tag:blogger.com,1999:blog-14170390688103657812024-03-13T12:38:52.305-07:00International Space Station Shuttle NASA Missions Google Earth Science Technology Marsstanley princehttp://www.blogger.com/profile/09280760443900821968noreply@blogger.comBlogger1184125tag:blogger.com,1999:blog-1417039068810365781.post-18775237900139986012014-03-25T02:14:00.000-07:002016-01-12T23:02:17.822-08:00Keeping foods fresher for a long duration in space with misting systems<div dir="ltr" style="text-align: left;" trbidi="on">
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Even though there are many advancement in technology, keeping foods fresher in space for a long period has been impossible. Research has been going on to keep fresh fruits and vegetables for long-term in space. It has been found that spraying waters over fruits and vegetables keep them fresher for a long period. It’s a fact that if a plant or a food has more solute than the environment surrounding it then to achieve equilibrium state water diffuses into the cell.</div>
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Thus by routinely spraying the vegetables with water it keeps up their turgor pressure and keeps them nice and crisp for us to eat.</div>
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And this can be achieved by creating a food locker installed with misting systems. A misting system can be used a water sprayer and can help to keep food fresher for a long period.</div>
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Based on the above considerations, our research and development team at mistingsystems.net designed an extraordinary misting product that can be used in the food lockers used in space to keep foods fresher for a longer period. This misting product creates a tiny mist at regular intervals that work as a water sprayer to keep foods and vegetables fresh over a long term.</div>
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Infact the mist generated by this specially designed misting product preserves the foods from being getting spoiled.</div>
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This may sound ridiculous but in a recent test conducted it has been proved that the foods kept under this product remained fresh for more than three months. Now with this product our astronauts can have fresh and tastier food in space as we have at earth.</div>
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stanley princehttp://www.blogger.com/profile/09280760443900821968noreply@blogger.com0tag:blogger.com,1999:blog-1417039068810365781.post-3521822733870554972012-10-19T04:44:00.004-07:002016-01-12T23:15:16.022-08:00NASA Curiosity touches the Mars rock shocked by scientists<div dir="ltr" style="text-align: left;" trbidi="on">
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The mars rock touches the NASA curiosity this time it touches the more different from before Tasks. <br />
The mars rock is looks like some odd rock to see from inside from the Earth. The traveler team used 2 instruments to determine the curiosity and structure of the rock is football that type of rock is known as “Jake Matijevic “.</div>
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Edward Stopler says that the rocks looks like odd rock but it is also known as igneous rock it’s mostly found only at many volcanic regions on earth surface this statement is supposed by Edward Stopler in Pasadena he is a curiosity co investigator. The Martian rock touches mars its surprising by the by they are investigating that the Martian type but it’s very difficult to know what kind of procedures.</div>
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The Jake rock is comes under many procedures in the planets layers and the outer layer of the rock from the term crystallization and the rock contains water rich magma eminent with pressure.<br />
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The work is under the process and drive curiosity about 100 yards eastward and to target the rock using drill tool.<br />
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stanley princehttp://www.blogger.com/profile/09280760443900821968noreply@blogger.com0tag:blogger.com,1999:blog-1417039068810365781.post-62247723394521056012012-05-28T04:17:00.001-07:002016-01-12T23:18:22.209-08:00NASA Group to Analyze New Vehicle-Descent Technologies<div dir="ltr" style="text-align: left;" trbidi="on">
NASA technologists will get a opportunity next summer time to experience the good old days when Organization technical engineers would connect space-age devices to rockets just to see if the gadgets proved helpful.<br />
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In what will be the first of four high-altitude enhance routes to begin in the summertime season of 2013, technologists at NASA's Jet Space Clinical (JPL) in Pasadena, Calif., and Wallops Journey Ability in Wallops Isle, Va., are planning to evaluate new deceleration gadgets that could substitute present nice technological innovation for getting ever-larger payloads at higher levels on Mars. <br />
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NASA is using a sequence of explode snowmobile assessments at the U.S. Naval Air Weaponry Place at Chinese suppliers Pond, Calif., in planning for full-up assessments of the Low-Density Supersonic Decelerator Venture, or LDSD. The project is examining water and parachute decelerators to slowly spacecraft prior to getting and allow NASA to enhance arrived payload public, enhance getting precision and enhance the elevation of secure landing-sites. Credit: JPL<br />
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NASA hasn't examined deceleration technological innovation supersonically since 1972 when it performed four high-altitude assessments of a supersonic parachute used during the Viking program. "We’ve been trapped with that style ever since," said Level Adler, NASA’s Low-Density Supersonic Decelerator (LDSD) program lead. NASA will use the same technological innovation again this year when it provides the Fascination rover to Mars.<br />
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However, planetary landers of the next day will require much bigger move gadgets than any now in use. "What we need is new technological innovation to slowly bigger, bulkier landers from the supersonic connections of environmental use of subsonic ground-approach connections," Adler said.<br />
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The LDSD program is targeted at providing NASA a new and enhanced ability. Financed by NASA’s Area Technology Program, the JPL-led team programs to perform full-scale, stratospheric assessments of three possibly cutting-edge technological innovation. The aim is to increase their technology-readiness levels to about six, which means they could be used in a plane project, perhaps as early as 2018.<br />
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The first two are supersonic water decelerators, large stress boats that fill around an access automobile and slowly it from Mach 3.5 or quicker to about Mach 2. One of these water gadgets actions nearly 20 toes across (six meters), the other nearly 26 toes (eight meters). The third technological innovation is a 110-foot (33.5-meter) parachute to further slowly the access automobile from Mach 2 to subsonic connections needed for a secure getting. All three would be the biggest gadgets of their kind ever traveled at connections several times greater than the rate of audio.<br />
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The style involves the group to connect the test automobile outfitted with the decelerator and parachute to a Wallops-provided high-altitude enhance. Once the enhance gets to an elevation of about 22 kilometers (36 kilometers) above Global exterior, the explode would flame its applications and bring check automobile to Martian environmental densities at an elevation of 31 kilometers (50 kilometers) at Mach 4. There, check automobile would set up the supersonic decelerator, followed by the parachute.<br />
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<b>Perfect Wedding of Capabilities</b><br />
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The project harnesses the strong points of both companies, said Scott Schaire, Wallops LDSD performing project administrator. While NASA JPL and its companies are creating check automobile, decelerators, and parachute, NASA Wallops is accountable for enhance functions, enhance instrumentation, and other functions associated with enhance releases.<br />
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One considerable NASA Wallops-provided technological innovation is an entirely new enhance release program — an attempt Schaire's team started particularly for the supersonic assessments. With this new program, check automobile will be revoked from a straight, 80-foot structure. Its job is avoiding check automobile from reaching the earth as the enhance starts to increase off. A customized equipment that appears like a farm-irrigation program will help specialists lay out the enhance and a new reel automobile will hold the enhance until release. <br />
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For More Details Visit : <a href="http://www.nasa.gov/topics/technology/features/gizmo-launches.html">http://www.nasa.gov/topics/technology/features/gizmo-launches.html</a><br />
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stanley princehttp://www.blogger.com/profile/09280760443900821968noreply@blogger.com0tag:blogger.com,1999:blog-1417039068810365781.post-9356952054398902942012-05-11T02:50:00.000-07:002012-05-11T02:51:04.679-07:00NASA Spacecraft Detects Changes in Martian Sand Dunes<div dir="ltr" style="text-align: left;" trbidi="on">
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NASA's Mars Reconnaissance Orbiter has revealed that movement in sand dune fields on the Red Planet occurs on a surprisingly large scale, about the same as in dune fields on Earth.<br />
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This is unexpected because Mars has a much thinner atmosphere than Earth, is only about one percent as dense, and its high-speed winds are less frequent and weaker than Earth's.<br />
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For years, researchers debated whether sand dunes observed on Mars were mostly fossil features related to past climate, rather than currently active. In the past two years, researchers using images from Mars Reconnaissance Orbiter's High Resolution Imaging Science Experiment (HiRISE) camera have detected and reported sand movement.<br />
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Now, scientists using HiRISE images have determined that entire dunes as thick as 200 feet (61 meters) are moving as coherent units across the Martian landscape. The study was published online today by the journal Nature.<br />
