Finding the Galactic Habitable Zone

Finding the Galactic Habitable Zone

Astronomers who specialize in galaxies and galaxy evolution have started to weigh in on habitability from a completely new perspective. Instead of trying to determine the zone around a star where an orbiting planet could sustain life, they are modeling the zones within the galaxy where planets that harbor complex life would be most likely to form. They dub this zone the Galactic Habitable Zone, or GHZ.

The Kepler Exoplanet Census

The Kepler Exoplanet Census

What does the Kepler data tell us about the number of planets per star and the distribution of planets in radius and orbital period? Andrew Youdin addresses that question by considering the selection effects in the Kepler sample and fitting a joint powerlaw in radius and orbital period.

Pack your suitcase? Super-Earth Gliese 581d is in the ‘Habitable Zone’

Pack your suitcase? Super-Earth Gliese 581d is in the ‘Habitable Zone’

One of the important goals of exoplanet science is to discover habitable planets that have the necessary conditions for life to form and thrive. Such planets will exist within the ‘habitable zone’ of a star. In this paper, the authors present Global Circulation Models which suggest that Gliese 581d could be in the habitable zone if it has a thick carbon dioxide-rich atmosphere.