’s radiator panel No. 4 was not discovered until post-flight servicing at the Kennedy Space Center.A senior NASA manager said the impact damage was unlikely to prompt a change in the shuttle’s orbital orientation. He said program managers understand the radiator panels and cockpit windows face a higher risk of impact damage because of the shuttle’s orientation. But he said the risks associated with wing leading edge impacts are more severe.The shuttle has two Freon coolant loops and while the loss of one would force a crew to return to Earth at the next available U.S. landing site, computer software is in place to immediately isolate a leak even if the event occurred when the crew was asleep or otherwise occupied. Assuming a leak was quickly isolated, the astronauts could implement contingency procedures and press ahead with a near-normal mission despite the damage to one radiator panel.As for an impact on the shuttle’s cockpit windows, engineers do not yet know if the debris in question would have penetrated the thick multi-pane glass. The three panes making up the six forward cockpit windows have a combined thickness of 2.55 inches. The three panes making up each overhead window have a combined thickness of 1.58 inches.Some 11,000 objects 3.9 inches in diameter or greater are currently tracked by Air Force radars and optical systems. About 100,000 objects are believed to be present that are between .39 inches across and 3.9 inches in diameter. Most of those are not tracked and pose a threat to spacecraft in low-Earth orbit and to communications and weather satellites in higher orbits.Final Shuttle Mission PatchFree shipping to U.S. addresses!The crew emblem for the final space shuttle mission is now available in our store. Get this piece of history!STS-134 PatchFree shipping to U.S. addresses!The final planned flight of space shuttle Endeavour is symbolized in the official embroidered crew patch for STS-134. Available in our store!Ares 1-X PatchThe official embroidered patch for the Ares 1-X rocket test flight, is available for purchase.Apollo CollageThis beautiful one piece set features the Apollo program emblem surrounded by the individual mission logos.Project OrionThe Orion crew exploration vehicle is NASA’s first new human spacecraft developed since the space shuttle a quarter-century earlier. 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    September 20th, 2014 at 8:36 pm (#)

  275. Ray Ban Junior says:

    SPACE FLIGHT EXPERIENCE: Tanner flew aboard the Space Shuttle Atlantis on the STS-66, November 3-14, 1994, performing the Atmospheric Laboratory for Applications and Science-3 (ATLAS-3) mission. ATLAS-3 was the third in a series of flights to study the Earth’s atmosphere composition and solar effects at several points during the Sun’s 11-year cycle. The mission also carried the CRISTA-SPAS satellite that was deployed to study the chemical composition of the middle atmosphere and retrieved later in the mission. Tanner logged 262 hours and 34 minutes in space and 175 orbits of the Earth.

    September 20th, 2014 at 8:36 pm (#)

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    STORY WRITTEN FOR & USED WITH PERMISSIONPosted: December 17, 2006Faced with an unforgiving space station assembly sequence, NASA managers were forced to shoehorn an additional spacewalk into Discovery’s mission to complete the retraction of a recalcitrant solar array. The spacewalk came at the expense of a landing weather contingency day but it was either that or give up a post-undocking heat shield inspection, an option many shuttle engineers were reluctant to consider.The issue illustrates the difficulty NASA managers may face balancing flight safety with schedule pressure resulting from the Bush administration’s 2010 deadline for completing the international space station and retiring the shuttle. That somewhat arbitrary deadline leaves NASA little maneuvering room when it comes to dealing with unexpected problems like the partially retracted solar array that has disrupted the Discovery crew’s schedule.In this case, NASA’s options are limited by the amount of hydrogen and oxygen the shuttle can carry to generate electricity and a pre-launch decision to add a docked day to the flight because of the mission’s complexity and the possibility a day would be needed to correct problems activating the lab’s permanent power system.As such, Discovery’s flight is classified as a 12-plus-zero-plus-two-day mission, i.e., a 12-day flight with two weather contingency days. There is not be enough hydrogen and oxygen on board to extend the mission itself beyond 12 days and still preserve two backup landing days.NASA went into Discovery’s flight with an understanding that the post-undocking heat shield checkout could be taken off the table if the astronauts had problems with the space station electrical work that might require an additional spacewalk. Late inspection, in fact, did not even show up on a list of pre-flight mission priorities.This was not an issue under the original flight plan, which called for undocking Monday, late inspection Tuesday and a landing Thursday at the Kennedy Space Center, with Friday and Saturday as weather backups. But the flight plan was thrown into disarray when the astronauts ran into problems retracting a solar array on the international space station.NASA engineers concluded the P6-4B solar array could be safely left in its partially deployed state for several months, but it had to be dealt with eventually. The P6 array, which provided interim power during the lab’s initial assembly, is scheduled to be moved to the left end of the station’s main solar power truss in September and it cannot be moved with either of its two wings even partially extended.Only three options were available:Adding a spacewalk to Discovery’s mission to complete the retractionDeferring any repair attempt to the station crew after the shuttle’s departureDeferring the work to the next shuttle mission, assembly flight 13A, in MarchAdding a spacewalk to Discovery’s mission, it was believed, would force NASA to give up the late heat shield inspection. That was the going-in position when agency managers approved the 12-0-2 mission plan. But it soon became clear many in the post-Columbia shuttle program viewed the late inspection as a high priority regardless of where it ranked on NASA’s official list.At the same time, station managers were not keen to add a spacewalk to the three-person Expedition 14 crew’s already busy schedule. Spacewalks use the buddy system and a single astronaut would be required to stay inside and operate the retraction system as well as the space station’s big robot arm.”We’re choreographed pretty tightly now to get from here to assembly complete,” station Program Manager Mike Suffredini told reporters Saturday night. “And the next step for us as a program is to go into this stage where (the Expedition 14 crew has) three EVAs where we have to finish the reconfigurations … and hook up the lab to the central cooling system.”Adding a solar array repair spacewalk would require “arm operations, two crew outside, commanding the solar array,” Suffredini said. “That right there is at least four crew and you still haven’t talked about your (spacewalk coordinator) crew person we normally have for each EVA.”Station planners also were reluctant to add solar array repair work to the next shuttle assembly mission scheduled for March. During that flight, the other wing of the P6 array must be retracted and a new set of arrays installed.In the end, the MMT, chaired by John Shannon, decided Saturday to add a spacewalk to Discovery’s mission to resolve the matter sooner rather than later. To the surprise of many shuttle observers, however, the MMT opted to retain the late inspection, giving up one of the two available landing weather contingency day instead.NASA has three shuttle landing sites in the United States: The Kennedy Space Center in Florida, Edwards Air Force Base, Calif., and Northrup Strip in White Sands, N.M. Landings at Edwards add more than a week to a shuttle’s turnaround time. Only one shuttle mission ever ended at Northrup, in 1983, and it’s not clear how much time would be needed to get Discovery back from New Mexico.As it turns out, the landing site is not as much of an issue for Discovery as it might normally be. Whenever the orbiter gets back to Kennedy, it will be taken off flight status for a major inspection and overhaul. The shuttle Endeavour, coming out of its own orbiter maintenance and down period, or OMDP, will serve as the emergency rescue vehicle for the March shuttle flight.But Discovery’s next flight is STS-122, a high-priority mission scheduled for launch next October to carry the European Space Agency’s Columbus research module into orbit. While NASA likely could make up any lost time getting Discovery back to Florida, the schedule is tight and program managers don’t like to lose time on the front end of such an important processing flow.In any case, when only two landing days are available NASA flight rules require all three landing sites to be staffed and for the shuttle to come home on the first available opportunity.”With that day (Friday) being the day before the last opportunity – we have to be on the ground by Saturday – that means we’re going to call up all three landing sites, Edwards, KSC and Northrup, and our intent will be to put the vehicle on the ground somewhere that day at one of those sites,” said Phil Engelauf, a senior manager in the mission operations directorate at the Johnson Space Center.Engelauf said the unusual decision to give up a landing day turned on the importance many engineers attach to the late inspection, regardless of how it is officially classified. At orbital velocities, a 0.05-inch-wide piece of aluminum carries the kinetic energy of a 22-caliber long rifle bullet. The overall threat of a potentially catastrophic micrometeoroid strike, or an impact with space debris, is believed to be on the order of 1-in-250.The heat shield is photographed during launch and inspected in excruciating detail before docking. The late inspection is designed to spot any damage that might have occurred after that point, during the normal course of the mission.”It was a very complicated discussion and there were a lot of issues put on the table,” Engelauf said. “Since return to flight, we’ve spent a lot of time talking about MMOD (micrometeoroid/orbital debris), which is one of the top risks in the program. We have wing leading edge sensors and we’ve signed up to add late inspection to the missions. We do go through a process before the mission, placing the mission activities in relative priority and the late inspection is usually placed below those activities that would cost us reflight.”That means, he said, that NASA would give up late inspection in cases where a spacewalk or some other crew action could resolve a situation that otherwise might require another shuttle mission. That logic also would apply for an event that “might have a significant impact on the assembly sequence such that the next mission could not happen in its proper order or that we would have to change the sequence of the assembly because we had to redo an EVA task.”"Trading that particular element, the importance of MMOD risk and the importance of the inspection and the relative newness of that topic in the program … folks still believe that the priority to do that is extremely high,” Engelauf said.He agreed that NASA has never before “given up a landing opportunity for routine payload operations or other objectives.”"But this is not a routine objective,” he said. “This is a fairly significant impact to the subsequent flights that puts it back up into that regime of whether or not it falls above late inspection to do the solar array work. When we added all of those things up, MMOD risk is eventually a safety discussion. And talking about the probability of safely getting the vehicle back on the ground.”When you compare that to the landing-site-opportunity discussion, it’s a schedule risk issue, whether or not you’re going to get to a preferred landing site and whether there’s going to be a schedule implication. The program managers spent a lot of time thinking real hard about this decision and the ultimate conclusion was we wanted to protect the safety issue of late inspection over the schedule issue.”Against that backdrop is the overriding drive to complete the station by 2010. Given a tight schedule and limited resources, NASA does not have the leeway it once did to handle unexpected problems. But Engelauf said safety would always trump any perceived schedule pressure.”There is a constant awareness and people are continuously on the lookout for situations where we could feel like there’s pressure to do something that might be not in the best interest of safety of the program,” he said. “I think in this particular case, all of those decisions were, in fact, put on the table, all of those decisions were talked about and there was pretty unanimous support for the decision we came up with. I don’t recall anybody bringing up a dissenting opinion.”As for the 2010 deadline, “that’s not worth debating from my perspective,” he said. “It is what it is. We are charged with executing this program with the tools that we have and I think the community is really doing an outstanding job of vigilance, of making good, safe and well-considered decisions independent of the other deadline issues.”In the end, he said, “I think we’ve got a good workable plan, we think we’ve minimized the risk to both programs. We have incurred, I think, some programmatic schedule risk that we’re going to put the orbiter at a landing site that might cost us a little bit more turnaround time. But we think the bigger picture trade warrants that, given the significance of getting this array retracted for station and what that means to the rest of the sequence.”Video coverage for subscribers only:VIDEO:WIDESCREEN VIEW FROM PLAYALINDA BEACH TRACKER VIDEO:DISCOVERY’S LAUNCH THROUGH FUEL TANK SEPARATION VIDEO:SHORT CLIP OF DISCOVERY BLASTING OFF VIDEO:ASTRONAUTS DEPART QUARTERS FOR PAD VIDEO:CREW FINISHES DONNING SPACESUITS VIDEO:ASTRONAUTS IN DINING ROOM VIDEO:TIME-LAPSE MOVIE OF PAD GANTRY ROLLBACK VIDEO:LONGER LENGTH MOVIE OF THE SCRUB VIDEO:SCRUB CALLED DUE TO LOW CLOUDS VIDEO:ASTRONAUTS DEPART QUARTERS FOR PAD VIDEO:CREW FINISHES DONNING SPACESUITS VIDEO:ASTRONAUTS IN DINING ROOM THURSDAY VIDEO:PAD’S ROTATING SERVICE STRUCTURE ROLLED BACK VIDEO:POST-ARRIVAL COMMENTS FROM THE CREW VIDEO:ASTRONAUTS ARRIVE IN WAVE OF T-38 JETS VIDEO:BIOGRAPHIES OF THE DISCOVERY ASTRONAUTS VIDEO:NARRATED STS-116 MISSION PREVIEW MOVIE VIDEO:WEDNESDAY’S SHUTTLE BRIEFING IN ITS ENTIRETY BRIEFING SOUNDBITES:VIDEO:THE ISSUES DISCUSSED AT FRR VIDEO:NOT YOUR FATHER’S FRR VIDEO:READY TO RESUME NIGHT LAUNCHES VIDEO:LAUNCH PREPS PROCEEDING WELL VIDEO:YEAR-END ROLLOVER CONCERNS VIDEO:REASSESSING TANK FOAM RISK VIDEO:STATION SOLAR ARRAY DRIVE SYSTEM PROBLEM VIDEO:PRESSURIZATION PRECAUTIONS AT THE PAD VIDEO:OVERVIEW OF STS-116 MISSION VIDEO:SHUTTLE/ISS PROGRAM PERSPECTIVE VIDEO:PREVIEW OF MISSION’S SPACEWALKS VIDEO:ASTRONAUTS’ PRE-FLIGHT NEWS BRIEFING VIDEO:COVERAGE OF PRACTICE COUNTDOWN ACTIVITIES VIDEO:DISCOVERY ROLLS TO THE PAD VIDEO:DISCOVERY MATED TO TANK AND BOOSTERS VIDEO:SHUTTLE HOISTED VERTICALLY INSIDE VAB VIDEO:DISCOVERY HAULED FROM HANGAR TO VAB VIDEO:PORT 5 TRUSS PAYLOAD PACKED UP VIDEO:CREW VISITS KENNEDY SPACE CENTER VIDEO:EXTERNAL FUEL TANK MATED TO BOOSTERS MORE: John Glenn Mission PatchFree shipping to U.S. addresses!The historic first orbital flight by an American is marked by this commemorative patch for John Glenn and Friendship 7.Final Shuttle Mission PatchFree shipping to U.S. addresses!The crew emblem for the final space shuttle mission is available in our store. Get this piece of history!Celebrate the shuttle programFree shipping to U.S. addresses!This special commemorative patch marks the retirement of NASA’s Space Shuttle Program. Available in our store!Anniversary Shuttle PatchFree shipping to U.S. addresses!This embroidered patch commemorates the 30th anniversary of the Space Shuttle Program. The design features the space shuttle Columbia’s historic maiden flight of April 12, 1981.Mercury anniversaryFree shipping to U.S. addresses!Celebrate the 50th anniversary of Alan Shephard’s historic Mercury mission with this collectors’ item, the official commemorative embroidered patch.Fallen Heroes Patch CollectionThe official patches from Apollo 1, the shuttle Challenger and Columbia crews are available in the store. | | | | 2014 Spaceflight Now Inc.Discovery astronauts arrive at the Cape for launch BY WILLIAM HARWOOD

