Tidal obliquity evolution of potentially habitable planets

Astronomy and Astrophysics

Volumn 528, Issue , 2011, Pages

  Heller, R ^a,b   Leconte, J ^c   Barnes, R ^d,e  

^a ASTROPHYSIKALISCHES INSTITUT POTSDAM   (Germany)

^b UNIVERSITY OF HAMBURG   (Germany)

^c UNIVERSITÉ DE LYON   (France)

^d UNIVERSITY OF WASHINGTON   (United States)

^e Virtual Planetary Laboratory   (United States)

Author keywords

astrobiology; celestial mechanics; planet star interactions; planets and satellites: dynamical evolution and stability; planets and satellites: tectonics; stars: low mass

Indexed keywords

ASTROBIOLOGY; ASTROPHYSICS; EARTH (PLANET); EROSION; GIANT STARS; HEATING; INCIDENT SOLAR RADIATION; PLANETS; SATELLITES; TECTONICS; TIDES;

CELESTIAL MECHANICS; PLANET-STAR INTERACTIONS; PLANETS AND SATELLITES; PLANETS AND SATELLITES: DYNAMICAL EVOLUTION AND STABILITIES; STARS: LOW MASS;

ORBITS;

EID: 79952139368     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361/201015809     Document Type: Article

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