Posted on by Fraser Cain

New Class of Planets Found

Astronomers announced today the first discovery of a new class of planets beyond our solar system about 10 to 20 times the size of Earth – far smaller than any previously detected. The planets make up a new class of Neptune-sized extrasolar planets.

In addition, one of the new planets joins three others around the nearby star 55 Cancri to form the first known four-planet system.

The discoveries consist of two new planets. They were discovered by the world renowned planet-hunting team of Drs. Paul Butler and Geoffrey Marcy of the Carnegie Institute of Washington and University of California, Berkeley, respectively; and Barbara McArthur of the University of Texas, Austin. Both findings were peer- reviewed and accepted for future publication in the Astrophysical Journal. NASA and the National Science Foundation funded the research.

“NASA, along with our partner NSF, is extremely proud of this significant planetary discovery,” said Al Diaz, Associate Administrator of NASA’s Science Mission Directorate. “The outcome of the tremendous work of the project scientists is a shining example of the value of space exploration.”

“These Neptune-sized planets prove that Jupiter-sized, gas giants aren’t the only planets out there,” Marcy said. Butler added, “We are beginning to see smaller and smaller planets. Earth-like planets are the next destination.”

Future NASA planet-hunting missions, including Kepler, the Space Interferometry Mission and the Terrestrial Planet Finder, will seek such Earth-like planets. Nearly 140 extrasolar planets have been discovered.

Both of the new planets stick very close to their parent stars, whipping around them in a matter of days. The first planet, discovered by Marcy and Butler, circles a small star called Gliese 436 about every two-and-one-half days at just a small fraction of the distance between Earth and the Sun, or 4.1 million kilometers (2.6 million miles). This planet is only the second known to orbit an M dwarf, a type of low-mass star four-tenths the size of our own sun. Gliese 436 is located in our galactic backyard, 30 light-years away in the constellation Leo.

The second planet, found by McArthur, speeds around 55 Cancri in just under three days, also at a fraction of the distance between Earth and the sun, at approximately 5.6 million kilometers (3.5 million miles). Three larger planets also revolve around the star every 15, 44 and 4,520 days, respectively. Marcy and Butler discovered the outermost of these in 2002. It is still the only known Jupiter-like gas giant to reside as far away from its star as our own Jupiter. The 55 Cancri is about 5 billion years old, a bit lighter than the sun, and is located 41 light-years away in the constellation Cancer. “55 Cancri is a premier laboratory for the study of planetary system formation and evolution,” McArthur said.

Because the new planets are smaller than Jupiter, it is possible they are made of rock, or rock and ice, rather than gas. According to the scientists, the planets may have, like Earth, formed through gradual accumulation of rocky bodies. “A planet of Neptune’s size may not have enough mass to hold onto gas, but at this point we don’t know,” Butler said.

Both discoveries were made using the “radial velocity” technique, in which a planet’s gravitational tug is detected by the wobble it produces in the parent star. Butler, Marcy and collaborators, including Dr. Deborah Fischer of San Francisco State University and Dr. Steven Vogt of the University of California, Santa Cruz, discovered their “Neptune” after careful observation of 950 nearby stars with the W.M. Keck Observatory in Mauna Kea, Hawaii. They were able to spot such a relatively small planet, because the star it tugs on is small and more susceptible to wobbling.

McArthur and collaborators Drs. Michael Endl, William Cochran and Fritz Benedict of the University of Texas discovered their “Neptune” after obtaining over 100 observations of 55 Cancri from the Hobby- Eberly Telescope at McDonald Observatory in West Texas. Combining this data with past data from Marcy, Fischer and Butler from the Lick Observatory in California, and archival data from NASA’s Hubble Space Telescope, the team was able to model the orbit of 55 Cancri’s outer planet. This, in turn, allowed them to clearly see the orbits of the other three inner planets, including the new Neptune-sized one.

