First Soyuz lift from Europe’s Spaceport in French Guiana on 21 October 2011. Credits:Thilo Kranz/DLR
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Russia’s legendary Soyuz rocket soared skywards today (Oct.21) on its historic 1st ever blastoff from a new European space base in the equatorial jungles of South America. The history making liftoff of the Soyuz ST-B launcher from French Guiana occurred at exactly 6:30:26 a.m. EST (10:30:26 GMT) and lofted the first two operational satellites of Europe’s new Galileo GPS navigation system.
The flawless liftoff of the Soyuz booster from the ELS pad in French Guiana marked the first time that a Soyuz was launched from outside of the six existing pads in Russia and Kazakhstan. The joint Russian-European project was started back in 2004 and culminated with today’s launch of the Soyuz-VSO1 mission.
“This launch represents a lot for Europe: we have placed in orbit the first two satellites of Galileo, a system that will position our continent as a world-class player in the strategic domain of satellite navigation, a domain with huge economic perspectives,” said Jean-Jacques Dordain, Director General of ESA.
First Soyuz lift blastoff from Europe’s Spaceport in French Guiana on 21 October 2011. Mobile gantry at left. Credits:Thilo Kranz/DLR - Special to Universe Today
Soyuz lineage dates back to the beginning of the Space Age with the launch of Sputnik-1 in 1957 and the first man in space, Yuri Gagarin, in 1961. Soyuz had flown 1776 times to date.
First Soyuz lift from Europe’s Spaceport in French Guiana on 21 October 2011. Credits: ESA/CNES/ARIANESPACE - S. Corvaja, 2011
The launcher is based on the existing Soyuz design with a few changes to accommodate European safety standards and the construction of the ELS launch pad was modeled after the existing pads in Baikonur in Kazakhstan and Plesetsk in Russia. One significant difference is the construction of a 45 meter (170 foot) mobile gantry
A leaky valve delayed the flight by one day.
The duo of 700 kg Galileo satellites were mounted side by side on the Fregat upper stage atop the three stage Soyuz-2 rocket. These two Galileo In-orbit Validation (IOV) model satellites are experimental models that will be used to test the GPS technology.
Soyuz lifts off for the first time on 21 October 2011 from Europe’s Spaceport in French Guiana carrying the first two Galileo In-Orbit Validation satellites. Credits: ESA/CNES/ARIANESPACE - S. Corvaja, 2011
Two additional Galileo IOV satellites will be launched in 2012 as the initial segment of a 30 strong constellation of satellites in total.
The Galileo satelites will provide pinpoint accuracy to within about 1 meter (3 feet) compared to about 3 meters (10 feet) for the GPS system.
The 4 meter diameter payload fairing jettisoned as planned three minutes into the flight and the first of two firings of the Fregat upper stage was successfully completed after burnout of the lower stages. The second Fregat firing was accomplished about 4 hours after launch and injected the Galileo satellites into orbit some 23,000 km (14,000 miles) miles high.
The Fregat upper stage was designed to reignite and fire up to 20 times. It is fueled with nitrogen tetroxide and unsymmetrical dimethylhydrazine (UDMH).
First Soyuz lift from Europe’s Spaceport in French Guiana on 21 October 2011. Credits: ESA/CNES/ARIANESPACE - S. Corvaja, 2011
By launching from near the equator (5°N), the Soyuz gains about a 50% performance boost from 1.7 tons to nearly 3 tons to geostationary orbit due to the Earth’s faster spin compared to Baikonur (46°N).
Manned Soyuz missions from South America could be possible at some future date if the political and funding go ahead was approved by ESA and Russia. It is technically possible to reach the ISS from the French Guiana pad and would require the installation of additional ground support equipment.
The next Soyuz launch from South America is set for Dec. 16, 2011. 17 contracts have already been signed for future liftoffs at a rate of 2 to 3 per year.
The Apollo Guidance Computer hasa lot to offer many different types of readers. Photo Credit: Springer/Praxis
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Springer/Praxis has produced a small library’s worth of books about the Apollo Program. A recent offering from the publisher focuses in on the Apollo Guidance Computer. This topic, for the uninitiated, can be more than a little intimidating and if it is handled wrong veer off the path of a book about space flight and toward a pure “tech” book. This is not a problem that Springer/Praxis’ offering The Apollo Guidance Computer has, the book is well rounded, in-depth and easy-to-read.
Written by Frank O’Brien, The Apollo Guidance Computer is a thorough review of the computer system used during the Apollo missions. The Apollo Guidance Computer rings in at a whopping 430 pages – most readers will likely only pick out certain parts of the book to read. The book is, in a number of ways, many separate books in one – with details of the guidance computer, its development, the requirements to send astronauts to and from the Moon as well as the challenges that the engineers face in developing this revolutionary piece of equipment – all detailed within.
