HD 93385
Appearance
Observation data Epoch J2000 Equinox J2000 | |
---|---|
Constellation | Vela |
Right ascension | 10h 46m 15.116s[1] |
Declination | –41° 27′ 51.73″[1] |
Apparent magnitude (V) | 7.486[2] |
Characteristics | |
Spectral type | G2/G3 V[3] |
B−V color index | 0.595[4] |
Details | |
Gyr | |
Database references | |
SIMBAD | data |
HD 93385 is a
light years from the Sun. It is drifting further away with a radial velocity
of +47.8 km/s.
This is an ordinary
Maunder minimum analog.[4]
A physical companion star with an apparent visual magnitude of 12.29 is located at an
arcseconds (equivalent to projected separation of 448 AU) along a position angle of 288°. It is estimated to have 45% of the mass of the Sun.[8] A 2015 survey ruled out the existence of any additional stellar companions at projected distances from 12 to 352 astronomical units.[9]
Planetary system
This star hosts two close-orbiting, super-Earth-like planets, suspected since 2011 and confirmed in 2021.[10][11] The first has 8.3 times the mass of the Earth and an orbital period of 13.186 days. The second is 10.1 times the Earth's mass with a period of 46.025 days.[12] A third planet on an innermost orbit was discovered in 2017[13] and confirmed in 2021.[11]
Companion (in order from star) |
Mass | Semimajor axis (AU) |
Orbital period (days) |
Eccentricity | Inclination | Radius |
---|---|---|---|---|---|---|
b | ≥4.2±0.5 M🜨 | 0.0756±0.0013 | 7.3426±0.0012 | <0.295 | — | — |
c | ≥7.1±0.6 M🜨 | 0.112±0.002 | 13.180±0.003 | <0.20 | — | — |
d | ≥8.7±0.9 M🜨 | 0.2565±0.0043 | 45.85±0.05 | 0.09+0.15 −0.05 |
— | — |
References
- ^ .
- ^ .
- ^ Bibcode:1978mcts.book.....H.
- ^ .
- doi:10.1086/430500.
- ^ S2CID 118565025.
- ^ "HD 93385". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 2013-10-07.
{{cite web}}
: CS1 maint: postscript (link) - S2CID 43663915.
- hdl:1887/49340, retrieved 19 June 2020.
- S2CID 118410500.
- ^ , A104
- ^ Zolotukhin, Ivan, "Catalog", Extrasolar Planets Encyclopaedia, retrieved 2013-10-07.
- , A117