Original Source: NASA News Release

Posted on by Fraser Cain

Station Will Get a Better View

Development phase completion of the European-built observation module, or “cupola”, for the International Space Station will be marked by a ceremony at the Alenia Spazio facility in Turin, Italy on Monday 6 September.

The cupola, currently scheduled for launch in January 2009, is an observation and control tower for the ISS, with windows that will provide a panoramic view for observing and guiding operations on the outside of the station.

The pressurised module will accommodate command and control workstations and other hardware, enabling crewmembers to control the station?s robotic arm – for attaching and assembling various station elements – and to communicate with other crewmembers in other parts of the station or outside during spacewalk activities. The cupola will also be used for observational applications in the areas of Earth observation and space science.

The cupola project is the outcome of a bilateral barter agreement between the European Space Agency and NASA, under which ESA is providing the cupola for the ISS in exchange for Shuttle transportation of European equipment and experiments to the station.

The completion of the cupola marks the end of the development phase of the project, which began with the signing of the cupola contract between ESA and Alenia Spazio on 8 February 1999. Under the contract, Alenia Spazio acted as prime contractor for production, responsible for coordinating six other firms: CASA (Spain), APCO (Switzerland), SAAB Ericsson and Lindholmen Development (Sweden), EADS Space Transportation (Germany) and Verhaert (Belgium).

The 1.8-tonne cupola is now ready to be transported to the Kennedy Space Center at Cape Canaveral, Florida. There, it will go through a final set of checks before being put into storage for four years, at the end of which it will be prepared for launch.

Original Source: ESA News Release

Posted on by Fraser Cain

X-43 Receives Guinness World Record

Guinness World Records has recognized the world speed record set by NASA’s hypersonic X-43A aircraft in an experimental flight over the Pacific Ocean earlier this year. The unpiloted, 12- foot-long aircraft achieved Mach 6.83 — almost seven times the speed of sound — or nearly 5,000 mph, while its supersonic-combustion ramjet (scramjet) engine propelled the craft for 11 seconds during the flight on March 27.

The accomplishment will be included in the 2006 Guinness World Records book, set for release this time next year, as follows:

“On 27 March 2004, NASA’s unmanned Hyper-X (X-43A) airplane reached Mach 6.83, almost seven times the speed of sound. The X-43A was boosted to an altitude of 29,000 m (95,000 ft) by a Pegasus rocket launched from beneath a B52-B aircraft. The revolutionary ‘scramjet’ aircraft then burned its engine for around 11 seconds during flight over the Pacific Ocean.”

If NASA researchers have their way, the record won’t stand long. The final flight in the Hyper-X program is scheduled to take place in October, when another X-43A aircraft will attempt to fly at Mach 10 — ten times the speed of sound — or 7,200 mph.

The flight was part of NASA’s Hyper-X program, designed to demonstrate advanced high-speed propulsion system concepts to overcome one of the greatest aeronautical research challenges – air-breathing hypersonic flight. The advantage of air-breathing flight is that the vehicle — whether it is aircraft or spacecraft ?scoops the air its engines need from the atmosphere rather than carrying heavy, bulky tanks, as rockets do.

The challenge is to introduce fuel, ignite it and produce positive thrust while highly compressed air rushes through the engine in mere milliseconds — roughly analogous to lighting a match and keeping it burning in a hurricane-force wind.

Compared to rocket-powered vehicles like the Space Shuttle, scramjets promise more airplane-like operations for increased affordability, flexibility and safety for ultra high-speed flights within the atmosphere and into Earth orbit.

The X-43A flight easily set a world speed record for an air-breathing engine aircraft. The previous known record was held by a ramjet-powered missile, which achieved slightly more than Mach 5. A ramjet operates by subsonic combustion of fuel in a stream of air compressed by the forward speed of the aircraft itself, as opposed to a normal jet engine, in which the compressor section (the fan blades) compresses the air. A scramjet (supersonic-combustion ramjet) is a ramjet engine in which the airflow through the whole engine remains supersonic.

