GJ 1061
Observation data Epoch J2000 Equinox J2000 | |
---|---|
Constellation | Horologium |
Right ascension | 03h 35m 59.69s[1] |
Declination | −44° 30′ 45.3″[1] |
Apparent magnitude (V) | 13.03[2] |
Characteristics | |
Spectral type | M5.5 V[2] |
Apparent magnitude (J) | 7.52 ± 0.02[3] |
U−B color index | 1.52[3] |
B−V color index | 1.90[3] |
Astrometry | |
Radial velocity (Rv) | −8 km/s |
Proper motion (μ) | RA: 750.01[4] mas/yr Dec.: -349.98[5] mas/yr |
Parallax (π) | 270.86 ± 1.29 mas[6] |
Distance | 12.04 ± 0.06 ly (3.69 ± 0.02 pc) |
Absolute magnitude (MV) | 15.26[4] |
Details | |
Mass | 0.113[5] M☉ |
Luminosity | 0.001[5] L☉ |
Metallicity [Fe/H] | −0.09±0.09[7] dex |
Rotational velocity (v sin i) | ≤ 5[8] km/s |
Other designations | |
Database references | |
SIMBAD | data |
Gliese 1061 is a red dwarf star located approximately 12 light-years from Earth in the southern constellation of Horologium. Even though it is a relatively nearby star it has an apparent visual magnitude of about 13[2] so it can only be seen with at least a moderately-sized telescope.
The proper motion of Gliese 1061 has been known since 1974, but it was estimated to be further away: approximately 25 light-years distant based upon an estimated parallax of 0.130″. Its distance was only accurately determined in 1997 by the RECONS team. At that time, it was the 20th-nearest star system to the Sun. The discovery team noted that many more stars such as this are likely to be discovered nearby.[2]
This star is a very small, dim, red dwarf, close to the lower mass limit for a star. It has an estimated mass of about 11.3% of the Sun and is only 0.1% as luminous.[5] The star displays no significant infrared excess due to circumstellar dust.[9]
Planetary system
On August 13, 2019, a planetary system was announced orbiting the star Gliese 1061 by the Red Dots project of detecting terrestrial planets around nearby red dwarf stars.[10] The planet Gliese 1061 d orbits in the conservative circumstellar habitable zone of its star and the planet Gliese 1061 c orbits in the inner edge of the habitable zone.[10] Gliese 1061 is a non-variable star that does not suffer flares, so there is a greater probability that the exoplanets still conserves their atmosphere if they had one.[11]
Companion (in order from star) |
Mass | Semimajor axis (AU) |
Orbital period (days) |
Eccentricity | Inclination | Radius |
---|---|---|---|---|---|---|
b | 1.38+0.16 −0.15 M🜨 |
0.021 ± 0.001 | 3.204 ± 0.001 | < 0.31 | — | — |
c | 1.75 ± 0.23 M🜨 | 0.035 ± 0.001 | 6.689 ± 0.005 | < 0.29 | — | — |
d | 1.68+0.25 −0.24 M🜨 |
0.054 ± 0.001 | 13.031+0.025 −0.032 |
< 0.53 | — | — |
Gliese 1061 c
Discovery[10] | |
---|---|
Discovered by | Dreizler et al. 2019[10] |
Discovery date | 13 August 2019 |
Doppler spectroscopy | |
Orbital characteristics | |
0.035 ± 0.001 au | |
Eccentricity | < 0.29 |
6.689 ± 0.005 d | |
88+95 −85° | |
JD 2458300.2+1.9 −1.5 | |
Semi-amplitude | 2.48+0.28 −0.29 km/s |
Star | Gliese 1061 |
Physical characteristics | |
Mass | >1.75 ± 0.23 |
Gliese 1061 c (also known as GJ 1061 c) is an exoplanet orbiting the red dwarf Gliese 1061, 12 light years away from Earth.[12]
Gliese 1061 c is 75% more massive than the Earth, it receives 35% more stellar flux and has an equilibrium temperature of 275 K (2 °C; 35 °F).[13]
Gliese 1061 c orbits its star every 6.7 days, so it is probably in synchronous rotation with its star.
It is an exoplanet warmer than Earth, with an equilibrium temperature of almost 20 K greater, so the average temperature on the surface could be around 34 °C (307 K; 93 °F), provided the atmosphere is of similar composition to the Earth's.
Gliese 1061 d
Discovery | |
---|---|
Discovery date | 13 August 2019 |
Doppler spectroscopy | |
Orbital characteristics | |
0.052 (± 0.001) au | |
Eccentricity | 0.54 |
13.031 d[14] | |
Star | Gliese 1061 |
Physical characteristics | |
Mass | 1.64 |
Gliese 1061 d is a potentially habitable exoplanet orbiting the red dwarf star Gliese 1061, 12 light-years away.[15][16][10]
The exoplanet is estimated to have a mass of 1.64 Earth masses, an equilibrium temperature of 218 K (−55 °C; −67 °F), and an orbital period of 13 days.[15][14] Due to Gliese 1061 d's semi-major axis, it is likely that the exoplanet is tidally locked.
