Crustal Block Tectonics Offer Clues to Venus’ Geology, Study Finds
- Study identifies previously unrecognized pattern of tectonic deformation on Venus.
- Baylor University planetary physicist Peter James, Ph.D., provided calculations of the various mechanisms that could be responsible for the force driving the geologic activity on Venus. (Robert Rogers/Baylor University)
New study that includes contributions by Baylor planetary geophysicist Peter James, identifies previously unrecognized pattern of tectonic deformation on Venus
WACO, Texas (June 21, 2021) – A new analysis of Venus’ surface shows evidence of tectonic motion in the form of crustal blocks that have jostled against each other like broken chunks of pack ice. Published in PNAS (Proceedings of the National Academy of Sciences), the study — which includes contributions by Baylor University planetary physicist Peter James, Ph.D. — found that the movement of these blocks could indicate that Venus is still geologically active and give scientists insight into both exoplanet tectonics and the earliest tectonic activity on Earth.
“We have identified a previously unrecognized pattern of tectonic deformation on Venus, one that is driven by interior motion just like on Earth,” said Paul Byrne, Ph.D., associate professor of planetary science at North Carolina State University and lead and co-corresponding author of the work. “Although different from the tectonics we currently see on Earth, it is still evidence of interior motion being expressed at the planet’s surface.”
Venus had long been assumed to have an immobile solid outer shell, or lithosphere, just like Mars or Earth’s moon. In contrast, Earth’s lithosphere is broken into tectonic plates, which slide against, apart from, and underneath each other on top of a hot, weaker mantle layer.
James, an assistant professor of planetary geophysics and founder of Baylor University’s Planetary Research Group, was part of the international group of researchers involved with the study. He has taken part in three NASA missions and specializes in using spacecraft data to study the crusts and mantles of planets and moons.
“Earth is the only planet in the solar system with plate tectonics, so our planet is quite exceptional in that regard,” James said. “That is particularly interesting when it comes to Venus: Why does a planet like Venus — roughly the same size as Earth and made of the same types of rocks — not behave the same way as Earth geologically?”
To answer that question, the team used radar images from NASA’s Magellan mission to map the surface of Venus. In examining the extensive Venusian lowlands that make up most of the planet surface, they saw areas where large blocks of the lithosphere seem to have moved: pulling apart, pushing together, rotating and sliding past each other like broken pack ice over a frozen lake.
James provided calculations of the various mechanisms that could be responsible for the force driving the geologic activity on Venus. NASA’s Magellan spacecraft measured the gravity field of Venus — the subtle changes in the strength of gravity in different places on the planet. James was able to use this gravity field to demonstrate that viscous mantle flow, or slow churning, is strongly coupled to the crust.
“The mantle inside Venus pushes and pulls on the surface of the planet more strongly than Earth’s mantle does. These calculations of the driving forces corroborated the discovery of block motion and helped us have a better understanding of how it works,” James said.
The interior mantle flow found by the study’s calculations is significant because it hasn’t been demonstrated on a global scale previously. The movement of these crustal blocks could also indicate that Venus is still geologically active.
“We know that much of Venus has been volcanically resurfaced over time, so some parts of the planet might be really young, geologically speaking,” Byrne said. “But several of the jostling blocks have formed in and deformed these young lava plains, which means that the lithosphere fragmented after those plains were laid down. This gives us reason to think that some of these blocks may have moved geologically very recently – perhaps even up to today.”
The researchers are optimistic that Venus’ newly recognized “pack ice” pattern could offer clues to understanding tectonic deformation on planets outside of our solar system, as well as on a much younger Earth.
“One of the neat things about planet research like this is that it helps us understand why our own planet works the way it does,” James said. “The theme of our Planetary Research Group at Baylor is a quote from C.S. Lewis’s Mere Christianity: ‘Aim at heaven and you will get Earth thrown in.’ That quote is intended in a spiritual context — we should seek the kingdom of God before all else, and then this kingdom-mindset can even bear fruit in a secular sense. We like the double meaning of using space research to understand our own planet better.”
Science related to Venus is especially timely — NASA recently announced that it would be sending two new spacecrafts to Venus, VERITAS and DAVINCI+. These will be the first NASA missions launched to Venus since the 1980s. Additionally, the European Space Agency announced last week that it would be sending its own spacecraft called Envision to Venus.
“Strategically, this research is positioning Baylor to be involved with upcoming spacecraft missions. Venus is becoming a bigger priority for space agencies around the world, and we’re plugged in to the exciting science opportunities that are on the horizon,” James said.
Baylor will continue to be part of Venus research through James’ lab. Rudger Dame, a Ph.D. candidate in James’ lab, is focusing on Venus for his dissertation research. He has an internship this summer with the NASA Jet Propulsion Laboratory, under the advisement of Sue Smrekar, the principal investigator for the recently announced VERITAS spacecraft.
In addition, James is collaborating with NASA’s Goddard Space Flight Center to study the planet Mercury’s crust. He also led a recent study published in the journal Geophysical Research Letters about the discovery of a mysterious huge mass of material on the far side of the Moon — beneath the largest crater in our solar system. The mass — at least five times larger than the Big Island of Hawaii — may contain metal from an asteroid that may have crashed into the Moon and formed the crater.
The South Pole-Aitken basin — thought to have been created about 4 billion years ago — is “one of the best natural laboratories for studying catastrophic impact events, an ancient process that shaped all of the rocky planets and moons we see today.”
*Sean Solomon of Columbia University is co-corresponding author. Richard Ghail of the University of London, Surrey; A. M. Celâl Şengör of Istanbul Technical University; and Christian Klimczak of the University of Georgia also contributed to the work.
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