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Revision as of 16:29, 29 January 2019 by Psyluke (talk | contribs) (Names of redirects in bold, and remove a red link)(diff) ← Previous revision | Latest revision (diff) | Newer revision → (diff)Observation data Epoch J2000 Equinox J2000 | |
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Constellation | Andromeda |
Groombridge 34 A | |
Right ascension | 00 18 22.8850 |
Declination | +44° 01′ 22.6373″ |
Apparent magnitude (V) | 8.119 |
Groombridge 34 B | |
Right ascension | 00 18 25.8244 |
Declination | +44° 01′ 38.0912″ |
Apparent magnitude (V) | 11.007 |
Characteristics | |
Spectral type | M1.4V + M4.1V |
U−B color index | +1.24/+1.40 |
B−V color index | +1.56/+1.80 |
Variable type | Flare stars |
Astrometry | |
Groombridge 34 A | |
Radial velocity (Rv) | +11.62±0.08 km/s |
Proper motion (μ) | RA: 2891.525±0.061 mas/yr Dec.: 411.903±0.034 mas/yr |
Parallax (π) | 280.6902 ± 0.0429 mas |
Distance | 11.620 ± 0.002 ly (3.5626 ± 0.0005 pc) |
Groombridge 34 B | |
Proper motion (μ) | RA: 2863.284±0.069 mas/yr Dec.: 336.529±0.039 mas/yr |
Parallax (π) | 280.7866 ± 0.0519 mas |
Distance | 11.616 ± 0.002 ly (3.5614 ± 0.0007 pc) |
Orbit | |
Companion | Groombridge 34 B |
Period (P) | 2,600 yr |
Semi-major axis (a) | 41.15″ |
Eccentricity (e) | 0.00 |
Inclination (i) | 61.4° |
Longitude of the node (Ω) | 45.3° |
Periastron epoch (T) | 1745 |
Details | |
Groombridge 34 A | |
Mass | 0.404 M☉ |
Radius | 0.3863 ± 0.0021 R☉ |
Luminosity (bolometric) | 0.02589 L☉ |
Luminosity (visual, LV) | 0.00637 L☉ |
Habitable zone inner limit | 0.112 AU |
Habitable zone outer limit | 0.239 AU |
Surface gravity (log g) | 4.89 cgs |
Temperature | 3,730 ± 49 K |
Metallicity | -0.32 dex |
Groombridge 34 B | |
Mass | 0.159 M☉ |
Radius | 0.192 R☉ |
Luminosity (bolometric) | ~0.00262 L☉ |
Luminosity (visual, LV) | 0.00041 L☉ |
Habitable zone inner limit | 0.048 AU |
Habitable zone outer limit | 0.103 AU |
Temperature | 3,218 K |
Metallicity | −0.30 dex |
Other designations | |
GX/GQ Andromedae, BD+43° 44, GCTP 49, GJ 15 A/B, G 171-047/171-048, HD 1326, HIP 1475, LHS 3/4, LTT 10108/10109, SAO 36248. | |
Database references | |
SIMBAD | GJ 15 A |
GJ 15 Ab | |
GJ 15 B | |
ARICNS | GJ 15 A |
GJ 15 B |
Groombridge 34 is a binary star system in the northern constellation of Andromeda. It was listed as entry number 34 in A Catalogue of Circumpolar Stars, published posthumously in 1838 by British astronomer Stephen Groombridge. Based upon parallax measurements taken by the Gaia spacecraft, the system is located about 11.6 light-years from the Sun. This positions the pair among the nearest stars to the Solar System.
Both components are small, dim red dwarf stars that are too faint to be seen with the naked eye. They orbit around their common barycenter in a nearly circular orbit with a separation of about 147 AU and a period of around 2,600 years. Both stars exhibit random variation in luminosity due to flares and they have been given variable star designations: the brighter member Groombridge 34 A is designated GX And, while the smaller component is designated GQ And.
The star system has a relatively high proper motion of 2.9 arc seconds per year, and is moving away from the Solar System at a velocity of 11.6 km/s. It achieved perihelion some 15,000 years ago when it came within 11 ly (3.5 pc) of the Sun.
Planetary system
In August 2014, a planet orbiting around Groombridge 34 A was reported. The planet's existence was deduced from analysis of the radial velocities of the parent Star by the Eta-Earth Survey using HIRES at Keck Observatory.
The planet is thought to have a minimum mass of 5.35 ± 0.75 Earth masses, and at its discovery was the sixth-nearest known exoplanet.
Using the CARMENES spectrograph combined with the measurements of the HARPS and HIRES spectrographs, researchers failed to detect the purported Groombridge 34 Ab. However, they did propose another that another planet (Groombridge 34 Ac, GJ 15 Ac) with a mass of 51.8 Earth masses and a long orbital period of about 7,026 days, could be orbiting the parent star.