The book starts out by turning the clock back about 50 years to allow the reader to see what technology was like half a century ago. During this time period computers generally filled an entire room. This (obviously) was not possible in the case of Apollo’s guidance computer – and The Apollo Guidance Computer works to detail that story.
As far as O’Brien is concerned, he sees the book as something that techies, looking to learn how this computer system was developed, and space buffs who are seeking to learn the various intricacies of traveling to the Moon – can both enjoy.
While fairly primitive by today's standards, the Apollo guidance computer was revolutionary for its time. Photo Credit: NASA/Dryden
“It’s a bit different from other books that are found in spaceflight libraries, in that it is appealing to two very different groups,” said O’Brien during a recent interview. “Sometimes I joke that those interested in computers read it from the beginning till the end – whereas space enthusiasts –read it from the end to the beginning.”
For his part O’Brien acknowledges that not all parts of the book will interest all people. He is fine with that as long as readers enjoy the elements of the book that relate to them. He does hope that all readers pick up on how designers managed to pack away so much capability into a very limited structure. There was no disk, tape, or secondary storage – of any kind.
The book works to provide a link to demonstrate how the Apollo guidance computer allowed for one of the greatest accomplishments in human history. It details how difficult the actual lunar landing was and how the computer system was instrumental in accomplishing this feat.
Whereas many of Springer/Praxis’ offerings detail flight aspects of the Apollo era, this text takes a look at one of the essential elements that made those missions possible. While other books provide understanding of the Apollo Program in the broadest of strokes – this book allows readers to see the moon shot’s finest details. It also provides context into the era in which this machine was developed. Only in the 60s could an entry code be entitled BURNBABY (as in “Burn Baby Burn!”).
Frank O'Brien, the author of "The Apollo Guidance Computer" spoke to Universe Today about his thoughts on the book. Photo Courtesy of Frank O'Brien
With the completion of the fourth CCDEV milestone, Space Exploration Technologies is one step closer to launching astronauts into orbit. Photo Credit: SpaceX
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Space Exploration Technologies (SpaceX) is now one more step closer to sending astronauts to orbit. The commercial space firm announced today that it has completed a successful review of the company’s launch abort system (LAS). SpaceX’s LAS, dubbed “DragonRider” is designed differently than abort systems that have been used in the past.
The first review of the system’s design and its subsequent approval by NASA represents a step toward the realization of the space agency’s current objective of having commercial companies provide access to the International Space Station (ISS) while it focuses on sending astronauts beyond low-Earth-orbit (LEO) for the first time in four decades.
The DragonRider launch abort system would allow astronauts to be safely pulled away from the Falcon 9 launch vehicle in the advent of an emergency. Image Credit: SpaceX
“Each milestone we complete brings the United States one step closer to once again having domestic human spaceflight capability,” said former astronaut Garrett Reisman, who is one of the two program leads who are working on SpaceX’s DragonRider program.
With the space shuttle program over and its fleet of orbiters headed to museums, the United States is paying Russia an estimated $63 million per seat on its Soyuz spacecraft. SpaceX has estimated that, by comparison, flights on a man-rated version of its Dragon spacecraft would cost approximately $20 million. Despite the dramatically lower cost, SpaceX has emphatically stated that safety is one of the key drivers of its spacecraft.
NASA, who currently lacks the capacity to launch astronauts on its own, has to pay fellow space station program partner $63 million a seat on its Soyuz spacecraft. SpaceX has estimated by comparison that flights on a man-rated Dragon would cost around $20 million. Photo Credit: NASA.gov
“Dragon’s integrated launch abort system provides astronauts with the ability to safely escape from the beginning of the launch until the rocket reaches orbit,” said David Giger, the other lead on the DragonRider program. “This level of protection is unprecedented in manned spaceflight history.”
SpaceX had already met three of NASA’s milestones under the Commercial Crew Development (CCDev) contract that the company has signed into with the U.S. space agency. With the Preliminary Design Review or PDR completed of the abort system SpaceX can now rack up another milestone that it has met.
SpaceX is currently working to see that the next flight of its Dragon spacecraft tentatively scheduled for late this year will incorporate mission objectives of both the second and third COTS demonstration flights and be allowed to dock with the International Space Station. Image Credit: SpaceX
Unlike conventional abort systems, which are essentially small, powerful rockets that are attached to the top of the spacecraft, Dragon’s LAS is actually built into the walls of the Dragon. This is not an effort just to make the spacecraft’s abort system unique – rather it is meant as a cost-cutting measure. The Dragon is intended to be reusable, as such its abort system needed to be capable of being reused on later flights as well. Traditional LAS simply do not allow for that. With every successful launch by conventional means – the LAS is lost.
