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Venus

Plot showing evolution of crustal thickness over time for mantle convection models of Venus with different yield strength
Posted inEditors' Highlights

What Happened When the Lithosphere of Venus Broke?

by Laurent G. J. Montési 5 January 202115 March 2022

Although Venus does not have plate tectonics today, previous episodes of intense tectonic activity could have resulted in a distribution of crustal thickness and age resembling the plate we see today.

Venus's clouds as seen by Mariner 10 in 1974
Posted inNews

¿Podría la Vida Estar Flotando en las Nubes de Venus?

Kimberly M. S. Cartier, News Writing and Production Intern for Eos.org by Kimberly M. S. Cartier 14 October 20208 September 2022

Si están presentes, los microbios podrían explicar patrones de evolución en la atmósfera planetaria de Venus, al observarse con luz ultravioleta.

GEER scientists examine geologic samples in the GEER chamber after a test
Posted inNews

Venus Exploration Starts in the Lab

Kimberly M. S. Cartier, News Writing and Production Intern for Eos.org by Kimberly M. S. Cartier 28 May 202022 November 2021

Most technology would not last a day on our planet’s evil twin. By creating Venus’s surface and atmospheric conditions here on Earth, a team of engineers is designing spacecraft technology that will last for months.

Diagram of Venus’s possible climate history
Posted inResearch Spotlights

How Long Was Venus Habitable?

Kate Wheeling, freelance science writer by Kate Wheeling 8 May 202010 November 2021

Climate simulations of Venus’s history could provide insights into the habitability of Earth and of exoplanets.

Illustration of an erupting volcano on Venus
Posted inFeatures

Resurrecting Interest in a “Dead” Planet

Damond Benningfield, Science Writer by Damond Benningfield 11 July 201917 January 2023

New research suggests that the surface of Venus is busy, but it may take new missions to our “sibling” planet to confirm this.

A false-color image of Venus’s atmosphere
Posted inResearch Spotlights

New Analysis Provides a Fresh View of the Atmosphere on Venus

Aaron Sidder, freelance science writer by Aaron Sidder 17 January 20195 January 2022

Researchers apply a radio holographic method to standard Venusian atmospheric data, resulting in outputs with finer vertical resolution and revealing small-scale atmospheric structures.

Venus’s clouds as seen by Mariner 10 in 1974
Posted inNews

Could Life Be Floating in Venus’s Clouds?

Kimberly M. S. Cartier, News Writing and Production Intern for Eos.org by Kimberly M. S. Cartier 7 November 20188 September 2022

If present, microbes could explain evolving patterns in the planet’s atmosphere when observed in ultraviolet light.

Posted inEditors' Highlights

How Did Venus Get its Youthful Surface?

by Steven A. Hauck, II 17 May 201816 November 2021

Catastrophic lithospheric recycling is unlikely to be the cause of Venus’s young surface from mantle convection models constrained by offset between the center of mass and center of shape of planet.

Posted inEditors' Highlights

Elevated Heat Flow at Coronae on Venus

by Steven A. Hauck, II 26 February 201811 January 2022

Enigmatic surface features on Venus called coronae are important for how Venus loses heat, and measurement of surface flexing around these features indicates higher heat flows than on Earth.

Posted inEditors' Vox

Why It’s Time for a New Mission to Venus

by J. Filiberto 12 April 20177 March 2022

A packed session entitled "Unveiling Venus" at the recent Lunar and Planetary Science Conference shows renewed interest in our sister planet.

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Over a dark blue-green square appear the words Special Report: The State of the Science 1 Year On.

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