HD 162020
HD 162020 is an orange dwarf star in Scorpius constellation with a brown dwarf companion.
Observation data Epoch J2000 Equinox J2000 | |
---|---|
Constellation | Scorpius |
Right ascension | 17h 50m 38.3562s[1] |
Declination | −40° 19′ 06.066″[1] |
Apparent magnitude (V) | 9.12[2] |
Characteristics | |
Spectral type | K3V[2] |
Astrometry | |
Proper motion (μ) | RA: 19.057±0.140[1] mas/yr Dec.: −26.278±0.101[1] mas/yr |
Parallax (π) | 32.52 ± 0.24[1] mas |
Distance | 100.3 ± 0.7 ly (30.8 ± 0.2 pc) |
Details[3] | |
Mass | 0.75 M☉ |
Surface gravity (log g) | 4.76±0.25 cgs |
Temperature | 4830±80 K |
Metallicity [Fe/H] | 0.01±0.11 dex |
Rotational velocity (v sin i) | 1.9 km/s |
Other designations | |
Database references | |
SIMBAD | data |
Exoplanet Archive | data |
HD 162020 b
Discovery | |
---|---|
Discovered by | Udry et al. |
Discovery date | April 15, 2000[4] |
Doppler Spectroscopy | |
Orbital characteristics | |
00,751 AU (1.123×1011 km) | |
Eccentricity | 0.277 ± 0.02 |
8.428198 ± 0.000056 d | |
2451990.6768 ± 0.0050 | |
28.40 ± 0.23 | |
Semi-amplitude | 1813 ± 4 |
Physical characteristics | |
Mass | >15.0 MJ |
HD 162020 b is a brown dwarf with mass 15.0 MJ. The mass is minimum since inclination is not known. This planetar orbits very close to the star at a distance of 0.075 AU. Despite of this, it has an eccentric orbit of 27.7%. The distance from the star ranges from 0.054 to 0.096 AU. It has an extremely high semi-amplitude of 1.813 km/s. The discovery was announced on April 15, 2000 by the Geneva Extrasolar Planet Search Team.[4][3]
gollark: Why does that URL say *darkness*?
gollark: I don't think "obliterate entire polity" is a very good idea generally.
gollark: And/or just fiddling with the universe at a lower level.
gollark: I've wanted to play D&D for ages but never actually got round to doing anything about it…
gollark: What if you somehow combine the roles? A musical pole or something?
References
- Brown, A. G. A; et al. (2016). "Gaia Data Release 1. Summary of the astrometric, photometric, and survey properties". Astronomy and Astrophysics. 595. A2. arXiv:1609.04172. Bibcode:2016A&A...595A...2G. doi:10.1051/0004-6361/201629512.Gaia Data Release 1 catalog entry
- "HD 162020". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 2018-04-02.
- Udry, M.; et al. (2002). "The CORALIE survey for southern extra-solar planets VIII. The very low-mass companions of HD 141937, HD 162020, HD 168443, HD 202206: Brown dwarfs or "superplanets"?". Astronomy and Astrophysics. 390 (1): 267–279. arXiv:astro-ph/0202458. Bibcode:2002A&A...390..267U. doi:10.1051/0004-6361:20020685.
- "Exoplanets Galore!" (Press release). Garching, Germany: European Southern Observatory. April 15, 2000. Retrieved December 30, 2012.
External links
- "Notes for star HD 162020". The Extrasolar Planets Encyclopaedia. Retrieved December 21, 2007.
- "Notes for planet HD 162020 b". The Extrasolar Planets Encyclopaedia. Retrieved December 21, 2007.
This article is issued from Wikipedia. The text is licensed under Creative Commons - Attribution - Sharealike. Additional terms may apply for the media files.