The highest speed attained by a rocket-powered airplane, NASA’s X-15 aircraft, was Mach 6.7.The fastest air-breathing, manned vehicle, the SR-71, achieved slightly more than Mach 3.2. The X-43A more than doubled the top speed of the jet-powered SR-71.

Guinness World Records? science editor David Hawksett has already expressed a n interest in attending the fall flight.

“Operating an atmospheric vehicle at almost Mach 7 is impressive enough, but to be able to use oxygen from the air, instead of a fuel tank, as it screams into the engine intakes at 5,000 mph is a mind-boggling technical achievement. It?s wonderful to see scramjet technology finally begin to take off,” said Hawksett.

The Hyper-X program is conducted by NASA’s Aeronautics Research Mission Directorate with the NASA Langley Research Center, Hampton, Va., as lead center with responsibility for hypersonic technology development and the NASA Dryden Flight Research Center, Edwards, Calif., responsible for flight research and testing.

Guinness World Records issued a certificate to NASA documenting the X-43A accomplishment, and will feature the story on its web site: http://www.guinnessworldrecords.com/

For more information on NASA’s Aeronautics Research Mission Directorate programs, including Hyper-X, on the Internet, visit: http://www.aeronautics.nasa.gov/

Original Source: NASA News Release

Here’s an article about the biggest airplane in the world.

Posted on by Fraser Cain

Plankton’s Glow Seen from Space

For the first time, scientists may now detect a phytoplankton bloom in its early stages by looking at its red “glow” under sunlight, due to the unique data from two NASA satellites. According to a study conducted in the Gulf of Mexico, this phenomenon can forewarn fishermen and swimmers about developing cases of red tides that occur within plumes of dark-colored runoff from river and wetlands, sometimes causing “black water” events.

Dark-colored river runoff includes nitrogen and phosphorus, which are used as fertilizers in agriculture. These nutrients cause blooms of marine algae called phytoplankton. During extremely large phytoplankton blooms where the algae is so concentrated the water may appear black, some phytoplankton die, sink to the ocean bottom and are eaten by bacteria. The bacteria consume the algae and deplete oxygen from the water that leads to fish kills.

Chuanmin Hu and Frank Muller-Karger, oceanographers at the College of Marine Science of University of South Florida, St. Petersburg, Fla., used fluorescence data from NASA’s Moderate Resolution Imaging Spectroradiometer (MODIS) instruments aboard both NASA’s Terra and Aqua satellites. MODIS detects the glow or phytoplankton fluorescence, from the plant’s chlorophyll. The human eye cannot detect the red fluorescence.

The ability to detect glowing areas of water helps researchers identify whether phytoplankton are present in large dark water patches that form off the coast of Florida. Without these data, it is impossible to differentiate phytoplankton blooms from plumes of dark river runoff that contain few individual phytoplankton cells.

Because colored dissolved organic matter that originates in rivers can absorb similar amounts of blue and green color signals as plants do, traditional satellites that simply measure ocean color cannot distinguish phytoplankton blooms within such patches.

Although satellites cannot directly measure nutrients in lakes, rivers, wetlands and oceans, remote sensing technology measure the quantities of plankton. Scientists can then calculate how much nutrient might be needed to grow those amounts of plankton.

Hu and others used this technique to study the nature and origin of a dark plume event in the fall of 2003 near Charlotte Harbor, off the south Florida coast. Moderate concentrations of one of Florida’s red tide species, were found from water samples.

“Our study traces the black water patches near the Florida Keys to some 200 kilometers (124 miles) away upstream,” said Hu. “These results suggest that the delicate Florida Keys ecosystem is connected to what happens on land and in two remote rivers, the Peace and Caloosahatchee, as they drain into the ocean. Extreme climate conditions, such as abnormally high rainfall in spring and summer 2003, may accelerate such connections,” he added.

