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http://kev65.Com <- Ŭ·´5678 Á¶°Ç¸¸³²,ÀÎÅÍ³Ý Á¶°Ç¸¸³²,äÆà Á¶°Ç¸¸³²,Á¶°Ç¸¸³² »çÀÌÆ®,¸Þ½ÅÀú Á¶°Ç¸¸³²,
http://kev65.Com <- Á¶°Ç¸¸³² °¡°Ý,Á¶°Ç¸¸³² ¿¬¶ôó,Á¶°Ç¸¸³² ÀÎÅͳÝ,°Ç¸¸³² »çÀÌÆ®,Á¶°ÇÀÖ´Â ¸¸³²,
http://kev65.Com <- Á¶°Ç¾ø´Â ¸¸³²,¿øÁ¶±³Àç,¸Å³Ê¸¸³²,µµ¿ò¸¸³²,Áö¼Ó¸¸³²,¾ßÇѸ¸³²,¾ß½ÃÇѸ¸³²,Àº¹ÐÇѸ¸³²,
http://kev65.Com <- È­²öÇѸ¸³²,Â¥¸´ÇѸ¸³²,ÆÄÆ®³Ê,ÆÄÆ®³Ê ±¸Çϱâ,¼½½ºÆÄÆ®³Ê,sexÆÄÆ®³Ê,sexpartner,
http://kev65.Com <- ¼½ÆÄ,¼½ÆÄ ±¸Çϱâ,›®ÆÄ,»öÆÄ,½ÙÆÄ,¿£Á¶ÀÌÆÄÆ®³Ê,¿£Á¶ÀÌÆÄÆ®³Ê ±¸Çϱâ,Á¶°Ç¸¸³² ÆÄÆ®³Ê,
http://kev65.Com <- Á¶°Ç¿©,Á¶°Ç³à,Á¶°Ç³à ±¸Çϱâ,´É·Â³²,¸Å³Ê³²,¾ó¯,¸ö¯,ÄýÄ«,Å·Ä«,ÂßÂß»§»§,Âß»§,¼½½Ã,
http://kev65.Com <- È­²ö°É,½ºÆù¼­±¸ÇÔ,¾ÖÀδëÇà,¿ªÇÒ´ëÇà,´ëÇàÀü¹®»çÀÌÆ®,¹ø°³ÆÃ,¹ø°³³à,¼­¿ï Á¶°Ç¸¸³²°É,
http://kev65.Com <- ºÎ»ê Á¶°Ç¸¸³²°É,´ë±¸ Á¶°Ç¸¸³²°É,±¤ÁÖ Á¶°Ç¸¸³²°É,´ëÀü Á¶°Ç¸¸³²°É,ÀÎõ Á¶°Ç¸¸³²°É,
http://kev65.Com <- °æ±â Á¶°Ç¸¸³²°É,¾È¾ç Á¶°Ç¸¸³²°É,°­¿ø Á¶°Ç¸¸³²°É,Ãæû Á¶°Ç¸¸³²°É,°æ»ó Á¶°Ç¸¸³²°É,
http://kev65.Com <- Àü¶ó Á¶°Ç¸¸³²°É,Á¦ÁÖ Á¶°Ç¸¸³²°É,¼­¿ïÁ¶°Ç¸¸³²,°æ±âÁ¶°Ç¸¸³²,¼ö¿øÁ¶°Ç¸¸³²,°­¿øÁ¶°Ç¸¸³²,
http://kev65.Com <- ´ëÀüÁ¶°Ç¸¸³²,±¤ÁÖÁ¶°Ç¸¸³²,ºÎ»êÁ¶°Ç¸¸³²,ÀÎõÁ¶°Ç¸¸³²,¿ï»êÁ¶°Ç¸¸³²,Á¶°Ç¸¸³² »çÀÌÆ®,
http://kev65.Com <- Á¶°Ç¸¸³²Á¦ÁÖ,Á¶°Ç¸¸³² ¼­¿ï,¸Þ½ÅÀú Á¶°Ç¸¸³²,Á¶°Ç¸¸³² °¡°Ý,Á¶°Ç¸¸³² ¾È¾ç,Á¶°Ç¸¸³² ¿¬¶ôó,
http://kev65.Com <- Á¶°Ç¸¸³² ÀÎÅͳÝ,½ºÆù¼­,½ºÆù±¸ÇÔ,´É·ÂÀִ½ºÆù,¼­¿ï½ºÆù,´ëÀü½ºÆù,°­¿ø½ºÆù,±¤ÁÖ½ºÆù,
http://kev65.Com <- ºÎ»ê½ºÆù,ÀÎõ½ºÆù,¿ï»ê½ºÆù,¾ßµ¿Ãµ±¹,¼½½ºÄÚ¸®¾Æ,¿À¸¶´ã,´ëµþ¹æ,¸Á°¡,¼ºÀθ¸È­,
http://kev65.Com <- ·¹À̰̽ɴ©µå ¹«·áÀΰ÷,ÀÌÀçÀº,ÃßÀÚ¿¬,Àå¹Î¾Æ,ȲÀοµ¼½½ÃÈ­º¸Áý,¿¬¿¹Àδ©µåÁý,´©µå°øÀ¯,
http://kev65.Com <- »çÁø ¹«·á°¨»ó,¼ºÀÎÈ­»óäÆÃ,¼ºÀξߵ¿,¿µÈ­°¨»ó,ÀϺ»AV¸ðµ¨,Çϵθ® ¾ßÇѵ¿¿µ»ó ¹«·á,
http://kev65.Com <- ¸ðÅÚ°¡À̵å,¸ðÅÚÅõ¾î,¸ð°¡,¿¹»ÛÆæ¼Ç Ãßõ,È£ÅÚ,¼÷¹Ú ¿¹¾à,¸ô·¡Ä«¸Þ¶ó,¸ôÄ«,È­»óÄ·,·¹À̰̽É,
http://kev65.Com <- ³ª·¹ÀÌÅÍ,¸ðµ¨,¼½½Ã,¸ð¹ÙÀÏÈ­º¸,¿±±â,À¯¸Ó,¼½½º,¼º±³,¼º°ü°è,°­°£,¾ß¼³,º¯ÅÂ,Å°½º,°¢¼±¹Ì,
http://kev65.Com <- ºñÅ°´Ï,±Û·¡¸Ó,ÀÓ½Å,·¹À̽Ì,ÆÒƼ,°¡½¿,ºê·¡Áö¾î,ÆÒƼ,¶õÁ¦¸®,¼Ó¿Ê,»ý¸®,È­Àå½Ç,¼ºÇü,¼ºÆøÇà,
http://kev65.Com <- ¼ºÃßÇà,µ¿°Å,´Ù¸®,¼º°ü°è,¹ß±â,´Ù¸®,È­°£,¿À¸£°¡½¿,È­°£,¼º±³À°,¼½½ºÃ¤³Î,³ªÃ¼,¸ÅÃá,À¯»ç¼ºÇà
http://kev65.Com <- °¥º¸,°­°£,°³»õ³¢,°³³â,±ÍµÎ,°ÌÅ»,±×·ì¼½½º,±ÙÄ£»ó°£,°íÃß,³ª°¡¿ä,²É¹ì,³­±³,ÀÚÀ§±â±¸,³ëºê¶ó
http://kev65.Com <- ³ëÆÒƼ,´Ï¹Ì,´Ü¶õÁÖÁ¡,´ëÆ÷Â÷,´ëÆ÷ÅëÀå,´ëÆ÷Æù,µôµµ,µþµþÀÌ,¶Ç¶óÀÌ,·Î¸®Å¸,·ë»ì·Õ,¸Á°¡,¸ÅÃá,
http://kev65.Com <- ¸ô·¡,¸ôÄ«,¸öÆĶó,¹«»èÁ¦ÆÇ,¹Ì¼Ò³à,¹Ì½Ã,¹Ì¾¾ÃÌ,¹Ì¾Æ¸®,¹ÌÄ£,¹ÙÀ̺극ÀÌÅÍ,¹ß±â,º¯ÅÂ,º´½Å,
http://kev65.Com <- ºÒ¾Ë,»¡±â,»çÁ¤,»çâ°¡,¼º°¨´ë,¼º±â±¸,¼º¹æ,¼º¿å±¸,¼ºÀοµÈ­,¼ºÀοëÇ°,¼ºÃ¼À§,¼ºÅ¬¸®´Ð,
http://kev65.Com <- ¼ºÅ×Å©´Ð,¼ºÇàÀ§,¼îÅ·,¼ö¿ë,½ºÅ¸Å·,½ºÅÍÇÁ,½º¿ÍÇÎ,½ºÆ®¸³¼î,¸¶½ºÅͺ£À̼Ç,¸¶¾à,½ÎÀÌÄÚ,º¸Áö,
http://kev65.Com <- ¾Æ°¡¸®,¿Í·¹Áî,¾Ö¹«,¿¢½ºÅͽÃ,¿øÁ¶±³Á¦,¾Ö¹«,¿¡·Î,¿À¶ö,¿À¸£°¡Áò,¿ëÁÖ°ñ,À¯µÎ,À¯¹æ,À°°¨,¿å±¸
http://kev65.Com <- À±¶õ,À½°æ,À½¶õ,À½¸ð,À½ºÎ,À̹Ý,ÀÚ»ì,ÀÚÀ§,ÀÚÁö,Àü¶ó,ÀüÈ­¹æ,Á¤»ç,Á¶°Ç¸¸³²,Á¶·ç,Á¿,Áú,â³à,
http://kev65.Com <- ÃÖÀ½Á¦,ü¸ð,üÀ§,Ä¡¸¶¼Ó,Ä«¼½½º,Ŭ¸®Å丮½º,¹ß±âºÎÀü,ºñ¾Æ±×¶ó,Æä´Ï½º,ÆäƼ½¬,ÆÒƼ,Æç¶óÄ¡¿À
http://kev65.Com <- Æ÷¸£³ë,Çϵθ®,ÇϵåÄÚ¾î,ÇîŸÀÌ,Ç×¹®,Çì·ÎÀÎ,È£½ºÆ¼½º,È¥À½,È­·ù,È­»óäÆÃ,¿©°í»ý,Äܵ¼,ºÎºÎ,
http://kev65.Com <- ¹ß±âºÎÀüÄ¡·áÁ¦,´Ù¹æ,µ¿¼º¾Ö,º¸µµ¹æ,Æä·Î¸ó,¹ß¸®Åõµµ,¼ºÀλçÀÌÆ®,¼ºÀξִÏ,±Ã,È­»óäÆÃ,äÆÃ,
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http://kev65.Com <- ¸á·Î,¹«Çù,¾¾³×,¹÷½º,µµ³ÊÃ÷,ºñµð¾î,¼ºÀι°,¼ºÀε¿¿µ»ó,¼½½Ã,¼½½º,½Ù½ÙÀÌ,Æ÷¸£³ë,Æ÷¸£³ëÀÚÅ°,
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As a result, technicians will be unable to re-install a rain cover over one of the ship's forward thrusters that was blown off during a recent storm.Water in the thruster can freeze as the shuttle climbs to space and interfere with operation of a pressure sensor. That, in turn, can fool the shuttle's computers into believing the thruster failed. But the thruster in question points to one side, not straight up, and engineers are hopeful any rain showers later today will not cause problems.Additional coverage for subscribers:VIDEO:TODAY'S LAUNCH ATTEMPT SCRUBBED VIDEO:CREW DEPARTS QUARTERS FOR THE PAD TODAY VIDEO:ASTRONAUTS SUIT UP FOR LAUNCH VIDEO:CREW'S LAUNCH MORNING SNACK TIME VIDEO:ATLANTIS CLEARED FOR LAUNCH FRIDAY   VIDEO:BRIEFING ON FUEL CELL DELAY   VIDEO:TUESDAY'S STATUS UPDATE BRIEFING   VIDEO:PRE-LAUNCH NEWS BRIEFING   VIDEO:MONDAY'S COUNTDOWN STATUS   VIDEO:BIOGRAPHY MOVIE ON THE SIX ASTRONAUTS VIDEO:SHORT MOVIE PREVIEW OF ATLANTIS' MISSION VIDEO:OUTLOOK ON UPCOMING STATION ASSEMBLY FLIGHTS VIDEO:CREW ARRIVES IN T-38 TRAINING JETS VIDEO:COMMENTS FROM CREW AFTER ARRIVAL VIDEO:NEWS BRIEFING ON RETURN TO PAD   VIDEO:ATLANTIS ROLLBACK BEGINS   VIDEO:OFFICIALS EXPLAIN LIGHTNING SCRUB VIDEO:SEE THE LIGHTNING STRIKE AT PAD B VIDEO:ANOTHER VIEW OF LIGHTNING STRIKE VIDEO:COMPLETE PREVIEW OF ATLANTIS MISSION VIDEO:DETAILS OF THE THREE SPACEWALKS VIDEO:MEET THE SIX ASTRONAUTS MORE: STS-115 patchThe official crew patch for the STS-115 mission of space shuttle Atlantis to resume orbital construction of the International Space Station.Choose your store: -  -  - 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. 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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.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.Gallery: Travels of AtlantisThis collection of photos shows space shuttle Atlantis' rollback from launch pad 39B forced by tropical storm Ernesto. 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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.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.Veteran credits rookies with saving the day on station     BY WILLIAM HARWOOD 14-12-02 20:58
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We're ready to press forward from here."Launch Director Mike Leinbach said engineers may move the launch pad service gantry away from Atlantis an hour or so early today to beat the onset of expected afternoon thunderstorms."If we get it back before the weather sets in, that's great," he said. "If not, we'll recover that time after the weather passes. Typically, we hold four or five hours in abeyance for RSS (rotating service structure) retract. So if we do get hit by the afternoon weather, that really shouldn't pose a problem for us."The Mission Management Team plans to meet at 1:45 a.m. Wednesday to assess the weather and give engineers clearance to proceed with loading Atlantis' external tank with liquid oxygen and hydrogen rocket fuel.Fueling is scheduled to begin at 2:33 a.m. and if all goes well, commander Brent Jett, pilot Chris Ferguson, flight engineer Dan Burbank, Joe Tanner, Canadian astronaut Steve MacLean and Heidemarie Stefanyshyn-Piper will begin strapping in around 9:09 a.m.Liftoff is targeted for 12:28:49 p.m. If Atlantis fails to get off the ground Wednesday, NASA can try again Thursday and Friday. After that, the flight will be delayed until after the Russians launch a fresh crew to the international space station Sept. 18 and bring the lab's outgoing crew back to Earth Sept. 29. The next daylight launch opportunity or the shuttle after Friday is Oct. 26.With an on-time launching, Atlantis will dock with the space station Friday at 8:40 a.m. The next day, a new solar array truss will be attached to the outpost and the crew will stage the first of three spacewalks to make critical electrical connections, remove launch restraints and perform other activation tasks.As it now stands, a second spacewalk would be carried out the next day, followed by solar array extension the day after that and then a third spacewalk. But managers may insert an extra day between the first two spacewalks to let the crew carry out "focused inspections" of the shuttle's heat shield based on whatever they see during an initial inspection the day after launch."We don't (currently) have that scheduled in the STS-115 timeline, but we know that is a likely possibility based on the flight day two or three inspections, that we'll need to go back and look at some areas in more focused detail," said shuttle Program Manager Wayne Hale. "There's a hope that perhaps we won't need to do that."The more difficult case for the team to execute, both the astronauts in orbit and mission control, is two back-to-back EVAs. If we need to do a focused inspection, the thinking is ... we would insert a day between the first and second EVAs. That becomes a somewhat lighter day for the crew and mission control, so it's an easier day to stand by for."What we'd really like to do is not have to do focused inspection, in other words, have such a clean vehicle that no