| Observation data Epoch J2000.0 Equinox J2000.0 | |
|---|---|
| Constellation | Chamaeleon |
| Right ascension | 11h 06m 28.7626s [1] |
| Declination | −77° 37′ 33.1444″ [1] |
| Characteristics | |
| Spectral type | M3 [2] |
| Astrometry | |
| Proper motion (μ) |
RA: −22.193±0.233
[1]
mas/
yr Dec.: 0.215±0.206 [1] mas/ yr |
| Parallax (π) | 5.2343 ± 0.1759 mas [1] |
| Distance | 620 ± 20
ly (191 ± 6 pc) |
| Details [3] | |
| Mass | 0.32 ± 0.11 M☉ |
| Radius | 0.83 ± 0.04 R☉ |
| Luminosity | 0.09 ± 0.07 L☉ |
| Temperature | 3490 ± 180 K |
| Age | 2±1 [4] Myr |
| Other designations | |
| Database references | |
| SIMBAD | data |
CHXR 73 is a star in the constellation Chamaeleon, about 620 light-years away from Earth. [1] [6]
The star is located within Cha I, a molecular cloud. [5] It has a low temperature of 3,490 K typical of red dwarfs, but unlike typical red dwarfs it has an unusually large radius of 0.83 R☉—this is because of its young age, only 8 million years. [3]
Planetary system
A companion, CHXR 73 b, has been found via direct imaging. CHXR 73 has a mass of about 12 Jupiters. [7] This is close to the upper mass limit for planets, making its classification difficult.
| Companion (in order from star) |
Mass |
Semimajor axis ( AU) |
Orbital period ( days) |
Eccentricity | Inclination | Radius |
|---|---|---|---|---|---|---|
| b | 13±6 MJ | 210 | — | — | — | — |
References
- ^ a b c d e f Brown, A. G. A.; et al. (Gaia collaboration) (August 2018). "Gaia Data Release 2: Summary of the contents and survey properties". Astronomy & Astrophysics. 616. A1. arXiv: 1804.09365. Bibcode: 2018A&A...616A...1G. doi: 10.1051/0004-6361/201833051. Gaia DR2 record for this source at VizieR.
- ^ "Notes on CHXR 73 b". Extrasolar Planets Encyclopaedia. Retrieved 24 December 2016.
- ^ a b Daemgen, S.; Petr-Gotzens, M. G.; Correia, S.; Teixeira, P. S.; Brandner, W.; Kley, W.; Zinnecker, H. (2013). "Protoplanetary disk evolution and stellar parameters of T Tauri binaries in Chamaeleon I". Astronomy & Astrophysics. 554: A43. arXiv: 1304.1150. Bibcode: 2013A&A...554A..43D. doi: 10.1051/0004-6361/201321220. S2CID 59440639.
- ^ a b Bowler, Brendan P. (2016), "Imaging Extrasolar Giant Planets", Publications of the Astronomical Society of the Pacific, 128 (968): 102001, arXiv: 1605.02731, doi: 10.1088/1538-3873/128/968/102001, S2CID 118614968
- ^ a b "CHXR 73". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 13 November 2016.
- ^ "Newfound Object Further Blurs Planet Definition". Space.com. Retrieved 13 November 2016.
- ^ Luhman, K. (2006). "Discovery of a Young Substellar Companion in Chamaeleon". The Astrophysical Journal. 649 (2): 894–899. arXiv: astro-ph/0609187. Bibcode: 2006ApJ...649..894L. doi: 10.1086/506517. S2CID 14609766.
 | This article about a red dwarf is a stub. You can help Wikipedia by expanding it. |
| Observation data Epoch J2000.0 Equinox J2000.0 | |
|---|---|
| Constellation | Chamaeleon |
| Right ascension | 11h 06m 28.7626s [1] |
| Declination | −77° 37′ 33.1444″ [1] |
| Characteristics | |
| Spectral type | M3 [2] |
| Astrometry | |
| Proper motion (μ) |
RA: −22.193±0.233
[1]
mas/
yr Dec.: 0.215±0.206 [1] mas/ yr |
| Parallax (π) | 5.2343 ± 0.1759 mas [1] |
| Distance | 620 ± 20
ly (191 ± 6 pc) |
| Details [3] | |
| Mass | 0.32 ± 0.11 M☉ |
| Radius | 0.83 ± 0.04 R☉ |
| Luminosity | 0.09 ± 0.07 L☉ |
| Temperature | 3490 ± 180 K |
| Age | 2±1 [4] Myr |
| Other designations | |
| Database references | |
| SIMBAD | data |
CHXR 73 is a star in the constellation Chamaeleon, about 620 light-years away from Earth. [1] [6]
The star is located within Cha I, a molecular cloud. [5] It has a low temperature of 3,490 K typical of red dwarfs, but unlike typical red dwarfs it has an unusually large radius of 0.83 R☉—this is because of its young age, only 8 million years. [3]
Planetary system
A companion, CHXR 73 b, has been found via direct imaging. CHXR 73 has a mass of about 12 Jupiters. [7] This is close to the upper mass limit for planets, making its classification difficult.
| Companion (in order from star) |
Mass |
Semimajor axis ( AU) |
Orbital period ( days) |
Eccentricity | Inclination | Radius |
|---|---|---|---|---|---|---|
| b | 13±6 MJ | 210 | — | — | — | — |
References
- ^ a b c d e f Brown, A. G. A.; et al. (Gaia collaboration) (August 2018). "Gaia Data Release 2: Summary of the contents and survey properties". Astronomy & Astrophysics. 616. A1. arXiv: 1804.09365. Bibcode: 2018A&A...616A...1G. doi: 10.1051/0004-6361/201833051. Gaia DR2 record for this source at VizieR.
- ^ "Notes on CHXR 73 b". Extrasolar Planets Encyclopaedia. Retrieved 24 December 2016.
- ^ a b Daemgen, S.; Petr-Gotzens, M. G.; Correia, S.; Teixeira, P. S.; Brandner, W.; Kley, W.; Zinnecker, H. (2013). "Protoplanetary disk evolution and stellar parameters of T Tauri binaries in Chamaeleon I". Astronomy & Astrophysics. 554: A43. arXiv: 1304.1150. Bibcode: 2013A&A...554A..43D. doi: 10.1051/0004-6361/201321220. S2CID 59440639.
- ^ a b Bowler, Brendan P. (2016), "Imaging Extrasolar Giant Planets", Publications of the Astronomical Society of the Pacific, 128 (968): 102001, arXiv: 1605.02731, doi: 10.1088/1538-3873/128/968/102001, S2CID 118614968
- ^ a b "CHXR 73". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 13 November 2016.
- ^ "Newfound Object Further Blurs Planet Definition". Space.com. Retrieved 13 November 2016.
- ^ Luhman, K. (2006). "Discovery of a Young Substellar Companion in Chamaeleon". The Astrophysical Journal. 649 (2): 894–899. arXiv: astro-ph/0609187. Bibcode: 2006ApJ...649..894L. doi: 10.1086/506517. S2CID 14609766.
|
| This article about a red dwarf is a stub. You can help Wikipedia by expanding it. |