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7 April 2008
XMM-Newton has been surprised by a rare type of galaxy, from which it has detected a higher number of X-rays than thought possible. The observation gives new insight into the powerful processes shaping galaxies during their formation and evolution.
Scientists working with XMM-Newton were looking into the furthest reaches of the universe, at celestial objects called quasars. These are vast cosmic engines that pump energy into their surroundings. It is thought an enormous black hole drives each quasar.
As matter falls into the black hole, it collects in a swirling reservoir called the accretion disc, which heats up. Computer simulations suggest that powerful radiation and magnetic fields present in the region eject some of gas from the gravitational clutches of the black hole, throwing it back into space.
This outflow has a profound effect on its surrounding galaxy. It can create turbulence in the gas throughout the galaxy, hampering star formation. Thus, understanding quasars is an important step to understanding the early history of galaxies.
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BAL quasar, top view |
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BAL quasar, side view |
The Cassini spacecraft tasted and sampled a surprising organic brew erupting in geyser-like fashion from Saturn's moon Enceladus during a close flyby on 12 March. Scientists are amazed that this tiny moon is so active, ‘hot’ and brimming with water vapour and organic chemicals.
New heat maps of the surface show higher temperatures than previously known in the south polar region, with hot tracks running the length of giant fissures. Additionally, scientists say the organics ‘taste and smell’ like some of those found in a comet. The jets themselves harmlessly peppered Cassini, exerting measurable torque on the spacecraft, and providing an indirect measure of the plume density.
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Gas and dust jets match up |
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Enceladus plume neutral mass spectrum |

Image above: Steve Wilkinson (left) with Michael Phelps.
Credit: NASA/Kathy Barnstorff
World champion swimmer Michael Phelps knows a thing or two about swimsuits. He owns 29 U.S. national swimming titles and won six gold medals and two bronze at the last Summer Olympics four years ago in Australia.
NASA researcher Steve Wilkinson doesn't know that much about swimwear, but he does know a thing or two about drag reduction … how to make something propel through air or water faster and more efficiently.
The swimmer and the researcher met for the first time in New York City at the unveiling of a new product they both had a part in developing. It's called by its manufacturer the "world's fastest swimsuit."
"When I hit the water, I feel like a rocket," said Phelps. "I can't wait to race in it. This is going to take the sport of swimming to a new level."
Phelps and other U.S. athletes may prove that this August at the 2008 Summer Olympics in Beijing. Wilkinson already knows the fabric Phelps will be wearing has gone through a new level of extensive testing at NASA's Langley Research Center in Hampton, Va., and other laboratories.
Image above: The new swimsuits were unveiled in New York.
Credit: NASA/Kathy Barnstorff
"We evaluated the surface roughness effects of nearly 60 fabrics or patterns in one of our small low speed wind tunnels," said Wilkinson. "We were assessing which fabrics and weaves had the lowest drag."
But how can you test a fabric that's supposed to be used in water in a wind tunnel that uses air? It turns out that air and water obey the same physical laws of motion, so a wind tunnel can simulate similar drag a fabric would experience in water. Testing in air is also less expensive, simpler and offers more testing options than testing in water.
Warnaco Inc., which is the U.S. licensee of the Speedo swimwear brand, approached NASA Langley to test fabric samples, since NASA Langley has researched drag reduction for aircraft and even boats for decades.
Just like reducing drag helps planes fly more efficiently, reducing drag helps swimmers go faster. Studies indicate viscous drag or skin friction is almost one-third of the total restraining force on a swimmer. Wind tunnel tests measure the drag on the surface of the fabrics.
"This is the first time I've tested a fabric and there were some challenges involved," said researcher Wilkinson. "It was a challenge to figure out how to get the fabric on a test plate and how to prepare the edges so nothing would interfere with air flow over the fabric. I think we've done a really good job with the help of Speedo coming up with a protocol that lets us to test these fabrics with ease and precision."
Image above: Steve Wilkinson prepares a swimsuit fabric sample for a wind tunnel test.
Credit: NASA/Sean Smith
The candidate materials Wilkinson receives from the company come in the form of tubes. He stretches the tubes over a smooth, flat aluminum plate, then tapes down the edges. The plate goes into the small wind tunnel test section. With a flip of a switch, air flows over it. Wilkinson runs the tunnel through a number of wind speeds and, with the help of sensors, measures drag on the surface. He records the data and then sends it on to Speedo researchers.
"It turns out to simulate a swimmer in the water at about two meters per second, we need to run the wind tunnel at about 28 meters per second (about 63 miles per hour), which is well within its capability," added Wilkinson. "The tests have generally shown the smoother the fabric, the lower the drag."
Speedo's research and development team, Aqualab, took those results and used them to help create a new swimsuit that the company says is its most hydro-dynamically advanced swimsuit to date.
Kathy Banstorff
NASA Langley Research Center
7 March 2008
The Cassini spacecraft has found evidence of material orbiting Rhea, Saturn's second largest moon. This is the first time rings may have been found around a moon.
A broad debris disc and at least one ring appear to have been detected by a suite of six instruments on Cassini specifically designed to study the atmospheres and particles around Saturn and its moons.
7 March 2008
Swooping through space are solitary waves, which in theory do not change form or lose energy as they go along. These waves, which exist on Earth in different media, have been detected and explained for the first time in space thanks to Cluster data.
In theory, these solitary waves, called solitons, propagate endlessly maintaining their shape and form as well as velocity, which means that they do not lose energy with time.
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28 February 2008
A trio of NASA and ESA spacecraft orbiting Mars are preparing for the 25 May arrival of NASA's Phoenix lander. ESA's Mars Express has already started adjusting its orbit to provide critical back-up monitoring of Phoenix.
In May, when Phoenix enters the Red Planet's atmosphere at over