    September 20th, 2014 at 8:37 pm (#)

  277. The North Face says:

    STORY WRITTEN FOR & USED WITH PERMISSIONPosted: July 9, 2006After around-the-clock analysis, NASA managers today officially gave the shuttle Discovery’s heat shield a clean bill of health, concluding there are no problems with tiles, the ship’s nose cap or wing leading edge panels that require any repair work by the astronauts.It was a long awaited moment for thousands of NASA and contractor engineers and managers who have put in long hours since Discovery’s last flight to correct potentially catastrophic problems with foam insulation.As it turned out, Discovery’s external tank lost less foam than any tank before it and the orbiter suffered virtually no impact damage or other serious problems with its fragile heat shield.Discovery’s crew was given the news just before bedtime, after engineers worked through the night to resolve questions about a protruding gap filler and tears in two small insulation blankets.”So with that, we’ve closed out all issues on the TPS (thermal protection system) and we deem the TPS as 100 percent cleared for entry,” astronaut Lee Archambault radioed from mission control.”Well, that is great news, that’s fantastic,” replied Discovery commander Steve Lindsey. “To get all that done by the end of flight day six, when we did focused inspection on flight day four, is just amazing. So our thanks to the imagery team, the MMT and all the engineers working on this to get the vehicle cleared this quickly. That’s very impressive.”"Everyone here around the room as you can imagine is most happy,” Archambault said. “I think you’ll be delighted when you see the images that you guys sent down after you get back. They really were amazing.”Flight controllers were equally wowed by stunning movies shot by cameras mounted in the shuttle’s twin solid-fuel boosters. The rocketcam videos made it back to the Johnson Space Center today, providing engineers with never-before-seen views of launch and booster separation. The giant solid-fuel rockets performed normally, officials said today, with no problems of any significance.John Shannon, chairman of NASA’s Mission Management Team, said he remains optimistic NASA will resolve the few problems that have cropped up during Discovery’s flight in time to launch the shuttle Atlantis Aug. 28 on a space station assembly mission, the first shuttle construction flight since Columbia went down in 2003.”This has really been two missions for us,” he said. “The first was to go and do … a lot of things to assess orbiter health and potential repair capabilities. The other piece of it that’s just as important is what we have done for the space station.”We’ve talked a lot about how wonderful the orbiter looks and how well the external tank performed and how good the boom was. But I don’t want to lose sight of the other half of this, which is how much we’re doing to get ourselves ready in August for beginning the assembly of the space station again.”The August mission depends on the success of a spacewalk Monday by astronauts Piers Sellers and Mike Fossum to repair a stalled robot arm transporter on the station’s solar array truss. The robotic transporter is required to move the station’s robot arm from work site to work site on the unfinished truss and until it is fixed, station assembly is on hold.Last December, a spring-loaded cable cutter inadvertently fired, severing one of two power and data cables leading to the transporter. Sellers and Fossum plan to replace the cable reel mechanism Monday during a tricky make-or-break spacewalk.”We need that thing to be working, to move big pieces around during the assembly,” Sellers said today. “Right now, it’s dead on one side. Our job (Monday) is basically to replace the unit that supplies power to the truck so it can be ready for the next stage of assembly. It’s important to get that done before the next guys show up.”A third spacewalk is on tap Wednesday to test wing leading edge repair techniques. Engineers briefly worried the astronauts might have to pluck a protruding gap filler from Discovery’s belly during the third excursion, but Steve Poulos, manager of the orbiter projects office at the Johnson Space Center, said today a detailed analysis showed Discovery can safely re-enter the atmosphere as is.”Nobody had any concerns whatsoever we were going to exceed any of their limits,” he said. “We had no dissension across the entire community, everybody was 100 percent on board.”Gap fillers are thin, heat-resistant spacers between tiles to prevent chafing during the vibrations and temperature extremes of launch and orbital flight. Some 16,000 gap fillers are in place, including more than 5,000 that were replaced in wake of Discovery’s flight last summer on the first post-Columbia mission.Gap fillers can occasionally shake loose and if they stick up too far into the air stream during re-entry, they can break up the smooth flow across the belly of the shuttle, creating turbulence that can raise downstream temperatures.During Discovery’s approach to the space station earlier this week, engineers saw a gap filler sticking up from tiles near a propellant feedline access door. The high-resolution photography by the station’s crew showed the gap filler was damaged and creased.Poulos said engineers conducted tests showing the gap filler most likely will roll over in the re-entry air stream. But even if it doesn’t, testing showed Discovery is in no danger of excessive heating.During a normal re-entry, the tiles in that area should not experience temperatures higher than 2,300 degrees at their surface, more than 625 degrees at the bondline where they attach to the shuttle’s skin and 350 degrees for the aluminum skin itself.In a worst-case scenario, Poulos said, one in which the protruding access door gap filler disturbed the insulating “boundary layer” just after atmospheric entry at 24.7 times the speed of sound, temperatures on the tile surface would not exceed 2,254 degrees. The bondline temperatures would not rise above 579 degrees and the shuttle’s skin down stream of the gap filler would not get hotter than about 344 degrees.If the gap filler rolls over like engineers expect, tripping the boundary layer around 19.5 times the speed of sound, conditions will be even more benign: 2,254 degrees at the downstream tile surface; 496 degrees at the bondline; and 289 degrees on the skin.”With all that data, we were able to clear that gap filler as a non constraint for entry,” he said.Engineers worked one other open item overnight, conducting tests and computer analyses to show two small, damaged thermal blankets near the shuttle’s nose will not pull off during entry and pose an impact threat to Discovery’s cockpit windows or other areas.Testing showed the blankets would not begin to peel away unless relatively large “loads” were applied – more than five pounds of pull. The testing and computer analysis showed the blankets would experience no more than about 0.9 pounds of loading during entry.”In my terminology, not only did the team pound these issues flat, they put a dimple in the board when it was all said and done,” Poulos said. “So we are absolutely clear and ready to bring this vehicle home whenever the mission is accomplished.”In one minor correction, Shannon said additional analysis showed a piece of foam insulation that peeled off Discovery’s external tank during launch weighed just .055 pounds instead of .11 pounds as he earlier reported. 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    ちょっとそこ!これがあなたのブログに私の最初の訪問です!ボランティアのコレクションチームグループと新しい開始|同じニッチのコミュニティにおける主導のプロジェクトを私たちはいる。作業する情報はあなたのブログは私たちに便利な価値あるを提供しました。仕事には、特別素晴らしい素晴らしいを行っている!

    September 20th, 2014 at 10:14 pm (#)

  341. 靴市場 says:

    あなたのためにサイトブログあなたは記事の作家を探しているなら、私に知らせてください。 記事と私は|あなたはいくつかの本当に良い素晴らしいを持つ感じ私は良い資産になる。戻って鉱山へのリンクと引き換えにあなたのブログのための記事コンテンツ素材いくつかの書き込みにあなたがこれまで負荷の一部を取るしたい場合は、私が本当に似絶対に愛すると思います。 シュートしてください私にメール興味あれば。 ありがとうござい!