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"This exciting discovery will inform scientists trying to better understand the changing surface conditions of Mars on a more global scale," said Doug McCuistion, director, NASA's Mars Exploration Program, Washington. "This improved understanding of surface dynamics will provide vital information in planning future robotic and human Mars exploration missions."<br />
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Researchers analyzed before-and-after images using a new software tool developed at the California Institute of Technology (Caltech) in Pasadena, Calif. The tool measured changes in the position of sand ripples, revealing the ripples move faster the higher up they are on a dune.<br />
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The study examined images taken in 2007 and 2010 of the Nili Patera sand dune field located near the Martian equator. By correlating the ripples' movement to their position on the dune, the analysis determined the entire dunes are moving. This allows researchers to estimate the volume, or flux, of moving sand.<br />
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"We chose Nili Patera because we knew there was sand motion going on there, and we could quantify it," said Nathan Bridges, a planetary scientist at Johns Hopkins University Applied Physics Laboratory in Laurel, Md., and lead author of the Nature paper. "The Nili dunes also are similar to dunes in places like Antarctica and to other locations on Mars."<br />
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The study adds important information about the pace at which blowing sand could be actively eroding rocks on Mars. Using the new information about the volume of sand that is moving, scientists estimate rocks in Nili Patera would be worn away at about the same pace as rocks near sand dunes in Antarctica, where similar sand fluxes occur.<br />
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"Our new data shows wind activity is indeed a major agent of evolution of the landscape on Mars," said Jean-Philippe Avouac, Caltech team leader. "This is important because it tells us something about the current state of Mars and how the planet is working today, geologically."<br />
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For more information visit <a href="http://www.nasa.gov/mission_pages/MRO/news/mro20120509.html" rel="nofollow">http://www.nasa.gov/mission_pages/MRO/news/mro20120509.html</a>
</div>stanley princehttp://www.blogger.com/profile/09280760443900821968noreply@blogger.com0tag:blogger.com,1999:blog-1417039068810365781.post-91103547904042258372012-05-08T04:49:00.000-07:002012-05-08T04:49:16.659-07:00NASA to Fly Deep Space Atomic Clock to Improve Navigation Technology<div dir="ltr" style="text-align: left;" trbidi="on">
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When people think of space technologies, many think of high-tech solar panels, complex and powerful propulsion systems or sophisticated, electronic guidance systems. Another critical piece of spaceflight technology, however, is an ultra stable, highly accurate device for timing - essential to NASA's success on deep-space exploration missions.<br><br>
NASA is preparing to fly a Deep Space Atomic Clock, or DSAC, demonstration that will revolutionize the way we conduct deep-space navigation by enabling a spacecraft to calculate its own timing and navigation data in real time. This one-way navigation technology would improve upon the current two-way system in which information is sent to Earth, requiring a ground team to calculate timing and navigation and then transmitting it back to the spacecraft. A real-time, on-board navigation capability is key to improving NASA’s capabilities for executing time critical events, such as a planetary landing or planetary "fly-by," when signal delays are too great for the ground to interact with the spacecraft during the event.<br><br>
"Adopting DSAC on future NASA missions will increase navigation and radio science data quantity by two to three times, improve data quality by up to 10 times and reduce mission costs by shifting toward a more flexible and extensible one-way radio navigation architecture," said Todd Ely, principal investigator of the Deep Space Atomic Clock Technology Demonstration at NASA's Jet Propulsion Laboratory in Pasadena, Calif. The project is part of NASA's Technology Demonstration Missions program, managed by the Marshall Space Flight Center in Huntsville, Ala., for NASA's Office of the Chief Technologist in Washington.<br><br>
The one-way deep space navigation enabled by DSAC uses the existing deep space network more efficiently than the current two-way system, thus expanding the network’s capacity without adding any new antennas or their associated costs. This is important, since future human exploration of deep space will demand more tracking from the deep space network than can currently be delivered with the existing system.<br><br>
"The Deep Space Atomic Clock flight demonstration mission will advance this laboratory-qualified technology to flight readiness and will make a practical atomic clock available to a variety of space missions," Ely said.<br><br>
The clock is a miniature mercury-ion atomic device the DSAC team will fly as a payload on an Earth orbiter in a one-year experiment to validate its operability in space and its usefulness for one-way navigation.<br><br>
"A potential use for DSAC on a future mission would be in a follow-up to the Mars Reconnaissance Orbiter," Ely said. NASA's Mars Reconnaissance Orbiter launched to Mars in 2005 on a search for evidence that water existed on the planet's surface for enough time to provide a habitat for life. The orbiter completed its primary science phase in 2008 and continues to work in an extended mission. Atomic clocks are the most accurate timekeeping method known and are used as the primary standard for international time distribution services -- to control the frequency of television broadcasts, and in global navigation satellite systems such as the Global Positioning System.<br><br>
For more information visit <a href="http://www.nasa.gov/mission_pages/tdm/clock/dsac.html" rel="nofollow">http://www.nasa.gov/mission_pages/tdm/clock/dsac.html</a>
<br /></div>stanley princehttp://www.blogger.com/profile/09280760443900821968noreply@blogger.com0tag:blogger.com,1999:blog-1417039068810365781.post-10060721143146023992012-05-04T23:53:00.000-07:002015-03-12T23:33:29.891-07:00NASA's WISE Catches Aging Star Erupting With Dust<div dir="ltr" style="text-align: left;" trbidi="on">
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Images from NASA's Wide-field Infrared Survey Explorer (WISE) reveal an old star in the throes of a fiery outburst, spraying the cosmos with dust. The findings offer a rare, real-time look at the process by which stars like our sun seed the universe with building blocks for other stars, planets and even life.<br><br>
The star, catalogued as WISE J180956.27-330500.2, was discovered in images taken during the WISE survey in 2010, the most detailed infrared survey to date of the entire celestial sky. It stood out from other objects because it glowed brightly with infrared light. When compared to images taken more than 20 years ago, astronomers found the star was 100 times brighter.<br><br>
"We were not searching specifically for this phenomenon, but because WISE scanned the whole sky, we can find such unique objects," said Poshak Gandhi of the Japan Aerospace Exploration Agency (JAXA), lead author of a new paper to be published in the Astrophysical Journal Letters.<br><br>
Results indicate the star recently exploded with copious amounts of fresh dust, equivalent in mass to our planet Earth. The star is heating the dust and causing it to glow with infrared light.<br><br>
"Observing this period of explosive change while it is actually ongoing is very rare," said co-author Issei Yamamura of JAXA. "These dust eruptions probably occur only once every 10,000 years in the lives of old stars, and they are thought to last less than a few hundred years each time. It's the blink of an eye in cosmological terms."<br><br>
The aging star is in the "red giant" phase of its life. Our own sun will expand into a red giant in about 5 billion years. When a star begins to run out of fuel, it cools and expands. As the star puffs up, it sheds layers of gas that cool and congeal into tiny dust particles. This is one of the main ways dust is recycled in our universe, making its way from older stars to newborn solar systems. The other way, in which the heaviest of elements are made, is through the deathly explosions, or supernovae, of the most massive stars.<br><br>
"It's an intriguing glimpse into the cosmic recycling program," said Bill Danchi, WISE program scientist at NASA Headquarters in Washington. "Evolved stars, which this one appears to be, contribute about 50 percent of the particles that make up humans."<br><br>
Astronomers know of one other star currently pumping out massive amounts of dust. Called Sakurai's Object, this star is farther along in the aging process than the one discovered recently by WISE.<br><br>
After Poshak and his team discovered the unusual, dusty star with WISE, they went back to look for it in previous infrared all-sky surveys. The object was not seen at all by the Infrared Astronomical Satellite (IRAS), which flew in 1983, but shows up brightly in images taken as part of the Two Micron All-Sky Survey (2MASS) in 1998.<br><br>
Poshak and his colleagues calculated the star appears to have brightened dramatically since 1983. The WISE data show the dust has continued to evolve over time, with the star now hidden behind a very thick veil. The team plans to follow up with space- and ground-based telescopes to confirm its nature and to better understand how older stars recycle dust back into the cosmos.<br><br>
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For more information visit <a href="http://www.nasa.gov/mission_pages/WISE/news/wise_20120426.html" rel="nofollow">http://www.nasa.gov/mission_pages/WISE/news/wise_20120426.html</a>
</div>stanley princehttp://www.blogger.com/profile/09280760443900821968noreply@blogger.com0tag:blogger.com,1999:blog-1417039068810365781.post-34507252744068673122012-04-19T03:08:00.001-07:002012-04-19T03:11:21.038-07:00Dark Heart of a Cosmic Collision<div dir="ltr" style="text-align: left;" trbidi="on"><div class="separator" style="clear: both; text-align: center;"><img border="0" height="300" src="http://2.bp.blogspot.com/-DZbTqGru2Tg/T4_jQegL-RI/AAAAAAAAAeA/2Isa6eaP-oY/s400/infraredwavelength.jpg" width="400" /></div><br />
Infrared and X-ray observations from two space telescopes have been combined to create a unique look at violent events within the giant galaxy Centaurus A. The observations strengthen the view that the galaxy may have been created by the cataclysmic collision of two older galaxies.<br />
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The infrared light was captured by the European Space Agency's Herschel Space Observatory, a mission with important NASA contributions. The X-ray observations were made by the European Space Agency's XMM-Newton space telescope.<br />
