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In 2015, NASA's Mars Atmosphere and Volatile Evolution (MAVEN) mission provided compelling evidence that early Mars, approximately 3 billion years ago, hosted a substantial ocean of liquid water covering potentially 19% of its surface. By analyzing the ratio of deuterium to hydrogen in the Martian atmosphere, scientists determined that Mars lost a significant amount of water over its history. This finding bolsters the possibility that ancient Mars could have supported microbial life.
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Why It’s Fascinating
For decades, evidence has accumulated suggesting that Mars was once a wetter planet, but the extent and duration of this water have been subjects of intense debate. The MAVEN mission, led by principal investigator Bruce Jakosky, specifically focused on understanding how atmospheric loss has affected the planet's climate and water over time. Their findings, published in *Science* in 2015, indicated that early Mars, with its thicker atmosphere and stronger magnetic field, retained a significant volume of water, possibly forming a large ocean in the northern hemisphere. This dramatic shift from a potentially habitable, watery world to the arid planet we see today is a key puzzle in Martian science. The discovery significantly boosts the prospects for finding evidence of past life on Mars and guides future exploration efforts towards regions that were once submerged. It prompts us to consider the delicate balance required for a planet to sustain liquid water and the factors that can lead to its loss.
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