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Ross 128 b information


Ross 128 b
Artist's impression of the planet Ross 128 b, with the star Ross 128 in the background.
Discovery
Discovered byXavier Bonfils
Discovery dateNovember 15, 2017
Detection method
Radial velocity
Orbital characteristics
Apastron0.0511 (± 0.0031) AU
Periastron0.0475 (± 0.0031) AU
Semi-major axis
0.0496 (± 0.0017) AU
Eccentricity0.036 (± 0.092)
Orbital period (sidereal)
9.8658 (± 0.0070) d
StarRoss 128
Physical characteristics
Mean radius
1.6+1.1
−0.65
[1]R🜨
Mass1.8+0.56
−0.43
[1] ME
Temperature213–301 K (−60–28 °C; −76–82 °F)

Ross 128 b is a confirmed Earth-sized exoplanet, likely rocky, that is orbiting within the inner habitable zone of the red dwarf star Ross 128, at a distance of around 11 light-years from Earth.[2] The exoplanet was found using a decade's worth of radial velocity data using the European Southern Observatory's HARPS spectrograph (High Accuracy Radial velocity Planet Searcher) at the La Silla Observatory in Chile. Ross 128 b is the nearest exoplanet around a quiet red dwarf, and is considered one of the best candidates for habitability. The planet is only 35% more massive than Earth, receives only 38% more starlight, and is expected to be a temperature suitable for liquid water to exist on the surface, if it has an atmosphere.[3]

The planet does not transit its host star, which historically made atmospheric characterization very difficult, but this has become possible with the construction of larger telescopes like the James Webb Space Telescope.[3]

  1. ^ a b Tasker, Elizabeth J.; Laneuville, Matthieu; Guttenberg, Nicholas (7 January 2020). "Estimating Planetary Mass with Deep Learning". The Astronomical Journal. 159 (2): 41. arXiv:1911.11035. Bibcode:2020AJ....159...41T. doi:10.3847/1538-3881/ab5b9e. ISSN 1538-3881. S2CID 208267900.
  2. ^ Newfound Earth-like exoplanet a good spot to hunt for aliens. Eric Mack, CBS News. 15 November 2017.
  3. ^ a b Bonfils, Xavier (2017). "A temperate exo-Earth around a quiet M dwarf at 3.4 parsecs". Astronomy and Astrophysics. 613: A25. arXiv:1711.06177. Bibcode:2018A&A...613A..25B. doi:10.1051/0004-6361/201731973. S2CID 37148632.

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