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Centaurus A is the closest giant elliptical galaxy to Earth, at a distance of around 12 million light-years. It stands out because it harbors a massive black hole at its core and emits intense blasts of radio waves.<br />
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While previous images taken in visible light hinted at the complex inner structure in Centaurus A, combining the output of two orbiting observatories working at almost opposite ends of the electromagnetic spectrum has revealed the unusual structure in much greater detail.<br />
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The galaxy was observed by astronomer Sir John Herschel in 1847 during his survey of the southern skies. Now, more than 160 years later, the observatory bearing his family name has played a unique role in uncovering some of its secrets.<br />
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With the Herschel observatory, the giant black scar of obscuring dust crossing the center of Centaurus A all but disappears when viewed at long infrared wavelengths. The images show the flattened inner disk of a spiral galaxy, the shape of which scientists believe is due to a collision with an elliptical galaxy during a past epoch.<br />
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The Herschel data also uncover evidence for intense star birth toward the center of the galaxy, along with two jets emanating from the galaxy's core -- one of them 15,000 light-years long. Newly discovered clouds co-aligned with the jets can also be seen in Herschel's view.<br />
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The XMM-Newton X-ray observatory recorded the high-energy glow from one of the jets, extending more than 12,000 light-years away from the galaxy's bright nucleus. XMM-Newton's view shows not only the way that the jet interacts with the surrounding interstellar matter, but also the galaxy's intensely active nucleus, and its large gaseous halo.<br />
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The jets seen by both satellites are evidence of the supermassive black hole --10 million times the mass of our sun -- at the center of the galaxy. <br />
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For more information visit <a href="http://www.nasa.gov/mission_pages/herschel/news/herschel20120404.html" rel="nofollow">http://www.nasa.gov/mission_pages/herschel/news/herschel20120404.html</a></div>stanley princehttp://www.blogger.com/profile/09280760443900821968noreply@blogger.com0tag:blogger.com,1999:blog-1417039068810365781.post-24902528846131307012012-04-10T01:33:00.000-07:002012-04-10T01:33:25.375-07:00New Ideas Sharpen Focus for Greener Aircraft<div dir="ltr" style="text-align: left;" trbidi="on"><div class="separator" style="clear: both; text-align: center;"><img border="0" height="459" src="http://4.bp.blogspot.com/-HRUfAUIakD8/T4PwJRTlOlI/AAAAAAAAAd0/uKD3VzhZ5L4/s640/aircraft.jpg" width="640" /></div><br />
Leaner, greener flying machines for the year 2025 are on the drawing boards of three industry teams under contract to the NASA Aeronautics Research Mission Directorate's Environmentally Responsible Aviation Project.<br />
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Teams from The Boeing Company in Huntington Beach, Calif., Lockheed Martin in Palmdale, Calif., and Northrop Grumman in El Segundo, Calif., have spent the last year studying how to meet NASA goals to develop technology that would allow future aircraft to burn 50 percent less fuel than aircraft that entered service in 1998 (the baseline for the study), with 50 percent fewer harmful emissions; and to shrink the size of geographic areas affected by objectionable airport noise by 83 percent.<br />
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"The real challenge is we want to accomplish all these things simultaneously," said ERA project manager Fay Collier. "It's never been done before. We looked at some very difficult metrics and tried to push all those metrics down at the same time."<br />
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So NASA put that challenge to industry – awarding a little less than $11 million to the three teams to assess what kinds of aircraft designs and technologies could help meet the goals. The companies have just given NASA their results.<br />
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"We'll be digesting the three studies and we'll be looking into what to do next," said Collier.<br />
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Boeing's advanced vehicle concept centers around the company's now familiar blended wing body design as seen in the sub-scale remotely piloted X-48, which has been wind tunnel tested at NASA's Langley Research Center and flown at NASA's Dryden Flight Research Center. One thing that makes this concept different from current airplanes is the placement of its Pratt & Whitney geared turbofan engines. The engines are on top of the plane's back end, flanked by two vertical tails to shield people on the ground from engine noise. The aircraft also would feature an advanced lightweight, damage tolerant, composite structure; technologies for reducing airframe noise; advanced flight controls; hybrid laminar flow control, which means surfaces designed to reduce drag; and long-span wings which improve fuel efficiency.<br />
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Lockheed Martin took an entirely different approach. Its engineers proposed a box wing design, in which a front wing mounted on the lower belly of the plane is joined at the tips to an aft wing mounted on top of the plane. The company has studied the box wing concept for three decades, but has been waiting for lightweight composite materials, landing gear technologies, hybrid laminar flow and other tools to make it a viable configuration. Lockheed's proposal combines the unique design with a Rolls Royce Liberty Works Ultra Fan Engine. This engine has a bypass ratio that is approximately five times greater than current engines, pushing the limits of turbofan technology. <br />
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For more information visit <a href="http://www.nasa.gov/topics/aeronautics/features/greener_aircraft.html" rel="nofollow">http://www.nasa.gov/topics/aeronautics/features/greener_aircraft.html</a></div>stanley princehttp://www.blogger.com/profile/09280760443900821968noreply@blogger.com0tag:blogger.com,1999:blog-1417039068810365781.post-49829186334793224812012-03-04T22:57:00.001-08:002012-03-04T22:58:20.289-08:00Supersonic Research Fleet Grows at Kennedy<div dir="ltr" style="text-align: left;" trbidi="on"><div class="separator" style="clear: both; text-align: center;"><img border="0" height="267" src="http://4.bp.blogspot.com/-MhTpMYPbHfY/T1Ri8ozjljI/AAAAAAAAAdQ/r-E2tnIJaVg/s400/main11_2012-1070.jpg" width="400" /></div><br />
<div style="text-align: justify;">The final pieces of a unique squadron of supersonic fighters arrived at NASA's Kennedy Space Center in Florida on Thursday, Jan. 19, where they will be reassembled and put to work with a private company aiming to use them for research and microgravity training.</div><div style="text-align: justify;"><br />
</div><div style="text-align: justify;">The new planes were part of a group of five F-104 fighters bought by Starfighters Inc. from the Italian Air Force. The company already had four of the aircraft, but that wasn't enough for the company to pursue a number of different opportunities.</div><div style="text-align: justify;"><br />
</div><div style="text-align: justify;">With nine aircraft at his disposal, Starfighters owner Rick Svetkoff said there will always be aircraft available to fly missions for a variety of customers. As importantly, the company will have what it needs to fly two aircraft on a single mission, with one serving as a chase plane to photograph experiments.</div><div style="text-align: justify;"><br />
</div><div style="text-align: justify;">"Now we're in a position where we can really start operations," Svetkoff said. "Before, we couldn't do a lot of things we wanted to do."</div><div style="text-align: justify;"><br />
</div><div style="text-align: justify;">Starfighters operates out of a hangar at the Shuttle Landing Facility at Kennedy under an agreement with Kennedy. Svetkoff's main goal is to fly research and development missions, ranging from experiments flown for universities to evaluating rocket and spacecraft components in high-stress environments including high-acceleration and microgravity.</div><div style="text-align: justify;"><br />
</div><div style="text-align: justify;">Space Florida and Embry-Riddle University already have partnerships with the company.</div><div style="text-align: justify;"><br />
</div><div style="text-align: justify;">Because the aircraft can soar to some 70,000 feet and speed past Mach 2, it can be used to launch small satellites into space. The 19-foot-long, 900-pound rocket, about the size of a Sparrow missile, has already been tested in a series of taxi runs hanging from an F-104's wings.</div><div style="text-align: justify;"><br />
</div><div style="text-align: justify;">Test flights carrying the rocket but not launching it will be conducted in the next month and the first launch is in works to take place in the summer.</div><div style="text-align: justify;"><br />
</div><div style="text-align: justify;">The rocket is meant to take small experiments into space but not into orbit. Instead, the rocket will parachute back to Earth and be recovered from the ocean for reuse. Svetkoff expects to launch about 100 suborbital missions a year from the Starfighters.</div><div style="text-align: justify;"><br />
</div><div style="text-align: justify;">In less than a year, though, Svetkoff said he expects to start launching nanosatellites into orbit using a similar approach. After all, an F-104 can match a rocket's launch performance in some areas.</div><div style="text-align: justify;"><br />
</div><div style="text-align: justify;">The F-104 Starfighter is a decades-old, supersonic fighter design that was put into service during the Cold War to intercept Soviet aircraft. Known as "the missile with a man in it" because of its high speed and stubby wings, the fighter was developed by Lockheed Martin's Kelly Johnson, the aerospace icon who also developed the SR-71 and U-2 aircraft.</div><div style="text-align: justify;"><br />
</div><div style="text-align: justify;">Able to reach a top speed of Mach 2.4 and fly to about 70,000 feet, the F-104 found a second career with NASA in the 1960s. It helped train astronauts for microgravity and to keep their skills up in the demanding world of high-speed flight.</div><div style="text-align: justify;"><br />
</div><div style="text-align: justify;">"Anything an F-16 or an F-18 can do, we can do with this aircraft, performance-wise," Svetkoff said.</div><div style="text-align: justify;"><br />
</div><div style="text-align: justify;">The Starfighters fleet includes a mix of single-seat versions and two-seaters, each playing specific roles for the company.</div><div style="text-align: justify;"><br />
