Using an analysis of the chemical composition of Venus's atmosphere, the team inferred that the planet's interior lacks the moisture necessary to sustain oceans. This discovery challenges theories of a once temperate Venus and suggests its surface has always been unfit for Earth-like life.
The findings, published in Nature Astronomy, have significant implications for understanding Earth's unique habitability and refining the search for life on exoplanets. The study suggests astronomers should prioritize Earth-like planets over Venus-like ones in their search for habitable worlds.
"Venus and Earth may appear similar from a distance," said lead researcher Tereza Constantinou, a PhD candidate at Cambridge's Institute of Astronomy. "However, Venus's surface, with its intense heat and sulfuric acid clouds, tells a very different story. If Venus never had oceans, it's hard to imagine it ever supporting life like that on Earth."
"Venus provides a critical reference point for defining the habitable zone in planetary systems," Constantinou explained. "It's an invaluable example of how a rocky planet can evolve differently, even within a similar proximity to its star."
Two dominant theories have shaped debates about Venus's past. One posits that Venus was once temperate and water-rich but experienced a runaway greenhouse effect due to extensive volcanism. The other suggests Venus has always been too hot for water to condense, rendering it uninhabitable from its formation 4.6 billion years ago.
Volcanism, which releases gases into the atmosphere during eruptions, serves as a window into the planet's interior. On Earth, volcanic eruptions are steam-rich due to our water-abundant interior. On Venus, however, volcanic gases are only about six percent water, reflecting a dehydrated planetary interior.
"This data suggests Venus has been dry for most, if not all, of its existence," Constantinou noted. "The volcanic gases necessary to sustain the atmosphere don't indicate any significant water content in the interior."
"If Venus has always been dry, it diminishes the chances of Venus-like exoplanets being habitable," Constantinou said. "We must focus our efforts on Earth-like planets, as instruments like the James Webb Space Telescope are optimized for studying planets closer to their stars, such as Venus."
While the findings may be disappointing for those hoping Venus once resembled Earth, they offer a clearer pathway for identifying habitable planets in the galaxy. "It's a bittersweet realization," Constantinou added. "But refining our understanding helps us better target our search for life elsewhere in the universe."
Research Report:A dry Venusian interior constrained by atmospheric chemistry
Related Links
University of Cambridge
Venus Express News and Venusian Science
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