These findings are based on scientific analyses of several things. Data used include satellite ocean color from MODIS and Sea-viewing Wide Field-of-view Sensor (SeaWiFS), and wind data from NASA’s QuikSCAT satellite. U.S. Geological Survey, National Oceanic and Atmospheric Administration (NOAA), Florida?s Fish and Wildlife Research Institute, and other organizations provided rain, river discharge, and field survey information.

By knowing which way the winds blow and the currents flow, Hu and colleagues can predict where black water may move.

Red tides occur every year off Florida and are known to cause fish kills, coral stress and mortality, and skin and respiratory problems in humans. Previous studies show that prolonged “black water” patches cause water quality degradation and may cause coral death. The use of remote sensing satellites provides effective means for monitoring and predicting such events.

The link between coastal runoff and black water events is an example of how land and ocean ecosystems are linked together. “Coastal and land managers over large areas need to work together, to alleviate more black water events from taking place in the future,” said Muller-Karger.

This study appeared in a recent issue of the American Geophysical Union’s Geophysical Research Letters. Coauthors of the article include Gabriel Vargo and Merrie Beth Neely from University of South Florida and Elizabeth Johns from NOAA’s Atlantic Oceanographic and Meteorological Laboratory.

NASA’s Science Directorate works to improve the lives of all humans through the exploration and study of Earth’s system, the solar system and the Universe.

Original Source: NASA News Release

Posted on by Fraser Cain

What Impact Would Set the World on Fire?

Image credit: Josh O?Conner and wildlandfire.com
Scientists conclude that, 65 million years ago, a 10-kilometer-wide asteroid or comet slammed into what is now the Yucat?n peninsula, excavating the Chicxulub impact crater and setting into motion a chain of catastrophic events thought to precipitate the extinction of the dinosaurs and 75 percent of animal and plant life that existed in the late Cretaceous period.

“The impact of an asteroid or comet several kilometers across heaps environmental insult after insult on the world,” said Dr. Daniel Durda, a senior research scientist at Southwest Research Institute? (SwRI?). “One aspect of the devastation wrought by large impacts is the potential for global wildfires ignited by material ejected from the crater reentering the atmosphere in the hours after the impact.”

Large impacts can blast thousands of cubic kilometers of vaporized impactor and target sediments into the atmosphere and above, expanding into space and enveloping the entire planet. These high-energy, vapor-rich materials reenter the atmosphere and heat up air temperatures to the point that vegetation on the ground below can spontaneously burst into flame.

“In 2002, we investigated the Chicxulub impact event to examine the extent and distribution of fires it caused,” said Durda. This cosmic collision carved out a crater some 40 kilometers (25 miles) deep and 180 kilometers (112 miles) across at the boundary between two geologic periods, the Cretaceous, when the dinosaurs ruled the planet, and the Tertiary, when mammals took supremacy.

“We noted that fires appeared to be global, covering multiple continents, but did not cover the entire Earth,” Durda continued. “That suggested to us that the Chicxulub impact was probably near the threshold size event necessary for igniting global fires, and prompted us to ask ‘What scale of impact is necessary for igniting widespread fires?'”

In a new study, Durda and Dr. David Kring, an associate professor at the University of Arizona Lunar and Planetary Laboratory, published a theory for the ignition threshold for impact-generated fires in the August 20, 2004, issue of the Journal of Geophysical Research. Their research indicates that impacts resulting in craters at least 85 kilometers wide can produce continental-scale fires, while impact craters more than 135 kilometers wide are needed to cause global-scale fires.

To calculate the threshold size impact required for global ignition of various types of vegetation, Durda and Kring used two separate, but linked, numerical codes to calculate the global distribution of debris reentering the atmosphere and the kinetic energy deposited in the atmosphere by the material. The distribution of fires depends on projectile trajectories, the position of the impact relative to the geographic distribution of forested continents and the mass of crater and projectile debris ejected into the atmosphere.

They also examined the threshold temperatures and durations required to spontaneously ignite green wood, to ignite wood in the presence of an ignition source (such as lightning, which would be prevalent in the dust-laden energetic skies following an impact event) and to ignite rotting wood, leaves and other common forest litter.