SpaceX is also working to see that this system not only can save astronaut lives in the advent of an emergency – but that it can actually allow the spacecraft to conduct pinpoint landings one day. Not just on Earth – but possibly other terrestrial bodies – including Mars.
SpaceX is hopeful that if all goes well with its DragonRider system that it could one deay be developed to land future versions of the company's spacecraft on other terrestrial bodies - including the planet Mars. Image Credit: SpaceX
To date, SpaceX has launched two of its Falcon 9 launch vehicles. The first occurred on June 4 of 2010 and the second, and the first under the Commercial Orbital Transportation Services (COTS) contract took place six months later on Dec. 8. This second mission was the first to include a Dragon spacecraft, which was recovered in the Pacific Ocean off the coast of California after successfully completing two orbits.
“We have accomplished these four milestones on time and budget, while this is incredibly important, it is business as usual for SpaceX,” said SpaceX’s Vice-President for Communications Bobby Block during an interview. “These are being completed under a Space Act Agreement that demonstrates the innovative and efficient nature of what can be accomplished when the commercial sector and NASA work together.”
SpaceX's Vice-President for Communications, Bobby Block, said that the fact that SpaceX has accomplished these milestones on time and budget should show what can happen when NASA and the private industry work together. Photo Credit: Alan Walters/awaltersphoto.com
1st Russian Soyuz poised for blastoff from Europe’s Spaceport in South America. Soyuz VS01, the first Soyuz flight from Europe’s Spaceport in French Guiana is scheduled to liftoff on 20 October 2011. Credit: ESA - S. Corvaja
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A Russian Soyuz-2 rocket sits poised for its first ever blast off in less than 24 hours from a brand new launch pad built in the jungles of French Guiana, South America by the European Space Agency (ESA) .
The payload for the debut liftoff of the Soyuz ST-B booster consists of the first pair of operational Galilieo satellites, critical to Europe’s hopes for building an independent GPS navigation system in orbit.
Soyuz VS01, the first Soyuz flight from Europe’s Spaceport in French Guiana, will lift off on 20 October 2011. The rocket will carry the first two satellites of Europe’s Galileo navigation system into orbit. Credit:ESA - S. Corvaja
The Soyuz VS01 mission is set to soar on Thursday, Oct. 20 at 6:34 a.m. EDT (1034 GMT ) from Europe’s new South American pad, specially built for the Soyuz rocket. The three stage rocket was rolled out 600 meters horizontally to the launch pad and vertically raised to its launch position.
Soyuz VS01 on launch pad. Soyuz VS01vehicle was rolled out horizontally on its erector from the preparation building to the launch zone and then raised into the vertical position. The ‘Upper Composite’, comprising the Fregat upper stage, payload and fairing, was also transferred and added onto the vehicle from above, completing the very first Soyuz on its launch pad at Europe’s Spaceport. Soyuz VS01 will lift off on 20 October 2011. The rocket will carry the first two satellites of Europe’s Galileo navigation system into orbit. Credit: ESA - S. Corvaja
The two Galileo satellites were mated to the Fregat-MT upper stage, enclosed inside their payload fairing and then hoisted atop the Soyuz rocket. They should seperate from the upper stage about 3.5 hous after launch.
Because French Guiana is so close to the equator, the Soyuz gains a significant boost in performance from 1.7 tons to 3 tons due to the Earth’s greater spin.
This marks the first time in history that the renowned Soyuz workhorse will blast off from outside of Kazakhstan or Russia and also the start of orbital construction of Europe’s constellation of 30 Gallileo satellites.
28 more of the navigation satellites, built by the EADS consortium based in Germany, will be lofted starting in 2012 aboard the medium class Soyuz rockets.
French Guiana is already home to Europe’s venerable Ariane rocket family and will soon expand further to include the new Vega rocket for smaller class satellites.
ESA will begin live streaming coverage starting about an hour before the planned launch time of 6:34 a.m. EDT (1034 GMT)
Soyuz VS01 poised for launch on Oct. 20, 2011. Credit: ESA - S. Corvaja
Russia’s Phobos-Grunt sample return spacecraft is uncrated after arriving at the Baikonur Cosmodrome on Oct. 17, 2011. Launch to Mars is scheduled for sometime in November 2011. Folded solar panels and Phobos sample return vehicle at left. Phobos Lander and Yinghou-1 Orbiter at center, right. Credit: Roskosmos.
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Barely in the nick of time, Russia’s groundbreaking Phobos-Grunt interplanetary spacecraft to Mars finally arrived on Monday (Oct. 17) at the Baikonur Cosmodrome launch site in Kazakhstan – and today (Oct. 18) an eye-popping collection of great images (see below) was at last published by Roskosmos, the Russian Federal Space Agency.
This first-of-its-kind spaceship is due to blast off quite soon – sometime in the first half of November – although Roskosmos has yet to announce an official launch date and time is running out. The deadline to Mars is Nov. 25.