    September 20th, 2014 at 10:15 pm (#)

  342. 激安スニーカーブーツ says:

    うーん、それがようだあなたのように食べた私の最初のコメント(それがあった極めて長い)ので、私はちょうど私が書いたと私は徹底的にあなたのブログを楽しんでい、と言う。私はあまりに志望のブログですライターが、私はまだ全部に新たなんだ。 提言あなたがいずれかを持っていますか、ブログライター初心者のために?私は確かに本当にと思い、それを感謝しています。

    September 20th, 2014 at 10:15 pm (#)

  343. クロムハーツ ピンキーリング says:

    私が仕事であったが、私のいとこは今日昨日25|アップルipadのiPad、それは私を盗んだ40日下垂足は、ちょうどので、彼女はYouTubeの感覚することができます。私と彼女は83景色を眺めることができますアップルipadは今破壊さ壊れされている。私は、これは知っているオフトピック完全に完全に完全にが、私は誰かとそれを共有していた!

    September 20th, 2014 at 10:15 pm (#)

  344. cole haan 靴 メンズ says:

    ヘイ!あなたは、Twitterを使用していますか? 大丈夫大丈夫私はそれがであるかどうあなたをフォローしたいと思います。私は間違いなく絶対によあなたのブログを楽しんで、新しい投稿を楽しみにしています。

    September 20th, 2014 at 10:15 pm (#)

  345. abcマート限定 ティンバーランド says:

    それはだかどうか|皆 に問題あなたのサイト。 の一部書かれたテキストのあなた投稿がオフに実行されている画面。 他人ことができますしてくださいフィードバックを提供、これは彼らに何が起こっているなら、私に知らせて同様に?私はこれが起こる持っていたので、 これは可能性が前に以前、私と問題問題であること。 ありがとうございます

    September 20th, 2014 at 10:16 pm (#)

  346. toms worker says:

    エクセレントサイトあなたはここにあるが、私はした、任意の掲示板ここ|この記事にで議論|同じトピックをカバーフォーラムは}{の話? ご意見私が得ることができ、他からは私は本当に好き本当に愛したい個人。何か持っている場合は提言、私に知らせてください。 感謝!

    September 20th, 2014 at 10:16 pm (#)

  347. Paiement says:

    Oleh : Adzra??STPM dah nak dekat pun,masih nak keluar lagi?Ada baiknya Zara belajar.??Ayah seolah-olah melarangku keluar.??Kalau Zara cemerlang dalam STPM sekalipun,Zara tetap duduk kat ceruk dapur kan ???Tanyaku.Mula mencebik.Masih tersentap sebenarnya…

    September 20th, 2014 at 10:48 pm (#)

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    September 20th, 2014 at 10:49 pm (#)

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    September 20th, 2014 at 10:49 pm (#)

  351. UGG 5225 Ultra Short Botas says:

    Launch highlights from first Vandenberg’s Delta 4-Heavy. Credit: ULAA new strategy, being employed to reduce the hydrogen flames generated during startup of the three Aerojet Rocketdyne RS-68 main engines, will see the triple-body rocket light one engine two seconds before the other two. Counting down to liftoff at 10:52 a.m. local (1:52 p.m. EDT; 1752 GMT), the Terminal Countdown sequencer will take control at T-minus 10 seconds and the starboard engine begins to ignite at T-minus 7 seconds. Unburned hydrogen is released through the engine and hits the burnoff sparklers beneath the rocket, creating a dramatic fireball around the vehicle’s base, something that has become a customary trademark for Delta 4 launches over the past decade.But the new staggered process is designed to lessen that pre-liftoff fire before the 23-story-tall Heavy takes to the sky. With the first engine running and working to aspirate the forthcoming hydrogen flame from the other two boosters, the center and port engines will begin their ignition process at T-minus 5 seconds and see a significant portion of the resulting fire drawn into launch table instead of rising up.Vandenberg’s previous Heavy lifts off in 2011. Credit: Pat Corkery/United Launch AllianceThe six previous launches of Delta 4-Heavy rockets — five from Cape Canaveral and one from Vandenberg — commanded all three engines to ignite simultaneously.The earlier Vandenberg launch in 2011, however, saw the ignition plume catch external insulation on fire as the vehicle lifted off and cleared to the pad. The flames extinguished a few seconds later and the mission proceeded successfully.The staggered engine sequence is meant to prevent such a reoccurrence without altering the engines’ operations during flight, providing a cleaner and less dramatic launch.The debut of this procedure on the East Coast will be made next year when a Heavy launches NASA’s Orion deep-space capsule on a three-orbit shakedown cruise around the Earth.Each engine guzzles nearly a ton of propellants per second to produce 656,000 pounds of sea-level rated thrust. The upper stage, with its Aerojet Rocketdyne RL10B-2 engine, takes over about six minutes into flight.Wednesday’s mission, flying southward from Vandenberg, will place a classified payload into polar orbit for the U.S. National Reconnaissance Office, the agency responsible for operating the country’s fleet for spy satellites.The Delta 4-Heavy is America’s largest unmanned rocket currently in service, capable of lofting the biggest and heftiest cargos. The mammoth vehicle is created by taking three Common Booster Cores — the liquid hydrogen-fueled motor that forms a Delta 4-Medium’s first stage — and strapping them together to form a triple-barrel rocket, and then adding an upper stage. The first West Coast Delta 4-Heavy at Vandenberg’s SLC 6 in 2011. Credit: Pat Corkery/United Launch Alliance”There’s nothing bigger that the United States launches — period — in any way, shape or form, and that is absolutely amazing,” said Lt. Col. Jim Bodnar, commander of the 4th Space Launch Squadron at Vandenberg.A Heavy launching from Vandenberg is capable of putting school bus-sized reconnaissance observatories into polar orbit, a performance roughly comparable to the retired space shuttles and Titan 4 rockets.The target launch date for this mission, designated NROL-65, has remained unchanged for months, staying on schedule despite sequestration and personnel furloughs.”I don’t want to jinx myself, but it has been an extremely smooth flow,” Bodnar said. “It is a testament to the work ULA does and that the 4th Space Launch Squadron oversees. I dare say this has been one of the smoothest flows that I’ve seen.”A lengthy series of readiness reviews ranging from subsystems to the payload has been underway since last week. The assessments culminate with the final launch approval to be given Tuesday, Bodnar said.”The launch business is probably one of the most risk-adverse businesses out there,” Bodnar said. “The extra time the reviews take are well worth the cost because the alternative is unthinkable.”Crews at the Space Launch Complex 6 pad, the site formerly envisioned for West Coast space shuttle missions, will retract the mobile assembly shelter to its launch position on Monday. The 9-million-pound structure provides environmentally-friendly working conditions at the pad, originally to avoid high winds during shuttle stacking operations.The 13-million-pound mobile service tower that provides all-level access to the rocket will be wheeled back Tuesday night ahead of the countdown.Clocks will start ticking at 4:52 a.m. local Wednesday, followed a short time later by fueling operations for the eight cryogenic liquid hydrogen and liquid oxygen tanks aboard the vehicle.A planned built-in hold is scheduled at T-minus 4 minutes and will last for 45 minutes, leading to liftoff at 10:52 a.m. local (1:52 p.m. EDT; 1752 GMT).It will be the 364th flight of a Delta rocket, the 24th for the Delta 4 family, the NRO’s eighth use of the Delta 4 and ULA’s 74th mission, the eighth just this year.”Rarely do you see dry eyes when the rocket launches and you know that it’s successful,” Bodnar said. “The fact that we actually get to see the fruits of all of that labor is actually amazing. They’re awe-inspiring.”Final Shuttle Mission PatchFree shipping to U.S. addresses!The crew emblem for the final space shuttle mission is now available in our store. Get this piece of history!STS-134 PatchFree shipping to U.S. addresses!The final planned flight of space shuttle Endeavour is symbolized in the official embroidered crew patch for STS-134. Available in our store!Ares 1-X PatchThe official embroidered patch for the Ares 1-X rocket test flight, is available for purchase.Apollo CollageThis beautiful one piece set features the Apollo program emblem surrounded by the individual mission logos.Project OrionThe Orion crew exploration vehicle is NASA’s first new human spacecraft developed since the space shuttle a quarter-century earlier. The capsule is one of the key elements of returning astronauts to the Moon.Fallen Heroes Patch CollectionThe official patches from Apollo 1, the shuttle Challenger and Columbia crews are available in the store. | | | | 2014 Spaceflight Now Inc.An introduction to general relativityNASAPRESS KIT

    September 20th, 2014 at 10:50 pm (#)

