Tuesday, October 13, 2009

Orion Main Parachute Testing Technique Demonstrated

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NASA and engineering support contractors completed a demonstration test of the main parachute test equipment for the Orion crew exploration vehicle Oct. 2 at the U.S. Army’s Yuma Proving Grounds in Yuma, Ariz.

The demonstration is part of a series of tests to support the design and development of the Orion parachute recovery system, which is derived from the system NASA used to recover the Apollo spacecraft.

In August 2008, NASA experienced an anomaly in the test technique when deploying a full-scale Orion boilerplate parachute test vehicle (PTV). To improve the testing technique and prevent such an anomaly from occurring again, NASA is developing “smart” systems to make the extraction of large, oversized payloads from the C-17 aircraft repeatable and creation of the right test conditions more reliable.

For the recent test, a 20,700-pound test vehicle was extracted from a C-130 aircraft at an altitude of 20,500 feet. The test conditions simulated the dynamic environment that the test vehicle experiences when extracted from an aircraft. The new “smart” avionic systems are designed to sense the attitude and pitch rate of the test vehicle and trigger the proper time to release the vehicle from the test platform to begin the parachute test. All of the new avionics worked as planned, recorded the proper release points and the equipment landed safely.

The test vehicle consisted of a nine-foot-wide by 24-foot-long platform with a 16-foot-long weight tub. The tub included a backstop structure to provide a positive angle of attack when the vehicle was descending under the programmer parachute. Honeycomb was built up on the weight tub to simulate the profile and aerodynamics of the actual test vehicle that will be used in later testing. Simulating the aerodynamics of the vehicle is important since that contributes to the pitch motion when the vehicle is extracted from an aircraft.

The next demonstration of the new test equipment is scheduled for November 2009. A third demonstration focused on better understanding the wake effects of the programmer parachute is scheduled for January 2010. Tests for the pilots, drogues and main parachutes are scheduled to begin in late 2010 and continue through 2014.

To gather additional useful data during this demonstration of the testing technique, two Orion main parachutes were deployed with over-inflation control lines to investigate their effects on drag oscillation.

One of the causes of drag oscillation is the “breathing” of the large ring sail parachutes resulting in time-varying drag performance. Better understanding the drag performance will improve the calculations of Orion’s touchdown velocity and the impact loads the vehicle must be designed to sustain. Engineers will study the data collected to see if the design modifications can be used to optimize the main parachute performance.

Orion will carry NASA's next generation of astronauts to the International Space Station and beyond. NASA's Johnson Space Center in Houston manages the Orion Project for the Constellation Program and leads the design and development of the crew exploration vehicle recovery system. The Houston division of Jacobs Technology Inc. in conjunction with Airborne Systems of Santa Ana, Calif. are designing, developing and testing the parachutes in Yuma.

Monday, October 12, 2009

Space Station Joint Crew News Conference

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Soyuz Landing Caps Historic Space Station Increment

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International Space Station Expedition 20 Commander Gennady Padalka and Flight Engineer Michael Barratt landed their Soyuz TMA-14 spacecraft on the steppes of Kazakhstan Sunday, wrapping up a six-month stay. Joining them was spaceflight participant Guy Laliberte, who spent 11 days in space.

Padalka, the Soyuz commander, guided the spacecraft to a parachute-assisted landing at 12:32 a.m. EDT at a site northeast of the town of Arkalyk.

Russian recovery teams were on hand within minutes of landing to help the crew exit from the Soyuz vehicle and reacclimate to gravity. The crew members will return to the Gagarin Cosmonaut Training Center in Star City, outside of Moscow, for reunions with their families.

Padalka and Barratt spent 199 days in space and 197 days on the station after their March 26 launch. Laliberte launched with the Expedition 21 crew on a Soyuz vehicle Sept. 30 and returned after nine days on the station.

Padalka and Barratt presided over the inauguration of a six-person crew and two space shuttle assembly and resupply missions to the station. They also were station crew members during the delivery of tons of cargo and new science facilities for expanded research, and the arrival of the first Japanese H-II Transfer cargo vehicle.

The station now is occupied by Expedition 21 Commander Frank De Winne of the European Space Agency and Flight Engineers Roman Romanenko and Max Suraev of Russia, Bob Thirsk of the Canadian Space Agency and Nicole Stott and Jeff Williams of NASA.