Top view of Phobos-Grunt, sample return vehicle. Credit: Roskosmos.
The explicit close-up photos show both the Phobos-Grunt orbiter/lander vehicle and her companion Yinghou-1 Mars orbiter, built by China, being uncrated from a huge shipping container, uprighted and then showcased from many revealing angles from top to bottom, tilted from side to side and looking inside her hardware stack.
The photos illustrate the solar panels, landing legs, J-shaped soil sampling tube, Earth return vehicle and descent capsule, star trackers, communications antennae, maneuvering thrusters and more.
Top view of Phobos-Grunt, sample return vehicle. Credit: Roskosmos.
The Yinghou-1 mini-satellite is clearly visible tucked inside a truss situated between the Phobos-Grunt landing ship and the MDU propulsion stage.
Phobos-Grunt was just air shipped from Moscow to Baikonur inside an Antonov An-124-100 “Ruslan” cargo plane operated by “Polyot” airline.
The cargo canister was offloaded and transported by truck to Facility 31. The spacecraft was then placed on a test stand to begin an intense period of final prelaunch payload processing activites to ready the probe for launch.
The Zenit-2SB booster rocket also recently arrived at Baikonur for ongoing prelaunch processing at nearby Building 42.
Chinese Yinghou-1 mini-satellite tucked truss at right, situated below the Phobos-Grunt lander at left. Credit: Roskosmos.
Russia’s engineers and technicians will have to work diligently in the few weeks remaining in order to complete all preflight activities to achieve a liftoff to the Red Planet before the unforgiving and narrow launch window closes for another 26 months.
Phobos-Grunt Earth return spacecraft. Close-up view of solar panels, Earth descent capsule and soil sample transfer tube. Credit: Roskosmos.Phobos-Grunt sample collecting and sample return vehicle. Credit: Roskosmos.
Tilted view of Phobos-Grunt attached to test stand for final prelaunch processing. Credit: Roskosmos.
Earth is actually lofting two exciting science missions to Mars this November. NASA’s Curiosity Mars Science Laboratory rover is due to blastoff on Nov. 25 and her launch window extends until Dec. 18. Both spaceships missed their initially targeted launch windows in 2009 due to the need to fix unresolved technical issues.
Phobos-Grunt is a daring sample return mission whose goal is to retrieve up to 200 grams of soil and rock from the tiny Martian moon Phobos, that will help elucidate the origin and evolution of Phobos, Mars and the Solar System.
Tilted view of Phobos-Grunt attached to test stand for final prelaunch processing. Credit: Roskosmos.
Side view of Phobos-Grunt and Yinghou-1 orbiter (bottom) attached to test stand for final prelaunch processing. Credit: Roskosmos. Labeled Schematic of Phobos-Grunt and Yinghou-1 (YH-1) orbiter
Southern Hemisphere of Vesta; Rheasilvia and Older Basin. Colorized shaded-relief map showing identification of older 375-kilometer-wide impact basin beneath and overlapping with the more recent Rheasilvia impact structure at asteroid Vesta’s South Pole. Credit: NASA/JPL-Caltech/UCLA/MPS/DLR/IDA
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Scientists leading NASA’sDawn mission have discovered a 2nd giant impact basin at the south pole of the giant asteroid Vesta, which has been unveiled as a surprisingly “dichotomous” and alien world. Furthermore, the cosmic collisions that produced these two basins shuddered through the interior and created vast Vestan troughs, a Dawn scientist told Universe Today.
The newly discovered impact basin, nicknamed ‘Older Basin’, is actually significantly older in age compared to the initially discovered South Pole basin feature named ‘Rheasilvia’ – perhaps by more than a billion years. And that is just one of the many unexplained mysteries yet to be reconciled by the team as they begin to sift through the millions of bits of new data streaming back daily to Earth.
Scientists speculate that ‘Older Basin’ is on the order of 3.8 Billion years old, whereas ‘Rheasilvia’ might be as young as about 2.5 Billion years, but those are just tentative estimates at this time and subject to change. Measurements so far indicate Rheasilvia is composed of basaltic material.
Shaded-relief topographic map of Vesta southern hemisphere showing two large impact basins - Rheasilvia and Older Basin.
Credit: NASA/JPL-Caltech/UCLA/MPS/DLR/IDA
“We found many surprising things at Vesta, which is quite unique and the results have exceeded our expectations”, said Dr. Carol Raymond, Dawn deputy principal investigator, of NASA’s Jet Propulsion Laboratory, Pasadena, Calif.
Researchers presented the latest findings from Dawn’s initial science mapping orbit at a news briefing at the annual meeting of the Geological Society of America in Minneapolis, Minn., on Oct. 13.
The team considers Vesta to be the smallest terrestrial planet.
