Category Astronomy/Space

New Model explains what we see when a Massive Black Hole Devours a Star

Illustration of emissions from a tidal disruption event shows in cross section what happens when the material from a disrupted star is devoured by a black hole. The material forms an accretion disk, which heats up and emits vast amounts of light and radiation. The emissions we are able to see from Earth depend on our viewing angle with respect to the orientation of the black hole. Credit: Illustration by Jane Lixin Dai

Illustration of emissions from a tidal disruption event shows in cross section what happens when the material from a disrupted star is devoured by a black hole. The material forms an accretion disk, which heats up and emits vast amounts of light and radiation. The emissions we are able to see from Earth depend on our viewing angle with respect to the orientation of the black hole. Credit: Illustration by Jane Lixin Dai

A star that wanders too close to the supermassive black hole in the center of its galaxy will be torn apart by the black hole’s gravity in a violent cataclysm called a tidal disruption event (TDE), producing a bright flare of radiation...

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EOVSA reveals new insights into Solar Flares’ Explosive Energy Releases

This is a EOVSA radio intensity spectrogram of the 2017 September 10 solar flare, with frequency (vertical scale) and time (horizontal scale). Credit: New Jersey Institute of Technology's expanded Owens Valley Solar Array

This is a EOVSA radio intensity spectrogram of the 2017 September 10 solar flare, with frequency (vertical scale) and time (horizontal scale). Credit: New Jersey Institute of Technology’s expanded Owens Valley Solar Array

Last September, a massive new region of magnetic field erupted on the Sun’s surface next to an existing sunspot. The powerful collision of magnetic fields produced a series of potent solar flares, causing turbulent space weather conditions at Earth. These were the first flares to be captured, in their moment-by-moment progression, by New Jersey Institute of Technology’s (NJIT) recently expanded Owens Valley Solar Array (EOVSA).

With 13 antennas now working together, EOVSA was able to make images of the flare in multiple radio frequencies simultaneously for the first time...

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Mars Rocks may Harbor signs of Life from 4 billion years ago

The Jezero Crater delta, a well-preserved ancient river delta on Mars. Credit: NASA/JPL-Caltech/MSSS/JHU-APL

The Jezero Crater delta, a well-preserved ancient river delta on Mars. Credit: NASA/JPL-Caltech/MSSS/JHU-APL

Iron-rich rocks near ancient lake sites on Mars could hold vital clues that show life once existed there, research suggests. These rocks – which formed in lake beds – are the best place to seek fossil evidence of life from billions of years ago, researchers say. A new study that sheds light on where fossils might be preserved could aid the search for traces of microbes — on Mars, which it is thought may have supported primitive life forms around four billion years ago.

A team of scientists has determined that sedimentary rocks made of compacted mud or clay are the most likely to contain fossils. These rocks are rich in iron and a mineral called silica, which helps preserve fossils...

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Scientists introduce Cosmochemical Model for Pluto Formation

Ralph Instrument Pluto Maps. New Horizons not only showed humanity what Pluto looks like, but also provided information on the composition of Pluto’s atmosphere and surface. These maps — assembled using data from the Ralph instrument — indicate regions rich in methane (CH4), nitrogen (N2), carbon monoxide (CO) and water (H2O) ices. Sputnik Planitia shows an especially strong signature of nitrogen near the equator. SwRI scientists combined these data with Rosetta’s comet 67P data to develop a proposed “giant comet” model for Pluto formation. Credit: Image Courtesy of NASA/Johns Hopkins University Applied Physics Laboratory/Southwest Research Institute

Ralph Instrument Pluto Maps. New Horizons not only showed humanity what Pluto looks like, but also provided information on the composition of Pluto’s atmosphere and surface. These maps — assembled using data from the Ralph instrument — indicate regions rich in methane (CH4), nitrogen (N2), carbon monoxide (CO) and water (H2O) ices. Sputnik Planitia shows an especially strong signature of nitrogen near the equator. SwRI scientists combined these data with Rosetta’s comet 67P data to develop a proposed “giant comet” model for Pluto formation. Credit: Image Courtesy of NASA/Johns Hopkins University Applied Physics Laboratory/Southwest Research Institute

New Horizons, Rosetta data fusion points to new theory...

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