An international team of researchers has found that some of the oldest terrain on Venus, known as tesserae, has layering that seems consistent with volcanic activity. The finding could provide insights into the enigmatic planet’s geological history. Tesserae are tectonically deformed regions on the surface of Venus that are often more elevated than the surrounding landscape.
A simulated view from above Tellus Tessera, one of the regions on Venus where Byrne et al. identify the presence of layering. Image generated from NASA’s Magellan mission data. (Image: via North Carolina State University)
They comprise about 7 percent of the planet’s surface and are always the oldest feature in their immediate surroundings, dating to about 750 million years old. In a new study appearing in Geology, the researchers show that a significant portion of the tesserae have striations consistent with layering. Paul Byrne, associate professor of planetary science at North Carolina State University and lead author of the study, said:
“There are generally two explanations for tesserae — either they are made of volcanic rocks, or they are counterparts of Earth’s continental crust. But the layering we find on some of the tessera isn’t consistent with the continental crust explanation.”
The tesserae on Venus cannot be portions of continental crust
The team analyzed images of the surface of Venus from NASA’s 1989 Magellan mission, which used radar to image 98 percent of the planet through its dense atmosphere. While researchers have studied the tesserae for decades, prior to this work the layering of the tesserae hasn’t been recognized as widespread. And according to Byrne, that layering would not be possible if the tesserae were portions of continental crust. Byrne says:
“Continental crust is composed mainly of granite, an igneous rock formed when tectonic plates move and water is subducted from the surface. But granite doesn’t form layers. If there’s continental crust on Venus, then it’s below the layered rocks we see.
“Aside from volcanic activity, the other way to make layered rock is through sedimentary deposits, like sandstone or limestone. There isn’t a single place today on Venus where these kinds of rocks could form. The surface of Venus is as hot as a self-cleaning oven and the pressure is equivalent to being 900 meters (about 985 yards) underwater. So the evidence right now points to some portions of the tesserae being made up of layered volcanic rock, similar to that found on Earth.”
Byrne hopes that the work will help to shed light on more of Venus’ complicated geological history, saying:
“While the data we have now point to volcanic origins for the tesserae, if we were one day able to sample them and find that they are sedimentary rocks, then they would have had to have formed when the climate was very different — perhaps even Earth-like.
“Venus today is hellish, but we don’t know if it was always like this. Was it once like Earth but suffered catastrophic volcanic eruptions that ruined the planet? Right now we cannot say for certain, but the fact of the layering in the tesserae narrows down the potential origins of this rock.”
Provided by: Tracey Peake, North Carolina State University [Note: Materials may be edited for content and length.]
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