[PDF] A PALETTE OF CLIMATES FOR GLIESE 581g - IOPscience

13 déc 2010 · Gliese 581g (Vogt et al 2010) sits squarely in the habitable zone of its star based on Selsis et al (2007), in the sense that it



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[PDF] Gliese 581d is the first discovered terrestrial-mass - Harvard SEAS

12 mai 2011 · GLIESE 581D IS THE FIRST DISCOVERED TERRESTRIAL-MASS EXOPLANET IN THE HABITABLE ZONE ROBIN D WORDSwORTH1, 



[PDF] 1S13 Exoplanète

L'exoplanète Gliese 581 D est dans la zone habitable de l'étoile Gliese 581, elle réunit donc les conditions nécessaires à la présence d'eau liquide De plus, son  



[PDF] Gliese 581d: A Possibly Habitable Planet around a - ResearchGate

Gliese 581d is a terrestrial super-earth planet, located on the inside edge of the habitable zone away from its parent star If Mars would be that size in our Solar



[PDF] Gliese 581d: A Habitable Exoplanet? Are there other planets

Gliese 581d: A Habitable Exoplanet? Are there other planets inhabited like the Earth, or at least habitable? The discovery of the first habitable planet has 



The extrasolar planet Gliese 581d: a potentially habitable planet?

The planetary system around the M star Gliese 581 contains at least three close- in potentially low-mass planets, Gl 581c, d, and e In order to address the 



Is Gliese 581d habitable? - Astronomy & Astrophysics

To investigate the possible climate of Gl 581d under a range of conditions, we have performed one-dimensional radiative- convective calculations In Sect 2 we  



[PDF] The Lick-Carnegie Exoplanet Survey: A 31 Earth-Mass Planet in the

M3V star Gliese 581, combining our data set of 122 precision RVs with an ex- 433 days and a 6th planet, GJ 581g, a minimum-mass 3 1M planet orbiting at ⊕



Habitability of super-Earths: Gliese 581c & 581d - Cambridge

Very recently, Udry et al (2007) announced the detection of two super-Earth planets in the Gliese 581 system; namely, Gl 581c with a mass of 5 06 M⊕ and a semi 



A PALETTE OF CLIMATES FOR GLIESE 581g - IOPscience

13 déc 2010 · Gliese 581g (Vogt et al 2010) sits squarely in the habitable zone of its star based on Selsis et al (2007), in the sense that it

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