</div><div style="text-align: justify;">Research and development flights are expected to add another 100 missions to the Starfighters' log each year, Svetkoff said.</div><div style="text-align: justify;"><br />
</div><div style="text-align: justify;">The experimentation is not expected to end with machinery and experiments, though. As private companies develop their own spacecraft to launch humans into space in partnerships with NASA, some of those companies are already talking about using the Starfighters to train for microgravity and other situations, just as NASA's astronauts did in past decades.</div><div style="text-align: justify;"><br />
</div><div style="text-align: justify;">For the moment though, the attention is on getting the new aircraft cleaned and assembled. The engines and other components will be taken apart and cleaned, and then put back together. New avionics packages including digital displays will be added to the new aircraft, too. It will take about three months to complete the first one, but the squadron should be ready in six months.</div><div style="text-align: justify;"><br />
</div><div style="text-align: justify;">"This shows a serious commitment," Svetkoff said.</div><div style="text-align: justify;"><br />
</div>For more information visit <a href="http://www.nasa.gov/centers/kennedy/news/starfightersnewplanes.html" rel="nofollow">http://www.nasa.gov/centers/kennedy/news/starfightersnewplanes.html </a><br />
<br />
</div>stanley princehttp://www.blogger.com/profile/09280760443900821968noreply@blogger.com0tag:blogger.com,1999:blog-1417039068810365781.post-83343423195075954842012-03-02T22:23:00.002-08:002012-03-02T22:23:37.576-08:00Get Your Site Analysis Report from Search Engine Genie<div dir="ltr" style="text-align: left;" trbidi="on">The one best start that you can give yourself on knowing how to make your website get the attention it deserves is by knowing how much Search Engine Friendly it is? You know that your website is good enough to win business when customers visit but, you are left clue less about the reasons for which your site getting only a few visitors. There might be many reasons for this and the right way to know what your site lacks is to contact a Search Engine Optimization company and ask them a Comprehensive site analysis. <br />
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The use of knowing about your website in detail is to know where it falls back and what can be done to give a lift to its setback. While you know that expert help is necessary in this, it is wise to hold on to an experienced Search Engine Marketing and optimization firm like Search Engine Genie for further assistance. With the amount of care they show in analyzing about your website’s state, you should know about their genuine efforts in ranking your website high within the time frame they agree upon. It is time hire <b>searchenginegenie</b> and beat your competitors. Log on to <b>searchenginegenie.com</b> to find more about their services and how they are equipped to handle the ranking factors of search engines.</div>stanley princehttp://www.blogger.com/profile/09280760443900821968noreply@blogger.com0tag:blogger.com,1999:blog-1417039068810365781.post-84522193577321294242012-03-01T22:30:00.000-08:002012-03-01T22:30:14.413-08:00Add Salt? Astronauts' Bones Say Please Don't<div dir="ltr" style="text-align: left;" trbidi="on"><div class="separator" style="clear: both; text-align: center;"><img border="0" height="400" src="http://4.bp.blogspot.com/-5vxy6dlViH8/T1BolclEPDI/AAAAAAAAAdE/BmNLdDr42UE/s400/625401main_skeleton_XL11.jpg" width="320" /></div><br />
<div style="text-align: justify;">Osteoporosis is a harsh disease that reduces the quality of life for millions and costs Europe around €25 billion ($31 billion) each year. It typically affects the elderly, so the rise in life expectancy in developed countries means the problems inflicted by osteoporosis are increasing.</div><div style="text-align: justify;"><br />
</div><div style="text-align: justify;">Fortunately, research done in space may change the game. Astronauts on the International Space Station experience accelerated osteoporosis because of weightlessness, but it is carefully controlled, and they can regain their lost bone mass once they are back on Earth.</div><div style="text-align: justify;"><br />
</div><div style="text-align: justify;">Studying what happens during long spaceflights offers a good insight into the process of osteoporosis -- losing calcium and changing bone structure -- and helps to develop methods to combat it.</div><div style="text-align: justify;"><br />
</div><div style="text-align: justify;">It has been known since the 1990s that the human body holds on to sodium, without the corresponding water retention, during long stays in space. But the textbooks said this was not possible. "Sodium retention in space" became an important subject to study.</div><div style="text-align: justify;"><br />
</div><div style="text-align: justify;">Salt intake was investigated in a series of studies, in ground-based simulations and in space, and it was found that not only is sodium retained (probably in the skin), but it also affects the acid balance of the body and bone metabolism. So, high salt intake increases acidity in the body, which can accelerate bone loss.</div><div style="text-align: justify;"><br />
</div><div style="text-align: justify;">The European Space Agency's, or ESA’s, recent SOdium LOad in microgravity, or SOLO, study zoomed in on this question. Nine crew members, including ESA's Frank De Winne and Paolo Nespoli during their long-duration flights in 2010 and 2011, followed low -- and high-salt diets. The expected results may show that additional negative effects can be avoided either by reducing sodium intake or by using a simple alkalizing agent like bicarbonate to counter the acid imbalance.</div><div style="text-align: justify;"><br />
</div><div style="text-align: justify;">This space research directly benefits everybody on Earth who is prone to osteoporosis.</div><br />
For more information visit <a href="http://www.nasa.gov/mission_pages/station/research/benefits/salt.html" rel="nofollow">http://www.nasa.gov/mission_pages/station/research/benefits/salt.html</a></div>stanley princehttp://www.blogger.com/profile/09280760443900821968noreply@blogger.com0tag:blogger.com,1999:blog-1417039068810365781.post-7499467286224907462012-02-27T01:46:00.000-08:002012-02-27T01:46:13.757-08:00Fifth ATV named following Georges Lemaitre<div dir="ltr" style="text-align: left;" trbidi="on"><!--[if gte mso 9]><xml> <o:OfficeDocumentSettings> <o:RelyOnVML/> <o:AllowPNG/> </o:OfficeDocumentSettings> </xml><![endif]--><!--[if gte mso 9]><xml> <w:WordDocument> <w:View>Normal</w:View> <w:Zoom>0</w:Zoom> <w:TrackMoves/> <w:TrackFormatting/> <w:PunctuationKerning/> <w:ValidateAgainstSchemas/> <w:SaveIfXMLInvalid>false</w:SaveIfXMLInvalid> <w:IgnoreMixedContent>false</w:IgnoreMixedContent> <w:AlwaysShowPlaceholderText>false</w:AlwaysShowPlaceholderText> <w:DoNotPromoteQF/> <w:LidThemeOther>EN-US</w:LidThemeOther> <w:LidThemeAsian>X-NONE</w:LidThemeAsian> <w:LidThemeComplexScript>X-NONE</w:LidThemeComplexScript> <w:Compatibility> <w:BreakWrappedTables/> <w:SnapToGridInCell/> <w:WrapTextWithPunct/> <w:UseAsianBreakRules/> <w:DontGrowAutofit/> <w:SplitPgBreakAndParaMark/> <w:DontVertAlignCellWithSp/> <w:DontBreakConstrainedForcedTables/> <w:DontVertAlignInTxbx/> <w:Word11KerningPairs/> <w:CachedColBalance/> </w:Compatibility> <m:mathPr> <m:mathFont m:val="Cambria Math"/> <m:brkBin m:val="before"/> <m:brkBinSub m:val="--"/> <m:smallFrac m:val="off"/> <m:dispDef/> <m:lMargin m:val="0"/> <m:rMargin m:val="0"/> <m:defJc m:val="centerGroup"/> <m:wrapIndent m:val="1440"/> <m:intLim m:val="subSup"/> <m:naryLim m:val="undOvr"/> </m:mathPr></w:WordDocument> </xml><![endif]--><!--[if gte mso 9]><xml> <w:LatentStyles DefLockedState="false" DefUnhideWhenUsed="true"
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<b>Georges Lemaitre </b>teaching at the Catholic University of Leuven, Belgium. In 1927, Georges Lemaitre exposed a family of solutions to Einstein's relativity equations that describe an expanding Universe quite than a static one, and provide the first observational opinion of the Hubble steady. The theory later became much improved known as the Big Bang theory. Identification <b>ESA</b>'s fifth Automated Transfer Vehicle after Belgian scientist Georges Lemaitre continue the custom of drawing on great European visionaries to reflect Europe's bottomless roots in science, technology and culture. Credits: Katholieke Universiteit Leuven.<br />
<br />
<b>ESA's Automated Transfer Vehicles (ATVs) </b>are a necessary contribution by Europe to organization the International Space Station. Naming the fifth after Belgian scientist Georges Lemaitre continues the custom of drawing on great European visionaries to reflect Europe's deep roots in science, technology and culture.<br />
<br />
The first Automated Transfer Vehicle (ATV), which made a flawless flight in 2008, was sname after French science fiction author Jules Verne. It was follow in 2011 by ATV-2, named in honor of German mathematician and astronomer Johannes Kepler.<br />
<br />
It will be the twist of the third ATV, name following the Italian physicist and space pioneer Edoardo Amaldi, to head towards the Space Station on 9 March.ATV-4, aim for launch in early 2013, carries the name of Albert Einstein.Naming the last vehicle of the family, ATV-5, after Belgian physicist Georges Lemaitre, father of the Big Bang theory, continue this approach.<br />
</div>stanley princehttp://www.blogger.com/profile/09280760443900821968noreply@blogger.com0tag:blogger.com,1999:blog-1417039068810365781.post-68568059165070776072012-02-20T02:51:00.000-08:002012-02-20T02:51:00.193-08:00NuSTAR mate to Its Rocket<div dir="ltr" style="text-align: left;" trbidi="on"><!--[if gte mso 9]><xml> <w:WordDocument> <w:View>Normal</w:View> <w:Zoom>0</w:Zoom> <w:TrackMoves/> <w:TrackFormatting/> <w:PunctuationKerning/> <w:ValidateAgainstSchemas/> <w:SaveIfXMLInvalid>false</w:SaveIfXMLInvalid> <w:IgnoreMixedContent>false</w:IgnoreMixedContent> <w:AlwaysShowPlaceholderText>false</w:AlwaysShowPlaceholderText> <w:DoNotPromoteQF/> <w:LidThemeOther>EN-US</w:LidThemeOther> <w:LidThemeAsian>X-NONE</w:LidThemeAsian> <w:LidThemeComplexScript>X-NONE</w:LidThemeComplexScript> <w:Compatibility> <w:BreakWrappedTables/> <w:SnapToGridInCell/> <w:WrapTextWithPunct/> <w:UseAsianBreakRules/> <w:DontGrowAutofit/> <w:SplitPgBreakAndParaMark/> <w:DontVertAlignCellWithSp/> <w:DontBreakConstrainedForcedTables/> <w:DontVertAlignInTxbx/> <w:Word11KerningPairs/> <w:CachedColBalance/> </w:Compatibility> <w:BrowserLevel>MicrosoftInternetExplorer4</w:BrowserLevel> <m:mathPr> <m:mathFont m:val="Cambria Math"/> <m:brkBin m:val="before"/> <m:brkBinSub m:val="--"/> <m:smallFrac m:val="off"/> <m:dispDef/> <m:lMargin m:val="0"/> <m:rMargin m:val="0"/> <m:defJc m:val="centerGroup"/> <m:wrapIndent m:val="1440"/> <m:intLim m:val="subSup"/> <m:naryLim m:val="undOvr"/> </m:mathPr></w:WordDocument> </xml><![endif]--><!--[if gte mso 9]><xml> <w:LatentStyles DefLockedState="false" DefUnhideWhenUsed="true"
