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Topic: Galaxy

NASA reports discovery of Wind Nebula around Ultra-Magnetic Neutron Star

 

Written by Francis Reddy
NASA’s Goddard Space Flight Center

NASA - National Aeronautics and Space AdministrationGreenbelt, MD – Astronomers have discovered a vast cloud of high-energy particles called a wind nebula around a rare ultra-magnetic neutron star, or magnetar, for the first time. The find offers a unique window into the properties, environment and outburst history of magnetars, which are the strongest magnets in the universe.

A neutron star is the crushed core of a massive star that ran out of fuel, collapsed under its own weight, and exploded as a supernova. Each one compresses the equivalent mass of half a million Earths into a ball just 12 miles (20 kilometers) across, or about the length of New York’s Manhattan Island.

This illustration compares the size of a neutron star to Manhattan Island in New York, which is about 13 miles long. A neutron star is the crushed core left behind when a massive star explodes as a supernova and is the densest object astronomers can directly observe. (NASA's Goddard Space Flight Center)

This illustration compares the size of a neutron star to Manhattan Island in New York, which is about 13 miles long. A neutron star is the crushed core left behind when a massive star explodes as a supernova and is the densest object astronomers can directly observe. (NASA’s Goddard Space Flight Center)

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NASA’s Kepler space telescope data reveals insights into Planet Migration

 

Written by Steve Koppes
University of Chicago

NASA - National Aeronautics and Space AdministrationChicago, IL – The four planets of the Kepler-223 star system appeared to have little in common with the planets of our own solar system today. But a new study using data from NASA’s Kepler space telescope suggests a possible commonality in the distant past.

The Kepler-223 planets orbit their star in the same configuration that Jupiter, Saturn, Uranus and Neptune may have had in the early history of our solar system, before migrating to their current locations.

Sean Mills (left) and Daniel Fabrycky (right), researchers at the University of Chicago, describe the complex orbital structure of the Kepler-223 system in a new study. (Nancy Wong/University of Chicago)

Sean Mills (left) and Daniel Fabrycky (right), researchers at the University of Chicago, describe the complex orbital structure of the Kepler-223 system in a new study. (Nancy Wong/University of Chicago)

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NASA’s Kepler Space Telescope given new mission to discover exoplanets in the center of Milky Way Galaxy

 

Written by Whitney Clavin
NASA’s Jet Propulsion Laboratory

NASA - National Aeronautics and Space AdministrationPasadena, CA – Astronomers have made great strides in discovering planets outside of our solar system, termed “exoplanets.” In fact, over the past 20 years more than 5,000 exoplanets have been detected beyond the eight planets that call our solar system home.

The majority of these exoplanets have been found snuggled up to their host star completing an orbit (or year) in hours, days or weeks, while some have been found orbiting as far as Earth is to the sun, taking one Earth year to circle.

As an exoplanet passes in front of a more distant star, its gravity causes the trajectory of the starlight to bend, and in some cases, results in a brief brightening of the background star as seen by a telescope. The artistic animation illustrates this effect. This phenomenon of gravitational microlensing enables scientists to search for exoplanets that are too distant and dark to detect any other way. (NASA Ames/JPL-Caltech/T. Pyle)

As an exoplanet passes in front of a more distant star, its gravity causes the trajectory of the starlight to bend, and in some cases, results in a brief brightening of the background star as seen by a telescope. The artistic animation illustrates this effect. This phenomenon of gravitational microlensing enables scientists to search for exoplanets that are too distant and dark to detect any other way. (NASA Ames/JPL-Caltech/T. Pyle)

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NASA’s Hubble Space Telescope and Gemini Telescope discover Huge Supermassive Black Hole

 

Written by Ray Villard
Space Telescope Science Institute

NASA - National Aeronautics and Space AdministrationBaltimore, MD – Astronomers have uncovered a near-record breaking supermassive black hole, weighing 17 billion suns, in an unlikely place: in the center of a galaxy in a sparsely populated area of the universe. The observations, made by NASA’s Hubble Space Telescope and the Gemini Telescope in Hawaii, may indicate that these monster objects may be more common than once thought.

