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Supermassive black holes and hot galaxies in giant haul

Wise telescope data Wise has been able to see objects not visible to past science instruments

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A space telescope has added to its list of spectacular finds, spotting millions of supermassive black holes and blisteringly hot, "extreme" galaxies.

The finds, by US space agency Nasa's Wide-Field Infrared Survey Explorer (Wise), once lay obscured behind dust.

 

But Wise can see in wavelengths correlated with heat, seeing for the first time some of the brightest objects in the Universe.

 

The haul will help astronomers work out how galaxies and black holes form.

It is known that most large galaxies host black holes at their centres, sometimes feeding on nearby gas, dust and stars and sometimes spraying out enough energy to halt star formation altogether.

 

How the two evolve together has remained a mystery, and the Wise data are already yielding some surprises.

 

Wise gives astronomers what is currently a unique view on the cosmos, looking at wavelengths of light far beyond those we can see but giving information that we cannot get from wavelengths we can.

Black holes

Artist's depiction of black hole
  • These are regions of space where gravity is so powerful that not even light can escape
  • One way they can form is when huge stars collapse in on themselves
  • So-called supermassive black holes sit at the centres of galaxies, including the Milky Way

Among its other discoveries, in 2011 Wise spotted in a "Trojan" asteroid ahead of the Earth in its orbit.

 

But with the latest results, Wise has come into its own as an unparalleled black hole hunter.

 

"We've got the black holes cornered," said Daniel Stern of Nasa's Jet Propulsion Laboratory (JPL), lead author of one of the three studies presented on Wednesday.


Dr Stern and his colleagues used the Nuclear Spectroscopic Telescope Array (Nustar) space telescope to examine the X-rays coming out of the black hole candidates spotted by Wise, presenting their findings in a paper to appear in

Astrophysical Journal.

 

"Wise is finding them across the full sky, while Nustar is giving us an entirely new look at their high-energy X-ray light and learning what makes them tick," he said.

 

The other two studies presented - one already published in Astrophysical journal and another yet to appear - focussed on extremely hot, bright galaxies that have until now remained hidden: hot dust-obscured galaxies, or hot-Dogs.


There are so far about 1,000 candidate galaxies, some of which can out-shine our Sun by a factor of 100 trillion.

 

"These dusty, cataclysmically forming galaxies are so rare Wise had to scan the entire sky to find them," said Peter Eisenhardt of JPL, lead author of the paper describing Wise's first hot-Dog find.

 

"We are also seeing evidence that these record-setters may have formed their black holes before the bulk of their stars. The 'eggs' may have come before the 'chickens'."


The data from the Wise mission are made publicly available so that scientists outside the collaboration can also carry out their own studies, so the future will hold a wealth of studies from these extreme and otherwise hidden corners of the Universe.

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Originally Posted by ABIDHA:

Why mention the name of God when you don't believe in God? How does an atheist know God plays dice when you're speaking in scientific terms?

atheists rationally conclude on their belief system rather than accept the default cultural offerings.

 

Were you cognizant of the context where that statement was made you would understand the title of the thread. I leave the analysis to better informed discussants.

FM
 
September 5, 2012 1:45 PM
<dl class="storyBlogByline"><dt class="storyBlogBy">By</dt><dd>SPACE.com Staff</dd></dl>

This artist's concept depicts a cometlike tail of a possible disintegrating super Mercury-size planet candidate as it transits, or crosses, its parent star, named KIC 12557548. (NASA/JPL-Caltech)

 

 

(SPACE.com) Astronomers have found a dusty tail streaming off a faraway alien planet, suggesting that the tiny, scorching-hot world is indeed falling apart.

 

 

In May, researchers announced the detection of a possibly distintegrating exoplanet, a roughly Mercury-size world being boiled away by the intense heat of its parent star. Now, a different team has found strong evidence in support of the find -- a massive dust cloud shed by the planet, similar to the tail of a comet.

 

 

Both studies used observations from NASA's Kepler space telescope, which spots alien planets by flagging the telltale brightness dips caused when they pass in front of their parent stars from the instrument's perspective.

