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BeschreibungThe habitable zone around some stars with planets.jpg
English: A team of astronomers has shown that the newly discovered exoplanet HD 85512 b lies at the edge of the habitable zone of its star, where liquid water oceans could potentially exist if the atmosphere of the planet has sufficient cloud cover. This diagram shows the distances of the planets in the Solar System (upper row) in the new HD 85512 system (middle) and in the Gliese 581 system (lower row), from their respective stars (left). The habitable zone is indicated as the blue area
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Bildtitel
A team of astronomers has shown that the newly discovered exoplanet HD 85512 b lies at the edge of the habitable zone of its star, where liquid water oceans could potentially exist if the atmosphere of the planet has sufficient cloud cover. This diagram shows the distances of the planets in the Solar System (upper row) in the new HD 85512 system (middle) and in the Gliese 581 system (lower row), from their respective stars (left). The habitable zone is indicated as the blue area. Note that some early versions of this diagram were in error - please use the most recent. Based on an original diagram by Franck Selsis, Univ. of Bordeaux.
Namensnennung/Veröffentlicher
ESO
Quelle
European Southern Observatory
Kurztitel
The habitable zone around some stars with planets
Nutzungsbedingungen
Creative Commons Attribution 4.0 International License
Erfassungszeitpunkt
18:00, 12. Sep. 2011
JPEG-Dateikommentar
A team of astronomers has shown that the newly discovered exoplanet HD 85512 b lies at the edge of the habitable zone of its star, where liquid water oceans could potentially exist if the atmosphere of the planet has sufficient cloud cover. This diagram shows the distances of the planets in the Solar System (upper row) in the new HD 85512 system (middle) and in the Gliese 581 system (lower row), from their respective stars (left). The habitable zone is indicated as the blue area. Note that some early versions of this diagram were in error - please use the most recent. Based on an original diagram by Franck Selsis, Univ. of Bordeaux.