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Cosmic engines surprise XMM-Newton

 

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.
 
 
BAL quasar, top view
BAL quasar, top view
However, the structure surrounding a quasar is difficult to see because they are so distant. The light and X-rays from them takes thousands of millions of years to reach us.

About 10-20% of quasars are of a special type called BAL quasars. The BAL stands for ‘broad absorption line’ and seems to indicate that a thick cocoon of gas surrounds the quasar.

Most researchers believe that gas flows away from a BAL quasar along the equatorial direction of the accretion disc. These quasars show little X-ray emission, indicating that there is enough gas to absorb most of the X-rays given out from the region near the black hole.

But some BAL quasars appear to be spewing material out along their polar axes, at right angles to the accretion discs.

JunXian Wang, Center for Astrophysics, University of Science and Technology of China, Hefei, and his colleagues including Tinggui Wang and Hongyan Zhou, used XMM-Newton to target four such polar BAL quasars, identified by them previously. They were investigating whether the X-rays were being absorbed strongly.
 
 
BAL quasar, side view
BAL quasar, side view
XMM-Newton observed the quasars at specific times during 2006 and 2007. Two of them emitted more X-rays than the researchers anticipated, indicating that there is no veil of absorbing gas surrounding these particular quasars. “Our results can help refine the computer simulations of how these quasars work,” says Wang.
 
 
It may mean that BAL quasars are more complicated than originally thought. “Perhaps there can be both equatorial outflows and polar outflows simultaneously from these objects,” says Wang. Maybe, the outflows are even produced by similar means.

Computer simulations suggest that the polar outflows, like the gas ejected from the accretion disc, are also material falling in, turned away by fierce radiation before it comes near the black hole.
 
 
Wang and colleagues are now following this work up. They hope to monitor more BAL quasars over a longer period of time. “We need more data so that we can look into the details of the X-ray emission,” says Wang.

It seems that the more astronomers look into the distant universe, the more complex it becomes.
 
 
Notes for editors:
 
The findings appear in ‘XMM observations of BAL Quasars with polar outflows’ by J. Wang, P. Jiang, H. Zhou, T. Wang, X. Dong, and H. Wang, published in the Astrophysical Journal Letters on `20 March 2008

نوشته شده توسط احسان صادقی در جمعه بیست و سوم فروردین 1387 | موضوع: تازه ترین اخبار هوا و فضا به زبان انگلیسی
Cassini 'tastes' organic brew at Saturn’s geyser moon

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.
 
 
Gas and dust jets match up
Gas and dust jets match up
"A completely unexpected surprise is that the chemistry of Enceladus, what's coming out from inside, resembles that of a comet," said Hunter Waite, principal investigator for the Cassini Ion and Neutral Mass Spectrometer at the Southwest Research Institute in San Antonio. "To have primordial material coming out from inside a Saturn moon raises many questions on the formation of the Saturn system."

"Enceladus is by no means a comet. Comets have tails and orbit the sun, and Enceladus's activity is powered by internal heat while comet activity is powered by sunlight. Enceladus's brew is like carbonated water with an essence of natural gas," said Waite.
 
 
Enceladus plume neutral mass spectrum
Enceladus plume neutral mass spectrum
The Ion and Neutral Mass Spectrometer saw a much higher density of volatile gases, water vapour, carbon dioxide and carbon monoxide, as well as organic materials, some 20 times denser than expected. This dramatic increase in density was evident as the spacecraft flew over the area of the plumes.

New high-resolution heat maps of the south pole by Cassini's Composite Infrared Spectrometer show that the so-called tiger stripes, giant fissures that are the source of the geysers, are warm along almost their entire lengths, and reveal other warm fissures nearby. These more precise new measurements reveal temperatures of at least minus 93º Celsius. That is 17º warmer than previously seen and 93º Celsius warmer than other regions of the moon. The warmest regions along the tiger stripes correspond to two of the jet locations seen in Cassini images.
 