Friday, October 9, 2009

NASA Spacecraft Impacts Lunar Crater in Search for Water Ice!

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NASA's Lunar Crater Observation and Sensing Satellite, or LCROSS, created twin impacts on the moon's surface early Friday in a search for water ice. Scientists will analyze data from the spacecraft's instruments to assess whether water ice is present. The satellite traveled 5.6 million miles during an historic 113-day mission that ended in the Cabeus crater, a permanently shadowed region near the moon's south pole. The spacecraft was launched June 18 as a companion mission to the Lunar Reconnaissance Orbiter from NASA's Kennedy Space Center in Florida.

"The LCROSS science instruments worked exceedingly well and returned a wealth of data that will greatly improve our understanding of our closest celestial neighbor," said Anthony Colaprete, LCROSS principal investigator and project scientist at NASA's Ames Research Center in Moffett Field, Calif. "The team is excited to dive into data."

In preparation for impact, LCROSS and its spent Centaur upper stage rocket separated about 54,000 miles above the surface of the moon on Thursday at approximately 6:50 p.m. PDT.

Moving at a speed of more than 1.5 miles per second, the Centaur hit the lunar surface shortly after 4:31 a.m. Oct. 9, creating an impact that instruments aboard LCROSS observed for approximately four minutes. LCROSS then impacted the surface at approximately 4:36 a.m.

"This is a great day for science and exploration," said Doug Cooke, associate administrator for the Exploration Systems Mission Directorate at NASA Headquarters in Washington. "The LCROSS data should prove to be an impressive addition to the tremendous leaps in knowledge about the moon that have been achieved in recent weeks. I want to congratulate the LCROSS team for their tremendous achievement in development of this low cost spacecraft and for their perseverance through a number of difficult technical and operational challenges."‪

Other observatories reported capturing both impacts. The data will be shared with the LCROSS science team for analysis. The LCROSS team expects it to take several weeks of analysis before it can make a definitive assessment of the presence or absence of water ice.

"I am very proud of the success of this LCROSS mission team," said Daniel Andrews, LCROSS project manager at Ames. "Whenever this team would hit a roadblock, it conceived a clever work-around allowing us to push forward with a successful mission."

The images and video collected by the amateur astronomer community and the public also will be used to enhance our knowledge about the moon.

"One of the early goals of the mission was to get as many people to look at the LCROSS impacts in as many ways possible, and we succeeded," said Jennifer Heldmann, Ames' coordinator of the LCROSS observation campaign. "The amount of corroborated information that can be pulled out of this one event is fascinating."

"It has been an incredible journey since LCROSS was selected in April 2006," said Andrews. "The LCROSS Project faced a very ambitious schedule and an uncommonly small budget for a mission of this size. LCROSS could be a model for how small robotic missions are executed. This is truly big science on a small budget."

NASA to Rebroadcast Global Event from the Space Station

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NASA Television will rebroadcast the Oct. 9 global event International Space Station resident Guy Laliberte designed to raise awareness about the need for clean water. Laliberte, who founded Cirque du Soleil, hosts the event from aboard the station.

"Moving Stars and Earth for Water," will take place in 14 cities across five continents between 9 and 11 p.m. EDT, and will be streamed live on the Web site of Laliberte's ONE DROP foundation at:

http://www.onedrop.org

NASA Television will re-air the entire broadcast beginning Saturday, Oct. 10, at 1 p.m. with encore broadcasts Oct. 11 and 12. For NASA TV streaming video, schedule and downlink information, visit:

http://www.nasa.gov/ntv

NASA signed a memorandum of understanding with Cirque du Soleil regarding the event, which will include video from aboard the space station and also discussion about water recycling aboard the station and about NASA technologies affecting everyday life. Event participants include former Vice President Al Gore, Canadian Space Agency astronaut Julie Payette, actress Salma Hayek and singers Shakira and Bono.

Laliberte flew to the station for a nine-day stay under an agreement between the Russian Federal Space Agency and Space Adventures, Ltd. He and two station crewmates, Mike Barratt and Gennady Padalka, will return to Earth on Sunday, Oct. 11.

For more information about the space station, visit:

http://www.nasa.gov/station

Thursday, October 8, 2009

NASA Selects High School Students for Inspire Education Program

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NASA has selected 1,732 high school students from 48 states, the District of Columbia and Puerto Rico to participate in its Interdisciplinary National Science Program Incorporating Research Experience, also known as Inspire. The Inspire project is designed to encourage students in grades nine through 12 to pursue careers in science, technology, engineering and mathematics.

