Energy Budgets for Terrestrial Extrasolar Planets
نویسندگان
چکیده
منابع مشابه
A Possible Aeronomy of Extrasolar Terrestrial Planets
Terrestrial planetary systems may exist around nearby stars as the Earthsized counterparts to the many giant planets already discovered within the solar neighborhood. In this chapter we first discuss the numerous techniques which have been suggested to search for extrasolar terrestrial planets. We then focus on the expected results from that technique in which an orbiting telescope or interfero...
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Copyright and Moral Rights for the articles on this site are retained by the individual authors and/or other copyright owners. For more information on Open Research Online's data policy on reuse of materials please consult the policies page. The climate on Earth is generally determined by the amount and distribution of incoming solar radiation, which must be balanced in equilibrium by the emiss...
متن کاملExploring extrasolar worlds: from gas giants to terrestrial habitable planets.
Almost 500 extrasolar planets have been found since the discovery of 51 Peg b by Mayor and Queloz in 1995. The traditional field of planetology has thus expanded its frontiers to include planetary environments not represented in our Solar System. We expect that in the next five years space missions (Corot, Kepler and GAIA) or ground-based detection techniques will both increase exponentially th...
متن کامل[Extrasolar terrestrial planets and possibility of extraterrestrial life].
Recent development of research on extrasolar planets are reviewed. About 120 extrasolar Jupiter-mass planets have been discovered through the observation of Doppler shift in the light of their host stars that is caused by acceleration due to planet orbital motions. Although the extrasolar planets so far observed may be limited to gas giant planets and their orbits differ from those of giant pla...
متن کاملExtrasolar Terrestrial Planets : Can We Detect Them Already ?
With the example of Proxima Centauri we discuss the feasibility of detecting terrestrial planets (1 to a few M⊕) using the high precision radial velocity (RV ) technique. If a very high RV precision for M stars is achieved even planets with these extremely low masses become detectable. For Proxima Cen (M5V), one of the prime targets of our Mstars planet search program using the UVES spectrograp...
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ژورنال
عنوان ژورنال: The Astrophysical Journal
سال: 2019
ISSN: 2041-8213
DOI: 10.3847/2041-8213/ab44ce