Until now, the biggest supermassive black holes – those roughly 10 billion times the mass of our sun – have been found at the cores of very large galaxies in regions of the universe packed with other large galaxies.

This computer-simulated image shows a supermassive black hole at the core of a galaxy. The black region in the center represents the black hole’s event horizon, where no light can escape the massive object’s gravitational grip. The black hole’s powerful gravity distorts space around it like a funhouse mirror. Light from background stars is stretched and smeared as the stars skim by the black hole. (NASA, ESA, and D. Coe, J. Anderson, and R. van der Marel (STScI))

This computer-simulated image shows a supermassive black hole at the core of a galaxy. The black region in the center represents the black hole’s event horizon, where no light can escape the massive object’s gravitational grip. The black hole’s powerful gravity distorts space around it like a funhouse mirror. Light from background stars is stretched and smeared as the stars skim by the black hole. (NASA, ESA, and D. Coe, J. Anderson, and R. van der Marel (STScI))

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NASA says Caltech’s CHIMERA instrument to examine Objects in Kuiper Belt

 

Written by Elizabeth Landau
NASA’s Jet Propulsion Laboratory

NASA - National Aeronautics and Space AdministrationPasadena, CA – At the Palomar Observatory near San Diego, astronomers are busy tinkering with a high-tech instrument that could discover a variety of objects both far from Earth and closer to home.

The Caltech HIgh-speed Multi-color camERA (CHIMERA) system is looking for objects in the Kuiper Belt, the band of icy bodies beyond the orbit of Neptune that includes Pluto. It can also detect near-Earth asteroids and exotic forms of stars. Scientists at NASA’s Jet Propulsion Laboratory and the California Institute of Technology, both in Pasadena, are collaborating on this instrument.

The CHIMERA instrument is located at the Hale Telescope at the Palomar Observatory near San Diego, California. (Gregg Hallinan)

The CHIMERA instrument is located at the Hale Telescope at the Palomar Observatory near San Diego, California. (Gregg Hallinan)

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NASA Scientists study Galaxy Clusters to better understand Dark Matter

 

Written by Elizabeth Landau
NASA’s Jet Propulsion Laboratory

NASA - National Aeronautics and Space AdministrationPasadena, CA – Dark matter is a mysterious cosmic phenomenon that accounts for 27 percent of all matter and energy. Though dark matter is all around us, we cannot see it or feel it. But scientists can infer the presence of dark matter by looking at how normal matter behaves around it.

Galaxy clusters, which consist of thousands of galaxies, are important for exploring dark matter because they reside in a region where such matter is much denser than average. Scientists believe that the heavier a cluster is, the more dark matter it has in its environment. But new research suggests the connection is more complicated than that.

This image from NASA's Hubble Space Telescope shows the inner region of Abell 1689, an immense cluster of galaxies. Scientists say the galaxy clusters we see today have resulted from fluctuations in the density of matter in the early universe. (NASA/ESA/JPL-Caltech/Yale/CNRS)

This image from NASA’s Hubble Space Telescope shows the inner region of Abell 1689, an immense cluster of galaxies. Scientists say the galaxy clusters we see today have resulted from fluctuations in the density of matter in the early universe. (NASA/ESA/JPL-Caltech/Yale/CNRS)

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NASA’s Wide-field Infrared Survey Explorer (WISE) observes one of the Brightest Galaxies destroying itself

 

Written by Elizabeth Landau
NASA’s Jet Propulsion Laboratory

NASA - National Aeronautics and Space AdministrationPasadena, CA – In a far-off galaxy, 12.4 billion light-years from Earth, a ravenous black hole is devouring galactic grub. Its feeding frenzy produces so much energy, it stirs up gas across its entire galaxy.

“It is like a pot of boiling water being heated up by a nuclear reactor in the center,” said Tanio Diaz-Santos of the Universidad Diego Portales in Santiago, Chile, lead author of a new study about this galaxy.

