Written by Whitney Clavin
NASA’s Jet Propulsion Laboratory
Pasadena, CA – Astronomers have spotted the “greenest” of galaxies, one that converts fuel into stars with almost 100-percent efficiency.
The findings come from NASA’s Wide-field Infrared Survey Explorer (WISE), NASA’s Hubble Space Telescope and the IRAM Plateau de Bure interferometer in the French Alps.
“This galaxy is remarkably efficient,” said Jim Geach of McGill University in Canada, lead author of a new study appearing in the Astrophysical Journal Letters. “It’s converting its gas supply into new stars at the maximum rate thought possible.”
 The tiny red spot in this image is one of the most efficient star-making galaxies ever observed, converting gas into stars at the maximum possible rate. (Image credit: NASA/JPL-Caltech/STScI/IRAM)
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NASA reports Herschel Space Telescope completes mission
May 1, 2013 |
Written by Whitney Clavin
NASA’s Jet Propulsion Laboratory
Pasadena, CA – The Herschel observatory, a European space telescope for which NASA helped build instruments and process data, has stopped making observations after running out of liquid coolant as expected.
The European Space Agency mission, launched almost four years ago, revealed the universe’s “coolest” secrets by observing the frigid side of planet, star and galaxy formation.
 Herschel spacecraft artist’s concept. (Copyright ESA/AOES Medialab)
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NASA Astronomers using Herschel Space Observatory discover oldest star producing Galaxy to date
April 18, 2013 |
Written by Whitney Clavin
NASA’s Jet Propulsion Laboratory
Pasadena, CA – Astronomers, including Matt Bradford, Jamie Bock, Darren Dowell, Hien Nguyen and Jonas Zmuidzinas of NASA’s Jet Propulsion Laboratory, Pasadena, CA, have discovered a dust-filled, massive galaxy churning out stars when the cosmos was a mere 880 million years old. This is the earliest starburst galaxy ever observed.
The discovery, appearing in the April 18th issue of Nature, was made using the European Space Agency’s Herschel space observatory, for which JPL helped build two instruments.
 This artist’s impression shows the “starburst” galaxy HFLS3. The galaxy appears as little more than a faint, red smudge in images from the Herschel space observatory. (Image credit: ESA-C. Carreau)
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NASA reports astronomers use Suzaku Satellite to gain better understanding of Supernovas
April 10, 2013 |
Written by Francis Reddy
NASA’s Goddard Space Flight Center
Greenbelt, MD – An exploding star observed in 1604 by the German astronomer Johannes Kepler held a greater fraction of heavy elements than the sun, according to an analysis of X-ray observations from the Japan-led Suzaku satellite.
The findings will help astronomers better understand the diversity of type Ia supernovae, an important class of stellar explosion used in probing the distant universe.
 This composite of images from NASA’s Chandra X-ray Observatory shows the remnant of Kepler’s supernova in low (red), intermediate (green) and high-energy (blue) X-rays. The background is an optical star field taken from the Digitized Sky Survey. The distance to the object is uncertain, with estimates ranging from 13,000 to 23,000 light-years, but recent studies favor the maximum range. This image spans 12 arcminutes or about 80 light-years at the greatest distance. *Credit: X-ray: NASA/CXC/NCSU/M.Burkey et al.; optical: DSS)
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NASA’s Kepler space telescope discovers White Dwarf bending light of nearby Star
April 7, 2013 |
Written by Whitney Clavin
NASA’s Jet Propulsion Laboratory
Pasadena, CA – NASA’s Kepler space telescope has witnessed the effects of a dead star bending the light of its companion star. The findings are among the first detections of this phenomenon — a result of Einstein’s general theory of relativity — in binary, or double, star systems.
The dead star, called a white dwarf, is the burnt-out core of what used to be a star like our sun. It is locked in an orbiting dance with its partner, a small “red dwarf” star. While the tiny white dwarf is physically smaller than the red dwarf, it is more massive.