The selectees will participate in an online learning community in which students and parents have the opportunity to interact with their peers and NASA engineers and scientists. It also provides appropriate grade-level educational activities, discussion boards and chat rooms for participants and their families to gain exposure to the many career opportunities at NASA.

The selected students will have the option to compete for workshops and internships at NASA facilities and participating universities throughout the nation during the summer of 2010. The summer experience provides students a hands-on opportunity to investigate careers in science, technology, engineering and mathematics.

The INSPIRE project is part of NASA's education efforts to engaging and retaining students in disciplines critical to the agency's missions.

For information about the program, visit:

Wednesday, October 7, 2009

Events and Mission Activities at NASA

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Buzz, Astronauts Shine as Stars of Disney Parade

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Buzz Lightyear didn't quite make it to infinity, but he went well beyond the realm of other action figures.

The icon of Disney's "Toy Story" films spent 15 months on the International Space Station and got a ticker-tape parade alongside real-life moonwalker Buzz Aldrin and Expedition 18 Commander and NASA astronaut Mike Finke to welcome him home to Disney World in Orlando, Fla., on Oct. 2.

"Buzz was the perfect crewmate," Finke said. "He lifted our spirits, he didn't talk much and he didn't eat much, so he left us his extra portions."

While Buzz Lightyear is a space ranger, Finke said the character's best work has been in serving as a bridge between the fun, fanciful side of spaceflight and the technical and scientific skills NASA uses to make spaceflight happen in real life.

"Buzz is internationally known, and Buzz is a space ranger, so by sharing some of Buzz's adventures with what we do at NASA, it really highlights a lot of good things for NASA and shows what we really do, what astronauts do," Finke said.

The toy’s popularity gives NASA a head start in getting children's attention in a world in which focus is short-lived, said Joyce Winterton, NASA's associate administrator for Education.

"It's something that students and children can relate to," Winterton said. "So when they see him going up in space on the shuttle or the station it becomes a touch point for them. Sometimes I think they see an astronaut as something they can achieve, but when they see a toy, they somehow think, 'Hey, I can do that, too.'"

The parade coincided with a NASA education initiative that includes an opportunity for students to propose an experiment which will be flown on the International Space Station. There also is a contest to design a mission patch that will go into orbit on the station.

"We've got the attention of thousands of students because of Buzz Lightyear," Winterton said. "And hopefully we'll have a large number of students say let's plan an experiment. And of those we'll pick 12 that will fly on the International Space Station, and that's pretty great."

Disney also developed and posted several Web-based educational games for Buzz's launch and landing based on NASA's missions and goals.

Finke also shared a stage with Buzz at Disney's Magic Kingdom to talk to school children about space travel, science and technology.

Veronica Franco, an education specialist at NASA's Kennedy Space Center near Orlando, led a number of space-related demonstrations, including freezing and crumbling plants using liquid nitrogen. With help from "Spaceman" from the Kennedy Space Center Visitor Complex, she showed how astronauts get dressed for a spacewalk.

Then it was Finke's turn to wow the students with firsthand accounts from his two, six-month stays in the weightlessness of space. He looked at stars, conducted research on changes to the body and basically adjusted his body to cope with the unpredictable nature of things in zero gravity.

So what did students want to hear about first? The technologically advanced toilet.

Buzz didn't have to learn that lesson during his time in orbit.

Disney was aware of the somewhat mixed goals for NASA and the entertainment company, and backed down its normal commercial considerations for the chance to send Buzz into space.

"You've got to strike a balance," said Disney's Duncan Wardle, the company's global vice president for Public Relations Integration. "And it's a hard role for a government organization sponsored by the taxpayer, but you've got to excite the next generation of space travelers."

Buzz has proven an attraction in ways Wardle said he didn’t expect. For instance, a U.S. Air Force officer at Edwards Air Force Base in California asked for a photo with Buzz after the shuttle touched down there in September after space shuttle Discovery’s STS-128 mission.

But the idea was hardly a certainty when Wardle pitched it to a roomful of NASA officials.

"My sense was 50 percent loved the idea but probably didn't want to say it, and 50 percent of the room wanted to pick me up and throw me out the window," Wardle recalled.