inspections are required. Then we can save that day, bank it, and keep it (for) the end of the mission in case we run into any difficulties in the assembly process. Lifting off tomorrow or even the day after tomorrow, we really will have the capability to extend not one, but two days to the docked period so we would have the capability to handle both contingencies."If an extension day is, in fact, inserted after the first spacewalk, the second spacewalk would occur on Sept. 11, the fifth anniversary of the terrorist attacks on New York City and Washington.In other developments, Hale gave reporters an update on NASA's work to develop safer ice-frost ramps on the shuttle's external tank. The ice-frost ramps are buildups of foam insulation around brackets that support two pressurization lines and a cable tray. The insulation prevents ice from forming that could break off during launch and strike the shuttle.The IFRs are manually sprayed on and then sculpted on top of so-called acreage foam. Post-Columbia testing shows areas where foam is applied on top of other foam are susceptible to cracking due to differential thermal effects. Cracks, in turn, can lead to foam shedding during launch.The IFRs are officially classified as "probable/catastrophic," meaning there is a 50-50 chance of a catastrophic failure over the 100-flight life of a space shuttle. It is the only system on the shuttle that is so classified and NASA is developing a near-term fix to reduce the chances of foam debris breaking away."One of the options was to cover these little pieces of foam, about a pound or two pounds of foam at every bracket, cover them with a titanium shell, titanium being a metal that would retain the foam," Hale said today. "Titanium has a low thermal conductivity, so the hope was they could fasten that to this tank and not have ice form on the outside."They were unsuccessful in the environmental testing and the thermal testing to prevent ice from forming on the outside of the metal brackets. So the option (under development) is to reshape the foam, a reformulation of the foam to remove the SLA, or super-lightweight ablative foam core, and just use the standard foam."The all-foam design "will be what we take to the wind tunnel tests later this month to make sure it will hold together," Hale said. The new design is similar in appearance to an earlier design that broke apart during wind tunnel testing last spring. It was that failure that prompted NASA to stick with the current design, accepting the associated risk, while engineers developed an improved design."To the casual observer, it's not going to look a whole lot different than what we tried last April that didn't hold together in the wind tunnel," Hale said. "There are some differences internally in the way it's put together and some small shape differences. The bottom line is, we want to reduce the footprint."Every one of these 17 ice-frost ramps on the hydrogen part of the tank has a footprint of foam over foam, which is what we believe causes us concern with shedding of foam. So we have reduced the area of foam on top of foam, it's a much smaller footprint, and the thermal analysis indicates we will be much less susceptible to the thermally induced cracking that occurs in the underlying foam region, which is the goal of this exercise."This is an interim fix," Hale said. "We're coming back with a final fix in about eight more tanks after that. So we think we've got a good design, we'll put it in the wind tunnel later this month to make sure we've got a good design. We're going to have the critical design review before we start modifying the tank that's in production at the Michoud Assembly Facility, which we hope to ship about mid December."That tank, Hale said, will be used with shuttle mission STS-117 next February.Additional coverage for subscribers:VIDEO:MONDAY'S COUNTDOWN STATUS   VIDEO:BIOGRAPHY MOVIE ON THE SIX ASTRONAUTS VIDEO:SHORT MOVIE PREVIEW OF ATLANTIS' MISSION VIDEO:OUTLOOK ON UPCOMING STATION ASSEMBLY FLIGHTS VIDEO:CREW ARRIVES IN T-38 TRAINING JETS VIDEO:COMMENTS FROM CREW AFTER ARRIVAL VIDEO:NEWS BRIEFING ON RETURN TO PAD   VIDEO:ATLANTIS ROLLBACK BEGINS   VIDEO:OFFICIALS EXPLAIN LIGHTNING SCRUB VIDEO:SEE THE LIGHTNING STRIKE AT PAD B VIDEO:ANOTHER VIEW OF LIGHTNING STRIKE VIDEO:COMPLETE PREVIEW OF ATLANTIS MISSION VIDEO:DETAILS OF THE THREE SPACEWALKS VIDEO:MEET THE SIX ASTRONAUTS MORE: STS-115 patchThe official crew patch for the STS-115 mission of space shuttle Atlantis to resume orbital construction of the International Space Station.Choose your store: -  -  - Telescopes.comLargest selection and the best prices anywhere in the world. 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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.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.Heat shield cleared; Shannon talks night launches, Hubble     BY WILLIAM HARWOOD 14-12-04 12:30
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The shuttle's patched-up external fuel tank, its foam insulation heavily damaged by hail in February, appeared to withstand the rigors of launch without shedding any dangerous foam debris.    Credit: Ben Cooper/Spaceflight NowWith commander Rick Sturckow and pilot Lee Archambault at the controls, Atlantis' three hydrogen-fueled main engines roared to life and spun up to full throttle before ignition of the ship's twin solid-fuel boosters at 7:38:04 p.m.The fuel-laden 4.5-million-pound spaceship instantly climbed away from pad 39A at the Kennedy Space Center, wheeled about to line up on a northesterly trajectory and rocketed away up the East Coast to kick off NASA's 118th shuttle flight.Launch originally was scheduled for March 15, but the flight was put on hold after a freak Feb. 26 hail storm that blasted the top of the tank's foam insulation. More than 3,000 dings and gouges had to be repaired with poured or sprayed-on foam insulation, giving the tank a pockmarked, two-tone complexion.The first 135 seconds or so of flight are considered the most critical from a debris impact perspective because during that period, the shuttle is still in the lower atmosphere. Any lightweight foam debris that separates from the tank would decelerate rapidly in the thicker atmosphere, allowing the shuttle to run into it at a high relative velocity. Higher up in thinner air, debris does not slow as rapidly and impact velocities are lower.While detailed analysis of launch camera and video footage is not yet complete, television views beamed down from a camera mounted on the side of the tank showed a clean ascent with only one small piece of debris spotted just after solid rocket booster separation two minutes and five seconds after launch."We are glad to report that the external tank has performed in a magnificent manner," said shuttle Program Manager Wayne Hale. "I couldn't be prouder of the team and I think this bodes well for the future as we look forwared to the completion of the international space station."As for the debris, Hale said a preliminary analysis of launch video "indicates it didn't strike the orbiter.""It was at the very end, or just past, the aerodynamically sensitive time," he said. "Hopefully as we continue to make improvements in the tank we will eliminate even that, which should not be a hazard occurring that late in the flight."The remainder of Atlantis' eight-and-a-half-minute climb to orbit was uneventful. Aboard the space station half a world away, commander Fyodor Yurchikhin, flight engineer Oleg Kotov and Sunita Williams watched the launch on a video feed provided by flight controllers in Houston. If all goes well, Sturckow will guide the shuttle to a docking with the space station around 3:38 p.m. Sunday afternoon."What a great way to start the year and what a great way to start this mission," said Bill Gerstenmaier, chief of space operations at NASA headquarters.    