“The Chicxulub impact event may have been the only known impact event to have caused wildfires around the globe,” Kring noted. “The Manicouagan (Canada) and Popigai (Russia) impact events, however, may have caused continental-scale fires. The Manicouagan impact occurred in the late Triassic, and the Popigai impact event occurred in the late Eocene, but neither has been firmly linked yet to the mass extinction events that occurred at those times.”

Kring is currently at the International Geological Congress in Florence, Italy, giving a keynote address on the Chicxulub impact event and its relationship to the mass extinctions at the Cretaceous-Tertiary boundary period. Durda is available for comment at the SwRI offices in Boulder, Colo.

Original Source: SWRI News Release

Posted on by Fraser Cain

Mars Express View of Eos Chasma

This image, taken by the High Resolution Stereo Camera (HRSC) on board ESA’s Mars Express spacecraft, shows the southern part of Valles Marineris, called Eos Chasma.

The images was taken during orbit 533 in June 2004, and is centred at Mars longitude 322? East and latitude 11? South. The image resolution is approximately 80 metres per pixel.

Between surrounding plains and the smooth valley floor, a height difference of about 5000 metres has been measured.

The plain to the south, above Eos Chasma, is covered by several impact craters with diameters of around 20 kilometres and drainage channels.

To the east on this plain, isolated regions with cracked surfaces become more prominent. The direction of flow of the drainage channels in this area of the plain is ambiguous, as the channels to the north-east drain towards the south-east, and those in the south-west normally flow to the north-west.

The northern part of Eos Chasma?s valley floor is a rough area with angular hills reaching almost 1000 metres. In contrast, the southern part reveals a smooth topography with distinct flow structures.

In some areas of the southern slope, at least two terrace levels can be observed. Some haze in the valley hints at the presence of aerosols (airborne microscopic dust or liquid droplets).

Original Source: ESA News Release

Posted on by Fraser Cain

Wallpaper: Hurricane Frances

This photo of Hurricane Frances was taken by Astronaut Mike Fincke aboard the International Space Station as he flew 230 statute miles above the storm at about 9 a.m. CDT Friday, Aug. 27, 2004. At the time, Frances was located 820 miles east of the Lesser Antilles in the Atlantic Ocean, moving west-northwest at 10 miles per hour, with maximum sustained winds of 105 miles per hour. Fincke, the NASA ISS Science Officer and Flight Engineer, and Expedition 9 Commander Gennady Padalka are in the fifth month of a six-month flight aboard the Station.

Original Source: NASA News Release

Posted on by Fraser Cain

Satellites Track Inland Water Levels From Space

A few NASA satellites designed to study heights of Earth’s ocean surfaces are now also coming in handy for tracking water levels of inland lakes and reservoirs.

When analysts at the United States Department of Agriculture (USDA) Foreign Agriculture Service (FAS) learned that NASA satellites could be used for measuring lake water heights, they saw a chance to get vital information for managing irrigation and forecasting crop production in out-of-the way places.

Since early this year, NASA has supplied the USDA with near-real time data on lake and reservoir heights from around the world. The USDA has posted this information on a web site that allows users with a computer and Internet to access it for their varied uses. Analysts who forecast crop production, scientists, in-country water and irrigation managers, those involved in fishing industries, and the general public have all been making use of the site.

NASA and the French space agency Le Centre National d?Etudes Spatiales (CNES) teamed up to design, build and launch the TOPEX/Poseidon and the Jason-1 satellites. These satellites were designed to study many aspects of the ocean. The TOPEX/Poseidon satellite, for example, orbits at a height of 1336 kilometers (830 miles) above Earth, and can measure the height of the ocean surface directly underneath the satellite with an accuracy of 4-5 centimeters (better than 2 inches). Jason-1 and TOPEX/Poseidon cover the global oceans every 10 days. With these capabilities, this technology is surprisingly valuable for looking at larger areas of inland water.

