Gliese 555
Gliese 555 (HN Librae) is a red dwarf star of spectral type M4.0V, located in the constellation Libra at a distance of 20.4 light-years (6.3 parsecs) from Earth.[14]
| Observation data Epoch J2000.0 Equinox J2000.0 | |
|---|---|
| Constellation | Libra |
| Right ascension | 14h 34m 16.81166s[2] |
| Declination | −12° 31′ 10.4145″[2] |
| Apparent magnitude (V) | 11.317 |
| Characteristics | |
| Spectral type | M4.0V |
| Variable type | BY Dra |
| Astrometry | |
| Radial velocity (Rv) | −1.36±0.20[2] km/s |
| Proper motion (μ) | RA: −355.138 mas/yr[2] Dec.: 593.040 mas/yr[2] |
| Parallax (π) | 159.9225 ± 0.0546 mas[2] |
| Distance | 20.395 ± 0.007 ly (6.253 ± 0.002 pc) |
| Details | |
| Mass | 0.291±0.014[3] M☉ |
| Other designations | |
| Database references | |
| SIMBAD | data |
![]() Gliese 555 Location of Gliese 555 in the constellation Libra | |
Planetary system
In 2019, one planet candidate detected by radial velocity was reported in a preprint, among 118 planets around M dwarf stars. This would have a minimum mass about 30 times that of Earth and orbit with a period of about 450 days.[15] However, a 2023 paper discussing radial velocity observations by the CARMENES survey lists a different planet around this star, citing a discovery paper that has yet to be published as of May 2023. This is a super-Earth with a minimum mass of 2.6 Earths and a period of 36 days.[3]
| Companion (in order from star) |
Mass | Semimajor axis (AU) |
Orbital period (days) |
Eccentricity | Inclination | Radius |
|---|---|---|---|---|---|---|
| b (unconfirmed) | ≥2.59±0.34 M🜨 | — | 36.116+0.027 −0.029 |
— | — | — |
References
- Weis, Edward W. (March 1994). "Long Term Variability in Dwarf M Stars". The Astronomical Journal. 107: 1135–1140. Bibcode:1994AJ....107.1135W. doi:10.1086/116925. Retrieved 20 January 2022.
- Vallenari, A.; et al. (Gaia Collaboration) (2022). "Gaia Data Release 3. Summary of the content and survey properties". Astronomy & Astrophysics. arXiv:2208.00211. doi:10.1051/0004-6361/202243940. Gaia DR3 record for this source at VizieR.
- Ribas, I.; Reiners, A.; et al. (February 2023). "The CARMENES search for exoplanets around M dwarfs. Guaranteed time observations Data Release 1 (2016-2020)". Astronomy & Astrophysics. 670: A139. arXiv:2302.10528. Bibcode:2023A&A...670A.139R. doi:10.1051/0004-6361/202244879.
- Schönfeld, Eduard; et al. (1886). "BD -11 3759". Southern Durchmusterung.
- Gliese, W.; Jahreiß, H. (1991). "Gl 555". Preliminary Version of the Third Catalogue of Nearby Stars.
- Perryman; et al. (1997). "HIP 71253". The Hipparcos and Tycho Catalogues.
- Porter, J. G.; Yowell, E. J.; Smith, E. S. (1930). "A catalogue of 1474 stars with proper motion exceeding four-tenths year". Publications of the Cincinnati Observatory. 20: 1–32. Bibcode:1930PCinO..20....1P. Page 20 (Ci 20 870).
- Luyten, Willem Jacob (1979). "LHS 2945". LHS Catalogue, 2nd Edition.
- Luyten, Willem Jacob (1979). "NLTT 37751". NLTT Catalogue.
- Van Altena W. F.; Lee J. T.; Hoffleit E. D. (1995). "GCTP 3296". The General Catalogue of Trigonometric Stellar Parallaxes (Fourth ed.).
- Wolf, M. (1925). "Einige bewegte Sterne in Virgo und Libra". Astronomische Nachrichten. 225 (12): 215–216. Bibcode:1925AN....225R.215W. doi:10.1002/asna.19252251205. Page 215/216 (Wolf 1481)
- Perryman; et al. (1997). "HIP 71253". The Hipparcos and Tycho Catalogues.
- Hog; et al. (2000). "TYC 5572-804-1". The Tycho-2 Catalogue.
- Jao, Wei-Chun; Henry, Todd J.; Subasavage, John P.; Brown, Misty A.; Ianna, Philip A.; Bartlett, Jennifer L.; Costa, Edgardo; Méndez, René A. (2005). "The Solar Neighborhood. XIII. Parallax Results from the CTIOPI 0.9 Meter Program: Stars with mu >= 1.0" yr-1 (MOTION Sample)". The Astronomical Journal. 129 (4): 1954–1967. arXiv:astro-ph/0502167. Bibcode:2005AJ....129.1954J. doi:10.1086/428489. S2CID 16164903.
- Barnes, J. R.; Kiraga, M.; Diaz, M.; Berdiñas, Z.; Jenkins, J. S.; Keiser, S.; Thompson, I.; Crane, J. D.; Shectman, S. A. (2019-06-11). "Frequency of planets orbiting M dwarfs in the Solar neighbourhood". arXiv:1906.04644 [astro-ph.EP].
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