Characterising Extrasolar Planets in Reflected Light and Thermal Emission

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dc.creatorSchneider, Jean
dc.date2002-10-29
dc.date.accessioned2026-07-07T02:05:52Z
dc.date.available2026-07-07T02:05:52Z
dc.descriptionThe physical bases of the detection and characterisation of extrasolar planets in the reflected light and thermal emission regimes are reviewed. They both have their advantages and disadvantages, including artefacts, in the determination of planet physical parameters (mass, size, albedo, surface and atmospheric conditions etc. A special attention is paid for Earth-like planets and new perspectives for these different aspects are also presented.
dc.description7 pages, published in "SF2A: Scientific Highlights 2002". Eds. F. Combes and D. Barret. EDPScience, 2002, p. 563
dc.identifierhttps://arxiv.org/abs/astro-ph/0210622
dc.identifierhttp://arxiv.org/abs/astro-ph/0210622
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/5237
dc.subjectAstrophysics
dc.titleCharacterising Extrasolar Planets in Reflected Light and Thermal Emission
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