\n<\/p>\n
Venus today is not like Earth. Temperatures hover around 860 degrees Fahrenheit day and night, and clouds of sulfuric acid float in its atmosphere.<\/p>\n
But a study published Thursday in the journal Nature Astronomy suggests that Venus in its youth may have possessed a key Earth-like trait: plate tectonics, the continual reshaping of pieces of the planet\u2019s outer crust.<\/p>\n
\u201cOne of the takeaways from this study is that both planets very likely had plate tectonics operating roughly at the same period of time,\u201d said Matthew B. Weller, a planetary scientist at the Lunar and Planetary Institute in Houston who led the research.<\/p>\n
If true, that suggests Venus could have been much more like Earth in other ways. The geochemical reactions of plate tectonics could have buried much of the carbon dioxide that makes Venus so hellish today.<\/p>\n<\/div>\n<\/div>\n
That adds fodder to the notion that a few billion years ago, Venus may have been a place where life could have thrived.<\/p>\n
\u201cThat\u2019s a very likely scenario,\u201d Dr. Weller said. \u201cIt does suggest that certainly Venus would have been cooler and then there would have been more liquid water.\u201d<\/p>\n
Dr. Weller and his colleagues at Brown University and Purdue University did not spot any San Andreas fault-like fractures or other telltale visual signs of plate tectonics. Rather, they looked at the air \u2014 nitrogen, in particular.<\/p>\n
When rocky planets like Earth and Venus form, nitrogen is locked in minerals. But in volcanic eruptions, the minerals melt and chemical bonds break, and then nitrogen can escape into the atmosphere, where it tends to stay.<\/p>\n
\u201cSo nitrogen really becomes this kind of diagnostic tool\u201d for understanding a planet\u2019s tectonic history, Dr. Weller said.<\/p>\n<\/div>\n<\/div>\n
Then the scientists set up computer simulations exploring two types of tectonic models. One was what is called the stagnant lid, which describes worlds like Mars and the Earth\u2019s moon where the outer crust consists of a solid shell, unmoving. Most of the gases remain trapped beneath the outer crust lid.<\/p>\n
The second model was plate tectonics. On Earth, about 80 percent of volcanism occurs along mid-oceanic ridges where two tectonic plates are spreading apart and magma upwells. That releases much more gas into the atmosphere.<\/p>\n<\/div>\n<\/div>\n
If Venus had always possessed a stagnant lid crust, as it appears to have now, the simulations indicated there would be less nitrogen than what is observed today \u2014 3.5 percent of the atmosphere.<\/p>\n
The explanation that worked was a combination of the two models: an early phase of plate tectonics that released bountiful carbon dioxide and nitrogen, followed by the crust locking up into a stagnant lid.<\/p>\n<\/div>\n<\/div>\n
Scientists not involved with the research said the findings were suggestive but not conclusive.<\/p>\n
C\u00e9dric Gillmann, a planetary scientist at the Swiss Federal Institute of Technology who was not involved with the research, said the paper was interesting but cautioned that \u201cas with all model-based publications, these are very dependent on what is included and what is omitted.\u201d<\/p>\n
Joseph O\u2019Rourke, a professor of earth and space exploration at Arizona State University, said that perhaps the geological history of Venus did not fit neatly with either Earth-like plate tectonics or a Mars-like stagnant lid.<\/p>\n
\u201cPerhaps Venus is its own thing that is intermediate between Earth and Mars,\u201d he said.<\/p>\n
One proposed alternative explanation is called the plutonic squishy lid model \u2014 magma intrudes the outer crust, or lithosphere, without breaking it apart into tectonic plates. That could explain circular features called coronae on the surface of Venus, pushed upward by plumes of hot material rising from the mantle.<\/p>\n
\u201cThe lithosphere is more ooey gooey and features localized breakage,\u201d Dr. O\u2019Rourke said.<\/p>\n
Dr. Weller said that in the plutonic squishy lid model, most of the magma never reaches the surface and thus might not release gushes of nitrogen.<\/p>\n
Spacecraft headed to Venus in the coming years should provide crucial new data to help resolve the mysteries. Dr. O\u2019Rourke noted that he had just been born when Magellan, NASA\u2019s last mission there, entered orbit in 1990. \u201cI was like 10 days old,\u201d he said. \u201cSo I\u2019m stoked to actually see some new Venus missions in my lifetime.\u201d<\/p>\n<\/div>\n<\/div>\n
NASA\u2019s Davinci spacecraft, tentatively scheduled to launch in 2029, will use a parachuting probe to make precise measurements of the gases in the atmosphere, providing clues to present-day volcanism.<\/p>\n
Another anticipated NASA mission, Veritas, will make detailed measurements of the planet\u2019s gravity and take high-resolution images of the surface.<\/p>\n
\u201cThat will really help us look for potential plate boundaries,\u201d said Anna G\u00fclcher, a planetary scientist at the California Institute of Technology and NASA\u2019s Jet Propulsion Laboratory.<\/p>\n
The European Space Agency is also planning to launch a robotic mission, EnVision, to help scientists understand why conditions on Earth and Venus diverged so much.<\/p>\n
Dr. Weller\u2019s computer models could also help shed light on the geological history of planets around other stars by studying what is detected in the air around them.<\/p>\n
\u201cThat was the original idea for the work,\u201d Dr. Weller said, \u201cand it quickly migrated to being able to explain something about Venus.\u201d<\/p>\n<\/div>\n<\/div>\n