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61 de la Verge b.
61 de la Verge b és un planeta extrasolar[5][6] que orbita l'estel de tipus G 61 Virginis, localitzat aproximadament a 27 anys llum en la constel·lació de la Verge. Aquest planeta té una massa 5,1 vegades la de la Terra (classificant-se com una superterra) i triga 4 dies a completar el seu període orbital, sent el seu semieix major d'aproximadament 0,05 ua. Aquest planeta va ser descobert el 14 de desembre de 2009 usant el mètode de la velocitat radial i el telescopi Keck.[7][8]
- ↑ 1,0 1,1 1,2 1,3 Stefano Meschiari «A super-Earth and two Neptunes orbiting the nearby Sun-like star 61 Virginis» (en anglès). Astrophysical Journal, 2, 23-12-2009, pàg. 1366–1375. DOI: 10.1088/0004-637X/708/2/1366.
- ↑ 2,0 2,1 Afirmat a: Enciclopèdia Extrasolar Planets. Llengua del terme, de l'obra o del nom: anglès.
- ↑ 3,0 3,1 3,2 Jason Wright «The California Legacy Survey. I. A Catalog of 178 Planets from Precision Radial Velocity Monitoring of 719 Nearby Stars over Three Decades» (en anglès). The Astrophysical Journal Supplement Series, 1, juliol 2021, pàg. 8. DOI: 10.3847/1538-4365/ABE23C.
- ↑ 4,0 4,1 4,2 Floor van Leeuwen «Validation of the new Hipparcos reduction» (en anglès). Astronomy and Astrophysics, 2, 2007, pàg. 653–664. DOI: 10.1051/0004-6361:20078357.
- ↑ «Planet 61 Vir b» (en anglès). Extrasolar Planets Encyclopaedia. Observatori Meudon. [Consulta: 13 desembre 2020].
- ↑ «The planetary system 61 Vir hosts at least 3 planets.» (en anglès). Open Exoplanet Catalogue. [Consulta: 19 desembre 2020].
- ↑ Vogt, Steven. A Super-Earth and two Neptunes Orbiting the Nearby Sun-like star 61 Virginis. v1, 2009.
- ↑ Tim Stephens. «New planet discoveries suggest low-mass planets are common around nearby stars». UCSC News. UC Santa Cruz, 14-12-2009. Arxivat de l'original el 2009-12-23. [Consulta: 14 desembre 2009].
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61 de la Verge b
