Ross 128
Ross 128, stella variabilis etiam FI Vir appellata, est pumilio rubra constellationis Virginis. A tellure 10.89 spatiis lucis annuis distans, locum undecimum inter systemata stellaria proxima tenet. Magnitudine apparenti 11.13 videtur. Planeta extrasolaris terrestris Ross 128 b huic stellae intra zonam temperatam circumambulat.
Bibliographia[recensere | fontem recensere]
- X. Bonfils et al., "A temperate exo-Earth around a quiet M dwarf at 3.4 parsecs" in Astronomy & Astrophysics (8 Novembris 2017)
- Jack T. O’Malley-James, L. Kaltenegger, "Lessons from early Earth: UV surface radiation should not limit the habitability of active M star systems" in Monthly Notices of the Royal Astronomical Society vol. 485 (2019) pp. 5598–5603
- Diogo Souto et al., "Stellar and Planetary Characterization of the Ross 128 Exoplanetary System from APOGEE Spectra" (14 Iunii 2018) aoud arXiv.org pro Astrophysical Journal Letters
Nexus externi[recensere | fontem recensere]
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Data astronomica: "Ross 128" apud SIMBAD. "00912" apud ARICNS. |
- "Closest temperate world orbiting quiet star discovered" (15 Novembris 2017) apud Phys.org