Category Astronomy/Space

Why the Solar Wind is Hotter than Expected

A mirror machine is a linear fusion reactor. It allows scientists to apply research in the machines to an understanding of solar wind phenomena. COURTESY OF CARY FOREST

When the sun expels plasma, the solar wind cools as it expands through space – but not as much as the laws of physics would predict. Physicists now know the reason. University of Wisconsin-Madison physicists provide an explanation for the discrepancy in solar wind temperature. Their findings suggest ways to study solar wind phenomena in research labs and learn about solar wind properties in other star systems.

“People have been studying the solar wind since its discovery in 1959, but there are many important properties of this plasma which are still not well understood,” says Stas Boldyrev, professor of physics and lea...

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Astronomers detect Most Energetic Outflow from a Distant Quasar

noirlab2009a. The image at left shows an artist’s conception of the central portion of the galaxy that hosts the quasar SDSS J135246.37+423923.5 viewed at optical wavelengths. Thick winds obscure our view, and imprint signatures of the energetic outflow on the SDSS spectrum. The image at right shows the same artist’s view at infrared wavelengths, as seen by the Gemini GNIRS detector. The thick outflow is transparent at infrared wavelengths, giving us a clear line of sight to the quasar. The infrared spectrum yields the quasar redshift, and from that reference frame, we measured the record-breaking outflow velocity. Credit: International Gemini Observatory/NOIRLab/NSF/AURA/P. Marenfeld

Researchers using the Gemini North telescope on Hawai’i’s Maunakea have detected the most energeti...

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NASA missions help reveal the power of Shock waves in a Nova Explosion

V906 Carinae (circled) shines near peak brightness in this image taken on March 23, 2018, three days after the nova was discovered. The beautiful cloud of gas and dust dominating the picture is part of the Carina Nebula.
Credits: Copyright 2018 by A. Maury and J. Fabrega, used with permission

Unprecedented observations of a nova outburst in 2018 by a trio of satellites, including two NASA missions, have captured the first direct evidence that most of the explosion’s visible light arose from shock waves — abrupt changes of pressure and temperature formed in the explosion debris.

A nova is a sudden, short-lived brightening of an otherwise inconspicuous star...

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Scientists discover Supernova that Outshines all others

Artist’s impression of a supernova. Credit: Aaron Geller (Northwestern University)

A supernova at least twice as bright and energetic, and likely much more massive than any yet recorded has been identified by an international team of astronomers, led by the University of Birmingham.

The team, which included experts from Harvard, Northwestern University and Ohio University, believe the supernova, dubbed SN2016aps, could be an example of an extremely rare ‘pulsational pair-instability’ supernova, possibly formed from two massive stars that merged before the explosion. Their findings are published today in Nature Astronomy.

Such an event so far only exists in theory and has never been confirmed through astronomical observations.

Dr...

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