 This artist’s concept depicts a dense, dead star called a white dwarf crossing in front of a small, red star. The white dwarf’s gravity is so great it bends and magnifies light from the red star. (Image credit: NASA/JPL-Caltech)
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NASA Hubble Space Telescope sees Glow Worm like Galaxy
March 24, 2013 |
NASA’s Goddard Space Flight Center
Greenbelt, MD – This charming and bright galaxy, known as IRAS 23436+5257, was captured by the NASA/ESA Hubble Space Telescope. It is located in the northern constellation of Cassiopeia, which is named after an arrogant, vain, and yet beautiful mythical queen.
The twisted, wormlike structure of this galaxy is most likely the result of a collision and subsequent merger of two galaxies.
 Galaxy IRAS 23436+5257. (Credit: ESA/Hubble and NASA, Acknowledgement: Judy Schmidt)
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NASA’s Nuclear Spectroscopic Telescope Array (NuSTAR) helps scientists measure the spin rate of a Black Hole
March 4, 2013 |
Written by Whitney Clavin
NASA’s Jet Propulsion Laboratory
Pasadena, CA – Two X-ray space observatories, NASA’s Nuclear Spectroscopic Telescope Array (NuSTAR) and the European Space Agency’s XMM-Newton, have teamed up to measure definitively, for the first time, the spin rate of a black hole with a mass 2 million times that of our sun.
The supermassive black hole lies at the dust- and gas-filled heart of a galaxy called NGC 1365, and it is spinning almost as fast as Einstein’s theory of gravity will allow. The findings, which appear in a new study in the journal Nature, resolve a long-standing debate about similar measurements in other black holes and will lead to a better understanding of how black holes and galaxies evolve.
 This artist’s concept illustrates a supermassive black hole with millions to billions times the mass of our sun. Supermassive black holes are enormously dense objects buried at the hearts of galaxies. (Image credit: NASA/JPL-Caltech)
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NASA’s Kepler Space Telescope data shows possibility of Earth Size planet just 13 light years from Earth
February 8, 2013 |
Written by Whitney Clavin
NASA’s Jet Propulsion Laboratory
Pasadena, CA – Using publicly available data from NASA’s Kepler space telescope, astronomers at the Harvard-Smithsonian Center for Astrophysics estimate that six percent of red dwarf stars in the galaxy have Earth-size planets in the “habitable zone,” the range of distances from a star where the surface temperature of an orbiting planet might be suitable for liquid water.
The majority of the sun’s closest stellar neighbors are red dwarfs. Researchers now believe that an Earth-size planet with a moderate temperature may be just 13 light-years away.
 Astronomers estimate that six percent of red dwarfs have a temperate Earth-size planet, as close as 13 light-years away. (Image credit: D. Aguilar/Harvard-Smithsonian Center for Astrophysics)
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NASA’s Hubble Space Telescope proves that everything is not as it appears
January 28, 2013 |
NASA’s Goddard Space Flight Center
Greenbelt, MD – Globular clusters are roughly spherical collections of extremely old stars, and around 150 of them are scattered around our galaxy. Hubble is one of the best telescopes for studying these, as its extremely high resolution lets astronomers see individual stars, even in the crowded core.
The clusters all look very similar, and in Hubble’s images it can be quite hard to tell them apart – and they all look much like NGC 411, pictured below.
 Open cluster NGC 411 located in the Small Magellanic Cloud. (Photo credit ESA/Hubble & NASA)
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Herschel Space Observatory image reveals Betelgeuse Star headed for collision with Strange Bar of Matter
January 27, 2013 |
Written by Whitney Clavin
NASA’s Jet Propulsion Laboratory
Pasadena, CA – Orion, the famous hunter presiding over northern winter skies, may experience a stellar crash in its future. The red star at its shoulder, called Betelgeuse, appears to be set to collide with a dusty “wall” in 5,000 years.
A new image from the Herschel Space Observatory, a European Space Agency mission with important NASA participation, reveals the shedding, aging star — called Betelgeuse – is located near an odd, linear bar of material.
 The red supergiant star Betelgeuse is seen here in a new view from the Herschel Space Observatory, a European Space Agency mission with important NASA participation. (Image credit: ESA/Herschel/PACS/L. Decin et al)
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