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Posts Tagged ‘telescope’

NASA’s Black-Hole-Hunter Catches Its First 10 Supermassive Black Holes

September 10, 2013 Leave a comment

Sep. 9, 2013 — NASA’s black-hole-hunter spacecraft, the Nuclear Spectroscopic Telescope Array, or NuSTAR, has “bagged” its first 10 supermassive black holes. The mission, which has a mast the length of a school bus, is the first telescope capable of focusing the highest-energy X-ray light into detailed pictures.

 

An optical color image of galaxies is seen here overlaid with X-ray data (magenta) from NASA’s Nuclear Spectroscopic Telescope Array (NuSTAR). (Credit: NASA/JPL-Caltech)
 

The new black-hole finds are the first of hundreds expected from the mission over the next two years. These gargantuan structures — black holes surrounded by thick disks of gas — lie at the hearts of distant galaxies between 0.3 and 11.4 billion light-years from Earth.

“We found the black holes serendipitously,” explained David Alexander, a NuSTAR team member based in the Department of Physics at Durham University in England and lead author of a new study appearing Aug. 20 in The Astrophysical Journal. “We were looking at known targets and spotted the black holes in the background of the images.”

Additional serendipitous finds such as these are expected for the mission. Along with the mission’s more targeted surveys of selected patches of sky, the NuSTAR team plans to comb through hundreds of images taken by the telescope with the goal of finding black holes caught in the background.

 

Read more: http://www.sciencedaily.com/releases/2013/09/130909154918.htm

NASA-Funded Scientists Detect Water on Moon’s Surface that Hints at Water Below

September 2, 2013 Leave a comment

This image of the moon was generated by data collected by NASA's Moon Mineralogy MapperThis image of the moon was generated by data collected by NASA’s Moon Mineralogy Mapper on the Indian Space Research Organization’s Chandrayaan-1 mission. It is a three-color composite of reflected near-infrared radiation from the sun, and illustrates the extent to which different materials are mapped across the side of the moon that faces Earth. Image credit: ISRO/NASA/JPL-Caltech/Brown Univ./USGS
› Full image and caption

 

August 28, 2013

PASADENA – NASA-funded lunar research has yielded evidence of water locked in mineral grains on the surface of the moon from an unknown source deep beneath the surface. Using data from NASA’s Moon Mineralogy Mapper (M3) instrument aboard the Indian Space Research Organization’s Chandrayaan-1 spacecraft, scientists remotely detected magmatic water, or water that originates from deep within the moon’s interior, on the surface of the moon.

The findings, published Aug. 25 in Nature Geoscience, represent the first detection of this form of water from lunar orbit. Earlier studies had shown the existence of magmatic water in lunar samples returned during NASA’s Apollo program.

M3 imaged the lunar impact crater Bullialdus, which lies near the lunar equator. Scientists were interested in studying this area because they could better quantify the amount of water inside the rocks due to the crater’s location and the type of rocks it held. The central peak of the crater is made up of a type of rock that forms deep within the lunar crust and mantle when magma is trapped underground.

 

Read more: http://www.jpl.nasa.gov/news/news.php?release=2013-262

Hubble catches comet ISON hurtling toward The Sun


By Shaunacy Ferro @ popsci.com

Comet ISON

Comet ISON Image Credit: NASA, ESA, and the Hubble Heritage Team (STScI/AURA)

Fourth of July is the perfect time to watch fiery masses streak across the sky. This speedy guy, the comet ISON, looks like it pretty much fits that bill. Except that it’s actually quite icy at its core, and it’s barreling toward the sun at around 48,000 miles per hour, faster than any firework.

This five-second loop of video is a compression of images taken by the Hubble Space Telescope over a period of 43 minutes in May, during which ISON covered 34,000 miles.

Read more:  http://www.popsci.com/science/article/2013-07/hubble-catches-comet-ison-hurtling-across-sky

Hubble Space Telescope Captures The Ring Nebula In Astonishing Detail


By Clay Dillow Posted 05.24.2013

The Ring Nebula
The Ring Nebula New images of the Ring Nebula captured by the Hubble Space Telescope are redefining the way astronomers understand its shape. NASA, ESA, C.R. Robert O’Dell (Vanderbilt University), G.J. Ferland (University of Kentucky), W.J. Henney and M. Peimbert (National Autonomous University of Mexico)
Astronomers love to point their telescopes at the Ring Nebula. Located 2,000 light years away in the constellation Lyra, this ring of glowing gas has a distinctive elliptical shape when seen from Earth. But new images captured by the Hubble Space Telescope suggest that the nebula actually looks a lot more like a football or a misshapen doughnut.

NASA | SDO’s Ultra-high Definition View of 2012 Venus Transit

February 13, 2013 Leave a comment

Never-Before-Seen Stage of Planet Birth Revealed


by Nola Taylor Redd, SPACE.com Contributor
Date: 02 January 2013 Time: 01:00 PM ET
 ALMA observations of planet-forming bridge

Observations made with the Atacama Large Millimeter/submillimeter Array (ALMA) telescope of the disc of gas and cosmic dust around the young star HD 142527, showing vast streams of gas flowing across the gap in the disc. These are the first direct observations of these streams.
CREDIT: ALMA (ESO/NAOJ/NRAO), S. Casassus et al.

 
  Astronomers studying a newborn star have caught a detailed glimpse of planets forming around it, revealing a never-before seen stage of planetary evolution.