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<div class="MsoNormal"><b>NuSTAR </b>will search the newest, densest and most energetic objects in space, counting black holes and the remnants of exploded stars. It will be the primary space telescope to imprison sharp images in high-energy X-rays, giving astronomers a innovative tool for sympathetic the great side of our universe.</div><div class="MsoNormal"><br />
</div><div class="MsoNormal"><b>NuSTAR </b>is a little Explorer mission led by the California Institute of Technology and managed by NASA's Jet Propulsion Laboratory, both in Pasadena, Calif., for NASA's Science Mission Directorate. The spacecraft was build by Orbital Sciences Corporation, Dulles, Va. Its instrument was built by a consortium including Caltech; JPL; Columbia University, New York; NASA's Goddard Space Flight Center in Greenbelt, Md.; the Danish Technical University in Denmark; the University of California, Berkeley; and ATK Aerospace Systems, Goleta, Calif. </div><div class="MsoNormal"><br />
</div><div class="MsoNormal">NuSTAR will be operated by UC Berkeley, with the Italian Space Agency as long as its equatorial ground station located at Malindi, Kenya. The mission's outreach program is based at Sonoma State University, Calif. NASA's Explorer Program is managed by Goddard. JPL is managed by Caltech for NASA.</div></div>stanley princehttp://www.blogger.com/profile/09280760443900821968noreply@blogger.com0tag:blogger.com,1999:blog-1417039068810365781.post-41173790602634030122012-02-13T01:04:00.000-08:002012-02-13T01:04:25.454-08:00Astronauts seen as well as heard<div dir="ltr" style="text-align: left;" trbidi="on"><!--[if gte mso 9]><xml> <w:WordDocument> <w:View>Normal</w:View> <w:Zoom>0</w:Zoom> <w:TrackMoves/> <w:TrackFormatting/> <w:PunctuationKerning/> <w:ValidateAgainstSchemas/> <w:SaveIfXMLInvalid>false</w:SaveIfXMLInvalid> <w:IgnoreMixedContent>false</w:IgnoreMixedContent> <w:AlwaysShowPlaceholderText>false</w:AlwaysShowPlaceholderText> <w:DoNotPromoteQF/> <w:LidThemeOther>EN-US</w:LidThemeOther> <w:LidThemeAsian>X-NONE</w:LidThemeAsian> <w:LidThemeComplexScript>X-NONE</w:LidThemeComplexScript> <w:Compatibility> <w:BreakWrappedTables/> <w:SnapToGridInCell/> <w:WrapTextWithPunct/> <w:UseAsianBreakRules/> <w:DontGrowAutofit/> <w:SplitPgBreakAndParaMark/> <w:DontVertAlignCellWithSp/> <w:DontBreakConstrainedForcedTables/> <w:DontVertAlignInTxbx/> <w:Word11KerningPairs/> <w:CachedColBalance/> </w:Compatibility> <w:BrowserLevel>MicrosoftInternetExplorer4</w:BrowserLevel> <m:mathPr> <m:mathFont m:val="Cambria Math"/> <m:brkBin m:val="before"/> <m:brkBinSub m:val="--"/> <m:smallFrac m:val="off"/> <m:dispDef/> <m:lMargin m:val="0"/> <m:rMargin m:val="0"/> <m:defJc m:val="centerGroup"/> <m:wrapIndent m:val="1440"/> <m:intLim m:val="subSup"/> <m:naryLim m:val="undOvr"/> </m:mathPr></w:WordDocument> </xml><![endif]--><!--[if gte mso 9]><xml> <w:LatentStyles DefLockedState="false" DefUnhideWhenUsed="true"
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<div class="MsoNormal">Seeing <b>ESA astronaut</b> Andre Kuipers on the International Space Station is a regular incidence these days. You turn on your TV or check Twitter and there he is. Since present are no cable sprawling from the Station to Earth, just how does this come about?</div><div class="MsoNormal"><br />
</div><div class="MsoNormal">The reply, of course, is via satellite. While the reply may be simple, the method is more complex. Behind Andre's smiling face is a compound system of jargon-filled amplifiers, multiplexers, antennas, nodes and signal modulation.</div><div class="MsoNormal"><br />
</div><div class="MsoNormal">Thanks to satcoms, the team can directly take delivery of emails on the Space Station, they can create private calls via IP phones, and we can see them during televise video conference.</div><div class="MsoNormal"><br />
</div><div class="MsoNormal">The Station is airborne in a low orbit - around 400 km up - which income that shortest communications can happen only when it passes over a ground station. In its place, signals from the Station are primary sent to '<b>geostationary</b>' satellites balanced 36 000 km above the equator.</div><div class="MsoNormal"><br />
</div><div class="MsoNormal">Geostationary satellites take precisely a day to circle Earth, creation them appear stationary in our skies. This allows continuous contact with ground stations; enable them to communicate the Station's signals to a middle ground station on Earth additional often.The procedure is upturned when sites such as the Columbus control centre in <b>Munich, Germany</b>, send signal up to the Station.</div></div>stanley princehttp://www.blogger.com/profile/09280760443900821968noreply@blogger.com0tag:blogger.com,1999:blog-1417039068810365781.post-75088349035672756822012-01-30T22:20:00.000-08:002012-01-30T22:20:35.820-08:00Goddard Director Leaving for Ball Aerospace<div dir="ltr" style="text-align: left;" trbidi="on"><!--[if gte mso 9]><xml> <w:LatentStyles DefLockedState="false" DefUnhideWhenUsed="true"
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UnhideWhenUsed="false" Name="Colorful Grid Accent 4"/> <w:LsdException Locked="false" Priority="60" SemiHidden="false"
UnhideWhenUsed="false" Name="Light Shading Accent 5"/> <w:LsdException Locked="false" Priority="61" SemiHidden="false"
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UnhideWhenUsed="false" Name="Light Grid Accent 5"/> <w:LsdException Locked="false" Priority="63" SemiHidden="false"
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UnhideWhenUsed="false" QFormat="true" Name="List Paragraph"/> <w:LsdException Locked="false" Priority="29" SemiHidden="false"
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</style> <![endif]--> <div class="MsoNormal" style="text-align: justify;"><b>Robert Strain </b>will leave as director of <b>NASA’s Goddard Space Flight Center</b> in Greenbelt, Md., to turn out to be chief operating officer of Ball Aerospace & Technologies Corp. Strain’s last day at Goddard will be March 4, NASA spokesman Mark Hess said. damage, who has detained the top post at Goddard for more than three years, announced his acceptance <b>Jan. 30.</b></div><div class="MsoNormal" style="text-align: justify;"><br />
</div><div class="MsoNormal" style="text-align: justify;"><span style="mso-spacerun: yes;"> </span>NASA has not yet selected a substitute for Strain, Hess said.</div><div class="MsoNormal" style="text-align: justify;"><br />
</div><div class="MsoNormal" style="text-align: justify;"><span style="mso-spacerun: yes;"> </span>At Boulder, Colo.-based Ball, Strain will be accountable for day-to-day operation of the company’s Civil and Operational Space, Tactical Solutions, <b>National Defense,</b> and system Engineering Solutions units. He will report in a straight line to <b>David Taylor</b>, president and chief executive of Ball Aerospace.</div><div class="MsoNormal" style="text-align: justify;"><br />
</div><div class="MsoNormal" style="text-align: justify;"><span style="mso-spacerun: yes;"> </span>Before taking the wheel of Goddard in 2008, Strain was the head of the Space Department at the Johns Hopkins University Applied Physics Lab in Laurel, Md. Prior to joining Hopkins in 2004, Strain exhausted 10 years at Dulles, Va.-based satellite and rocket maker Orbital Sciences Corp., where he was decision-making vice president of space systems.</div><div class="MsoNormal" style="text-align: justify;"><br />
</div><div class="MsoNormal" style="text-align: justify;"><span style="mso-spacerun: yes;"></span>Ball is working on more than a few big projects being managed by Goddard. Among these is the Joint Polar Satellite System (<b>JPSS</b>), the next-generation of U.S. civil polar-orbiting weather satellites.</div><br />
Ball is the prime contractor for the JPSS-1 spacecraft, which NASA is procuring for the National Oceanic and Atmospheric management. Ball has a <b>$248 million</b> fixed-price contract to build JPSS-1, and a separate $82.4 million contract to construct a clone of the Ozone map and Profile Suite instrument.<br />
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</div><span style="mso-spacerun: yes;"> </span>The 2012 budget for <b>JPSS is $924 million.</b> </div>stanley princehttp://www.blogger.com/profile/09280760443900821968noreply@blogger.com0tag:blogger.com,1999:blog-1417039068810365781.post-21752414059761102912012-01-25T22:05:00.000-08:002012-01-25T22:05:56.134-08:00NASA'S J-2X locomotive kick Off 2012 With Power pack test<div dir="ltr" style="text-align: left;" trbidi="on"><!--[if gte mso 9]><xml> <w:WordDocument> <w:View>Normal</w:View> <w:Zoom>0</w:Zoom> <w:TrackMoves/> <w:TrackFormatting/> <w:PunctuationKerning/> <w:ValidateAgainstSchemas/> <w:SaveIfXMLInvalid>false</w:SaveIfXMLInvalid> <w:IgnoreMixedContent>false</w:IgnoreMixedContent> <w:AlwaysShowPlaceholderText>false</w:AlwaysShowPlaceholderText> <w:DoNotPromoteQF/> <w:LidThemeOther>EN-US</w:LidThemeOther> <w:LidThemeAsian>X-NONE</w:LidThemeAsian> <w:LidThemeComplexScript>X-NONE</w:LidThemeComplexScript> <w:Compatibility> <w:BreakWrappedTables/> <w:SnapToGridInCell/> <w:WrapTextWithPunct/> <w:UseAsianBreakRules/> <w:DontGrowAutofit/> <w:SplitPgBreakAndParaMark/> <w:DontVertAlignCellWithSp/> <w:DontBreakConstrainedForcedTables/> <w:DontVertAlignInTxbx/> <w:Word11KerningPairs/> <w:CachedColBalance/> </w:Compatibility> <w:BrowserLevel>MicrosoftInternetExplorer4</w:BrowserLevel> <m:mathPr> <m:mathFont m:val="Cambria Math"/> <m:brkBin m:val="before"/> <m:brkBinSub m:val="--"/> <m:smallFrac m:val="off"/> <m:dispDef/> <m:lMargin m:val="0"/> <m:rMargin m:val="0"/> <m:defJc m:val="centerGroup"/> <m:wrapIndent m:val="1440"/> <m:intLim m:val="subSup"/> <m:naryLim m:val="undOvr"/> </m:mathPr></w:WordDocument> </xml><![endif]--><!--[if gte mso 9]><xml> <w:LatentStyles DefLockedState="false" DefUnhideWhenUsed="true"
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<div class="MsoNormal" style="text-align: justify;">A innovative sequence of tests on the locomotive that will help take humans to bottomless space will begin next week at <i><b>NASA's Stennis Space Center in southern Mississippi.</b></i> The test on the J-2X engine bring NASA one pace closer to the first human-rated liquid oxygen and liquid hydrogen rocket train to be urbanized in <b>40 years.</b></div><div class="MsoNormal" style="text-align: justify;"><br />
</div><div class="MsoNormal" style="text-align: justify;">Tests will center on the power pack for the<b> J-2X. </b>This extremely well-organized and versatile higher rocket engine is being intended to power the upper stage of NASA's Space Launch System, a new heavy-lift launch vehicle capable of missions beyond low-Earth orbit. The power pack comprise components on the top portion of the engine, including the gas generator, oxygen and fuel turbo pumps, and related ducts and valves that bring the propellants jointly to make burning and make thrust.</div><div class="MsoNormal" style="text-align: justify;"><br />