  352. Anonymous says:

    STORY WRITTEN FOR & USED WITH PERMISSIONPosted: June 16, 2004To successfully send humans back to the moon and eventually on to Mars, NASA must implement sweeping cultural changes, transforming itself into a leaner, more innovative agency that relies much more heavily on private industry and international cooperation, a presidential panel reported today. Artist’s concept of astronauts at a moon base. Credit: NASA/Commission Report Equally important, the commission concluded, the American public must buy into the goals of the re-structured program and lawmakers must provide steady funding over the next two decades and beyond to turn the dream into reality.”This is a tremendous thing for NASA,” said panel chairman Edward “Pete” Aldridge Jr., a former Air Force secretary. “For years, they didn’t have a direction (like the one) clearly articulated by the president now. And it’s got to be multiple presidents. This has got to last through 10 presidential terms, at least. … It’s got to be sustainable over a long period of tiem.”The sustainability issue is very critical,” he added. “The American people have to achieve ownership of this. And they have to be shown the value of the space program to their way of life.”The President’s Commission on Implementation of United States Space Exploration Policy was created by executive order on Jan. 27, two weeks after President Bush unveiled his new moon-Mars initiative in a Jan. 14 speech at NASA headquarters. The president called for sending robots and then astronauts back to the moon between 2015 and 2020 and eventually, on to Mars. As part of that plan, the space shuttle will be retired by 2010, or whenever assembly of the international space station is complete, and NASA will develop a new manned spacecraft capable of carrying astronauts to and from low-Earth orbit and on into deep space.The moon-Mars initiative resulted in part from criticism by the Columbia Accident Investigation Board that pointed to a lack of clear, long-range goals in the space program that contributed in part to the shuttle disaster.The Aldridge commission was given 120 days to come up with a set of recommendations for turning the president’s vision into reality. Today, the results of that work – a 60-page report built around eight findings and 14 recommendations – was presented to Vice President Cheney at the White House.A key theme in the report is the need for NASA to cut its managerial ties to the past and to develop a new approach to conducting business on the high frontier.”We conclude that fundamental changes must take place in how the nation approaches space exploration and manages the vision for success,” Aldridge said in a cover letter to President Bush.”This national effort calls for a transformation of NASA, building a robust international space industry, a discovery-based science agenda and educational initiatives to support youth and teachers inspired by the vision.” Artist’s concept of astronauts on Mars. Credit: NASA/Commission Report The report offers a variety of sweeping recommendations for transforming NASA’s management structure and culture, increasing the role of private industry and bringing in international cooperation. But the central unknown remains just that: How to “sell” a restructured space program to the American public and how to ensure it receives the multi-decade support it will need from future presidents and congresses.In a section titled “Why Go?” the panel laid out its view of the answer to those questions. A sustained space exploration program, the report said, would inspire the nation’s youth, generate new jobs and markets and contribute to the nation’s security by ensuring leadership in high-technology fields. It would also, of course, expand the nation’s scientific horizons and answer fundamental questions about the birth, evolution and fate of the universe.”Exploring the moon, Mars and beyond is a great journey worthy of a great nation,” the report said. “The impulse to explore the unknown is a human imperative and a notable part of what animates us as a people. This endeavor presents an opportunity to inspire a new generation of American explorers, scientists, entrepreneurs and innovators who will provide positive American leadership to the world.”Listing three “imperatives for success,” the panel said the new initiative must be sustainable, affordable and credible to achieve the public support necessary for long-term survival.”The space exploration vision sets a complex course that must be sustained for several decades,” the commission wrote. “Obviously, this will require the support of multiple presidents, multiple Congresses and a couple of generations of American taxpayers.”And at its core, the vision requires a sustained commitment from the American public.”To get the program underway, the president’s plan would give NASA $1 billion in new funding over the next five years. Over the same period, NASA was directed to come up with another $11 billion from its own projected budget, money that would come from existing programs.Aldridge said NASA can accomplish the moon-Mars initiative within existing budgets and without the need for massive infusions of cash if the panel’s recommendations are carried out.”We support a ‘go as you can pay’ approach for funding, which allows specific exploration goals to be adjusted as technology advances and periodic milestones are achieved,” Aldridge said. “This also allows the space exploration program to remain affordable within the resources available. We do not believe an assessment of a mission’s affordability should be based on an unknowable and highly uncertain projection of total mission cost.”Aldridge said he’s frequently asked what that total mission cost might be.”The answer is, I don’t know,” he said today. “I’ll ask the same question. How much is the cure for cancer going to cost? I don’t know that, either. But I know what I can afford on an annual basis to try to get there. And this is the same model we’re using for the space program.NASA’S $16 billion budget, he said, “has to be passed at the levels that have been requested and if that is done, then we can get on with this project. The budgets that are projected beyond that are very, very modest, it’s less than seven-tenths of one percent of the federal budget. Most people don’t realize that the NASA budget is that small.”It’s less than one percent of the federal budget and we accomplish a lot for that small amount of money. If we can get that kind of level of funding for the next 20 years, we believe with the right allocation of the activities, such as phasing out the shuttle at the appropriate time and focusing our attention on this new mission, that it can be done within that which we believe to be affordable in this nation.” Artist’s concept of future astronauts on the moon. Credit: NASA/Commission Report Funding issues aside, the commission’s report focused on the need for management changes at NASA.The panel recommended establishment of a permanent Space Exploration Council, chaired by the vice president or some other high-ranking official, that would include representatives of all appropriate federal agencies. Reporting directly to the president, the council would be empowered “to develop policies and coordinate work by its agencies to share technologies, facilities and talent with NASA to support the national space exploration vision.”At the same time, NASA’s Apollo-era management structure “must be decisively transformed,” the commission said, recommending that:NASA should turn over many functions to private industry with the ultimate goal being to allow “private industry to assume the primary role of providing services to NASA, and most immediately in accessing low-Earth orbit. In NASA decisions, the preferred choice for operational activities must be competitively awarded contracts with private and non-profit organizations.” NASA’s role, the panel concluded, should be limited to those areas “where there is irrefutable demonstration that only government can perform the proposed activity.”NASA should define clear lines of authority and accountability as part of a more focused and integrated agency.NASA field centers should be restructured as Federally Funded Research and Development Centers in which a contractor operates the facility for the government. The Jet Propulsion Laboratory in Pasadena, Calif., which is operated for NASA by the California Institute of Technology, is an example of a working FFRDC. Putting other NASA centers on a similar footing would “enable innovation” and “stimulate economic development,” the panel said. Some functions, however, would remain under direct government control.Three new NASA organizations be created: A technical advisory board that would provide an independent assessment of technical feasibility and risk mitigation; an independent panel to verify cost estimates; a research organization to sponsor development of high-risk technology.NASA should adopt personnel and management reforms in line with accepted policies and practices in place across cutting edge government and industry organizations.The panel recommended that NASA establish teams to identify critical enabling technologies and “aggressively use its contractual authority to reach broadly into the commercial and non-profit communities to bring the best ideas, technologies and management tools into the accomplishment of exploration goals.”Congress should provide financial incentives, the commission said, to attract entrepreneurs to the high frontier. And Congress should re-examine existing treaties to resolve open questions about property rights in space to encourage development of space infrastructure.”The commission believes that commercialization of space should become a primary focus of the vision and that the creation of a space-based industry will be one of the principal benefits of this journey,” the commission wrote.”One of the challenges we face is to find commercial rewards and incentives in space. Creating these rewards is an indispensable part of making this partnership work in the right way. It will signal a major change in the way NASA deals with the private sector, and the commission believes that NASA should do all it can to create, nurture and sustain this new industry.”Aldridge said NASA likely would remain in charge of manned launch operations, but unmanned launches to deliver cargo to orbit could be turned over to private industry.”What we’re trying to get to is to have NASA focus on things that are inherently governmental,” Aldridge said today. “Probably the human spaceflight part of the NASA mission probably can’t be turned over to the private sector. But the unmanned, cargo-like processes could be. … We believe if NASA can focus on those very difficult, high-risk, clearly not-money-making missions and look for things that the private sector can do in helping NASA focus its attention on the real exploration stuff … that’s what we’re talking about.”The commission also recommended that NASA:Seek input from the scientific community to “ensure that maximum use is made of existing assets and emerging capabilities.”Ask the National Academy of Sciences to consider “how machines and humans, used separately and in combination, can maximize scientific returns.”Use a “discovery-based criterion” for selecting destinations beyond the moon and Mars “that also considers affordability, technical maturity, scientific important and emerging capabilities including access to in situ space resources.”Finally, the commission recommended that the president’s Space Exploration Steering Council develop an “action plan” to support math, science and engineering education.Additional coverage for subscribers:VIDEO:COMMISSION HOLDS NEWS CONFERENCE IN WASHINGTON VIDEO:NASA WORKERS ASK QUESTIONS TO O’KEEFE AND ALDRIDGE Fallen Heroes special patchThis special 12-inch embroidered patch commemorates the U.S. astronauts who made the ultimate sacrifice, honoring the crews of Apollo 1, Challenger and Columbia.Choose your store: – – – Moon RushThis book examines how the exploration of space, specifically a commercial base on the Moon and Mars would transform our economies on the Earth as surely as the discovery of the New World transformed the old world of Europe.Choose your store: – – – Apollo 11 special patchSpecial collectors’ patch marking the 35th anniversary of the historic Apollo 11 moon landing is now available.Choose your store: – – – Get inside Apollo!Full color drawings reveal like never before the details of the Apollo Command and Service Modules.Choose your store: – – – | | | | 2014 Spaceflight Now Inc.Swift satellite catches galaxy ablaze with starbirth NASA-GSFC NEWS RELEASEPosted: March 3, 2008Combining 39 individual frames taken over 11 hours of exposure time, NASA astronomers have created this ultraviolet mosaic of the nearby “Triangulum Galaxy.” Credit: NASA/Swift Science Team/Stefan ImmlerSee larger image “This is the most detailed ultraviolet image of an entire galaxy ever taken,” says Stefan Immler of NASA’s Goddard Space Flight Center in Greenbelt, Md.Immler used NASA’s Swift satellite to take the images, and he then assembled them into a mosaic that seamlessly covers the entire galaxy.The Triangulum Galaxy is also called M33 for being the 33rd object in Charles Messier’s sky catalog. It is located about 2.9 million light-years from Earth in the constellation Triangulum.It is a member of our Local Group, the small cluster of galaxies that includes our Milky Way Galaxy and the Andromeda Galaxy (M31). Despite sharing our Milky Way’s spiral shape, M33 has only about one-tenth the mass. M33′s visible disk is about 50,000 light-years across, half the diameter of our galaxy.Swift’s Ultraviolet/Optical Telescope (UVOT) took the images through three separate ultraviolet filters from December 23, 2007 to January 4, 2008. The mosaic showcases UVOT’s high spatial resolution. Individual star clusters and star-forming gas clouds are clearly resolved, even in the crowded nucleus of the galaxy. The image also includes Milky Way foreground stars and much more distant galaxies shining through M33. Young, hot stars are prodigious producers of ultraviolet light, which heat up the surrounding gas clouds to such high temperatures that they radiate brightly in ultraviolet light. The image shows the giant star-forming region NGC 604 as a bright spot to the lower left of the galaxy’s nucleus. With a diameter of 1,500 light-years (40 times that of the Orion Nebula), NGC 604 is the largest stellar nursery in the Local Group.”The ultraviolet colors of star clusters tell us their ages and compositions,” says Swift team member Stephen Holland of NASA Goddard. “With Swift’s high spatial resolution, we can zero in on the clusters themselves and separate out nearby stars and gas clouds. This will enable us to trace the star-forming history of the entire galaxy.”"The entire galaxy is ablaze with starbirth,” adds Immler. “Despite M33′s small size, it has a much higher star-formation rate than either the Milky Way or Andromeda. All of this starbirth lights up the galaxy in the ultraviolet.” STS-134 PatchFree shipping to U.S. addresses!The final planned flight of space shuttle Endeavour is symbolized in the official embroidered crew patch for STS-134. Available in our store!Final Shuttle Mission PatchFree shipping to U.S. addresses!The crew emblem for the final space shuttle mission is now available in our store. Get this piece of history!Apollo CollageThis beautiful one piece set features the Apollo program emblem surrounded by the individual mission logos.STS-133 PatchFree shipping to U.S. addresses!The final planned flight of space shuttle Discovery is symbolized in the official embroidered crew patch for STS-133. Available in our store!Anniversary Shuttle PatchFree shipping to U.S. addresses!This embroidered patch commemorates the 30th anniversary of the Space Shuttle Program. The design features the space shuttle Columbia’s historic maiden flight of April 12, 1981.Mercury anniversaryFree shipping to U.S. addresses!Celebrate the 50th anniversary of Alan Shephard’s historic Mercury mission with this collectors’ item, the official commemorative embroidered patch. | | | | 2014 Spaceflight Now Inc.Taurus XL rocket launches Taiwan’s new orbiting eye SPACEFLIGHT NOWPosted: May 20, 2004The first Taurus XL rocket, a beefed up model of Orbital Sciences’ small satellite launcher, darted into polar orbit Thursday, deploying a Taiwanese spacecraft and potentially attracting customers for future missions. The Taurus XL rocket blasts off carrying ROCSAT 2. Credit: Gene BlevinsFollowing a smooth countdown, the four-stage rocket blasted off on-time at 1747 GMT (1:47 p.m. EDT; 10:47 a.m. local) from pad 576E at Vandenberg Air Force Base, California.Fourteen minutes later, the rocket successfully completed the launch by releasing its cargo in space.”We are very pleased with the results of the Taurus launch and wish our customers from Taiwan’s National Space Program Office the very best with their satellite mission,” said Ron Grabe, Orbital’s executive vice president and general manager of its Launch Systems Group.Thursday’s launch was crucial for the Taurus rocket. Not only was the XL version making its debut, but it also marked the return-to-flight for the Taurus vehicle family after a failure nearly three years ago.”We’re clearly all a little anxious on this one. Like in any of these vehicles, you’ve got 100,000 parts that all have to do their job at the right time and you hope you’ve done everything you could from a test perspective to flush any bad parts out. But unfortuately until you actually go fly through the environment you don’t know,” Bill Wrobel, Orbital’s Taurus program manager, said in an interview.The last mission in September 2001 was lost when a steering mechanism on the second stage motor jammed at ignition, robbing the rocket of its speed and preventing it from achieving orbit. Taurus climbs away from its launch pad overlooking the Pacific Ocean. Credit: Gene BlevinsA redesigned steering system, which borrowed technology from the Ground-based Midcourse Defense Segment missile program, was used Thursday with a successful outcome.The XL version of Taurus uses longer second and third stages packed with additional propellant, providing up to 25 percent more performance during launch.”It’s something we always wanted to do,” Wrobel said.”The actual development phase of the vehicle went pretty well. We’ve had some smaller problems but honestly with the XL portion of things that’s been fairly straight-forward.”Orbital’s air-launched Pegasus rocket was up-sized from its original “standard” configuration to the XL version nearly a decade ago.”Taurus was one of the last hold outs still using the standard size,” Wrobel said.”The other thing is this mission required additional performance that we could not get with a standard vehicle. So it really was a requirement, more or less, under this mission to get that developed.”This mission lofted the 1,600-pound, French-built ROCSAT 2 spacecraft that becomes Taiwan’s second Earth-observing satellite.

