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

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

Data astronomica: "Ross 128" apud SIMBAD. "00912" apud ARICNS.