The unfortunate alien planet lies about 1,500 light-years away from Earth. It sits very close to its host star -- completing an orbit every 15 hours -- and is therefore incredibly hot, with surface temperatures estimated to be around

 

 

3,600 degrees Fahrenheit (1,982 degrees Celsius).

The discovery team noticed that light from the planet's star, which is called KIC 12557548, dims in oddly variable ways uncharacteristic of other planet-hosting stars. The researchers hypothesized that the brightness dips are caused by a somewhat amorphous, shape-shifting body, and they predicted that the planet is likely surrounded by a huge veil of dust and gas. [Gallery: A World of Kepler Planets]

 

In the new study, a different team of scientists affirms the existence of this planetary dust tail. Looking closely at Kepler's data, they found clear signals that KIC 12557548's light is being scattered and absorbed by large amounts of dust.

 

 

"Some of this dust escapes into space, where the intense stellar radiation quickly evaporates it," study lead author Matteo Brogi, of Leiden University in the Netherlands, said in a statement. "The variable amount of dust leads to the observed variability in the star's dimming." 

 

 

Further work with different instruments could help nail down just what the planet is made of, researchers said.

 

 

"By observing the dust clouds in different colors, something Kepler cannot do, we will be able to determine the amount and the composition of the dust and estimate its lifetime," said co-author Christoph Keller, also of Leiden University. "As the evaporation peels the planet like an onion, we can now see what used to be the inside of a planet."

The study has been accepted for publication in the journal Astronomy & Astrophysics.

 

 

The $600 million Kepler space telescope launched in March 2009. Since then, it has detected more than 2,300 potential alien planets, 77 of which have been confirmed to date. Kepler scientists have estimated that at least 80 percent of the instrument's finds will end up being the real deal.



Follow SPACE.com for the latest in space science and exploration news on Twitter @Spacedotcom and on Facebook.

Copyright 2012 SPACE.com, a TechMediaNetwork company. All rights reserved. This material may not be published, broadcast, rewritten or redistributed.

Space.com. All rights reserved.

FM

Milky Way's Giant Black Hole to Eat Space Cloud in 2013

Date: 02 July 2012 Time: 11:42 AM ET
 
 
 
Space Cloud Falling into Sagittarius A*
This still from a computer animation shows a simulation of a giant space cloud falling into Sagittarius A*, the supermassive black hole at the center of our own Milky Way galaxy, in mid-2013. Image added on July 2, 2012.
CREDIT: European Research Media Center

The colossal black hole at the center of our Milky Way galaxy will soon to get a big, tasty meal, astronomers say.

A humongous gas cloud is on a collision course for the Milky Way's core — the home of Sagittarius A* (pronounced "Sagittarius A-star"), which scientists suspect is a supermassive black hole with the mass of 4 million suns.

When the huge gas cloud arrives in the vicinity, which it will appear to us to do in mid-2013, it will surely be swallowed up by the hungry black hole, scientists say.

 

Astrophysicist Stefan Gillessen of the Max Planck Institute for Extraterrestrial Physics in Munich, Germany, has been observing the Milky Way's center for about 20 years. So far, he's seen only two stars come as close to Sagittarius A* as the cloud will.

"They passed unharmed, but this time will be different: the gas cloud will be completely ripped apart by the tidal forces of the black hole," Gillessen said in a statement.

 

The cloud is due to pass within about 36 light-hours (about 25 billion miles, or 40 billion kilometers) of the black hole. Its speed, which is now more than 5 million mph (8 million km per hour), has nearly doubled in the last seven years as it approaches its doom. It has already started to shred, and is likely to break up completely before it hits the black hole.

While black holes themselves are impossible to see — they are objects whose gravitational pull is so strong, even light cannot escape — astronomers can watch what happens when matter falls into one. The areas around some active supermassive black holes are so bright, in fact, that they are visible across the universe.

 

Scientists are looking forward to the rare chance to see something fall into our own galaxy's black hole. As it falls nearer and nearer, the cloud is expected to heat up and release bright X-ray radiation that should be visible from Earth.

 

The collision-bound cloud was discovered by a team of astronomers led by Reinhard Genzel at the European Southern Observatory.

Follow Clara Moskowitz on Twitter @ClaraMoskowitz or SPACE.com @Spacedotcom. We're also on Facebook & Google

FM

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