</div><div class="separator" style="clear: both; text-align: center;"><a href="http://3.bp.blogspot.com/-V22V2_AZaSw/TyDtLmzSseI/AAAAAAAAAc4/aMtX4AS87w0/s1600/power-pack.png" imageanchor="1" style="margin-left: 1em; margin-right: 1em;"><img border="0" src="http://3.bp.blogspot.com/-V22V2_AZaSw/TyDtLmzSseI/AAAAAAAAAc4/aMtX4AS87w0/s1600/power-pack.png" /></a></div><div class="MsoNormal" style="text-align: center;"><br />
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</div><div class="MsoNormal" style="text-align: justify;"><i><b>"The J-2X upper stage engine is vital to achieve the full open ability of the heavy-lift Space Launch System," said William Gerstenmaier, NASA's associate manager for the Human examination and Operations Mission Directorate. "The testing today will help ensure that a key force element is ready to support exploration across the solar system."</b></i></div><div class="MsoNormal" style="text-align: justify;"><br />
</div><div class="MsoNormal" style="text-align: justify;">About a dozen power pack tests of unreliable length are slated now from side to side summer at Stennis' A-1 Test Stand. By unraveling the engine mechanism the thrust<b> chamber assembly, </b>counting the main combustion chamber, main injector and needle engineers can more with no trouble push the various components to function over a wide variety of conditions to ensure the parts' integrity, show the safety margin and better appreciate how the turbopumps operate.</div><div class="MsoNormal" style="text-align: justify;"><br />
</div><div class="MsoNormal" style="text-align: justify;">"By anecdotal the pressures, temperatures and flow rates, the power pack test series will evaluate the full range of operating circumstances of the engine components," said Tom Byrd, J-2X engine lead in the SLS Liquid Engines Office at <b>NASA</b>'s Marshall Space Flight Center in Huntsville, Ala. "This will enable us to verify the components' design and validate our analytical models against performance data, as well as ensure structural stability and verify the combustion stability of the gas generator."</div><div class="MsoNormal" style="text-align: justify;"><br />
</div><div class="MsoNormal" style="text-align: justify;">This is the second power pack test series for J-2X. The <b>powerpack </b>1A was tested in 2008 with J-2S engine turbo machinery originally developed for the Apollo Program. Engineers tested these heritage components to obtain data to help them modify the design of the turbomachinery to meet the higher performance requirements of the<b> J-2X engine.</b></div><div class="MsoNormal" style="text-align: justify;"><br />
</div><div class="MsoNormal" style="text-align: justify;">"The test engineers on the A-1 test team are excited and ready to begin another phase of testing which will provide critical data in support of the Space Launch System," said Gary Benton, J-2X engine testing project manager at Stennis.J-2X is being developed for Marshall by Pratt & Whitney Rocketdyne of Canoga Park, Calif.</div></div>stanley princehttp://www.blogger.com/profile/09280760443900821968noreply@blogger.com0tag:blogger.com,1999:blog-1417039068810365781.post-30937698038703499182012-01-19T00:52:00.000-08:002012-01-19T00:52:47.163-08:00Innovative journey 30 team Members open to Station<div dir="ltr" style="text-align: left;" trbidi="on"><!--[if gte mso 9]><xml> <w:WordDocument> <w:View>Normal</w:View> <w:Zoom>0</w:Zoom> <w:TrackMoves/> <w:TrackFormatting/> <w:PunctuationKerning/> <w:ValidateAgainstSchemas/> <w:SaveIfXMLInvalid>false</w:SaveIfXMLInvalid> <w:IgnoreMixedContent>false</w:IgnoreMixedContent> <w:AlwaysShowPlaceholderText>false</w:AlwaysShowPlaceholderText> <w:DoNotPromoteQF/> <w:LidThemeOther>EN-US</w:LidThemeOther> <w:LidThemeAsian>X-NONE</w:LidThemeAsian> <w:LidThemeComplexScript>X-NONE</w:LidThemeComplexScript> <w:Compatibility> <w:BreakWrappedTables/> <w:SnapToGridInCell/> <w:WrapTextWithPunct/> <w:UseAsianBreakRules/> <w:DontGrowAutofit/> <w:SplitPgBreakAndParaMark/> <w:DontVertAlignCellWithSp/> <w:DontBreakConstrainedForcedTables/> <w:DontVertAlignInTxbx/> <w:Word11KerningPairs/> <w:CachedColBalance/> </w:Compatibility> <w:BrowserLevel>MicrosoftInternetExplorer4</w:BrowserLevel> <m:mathPr> <m:mathFont m:val="Cambria Math"/> <m:brkBin m:val="before"/> <m:brkBinSub m:val="--"/> <m:smallFrac m:val="off"/> <m:dispDef/> <m:lMargin m:val="0"/> <m:rMargin m:val="0"/> <m:defJc m:val="centerGroup"/> <m:wrapIndent m:val="1440"/> <m:intLim m:val="subSup"/> <m:naryLim m:val="undOvr"/> </m:mathPr></w:WordDocument> </xml><![endif]--><!--[if gte mso 9]><xml> <w:LatentStyles DefLockedState="false" DefUnhideWhenUsed="true"
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<div class="MsoNormal">The <a href="http://en.wikipedia.org/wiki/Soyuz_TMA-03M"><b>Soyuz TMA-03M spacecraft</b> </a>transport three new Expedition 30 journey engineers’ launch from the Baikonur Cosmodrome in Kazakhstan. </div><div class="MsoNormal"><br />
</div><div class="MsoNormal">Expedition 30 Flight Engineers Don Pettit, Oleg Kononenko and Andre Kuipers launched at 8:16 a.m. EST on Wednesday, Dec. 21 <b>(7:16 p.m. local time)</b> from the Baikonur Cosmodrome in Kazakhstan. The three new global Space Station crew members launch in their Soyuz TMA-03M spacecraft start a two-day trip to the orbiting settlement.</div><div class="MsoNormal"><br />
</div><div class="separator" style="clear: both; text-align: center;"><a href="http://3.bp.blogspot.com/-nc8xAIb7498/TxfZtnNPGAI/AAAAAAAAAcw/YNRWSP1YRPQ/s1600/space+station.jpg" imageanchor="1" style="margin-left: 1em; margin-right: 1em;"><img border="0" src="http://3.bp.blogspot.com/-nc8xAIb7498/TxfZtnNPGAI/AAAAAAAAAcw/YNRWSP1YRPQ/s1600/space+station.jpg" /></a></div><div class="MsoNormal" style="text-align: center;"><br />
</div><div class="MsoNormal"><br />
</div><div class="MsoNormal">They are put to dock to the station's <b>Rassvet </b>mini-research module about 10:22 a.m. on Friday, Dec. 23. Expedition 30 Commander Dan Burbank and Flight Engineers<i><b> Anton Shkaplerov and Anatoly Ivanishin</b></i> will welcome their original crewmates on board the station a little while later at what time they open the hatches about 1 p.m.</div><div class="MsoNormal"><br />
</div><div class="MsoNormal">Pettit, Kononenko and Kuipers are planned to live and work aboard the orbit laboratory until May. They will become member of the Expedition 31 crew under the authority of Kononenko when Burbank, Shkaplerov and Ivanishin undock in their Soyuz TMA-22 spaceship in March.</div></div>stanley princehttp://www.blogger.com/profile/09280760443900821968noreply@blogger.com0tag:blogger.com,1999:blog-1417039068810365781.post-24977885403954799122012-01-09T04:15:00.000-08:002012-01-09T04:15:00.992-08:00NASA To Host Media Teleconference On Probes' Moon Orbit Insertion<div dir="ltr" style="text-align: left;" trbidi="on"><a href="http://www.nasa.gov/topics/aeronautics/index.html"><b>NASA </b></a>will hold a media teleconference at 11 a.m. PST on Wednesday, Dec. 28, to preview twin spacecraft being placed in orbit around the moon on New Year's Eve and New Year's Day. <br />
<br />
NASA's twin lunar Gravity Recovery and Interior Laboratory (<b>GRAIL</b>) probes were launched from Cape Canaveral Air Force Station on Sept. 10, 2011. GRAIL-A is scheduled to arrive in lunar orbit beginning at 1:21 p.m. PST on Saturday, Dec. 31, and GRAIL-B on Sunday, Jan. 1, beginning at 2:05 p.m. PST. After confirmation they are in orbit and operating nominally, the two solar-powered spacecraft will fly in tandem orbits to answer longstanding questions about the moon and give scientists a better understanding of how Earth and other rocky planets in the solar system formed. <br />
<br />
Participants are: <br />
- <i><b>Maria Zuber, principal investigator, Massachusetts Institute of Technology, Cambridge <br />
- David Lehman, project manager, NASA's Jet Propulsion Laboratory (JPL), Pasadena, Calif. </b> </i><br />
To participate, reporters must contact the JPL Media Relations Office at 818-354-5011 by 10:30 a.m. PST on Dec. 28 for the call-in number and passcode. </div>stanley princehttp://www.blogger.com/profile/09280760443900821968noreply@blogger.com0tag:blogger.com,1999:blog-1417039068810365781.post-23404275155237780702011-12-29T02:11:00.000-08:002012-01-04T02:11:54.726-08:00For NASA Webb Telescope Engineers, COCOA this Winter Means Precision Testing<div dir="ltr" style="text-align: left;" trbidi="on"><div class="separator" style="clear: both; text-align: center;"><img border="0" height="320" src="http://1.bp.blogspot.com/-eLblwwNaS7k/TwQlhFPCXLI/AAAAAAAAAcg/OwyE0_uzx8Q/s320/611087main_ITT%2BExelis_COCOA_2011.12.07%2B052-Cleaned-17.jpg" width="225" /></div><br />
<div style="text-align: justify;">Engineers working on NASA's James Webb Space Telescope are bringing out the COCOA this winter, but it's not a warm beverage. Rather, it’s a way to check that the mirrors are perfectly shaped and will work in the frosty environment of space.</div><div style="text-align: justify;"><br />
</div><div style="text-align: justify;">COCOA stands for "Center of Curvature Optical Assembly." Curvature is important in a mirror, just as the convex side mirrors on your car are shaped to give you a wide field of vision behind and beside your car. COCOA tests on the Webb telescope's concave mirror segments are critical because they will tell engineers if all of the mirrors work together to make a telescope that has the correct shape.</div><div style="text-align: justify;"><br />
</div><div style="text-align: justify;">"We need to check that the mirrors are of the right prescription, just like eyeglasses, so the images from our telescope are not blurry," said Lee Feinberg, Webb telescope Optical Telescope Manager at NASA's Goddard Space Flight Center, Greenbelt, Md.</div><div style="text-align: justify;"><br />
</div><div style="text-align: justify;">The Webb telescope has 21 mirrors, with 18 of these being six-sided segments working together as one large 21.3-foot (6.5-meter) mirror. Every individual mirror has been previously tested to confirm it has the correct shape, but testing them all together as an assembled telescope with COCOA ensures that the telescope as a whole works correctly.</div><div style="text-align: justify;"><br />
</div><div style="text-align: justify;">The COCOA is part of NASA's vacuum cryo equipment that will be used at NASA's Johnson Space Center in Houston to test the performance of the mirrors at operating temperatures. That's important because COCOA tells engineers if the full 18 segment mirror is functioning correctly in "operating temperatures" of 40 degrees Kelvin (-233 Celsius, or -387.4 Fahrenheit) prior to final assembly of the observatory before launch.</div><div style="text-align: justify;"><br />
</div><div style="text-align: justify;">COCOA was built by ITT Exelis of Rochester, N.Y., with subcontractor Micro Instruments in Rochester, N.Y. ITT Exelis and Micro Instruments engineers are assembling the large Center of Curvature test system.</div><div style="text-align: justify;"><br />
