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Gliese 22

From Wikipedia, the free encyclopedia
Star in the constellation Cassiopeia
Gliese 22

Ablue bandlight curve for a flare of Gliese 22A, adapted from Pettersen (1975)[1]
Observation data
EpochJ2000.0      EquinoxJ2000.0
ConstellationCassiopeia
Gliese 22 A
Right ascension00h 32m 29.4336s
Declination+67° 14′ 08.409″
Apparent magnitude (V)10.29
Gliese 22 B
Right ascension00h 32m 29.575s
Declination+67° 14′ 04.63″
Apparent magnitude (V)12.19
Gliese 22 C
Right ascension00h 32m 29.4s
Declination+67° 14′ 08″
Apparent magnitude (V)13.2
Characteristics
Spectral typeM2.5Ve / M3V
U−Bcolor index1.16
B−Vcolor index1.54
R−Icolor index0.99
Variable typeFlare stars
Astrometry
Radial velocity (Rv)10 km/s
Proper motion (μ)RA: 1739.0mas/yr
Dec.: −224.93mas/yr
Parallax (π)99.35±2.17 mas[2]
Distance32.8 ± 0.7 ly
(10.1 ± 0.2 pc)
Absolute magnitude (MV)11.83
Orbit[3]
PrimaryGliese 22 AC
CompanionGliese 22 B
Period (P)223.3yr
Semi-major axis (a)3.322″
Eccentricity (e)0.293
Inclination (i)47.3°
Longitude of the node (Ω)174.9°
Periastronepoch (T)JD 1859.4
Argument of periastron (ω)
(secondary)
146.3°
Orbit[4]
PrimaryGliese 22 A (Aa)
CompanionGliese 22 C (Ab)
Period (P)5,694.2±14.9 days
Semi-major axis (a)0.5106±0.0007
Eccentricity (e)0.163±0.002
Inclination (i)43.7±0.2°
Longitude of the node (Ω)178.3±0.2°
Periastronepoch (T)JD 51817.2
Argument of periastron (ω)
(secondary)
284.5±0.5°
Details[5]
Mass0.378(A) + 0.136(C) M
Radius0.5(A) R
Luminosity0.04 L
Temperature2000–3500 K
Details
B
Mass0.382[6] M
Radius0.394[6] R
Luminosity0.011[7] L
Temperature3,339[8] K
Metallicity [Fe/H]−0.24[9] dex
Rotational velocity (v sin i)<4[10] km/s
Other designations
2MASS J00322970+6714080,BD+66°34,CCDM J00325+6714,GJ 22,HIP 2552,LFT 47,V547 Cassiopeiae, ADS 440
Database references
SIMBADdata
Exoplanet Archivedata

Gliese 22, also cataloguedV547 Cassiopeiae orADS 440, is a hierarchicalstar system approximately 33light-years away in theconstellation ofCassiopeia. The system consists of pair ofred dwarfstars, Gliese 22A and Gliese 22C, orbited by a third red dwarf Gliese 22B in an outer orbit of about 223 years.

The discovery offlare activity on Gliese 22A was announced by Bjørn Ragnvald Pettersen in 1975,[1] which led to it being given avariable star designation, V547 Cassiopeiae, in 1977.[11]

Planetary system

[edit]

As of 2008, it was announced that a possibleextrasolar planet, Gliese 22B b, orbits Gliese 22B but this is currently unconfirmed. The study in 2011 has indicated the orbit of the purported planet is stable.[12]

The Gliese 22 B planetary system
Companion
(in order from star)
MassSemimajor axis
(AU)
Orbital period
(days)
EccentricityInclinationRadius
b(unconfirmed)16MJ5,5000