ادامه مطلب
نوشته شده توسط احسان صادقی در جمعه نهم فروردین 1387 | موضوع: تازه ترین اخبار هوا و فضا به زبان انگلیسی
Icy Promethei Planum

 

Promethei Planum

Promethei Planum 
Promethei Planum, an area seasonally covered with a more than 3500 m thick layer of ice in the martian south polar region, was the subject of the High Resolution Stereo Camera’s focus on 22 September 2005 as Mars Express was in orbit above the Red Planet

ادامه مطلب
نوشته شده توسط احسان صادقی در چهارشنبه بیست و دوم اسفند 1386 | موضوع: تازه ترین اخبار هوا و فضا به زبان انگلیسی
New lunar south polar maps from SMART-1

Lunar south pole mosaic

Lunar south pole mosaic

ادامه مطلب
نوشته شده توسط احسان صادقی در چهارشنبه بیست و دوم اسفند 1386 | موضوع: تازه ترین اخبار هوا و فضا به زبان انگلیسی
NASA Know-How Helps Athletes Rocket Through Water
 

Steve Wilkinson (left) with Michael Phelps

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.

The new swimsuits are unveiled at a press conference

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."

Steve Wilkinson testing swimsuits fabrics

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

نوشته شده توسط احسان صادقی در دوشنبه بیستم اسفند 1386 | موضوع: تازه ترین اخبار هوا و فضا به زبان انگلیسی
Saturn’s moon Rhea may also have rings

Rhea's rings

Rhea's rings

 
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.


ادامه مطلب
نوشته شده توسط احسان صادقی در شنبه هجدهم اسفند 1386 | موضوع: تازه ترین اخبار هوا و فضا به زبان انگلیسی
Solitary waves in translation
An artist's impression of the Cluster quartet
The Cluster quartet

 

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.


ادامه مطلب
نوشته شده توسط احسان صادقی در شنبه هجدهم اسفند 1386 | موضوع: تازه ترین اخبار هوا و فضا به زبان انگلیسی
Mars and Venus are surprisingly similar
 

 

5 March 2008
Using two ESA spacecraft, planetary scientists are watching the atmospheres of Mars and Venus being stripped away into space. The simultaneous observations by Mars Express and Venus Express give scientists the data they need to investigate the evolution of the two planets’ atmospheres.
 
Scientists call this work comparative planetology. Mars Express and Venus Express are so good at it because they carry very similar science instruments. In the case of the Analyser of Space Plasmas and Energetic Atoms (ASPERA), they are virtually identical. This allows scientists to make direct comparisons between the two planets.

The new results probe directly into the magnetic regions behind the planets, which are the predominant channels through which electrically-charged particles escape. They also present the first detection of whole atoms escaping from the atmosphere of Venus, and show that the rate of escape rose by ten times on Mars when a solar storm struck in December 2006.

By observing the current rates of loss of the two atmospheres, planetary scientists hope that they will be able to turn back the clock and understand what they were like in the past. “These results give us the potential to measure the evolution of planetary climates,” says David Brain, Supporting Investigator for plasma physics for Venus Express and Co-Investigator for ASPERA on Mars and Venus Express at the University of California, Berkeley.
  

ادامه مطلب
نوشته شده توسط احسان صادقی در چهارشنبه پانزدهم اسفند 1386 | موضوع: تازه ترین اخبار هوا و فضا به زبان انگلیسی
Mars Express one of three orbiters preparing for Phoenix landing
Mars Express artist's impression
Mars Express
 

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 20 000 km/h, two NASA spacecraft - Mars Odyssey and the Mars Reconnaissance Orbiter - will closely monitor the stream of data being transmitted. In case anything goes wrong, NASA has requested that ESA's Mars Express, which has been in orbit around Mars since December 2003, also monitors the 13-minute entry, descent and landing (EDL) phase.

 


ادامه مطلب
نوشته شده توسط احسان صادقی در سه شنبه چهاردهم اسفند 1386 | موضوع: تازه ترین اخبار هوا و فضا به زبان انگلیسی
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