    September 20th, 2014 at 10:50 pm (#)

  353. UGG Classic Corto Botas says:

    STORY WRITTEN FOR & USED WITH PERMISSIONPosted: January 12, 2005KENNEDY SPACE CENTER, Fla. (CBS) – In one of the boldest space missions ever attempted, a small European-built probe will slam into the atmosphere of Saturn’s mysterious moon Titan Friday for a two-and-a-half hour parachute descent to its smog-shrouded surface. An artist’s concept shows Huygens nearing Titan. Credit: ESABeaming pictures and a torrent of data to NASA’s Cassini Saturn orbiter, the flying saucer-shaped Huygens probe will give scientists their first close-up look at one of the largest expanses of unexplored territory in the solar system. Researchers are hopeful Huygens will answer their most pressing questions: whether hydrocarbons fall like rain and form pools of liquid ethane and similar compounds on the moon’s frigid surface; and what erosional or depositional processes are responsible for covering up impact craters and producing a relatively flat, mountain-free surface. No matter what Huygens actually sees on the surface, scientists expect to gain insights into the workings of a thick, complex atmosphere that in some respects mirrors Earth’s shortly after the planet’s birth. “We ought to be able to see a pretty good panorama of the area that the Huygens probe is going to land in,” Jonathan Lunine, a planetary scientist at the University of Arizona, said in a recent interview. “Those pictures will continue all the way down to the surface, they’ll be interrupted right at the end when the camera switches over to take what are called spectra, which will tell us about the composition of the surface. So we ought to be able to get a pretty good panorama to start with. “We ought to be able to see whether the probe came down in an area that’s mostly craters or other kinds of land forms. We ought to be able to get a hint of whether there might be pools or lakes of liquid in that area. It won’t be immediately apparent whether dark places are liquid or solid, but depending on where the probe lands, we might get some direct information on that. And we might see clouds in the sky toward the horizon. “There may be some detection of lightning,” he said, “although there probably isn’t a lot of lightning in Titan’s atmosphere. And then after impact, or touchdown, if the antennas aren’t pointed in a strange direction, we should be able to get some information about the surface. If we’re lucky enough to land in liquid, then the probe should be bobbing up and down and there’s a tilt meter that will tell us that. And we might be able to get samples of surface material because the probe will still be warm and anything like these liquid hydrocarbons will vaporize and go up into the sample inlets.”Huygens was released from Cassini on Christmas Eve, placed on a collision course with Titan that was set up to ensure the proper atmospheric entry angle. David Southwood, the European Space Agency’s science director, thanked NASA for the lift, saying “now all our hopes and expectations are focused on getting the first in situ data from a new world we?ve been dreaming of exploring for decades.”During flybys of Titan in late October and again in December, Cassini’s powerful cameras, an imaging radar system and other instruments mapped the surface in unprecedented detail, revealing a relatively flat terrain and unusual, sharply defined features that defied easy explanation. Only a handful of large crater-like circular structures were apparent and researchers did not see the sort of specular reflections one might expect from sunlight glinting off a liquid surface. Whether Huygens will detect standing lakes or pools is a major question mark going into Friday’s descent. So far, said Torrence Johnson, a Cassini imaging team member at the Jet Propulsion Laboratory in Pasadena, Calif., “we don’t have any evidence (for liquids).” “Just like we don’t have any clear evidence of something we know is a crater, there’s nothing there that anybody’s willing to hang their hat on yet that yes, we absolutely have a liquid surface,” he said in a telephone interview Monday. “What we saw (in the initial Cassini flybys), of course, was a surface that was much stranger than most of us thought we would see,” he said. “The real story so far has been the things we didn’t see.” Like large craters, hills or mountain ranges and obvious lakes or river-like structures. But that doesn’t mean liquids aren’t there. Just that Cassini didn’t spot them in its initial looks at the moon. “It’s a distinct possibility that I could be the very first scientist to carry out oceanography on an outer planet of the solar system,” said John Zarnecki, principal scientist for the Huygens Science Surface Package. “But equally the probe could land with a thud on hard ground or squelch into a morass of extraterrestrial slime – no one knows for sure. “In any event, the instruments onboard have been designed to handle a range of possibilities,” he said in a statement. “Let’s just say that, after a seven-year voyage and twenty years of planning, design and build, I will be extremely pleased to land, whatever the surface.” An artist’s concept shows Huygens descending on its parachute. Credit: ESAHuygens, if it survives long enough, should reveal the surface in sharp detail and send back a wealth of data about its thick atmosphere. But even that will not be enough to answer all the questions posed by the scientific community. “I think we’re going to have to wait several flybys, maybe even several years, before we get a really good indication of what’s going on,” said Carolyn Porco, the Cassini imaging team leader. “What Huygens will do, of course, is give us a very exquisitely detailed view of one place. So their information will (provide) the ‘ground truth’ for helping us interpret what we see.” Spinning at 7 rpm for stability, Huygens will slam into the atmosphere Friday at an altitude of 789 miles, traveling at some 12,400 mph. A thick carbon composite heat shield will protect the craft from the fierce heat of atmospheric friction – nearly 3,500 degrees – which will quickly slow the probe to more benign speeds. Maximum deceleration is expected to be around 16 Gs. When the velocity has dropped to about 870 mph, Huygens’ aft cover will be pulled away by a pilot chute and the spacecraft’s 27-foot-wide main parachute will deploy 2.5 seconds later. The main chute will be jettisoned 15 minutes later and from that point on, Huygens will ride beneath a smaller 9.8-foot-wide parachute. Impact on the surface at some 11 mph is expected about two-and-a-half hours after entry begins. Regardless of how long Huygens might survive on the surface, Cassini will sink below Titan’s horizon about 30 minutes after touchdown. Assuming the 705-pound Huygens doesn’t sink in a hydrocarbon lake, “we have good confidence the probe will survive landing,” said European Space Agency mission manager Jean-Pierre Lebreton. “The landing speed is very low.” Here is a detailed timeline of major entry events on Jan. 14 (in EST; all times represent when an event occurs relative to signals received on Earth). Explanations for key events from the European Space Agency’s ; Cassini timeline events provided by the :Jan. 1402:33 AM (-02h40m) – Cassini solid state recorders prepped for support02:45 AM (-02h28m) – Cassini transition to thruster control for relay02:55 AM (-02h18m) – Cassini: final recorder configuration for relay02:57 AM (-02h16m) – Turn on Probe receivers03:09 AM (-02h04m) – Cassini turns toward Titan03:21 AM (-01h52m) – Turn to Titan complete03:24 AM (-01h49m) – Cassini disables X-band downlink04:51 AM (-00h22m) – Probe turns transmitters on (low power mode)05:13 AM (-00h00m) – Probe reaches the discernible atmosphere: 789 miles05:16 AM (+00h03m) – Probe feels maximum deceleration05:17 AM (+00h04m) – Pilot chute: 106-118 miles altitude; Mach 1.5; The parachute deploys when Huygens detects that it has slowed to 895 mph, at about 112 miles above Titan’s surface. The pilot parachute is the probe’s smallest, only 8.5 feet in diameter. Its sole purpose is to pull off the probe’s rear cover, which protected Huygens from the frictional heat of entry. 2.5 seconds after the pilot parachute is deployed, the rear cover is released and the pilot parachute is pulled away. The main parachute, which is 27.2 feet in diameter, unfurls.05:18 AM (+00h05m) – At about 99 miles above the surface, the front shield is released. Forty-two seconds after the pilot parachute is deployed, inlet ports are opened up for the Gas Chromatograph Mass Spectrometer and Aerosol Collector Pyrolyser instruments, and booms are extended to expose the Huygens Atmospheric Structure Instruments. The Descent Imager/Spectral Radiometer will capture its first panorama, and it will continue capturing images and spectral data throughout the descent. The Surface Science Package will also be switched on, measuring atmospheric properties.05:32 AM (+00h19m) – Main parachute separates and drogue parachute deploys: The drogue parachute is 9.8 feet in diameter. At this level in the atmosphere, about 78 miles in altitude, the large main parachute would slow Huygens down so much that the batteries would not last for the entire descent to the surface. The drogue parachute will allow it to descend at the right pace to gather the maximum amount of data.05:49 AM (+00h36m) – Surface proximity sensor activated: Until this point, all of Huygens’s actions have been based on clock timers. At a height of 37 miles, it will be able to detect its own altitude using a pair of radar altimeters, which will be able to measure the exact distance to the surface. The probe will constantly monitor its spin rate and altitude and feed this information to the science instruments. All times after this are approximate.05:56 AM (+00h43m) – Possible icing effects to Probe (31 miles)06:57 AM (+01h41m) – Gas Chromatograph Mass Spectrometer begins sampling atmosphere: This is the last of Huygens’s instruments to be activated fully. The descent is expected to take 137 minutes in total, plus or minus 15 minutes. Throughout its descent, the spacecraft will continue to spin at a rate of between 1 and 20 rotations per minute, allowing the camera and other instruments to see the entire panorama around the descending spacecraft.07:19 AM (+02h06m) – Cassini closest approach: 37,282 miles flyby at 12,080 mph, 93 deg phase07:30 AM (+02h17m) – Descent Imager/Spectral Radiometer lamp turned on: Close to the surface, Huygens’s camera instrument will turn on a light. The light is particularly important for the ‘Spectral Radiometer’ part of the instrument to determine the composition of Titan’s surface accurately.07:34 AM (+02h21m) – Surface