Since achieving orbit in July, Dawn’s Framing Cameras (FC) have imaged most of Vesta at about 250 meter resolution and the Visible and Infrared mapping spectrometer(VIR) at about 700 meter resolution. The measurements were collected at the survey orbit altitude of 2700 km. Before Dawn, Vesta was just a fuzzy blob in humankind’s most powerful telescopes.
Vesta from Hubble (top) as a fuzzy blob and from Dawn in orbit (bottom) in crystal clear high resolution.
Credit: NASA/JPL-Caltech/ UCLA/MPS/DLR/IDA
“There is a global dichotomy on Vesta and a fundamental difference between the northern and southern hemispheres”, said Raymond. “The northern hemisphere is older and heavily cratered in contrast to the brighter southern hemisphere where the texture is more smooth and there are lots of sets of grooves. There is a massive mountain at the South Pole. One of the more surprising aspects is the set of deep equatorial troughs.”
“There is also a tremendous and surprising diversity of surface color and morphology. The south is consistent with basaltic lithology and the north with impacts. We are trying to make sense of the data and will integrate that with the high resolution observations we are now collecting.”
Indeed Vesta’s completely unique and striking dichotomy can be directly traced back to the basins which were formed by ancient cataclysmic impacts resulting in shockwaves that fundamentally altered the surface and caused the formation of the long troughs that ring Vesta at numerous latitudes.
“The troughs extend across 240 degrees of longitude,” said Debra Buczkowski, Dawn participating scientist, of the Applied Physics Laboratory at Johns Hopkins University, Laurel, Md. “Their formation can be tied back to the two basins at the South Pole.”
Asteroid Vesta and Equatorial Grooves
This full view of the giant asteroid Vesta was taken by NASA’s Dawn spacecraft, as part of a rotation characterization sequence on July 24, 2011, at a distance of 3,200 miles (5,200 kilometers). A rotation characterization sequence helps the scientists and engineers by giving an initial overview of the character of the surface as Vesta rotated underneath the spacecraft. This view of Vesta shows impact craters of various sizes and grooves parallel to the equator. The resolution of this image is about 500 meters per pixel. Credit: NASA/JPL-Caltech/UCLA/MPS/DLR/IDA
In an exclusive follow up interview with Universe Today, Raymond said “We believe that the troughs formed as a direct result of the impacts,” said “The two sets of troughs are associated with the two large basins [Rheasilvia and Older Basin].”
“The key piece of evidence presented was that the set of troughs in the northern hemisphere, that look older (more degraded) are circumferential to the older impact basin,” Raymond told me.
“The equatorial set are circumferential to Rheasilvia. That Rheasilvia’s age appears in places to be much younger is at odds with the age of the equatorial troughs. An explanation for that could be resurfacing by younger mass wasting features (landslides, slumps). We will be working on clarifying all these relationships in the coming months with the higher resolution HAMO (High Altitude Mapping Orbit) data.”
Dawn has gradually spiraled down closer to Vesta using her exotic ion thrusters and began the HAMO mapping campaign on Sept. 29.
Surface features are dated by crater counting methodology.
“Preliminary crater counting age dates for the equatorial trough region yields a very old age (3.8 Billion years). So there is a discrepancy between the apparent younger age for the Rheasilvia basin and the old age for the troughs. These could be reconciled if Rheasilvia is also 3.8 Billion years old but the surface has been modified by slumping or other processes,” Raymond elaborated.
Time will tell as further data is analyzed.
Dawn launch on September 27, 2007 by a Delta II Heavy rocket from Cape Canaveral Air Force Station, Florida. Credit: Ken Kremer
“Vesta is full of surprises, no more so than at the South Pole,” said Paul Schenk at the GSA briefing. Schenk is a Dawn participating scientist of the Lunar and Planetary Institute, Houston, Texas.
The ‘Rheasilvia’ basin was initially discovered in images of Vesta taken a decade ago by the Hubble Space Telescope which revealed it as a gaping hole in the southern hemisphere. But it wasn’t until Dawn entered orbit on July 16, 2011 after a nearly four year interplanetary journey that Earthlings got their first close up look at the mysterious polar feature and can now scrutinize it in detail to elucidate its true nature.
“The South Pole [Rheasilvia] basin is a roughly circular, impact structure and a deep depression dominated by a large central mound,” said Schenk. “It shows sharp scarps, smooth areas, landslide deposits, debris flows. It’s about 475 km in diameter and one of the deepest (ca. 20 -25 km) impact craters in the solar system.”
The central peak is an enormous mountain, about 22 km high and 180 km across- one of the biggest in the solar system. “It’s comparable in some ways to Olympus Mons on Mars,” Schenk stated.
“We were quite surprised to see a second basin in the mapping data outside of Rheasilvia. This was unexpected. It’s called ‘Older Basin’ for now.”