It is an exoplanet colder than Earth, with an equilibrium temperature of 218 K (−55 °C; −67 °F) degrees Celsius, so the average temperature on the surface could be around 250 K (−23 °C; −10 °F), provided the atmosphere is similar to that of Earth.
References
- ^ a b Cutri, R. M.; et al. (June 2003). "2MASS All-Sky Catalog of Point Sources". VizieR On-line Data Catalog: II/246. Bibcode:2003yCat.2246....0C.
- ^ a b c d Henry, Todd J.; et al. (1997). "The solar neighborhood IV: discovery of the twentieth nearest star". The Astronomical Journal. 114: 388–395. Bibcode:1997AJ....114..388H. doi:10.1086/118482.
- ^ a b c d "LHS 1565". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 2008-12-11.
- ^ a b Scholz, R.-D.; et al. (2000). "New high-proper motion survey in the Southern sky". Astronomy and Astrophysics. 353: 958–969. Bibcode:2000A&A...353..958S.
- ^ a b c d "The One Hundred Nearest Star Systems". RECONS. 2008-01-01. Retrieved 2008-12-11.
- ^ Lurie, John C.; et al. (2014). "The Solar Neighborhood. XXXIV. a Search for Planets Orbiting Nearby M Dwarfs Using Astrometry". The Astronomical Journal. 148 (5): 91. arXiv:1407.4820. Bibcode:2014AJ....148...91L. doi:10.1088/0004-6256/148/5/91. S2CID 118492541.
- ^ Neves, V.; et al. (August 2014). "Metallicity of M dwarfs. IV. A high-precision [Fe/H] and Teff technique from high-resolution optical spectra for M dwarfs". Astronomy & Astrophysics. 568: 22. arXiv:1406.6127. Bibcode:2014A&A...568A.121N. doi:10.1051/0004-6361/201424139. S2CID 118619790. A121.
- ^ Barnes, J. R.; et al. (April 2014). "Precision radial velocities of 15 M5-M9 dwarfs". Monthly Notices of the Royal Astronomical Society. 439 (3): 3094–3113. arXiv:1401.5350. Bibcode:2014MNRAS.439.3094B. doi:10.1093/mnras/stu172. S2CID 16005221.
{{cite journal}}
: CS1 maint: unflagged free DOI (link) - ^ Avenhaus, H.; et al. (December 2012). "The nearby population of M-dwarfs with WISE: a search for warm circumstellar dust". Astronomy & Astrophysics. 548: 15. arXiv:1209.0678. Bibcode:2012A&A...548A.105A. doi:10.1051/0004-6361/201219783. S2CID 56397054. A105.
- ^ a b c d e Dreizler, S.; Jeffers, S. V.; Rodríguez, E.; Zechmeister, M.; Barnes, J.R.; Haswell, C.A.; Coleman, G. A. L.; Lalitha, S.; Hidalgo Soto, D.; Strachan, J.B.P.; Hambsch, F-J.; López-González, M. J.; Morales, N.; Rodríguez López, C.; Berdiñas, Z. M.; Ribas, I.; Pallé, E.; Reiners, A.; Anglada-Escudé, G. (2019-08-13). "Red Dots: A temperate 1.5 Earth-mass planet in a compact multi-terrestrial planet system around GJ1061". Monthly Notices of the Royal Astronomical Society. arXiv:1908.04717. doi:10.1093/mnras/staa248. S2CID 199551874.
{{cite journal}}
: CS1 maint: unflagged free DOI (link) - ^ Starr, Michelle. "Three Rocky Exoplanets Have Been Found Orbiting a Star Just 12 Light-Years Away". ScienceAlert. Retrieved 2020-10-07.
- ^ "Exoplanet-catalog". Exoplanet Exploration: Planets Beyond our Solar System. Retrieved 2020-03-31.
- ^ "Trio of Super-Earths Found Orbiting Red Dwarf Gliese 1061 | Astronomy | Sci-News.com". Breaking Science News | Sci-News.com. Retrieved 2020-03-31.
- ^ a b "Exoplanet-catalog". Exoplanet Exploration: Planets Beyond our Solar System. Retrieved 2020-10-07.
- ^ a b "The Habitable Exoplanets Catalog - Planetary Habitability Laboratory @ UPR Arecibo". phl.upr.edu. Retrieved 2020-03-31.
- ^ "GJ 1061 d". exoplanetarchive.ipac.caltech.edu. Retrieved 2020-10-07.
See also
External links
- Gliese and GJ objects
- Horologium (constellation)
- Local Bubble
- M-type main-sequence stars
- Planetary systems with three confirmed planets
- Exoplanets discovered in 2019
- Exoplanets detected by radial velocity
- Near-Earth-sized exoplanets in the habitable zone
- Exoplanets in the Gliese Catalog
- TIC objects
- Exoplanet stubs