</div><div style="text-align: justify;">The Webb telescope is the world’s next-generation space observatory and successor to the Hubble Space Telescope. The most powerful space telescope ever built, the Webb telescope will provide images of the first galaxies ever formed, and explore planets around distant stars. It is a joint project of NASA, the European Space Agency and the Canadian Space Agency.</div><br />
For more information visit <a href="http://www.nasa.gov/topics/technology/features/webb-cocoa.html" rel="nofollow">http://www.nasa.gov/topics/technology/features/webb-cocoa.html</a></div>stanley princehttp://www.blogger.com/profile/09280760443900821968noreply@blogger.com0tag:blogger.com,1999:blog-1417039068810365781.post-4169079654459608002011-12-29T01:25:00.000-08:002012-01-04T01:25:50.248-08:00NASA's Cassini Delivers Holiday Treats From Saturn<div dir="ltr" style="text-align: left;" trbidi="on"><div class="separator" style="clear: both; text-align: center;"><img border="0" height="257" src="http://4.bp.blogspot.com/-R2c8N47LrTk/TwQa5_OmmgI/AAAAAAAAAbw/stAyRU06zm8/s400/612678main_pia14910-673-13.jpg" width="400" /></div><br />
<div style="text-align: justify;">No team of reindeer, but radio signals flying clear across the solar system from NASA's Cassini spacecraft have delivered a holiday package of glorious images. The pictures, from Cassini's imaging team, show Saturn's largest, most colorful ornament, Titan, and other icy baubles in orbit around this splendid planet. The release includes images of satellite conjunctions in which one moon passes in front of or behind another. Cassini scientists regularly make these observations to study the ever-changing orbits of the planet's moons. But even in these routine images, the Saturnian system shines. A few of Saturn's stark, airless, icy moons appear to dangle next to the orange orb of Titan, the only moon in the solar system with a substantial atmosphere. Titan's atmosphere is of great interest because of its similarities to the atmosphere believed to exist long ago on the early Earth.</div><div style="text-align: justify;"><br />
</div><div style="text-align: justify;">The images are online at: http://www.nasa.gov/cassini, http://saturn.jpl.nasa.gov and http://ciclops.org .</div><div style="text-align: justify;"><br />
</div><div style="text-align: justify;">While it may be wintry in Earth's northern hemisphere, it is currently northern spring in the Saturnian system and it will remain so for several Earth years. Current plans to extend the Cassini mission through 2017 will supply a continued bounty of scientifically rewarding and majestic views of Saturn and its moons and rings, as spectators are treated to the passage of northern spring and the arrival of summer in May 2017.</div><div style="text-align: justify;"><br />
</div><div style="text-align: justify;">"As another year traveling this magnificent sector of our solar system draws to a close, all of us on Cassini wish all of you a very happy and peaceful holiday season, " said Carolyn Porco, Cassini imaging team lead at the Space Science Institute, Boulder, Colo.</div><div style="text-align: justify;"><br />
</div><div style="text-align: justify;">More information about Cassini mission is online at http://www.nasa.gov/cassini and http://saturn.jpl.nasa.gov .</div><div style="text-align: justify;"><br />
</div><div style="text-align: justify;">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. 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 in Boulder, Colo.</div><br />
For more information visit <a href="http://www.nasa.gov/mission_pages/cassini/whycassini/cassini20111222.html" rel="nofollow">http://www.nasa.gov/mission_pages/cassini/whycassini/cassini20111222.html</a></div>stanley princehttp://www.blogger.com/profile/09280760443900821968noreply@blogger.com0tag:blogger.com,1999:blog-1417039068810365781.post-57060038335133997622011-12-28T04:01:00.000-08:002011-12-28T04:01:16.074-08:00Party dresses to make you brighter in parties<div dir="ltr" style="text-align: left;" trbidi="on"><div dir="ltr" style="text-align: left;" trbidi="on">Every woman likes to be present at festivities where she can completely explain her loveliness to others. And in parties ladies can be dressed in the majority good-looking dresses which are not good to be dressed in on other events. But several women experience hard to get appropriate party dresses to purchase, because such beautiful wears particularly necessitate women to be suspicious when wearing them for fear that the conflicting effect may be arrived.<br />
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</div><div class="separator" style="clear: both; text-align: center;"><a href="http://4.bp.blogspot.com/-jPVCpnS1xDU/TvsEpqEgjLI/AAAAAAAAAbY/KYQElJq8Uj8/s1600/3.jpg" imageanchor="1" style="margin-left: 1em; margin-right: 1em;"><img border="0" height="300" src="http://4.bp.blogspot.com/-jPVCpnS1xDU/TvsEpqEgjLI/AAAAAAAAAbY/KYQElJq8Uj8/s320/3.jpg" width="140" /></a></div><br />
Some dresses for women may be pleasant but may be not appropriate for a woman’s skin tone. Some others may be good-looking to wear but may be out of the fashion. Now <a href="http://www.idressonline.com/" style="color: orange;">evening gowns</a> are very common and several women adore them. They give enormous materials of ranges for women to prefer anything they like. Here are some instructions about how to prefer a dress for party.<br />
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<div class="separator" style="clear: both; text-align: center;"><a href="http://4.bp.blogspot.com/-VYqjvyLEMiU/TvsEw8ADQ4I/AAAAAAAAAbk/UqaXSye4OAQ/s1600/33.jpg" imageanchor="1" style="margin-left: 1em; margin-right: 1em;"><img border="0" height="300" src="http://4.bp.blogspot.com/-VYqjvyLEMiU/TvsEw8ADQ4I/AAAAAAAAAbk/UqaXSye4OAQ/s320/33.jpg" width="232" /></a></div><br />
When selecting party dresses, women must fully think their own skin tone. Women must select the dresses which can make their skin tones appear brighter not darker. Pick the color of the dresses which are darker than women’s skin tones, which will accomplish a fine result and make the skin appear brighter.<br />
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</div>stanley princehttp://www.blogger.com/profile/09280760443900821968noreply@blogger.com0tag:blogger.com,1999:blog-1417039068810365781.post-9343544220964929062011-12-19T02:05:00.000-08:002012-01-04T02:06:40.298-08:00NASA Presents Software of the Year Award<div dir="ltr" style="text-align: left;" trbidi="on"><div class="separator" style="clear: both; text-align: center;"><img border="0" height="210" src="http://1.bp.blogspot.com/-rmclhd23k5o/TwQkXKD2fgI/AAAAAAAAAcU/d8jjnVNUNKg/s640/609147main_pia15190-673-16.jpg" width="640" /></div><br />
<div style="text-align: justify;">Autonomous Exploration for Gathering Increased Science (AEGIS), novel autonomy software that has been operating on the Mars Exploration Rover Opportunity since December 2009, is NASA's 2011 Software of the Year recipient.</div><div style="text-align: justify;"><br />
</div><div style="text-align: justify;">The AEGIS software, developed by NASA's Jet Propulsion Laboratory in Pasadena, Calif., autonomously directs Opportunity's cameras to interesting science targets. AEGIS was developed to enhance the usual targeting process involving scientists on the ground, which can require the rover to stay in the same place for a day or more while data are transmitted to Earth and targets are selected from preliminary images.</div><div style="text-align: justify;"><br />
</div><div style="text-align: justify;">With AEGIS, the rover software analyzes images onboard, detects and prioritizes science targets in those images, and autonomously obtains novel, high-quality science data of the selected targets, within 45 minutes, with no communication back to Earth required. AEGIS chooses science targets based on pre-specified criteria set by the mission science team.</div><div style="text-align: justify;"><br />
</div><div style="text-align: justify;">AEGIS can be used as soon as the rover reaches a new area and is especially beneficial during and after long drives. It enables high-quality data to be collected more often and in a significantly reduced time frame. The incorporation of AEGIS in the Mars Science Laboratory flight software is in progress, and it is also being considered for future NASA missions.</div><div style="text-align: justify;"><br />
</div><div style="text-align: justify;">The AEGIS capability was developed as part of a larger autonomous science framework called OASIS (short for Onboard Autonomous Science Investigation System), which is designed to allow a rover to identify and react to serendipitous science opportunities. The AEGIS system takes advantage of the OASIS ability to detect and characterize interesting terrain features in rover images. This technology was created with assistance from NASA's Mars Exploration Rover Project and with funding from the New Millennium Program, the Mars Technology Program, the JPL Research and Technology Development Program, the JPL Interplanetary Network Development Program and the Intelligent Systems Program.</div><br />
For more information visit <a href="http://www.nasa.gov/topics/technology/features/tech20111208.html" rel="nofollow">http://www.nasa.gov/topics/technology/features/tech20111208.html</a></div>stanley princehttp://www.blogger.com/profile/09280760443900821968noreply@blogger.com0tag:blogger.com,1999:blog-1417039068810365781.post-83691423310825052412011-12-19T02:01:00.000-08:002012-01-04T02:02:34.376-08:00NASA Tests New Smart Card Access to Google Apps<div dir="ltr" style="text-align: left;" trbidi="on"><div class="separator" style="clear: both; text-align: center;"><img border="0" height="300" src="http://1.bp.blogspot.com/-ZrHCOqq9n4I/TwQjebCFKmI/AAAAAAAAAcI/k1nFu32OUkw/s400/609107main_badge_blind226-15.jpg" width="400" /></div><br />
NASA recently began a pilot using Google Apps, a suite of applications that brings services such as Gmail, Google Docs and other products together to help workers in today's business environment. NASA IT Labs, a part of the Office of the Chief Information Officer (CIO), sponsored the pilot to meet the growing demand from workers to access resources on any device.<br />
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About 600 IT staff from 11 NASA centers and facilities are participating in the pilot, which offers cost savings by managing user's identities, credentials and access via cloud computing using on-demand software. Cloud computing refers to resources and applications that are available on the Internet from nearly any Internet-connected device. No sensitive NASA data is being placed in the cloud.<br />
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Under the pilot, NASA users can connect to Google Apps for Government using an existing NASA work ID, which also functions as a smart card in the card reader of compatible computers. The card was created as a common identification standard for federal employees and contractors to increase security and reduce opportunities for identify fraud.<br />