The shuttle's launch exhaust creates a dazzling view over the Vehicle Assembly Building an hour after liftoff. Credit: Ben Cooper/Spaceflight NowThe primary goal of Atlantis' mission is to attach a huge new set of solar panels to the right side of the station's main power truss, along with a powerful rotary joint to keep the huge arrays face-on to the sun. The combined truss segments tip the scales at nearly 36,000 pounds, making this one of the heaviest space station payloads to date. The two new solar panels, when fully extended, will stretch 240 feet from tip to tip and slowly rotate like giant paddle wheels.The astronauts also hope to complete the retraction of another set of identical arrays, used to provide power to the lab complex during the initial stages of assembly, so it can be moved to its permanent position on the left end of the power truss later this year.The crew of shuttle Discovery ran into major problems retracting one side of the P6 array in December and ultimately staged an unplanned spacewalk, manually shaking free stuck grommets on frayed guide wires to fold the pleated blind-like array into its storage canister. While Atlantis' crew hopes to benefit from lessons learned and retract the remaining blanket automatically, they will be standing by to provide hands-on spacewalk assistance if necessary.Attaching the new $367.3 million S3/S4 solar array truss segments, completing the retraction of P6 and ultimately re-extending its two wings on the port side of the main power truss later this year will clear the way for attachment of European and Japanese research modules, both major milestones on the road to completing the station in 2010."I hesitate to say any part of the sequence is more critical than any other," NASA Administrator Mike Griffin told CBS News. "It's a chain and you can break any link, and the chain doesn't function. But you have to recognize that the sequence leading up to getting our first international partner module, the (European Space Agency's) Columbus lab, up is a very, very significant thing. It's going to assume an importance maybe even larger than it really has just because of the imagery of that."In August, the shuttle Endeavour will carry supplies to the station and attach a spacer segment to the S4 solar array installed during Atlantis' mission to permit the eventual attachment of a fourth and final set of arrays, known as S6.In October, Discovery will deliver a new multi-hatch node called Harmony, temporarily mounting it on the port side of the Unity module that connects the U.S. and Russian segments of the station. The astronauts then will move the retracted P6 solar array to its permanent location the left end of the main power truss in one of the most challenging assembly tasks yet attempted. If all goes well, the arrays will be re-extended, boosting the station's electrical power.After Discovery departs, the station crew will use the lab's robot arm to remove the shuttle docking port now on the forward end of the Destiny laboratory module and attach it to Harmony. The station astronauts then will move Harmony and its shuttle docking port to the front end of Destiny and stage a series of spacewalks to route power and cooling to the new module.That will set the stage for the long-awaited December launch of the Columbus research module, which will be attached to Harmony's starboard port. The Japanese Experiment Module will be bolted to Harmony's port hatch early next year."Everything now is pretty serial ... it is quite a production," said Anderson, a station crew member hitching a ride to the outpost aboard Atlantis. "We're going to put those pieces in place one step at a time and then if we do have any problems, we'll deal with those one step at a time such that we can get the Columbus module, the JEM modules on board the station, docked to Harmony, because that is a huge step to the international capability of the station. This is going to be a big four or five flights in a row."Under the original schedule, Anderson was to launch in June aboard the Endeavour, replacing astronaut Sunita Williams aboard the station as a member of the Expedition 15 long-duration station crew.But during an unusually violent storm that thundered over the launch pad on Feb. 26, Atlantis' external tank was blasted by hail. Most of the damage was restricted to the upper liquid oxygen section of Atlantis' tank and when all was said and done, it took three months to repair. As a result, Atlantis' flight slipped to June and Endeavour's to August.Williams was launched to the space station aboard Discovery last December. NASA managers initially said she could safely remain aloft until August but after additional consideration, they decided to bring her home in June, as originally planned, but on mission STS-117 instead of STS-118. Staying up through August was not a health threat for Williams, officials said, but her cumulative exposure to space radiation could preclude a future station flight. And so, the decision was made to bring her back to Earth on schedule aboard Atlantis.At the same time, NASA managers decided to move Anderson, Williams' replacement, from Endeavour to Atlantis.With today's on-time launch, Atlantis is scheduled to undock from the station June 17, leaving Anderson behind with Expedition 15 commanderYurchikhin and Kotov. Williams will return to Earth with Atlantis' crew, gliding to a touchdown at the Kennedy Space Center around 2:45 p.m. on June 19.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.Atlantis set to arrive at the space station today     BY WILLIAM HARWOOD 14-12-05 21:27
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Men Nike Roshe Full STORY WRITTEN FOR  & USED WITH PERMISSIONPosted: June 12, 2004    Cassini fires its engine to enter orbit around Saturn as illustrated in this artist's concept. Credit: NASA/JPLOn May 27, Cassini's flight computer fired the craft's main engine for six minutes and two seconds, setting up a June 11 flyby of Phoebe and fine-tuning the craft's trajectory for the all-important Saturn Orbit Insertion burn the night of June 30.   Trajectory Correction Maneuver 20 was a relatively short, but critical rocket firing because it marked the first use of the main engine system since the Deep Space Maneuver back in 1998. To everyone's relief, TCM-20 came off without a hitch. The helium latch valve opened 70 seconds before ignition and the leaky regulator worked as required to maintain the proper pressure.   "We've got a real nice propulsion system," said lead propulsion engineer Todd Barber. "It's a plumber's nightmare, there are so many valves and alternate paths and contingency paths available that basically, we're able to handle a lot of anomalies. And the regulator leak we saw was right after launch and we've been able to accommodate that with the way we time the opening of valves, etc."   Even so, Barber will feel much better after Cassini successfully brakes into orbit. "It's been a long time coming and the hopes and dreams of thousands of engineers are resting on that one evening. When we get the signal back is when we'll all go take a deep breath. Hold your ears, because they might pop."   To get into the desired orbit around Saturn, Cassini's main engine must fire for 96.4 minutes beginning at 10:35:42 p.m. EDT on June 30 (0235:42 GMT July 1). An underburn, or early cutoff, could doom the mission. Rocket Engine Assembly A - REA-A - must fire for more than 85 minutes to put Cassini into any kind of usable orbit. Asked what keeps him awake at night, program manager Bob Mitchell gave the obvious answer.   "In general, just worrying that SOI is going to work," he said in an interview. "The confidence that it will is very high, just based on all of the testing, all the elaborate work that we have put into this, as well as our experience with the spacecraft to date. We've done 15 or 16 maneuvers using the main engine ... and so we have every reason to believe this thing is going to work just fine."   But, he added, "the software the thing flies is all complex and I just worry about what bugs are still in there. I think it must be inevitable that there are still bugs in there for something this complex. We've tested it extensively, we have a test bed here in the basement of our building that is a quite high fidelity spacecraft simulator and the sequences have been run through there many, many times. We have injected faults, we've had various components break, where we simulated a break in the test bed and looked to see what response we got. And at the moment, everything works. All the tests that we've done, all the simulations indicate that everything is just fine."    This graphic shows the ring plane crossing and orbit insertion burn. Credit: NASA/JPLThe maneuver has little margin for error. Cassini first must avoid any crippling debris impacts when it crosses the ring plane between the F and G rings, moving from the lower side of the rings to the upper side as viewed from Earth.   