2002/10/29 by Jean Schneider, Schneider, Jean
Physics and Astronomy · #Astro and Planetary Science #Astronomy and Astrophysical Research #Astrophysics (astro-ph) #FOS: Physical sciences #Stellar, planetary, and galactic studies #astro-ph
paper · pdf · doi:10.48550/arxiv.astro-ph/0210622
7 pages, published in "SF2A: Scientific Highlights 2002". Eds. F. Combes and D. Barret. EDPScience, 2002, p. 563
arxiv created 2002/10/29 · openalex publication_date 2002/10/29 · arxiv updated 2009/12/01 · openalex created_date 2025/10/10 · openalex updated_date 2026/07/28
The physical bases of the detection and characterisation of extrasolar\nplanets in the reflected light and thermal emission regimes are reviewed. They\nboth have their advantages and disadvantages, including artefacts, in the\ndetermination of planet physical parameters (mass, size, albedo, surface and\natmospheric conditions etc. A special attention is paid for Earth-like planets\nand new perspectives for these different aspects are also presented.\n