Mars is a cold and barren desert today, but scientists think that in the
ancient past it was warm and wet. The loss of the early Martian
atmosphere may have led to this dramatic change, and one of the prime
suspects is the solar wind. Unlike Earth, Mars lacks a global magnetic
field to deflect the stream of charged particles continuously blowing
off the Sun. Instead, the solar wind crashes into the Mars upper
atmosphere and can accelerate ions into space. Now, for the first time,
NASA’s MAVEN spacecraft has observed this process in action – by
measuring the speed and direction of ions escaping from Mars. This data
visualization compares simulations of the solar wind and Mars
atmospheric escape with new measurements taken by MAVEN.
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