Ross 128
stella pumilio rubra
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
- 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
Data astronomica: "Ross 128" apud SIMBAD. "00912" apud ARICNS. |
- "Closest temperate world orbiting quiet star discovered" (15 Novembris 2017) apud Phys.org