‘Older Basin’ is about 375 km in diameter. They overlap at the place where Rheasilvia has a missing rim.
“These basins are interesting because we believe Vesta is the source of a large number of meteorites, the HED meteorites that have a spread of ages,” Schenk explained.
Images showing key components of Rheasilvia impact basin on Vesta in high resolution ,referred to Shaded-relief topographic map. Credit: NASA/JPL-Caltech/ UCLA/MPS/DLR/IDA
Multiple large impacts over time may explain the source of the HED (Howardite, Eucrite and Diogenite) meteorites.
“We did expect large impacts on Vesta, likely associated with the late heavy bombardment recognized in the lunar impact record,” Raymond told Universe Today. “The surprising element is that the two apparently largest impacts – keeping in mind that other larger impact basins may be lurking under the regolith – are overlapping.”
Dawn’s VIR spectrometer has detected pyroxene bands covering Vesta’s surface, which is indicative of typical basaltic material, said Federico Tosi, a VIR team member of the Italian Space Agency, Rome. “Vesta has diverse rock types on its surface.”
“VIR measured surface temperatures from 220K to 270 K at the 5 micron wavelength. The illuminated areas are warmer.”
So far there is no clear indication of olivine which would be a marker for seeing Vesta’s mantle, Tossi elaborated.
The VIR spectrometer combines images, spectral information and temperature that will allow researchers to evaluate the nature, composition and evolutionary forces that shaped Vesta’s surface.
The team is absolutely thrilled to see a complicated geologic record that’s been preserved for study with lots of apparent surface layering and surprisingly strong and complex structural features with a large range of color and brightness.
Stay tuned for a year of Vestan delights !
Asteroid Vesta from Dawn
South Pole Rheasilvia basin is at lower right. NASA's Dawn spacecraft obtained this image of the giant asteroid Vesta with its framing camera on July 24, 2011 from a distance of about 3,200 miles (5,200 kilometers). Dawn entered orbit around Vesta on July 16, and will spend a year orbiting the body.
Credit: NASA/JPL-Caltech/UCLA/MPS/DLR/IDA
Artist's rendering of a vacuum tube, one of the main components of an atomic clock. Credit: NASA
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When people think of space technologies, many think of solar panels, propulsion systems and guidance systems. One important piece of technology in spaceflight is an accurate timing device.
Many satellites and spacecraft require accurate timing signals to ensure the proper operation of scientific instruments. In the case of GPS satellites, accurate timing is essential, otherwise anything relying on GPS signals to navigate could be misdirected.
The third technology demonstration planned by NASA’s Jet Propulsion Laboratory is the Deep Space Atomic Clock. The DSAC team plans to develop a small, low-mass atomic clock based on mercury-ion trap technology and demonstrate it in space.
What benefits will a new atomic clock design offer NASA and other players in near-Earth orbit and the rest of our solar system?
The Deep Space Atomic Clock demonstration mission will fly and validate an atomic clock that is 10-times more accurate than today’s systems. The project will demonstrate ultra-precision timing in space as well as the benefits said timing offers.
The DSAC will fly on an Iridium spacecraft and make use of GPS signals to demonstrate precision orbit determination and confirm the clock’s performance. As mentioned previously, precise timing and navigation are critical to the performance of many aspects of deep space and near-Earth exploration missions.
The DSAC team believes the demonstration will offer enhancements and cost savings for new missions, which include:
Increase Data Quantity: A factor of 2 to 3 increase in navigation and radio science data quantity by allowing coherent tracking to extend over the full view period of Earth stations.
Improve Data Quality: Up to 10 times more accurate navigation, gravity science, and occultation science at remote solar system bodies by using one-way radiometric links.
Enabling New Missions: Shift towards a more flexible and extensible one-way radio navigation architecture enabling development of capable in-situ satellite navigation systems and autonomous deep space radio navigation.
Reduce Proposed Mission Costs: Reduce mission costs for using the Deep Space Network (DSN) through aperture sharing and one-way downlink only time.
Benefits to GPS: Improve clock stability of the next GPS system by 100 times.
One example use for the DSAC is for a future mission that is a follow-up to the Mars Reconnaissance Orbiter (MRO). A spacecraft equipped with the DSAC could avoid reliance on two-way communications using NASA’s Deep Space Network to perform orbital determination.
One of the benefits of avoiding said reliance on two-way communications would allow the mission to only require the DSN for one-way communication to transmit scientific data to Earth. Reducing the reliance on two-way communications would provide an additional benefit of cost savings.
In the previous example, the DSAC team estimates an $11 million dollar reduction in network operational costs, as well as a 100% increase in the amount of usable science and navigation data that could be received. Overview of Deep Space Atomic Clock (DASC) mission. Image Credit: NASA
The Space Communications and Navigation (SCaN) office in the Human Exploration and Operations Mission Directorate is collaborating with the NASA Office of the Chief Technologist in sponsoring this technology demonstration.
