Category Astronomy/Space

Astronomers Have Found The First Evidence For Tectonic Activity on an Exoplanet

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Artist’s illustration of LHS 3844b. (University of Bern / Thibaut Roger)

That evidence is a set of advanced simulations based on observations of the rocky planet LHS 3844b, which is slightly larger than Earth. Importantly for this particular piece of research, it doesn’t look as though the exoplanet has an atmosphere.

That leaves half of LHS 3844b permanently exposed to its sun and could mean temperatures of up to roughly 800 degrees Celsius (1,472 degrees Fahrenheit) on the ‘daytime’ side, and about minus 250 degrees Celsius (minus 418 degrees Fahrenheit) on the ‘night-time’ side.”We thought that this severe temperature contrast might affect material flow in the planet’s interior,” says astronomer Tobias Meier, from the University of Bern in Switzerland.

Based on phase curve o...

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Earth has a Hot New Neighbor – and it’s an Astronomer’s Dream

Artist's impression of the rocky terrain and lava rivers on the surface of Gliese 486b
It’s getting hot in here … 430 degrees Celsius hot, that is. Artist’s interpretation: RenderArea

A rocky planet discovered in the Virgo constellation could change how we look for life in the universe. It could be our best chance yet of studying rocky planet atmospheres outside the solar system, a new international study involving UNSW Sydney shows.

The planet, called Gliese 486b (pronounced Glee-seh), is a ‘super-Earth’: that is, a rocky planet bigger than Earth but smaller than ice giants like Neptune and Uranus. It orbits a red dwarf star around 26 light-years away, making it a close neighbour — galactically speaking.

With a piping-hot surface temperature of 430 degrees Celsius, Gliese 486b is too hot to support human life...

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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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