This artist's rendering shows a galaxy called W2246-0526, the most luminous galaxy known. New research suggests there is turbulent gas across its entirety, the first example of its kind. (NRAO/AUI/NSF; Dana Berry / SkyWorks; ALMA (ESO/NAOJ/NRAO))

This artist’s rendering shows a galaxy called W2246-0526, the most luminous galaxy known. New research suggests there is turbulent gas across its entirety, the first example of its kind. (NRAO/AUI/NSF; Dana Berry / SkyWorks; ALMA (ESO/NAOJ/NRAO))

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NASA Space Telescopes and Observatories study Young Galaxy Cluster in detail

 

Written by Whitney Clavin
NASA’s Jet Propulsion Laboratory

NASA - National Aeronautics and Space AdministrationPasadena, CA – Astronomers have used data from three of NASA’s Great Observatories to make the most detailed study yet of an extremely massive young galaxy cluster. This rare cluster, which is located 10 billion light-years from Earth, weighs as much as 500 trillion suns. This object has important implications for understanding how these megastructures formed and evolved early in the universe.

The galaxy cluster, called IDCS J1426.5+3508 (IDCS 1426 for short), is so far away that the light detected is from when the universe was roughly a quarter of its current age. It is the most massive galaxy cluster detected at such an early age.

Astronomers have made the most detailed study yet of an extremely massive young galaxy cluster using three of NASA's Great Observatories. (NASA/CXC/Univ of Missouri/M.Brodwin et al; NASA/STScI; JPL/CalTech)

Astronomers have made the most detailed study yet of an extremely massive young galaxy cluster using three of NASA’s Great Observatories. (NASA/CXC/Univ of Missouri/M.Brodwin et al; NASA/STScI; JPL/CalTech)

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NASA’s Spitzer and Hubble space telescopes discovers two massive stars in Eta Carinae system

 

Written by Whitney Clavin
NASA’s Jet Propulsion Laboratory

NASA - National Aeronautics and Space AdministrationPasadena, CA – Eta Carinae, the most luminous and massive stellar system within 10,000 light-years of Earth, is best known for an enormous eruption seen in the mid-19th century that hurled at least 10 times the sun’s mass into space.

This expanding veil of gas and dust , which still shrouds Eta Carinae, makes it the only object of its kind known in our galaxy. Now a study using archival data from NASA’s Spitzer and Hubble space telescopes has found five objects with similar properties in other galaxies for the first time.

Hubble view of M83 -- the only galaxy known to host two potential "Eta twins." Its high rate of star formation increases the chances of finding massive stars that have recently undergone an Eta Carinae-like outburst. Bottom: Hubble data showing the locations of M83's Eta twins. (NASA, ESA, the Hubble Heritage Team (STScI/AURA) and R. Khan (GSFC and ORAU))

Hubble view of M83 — the only galaxy known to host two potential “Eta twins.” Its high rate of star formation increases the chances of finding massive stars that have recently undergone an Eta Carinae-like outburst. Bottom: Hubble data showing the locations of M83’s Eta twins. (NASA, ESA, the Hubble Heritage Team (STScI/AURA) and R. Khan (GSFC and ORAU))

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NASA Space Telescopes observe wakes left by fast moving Stars

 

Written by Whitney Clavin
NASA’s Jet Propulsion Laboratory

NASA - National Aeronautics and Space AdministrationPasadena, CA – Astronomers are finding dozens of the fastest stars in our galaxy with the help of images from NASA’s Spitzer Space Telescope and Wide-field Infrared Survey Explorer, or WISE.

When some speedy, massive stars plow through space, they can cause material to stack up in front of them in the same way that water piles up ahead of a ship. Called bow shocks, these dramatic, arc-shaped features in space are leading researchers to uncover massive, so-called runaway stars.

Bow shocks thought to mark the paths of massive, speeding stars are highlighted in these images from NASA's Spitzer Space Telescope and Wide-field Infrared Survey Explorer, or WISE. (NASA/JPL-Caltech/University of Wyoming)

Bow shocks thought to mark the paths of massive, speeding stars are highlighted in these images from NASA’s Spitzer Space Telescope and Wide-field Infrared Survey Explorer, or WISE. (NASA/JPL-Caltech/University of Wyoming)

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