Companion (in order from star) |
Mass | Semimajor axis (AU) |
Orbital period (days) |
Eccentricity | Inclination | Radius |
---|---|---|---|---|---|---|
Ab (disputed) | ≥ 5.35±0.75 M🜨 | 0.0717±0.0034 | 11.4433±0.0017 | 0.12? | — | — |
Ac | ≥ 51.8+5.5 −5.8 M🜨 |
5.18+0.47 −0.31 |
7025+972 −629 |
— | — | — |
See also
Notes
- ^ From , where is the luminosity, is the radius, is the effective surface temperature and is the Stefan–Boltzmann constant
- ^ Using the absolute visual magnitude of Gliese 15 A, , and Gliese 15 B, , with the absolute visual magnitude of the Sun, , the two visual luminosities of the stars can be calculated by
References
- ^ 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.
- ^ Mann, Andrew W.; et al. (May 2015), "How to Constrain Your M Dwarf: Measuring Effective Temperature, Bolometric Luminosity, Mass, and Radius", The Astrophysical Journal, 804 (1): 38, arXiv:1501.01635, Bibcode:2015ApJ...804...64M, doi:10.1088/0004-637X/804/1/64, 64.
- ^ 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.
- ^ Mermilliod, J.-C. (1986), "Compilation of Eggen's UBV data, transformed to UBV (unpublished)", Catalogue of Eggen's UBV data. SIMBAD, Bibcode:1986EgUBV........0M.
- ^ Nidever, David L.; et al. (August 2002), "Radial Velocities for 889 Late-Type Stars", The Astrophysical Journal Supplement Series, 141 (2): 503–522, arXiv:astro-ph/0112477, Bibcode:2002ApJS..141..503N, doi:10.1086/340570.
- ^ Lippincott, S. L. (March 1972), "Parallax and orbital motion of the two nearby long period visual binaries Groombridge 34 and ADS 9090.", Astronomical Journal, 77: 165–168, Bibcode:1972AJ.....77..165L, doi:10.1086/111261.
- ^ Berger, D. H.; et al. (2006). "First Results from the CHARA Array. IV. The Interferometric Radii of Low-Mass Stars". The Astrophysical Journal. 644 (1): 475–483. arXiv:astro-ph/0602105. Bibcode:2006ApJ...644..475B. doi:10.1086/503318.
- ^ Howard, Andrew W.; et al. (October 2014), "The NASA-UC-UH ETA-Earth Program. IV. A Low-mass Planet Orbiting an M Dwarf 3.6 PC from Earth", The Astrophysical Journal, 794 (1): 9, arXiv:1408.5645, Bibcode:2014ApJ...794...51H, doi:10.1088/0004-637X/794/1/51, 51.
- ^ Cantrell, Justin R.; et al. (October 2013), "The Solar Neighborhood XXIX: The Habitable Real Estate of Our Nearest Stellar Neighbors", The Astronomical Journal, 146 (4): 99, arXiv:1307.7038, Bibcode:2013AJ....146...99C, doi:10.1088/0004-6256/146/4/99.
- "V* GX And". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 2016-02-09.
{{cite web}}
: CS1 maint: postscript (link) - Groombridge, Stephen (1838), Airy, George Biddell (ed.), A Catalogue of Circumpolar Stars, J. Murray, p. 2.
- Petit, M. (October 1990), "Catalogue des étoiles variables ou suspectes dans le voisinage du Soleil", Astronomy and Astrophysics Supplement (in French), 85 (2): 971, Bibcode:1990A&AS...85..971P.
- ^ Bailer-Jones, C. A. L. (March 2015). "Close encounters of the stellar kind". Astronomy & Astrophysics. 575: 13. arXiv:1412.3648. Bibcode:2015A&A...575A..35B. doi:10.1051/0004-6361/201425221. A35.
{{cite journal}}
: CS1 maint: postscript (link) - Howard, Andrew; et al. (2014), "The NASA-UC-UH Eta-Earth Program: IV. A Low-mass Planet Orbiting an M Dwarf 3.6 PC from Earth", Astrophysics Earth and Planetary Astrophysics, 794: 51, arXiv:1408.5645, Bibcode:2014ApJ...794...51H, doi:10.1088/0004-637X/794/1/51.
- ^ Trifonov, T; Kürster, M; Zechmeister, M; Tal-Or, L; Caballero, J; Quirrenbach, A; Ribas, I; Reiners, A (2017). "The CARMENES search for exoplanets around M dwarfs. First visual-channel radial-velocity measurements and orbital parameter updates of seven M-dwarf planetary systems". Astronomy & Astrophysics. 609: A117. arXiv:1710.01595. Bibcode:2018A&A...609A.117T. doi:10.1051/0004-6361/201731442.
External links
- SolStation entry
- www.richweb.f9.co.uk/
- Image Groombridge 34
- The One Hundred Nearest Star Systems, RECONS
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