Showing posts with label Extraterrestrial Physics. Show all posts
Showing posts with label Extraterrestrial Physics. Show all posts

Monday, February 27, 2012

Astrophysicists Discover Stellar Black Hole In Andromeda Galaxy

Astrophysicists claim to have discovered a stellar black hole in the Andromeda galaxy.

The scientists, from Clemson University and the Max Planck Institute for Extraterrestrial Physics, have discovered a stellar mass black hole in Andromeda, a spiral galaxy about 2.6 million light years from Earth.

The discovery was made with data from NASA's Chandra observatory.

The team was studying ultra-luminous X-Rays, emitted a long time ago.

The black hole was suspected when they detected an unusual X-Ray transient light source in Andromeda.

They concluded the source was emitting X-Rays because the black hole was absorbing material at very high rates.

"The brightness suggested that these X-rays belonged to the class of ultra=luminous X-ray sources, or ULXs," said Amanpreet Kaur, a graduate student in physics from the Clemson University, adding, "But ULXs are rare.

There are none at all in the Milky Way where Earth is located, and this is the first to be confirmed in Andromeda. Proving it required detailed observations." The team concluded the ULX source probably originated from a system similar to X-Ray binaries in our own galaxy.

Stellar black holes are small black holes formed by the collapse of very massive stars, each of which weighs about 10 times as much as our Sun.

"We were very lucky that we caught the ULX early enough to see most of its light curve, which showed a very similar behavior to other X-ray sources from our own galaxy," said Wolfgang Pietsch of the Max Planck Institute.

"This means that the ULX in Andromeda likely contains a normal, stellar black hole swallowing material at very high rates," he added.

Wednesday, August 31, 2011

Hubble movies reveal solar-system-sized traffic jams

Rice astronomer Patrick Hartigan displays a target from an experiment to re-create the physics of stellar jets on a small scale. Powerful lasers blasted a tiny plug of titanium inside the gold-coated cone, shooting the atomised material into a ball of foam-covered plastic. 

The experiment re-created some of the fluid dynamics that occur on a huge scale when newborn stars spew columns of high-speed gas and dust. Jeff Fitlow/Rice University


When it comes to big-budget action movies, Rice University astronomer Patrick Hartigan prefers Hubble to Hollywood.

Using Hubble Space Telescope images collected over 14 years, Hartigan has created time-lapse movies that offer astronomers their first glimpse of the dynamic behaviour of stellar jets, huge torrents of gas and particles that spew from the poles of newborn stars.

An analysis of the movies that was published in The Astrophysical Journal is forcing astronomers to rethink some of the processes that occur during the latter stages of star birth.

In an effort to learn even more, Hartigan and colleagues are using powerful lasers to recreate a small-scale version of the solar-system-sized jets in a lab in upstate New York.

"The Hubble's given us spectacular images," said Hartigan, professor of physics and astronomy at Rice. "In the nebulae where stars are born, for instance, we can see beautiful filaments and detailed structure.

We know these images are frozen snapshots in time, but we would need to watch for hundreds of thousands of years to see how things actually play out."

Hartigan said stellar jets are different because they move very quickly. Stellar jets blast out into space from the poles of newly formed stars at about 600,000 miles an hour.

Astronomers first noticed them about 50 years ago, and they believe the sun probably had stellar jets when it formed about 4.5 billion years ago.

Hartigan began using Hubble to collect still frames of stellar jets in 1994. The jets emerge from each pole of a young star, and Hartigan used Hubble to revisit the jets from three stars in 1994, 1998 and 2008.

All three stars are about 1,350 light years from Earth. Two are near the Orion Nebula, and the third is in the southern sky in the constellation Vela.

By lacing the images together and using a computer to fill in what occurred between still frames, Hartigan and his collaborators created time-lapse movies.

The movies clearly showed something that wasn't obvious in any of the still images; clouds of dust and gas within the jets move at different speeds.

"The bulk motion of the jet is about 300 kilometers per second," Hartigan said. "That's really fast, but it's kind of like watching a stock car race; if all the cars are going the same speed, it's fairly boring.

The interesting stuff happens when things are jumbling around, blowing past one another or slamming into slower moving parts and causing shockwaves."

Understanding what happens in those huge collisions is another challenge. The phenomena didn't look like anything that Hartigan and his astronomer colleagues had seen. But when he showed them to colleagues who were familiar with the physics of nuclear explosions, they immediately saw patterns in the shockwaves that looked familiar.

Thursday, June 30, 2011

ESA Integral: Challenges physics beyond Einstein

Integral’s IBIS instrument captured the gamma-ray burst (GRB) of 19 December 2004 that Philippe Laurent and colleagues have now analysed in detail.

It was so bright that Integral could also measure its polarisation, allowing Laurent and colleagues to look for differences in the signal from different energies.

The GRB shown here, on 25 November 2002, was the first captured using such a powerful gamma-ray camera as Integral’s. When they occur, GRBs shine as brightly as hundreds of galaxies each containing billions of stars.

Credits: ESA/SPI Team/ECF

Thursday, December 2, 2010

NASA Search for ET: Conference announcement

"NASA will hold a news conference at 2 pm EST (1900 GMT) on Thursday, December 2, to discuss an astrobiology finding that will impact the search for evidence of extraterrestrial life," it said on its website.
 
Space enthusiasts and believers in alien life took to the blogosphere in a flurry of speculation over the potential meaning of the announcement, though NASA declined to elaborate further.
 
Those scheduled to speak included Mary Voytek, who heads NASA's astrobiology program; Felisa Wolfe-Simon, a NASA astrobiology research fellow from the US Geological Survey; and Pamela Conrad, an astrobiologistat NASA's Goddard Space Flight Center.
 
Astrobiology relates to the study of life in the universe, including its origin and evolution, where it is located and how it might survive in the future

Friday, May 14, 2010

ESA ESERO Project: Summer Workshop for Secondary School Science Teachers

The International Space Station, the largest laboratory ever built in space, is the result of many years of cooperation between the USA, Russia, Canada, Japan and Europe.


This illustration shows the Automated Transfer Vehicle, ATV, that carries food, clothing, fuel tanks, air and drinking water to the ISS crew.

The first launch of this supply vessel in 2008 marked the first ever rendezvous and docking of a European spacecraft in orbit.


Credits: V. Bétoulaud

The European Space Agency is providing many innovative and inspiring aids to teachers to enhance their curriculum with space related subjects. Now ESA is inviting educators to a summer workshop at its establishment in the Netherlands from 28 to 30 June 2010.

ESA’s Directorate of Human Spaceflight has been using the International Space Station as a 'classroom in space' for many educational events and for the production of educational material made available to teachers, science educators and all interested.

ISS will continue in orbit till at least 2020 – and the educational side of the ISS will be even stonger in the future as the focus of the ISS activities is being turned from construction to routine operation.

For more information contact ESA directly by following this link

Thursday, May 13, 2010

Chandra X-Ray Observatory: Black Hole rips star apart

This artist impression illustrates the tremendous gravitational pull of a giant black hole on a passing star.

The doomed object is first stretched by tidal forces until it is torn apart.

Most of the gas making up the star is lost from the system but some of it is trapped by the black hole and forms a disc of gas around it.

In the disc, the gas is heated to millions of degrees and emits in the X-rays, before disappearing forever, swallowed by the black hole.

It is precisely the signature of this disc that ESA's XMM-Newton has detected.

Credits: ESA and Stefanie Komossa (Max Planck Institute for Extraterrestrial Physics)