Pioneers 10 and 11, along with Voyager 2, flew through the gap with no problems but Cassini flight planners are taking no chances. Before traversing the ring plane, the spacecraft will be oriented with its high-gain dish antenna facing the direction of travel to act as a shield.   Voyager 2 went through outer edge of the G ring and its instruments recorded "lots of evidence of micrometeoroid hits when going through, but nothing serious," said Voyager veteran Torrence Johnson, a Cassini imaging team member and chief scientist for the Galileo mission.   "So we have that maneuvering to do and then there's the fact that the place is just a junky system," he said in an interview. "We're going in close, we're skimming right over the rings, everybody thinks we've modeled all this right and we're being reasonably cautious. But I told some of the guys early on, if they're going to be scared of ring particles they ought to remember John Paul Jones' letter to Congress, 'give me a fast ship for I intend to sail in harm's way.'   "I don't think anybody's real complacent about this thing," Johnson said. "I think we've done everything we can to make sure we don't have any human or systems screw ups, but nature can still get you."   Jerry Jones, Cassini's chief navigator, said flying through the ring plane relatively close to Saturn will save propellant and makes the rocket firing more efficient. "But the real clincher, given all that, is the science in that close. We're going to be sitting there looking right down on those rings."   "We've got one class-A camera on this spacecraft," he said in an interview. "It's a beautiful telescope, it has great resolution, very sharp edges and for optical navigation, I'm just pleased as punch. ... The science opportunity going over the rings should be just fantastic, to say nothing of showing the public what they've paid for."   Once safely through the ring plane, Cassini will re-orient itself once again, swapping ends to put the main engine forward for the SOI burn. NASA originally planned to carry out the rocket firing "in the blind," with Cassini focusing on science observations while the engine put on the brakes. But in the wake of back-to-back Mars mission failures in 1999, NASA management ordered engineers to figure out a way for Cassini to provide at least some information about the start of the burn, its progress and its termination.    This graphic shows Cassini's track as it enters orbit around Saturn. Credit: NASA/JPL"So we went back and scrambled then," Barber said. "We had a compromise solution. We could have pointed the high-gain antenna to Earth during the whole burn and have telemetry but there was a large delta V (fuel) penalty to do so. So the plan is to switch to a low gain antenna and that will allow us to maintain Doppler during the burn."   While no actual data will be transmitted to Earth, analysis of the Doppler shift of a carrier signal from the spacecraft will tell engineers when the burn started, the precise deceleration it produces and when it stops.   "There were two key things we wanted to be sure we could differentiate between," Mitchell said. "One was in the event we just lost it entirely and never saw it again, we wanted to be able to differentiate between whether we had a problem going through the ring plane or whether we did that successfully and had a problem during the course of the burn itself. So with the data we have, we will know that quite well."   After re-orienting itself for SOI, Cassini will begin transmitting a carrier signal. Six minutes later, the burn will begin, showing up on computer screens at the Jet Propulsion Laboratory as a change in the slope of the carrier frequency. Thirty minutes later, the signal is expected to fade out for 25 minutes or so as Cassini passes behind Saturn's A ring as viewed from Earth.   Engineers then expect six minutes of carrier through the Cassini division before another 28-minute communications blackout while the spacecraft passes behind the broad B ring. Closest approach to Saturn - 12,400 miles from the planet's cloud tops - is expected at 12:03 a.m. EDT (0403 GMT) July 1, nine minutes before the SOI burn comes to an end. The first images and other data from the orbit insertion maneuver are expected around 8:39 a.m. EDT (1239 GMT).   Here is an edited timeline of critical events in the SOI maneuver for the evening of June 30 through the morning of July 1 (all times in EDT):    "We turn off of Earth line shortly prior to the ring plane crossing," Mitchell explained. "We turn to point the high-gain antenna in the direction we need to be in to shield the rest of the spacecraft and then there's a period of about an hour where we don't have any contact.   "Then when we turn back to go to the burn attitude, at about the time we get to that attitude, which is six minutes prior to the burn start, we will crank up a signal that comes from one of the low gain antennas. There's no telemetry, it's just a carrier.   "But that carrier will allow us to get Doppler and that'll tell us if the spacecraft is operating fine and has not had any safing events. And then during the course of the burn, that Doppler will let us see quite accurately what the acceleration levels are. So if the system is performing nominally or over performing or under performing, the Doppler will show that very well."   The day after orbit insertion, Cassini will pass within 205,000 miles of Titan, the first official Titan encounter of the mission and one that could prove, one way or the other, whether the spacecraft's cameras will be able to penetrate the hazy atmosphere as scientists hope. Between July 4 and 11, Cassini will be out of contact with Earth as Saturn passes behind the sun. The SOI sequence will end on July 30 as tour sequence No. 3 begins.   Sometime around Aug. 23, Cassini's main engine is scheduled to fire in what will be the last fully helium-regulated burn of the mission: a 51-minute maneuver that will change the spacecraft's velocity by 877 mph. The Perigee Raise Maneuver, or PRM, will raise the low point of Cassini's orbit and set up the first close flyby of Titan in October. After another flyby in December, the Huygens probe will be released for atmospheric entry during the mission's third Titan encounter in January.    Cassini's initial orbits around Saturn are illustrated in this graphic. Credit: NASA/JPLThe SOI maneuver is one of only three so-called "critical sequences" built into Cassini's mission software. A critical sequence is one that simply must execute properly to ensure mission success. The launch to Venus was one such sequence and the only other one is the Huygens data relay sequence.   SOI is "the only maneuver that we will do throughout the entire course of the mission where we just absolutely have to do this burn right now," Mitchell said at a news briefing. "If this burn doesn't work, then we would have a Saturn flyby and that's not what we're here about. So we have designed what we refer to as a critical sequence where no matter what fault might occur, the spacecraft will not let the burn halt. Now in some modes it will stop the burn, swap to the other engine and then continue on with the burn. But the burn will continue even in the presence of faults."   During normal operations, a problem with a spacecraft system would trigger fault-protection software that would shut down unnecessary activity, a condition known as safe mode. There are numerous variations, depending on the nature and timing of the fault and whether the spacecraft still knows its orientation in space. The end result, however, is the same: Cassini shuts down, finds the sun (Earth will never be more than six degrees away), switches to low-data-rate communications and awaits instructions from Earth.   Because of Saturn's great distance and the slow-speed radio link used in safe mode, engineers would need at least 48 hours to restore Cassini to normal operations. Such a fault during the SOI maneuver would shut the main engine down, interrupting the all-important rocket firing and possibly dooming the mission. But in critical sequence mode, that will not be allowed to happen.   "In critical mode, if the spacecraft detects a fault - we get a glint in the eye of the star scanner or the thrusters don't like what they're doing or a piece of hardware doesn't work right - the spacecraft will detect a fault," said Julie Webster, lead spacecraft engineer. "The sequence will halt and the spacecraft is allowed through its autonomous fault protection to go off and fix the fault.   "And then it will come back and say I've detected a fault, I've fixed the fault. And then it'll come back and say OK, critical sequence, you can restart. And the critical sequence will say Oh, but I've gotta remember where I was. We have what we call a mark and rollback strategy. So it'll roll back to the last good mark point and it will resend all the commands necessary to execute the next states that it needs to be in. It'll recommend all of those and continue on. And so, if there's a fault anytime during the critical sequence, it'll stop, halt, detect the fault, correct the fault and then restart the sequence."   That's where Cassini's second main engine comes in. If a fault of any kind interrupts the SOI sequence, the computer will fire up Rocket Engine Assembly B and continue the burn.    Cassini's two engines are seen in this pre-launch photo. Credit: NASA/JPL"In the burn, we have already disabled any fault protection activity that's not necessary to complete the burn," Webster said. "So we've got fault monitors, say, on the CDS (command and data system) computer and on the radio. Well, the radio's not necessary to complete a burn. Neither is the CDS, ironically, because the attitude and articulation control system also has its own computer and once the CDS has told it to go do a burn, it takes over and says I don't need you anymore, I'll complete this burn and I'll let you know when I'm done. So only the fault protection that's necessary to complete the burn is active.   "It would detect a fault in where it's pointing or the propulsion system wasn't acting right, maybe under thrusting or over thrusting. If there's a fault during the burn, then we terminate the burn. We try to fix the fault and then we mark and roll back, pick up where we did, restart but we're going to restart on the second engine. It takes at least two hours to cool down one engine. So 10 minutes later, we can restart on engine B and minimize our overall cost."   But any safe mode that would necessitate firing REA-B also would terminate priceless SOI science operations, a small price to pay if survival of the mission is at stake. Cassini has a seven-hour window in which to complete the SOI maneuver and "as long as we got the correct amount of burn at any time in that seven-hour period, we would get into orbit," Webster said. "We might not like the orbit, but we'd get into orbit."   While outwardly confident, many project officials are naturally anxious going into the make-or-break maneuver. But not Carolyn Porco. To her, the real issue is collecting the science required to meet Cassini's enormously challenging objectives.   "Everything's working very well. Cassini is a very robust spacecraft, the instruments are working very well and I have personally no worries about Saturn orbit insertion at all," she said. "That's not what worries me about Cassini. What worries me about Cassini is the magnitude of the job. It's absolutely enormous.   "What needs to be conveyed to people is the magnitude of this mission. It is not a Discovery-class mission. The breadth of its scientific objectives is tremendous. What we are going to do at Saturn will ultimately reach well beyond Saturn itself. It will teach us about the behavior of disk systems all throughout the universe. The processes going on in the disks of material from which planets are forming around other stars, it will tell us about what's going on in spiral galaxies, because the kind of things we find in Saturn's rings are directly applicable to what we find in galaxies.   "The study of Titan, it's the place to go in the solar system to find a body that is the most Earth-like. And so what we find at Titan will inform us about many aspects of the Earth and the behavior of its atmosphere, possibly processes that were part of the run up to the origin of life on Earth. On and on. It is really, truly the flagship mission of our time."MISSION PREVIEWStargaze II DVDThe Stargaze II DVD has arrived! It features over 65 minutes of all new videos of the universe with newly-composed dolby digital and DTS 5.1 Channel surround sound music. Choose your store: -  -  - Solar system poster  This new poster is popular for classrooms and children's bedrooms. It includes interesting facts and figures about the planets and their moons. Choose your store: -  -  - Apollo 15 DVD Relive on DVD the journey of Apollo 15, one of the great explorations of our time. This unique six-disc DVD set contains all the available television and 16mm film footage from the mission.Choose your store: -  -  - Shuttle patchesCollect the official mission patches for the first ten space shuttle flights and save off the regular price. Introducing the Space Shuttle Patch Collection.Choose your store: -  -  -  |  |  |   |   2014 Spaceflight Now Inc.Spaceflight Now +Premium video content for our Spaceflight Now Plus  .Cassini previewThe Cassini spacecraft's arrival at Saturn is previewed in this detailed news conference from NASA Headquarters on June 3. (50min 01sec file)Saturn arrival explainedCassini's make-or-break engine firing to enter orbit around Saturn is explained with graphics and animation. Expert narration is provided by Cassini program manager Robert Mitchell. (3min 33sec file)Cassini mission scienceThe scientific objectives of the Cassini mission to study the planet Saturn, its rings and moons are explained by Charles Elachi, director of the Jet Propulsion Laboratory. (4min 54sec file)Huygens mission scienceAfter entering orbit around Saturn, the Cassini spacecraft will launch the European Huygens probe to make a parachute landing on the surface of the moon Titan. The scientific objectives of Huygens are explained by probe project manager Jean-Pierre Lebreton. (3min 14sec file)Saturn's moon Iapetus as you've never seen it      CASSINI PHOTO RELEASEPosted: December 8, 2004New details on Iapetus are illuminated by reflected light from Saturn in this revealing Cassini image. Never-before-seen features on the Saturn-facing part of Iapetus' bright trailing hemisphere are visible for the first time, including many dark spots, and a sharper view of a dark, circular structure that was first seen at very low resolution by NASA's Voyager 1 in 1980. Iapetus diameter is 1,436 kilometers (892 miles).     Credit: NASA/JPL/Space Science InstituteThe image shows mainly the night side of Iapetus; part of the far brighter sunlit side appears at the right and is overexposed due to the long integration time of 180 seconds. Despite this long exposure time, almost no blurring due to the spacecraft's motion is apparent. This technique for imaging the night side of Iapetus will be used again during a flyby on Jan. 1, 2005, when Cassini will pass 13 times closer to the icy moon. The image was taken in visible light with the Cassini spacecraft narrow angle camera on Oct. 22, 2004, at a distance of 1.6 million kilometers (994,000 miles) from Iapetus, and from a Sun-Iapetus-spacecraft, or phase, angle of 161 degrees. The view is centered on 0.4 degrees north latitude, 317 degrees west longitude on Iapetus. The image scale is 9.4 kilometers (5.8 miles) per pixel.     