If successful the DSAC flight demonstration mission will bring the improved atomic clock technology to a technological readiness level that will allow it to be used in a wide variety of future space missions.
Read our earlier articles about the other technology demonstrations planned:
The Atlas Spaceflight Operations Center or ASOC is where the Atlas V launch vehicle, in this case the one which will launch the Mars Science Laboratory (MSL) rover on its mission Nov. 25 at 10:21 a.m. EDT. Photo Credit: United Launch Alliance
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CAPE CANAVERAL, Fla – United Launch Alliance (ULA) uses a structure that incorporates several launch and support operations into one centralized facility. Known as the Atlas Spaceflight Operations Center (ASOC) is about 9,290 square-meters (100,000 square-foot) in size. The ASOC provides all of the required elements – command, control and communication with the Atlas V. It is from the ASOC that the mission is managed as well as monitoring and evaluating launch operations.
The ASOC is actually two separate buildings that were combined into one. More accurately an existing structure had modern sections added to it. The first section was originally built back in the early 60s as part of the Titan III Program. The ASOC was built for the Titan II Chemical Systems Division Solid Rocket Motors. During this period, it was referred to as the Motor Inert Storage (MIS).
The ASOC is actually two buildings in one. The original structure was built in the 60s for the Titan Program. Later elements allowed for spacecraft processing as well as launch operations to be conducted all under one roof. Photo Credit: Alan Walters/awaltersphoto.com
Later, after the awarding of the Evolved Expendable Launch Vehicle (EELV) contract to Lockheed Martin in Oct. of 1998, they added three additional stories to the MIS. Part of this was the addition of the ASOC’s Launch Control Center (LCC).
The blockbuster film, Transformers 3, Dark of the Moon, had a few scenes filmed at the ASOC. Josh Duhamel, who played Lt. Colonel William Lennox, stood in the center of the LCC while battling the Decepticons. The filming took place back in October of 2010.
Key scenes of the blockbuster fiml "Transformers 3: Dark of the Moon" were shot within the ASOC. Image Credit: Paramount Pictures
The different manners in which the various rockets supported by the Denver, Colorado-based ULA are produced are in large part determined by the history of the rockets themselves.
“Launch vehicles are processed in various ways due to the design of the rocket, the backgrounds of the engineers, designing the rocket and how the rocket evolved all played their part,” said United Launch Alliance’s Mike Woolley. “The facilities available to the designers of the launch vehicle’s systems, the topography and geography of the installation as well as the rules, regulations, restrictions of the area played there part in how each of the individual launch systems are processed.”
The Atlas V launch vehicle is one of the two primary launch systems that is supported by the United Launch Alliance (the other being the Delta IV). Image Credit: Lockheed Martin
The ASOC is one part of the overall launch flow for the Atlas V launch vehicle. The other elements (excluding Space Launch Complex 41) are the Horizontal Integration Facility (HIF) and Vertical Integration Facility (VIF).
with a rooms looking down into it, The ASOC a Mission Directors Center, the Spacecraft Operations Center, the Engineering Support Facility, engineering support room which has been dubbed the “Gator Room” as well as an executive conference room.
Inside of the ASOC is the Atlas Launch Control Center or LCC. This allows for rockets to be prepard for flight as well as the launches themselves - to be managed from one building. Photo Credit: United Launch Alliance
The ASOC also has a hospitality room as well as a viewing room on the third floor (the roof is also made available for viewing launches). Lockheed Martin chose to cut back the number of support structures and decided to just build on to the existing MIS building. By doing this, Atlas engineers and technicians as well as the Atlas launch control center are close to the High ay where the Atlas V launch vehicle is processed for flight. This not only reduces the amount of time to process the Atlas booster, but it reduces costs as well.
The last Atlas V that was in the High Bay of the ASOC was the one that will be utilized to send the Mars Science Laboratory (MSL) rover, dubbed Curiosity. The Atlas V 541 (AV-028) recently underwent what is known as a Wet Dress Rehearsal (WDR) where the rocket is taken all the way up to launch. This is done to test out the rocket’s key systems before the payload is attached to the launch vehicle. Currently, MSL is set to launch from Space Launch Complex-41 (SLC-41) on Nov. 25 at 10:21 a.m. EDT.
The next mission that will be launched on the Atlas V Evolved Expendable Launch Vehicle is JPL's Mars Science Laboratory (MSL) rover. Photo Credit: Alan Walters/awaltersphoto.com
Jean-Jacques Dordain. Credit: ESA photo by S. Corvaja
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What’s new in the avenue of space exploration? Right now the European Space Agency (ESA) has issued a formal invitation to Russia to join the U.S.-European Mars exploration program in a last-ditch attempt to save the project from being cut in half, ESA Director-General Jean-Jacques Dordain said October 13th.
