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IISER Kolkata scientists simulate Mars on the computer, suggest how it lost its atmosphere
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The researchers model a Mars-like planet interacting with plasma wind from a Sun-like star
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Protective shroud: The magnetosphere enveloped Mars, shielding its atmosphere from erosion by solar wind.
  | Photo Credit:
Martin Holverda
The researchers model a Mars-like planet interacting with plasma wind from a Sun-like star
A new and exciting field in astronomy to study exoplanets and gauge whether they possess conditions that will favour the presence and sustainability of life. In this quest, an important part is looking at our own celestial backyard to gain insights – hence the many missions to Mars and Venus probing for signs of past life. One thing that astronomers search for in exoplanets, in the so-called Goldilocks zone of habitability, is the existence of liquid water and an atmosphere like that on Earth. In this context it is believed by many that Mars once had such an atmosphere. The mechanism as to why it lost its atmosphere has remained in doubt. Scientists from Indian Institution for Science Education and Research (IISER) Kolkata suggest that it was the planet’s intrinsic magnetic dynamo which, by shielding its atmosphere from the sun’s solar wind, protected its atmosphere. When the magnetic dynamo switched off, the atmosphere slowly was eroded by the solar wind and eventually vanished, leaving the thin remnant we see today. These results have been published in the journal

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