Credit: NASA/JPL/Space Science InstituteDownload larger image version IMAGE 2 These spectacular Cassini images of Saturn's moon Iapetus show an enticing world of contrasts. These are the sharpest views of Iapetus from Cassini so far, and they represent better resolution than the best images of this moon achieved by NASA's Voyager spacecraft. Images obtained using ultraviolet (centered at 338 nanometers), green (568 nanometers) and infrared (930 nanometers) filters were combined to produce the enhanced color views at left and center; the image at the right was obtained in visible white light. The images on the bottom row are identical to those on top, with the addition of an overlying coordinate grid. These views show parts of the moon's anti-Saturn side--the side that faces away from the ringed planet--which will not be imaged again by Cassini until Sept., 2007. In the central view, part of the moon's eastern edge was not imaged and appears to be cut off. With a diameter of 1,436 kilometers (892 miles), Iapetus is Saturn's third largest moon. It is famous for the dramatic contrasts in brightness on its surface--the leading hemisphere is as dark as a freshly-tarred street, and the trailing hemisphere and poles almost as bright as snow. Many impact craters can be seen in the bright terrain and in the transition zone between bright and dark, and for the first time in parts of the dark terrain. Also visible is a line of mountains that appear as a string of bright dots in the two color images at left, and on the eastern limb in the image at right. These mountains were originally detected in Voyager images, and might compete in height with the tallest mountains on Earth, Jupiter's moon Io and possibly even Mars. Further observations will be required to precisely determine their heights. Interestingly, the line of peaks is aligned remarkably close to the equator of Iapetus. The large circular feature rotating into view in the southern hemisphere is probably an impact structure with a diameter of more than 400 kilometers (250 miles), and was first seen in low-resolution Cassini images just two months earlier. Theses images were taken with the Cassini spacecraft narrow angle camera between Oct, 15 and 20, 2004, at distances of 1.2, 1.1 and 1.3 million kilometers (746,000, 684,000 and 808,000 miles) from Iapetus, respectively. The Sun-Iapetus-spacecraft, or phase, angle changes from 88 to 144 degrees across the three images. The image scale is approximately 7 kilometers (4.5 miles) per pixel. 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 Office of Space Science, Washington, D.C. The Cassini orbiter and its two onboard cameras, were designed, developed and assembled at JPL. The imaging team is based at the Space Science Institute, Boulder, Colo. 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.Saturn's moon Phoebe likely born in outer solar system      BY WILLIAM HARWOOD 14-12-13 05:02
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Air Max Thea Women STORY WRITTEN FOR  & USED WITH PERMISSIONPosted: January 14, 2005NASA's Cassini Saturn orbiter began downlinking science data from theEuropean Space Agency's Huygens probe at 11:19 a.m. EST (1619 GMT), confirming thespacecraft not only survived its high-speed plunge into the atmosphere ofSaturn's moon, Titan, but that its instruments worked to remotely exploreone of the strangest worlds in the solar system."Cassini has just started to deliver the data collected during thedescent," said Jean-Jacques Dordain, director general of the Eruopean SpaceAgency. "This is a fantastic success for Europe!"Cassini and Huygens mission managers, scientists and engineers eruptedin cheers and applause when the first data packets began showing up oncomputers screens at the European Space Agency's Space Operations Center inGermany. Successful reception of science data capped a morning of high dramaand ended any uncertainty that Europe had achieved one of its mostimpressive engineering and scientific triumphs."All instruments are on,"  a flight controller told the Huygens team.Mission managers already knew Cassini had survived its hellish plungeinto Titan's atmosphere and had made it to the moon's surface because of anunimaginably faint carrier signal that was detected by a network ofEarth-based radio telescopes. The signal, some 50 quadrillion times weakerthan a typical FM radio signal in a car radio, proved Huygens had survivedentry, deployed its main parachute and activated critical subsystems. Thesignal lasted more than two hours after the predicted landing, but it didnot carry any scientific data. It was merely a tone and while it showed thecraft was alive, it didn't prove whether it had accomplished its scientificobjectives.But the European spacecraft apparently worked as advertised and right onschedule, after Cassini dropped below Titan's horizon, the NASA mothershipturned back toward Earth and began transmitting data from Huygens' suite ofsix instruments."So the morning was good. The afternoon is better," Dordain said at anews conference. "This morning, we had an engineering success and we can saythis afternoon that we also have a scientific success. We are the firstvisitors to Titan and the scientific data we are collecting now shall unveilthe secrets of this new world."It will take several hours for mission scientists and engineers toextract and stitch together pictures from the data stream, but the firstpanoramic views showing the surface of Titan as Huygens descended throughits hazy atmosphere may be available between 5 p.m. and 6 p.m."The torch has been handed off from the engineers ... who've done theirjob of delivering the probe and delivering the data back," said DavidSouthwood, European Space Agency science director. "Now the scientists startwork. We're going to be working, I think, very hard in the next hours anddays but in fact, this data is data for posterity."This is a historic event. I don't think it's likely in the lifetime ofanyone in this room that we will repeat a landing on Titan. so this is thedata, it's for posterity, it's for mankind. But it's got to be unraveled,it's got to be put together and then scientists, being scientists, are goingto argue about what it means as we piece together our place in the universeand how we came to be. I think this is a very major step forward. But it'sonly the beginning for our science teams."NASA science chief Al Diaz choked back tears as he called the probemission "a tremendous success.""This really is another first," he said. "There will only be a firstsuccessful landing on Titan and this was it. The European Space Agencydeserves a tremendous amount of credit. We're glad we could have been apartner."Claudio Sollazzo, ESA's Huygens operations manager, said engineers wereinvestigating the apparent loss of data from one of two channels, or chains,of telemetry from Huygens. But he said the spacecraft was fully redundantand that "we can ensure that so far, on chain B, we see everything wentwell.""The probe went through the entry phase and the (main) parachute wasdeployed essentially at the time we predicted," he said. "We are anxious tosee what we call the history data, the telemetry that was recorded on boardthe probe before even the back cover came off so we can reconstruct how theprobe entered the atmosphere. This is very important information for thescientists to know how the higher atmospheric layers are. it is also veryimportant for the engineering community."Data on chain B showed "the batteries are OK, the computers worked asexpected, the software shows healthy status and instrument status as far aswe could receive ... were nominal," Sollazzo said. "The internal temperatureof the probe was about 25 degrees centigrade. So ... our instruments areworking at a very comfortable temperature."One of Huygens' six experiments, the Doppler Wind Experiment, relied inpart on chain A of the probe's communications system. It was designed tomeasure wind speeds by detecting subtle changes in the frequency of radiotransmissions as th craft is blown this way or that. If chain A did notwork, scientists will lose measurements of that shift between Huygens andCassini. But Sollazzo said similar measurements from Earth-based radiotelescopes will allow scientists to collect similar data to make up theshortfall, assuming the data on chain A is, in fact, lost."We have a wonderful mission on Titan," he said, "and we are eager todeliver the data to our scientists on time and then they will go on andanalyze the data and we should get some interesting results later tonight."Video coverage for subscribers only:VIDEO:STATUS REPORT DURING DESCENT   AUDIO:TODAY'S STATUS REPORT DURING DESCENT VIDEO:HUYGENS PRE-ARRIVAL NEWS BRIEFING   AUDIO:HUYGENS PRE-ARRIVAL NEWS BRIEFING VIDEO:OVERVIEW OF HUYGENS PROBE'S SCIENCE OBJECTIVES VIDEO:JULY NEWS BRIEFING ON CASSINI'S PICTURES OF TITAN VIDEO:PICTURES SHOWING TITAN SURFACE FROM OCT. FLYBY VIDEO:WHAT'S KNOWN ABOUT TITAN BEFORE THE FIRST FLYBY VIDEO:NARRATED MOVIE OF CLOUDS MOVING NEAR SOUTH POLE VIDEO:OCT. BRIEFING ON RADAR IMAGES OF TITAN SURFACE 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.Huygens test successful      EUROPEAN SPACE AGENCY NEWS RELEASEPosted: September 19, 2004ESA's Huygens probe, now orbiting Saturn on board the NASA/ESA/ASI Cassini spacecraft, is in good health and successfully passed its fifteenth 'In-Flight Checkout' on 14 September 2004.    