touchdown: This time may vary by plus or minus 15 minutes depending on how Titan’s atmosphere and winds affect Huygens’s parachuting descent. Huygens will hit the surface at a speed of 11.2-13.4 mph. Huygens could land on a hard surface of rock or ice or possibly land on an ethane sea. In either case, Huygens’s Surface Science Package is designed to capture every piece of information about the surface that can be determined in the three remaining minutes that Huygens is designed to survive after landing.09:44 AM (+04h31m) – Cassini stops collecting data; Huygens’s landing site drops below Titan’s horizon as seen by Cassini and the orbiter stops collecting data. Cassini will listen for Huygens’s signal as long as there is the slightest possibility that it can be detected. Once Huygens’s landing site disappears below the horizon, there’s no more chance of signal, and Huygens’s work is finished.09:46 AM (+04h33m) – Cassini probe data partitions write protected09:54 AM (+04h41m) – Cassini turns toward Earth09:57 AM (+04h44m) – Turn to Earth complete10:06 AM (+04h53m) – Critical sequence ends10:07 AM (+04h54m) – Post-Probe tracking begins (Canberra)10:14 AM (+05h01m) – First data sent to Earth: Getting data from Cassini to Earth is now routine, but for the Huygens mission, additional safeguards are put in place to make sure that none of Huygens’s data are lost. Giant radio antennas around the world will listen for Cassini as the orbiter relays repeated copies of Huygens data.10:17 AM (+05h04m) – Probe data replay begins (Canberra: 66,360 bps)12:57 PM (+07h44m) – End playback of first partition01:04 PM (+07h51m) – Ascending ring-plane crossing: 18.4 Saturn radii02:00 PM (+08h47m) – Start tracking at Madrid (142,200 bps)05:07 PM (+11h54m) – End first full playback of all Probe data08:29 PM (+15h16m) – Full data set on Earth (likely three hours earlier)10:35 PM (+17h22m) – Start tracking at GoldstoneJan. 1507:07 AM (+01d02h) – Power on of orbiter instruments08:30 AM (+01d03h) – End nominal playback of Probe dataCassini braked into orbit around Saturn on July 1 after a seven-year voyage from Earth. The original flight plan called for Huygens to enter Titan’s atmosphere in late November as Cassini streaked overhead at an altitude of just 746 miles. But engineers were forced to delay Huygens’ arrival to this month because of an issue with the radio aboard the Cassini mothership that will be used to relay data from Huygens to Earth. During a post-launch test, engineers discovered the radio receiver could not cope with the Doppler shift in the frequency of the signal coming from Huygens due to Cassini’s high relative velocity. Much like the pitch of a siren changes as a police car races past a stationary observer, the frequency of radio waves can shift a significant amount if relative velocities are high enough. “Originally, the closing speed of Cassini coming up on Huygens, which is for all practical purposes sitting still once it’s in the atmosphere, the closing speed was about 5.8 kilometers per second (13,000 mph),” Cassini program manager Bob Mitchell said in a recent interview. “And because we were coming in almost dead overhead and going off to the right at about 1,200 kilometers (746 miles) altitude.” The solution was to minimize the Doppler shift by reducing the relative velocities of the two spacecraft. That was accomplished by changing Cassini’s trajectory slightly and delaying Huygens’ release to Christmas Eve. During the Jan. 14 descent, Cassini now will be 37,300 miles from Titan and the difference in velocity between the two spacecraft will never be more than 8,500 mph. “We have pretty solid evidence that’s going to work,” Mitchell said. “We did some tests where we used the Deep Space Network stations transmitting an S-band signal with telemetry modulated onto the carrier so that from the receiver’s point of view on the Cassini spacecraft, it should have simulated the probe quite accurately. We adjusted the frequency, taking into account the motion of everything, so that the frequency of the received signal at the receiver should very closely if not exactly match the frequency that the receiver will see coming from Huygens.” The tests were successful and a potentially crippling design flaw was resolved with no significant loss of science. And so, the stage is set for a dramatic voyage of discovery. “Whatever is there is going to look pretty good, I think,” Johnson said. “The probe is spinning as it comes down, sort of a spin-scan imager looking out and down at an angle. Of course, the haze will get less as you go down. “We had hoped that once it got down to within a hundred kilometers of the surface or something like that we’d start seeing things that looked like pictures out of an airplane window. Based on our data, I think that maybe they will still see a very hazy surface even at longer wavelengths at that type of altitude. Because one of the things that we found is that some of the scattering that’s producing this fuzzy appearance on the surface is happening down under 10 kilometers. … But at some point, we ought to start seeing the surface more clearly. It may be in the last 10 kilometers of descent.” Johnson said he was especially looking forward to finding out “what sort of topography there is. Is it all flat down there? Or are there hints of underlying topography?” “I would hope we would be able to tell the difference between mantle material that’s been covered up by soft aerosols and areas where there might be really flat places with lakes, all of which could be hidden in the data we’re seeing now at the resolutions we have.” Whatever Huygens sees, “it could be pretty damn spectacular,” Johnson said. Huygens, of course, will send back much more than pictures. Here’s a summary from NASA’s Cassini press kit: “Throughout the descent, Huygens’ atmospheric structure instrument will measure the physical properties of the atmosphere,” according to NASA’s Cassini press kit. “The gas chromatograph and mass spectrometer will determine the chemical composition of the atmosphere as a function of altitude. The aerosol collector and pyrolyzer will capture aerosol particles – fine liquid or solid particles suspended in the atmosphere – heat them and send the resulting vapor to the chromatograph/spectrometer for analysis. “Huygens’ descent imager and spectral radiometer will take pictures of cloud formations and Titan’s surface and also determine the visibility within Titan’s atmosphere. As the surface looms closer, the instrument will switch on a bright lamp and measure the spectral reflectance of the surface. Throughout the descent, the Doppler shift of Huygens’ radio signal will be measured by the Doppler wind experiment onboard the Cassini orbiter to determine Titan’s atmospheric winds, gusts and turbulence. “As the probe is shifted about by winds, the frequency of its radio signal (will) change slightly in what is known as the Doppler effect – similar to how the pitch of a train whistle appears to rise and then fall as the train passes. Such changes in frequency can be used to deduce the wind speed experienced by the probe. “As Huygens nears impact, its surface science package will activate a number of sensors to measure surface properties. Huygens will impact the surface at about 15 miles per hour; the chief uncertainty is whether its landing will be a thud or a splash. “If Huygens lands in liquid, these instruments will measure the liquid’s properties while the probe floats for a few minutes. If Huygens lands in liquid ethane it will not be able to return data for very long, because the extremely low temperature of this liquid (about (-180 C (-290 F) would prevent the batteries from operating. “In addition, if liquid ethane permeates the probe’s science instrument packages, the radio would be badly tuned and probably not operate. Assuming Huygens continues to send data to Cassini from Titan’s surface, it will be able to do so for a maximum of about 30 minutes, when the probe’s battery power is expected to run out and the Cassini orbiter disappears over the probe’s horizon.”Ares 1-X PatchThe official embroidered patch for the Ares 1-X rocket test flight, is available for purchase.Apollo CollageThis beautiful one piece set features the Apollo program emblem surrounded by the individual mission logos.Expedition 21The official embroidered patch for the International Space Station Expedition 21 crew is now available from our stores.Hubble PatchThe official embroidered patch for mission STS-125, the space shuttle’s last planned service call to the Hubble Space Telescope, is available for purchase. | | | | 2014 Spaceflight Now Inc.Radar image shows Titan’s surface live and in color CASSINI PHOTO RELEASEPosted: November 6, 2004Saturn’s moon Titan shows a sharp contrast between its smooth and rough edges in a new false-color radar image.Titan’s surface lies beneath a thick coat of hazy clouds, but Cassini’s radar instrument can peer through to show finer surface features. Scientists have added color to emphasize finer details on Titan, as shown in the image.To provide a better perspective of the surface features, the color image is shown next to a black-and-white image that was previously released. Credit: NASA/JPLDownload larger image version Brighter areas may correspond to rougher terrains, slopes facing the radar, or different materials. The pink colors enhance smaller details on the surface, while the green color represents smoother areas. Winding linear features that cut across dark areas may be ridges or channels, although their nature is not yet understood. A large dark circular feature is seen at the western (top left) end of the image, but very few features on Titan resembling fresh impact craters are seen. The area shown is in the northern hemisphere of Titan and is about 150 kilometers (93 miles) wide by 300 kilometers (186 miles) long. The image is a part of a larger strip created from data taken on Oct. 26, 2004, when the Cassini spacecraft flew approximately 1,200 kilometers (745 miles) above Titan’s surface. The radar instrument works by bouncing radio signals off Titan’s surface and timing their return. This is similar to timing the returning echo of your voice across a canyon to tell how wide the canyon is. Approximately 1 percent of Titan’s surface was mapped during the Oct. 26 flyby.The Cassini-Huygens mission is a cooperative project of NASA, the European Space Agency and the Italian Space Agency. The Jet Propulsion Laboratory, a division of the California Institute of Technology in Pasadena, manages the Cassini-Huygens mission for NASA’s Science Mission Directorate, Washington, D.C. The radar instrument team is based at JPL.Cassini posterJust in time for the Cassini spacecraft’s arrival at Saturn, this new poster celebrates the mission to explore the ringed planet and its moons. 