“The satellites were designed with oceanographic objectives in mind, so the fact that they can be used for lakes and rivers are an added bonus,” said Charon Birkett, a University of Maryland researcher based at NASA’s Goddard Space Flight Center in Greenbelt, Md. It was Birkett’s work with satellites and inland water sources that caught the USDA’s interest.

Water level data for many lakes can be hard to get. Lakes may be located within inhospitable regions. Terrain may make it hard to install water level gauges, or some countries may not have the money for proper equipment. Even if there is equipment, someone must be available to regularly record the measurements. For an international agency like the USDA FAS, information on water levels in remote lakes in Africa or Asia, for example, may only be possible if a researcher happens to be passing by the area.

“Now we have this dataset which gives you a global picture of irrigation capabilities,” said Brad Doorn, Remote Sensing Technical Coordinator for the FAS. “It’s very much a night and day perspective as it relates to global irrigation potential.”

NASA/CNES satellites fly over 350 of the world’s largest lakes. The USDA decided to focus on about 150 of those that are important for agriculture. Of those, about 70 are currently online, with more being regularly added as Birkett and co-worker, Brian Beckley, from Raytheon’s Information Technology and Scientific Services (ITSS) team learn to extract information on the smaller lakes. Fifteen of the lakes that are currently online are in Africa.

The records begin with archived data from TOPEX/Poseidon, launched in 1992. They continued with data from the Jason-1 satellite, launched in December 2001. The two stayed in the same orbit for about 7 months, before the TOPEX/Poseidon satellite’s orbit was changed. These months of cross-over data were crucial for validating each of the satellites and for making sure the data records from Jason-1 were compatible with the TOPEX/Poseidon archive.

The information provided by the satellites, and made public through the web site, is a blessing to those who manage water for irrigation. Irrigated areas generally have less rainfall, and therefore crops in these drier regions are dependent on stores of water, like lakes, reservoirs and rivers.

The FAS analyzes crop production around the world. They regularly use computer models that simulate agricultural production based on inputs that include weather information. In this way they can examine global crop conditions and production. But in irrigated areas that are not rain fed, these methods are limited. For irrigated areas, you have to be able to determine how much water is actually stored, after seasonal precipitation passes.

“Satellite records of lake and reservoir water levels give you a good indication of whether there is going to be a systematic or major problem in water supply,” said Doorn. “If water is low, there may be problems for agricultural production.” This type of information is especially important for food aid partners, who must budget ahead for how much and where food aid is distributed.

Lake Tharthar in Central Iraq provides irrigation water to areas downstream. It is also linked to the Tigris and Euphrates Rivers. A drought that carried over many years severely cut grain output between 1999 and 2001. But since then, rainfall has increased, allowing grain production to recover and even surpass pre-drought levels. Knowledge of water levels in a region like this is crucial for the people who divvy out water for irrigation, and for those who plan aid.

The satellites have noticed some striking changes in lake levels around the world. In Iran, Lake Urmia has steadily decreased over the last 5 years. Also, between 1999 and 2001, Lake Hamoun in Iran near the Afghanistan border all but dried up and disappeared. By May 2003, water had returned to the lake. In that same time period, Lake Michigan levels have also declined.

On the other hand, when there is plenty of water, irrigation managers and farmers can assess the potential for more agriculture. When Caspian Sea levels rose in 1994, spill-over created a reservoir where little water existed before. As a result, the Kara Bogaz reservoir that borders the Caspian Sea was once largely desert and is now a large inland water body. Lake Nasser in Egypt also exists in a desert area where water supplies have increased.

As can be seen, the new technology allows researchers to get water level records regularly, globally, and in places where it is very hard to maintain or even acquire measurements. At the same time, there are also some limitations to the technology. For example, lake elevations can only be obtained during the lifetime of the satellite mission. Also, a satellite must pass directly over a lake for the radar to record water heights. But since the primary mission of these satellites is for studying the oceans, the fixed satellite orbit is determined by the community of oceanographers. That means people studying inland water have less input into the lakes that are monitored. In addition, some water bodies are simply too small for the instruments to pick up. These factors limit the number of observable lakes. “Sometimes, the lake that you want information about is the one you can’t get,” said Doorn.