Large gas giant planets appear to be clearing a gap in the disk of material surrounding the star, and using gravity to channel material across the gap to the interior, helping the star to grow. Theoretical simulations have predicted such bridges between outer and inner portions of disks surrounding stars, but none have been directly observed until now.

Read more: http://www.space.com/19100-alien-planet-birth-alma-telescope.html

Largest Quasar Ever Discovered Burns 100 Times Brighter Than Entire Milky Way

November 29, 2012 Leave a comment

By Emily Elert Posted 11.28.2012
 
Glowing galactic center located near a supermassive black hole
Artist's Rendering of Huge Quasar Outflow

Artist’s Rendering of Huge Quasar Outflow ESO/L. Calçada

Astronomers have found a galaxy whose super-luminous nucleus–called a quasar–is burning 100 times as much energy as the entire Milky Way galaxy.

Though theory has long predicted that quasars this powerful should exist, the newly-discovered object, known as SDSS J1106+1939, is by far the most energetic ever observed. The quasar is powered by a supermassive black hole that lies at its center.

Read more: http://www.popsci.com/science/article/2012-11/scientists-discover-biggest-quasar-ever-near-supermassive-black-hole

Planck spots hot gas bridging galaxy cluster pair

November 22, 2012 1 comment

Planck spots hot gas bridging galaxy cluster pair

 
Galaxy clusters connected by gas bridge

 20 November 2012
ESA’s Planck space telescope has made the first conclusive detection of a bridge of hot gas connecting a pair of galaxy clusters across 10 million light-years of intergalactic space.
 
Planck’s primary task is to capture the most ancient light of the cosmos, the Cosmic Microwave Background, or CMB. As this faint light traverses the Universe, it encounters different types of structure including galaxies and galaxy clusters – assemblies of hundreds to thousands of galaxies bound together by gravity.

If the CMB light interacts with the hot gas permeating these huge cosmic structures, its energy distribution is modified in a characteristic way, a phenomenon known as the Sunyaev–Zel’dovich (SZ) effect, after the scientists who discovered it.

This effect has already been used by Planck to detect galaxy clusters themselves, but it also provides a way to detect faint filaments of gas that might connect one cluster to another.

In the early Universe, filaments of gaseous matter pervaded the cosmos in a giant web, with clusters eventually forming in the densest nodes.

Much of this tenuous, filamentary gas remains undetected, but astronomers expect that it could most likely be found between interacting galaxy clusters, where the filaments are compressed and heated up, making them easier to spot.

 Read more: http://www.esa.int/SPECIALS/Planck/SEMRT791M9H_0.html

NASA locates most distant galaxy ever discovered

November 19, 2012 Leave a comment

The most distant galaxy ever seen in the universe has been detected by NASA’s Hubble and Spitzer space telescopes.

The most distant galaxy ever seen in the universe has been detected by NASA's Hubble and Spitzer space telescopes.

The newly discovered galaxy, named MACS0647-JD, is very young and only a tiny fraction of the size of our Milky Way Photo: Nasa

By , Science Correspondent

11:58AM GMT 16 Nov 2012

Light from the newly discovered galaxy, which astronomers have named MACS0647-JD, reached Earth after travelling across space for 13.3 billion years.

It provides a window on what the galaxy looked like just 420 million years after the big bang, when the universe was only three per cent of its current age.

The galaxy was detected using an effect known as gravitational lensing, where large clusters of galaxies are used as “natural zoom lenses” to enlarge the appearance of galaxies behind them.

Astronomers were able to detect a hint of light from MACS0647-JD because it was magnified as it passed around an enormous galaxy cluster known as MACS J0647+7015 as it travelled towards Earth.

Thanks to the gravitational force of the cluster, the Hubble telescope was able to detect the light at up to eight times the brightness it otherwise would.

Read more: http://www.telegraph.co.uk/science/space/9682959/NASA-locates-most-distant-galaxy-ever-discovered.html

 

Gravitational lens magnifies earliest galaxy yet seen

November 17, 2012 Leave a comment

by  – Nov 17 2012, 8:45pm GTBST

Small galaxy was producing stars only 425 million years after the Big Bang.

 

The contours of the gravitational lens (colored lines) along with the three images of the distant background galaxy (JD1-3).

The Universe’s first galaxies played a key role in shaping the environment in which we now find ourselves. They fostered the formation of the first stars, which died in spectacular explosions that enabled a new generation of smaller stars, orbited by rockier planets. And the galaxies themselves merged and grew, forming the large galaxies and clusters that populate the Universe today. But, despite their critical role in shaping the Universe, we’ve never actually been able to see one of them.

Slowly, that’s changing. The Hubble Deep Field exposures have helped us spot galaxies from the Universe’s early days. But now, a special Hubble project has used an intervening cluster of galaxies as a lens to spot what appears to be the most distant galaxy ever imaged, one that dates from just 425 million years after the Big Bang.

Since it takes light time to reach us from distant corners of the Universe, the further you look, the older the objects you see. The wavelength of the light also gets shifted towards the red by the expansion of the Universe, which stretches it out as it travels. As you get closer to the Big Bang, light that started out in the UV end of the spectrum gets pushed deeper and deeper into the infrared. To make these galaxies even harder to spot, the extreme distance means that very few photons actually make their way to Earth, so these objects are incredibly dim.

Read more: http://arstechnica.com/science/2012/11/gravitational-lens-magnifies-earliest-galaxy-yet-seen/