The ubiquity of M dwarfs, combined with the relative ease of detecting terrestrial-mass planets around them, has made them prime targets for finding and characterising planets in the "Habitable Zone" (HZ).
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Extrasolar Planets: January 2016
Calendar
- 18 Sep: Hearing: Developing Core Capabilities for Deep Space Exploration: An Update on NASA’s SLS, Orion, and Exploration Ground Systems
- 18 Sep: NASA Astrobiology Institute Virtual Workshopl: Astrovirology
- 23 Sep: Planetary Science Advisory Committee Meeting
- 26 Sep: Astronomy and Astrophysics Advisory Committee Meeting
- 1 Oct: Heliophysics Advisory Committee Meeting
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