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Earth’s ‘Evil Twin’ Venus May Have Been More Like Us Than We Thought

Earth’s ‘Evil Twin’ Venus May Have Been More Like Us Than We Thought

August 8, 2024
This six-panel illustration of a tidal disruption event around a supermassive black hole shows the following: 1) A supermassive black hole is adrift inside a galaxy, its presence only detectable by gravitational lensing; 2) A wayward star gets swept up in the black hole's intense gravitational pull; 3) The star is stretched or "spaghettified" by gravitational tidal effects; 4) The star's remnants form a disk around the black hole; 5) There is a period of black hole accretion, pouring out radiation across the electromagnetic spectrum, from X-rays to radio wavelengths; and 6) The host galaxy, seen from afar, contains a bright flash of energy that is offset from the galaxy's nucleus, where an even more massive black hole dwells. Credit: NASA, ESA, STScI, Ralf Crawford (STScI)

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Earth’s ‘Evil Twin’ Venus May Have Been More Like Us Than We Thought

by nasaspacenews
August 8, 2024
in News, Others, Solar System
0
Earth’s ‘Evil Twin’ Venus May Have Been More Like Us Than We Thought

The Earth seen from Apollo 17.jpg Venus globe.jpg Earth image: NASA/Apollo 17 crew Venus image: NASA

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 Earth’s ‘Evil Twin’ Venus May Have Mirrored Our Planet More Than Expected

Venus, often referred to as Earth’s “evil twin” due to its hostile environment, has revealed new secrets that bring it closer to our home planet than previously thought. Recent research led by Fabio Capitanio from Monash University has uncovered that Venus’s surface features, particularly the tesserae plateaus, share striking similarities with Earth’s early continents.
The study focuses on tesserae, large plateau regions on Venus that exhibit complex geological formations, including faults, folds, and volcanic features. These structures are analogous to Earth’s ancient cratons, ancient cores of continents.
Tesserae were found to have formed through intense tectonic activity similar to the processes that shaped Earth’s earliest continents. 

Some of Campbell’s research relies on earth-based observatories. Using the radio telescope in Arecibo, Puerto Rico, Campbell and his team made this radar image of Venus, which shows a web of tesserae–unusual landforms–in the Alpha Regio region. (Bruce Campbell/CEPS)

Currently, Venus has a stagnant lithosphere, meaning its surface is a single plate with minimal movement. Unlike Earth, which has active plate tectonics driving the movement of multiple plates, Venus’s tectonic activity is largely in the past. However, the discovery of tesserae suggests that Venus may have transitioned from a tectonically active state to its current stagnant lid model.

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The research opens new avenues for future missions to Venus, such as DAVINCI, VERITAS, and EnVision. These missions aim to delve deeper into Venus’s geological past and its connection to Earth.

Monash University – Research led by Fabio Capitanio from the Monash University School of Earth, Atmosphere and Environment. The findings were detailed in a study published in Nature Geoscience.

  • Monash University article

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This six-panel illustration of a tidal disruption event around a supermassive black hole shows the following: 1) A supermassive black hole is adrift inside a galaxy, its presence only detectable by gravitational lensing; 2) A wayward star gets swept up in the black hole's intense gravitational pull; 3) The star is stretched or "spaghettified" by gravitational tidal effects; 4) The star's remnants form a disk around the black hole; 5) There is a period of black hole accretion, pouring out radiation across the electromagnetic spectrum, from X-rays to radio wavelengths; and 6) The host galaxy, seen from afar, contains a bright flash of energy that is offset from the galaxy's nucleus, where an even more massive black hole dwells. Credit: NASA, ESA, STScI, Ralf Crawford (STScI)

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