2005 CalendarThe 2005 edition of the Universe of the Hubble Space Telescope calendar is available from our U.S. store and will soon be available worldwide. This 12×12-inch calendar features spectacular images from the orbiting observatory.Moon panoramaTaken by Apollo 14 commander Alan Shepard, this panoramic poster shows lunar module pilot Edgar Mitchell as a brilliant Sun glare reflects off the lunar module Antares.Mars Rover mission patchA mission patch featuring NASA’s Mars Exploration Rover is now available from the Astronomy Now Store.Apollo 11 special patchSpecial collectors’ patch marking the 35th anniversary of the historic Apollo 11 moon landing is now available.Choose your store: – | | | | 2014 Spaceflight Now Inc.Radio telescopes will add to Huygens discoveries NATIONAL RADIO ASTRONOMY OBSERVATORY NEWS RELEASEPosted: December 25, 2004When the European Space Agency’s Huygens spacecraft makes itsplunge into the atmosphere of Saturn’s moon Titan on January 14,radio telescopes of the National Science Foundation’s NationalRadio Astronomy Observatory (NRAO) will help international teamsof scientists extract the maximum possible amount of irreplaceableinformation from an experiment unique in human history. Huygensis the 700-pound probe that has accompanied the larger Cassinispacecraft on a mission to thoroughly explore Saturn, its ringsand its numerous moons.The Robert C. Byrd Green Bank Telescope (GBT) in West Virginiaand eight of the ten telescopes of the continent-wide VeryLong Baseline Array (VLBA), located at Pie Town and Los Alamos,NM, Fort Davis, TX, North Liberty, IA, Kitt Peak, AZ, Brewster,WA, Owens Valley, CA, and Mauna Kea, HI, will directly receivethe faint signal from Huygens during its descent.Along with other radio telescopes in Australia, Japan, andChina, the NRAO facilities will add significantly to theinformation about Titan and its atmosphere that will be gainedfrom the Huygens mission. A European-led team will use the radiotelescopes to make extremely precise measurements of the probe’sposition during its descent, while a U.S.-led team willconcentrate on gathering measurements of the probe’s descentspeed and the direction of its motion. The radio-telescopemeasurements will provide data vital to gaining a fullunderstanding of the winds that Huygens encounters inTitan’s atmosphere.Currently, scientists know little about Titan’s winds. Datafrom the Voyager I spacecraft’s 1980 flyby indicated thateast-west winds may reach 225 mph or more. North-south windsand possible vertical winds, while probably much weaker,may still be significant. There are competing theoreticalmodels of Titan’s winds, and the overall picture is bestsummarized as poorly understood. Predictions of wherethe Huygens probe will land range from nearly 250 mileseast to nearly 125 miles west of the point where itsparachute first deploys, depending on which wind modelis used. What actually happens to the probe as it makesits parachute descent through Titan’s atmosphere will givescientists their best-ever opportunity to learn aboutTitan’s winds.During its descent, Huygens will transmit data from itsonboard sensors to Cassini, the “mother ship” that broughtit to Titan. Cassini will then relay the data back toEarth. However, the large radio telescopes will be ableto receive the faint (10-watt) signal from Huygensdirectly, even at a distance of nearly 750 million miles.This will not be done to duplicate the data collection,but to generate new data about Huygens’ position andmotions through direct measurement.Measurements of the Doppler shift in the frequency of Huygens’radio signal made from the Cassini spacecraft, in an experimentled by Mike Bird of the University of Bonn, will largelygive information about the speed of Titan’s east-west winds.A team led by scientists at NASA’s Jet Propulsion Laboratoryin Pasadena, CA, will measure the Doppler shift in the probe’ssignal relative to Earth. These additional Doppler measurementsfrom the Earth-based radio telescopes will provide importantdata needed to learn about the north-south winds.”Adding the ground-based telescopes to the experiment willnot only help confirm the data we get from the Cassiniorbiter but also will allow us to get a much more completepicture of the winds on Titan,” said William Folkner, aJPL scientist.Another team, led by scientists from the Joint Institute forVery Long Baseline Interferometry in Europe (JIVE), inDwingeloo, The Netherlands, will use a world-wide networkof radio telescopes, including the NRAO telescopes, to trackthe probe’s trajectory with unprecedented accuracy. Theyexpect to measure the probe’s position within two-thirds ofa mile (1 kilometer) at a distance of nearly 750 million miles.”That’s like being able to sit in your back yard and watchthe ball in a ping-pong game being played on the Moon,”said Leonid Gurvits of JIVE.Both the JPL and JIVE teams will record the data collected bythe radio telescopes and process it later. In the case of theDoppler measurements, some real-time information may beavailable, depending on the strength of the signal, but thescientists on this team also plan to do their detailed analysison recorded data.The JPL team is utilizing special instrumentation from the Deep SpaceNetwork called Radio Science Receivers. One will be loaned to the GBTand another to the Parkes radio observatory. “This is the sameinstrument that allowed us to support the challenging communicationsduring the landing of the Spirit and Opportunity Mars roversas well as the Cassini Saturn Orbit Insertion when the receivedradio signal was very weak,” said Sami Asmar, the JPL scientistresponsible for the data recording.When the Galileo spacecraft’s probe entered Jupiter’satmosphere in 1995, a JPL team used the NSF’s Very LargeArray (VLA) radio telescope in New Mexico to directly trackthe probe’s signal. Adding the data from the VLA to thatexperiment dramatically improved the accuracy of thewind-speed measurements.”The Galileo probe gave us a surprise. Contrary to somepredictions, we learned that Jupiter’s winds got strongeras we went deeper into its atmosphere. That tells us thatthose deeper winds are not driven entirely by sunlight, butalso by heat coming up from the planet’s core. If we getlucky at Titan, we’ll get surprises there, too,” said RobertPreston, another JPL scientist.The Huygens probe is a spacecraft built by the European SpaceAgency (ESA). In addition to the NRAO telescopes, the JPL DopplerWind Experiment will use the Australia Telescope National Facilityand other radio telescopes in Parkes, Mopra, and Ceduna, Australia;Hobart, Tasmania; Urumqi and Shanghai, China; and Kashima,Japan. The positional measurements are a project led by JIVE andinvolving ESA, the Netherlands Foundation for Research in Astronomy,the University of Bonn, Helsinki University of Technology, JPL,the Australia Telescope National Facility, the National AstronomicalObservatories of China, the Shanghai Astronomical Observatory, andthe National Institute for Communication Technologies in Kashima,Japan.The Joint Institute for VLBI in Europe is funded by the national researchcouncils, national facilities and institutes of The Netherlands (NWO andASTRON), the United Kingdom (PPARC), Italy (CNR), Sweden (Onsala SpaceObservatory, National Facility), Spain (IGN) and Germany (MPIfR). TheEuropean VLBI Network is a joint facility of European, Chinese, SouthAfrican and other radio astronomy institutes funded by their nationalresearch councils. The Australia Telescope is funded by the Commonwealthof Australia for operation as a National Facility managed by CSIRO.The National Radio Astronomy Observatory is a facility of theNational Science Foundation, operated under cooperative agreementby Associated Universities, Inc.Ares 1-X PatchThe official embroidered patch for the Ares 1-X rocket test flight, is available for purchase.Apollo CollageThis beautiful one piece set features the Apollo program emblem surrounded by the individual mission logos.Expedition 21The official embroidered patch for the International Space Station Expedition 21 crew is now available from our stores.Hubble PatchThe official embroidered patch for mission STS-125, the space shuttle’s last planned service call to the Hubble Space Telescope, is available for purchase. | | | | 2014 Spaceflight Now Inc.Reading tale of ions in Saturn’s magnetosphere UNIVERSITY OF MARYLAND NEWS RELEASEPosted: July 2, 2004The Cassini spacecraft has barely begun its four-year tour around Saturn, but already a University of Maryland sensor is beginning to reveal new data about the immense magnetosphere of the ringed planet.Designed and built by scientists in the University of Maryland’s space physics group, the CHEMS (CHarge Energy Mass Spectrometer) sensor measures ions — positively charged atoms — in Saturn’s magnetosphere.A planet’s magnetosphere is the magnetic field and charged particle environment that surrounds it. The magnetosphere traps ions produced in and around a planet. And it shields a planet from, and interacts with, the solar wind – the high-speed stream of ionized particles flowing out in all directions from the Sun.”By determining the elemental composition and charge state of the ions within and around Saturn’s magnetosphere, CHEMS will identify the sources of the plasma found there and study the processes of plasma acceleration,” says Douglas C. Hamilton, a professor of physics at the University of Maryland and leader of the space physics team that designed and built the CHEMS sensor. “CHEMS has already yielded data indicating the plasma in Saturn’s magnetosphere consists mostly of hydrogen and oxygen ions and molecular ions derived from water,” says Hamilton. “This suggests that the plasma probably comes from the surfaces of Saturn’s icy moons and rings, and not from the atmosphere of Titan, which consists primarily of nitrogen.” Plasmas are the most common form of matter, comprising more than 99percent of the known visible universe including the Sun and other stars. These ionized gases generate and interact with magnetic and electric fields around planets, stars and other astrophysical environments. Plasma processes can accelerate some ions to incredible energies. Cosmic rays — which are some of the highest energy plasma particles — contain “signatures” of the birth and death of stars. Observing the properties of space plasmas and energetic particles provides scientists a rich source of information about the physical processes that energize these materials and the conditions that exist at the sites where this energizing takes place.Magnetospheric Imaging