An artist's concept shows Huygens parachuting to Titan after deployment from the Cassini orbiter. Credit: EADS AstriumThis in-flight checkout procedure was the last but one planned before separation of the Huygens probe from Cassini in December this year, and it included some specific activities that were intended to prepare for the separation. The main difference in this procedure from previous checkouts was that there was a test of the Master Timer Unit (MTU). Because Huygens will spend three weeks coasting towards Titan following separation from the Cassini orbiter, its systems and instruments are powered down. The MTU is the 'triple-redundant' alarm-clock that has the most important job of waking up Huygens a few hours before its entry into Titan's atmosphere. The checkout also included some specific payload activities required to configure the Huygens instruments before separation. The procedure was carried out live, with Cassini transmitting the data to Earth in real-time. However the data arrived on Earth with an 80-minute delay as this is the time taken for light, and therefore radio signals, to travel the distance between Saturn and Earth. The preliminary analysis of the real-time data received, performed within 12 hours after the test, indicates that the MTU test was successful, and that all instruments performed as expected.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.Spaceflight Now +Premium video content for our Spaceflight Now Plus subscribers.Huygens mission scienceAfter entering orbit around Saturn, the Cassini spacecraft will launch the European Huygens probe to make a parachute landing on the surface of the moon Titan. The scientific objectives of Huygens are explained by probe project manager Jean-Pierre Lebreton. (3min 14sec file)Saturn's moon TitanLearn more about Saturn's moon Titan, which is believed to harbor a vast ocean, in this narrated movie. (4min 01sec file)Relive Cassini's launchAn Air Force Titan 4B rocket launches NASA's Cassini spacecraft at 4:43 a.m. October 15, 1997 from Cape Canaveral, Florida. (5min 15sec file)Iapetus: A view from the top      CASSINI PHOTO RELEASEPosted: January 9, 2004This oblique view of Saturn's moon Iapetus from high latitude shows how the dark, heavily cratered terrain of Cassini Regio transitions to a bright, icy terrain at high latitudes.     Credit: NASA/JPL/Space Science InstituteDownload larger image version In this mosaic of two high resolution images taken during Cassini's New Year's Eve 2004 flyby of Iapetus, the direction toward the north pole is approximately 15 degrees below the horizontal on the right. At the equator terrains are uniformly covered with a dark mantle of material that has a reflectivity of about 4 percent. At latitudes toward the pole of about 40 degrees, the dark deposits become patchy and diffuse as the surface transitions to a much brighter, icy terrain near the pole. The brightest icy materials exhibit visual reflectivity over 60 percent. Superimposed on the bright terrain is a subtle, ghostly pattern of crudely parallel, north-south trending wispy streaks. The streaks, which were discovered during this flyby of Iapetus, are typically a few kilometers wide and sometimes tens of kilometers long. Their appearance and orientation may be connected with the emplacement of dark materials that cover Cassini Regio. The dark materials might represent the gradual accumulation of dark debris falling from space, or alternatively, may represent fallout from plume-style eruptions that may have accompanied the formation of Iapetus's enigmatic equatorial ridge. Also seen in this mosaic are conspicuous, north-facing bright crater walls. An example can be seen in the upper left where the bright, 4-kilometer-high (2.5 miles) walls of a 70 kilometer (44 mile) central-peak crater lies. The bright crater walls are often higher in brightness than the corresponding south-facing walls of the same crater. They are vaguely reminiscent of bright north-facing crater walls that were discovered by NASA's Voyager and Galileo spacecraft in craters near the poles of the Jovian satellites Callisto and Ganymede. In the case of the Jovian satellites, cold-trapping of frosts on north-facing slopes and sublimation of ices from south-facing slopes are thought to produce the north-south asymmetries in crater wall brightness. However, the occurrence of some young-appearing craters on Iapetus that have bright north-facing and dark south-facing slopes, and the pattern of streaks near the north pole of Iapetus suggests that another mechanism may be responsible for the crater wall brightness asymmetries on Iapetus. One possibility is that the south-facing slopes may be stained by the same process that emplaced the low brightness coating throughout the region. In this case, the north-pointing scarps might be bright because they face away and are shielded from the putative falling spray of dark materials. Bright south-facing slopes would exist primarily on young craters that have not been exposed to the darkening agent long enough to be stained. The image was obtained in visible light with the Cassini spacecraft narrow angle camera on Dec. 31, 2004, at a distance of about 123,370 kilometers (76,658 miles) from Iapetus and at a Sun-Iapetus-spacecraft, or phase, angle of 93 degrees. Resolution achieved in the original image was 732 meters (2,401 feet) per pixel. 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 mission for NASA's Science Mission Directorate, Washington, D.C. The Cassini orbiter and its two onboard cameras were designed, developed and assembled at JPL. The imaging team is based at the Space Science Institute, Boulder, Colo. 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.Instrument aims at Saturn's space environment      JHU-APL NEWS RELEASEPosted: June 30, 2004As NASA's Cassini-Huygens spacecraft begins its four-year orbital tour of the Saturn system, mission scientists will use an innovative imaging device to deliver the most detailed look yet at the relationship between the Sun, the giant ringed planet and the diverse collection of moons looping around it.The Magnetospheric Imaging Instrument - or MIMI - is one of 12 science instruments on the main Cassini spacecraft, set to enter orbit around Saturn on July 1 (EDT). The MIMI experiment, an international team effort led by the Johns Hopkins University Applied Physics Laboratory (APL), Laurel, Md., includes three distinct sensors that will profile the environment of charged particles at Saturn and obtain the first visible, global images of Saturn's magnetosphere."Until now, measuring a planet's magnetic field and charged particle environment - its magnetosphere - has been difficult," says Dr. Stamatios (Tom) Krimigis, of APL, MIMI principal investigator. "A spacecraft can measure it at one point when it flies past a planet, but you don't know what's happening somewhere else and you never get the entire picture. With our instrument, and from orbit around the planet, we'll be able to look at the changing patterns and dynamics of Saturn's space weather - actually see how it reacts to the solar wind over time and how it affects the surfaces and atmospheres of the moons embedded in the magnetosphere."MIMI's sensors combine three critical measurements to create that picture. Its high-energy particle detector (developed by APL, the Max Plank Institute and a number of co-investigator institutions) looks at the distribution and strength of energetic ions and electrons near the spacecraft. Its charge-energy mass spectrometer (built by the University of Maryland, College Park) measures the charge and determines the elemental composition of these particles.MIMI's ion and neutral camera takes a wider approach, using an APL-developed technique known as energetic neutral atom imaging to provide a global view of the entire magnetosphere - a deep-space mission first. The camera detects the "glow" of energized particles trapped in the planet's magnetic field, which will allow scientists to make three-dimensional images of the compression and expansion of Saturn's magnetosphere as it's buffeted by the solar wind, or as it sends streams of particles toward the surfaces of Titan and other nearby satellites."Magnetospheres can change dramatically over a matter of hours to days, so flybys such as the Voyager spacecrafts' only yield a snapshot in time and space," says MIMI Instrument Scientist