The appeal to Russia, which came in the form of a letter to the head of the Russian space agency, Roscosmos, is likely ESA’s only hope of saving the full U.S.-European Mars exploration project, which Europe calls ExoMars, Dordain said in an interview. At this point in time, the agency is hoping for a solid answer by the beginning of 2012. This will allow for planning for a two-launch mission of the ExoMars program and lead to a full partnership between the Russian Space Agency and NASA. What’s more, this partnership could mean additional support for the U.S.-European program and even incorporate a Proton rocket launch carrying a jointly-build Mars telecommunications orbiter and an entry, descent and landing system in 2016.
By cutting NASA’s budget, the U.S. contribution to world-wide space programs looks bleak… even with the planned 2018 launch, aboard a NASA-provided Atlas 5 rocket, of the Euro-American Mars rover. This lack of funds hurts everyone – including ESA – dashing hopes of of purchasing its own Ariane 5 rocket for the 2016 mission. Even though NASA appears to be committed at this point, there’s always the uncertainty of the U.S. economic picture.
“At this point I am becoming a Doubting Thomas in that I believe only what I can see,” Dordain said. “But NASA has said nothing that would lead me to believe the 2018 mission is not going forward. At this point I have only two options: Keep the mission as we would like it by finding an additional partner, or reduce the mission.”
This doesn’t mean that ESA isn’t trying. Even by cutting the budget to a single-launch isn’t totally the answer. By making such drastic changes in the middle of an already planned scenario means changing tactics when design teams are already on a tight schedule. Cutting the budget also means cutting jobs – and that’s a problem in its own right. At this point, ESA is even willing to release nations from their commitments to keep the program, with modifications, intact.
Dordain said his approach to Roscosmos is not simply a request for an in-kind contribution of a Proton rocket for the 2016 launch. He said he would like Russia involved in ExoMars as a full third participant with NASA and ESA, and that the Russian role could include provision of experiments. “This could end up being an even grander mission than it would have with a full Russian participation,” Dordain said. “It’s not simply a matter of asking the Russians, ‘Please provide us a launcher.’”
Dordain briefed ESA’s ruling council on the ExoMars situation October 13 and will give an update at the council’s mid-December meeting. The current ExoMars contract for the 2016 mission, which had already been extended while ESA waited for a NASA commitment that never came, runs through December and can be extended to January, Dordain said.
It will be a waiting game from here. With luck, the Russians will answer by January 2012 and NASA will have a clearer picture of its own financial responsibilities by February 2012. Let’s hope the ExoMars Mission doesn’t have to pay the price.
<>. Mission Poster for the Russian Phobos-Grunt soil sample return spacecraft set to launch to Mars and its moon Phobos in November 2011. Phobos-Grunt consistes Credit: Roskosmos - Russian Federal Space Agency
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Russia is marking the upcoming blastoff of their dauntingly complex Phobos-Grunt sample return mission to the Martian moon Phobos with the release of a quite cool looking mission poster – see above. Phobos-Grunt translates as Phobos-Soil and is due to liftoff on or about November 7, 2011 from the Baikonur Cosmodrome atop a Zenit rocket.
The holy grail of Mars exploration has long been a sample return mission. But with severe cutbacks to NASA’s budget that goal is realistically more than a decade away. That’s why Phobos- Grunt is so exciting from a scientific standpoint.
Phobos-Grunt Orbiter/Lander
Russia's Phobos-Grunt is designed to land on Mars' moon Phobos, collect soil samples and return them to Earth for study. The lander will also carry scientific instrumetns to study Phobos and its environment. It will travel to Mars together with Yinghuo-1, China's first mission to the Red Planet. Credit: NPO Lavochkin
Phobos-Grunt Robotic sampling arm. Credit: Roskosmos
If successful, this audacious probe will retrieve about 200 grams of soil from the diminutive moon Phobos and accomplish the round trip in three years time by August 2014. Scientists speculate that martian dust may coat portions of Phobos and could possibly be mixed in with any returned samples.
Included here are more photos and graphics of the Phobos-Grunt spacecraft which is equipped with two robotic arms and a sampling device to transfer regolith and rocks to the Earth return vehicle and an on board array of some 15 science instruments, including lasers, spectrometers, cameras and a microscope. Readers please feel free to help with Russian translations.
Phobos-Grunt Model
This is a full-scale mockup of Russia's Phobos-Grunt. The spacecraft will collect samples of soil on Mar's moon Phobos and to bring the samples back to Earth for detailed study. Credit: CNES
Phobos-Grunt is the first of Earth’s two missions launching to the Red Planet in 2011. NASA’s Curiosity Mars Science Laboratory is due to lift off on Nov. 25, 2011 from Cape Canaveral, Florida.