    September 20th, 2014 at 10:51 pm (#)

  354. Canada Goose Mujer says:

    STORY WRITTEN FOR & USED WITH PERMISSIONPosted: January 13, 2005Editor’s Note… Saturn currently is 751 million miles from Earth. One-way light time, i.e., the time needed for a radio signal to travel from the Cassini probe to Earth, is roughly 67 minutes. To avoid confusion, all times in the story below refer to “Earth received time,” or ERT. That is when an event, in theory, can be confirmed, not the time the event actually occurred.The European Space Agency’s Huygens probe, closing in on Saturn’s mysterious moon Titan, is racing toward a dramatic, high-speed plunge into the moon’s thick nitrogen atmosphere early Friday for a long-awaited parachute descent to an enigmatic surface. An artist’s concept shows Huygens parachuting to Titan after deployment from the Cassini orbiter. Credit: EADS AstriumReleased from NASA’s Cassini Saturn orbiter on Christmas Eve, the flying saucer-shaped probe is targeted to slam into Titan’s atmosphere at a velocity of 12,400 mph at 5:13 a.m. EST (1013 GMT). Over the next three to four minutes, the 705-pound probe is expected to endure peak heating of nearly 3,500 degrees and a braking force of some 16 Gs, slowing the craft to a more sedate 895 mph. At that point – 5:17 a.m. – the probe should release a small 8.5-foot pilot chute that will pull away a protective rear cover. Just 2.5 seconds later, the craft’s 27.2-foot-wide main parachute will unfurl. For the first time since pre-release tests, an on-board radio will begin transmitting data to Cassini around 5:18 a.m. as the NASA spacecraft streaks past Titan some 37,000 miles away. Huygens is expected to reach the surface of Titan around 7:31 a.m. But with its main antenna pointed toward the landing zone, Cassini will be out of contact with Earth, leaving anxious engineers and scientists in the dark until the NASA craft turns back toward Earth and begins transmitting recorded data around 10:17 a.m. That’s nearly three hours after Huygens touches down. “The probe is going to transmit data in realtime, Cassini will listen to them, but because Cassini is pointing its high gain antenna towards Titan, we would not be able to receive any data,” said Claudio Sollazzo, ESA’s Huygens operations manager. “So we will be here waiting for this data, but the mission will be over even before Cassini can turn back toward the Earth.” But if they’re lucky, scientists may get a near-realtime confirmation the probe survived the initial phases of its descent from large radio telescopes that will be monitoring the descent from Earth. No data will be received, but a carrier signal may be barely detectable. If so, project engineers and scientists will at least know Huygens survived entry. “This will indicate the probe is active, the probe is alive, the probe has entered the atmosphere of Titan, the main parachute has been deployed, the back cover has been removed and the computer has been activated,” Jean-Pierre Lebreton, ESA’s Huygens project scientist, told reporters Thursday. “It does not mean more than this (but) it tells us the probe is alive and descending under parachute.” Whether a carrier signal is detected or not, it will be a moment of high drama for the hundreds of scientists and engineers from Europe and the United States who have spent two decades planning Huygens’ Titan descent. “I’ve been involved in this mission almost 21 years,” said Lebreton. “I’m very excited, but I must say I’m also quite confident we’re going to see something very special.” Shaun Standley, an ESA systems engineer stationed at the Jet Propulsion Laboratory in Pasadena, Calif., echoed Lebreton’s confidence, saying on the eve of entry, “at this stage, it’s very, very, very exciting for all of us.” “The reason it’s exciting and not stressful is we know this is the absolute best that can be done,” he said in a telephone interview. “This represents a pinnacle achievement. It’s the best we can do and I’m looking forward to everybody sharing in that when these images and the rest of the science comes in.” Titan was discovered by Dutch astronomer Christiaan Huygens in 1655. Larger than both Pluto and Mercury, Titan has a dense nitrogen atmosphere and chemical processes that scientists believe mirror conditions on Earth shortly after the planet’s formation. Given the chemical constituents, the low temperatures and high pressures at the surface, theorist predict hydrocarbon rain and, possibly, lakes or streams of ethane and related compounds on the surface. Or, perhaps, some sort of hydrocarbon sludge. Cassini’s instruments failed to detect any obvious signs of liquids during two flybys of Titan in October and December. But Cassini was unable to resolve features smaller than about six tenths of a mile across and small pools or streams remain a possibility. Swinging beneath its main parachute in the hazy sky 90 to 100 miles above Titan, the half-dozen instruments aboard Huygens will begin sampling the atmosphere within moments of main chute deploy, probing its chemistry, looking for lightning and taking panoramic photographs. Nineteen minutes after entry, the main parachute will be released and a 9.8-foot drogue parachute will deploy to make sure the craft reaches the surface at the right time. Built at the University of Arizona, the probe’s innovative camera is known as the , or DISR. At an altitude of 90 miles above the surface, DISR will be able to detect surface features 500 feet across. But as it gets closer and closer to the surface, resolution will improve dramatically. “From 50 or 70 kilometers altitude (31 to 44 miles), we expect to break underneath the haze layer that’s made it so difficult to see the surface of Titan from the orbiter,” said Martin Tomasko, DISR principal investigator at the University of Arizona’s Lunar and Planetary Laboratory. “And from that point on down, we’ll have better than 20 times the best resolution that’s been obtained so far from the orbiter. “The views we’ve seen from the orbiter have been really tantalizing, they’ve given us the feeling that we’re looking at Titan through this veil of haze and it’s been extremely difficult to interpret these images to understand what the physical processes are that formed the surface, what’s really going on. It’s our hope that with the DISR cameras, basically the eyes in Huygens … for every kilometer that we descend, we’ll have that much less haze between us and the ground and we hope to have progressively clearer and clearer views and progressively higher and higher resolution.” Just before Huygens hits the surface, DISR should be able to resolve features smaller than a yard across. And it will continue transmitting from whatever surface it lands on. “If we land in a liquid, we may see us floating around in the liquid, we may see some features on the horizon,” Tomasko said. “If we land on a solid surface we’ll only see something from our aspect on the surface. In any case, the main mission will be from 150 kilometers (93 miles) to the ground. That’s where we expect to take our basic data and those data should provide a spectacular new view of Titan and hopefully a much clearer understanding of this new, mysterious world.” Here is a list of instruments aboard Huygens from the European Space Agency’s mission : Aerosol Collector and Pyrolyser (ACP) will collect aerosols for chemical-composition analysis. After extension of the sampling device, a pump will draw the atmosphere through filters which capture aerosols. Each sampling device can collect about 30 micrograms of material. Descent Imager/Spectral Radiometer (DISR) can take images and make spectral measurements using sensors covering a wide spectral range. A few hundred meters before impact, the instrument will switch on its lamp in order to acquire spectra of the surface material. Doppler Wind Experiment (DWE) uses radio signals to deduce atmospheric properties. The probe drift caused by winds in Titan’s atmosphere will induce a measurable Doppler shift in the carrier signal. The swinging motion of the probe beneath its parachute and other radio-signal-perturbing effects, such as atmospheric attenuation, may also be detectable from the signal. Gas Chromatograph and Mass Spectrometer (GCMS) is a versatile gas chemical analyser designed to identify and quantify various atmospheric constituents. It is also equipped with gas samplers which will be filled at high altitude for analysis later in the descent when more time is available.Huygens Atmosphere Structure Instrument (HASI) comprises sensors for measuring the physical and electrical properties of the atmosphere and an on-board microphone that will send back sounds from Titan.Surface Science Package (SSP) is a suite of sensors to determine the physical properties of the surface at the impact site and to provide unique information about its composition. The package includes an accelerometer to measure the impact deceleration, and other sensors to measure the index of refraction, temperature, thermal conductivity, heat capacity, speed of sound, and dielectric constant of the (liquid) material at the impact site. Huygens is expected to hit the surface of Titan at 7:31 a.m., plus or minus 15 minutes. With an impact velocity of 11 or 12 mph, “we have good hope that we are going to survive,” Lebreton said. “If we do, the probe is going to function as long as the batteries will provide electricity and the orbiter will continue to listen to the probe.” If Huygens lands in a liquid, ultra-low temperatures will sap the craft’s batteries faster than if it lands on a solid surface. On a solid surface, the batteries could, in theory, last two hours beyond the planned landing time, allowing the craft to beam data back to Cassini until the mothership disappears from view over Titan’s horizon. “We expect to get a total of about 750 images that have a lot of overlap in them and we expect to be able to put the closest images into context, in the view, with the images from farther away, from higher altitudes,” Tomasko said. “So I think we’ll be able to paint a pretty complete picture of the surface that is visible to the DISR cameras. As for DISR’s ability to distinguish between dark liquids and solid surface features, Tomasko said “we carry our own lamp and in the last couple of hundred meters, we will measure the specular reflectivity of the material we’re looking at as a function of wavelength. And we have already in our library the reflective spectra expected from liquid methane, liquid ethane, various mixtures of the two.” Also among the expected post-landing data are sounds from a microphone that might capture the rustling of frigid nitrogen winds or lapping waves. Sollazzo said Cassini will record four redundant sets of probe data that will be transmitted to Earth four times “just to make sure we do not lose any bit of information.” “So the first complete set will be here in the control center at 1900 local time (7 p.m. Central Europe Time, or 1 p.m. EST),” he said. “Within 40 minutes or even less, the control team will be able to deliver the science data from Huygens to our PIs (principal investigators). The team has already set up all their equipment and all their instrumentation to analyze the data realtime.” Here is a detailed timeline of major entry events (in EST/Earth received time). Explanations for key events from the European Space Agency’s ; Cassini timeline events provided by the :Friday02:33 AM (-02h40m) – Cassini solid state recorders prepped for support02:45 AM (-02h28m) – Cassini transition to thruster control for relay02:55 AM (-02h18m) – Cassini: final recorder configuration for relay02:57 AM (-02h16m) – Turn on Probe receivers03:09 AM (-02h04m) – Cassini turns toward Titan03:21 AM (-01h52m) – Turn to Titan complete03:24 AM (-01h49m) – Cassini disables X-band downlink04:51 AM (-00h22m) – Probe turns transmitters on (low power mode)05:13 AM (-00h00m) – Probe reaches the discernible atmosphere: 789 miles05:16 AM (+00h03m) – Probe feels maximum deceleration05:17 AM (+00h04m) – Pilot chute: 106-118 miles altitude; Mach 1.5; The parachute deploys when Huygens detects that it has slowed to 895 mph, at about 112 miles above Titan’s surface. The pilot parachute is the probe’s smallest, only 8.5 feet in diameter. Its sole purpose is to pull off the probe’s rear cover, which protected Huygens from the frictional heat of entry. 2.5 seconds after the pilot parachute is deployed, the rear cover is released and the pilot parachute is pulled away. The main parachute, which is 27.2 feet in diameter, unfurls.05:18 AM (+00h05m) – At about 99 miles above the surface, the front shield is released. Forty-two seconds after the pilot parachute is deployed, inlet ports are opened up for the Gas Chromatograph Mass Spectrometer and Aerosol Collector Pyrolyser instruments, and booms are extended to expose the Huygens Atmospheric Structure Instruments. The Descent Imager/Spectral Radiometer will capture its first panorama, and it will continue capturing images and spectral data throughout the descent. The Surface Science Package will also be switched on, measuring atmospheric properties.05:32 AM (+00h19m) – Main parachute separates and drogue parachute deploys: The drogue parachute is 9.8 feet in diameter. At this level in the atmosphere, about 78 miles in altitude, the large main parachute would slow Huygens down so much that the batteries would not last for the entire descent to the surface. The drogue parachute will allow it to descend at the right pace to gather the maximum amount of data.05:49 AM (+00h36m) – Surface proximity sensor activated: Until this point, all of Huygens’s actions have been based on clock timers. At a height of 37 miles, it will be able to detect its own altitude using a pair of radar altimeters, which will be able to measure the exact distance to the surface. The probe will constantly monitor its spin rate and altitude and feed this information to the science instruments. All times after this are approximate.05:56 AM (+00h43m) – Possible icing effects to Probe (31 miles)06:57 AM (+01h41m) – Gas Chromatograph Mass Spectrometer begins sampling atmosphere: This is the last of Huygens’s instruments to be activated fully. The descent is expected to take 137 minutes in total, plus or minus 15 minutes. Throughout its descent, the spacecraft will continue to spin at a rate of between 1 and 20 rotations per minute, allowing the camera and other instruments to see the entire panorama around the descending spacecraft.07:19 AM (+02h06m) – Cassini closest approach: 37,282 miles flyby at 12,080 mph, 93 deg phase07:30 AM (+02h17m) – Descent Imager/Spectral Radiometer lamp turned on: Close to the surface, Huygens’s camera instrument will turn on a light. The light is particularly important for the ‘Spectral Radiometer’ part of the instrument to determine the composition of Titan’s surface accurately.07:34 AM (+02h21m) – Surface touchdown: This time may vary by plus or minus 15 minutes depending on how Titan’s atmosphere and winds affect Huygens’s parachuting descent. Huygens will hit the surface at a speed of 11.2-13.4 mph. Huygens could land on a hard surface of rock or ice or possibly land on an ethane sea. In either case, Huygens’s Surface Science Package is designed to capture every piece of information about the surface that can be determined in the three remaining minutes that Huygens is designed to survive after landing.09:44 AM (+04h31m) – Cassini stops collecting data; Huygens’s landing site drops below Titan’s horizon as seen by Cassini and the orbiter stops collecting data. Cassini will listen for Huygens’s signal as long as there is the slightest possibility that it can be detected. Once Huygens’s landing site disappears below the horizon, there’s no more chance of signal, and Huygens’s work is finished.09:46 AM (+04h33m) – Cassini probe data partitions write protected09:54 AM (+04h41m) – Cassini turns toward Earth09:57 AM (+04h44m) – Turn to Earth complete10:06 AM (+04h53m) – Critical sequence ends10:07 AM (+04h54m) – Post-Probe tracking begins (Canberra)10:14 AM (+05h01m) – First data sent to Earth: Getting data from Cassini to Earth is now routine, but for the Huygens mission, additional safeguards are put in place to make sure that none of Huygens’s data are lost. Giant radio antennas around the world will listen for Cassini as the orbiter relays repeated copies of Huygens data.10:17 AM (+05h04m) – Probe data replay begins (Canberra: 66,360 bps)12:57 PM (+07h44m) – End playback of first partition01:04 PM (+07h51m) – Ascending ring-plane crossing: 18.4 Saturn radii02:00 PM (+08h47m) – Start tracking at Madrid (142,200 bps)05:07 PM (+11h54m) – End first full playback of all Probe data08:29 PM (+15h16m) – Full data set on Earth (likely three hours earlier)10:35 PM (+17h22m) – Start tracking at GoldstoneSaturday07:07 AM (+01d02h) – Power on of orbiter instruments08:30 AM (+01d03h) – End nominal playback of Probe dataAres 1-X PatchThe official embroidered patch for the Ares 1-X rocket test flight, is available for purchase.Apollo CollageThis beautiful one piece set features the Apollo program emblem surrounded by the individual mission logos.Expedition 21The official embroidered patch for the International Space Station Expedition 21 crew is now available from our stores.Hubble PatchThe official embroidered patch for mission STS-125, the space shuttle’s last planned service call to the Hubble Space Telescope, is available for purchase. | | | | 2014 Spaceflight Now Inc.Scientists elated by Cassini’s Titan observations BY WILLIAM HARWOOD

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