Kepler-10b
Kepler-10b est planeta extrasolaris qui stellam Kepler-10 constellationis Draconis circuit, anno 2011 primus omnium a satellita Kepler repertorum, primus planetarum terrestrium extrasolarium ab hominibus inventorum. A nobis annis luce mensis fere 560 distat. Planetae Kepler-10b periodus orbitalis 0.837495 dierum reportatur, massa 3.33 massae Telluris.
Bibliographia
[recensere | fontem recensere]- Natalie M. Batalha et al., "Kepler's first rocky planet: Kepler-10b" in Astrophysical Journal vol. 729 (2011) p. 27 ff.
- F. Fressin et al., "Kepler-10c, a 2.2-Earth radius transiting planet in a multiple system" in Astrophysical Journal (2011) Versio primitiva apud ArXiv
- Vincent Van Eylen, Simon Albrecht, "Eccentricity from transit photometry: small planets in Kepler multi-planet systems have low eccentricities" (2015) in Astrophysical Journal divulgatura
Nexus externi
[recensere | fontem recensere]
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Data astronomica: "Kepler-10b" apud SIMBAD. |
- Xavier Dumusque et al,, "The Kepler-10 planetary system revisited by HARPS-N: A hot rocky world and a solid Neptune-mass planet" apud ArXiv
- "Planet Kepler-10 b" apud The Extrasolar Planets Encyclopaedia