Dr. Donald Mitchell, of APL. "With Cassini we're going to get years and years of nearly continuous data, which will give us a much more complete understanding of this complex system. We'll be able to watch the whole dynamic between the sun and Saturn, and the planet and its moons."The camera was pointed toward Saturn's magnetosphere four months ago and has already collected impressive data, Mitchell says. MIMI had a successful test run during Cassini's flight past Jupiter in late 2000-early 2001, providing scientists with never-before-seen images of the giant planet's magnetosphere and underlying dynamics; a huge nebula of particles - spewed from volcanoes on the moon Io - enveloping Jupiter and extending some 22 million kilometers (13 million miles) past the planet; and a large and surprisingly dense gas cloud sharing an orbit with Jupiter's icy moon Europa.While the mission at Saturn is just beginning, Krimigis expects MIMI's data will eventually give scientists a better understanding of the space environment closer to home."Planetary magnetic fields have a lot in common, even if the planets themselves are very different," he says. "We hope to find some of the characteristics that affect both the Earth and Saturn, and feed this knowledge back into the models we have for space weather at Earth. Then we can devise accurate space weather forecasts that give advance warning of the electromagnetic storms that affect our satellites, communications, power grids and other technological systems."Including the APL-built MIMI, half of Cassini's instruments are designed to investigate the space environments around Saturn and its moons. Cassini - launched on Oct. 15, 1997 - will also release its piggybacked Huygens probe, built by the European Space Agency (ESA), this December for descent through the thick atmosphere of the moon Titan.The Cassini-Huygens mission is a cooperative project of NASA, ESA and the Italian Space Agency. The Jet Propulsion Laboratory, a division of the California Institute of Technology in Pasadena, manages the $3.3-billion mission for NASA's office of Space Science, Washington, D.C. The MIMI team includes investigators and expertise from APL; the University of Maryland, College Park; University of Kansas, Lawrence; University of Arizona, Tucson; Bell Laboratories, Murray Hill, N.J.; the Max Planck Institute for Solar System Research, Lindau, Germany; and the Centre d'Etude Spatiale des Rayonnements in Toulouse, France.The Applied Physics Laboratory, a division of The Johns Hopkins University, meets critical national challenges through the innovative application of science and technology.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.Latest color pictures from Cassini look like artwork      CASSINI PHOTO RELEASEPosted: August 19, 2004NASA has released three new stunning color pictures taken by the Cassini spacecraft exploring the planet Saturn. The images show the giant planet, its golden rings and several moons.    Credit: NASA/JPL/University of ArizonaDownload larger image version FIRST IMAGE: Saturn's atmosphere is prominently shown with the rings emerging from behind the planet at upper right. The two moons on the left of the image are Mimas and Enceladus. This image was taken on August 8, 2004, with the Cassini spacecraft narrow angle camera in red, green, and blue filters. This image was taken 8.5 million kilometers (5.3 million miles) from Saturn. Contrast has been enhanced to aid visibility.     Credit: NASA/JPL/University of ArizonaDownload larger image version SECOND IMAGE: Saturn's rings appear golden as the planet's shadow drapes across nearly the whole span of the rings. In the upper left corner is Saturn's moon Mimas. This color image was taken on August 15, 2004, with the Cassini spacecraft narrow angle camera, using the red, green, and blue filters. The image was taken 8.8 million kilometers (5.5 million miles) from Saturn. Contrast has been enhanced to aid visibility.     Credit: NASA/JPL/University of ArizonaDownload larger image version THIRD IMAGE: Saturn and its rings are prominently shown in this color image, along with three of Saturn's smaller moons. From left to right, they are Prometheus, Pandora and Janus. Prometheus and Pandora are often called the "F ring shepherds" as they control and interact with Saturn's interesting F ring, seen between them. This image was taken on June 18, 2004, with the Cassini spacecraft narrow angle camera 8.2 million kilometers (5.1 million miles) from Saturn. It was created using the red, green, and blue filters. Contrast has been enhanced to aid visibility. 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 Cassini orbiter and its two onboard cameras were designed, developed and assembled at JPL. 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.Mission has faced many hurdles and challenges      BY WILLIAM HARWOOD 14-12-15 19:14
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Nike Air Max Light sorti le mois dernier parlait de rupture et visiblement avait vu juste La chanteuse de 22 ans a en effet décidé de mettre un terme à sa relation avec Conor Kennedy La raison Le jeune homme de 18 ans "nétait pas prt pour une histoire sérieuse" selon ce qu'a expliqué une source proche du couple au site "Radar Online" "Taylor recherche lme sur et son obsession a un peu fait flipper Conor"Egalement en cause : les tendances fantasques de la chanteuse mettaient Conor mal-à-laise notamment sa fascination pour le clan Kennedy "Taylor est obsédée par les Kennedy et vivait un conte de fée avec Conor Mais ce qui lintéressait avant tout cétait de sortir avec un Kennedy par forcément le Kennedy avec qui elle sortait" explique la sourceElle achète une maison proche de son exTaylor Swift risque cependant de ne pas trop s'éloigner de son ex Cet été la chanteuse alors en pleine love story avec son boyfriend prévoyait d'acquérir une maison d'une valeur de 45 millions de dollars située tout à cté de la maison de vacances des Kennedy dans la région de Cape Cod sur la cte Est des Etats-Unis Un achat qu'elle prévoit toujours de faire malgré sa rupture avec Conor Kennedy Selon le magazine "Ok" qui a contacté l'agence immobilière chargée de la vente la chanteuse compte en effet toujours acquérir la maison en question et la vente devrait tre finalisée d'ici deux semaines La fascination de Taylor Swift pour les Kennedy va peut-tre un chouilla trop loin. il ëÎrit et r?lise Akoibon, elle nous avait manqué l'intro désormais traditionnelle de et son petit cté mélodramatique. ?servita a creare un vuoto mediatico che Sark?intende riempire con i contenuti: lavoro immigrazione e un nuovo libro che ripercorre le cose fatte nel quinquennio e quelle da fare Senza lasciare spazio ad altriAd esempio a Marine Le Pen a cui ha gi?rosicchiato un punto percentuale La leader del Front national ?al 175% ma con l?ncognita sulle firme necessarie a candidarsi al primo turno Sarkozy fa la parte del moderato: la sua squadra ha un altro volto destrorso Il ministro dell?nterno Claude Gu?nt che ha detto: Non tutte le culture sono uguali. Joseph Gordon Levitt.7 e 43 metri - sono in alluminio mentre boma avvolgibili e crocette sono in carbonio A Reatech Handy Superabile.O Val?ie B?ue se dëÎide finalement ?se pr?enter au concours de Miss R?nion. Qualcuno.Intervilles 14-12-23 13:10
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Billige MØÏnd Nike F ?he high school music directors do such a fantastic job of getting this all set up,?said Sara Eikenberry, the band director for Butler Junior High School in Oak Brook. Eikenberry had 41 seventh and eighth-graders with her from the school? concert band, which performed the ?arch Zuma.? 14-12-23 14:17
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Air Max Fitsole Mens 5 million and the drought is expected to shave about a percentage point off economic growth. first-served basis. Due to the high volume of applicants, I'm about to go eat me some donuts and play me some Modern Warfare 3." we can't blame that on "Survivor. nor even from Europe -- the first time that's happened, but the crowd in Rome didn't seem to mind, She also received, She is one of the few journalists to have flown in a B-52 on a combat mission in Kosovo and in an F-15 fighter jet Combat Air Patrol flight. is that if they have high blood pressure (hypertension) or diabetes. 14-12-27 05:41
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