Category Astronomy/Space

NASA’s Fermi finds record-breaking Binary in galaxy next door

LMC P3 (circled) is located in a supernova remnant called DEM L241 in the Large Magellanic Cloud, a small galaxy about 163,000 light-years away. The system is the first gamma-ray binary discovered in another galaxy and is the most luminous known in gamma rays, X-rays, radio waves and visible light. Unlabeled image Credit: NOAO/CTIO/MCELS, DSS

LMC P3 (circled) is located in a supernova remnant called DEM L241 in the Large Magellanic Cloud, a small galaxy about 163,000 light-years away. The system is the first gamma-ray binary discovered in another galaxy and is the most luminous known in gamma rays, X-rays, radio waves and visible light. Unlabeled image Credit: NOAO/CTIO/MCELS, DSS

Using data from NASA’s Fermi Gamma-ray Space Telescope and other facilities, an international team has found the first gamma-ray binary in another galaxy and the most luminous one ever seen. The dual-star system, dubbed LMC P3, contains a massive star and a crushed stellar core that interact to produce a cyclic flood of gamma rays, the highest-energy form of light...

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NASA’s Curiosity finds Chemistry of Mars Crust contributing to Atmosphere over time

Processes in Mars' surface material can explain why particular xenon (Xe) and krypton (Kr) isotopes are more abundant in the Martian atmosphere than expected, as measured by NASA's Curiosity rover. Cosmic rays striking barium (Ba) or bromine (Br) atoms can alter isotopic ratios of xenon and krypton. Credit: NASA/GSFC/JPL-Caltech

Processes in Mars’ surface material can explain why particular xenon (Xe) and krypton (Kr) isotopes are more abundant in the Martian atmosphere than expected, as measured by NASA’s Curiosity rover. Cosmic rays striking barium (Ba) or bromine (Br) atoms can alter isotopic ratios of xenon and krypton. Credit: NASA/GSFC/JPL-Caltech

It’s another clue that the history of the Red Planet’s atmosphere is more complex and interesting than a simple legacy of loss. The chemistry findings come from the rover’s Sample Analysis at Mars, or SAM, instrument suite, which studied the gases xenon and krypton in Mars’ atmosphere. The two gases can be used as tracers to help scientists investigate the evolution and erosion of the Martian atmosphere...

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Discovery of an Extragalactic Hot Molecular Core

Discovery of an extragalactic hot molecular core

Artist’s concept image of the hot molecular core discovered in the Large Magellanic Cloud. Credit: FRIS/Tohoku University. The figure is a derivative work of the following sources (ESO/M. Kornmesser; NASA, ESA, and S. Beckwith (STScI) and the HUDF Team; NASA/ESA and the Hubble Heritage Team (AURA/STScI)/HEI

Astronomers have discovered a ‘hot molecular core’, a cocoon of molecules surrounding a newborn massive star, for the first time outside our Galaxy. The discovery marks the first important step for observational studies of extragalactic hot molecular cores and challenges the hidden chemical diversity of our universe...

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A Perfect Sun-Storm solves a mystery

Visualization of Earth's magnetic environment, with the magnetic field as a protective shield, generated by the strong internal magnetic field in Earth's core (for more see the end of the press release). Credit: Martin Rother/GFZ

Visualization of Earth’s magnetic environment, with the magnetic field as a protective shield, generated by the strong internal magnetic field in Earth’s core.. Credit: Martin Rother/GFZ

A geomagnetic storm on 1/17/13, provided unique observations that finally resolved a long-standing scientific problem. For decades, scientists had asked how particles hitting Earth’s magnetosphere were lost. A likely mechanism involved certain electromagnetic waves scattering particles into Earth’s atmosphere. More recently, another mechanism was proposed that caused particles to be lost in interplanetary space...

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