Anthropic selection and the habitability of planets orbiting M and K dwarfs

• Published in: Icarus (New York, N.Y. 1962) N.Y. 1962), 2011-10, Vol.215 (2), p.518-521
• Main Author: Waltham, Dave
• Format: Article
• Language: English
• Subjects: Astronomy; Earth; Earth, ocean, space; Exact sciences and technology; Exobiology; Extrasolar planets; Solar system
• ISSN: 0019-1035; 1090-2643
• DOI: 10.1016/j.icarus.2011.07.023

► An index is developed which characterizes strength of anthropic effects. ► This index is calculated from exoplanet property statistics. ► If this index exceeds 1.59, anthropic effects are statistically significant. ► Application to stellar mass rules out strong selection for small stars. ► Implication is that small stars probably have relatively hostile habitable zones. The Earth may have untypical characteristics which were necessary preconditions for the emergence of life and, ultimately, intelligent observers. This paper presents a rigorous procedure for quantifying such “anthropic selection” effects by comparing Earth’s properties to those of exoplanets. The hypothesis that there is anthropic selection for stellar mass (i.e. planets orbiting stars with masses within a particular range are more favourable for the emergence of observers) is then tested. The results rule out the expected strong selection for low mass stars which would result, all else being equal, if the typical timescale for the emergence of intelligent observers is very long. This indicates that the habitable zone of small stars may be less hospitable for intelligent life than the habitable zone of solar-mass stars. Additional planetary properties can also be analyzed, using the approach introduced here, once relatively complete and unbiased statistics are made available by current and planned exoplanet characterization projects.