Despite the current limitations, users like the FAS are thrilled to have access to the technology. Their web site provides new measurements to the public about a week to ten days after the satellite passes over.

“When USDA approached us, we told them the satellite record is not as accurate as a gauge sitting in a lake, but we can get good information within one to two weeks for many lakes in data-poor regions such as Africa and Asia,” said Birkett.

“It’s been a great USDA and NASA cooperative effort,” said Doorn. “It’s exactly what we needed and the type of cooperation provided has made it a real win-win situation.”

The project has been a collaborative effort between the NASA GSFC, USDA FAS, the University of Maryland, and Raytheon ITSS. The project was funded by the USDA/FAS.

Original Source: NASA News Release

Posted on by Fraser Cain

3D Screensaver of Mars

I know you all like pretty pictures on your desktop, so here’s something that’ll help fill your bottomless need for photos. The European Space Agency releases screensavers from time to time filled with photos taken by their spacecraft. This one’s a little different, though, it’s a screensaver that displays 3D images. In order to properly see the perspective in the photo, you need a pair of those 3D glasses… you know the paper ones with a red and blue lens that you can get at 3D movies or with some books.

Download the screensaver. – 1.4 MB

It’s actually a good idea for you to keep a pair of these glasses on hand by your computer. Mars Express, Spirit and Opportunity can take pictures in stereo, so you can see a 3D view of what the Red Planet really looks like. You should be able to find a pair of glasses at your local bookstore. And here’s a website that’s giving away free 3D glasses.

Have fun,

Fraser Cain
Publisher
Universe Today

Posted on by Fraser Cain

Recent Launch Demonstrates NASA Radar System

Radar tracking data gathered during the Delta II launch of the MESSENGER spacecraft earlier this month has provided promising results that may benefit NASA’s Space Shuttle Program and Discovery’s Return to Flight.

A pair of radars installed at NASA’s Kennedy Space Center, Fla., at a site north of Haulover Canal tracked the launch phase of the Delta II, including separation of the nine solid rocket boosters and jettison of the first stage and the payload fairing, the “nose” of the rocket that protected the MESSENGER spacecraft during launch.

“This test was quite successful for us in proving a concept,” said NASA project manager Tony Griffith. “The use of high-resolution wide band and Doppler radars allows us to observe almost any possible debris during ascent and means we can observe the Space Shuttle without regard to limitations of visibility, cloud cover and darkness.”

More importantly, the tandem radars “saw” — in significant detail — ice shedding from the Delta first stage, ejection of the solid rocket booster nozzle throat plugs, and contents of their exhaust. These are normal Delta launch events. For the Space Shuttle Program, the test showed that the radars, working together, were effective in visualizing the vehicle elements in high resolution and the ability to attain speedy interpretation of the images for initial data analysis after a Shuttle launch.

The antennas have been on loan to NASA from the USNS Pathfinder, a U.S. Navy instrumentation ship. The 30-foot-diameter C-band wideband radar antenna and the smaller X-band Doppler radar worked together to image the Delta in flight. The Navy operated the radars for NASA during the MESSENGER launch. NASA was responsible for analyzing the imagery.

“This turned out to be a successful and mutually beneficial partnership with the Navy that we will pursue,” Griffith said.

Later this fall, a 50-foot-diameter C-band wide band radar will be installed on this site for a similar Return to Flight application and for use by the Navy. The radar is being relocated to KSC from the Roosevelt Roads Naval Station in Puerto Rico.

The radars used for the test are being returned to the USNS Pathfinder, though the C-band radar used in this test could return as a backup for Return to Flight, if available from the Navy. NASA is evaluating the procurement of two X-band Doppler radars for use on ships downrange, including one of the solid rocket booster retrieval ships.

Original Source: NASA News Release