Once the plan was approved, there was still a significant hurdle for the project: 12-inch Buzz Lightyear action figures had gone out of production months before and Wardle's team of employees could not find them in any store, warehouse or anywhere else.

"I was driving back to the office, and I got a call and all I heard was a voice, 'To Infinity and Beyond,'" Wardle said. "Then my wife said, 'Found it, it's been underneath (my son's) bed. It's been there six months collecting dust. And I was like, 'Right, that's it then, that's the Buzz Lightyear that's going into space. Wasn't quite in the plan, but . . . "

That Buzz went from bedroom floor to Houston in days, and into orbit a couple months later. At that point, there was not any talk of bringing the action figure back. Instead, he would stay on the station as a permanent resident, including during the station's fiery entry when it is de-orbited.

Wardle provided the winning argument for bringing Buzz back on the shuttle: "I said, guys, if you incinerate Buzz Lightyear, I'll have to tell the world's children."

So with his flight home approved, Buzz moved into Discovery during the STS-128 and returned to Earth. His education mission is not over though. Plans call for him to be displayed in the Smithsonian's National Air and Space Museum in Washington, Wardle said.

"This one is going to be hard to top," Finke said.

Tuesday, September 22, 2009

Radar Map of Buried Mars Layers Matches Climate Cycles

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New, three-dimensional imaging of Martian north-polar ice layers by a radar instrument on NASA's Mars Reconnaissance Orbiter is consistent with theoretical models of Martian climate swings during the past few million years.

Alignment of the layering patterns with the modeled climate cycles provides insight about how the layers accumulated. These ice-rich, layered deposits cover an area one-third larger than Texas and form a stack up to 2 kilometers (1.2 miles) thick atop a basal deposit with additional ice.

"Contrast in electrical properties between layers is what provides the reflectivity we observe with the radar," said Nathaniel Putzig of Southwest Research Institute, Boulder, Colo., a member of the science team for the Shallow Radar instrument on the orbiter. "The pattern of reflectivity tells us about the pattern of material variations within the layers."

Earlier radar observations indicated that the Martian north-polar layered deposits are mostly ice. Radar contrasts between different layers in the deposits are interpreted as differences in the concentration of rock material, in the form of dust, mixed with the ice. These deposits on Mars hold about one-third as much water as Earth's Greenland ice sheet.

Putzig and nine co-authors report findings from 358 radar observations in a paper accepted for publication by the journal Icarus and currently available online.

Their radar results provide a cross-sectional view of the north-polar layered deposits of Mars, showing that high-reflectivity zones, with multiple contrasting layers, alternate with more-homogeneous zones of lower reflectivity. Patterns of how these two types of zones alternate can be correlated to models of how changes in Mars' tilt on its axis have produced changes in the planet's climate in the past 4 million years or so, but only if some possibilities for how the layers form are ruled out.

"We're not doing the climate modeling here; we are comparing others' modeling results to what we observe with the radar, and using that comparison to constrain the possible explanations for how the layers form," Putzig said.

The most recent 300,000 years of Martian history are a period of less dramatic swings in the planet's tilt than during the preceding 600,000 years. Since the top zone of the north-polar layered deposits -- the most recently deposited portion -- is strongly radar-reflective, the researchers propose that such sections of high-contrast layering correspond to periods of relatively small swings in the planet's tilt.

They also propose a mechanism for how those contrasting layers would form. The observed pattern does not fit well with an earlier interpretation that the dustier layers in those zones are formed during high-tilt periods when sunshine on the polar region sublimates some of the top layer's ice and concentrates the dust left behind. Rather, it fits an alternative interpretation that the dustier layers are simply deposited during periods when the atmosphere is dustier.

The new radar mapping of the extent and depth of five stacked units in the north-polar layered deposits reveals that the geographical center of ice deposition probably shifted by 400 kilometers (250 miles) or more at least once during the past few million years.

"The radar has been giving us spectacular results," said Jeffrey Plaut of NASA's Jet Propulsion Laboratory, Pasadena, Calif., a co-author of the paper. "We have mapped continuous underground layers in three dimensions across a vast area."

The Italian Space Agency operates the Shallow Radar instrument, which it provided for NASA's Mars Reconnaissance Orbiter. The orbiter has been studying Mars with six advanced instruments since 2006. It has returned more data from the planet than all other past and current missions to Mars combined. For more information about the mission, visit: http://www.nasa.gov/mro.

