HD 86226
Appearance
Observation data Epoch J2000.0 Equinox J2000.0 | |
---|---|
Constellation | Hydra |
Right ascension | 09h 56m 29.84s |
Declination | –24° 05′ 57.8″ |
Apparent magnitude (V) | 7.932 |
Characteristics | |
Spectral type | G2V |
Apparent magnitude (B) | 8.563 |
Apparent magnitude (R) | 7.71 |
Apparent magnitude (J) | 6.839 |
Apparent magnitude (H) | 6.577 |
Apparent magnitude (K) | 6.463 |
B−V color index | 0.631 |
V−R color index | 0.22 |
Variable type | none |
Astrometry | |
Radial velocity (Rv) | +19.4 km/s |
Proper motion (μ) | RA: –176.37 mas/yr Dec.: 46.72 mas/yr |
Parallax (π) | 23.54 ± 0.85 mas |
Distance | 139 ± 5 ly (42 ± 2 pc) |
Absolute magnitude (MV) | 4.791 |
Details | |
Mass | 1.06 ± 0.03[1] M☉ |
Radius | 1.02 ± 0.03 R☉ |
Luminosity | 1.06 L☉ |
Surface gravity (log g) | 4.36 ± 0.04 cgs |
Temperature | 5903 ± 31 K |
Metallicity | 0.05 ± 0.03 |
Rotation | 23 ± 4 |
Age | 1.5 ± 1.3 Gyr |
Other designations | |
Database references | |
SIMBAD | data |
Exoplanet Archive | data |
HD 86226 is a G type yellowish white star found in the constellation of Hydra.
The survey in 2015 have ruled out the existence of any stellar companions at projected distances above 12 astronomical units.[2]
Planetary system
Due to the periodic spectrum shifts when it had when placed under a Doppler test, 13 Magellan Doppler Velocity observations were made of an object found near the star. The object discovered in 2010 had a Keplerian orbit, was declared an exoplanet and dubbed HD 86226 b.[3][4][5][6]
A hot Super-Earth planet HD 86226 c was also discovered in 2020.[7]
Companion (in order from star) |
Mass | Semimajor axis (AU) |
Orbital period (days) |
Eccentricity | Inclination | Radius
|
---|---|---|---|---|---|---|
c | 7.25+1.19 −1.12 M🜨 |
0.049±0.001 | 3.98442±0.00018 | 0.075+0.065 −0.048 |
86.45+0.26 −0.16° |
2.16±0.08 R🜨 |
b | 0.45+0.04 −0.05 MJ |
2.73±0.06 | 1628+22 −21 |
0.059+0.062 −0.039 |
— | — |
See also
References
- ^ a b
Marmier, M.; Ségransan, D.; Udry, S.; Mayor, M.; Pepe, F.; Queloz, D.; Lovis, C.; Naef, D.; Santos, N. C.; Alonso, R.; Alves, S.; Berthet, S.; Chazelas, B.; Demory, B.-O.; Dumusque, X.; Eggenberger, A.; Figueira, P.; Gillon, M.; Hagelberg, J.; Lendl, M.; A. Mardling, R.; Mégevand, D.; Neveu, M.; Sahlmann, J.; Sosnowska, D.; Tewes, M.; Triaud, A. H. M. J. (March 2013). "The CORALIE survey for southern extrasolar planets XVII. New and updated long period and massive planets". Astronomy and Astrophysics. 551. arXiv:1211.6444. Bibcode:2013A&A...551A..90M. doi:10.1051/0004-6361/201219639.
{{cite journal}}
: Unknown parameter|displayauthors=
ignored (|display-authors=
suggested) (help) - ^ Mugrauer, M.; Ginski, C. (12 May 2015). "High-contrast imaging search for stellar and substellar companions of exoplanet host stars". Monthly Notices of the Royal Astronomical Society. 450 (3). doi:10.1093/mnras/stv771. Retrieved 19 June 2020.
{{cite journal}}
: CS1 maint: unflagged free DOI (link) - ^ "Constellations: Hydra 'the Sea Serpent'". h2g2. Retrieved 2010-02-10.[unreliable source?]
- ^ Arriagada, Pamela; Butler, R. Paul; Minniti, Dante; López-Morales, Mercedes; Shectman, Stephen A.; Adams, Fred C.; Boss, Alan P.; Chambers, John E. (2010). "Five Long-period Extrasolar Planets in Eccentric orbits from the Magellan Planet Search Program". The Astrophysical Journal. 711 (2). arXiv:1001.4093. Bibcode:2010ApJ...711.1229A. doi:10.1088/0004-637X/711/2/1229.
{{cite journal}}
: Unknown parameter|displayauthors=
ignored (|display-authors=
suggested) (help) - ^ "HD 86226". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 2010-02-10.
- ^ "Star : HD 86226". The Extrasolar Planets Encyclopaedia. Retrieved 2010-02-10.
- ^ a b TESS Reveals a Short-period Sub-Neptune Sibling (HD 86226c) to a Known Long-period Giant Planet, 2020, arXiv:2007.13927
External links
- "HD 86226". SAO/NASA Astrophysics Data System (ADS) (Database query).