References

[edit]
  1. ^abPettersen, B. R. (June 1975)."Discovery of flare activity on BD +66 34 (= Gliese 22 A)".Astronomy and Astrophysics.41: 113.Bibcode:1975A&A....41..113P.Archived from the original on 27 November 2021. Retrieved27 November 2021.
  2. ^van Leeuwen, F. (November 2007). "Validation of the new Hipparcos reduction".Astronomy and Astrophysics.474 (2):653–664.arXiv:0708.1752.Bibcode:2007A&A...474..653V.doi:10.1051/0004-6361:20078357.S2CID 18759600.
  3. ^Docobo, J. A.; Tamazian, V. S.; Balega, Y. Y.; Andrade, M.; Schertl, D.; Weigelt, G.; Campo, P.; Palacios, M. (2008)."A methodology for studying physical and dynamical properties of multiple stars. Application to the system of red dwarfs Gl 22".Astronomy and Astrophysics.478 (1): 187.Bibcode:2008A&A...478..187D.doi:10.1051/0004-6361:20078594.
  4. ^Benedict, G. F.; et al. (2016)."The Solar Neighborhood. XXXVII: The Mass-Luminosity Relation for Main-sequence M Dwarfs".The Astronomical Journal.152 (5). 141.arXiv:1608.04775.Bibcode:2016AJ....152..141B.doi:10.3847/0004-6256/152/5/141.
  5. ^McCarthy, D. W.; Henry, Todd J.; McLeod, Brian; Christou, Julian C. (1991). "The Low-Mass Companion of Gliese 22A: First Results of the Steward Infrared Speckle Camera".The Astronomical Journal.101: 214.Bibcode:1991AJ....101..214M.doi:10.1086/115681.
  6. ^abNewton, Elisabeth R.; Irwin, Jonathan; Charbonneau, David; Berlind, Perry; Calkins, Michael L.; Mink, Jessica (2017)."The Hα Emission of Nearby M Dwarfs and its Relation to Stellar Rotation".The Astrophysical Journal.834 (1): 85.arXiv:1611.03509.Bibcode:2017ApJ...834...85N.doi:10.3847/1538-4357/834/1/85.S2CID 55000202.
  7. ^McLean, M.; Berger, E.; Reiners, Ansgar (February 2012). "The Radio Activity-Rotation Relation of Ultracool Dwarfs".The Astrophysical Journal.746 (1): 23.arXiv:1108.0415.Bibcode:2012ApJ...746...23M.doi:10.1088/0004-637X/746/1/23.S2CID 119159519.
  8. ^Houdebine, Éric R.; Mullan, D. J.; Doyle, J. G.; de la Vieuville, Geoffroy; Butler, C. J.; Paletou, F. (2019)."The Mass-Activity Relationships in M and K Dwarfs. I. Stellar Parameters of Our Sample of M and K Dwarfs".The Astronomical Journal.158 (2): 56.arXiv:1905.07921.Bibcode:2019AJ....158...56H.doi:10.3847/1538-3881/ab23fe.S2CID 159041104.
  9. ^Mann, Andrew W.; Dupuy, Trent; Kraus, Adam L.; Gaidos, Eric; Ansdell, Megan; Ireland, Michael; Rizzuto, Aaron C.; Hung, Chao-Ling; Dittmann, Jason; Factor, Samuel; Feiden, Gregory; Martinez, Raquel A.; Ruíz-Rodríguez, Dary; Chia Thao, Pa (2019), "How to constrain your M dwarf. II. The Mass-Luminosity-Metallicity relation from 0.075 to 0.70 solar masses",The Astrophysical Journal,871 (1): 63,arXiv:1811.06938,Bibcode:2019ApJ...871...63M,doi:10.3847/1538-4357/aaf3bc,S2CID 119372932
  10. ^Jeffers, S. V.; Schöfer, P.; Lamert, A.; Reiners, A.; Montes, D.; Caballero, J. A.; Cortés-Contreras, M.; Marvin, C. J.; Passegger, V. M.; Zechmeister, M.; Quirrenbach, A.; Alonso-Floriano, F. J.; Amado, P. J.; Bauer, F. F.; Casal, E.; Diez Alonso, E.; Herrero, E.; Morales, J. C.; Mundt, R.; Ribas, I.; Sarmiento, L. F. (2018). "CARMENES input catalogue of M dwarfs. III. Rotation and activity from high-resolution spectroscopic observations".Astronomy and Astrophysics.614: A76.arXiv:1802.02102.Bibcode:2018A&A...614A..76J.doi:10.1051/0004-6361/201629599.S2CID 56147445.
  11. ^Kukarkin, B. V.; Kholopov, P. N.; Fedorovich, V. P.; Kireyeva, N. N.; Kukarkina, N. P.; Medvedeva, G. I.; Perova, N. B. (March 1977)."62nd Name-List of Variable Stars".Information Bulletin on Variable Stars.1248 (1248): 1.Bibcode:1977IBVS.1248....1K. Retrieved28 August 2024.
  12. ^Andrade, Manuel; Docobo, José A. (2011). "On the dynamical stability of the very low-mass object Gliese 22 Bb".Icarus.215 (2): 712.Bibcode:2011Icar..215..712A.doi:10.1016/j.icarus.2011.07.008.

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