There is something shifty about plate tectonics

“Across the lansdcape, steam vents hiss gaseous breath from deep inside the planet, creating an environment that feels like it hangs in the balance between our world and another.”
― Stefanie Payne, A Year in the National Parks: The Greatest American Road Trip

The team designed models of geological activity beneath the surface of Venus. These 3D models of showed the formation of coronae formation identified features that could only be produced by recent volcanic activity on the surface of Venus. This finding provides the first evidence that the surface of Venus is still active, betraying active geology beneath the crust.

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A global map of Venus showing both active (red) and inactive (white) coronae. Image credit: Anna Gülcher

“I focus on the lithosphere and surface geology, which is relatively accessible to planetary missions data. I like to call this kind of work comparative planetology. Venus is of special interest because of its gross similarity to the Earth. Yet the geology we observe is very different from that of the Earth. It has volcanoes and faults, yes, but they are organized very differently from the Earth. It does not have global tectonics like we do (at least at present day),” Montési tells The Cosmic Companion.

Without plate tectonics, movement of hot material through the planetary surface is the dominant force driving geological change on Venus today.

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In the video above, you can take look at the planned EnVision mission to Venus, scheduled for launch in 2032. (Video credit: Thomas Widemann)

The surface of Venus was likely reworked on a large scale by volcanoes between 500 and 300 million years ago. Eruptions there have some similarities, as well as some differences to geological activity here on Earth.

“Volcanoes on Venus actually look a lot like those on Earth: they have similar slope, activity on the summit etc. However, there are many regions of Venus that are covered with lava flows without necessarily a clear source. We see that in a few places on Earth, in regions called flood basalt provinces or traps. In our study we focused on very unusual structures called coronae, which do not have a good equivalent in terrestrial geology. They have a ring of faults and lava flow, and their interior can be quite complex, maybe have volcanic edifices, but these are not very well documented yet,” Montési describes.

This finding could assist teams heading future missions to Venus, including Europe’s EnVision mission, scheduled for launch in 2032.

This article was originally published on The Cosmic Companion by James Maynard, founder and publisher of The Cosmic Companion. He is a New England native turned desert rat in Tucson, where he lives with his lovely wife, Nicole, and Max the Cat. You can read this original piece here.

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