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| Keywords: HD85512bWithHZ.svg en Plot of the orbit of HD 85512 b compared to the star's habitable zone Orbit data taken from http //arxiv org/abs/1108 3447 Pepe et al 2011 arXiv 1108 3447v1 astro-ph EP The HARPS search for Earth-like planets in the habitable zone I � Very low-mass planets around HD20794 HD85512 and HD192310 The configuration is given in Table 5 Uncertainties in the quantities are not depicted The habitable zone limits are computed using the formulae given in http //adsabs harvard edu/abs/2003IJAsB 2 289U Underwood et al 2003 International Journal of Astrobiology vol 2 4 pp 289 �299 The evolution of habitable zones during stellar lifetimes and its implications on the search for extraterrestrial life The habitable zone is colour-coded as follows Red Recent Venus inner � Runaway greenhouse outer Yellow Runaway greenhouse inner � Water loss outer Green Water loss inner � First CO<sub>2</sub> condensation outer Cyan First CO<sub>2</sub> condensation inner � Maximum greenhouse outer Blue Maximum greenhouse inner � Early Mars outer Using this definition of the habitable zone the most conservative habitable zone is the green region the inner boundary corresponding to the start of water loss and the outer limit corresponding to the first condensation of carbon dioxide in the atmosphere Scale 10000 SVG units 1 AU own Icalanise 2011-08-19 Cc-zero Exoplanet diagrams HD 85512 b | ||||