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The pilot complies with the Federal Information Security Management Act of 2002, which is designed to protect the nation's critical information infrastructure. Because no new ID or credential is needed, NASA complies with the law and workers can access secure materials from any smart device.<br />
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NASA also accepts and electronically verifies personal identity verification (PIV) credentials issued by other federal agencies through a credential registration process. With this capability, any authorized federal PIV card, which includes the DoD Common Access Card, may be used today for authentication to the Google Apps for Government NASA site.<br />
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For more information visit <a href="http://www.nasa.gov/topics/technology/features/google_apps.html" rel="nofollow">http://www.nasa.gov/topics/technology/features/google_apps.html</a></div>stanley princehttp://www.blogger.com/profile/09280760443900821968noreply@blogger.com0tag:blogger.com,1999:blog-1417039068810365781.post-51290710755876257742011-12-16T01:30:00.000-08:002012-01-04T01:30:39.139-08:00Curiosity and the Solar Storm<div dir="ltr" style="text-align: left;" trbidi="on"><div class="separator" style="clear: both; text-align: center;"><img border="0" height="300" src="http://1.bp.blogspot.com/-ppkT1aQj5iE/TwQcDhZER-I/AAAAAAAAAb8/WlvuRYyf2I0/s400/611113main_msl-launch-14.jpg" width="400" /></div><br />
On Nov. 26, 2011, Curiosity blasted off from Cape Canaveral atop an Atlas 5 rocket. Riding a plume of fire through the blue Florida sky, the car-sized rover began a nine month journey to search for signs of life Mars.<br />
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Meanwhile, 93 million miles away, a second lesser-noticed Mars launch was underway. Around the time that Curiosity's rocket was breaking the bonds of Earth, a filament of magnetism erupted from the sun, hurling a billion-ton cloud of plasma (a coronal mass ejection or CME) toward the Red Planet.<br />
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There was no danger of a collision -- Mars rover vs. solar storm. Racing forward at 2 million mph, the plasma cloud outpaced Curiosity's rocket by a wide margin.<br />
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Next time could be different, however. With solar activity on the upswing (Solar Max is expected in 2012-2013) it's only a matter of time before a CME engulfs the Mars-bound rover.<br />
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That suits some researchers just fine. As Don Hassler of the Southwest Research Institute (SWRI) in Boulder, Colorado, explains, "We look forward to such encounters because Curiosity is equipped to study solar storms."<br />
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Hassler is the principal investigator for Curiosity's Radiation Assessment Detector --"RAD" for short. The instrument, developed at SWRI and Christian Albrechts University in Kiel, Germany, counts cosmic rays, neutrons, protons and other particles over a wide range of energies. Tucked into the left front corner of the rover, RAD is about the size of a coffee can and weighs only three pounds, but has capabilities of Earth-bound instruments nearly 10 times its size.<br />
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Encounters with CMEs pose little danger to Curiosity. By the time a CME reaches the Earth-Mars expanse, it is spread so thin that it cannot truly buffet the spacecraft. Nevertheless, RAD can sense what happens as the CME passes by.<br />
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"RAD will be able to detect energetic particles accelerated by shock waves in some CMEs," says Arik Posner of NASA's Heliophysics Division in Washington DC. "This could give us new insights into the inner physics of these giant clouds."<br />
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There's more to this, however, than pure heliophysics. Future human astronauts will directly benefit from RAD's measurements during the cruise phase.<br />
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"Curiosity is nestled inside its spacecraft, just like a real astronaut would be," notes Frank Cucinotta, Chief Scientist for NASA's Space Radiation Program at the Johnson Space Center. "RAD will give us an idea of the kind of radiation a human can expect to absorb during a similar trip to Mars."<br />
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Of particular interest are secondary particles. Galactic cosmic rays and solar energetic particles hit the walls of the spacecraft, creating an inward spray of even more biologically dangerous neutrons and atomic nuclei. RAD will analyze the spray from the only realistic place to make such measurements—inside the spaceship.<br />
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In this way, "RAD is a bridge between the science and exploration sides of NASA," says Hassler. "The two objectives are equally exciting."<br />
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RAD was activated on Dec. 6, 2011. Of the rover's ten science instruments, it will be the only one active during the cruise to Mars. Daily transmissions to Earth will let Hassler and colleagues monitor what's going on "out there."<br />
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"We're very excited about the possibility of more solar storms," he adds.<br />
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As important as RAD’s cruise phase measurements are, the instrument’s primary mission doesn’t really begin until it lands on the Red Planet.<br />
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Mars has a very thin atmosphere and no global magnetic field to protect it from space radiation. Energetic particles reaching ground level might be dangerous to life--both future human astronauts and extant Martian microbes. RAD will find out how much shielding human explorers need on the surface of Mars. RAD will also help researchers estimate how far below ground a microbe might have to go to reach a radiation "safe zone."<br />
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For more information visit <a href="http://www.nasa.gov/mission_pages/sunearth/news/curiosity-cme.html" rel="nofollow">http://www.nasa.gov/mission_pages/sunearth/news/curiosity-cme.html</a></div>stanley princehttp://www.blogger.com/profile/09280760443900821968noreply@blogger.com0tag:blogger.com,1999:blog-1417039068810365781.post-58529806724207146662011-12-14T23:38:00.000-08:002011-12-14T23:41:13.174-08:00NASA Mars-Bound Rover Begins Research in Space<div dir="ltr" style="text-align: left;" trbidi="on"><div class="separator" style="clear: both; text-align: center;"><img border="0" height="300" src="http://4.bp.blogspot.com/-5QjtlTYmxx8/Tumj43AdgiI/AAAAAAAAAbM/yH3dyN0hSng/s400/main2_pia14831-43_946-710.jpg" width="400" /></div><br />
<div style="text-align: justify;">NASA's car-sized Curiosity rover has begun monitoring space radiation during its 8-month trip from Earth to Mars. The research will aid in planning for future human missions to the Red Planet.</div><div style="text-align: justify;"><br />
</div><div style="text-align: justify;">Curiosity launched on Nov. 26 from Cape Canaveral, Fla., aboard the Mars Science Laboratory. The rover carries an instrument called the Radiation Assessment Detector (RAD) that monitors high-energy atomic and subatomic particles from the sun, distant supernovas and other sources.</div><div style="text-align: justify;"><br />
</div><div style="text-align: justify;">These particles constitute radiation that could be harmful to any microbes or astronauts in space or on Mars. The rover also will monitor radiation on the surface of Mars after its August 2012 landing.</div><div style="text-align: justify;"><br />
</div><div style="text-align: justify;">"RAD is serving as a proxy for an astronaut inside a spacecraft on the way to Mars," said Don Hassler, RAD's principal investigator from the Southwest Research Institute in Boulder, Colo. "The instrument is deep inside the spacecraft, the way an astronaut would be. Understanding the effects of the spacecraft on the radiation field will be valuable in designing craft for astronauts to travel to Mars."</div><div style="text-align: justify;"><br />
</div><div style="text-align: justify;">Previous monitoring of energetic-particle radiation in space has used instruments at or near the surface of various spacecraft. The RAD instrument is on the rover inside the spacecraft and shielded by other components of Mars Science Laboratory, including the aeroshell that will protect the rover during descent through the upper atmosphere of Mars.</div><div style="text-align: justify;"><br />
</div><div style="text-align: justify;">Spacecraft structures, while providing shielding, also can contribute to secondary particles generated when high-energy particles strike the spacecraft. In some circumstances, secondary particles could be more hazardous than primary ones.</div><div style="text-align: justify;"><br />
</div><div style="text-align: justify;">These first measurements mark the start of the science return from a mission that will use 10 instruments on Curiosity to assess whether Mars' Gale Crater could be or has been favorable for microbial life.</div><div style="text-align: justify;"><br />
</div><div style="text-align: justify;">"While Curiosity will not look for signs of life on Mars, what it might find could be a game-changer about the origin and evolution of life on Earth and elsewhere in the universe," said Doug McCuistion, director of the Mars Exploration Program at NASA Headquarters in Washington. "One thing is certain: The rover's discoveries will provide critical data that will impact human and robotic planning and research for decades."</div><div style="text-align: justify;"><br />
</div><div style="text-align: justify;">As of 9 a.m. PST (noon EST) on Dec. 14, the spacecraft will have traveled 31.9 million miles (51.3 million kilometers) of its 352-million-mile (567-million-kilometer) flight to Mars. The first trajectory correction maneuver during the trip is being planned for mid-January.</div><div style="text-align: justify;"><br />
</div><div style="text-align: justify;">Southwest Research Institute, together with Christian Albrechts University in Kiel, Germany, built RAD with funding from the Human Exploration and Operations Mission Directorate, NASA Headquarters, Washington, and Germany's national aerospace research center, Deutsches Zentrum für Luft- und Raumfahrt.</div><br />
For more information visit <a href="http://www.nasa.gov/mission_pages/msl/news/msl20111213.html" rel="nofollow">http://www.nasa.gov/mission_pages/msl/news/msl20111213.html</a></div>stanley princehttp://www.blogger.com/profile/09280760443900821968noreply@blogger.com0