THERMAL ESCAPE FROM SUPER EARTH ATMOSPHERES IN THE HABITABLE ZONES OF M STARS
A fundamental question for exoplanet habitability is the long-term stability of the planet's atmosphere. We numerically solve a one-dimensional multi-component hydrodynamic thermosphere/ionosphere model to examine the thermal and chemical responses of the primary CO[subscript 2] atmospheres of...
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| Format: | Article |
| Language: | English |
| Published: |
Institute of Physics/American Astronomical Society,
2015-03-26T15:36:24Z.
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| Online Access: | Get fulltext |