Category Astronomy/Space

Astrophysicist’s 2004 Theory Confirmed: Why the Sun’s Composition Varies

The solar corona viewed in white light during the total solar eclipse on Aug. 21, 2017 from Mitchell, Oregon. The moon blocks out the central part of the Sun, allowing the tenuous outer regions to be seen in full detail. The image is courtesy of Benjamin Boe and first published in “CME-induced Thermodynamic Changes in the Corona as Inferred from Fe XI and Fe XIV Emission Observations during the 2017 August 21 Total Solar Eclipse”, Boe, Habbal, Druckmüller, Ding, Hodérova, & Štarha, Astrophysical Journal, 888, 100, (Jan. 10, 2020). (Photo by AAS)

About 17 years ago, J. Martin Laming, an astrophysicist at the U.S. Naval Research Laboratory, theorized why the chemical composition of the Sun’s tenuous outermost layer differs from that lower down...

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‘Space Hurricane’ in Earth’s Upper Atmosphere discovered

Analysis of observations made by satellites in 2014 has revealed a long-lasting ‘space hurricane’ – a swirling mass of plasma several hundred kilometers above the North Pole, raining electrons instead of water.

Hurricanes in the Earth’s low atmosphere are known, but they had never before been detected in the upper atmosphere.

An international team of scientists led by Shandong University in China analysed observations made by satellites in 2014 to reveal a long-lasting hurricane, resembling those in the lower atmosphere, in the polar ionosphere and magnetosphere with surprisingly large energy and momentum deposition despite otherwise extremely quiet geomagnetic conditions.

The analysis allowed a 3D image to be created of the 1,000km-wide swirling mass of plasma several hundre...

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Astronomers Accurately Measure the Temperature of Red Supergiant Stars

A dark background. An orange amorphous cloud.
Betelgeuse. The red supergiant appears as a red starburst between two orange clouds. © 2021 Andrew Klinger

Red supergiants are a class of star that end their lives in supernova explosions. Their lifecycles are not fully understood, partly due to difficulties in measuring their temperatures. For the first time, astronomers develop an accurate method to determine the surface temperatures of red supergiants.

Stars come in a wide range of sizes, masses and compositions. Our sun is considered a relatively small specimen, especially when compared to something like Betelgeuse which is known as a red supergiant...

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Cold Gas Pipelines Feeding Early, Massive Galaxies

Graphic illustrating detection of a cold gas accretion stream in absorption
Researchers led by the University of Iowa have detected cosmic pipelines supplying the cold gases necessary for the formation of massive galaxies and the creation of stars. It is the first direct observational evidence of the phenomenon in the early universe. Image courtesy of Hai Fu.

Researchers have detected cosmic pipelines supplying the cold gases necessary for the formation of massive galaxies and the creation of stars. It is the first direct observational evidence of the phenomenon in the early universe.

To come into being, galaxies need a steady diet of cold gases to undergo gravitational collapse. The larger the galaxy, the more cold gas it needs to coalesce and to grow.

Massive galaxies found in the early universe needed a lot of cold gas — a store totaling as much as 10...

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