Sunday, September 20, 2009

NASA Selects Target Crater for Lunar Impact

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NASA's Lunar Crater Observation and Sensing Satellite (LCROSS) is racing toward a double-impact on the moon at 7:30 am EDT on Oct. 9th. Today NASA announced exactly where the crash will take place.

The target crater is Cabeus A. It was selected after an extensive review of the best places to excavate frozen water at the lunar south pole.

"The selection of Cabeus A was a result of a vigorous debate within the lunar science community. We reviewed the latest data from Earth-based observatories and our fellow lunar missions Kaguya, Chandrayaan-1, and the Lunar Reconnaissance Orbiter," says Anthony Colaprete, LCROSS project scientist and principle investigator at NASA's Ames Research Center. "The team is looking forward to wealth of information this unique mission will produce."

LCROSS will search for ice by plunging its spent upper-stage Centaur rocket into the permanent shadows of Cabeus A, where water might be trapped in frozen form. The LCROSS satellite will then fly into the plume of debris kicked up by the impact and measure the properties of the plume before it also collides with the lunar surface.

The LCROSS team selected Cabeus A based on a set of conditions that includes favorable illumination of the debris plume for visibility from Earth, where astronomers will be watching closely. Cabeus A also has a high concentration of hydrogen (a constituent of water, H2O) and favorable terrain such as a flat floor, gentle slopes and the absence of large boulders.

Professional astronomers will use many of Earth's most capable observatories to monitor the impacts. These observatories include the Infrared Telescope Facility and Keck telescope in Hawaii; the Magdalena Ridge and Apache Ridge Observatories in New Mexico and the MMT Observatory in Arizona; the newly refurbished Hubble Space Telescope; and the Lunar Reconnaissance Orbiter, among others.

Amateur astronomers can monitor the impact, too. Observing tips may be found here.

"Telescopes participating in the LCROSS Observation Campaign will provide observations from different vantage points using different types of measurement techniques," says Jennifer Heldmann, lead for the LCROSS Observation Campaign at Ames. "These multiple observations will complement the LCROSS spacecraft data to help determine whether or not water ice exists in Cabeus A."

During a media briefing Sept. 11, Daniel Andrews, LCROSS project manager at Ames, provided a mission status update: The spacecraft is healthy and has enough fuel to successfully accomplish all mission objectives. Andrews also announced the dedication of the LCROSS mission to the memory of legendary news anchor, Walter Cronkite, who provided coverage of NASA's missions from the beginning of America's manned space program to the age of the space shuttle.



"Dad would sure be proud to be part, if just in name, of getting humans back up to the moon and beyond," says Chip Cronkite, son of the famed news anchor.

"We're looking forward to October 9th," Andrews says. "The next 28 days will undoubtedly be very exciting."

Cabeus A, here we come!

Thursday, September 17, 2009

This Week @ NASA 091109

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Tuesday, September 15, 2009

Best International Space Station Photos

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The International Space Station (ISS) is a research facility currently being assembled in Low Earth Orbit. On-orbit construction of the station began in 1998 and is scheduled to be complete by 2011, with operations continuing until at least 2015. As of 2009, the ISS is the largest artificial satellite in Earth orbit, with a mass larger than any previous space station.

The ISS is a joint project among the space agencies of the United States (National Aeronautics and Space Administration - NASA), Russia (Russian Federal Space Agency - RKA), Japan (Japan Aerospace Exploration Agency - JAXA), Canada (Canadian Space Agency - CSA) and ten European nations (European Space Agency - ESA). The Brazilian Space Agency (AEB) participates through a separate contract with NASA. The Italian Space Agency (ASI) similarly has separate contracts for various activities not done within the framework of ESA's ISS projects (where Italy also fully participates). China has reportedly expressed interest in the project, especially if it would be able to work with the RKA, although as of 2009 it is not involved.

Sunday, September 13, 2009

Discovery ends ISS mission in Mojave Desert

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The Discovery space shuttle has successfully touched down after its return from the International Space Station (ISS) was temporarily delayed by poor weather conditions and a close call with some potentially problematic orbiting space junk.

However, while the shuttle is now safely back on terra firma, the enforced 24-hour delay left NASA with little option but to divert the landing of its stalwart orbiter from the Kennedy Space Center in Florida to the Edwards Air Force Base in California.

Landing smoothly on Runway 22 at Edwards on Friday, the shuttle’s arrival ended NASA’s latest supply and maintenance mission to the ISS, during which the shuttle delivered some nine tons of equipment and a fresh crewmember for the orbiting scientific team.

The U.S. space administration opted for a landing at its Mojave Desert back-up strip after Entry Flight Director Richard Jones deemed persistently poor weather conditions in Florida to be too much of an issue.

“Welcome home, Discovery,” trumpeted Colonel Eric A. Boe of the U.S. Air Force as the shuttle rolled to a stop at Edwards. “Congratulations on an extremely successful mission, stepping up science to a new level on the International Space Station.”

While docked with the ISS, the crew of the Discovery completed three space walks, and delivered a sample freezer, a sleep station, and a carbon dioxide removal system. They also helped install a new ammonia coolant tank, retrieve two external experiments, and paved the way for the arrival of a new crew module in 2010.

Monday, September 7, 2009

Berlin TV tower 'stolen' by Nasa

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Footage of the Berlin TV tower, one of the most recognisable buildings in Germany, being fired into space in an audacious Nasa "theft" has become a web hit.

The 1,200ft tower, which bears a striking resemblance to a rocket, engulfs the centre of the city with smoke as it rises from the Berlin skyline.

The impressive launch footage was created from a combination of genuine Nasa audio recordings, library images of the tower and the computer trickery of a young animator.

Fabian Tischer, 28, grew up just a few miles from the telecommunications tower and produced the clip to realise his childhood fantasy of watching the iconic building lift off into space.

"As a child, I used to think the TV tower in the centre of the former capital of East Germany was a rocket. And now, with my technical possibilities, I have transformed it into that," he told Telegraph.co.uk.

He playfully titled his creation Nasa steals Berlin TV tower to capture the attention of viewers on YouTube and Video, the video-sharing websites where it was posted.

Judging by the comments, most people were impressed with his efforts.

"Congrats! Very nice idea. Funny. Technically good too, I like the cheap handcam look," wrote one commenter on Vimeo.

Another urged Mr Tischer to turn his talents to other landmarks: "Please make more rocket-powered famous buildings."

The Berlin TV tower has become one of the symbols of Berlin since it was erected 40 years ago, but its rocket-like design has not earned universal popularity. It is occasionally referred to as the "Telespargel", or TV asparagus.

Mr Tischer says that he has been "floored" with the response to his video, which he produced in part to generate buzz about his freelance animation and computer graphics work.


Friday, September 4, 2009

NASA Lunar Reconnaissance Snapped

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NASA's Lunar Reconnaissance Orbiter (LRO) has snapped the Apollo 12 landing site where, on 14 November 1969, astronauts Alan Bean and Pete Conrad touched down to begin their 32-hour stay on the lunar surface:

The Intrepid spacecraft touched down within 200 metres of the unmanned Surveyor 3 lander - launched two years earlier - at an "equatorial site on a flat lava plain" in western Oceanus Procellarum. NASA's caption to the picture explains: "The Intrepid lunar module descent stage, experiment package (ALSEP) and Surveyor 3 spacecraft are all visible. Astronaut footpaths are marked with unlabeled arrows. This image is 824 meters (about 900 yards) wide."



During two moonwalks, each of about four hours, Bean and Conrad deployed the aforementioned ALSEP and inspected the condition of the inactive Surveyor 3 (see pic below, featuring Alan Bean). They removed parts of the surveyor for return to Earth and "terrestrial analysis", which would yield "crucial data for present-day designers of lunar surface hardware".

The pair also scooped up 32kg of lunar samples during their mission, described by NASA as an "incredible success".



NASA has more details here, and pictures of other Apollo landing sites also captured by the LRO's Lunar Reconnaissance Orbiter Camera.

Thursday, September 3, 2009

Astronauts Informed of Possible Conjunction Maneuver!

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NASA space shuttle Capcom Tony Antonelli informed Discovery commander Rick Sturckow about a possible conjunction with debris from a portion of an Ariane 5 rocket body. The conversation was preempted on NASA Television by the HTV preflight briefing and was replayed after the briefing at 2:41 p.m. EDT.

Tony Antonelli: We’ve been analyzing whether we need to do Debris Avoidance Maneuver (DAM). We’re considering all the options and they’re all still on the table. The closest point of approach is at GMT 247:15:06 minutes (11:06 a.m. EDT Friday). The options that are still being considered are: we don’t need to do anything; there would be an attitude maneuver with a reboost option that we would accomplish post-EVA; the other is a deboost that will take a good chunk of the time tomorrow and would delay EVA 2 by a day. We will know more later today. We plan to do the campout tonight either way to keep our options open.


NASA PAO commentary summarized that Mission Control has not yet decided if there is a need for an avoidance maneuver. Flight controllers will continue to evaluate the conjunction before making that determination. The object, with unknown dimensions, is in a highly-elliptical orbit, 32,000 by 317 kilometers. Experts in Mission Control believe the object will make its closest approach to the shuttle and station on Friday morning just after 11 a.m. EDT, at a distance of just under 11 kilometers.Since no DAM decision has been made, preparations will continue to conduct the second spacewalk today.


Crew Prepares for Second Spacewalk:
Astronauts Danny Olivas and Christer Fuglesang are camping out in the Quest airlock starting at 2:54 a.m. EDT Thursday, in preparation for the second STS-128 spacewalk which begins at 5:19 p.m.


John McCullough, chief of the Flight Director Office, stated that it doesn’t look like the International Space Station will have to do a debris avoidance maneuver. However, the final decision will be made during the last hour of Thursday’s spacewalk. Mission Control is building a plan to conduct a reboost just in case. The piece of debris that is being tracked is approximately 19 square meters and is in an elliptical orbit. It is a fairly big piece which makes it easier to track. The closest approach (about 3 kilometers from the station) is expected at 10:06 a.m. Friday.



Monday, August 31, 2009

NASA Sets Briefing, TV Coverage of Japan's First Cargo Spacecraft

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NASA will hold a news briefing at 12:30 p.m. CDT on Wednesday, Sept. 2, to preview the maiden launch and flight of Japan's unpiloted H-II Transfer Vehicle (HTV) cargo spacecraft to the International Space Station.

NASA Television will broadcast the briefing live from NASA's Johnson Space Center in Houston. Participants in the briefing will include officials from NASA and the Japan Aerospace Exploration Agency (JAXA). NASA TV also will broadcast live HTV's launch and flight.

The HTV is scheduled to lift off on an H-IIB rocket from JAXA's Tanegashima Space Center in southern Japan at approximately noon Sept. 10 (about 2 a.m. Sept. 11 Japan time). NASA TV coverage of the launch will begin at 11:45 a.m. The HTV will augment the European Space Agency's Automated Transportation Vehicles and the Russian Progress ships that deliver supplies to the space station.

NASA conducted an HTV readiness review on Aug. 27. The HTV was formally approved for flight and rendezvous. The launch window will be open from Sept. 10-30. In the event of a launch postponement after the H-IIB rocket is fueled, a 72-hour turnaround will be required before the next launch attempt.

As the 16.5-ton cargo craft makes its week-long journey to the space station, flight controllers in Tsukuba, Japan, and at Mission Control in Houston will conduct a number of tests of HTV's rendezvous and navigation systems.

NASA TV coverage of the cargo craft's arrival at the station will begin at 2 p.m. Sept. 17. As the HTV moves within about 40 feet of the orbiting laboratory, space station crew members will capture the craft using the station's Canadarm2 robotic arm. The crew then will attach the HTV to an Earth-facing docking port on the station's Harmony connecting module. The robotic maneuvers are set to begin at about 2:50 p.m. Sept. 17.

The HTV will remain attached to the station for about six weeks while supplies are transferred. In addition to interior supplies and equipment, two new experiments carried on the exterior of the HTV will be moved to the Japanese Kibo module's external experiment porch using a combination of maneuvers with the station's Canadarm2 and Kibo's robotic arm.

NASA's Latest High-tech Autonomous Robotic Life Forms

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Astronomy Picture of the Day

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Many stars like our Sun were formed in open clusters. The above pictured open cluster, M25, contains thousands of stars and is about two thousand light years distant. The stars in this cluster all formed together about 90 million years ago. The bright young stars in M25 appear blue. Open clusters, also called galactic clusters, contain fewer and younger stars than globular clusters. Also unlike globular clusters, open clusters are generally confined to the plane of our Galaxy. M25 is visible with binoculars towards the constellation of the Archer ( Sagittarius).