Astronomy:Gliese 849

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Short description: Star in the constellation Aquarius
Gliese 849
Observation data
Equinox J2000.0]] (ICRS)
Constellation Aquarius
Right ascension  22h 09m 40.34431s[1]
Declination –04° 38′ 26.6508″[1]
Apparent magnitude (V) 10.41[2]
Characteristics
Evolutionary stage Main sequence[3]
Spectral type M3.5V[4]
U−B color index 1.055[2]
B−V color index 1.531±0.035[2]
V−R color index 1.12[2]
R−I color index 1.41[2]
Astrometry
Radial velocity (Rv)−15.26±0.10[2] km/s
Proper motion (μ) RA: 1,132.583(39)[1] mas/yr
Dec.: −22.157(37)[1] mas/yr
Parallax (π)113.4447 ± 0.0300[1] mas
Distance28.750 ± 0.008 ly
(8.815 ± 0.002 pc)
Absolute magnitude (MV)10.62[2]
Details[5]
Mass0.465±0.011 M☉
Radius0.464±0.018 R☉
Luminosity0.02887±0.00025 L☉
Surface gravity (log g)4.771±0.032 cgs
Temperature3,467±68[6] K
Metallicity [Fe/H]0.09±0.09[6] dex
Rotation40.45+0.19
−0.18 d[6]
Rotational velocity (v sin i)2.4[3] km/s
Other designations
BD−05°5715, GJ 849, HIP 109388, LFT 1689, LHS 517, LPM 814, LTT 8889, NLTT 53078, 2MASS J22094029-0438267[7]
Database references
SIMBADdata
Exoplanet Archivedata
ARICNSdata
Planet
Gliese 849b data

Gliese 849, or GJ 849, is a small, solitary star in the equatorial constellation of Aquarius. It has a reddish hue and is invisible to the naked eye with an apparent visual magnitude of 10.41.[2] The distance to this star is 28.8 light-years (8.8 parsecs) based on parallax,[1] but it is drifting closer to the Sun with a radial velocity of −15.3 km/s.[2] It has a pair of confirmed gas giant companions.[8]

The stellar classification of GJ 849 is M3.5V,[4] which means this is a small red dwarf star generating energy through hydrogen fusion at its core region. Various studies have found super-solar abundances in the spectra,[8] indicating that the elemental abundances of higher mass elements is significantly higher than in the Sun. The star has about half the mass and size of the Sun,[3] and is spinning slowly with a rotation period of approximately 39 days.[9] The estimated age of the star is more than three billion years.[3] It is radiating a mere 2.9%[5] of the luminosity of the Sun from its photosphere at an effective temperature of 3,490 K.[5]

Planetary system

In late 2006, a long-period Jupiter-like exoplanet was reported to be orbiting the red dwarf in a period just over 5 years in length. There was also a linear trend in the radial velocities which suggested another longer period companion.[3] The trend in the radial velocities was confirmed in 2013.[10] An orbit for the second exoplanet was finally determined in 2015. The first planet discovered, Gliese 849 b, was the first planet discovered orbiting a red dwarf with a semi-major axis greater than 0.21 AU.[8]

The Gliese 849 planetary system[6]
Companion
(in order from star) 		Mass Semimajor axis
(AU) 		Orbital period
(days) 		Eccentricity Inclination Radius
b ≥0.893+0.094
−0.097 MJ 		2.32+0.11
−0.13 		1925.31±6.5 0.029±0.019 — —
c ≥0.99±0.11 MJ 4.95+0.25
−0.28 		5990+110
−100 		0.092+0.038
−0.036 		— —

See also

References

  1. ↑ 1.0 1.1 1.2 1.3 1.4 Vallenari, A. et al. (2022). "Gaia Data Release 3. Summary of the content and survey properties". Astronomy & Astrophysics. doi:10.1051/0004-6361/202243940  Gaia DR3 record for this source at VizieR.
  2. ↑ 2.0 2.1 2.2 2.3 2.4 2.5 2.6 2.7 2.8 Anderson, E.; Francis, Ch. (2012). "XHIP: An extended hipparcos compilation". Astronomy Letters 38 (5): 331. doi:10.1134/S1063773712050015. Bibcode: 2012AstL...38..331A. 
  3. ↑ 3.0 3.1 3.2 3.3 3.4 Butler, R. Paul et al. (2006). "A Long-Period Jupiter-Mass Planet Orbiting the Nearby M Dwarf GJ 849". Publications of the Astronomical Society of the Pacific 118 (850): 1685–1689. doi:10.1086/510500. Bibcode: 2006PASP..118.1685B. 
  4. ↑ 4.0 4.1 Schweitzer, A. et al. (May 2019). "The CARMENES search for exoplanets around M dwarfs. Different roads to radii and masses of the target stars". Astronomy & Astrophysics 625: 16. doi:10.1051/0004-6361/201834965. A68. Bibcode: 2019A&A...625A..68S. 
  5. ↑ 5.0 5.1 5.2 Pineda, J. Sebastian; Youngblood, Allison; France, Kevin (September 2021). "The M-dwarf Ultraviolet Spectroscopic Sample. I. Determining Stellar Parameters for Field Stars". The Astrophysical Journal 918 (1): 23. doi:10.3847/1538-4357/ac0aea. 40. Bibcode: 2021ApJ...918...40P. 
  6. ↑ 6.0 6.1 6.2 6.3 Pinamonti, M. et al. (June 2023). "The GAPS programme at TNG. XLVI. Deep search for low-mass planets in late-dwarf systems hosting cold Jupiters". Astronomy & Astrophysics 677. doi:10.1051/0004-6361/202346476. Bibcode: 2023A&A...677A.122P. 
  7. ↑ "BD-05 5715". SIMBAD. Centre de données astronomiques de Strasbourg. http://simbad.u-strasbg.fr/simbad/sim-basic?Ident=BD-05+5715. 
  8. ↑ 8.0 8.1 8.2 Feng, Y. Katherina et al. (2015). "The California Planet Survey IV: A Planet Orbiting the Giant Star HD 145934 and Updates to Seven Systems with Long-period Planets". The Astrophysical Journal 800 (1): 22. doi:10.1088/0004-637X/800/1/22. Bibcode: 2015ApJ...800...22F. 
  9. ↑ Suárez Mascareño, A. et al. (September 2015), "Rotation periods of late-type dwarf stars from time series high-resolution spectroscopy of chromospheric indicators", Monthly Notices of the Royal Astronomical Society 452 (3): 2745–2756, doi:10.1093/mnras/stv1441, Bibcode: 2015MNRAS.452.2745S. 
  10. ↑ Bonfils, Xavier; Delfosse, Xavier; Udry, Stéphane; Forveille, Thierry; Mayor, Michel; Perrier, Christian; Bouchy, François; Gillon, Michaël et al. (2011). "The HARPS search for southern extra-solar planets XXXI. The M-dwarf sample". Astronomy and Astrophysics 549: A109. doi:10.1051/0004-6361/201014704. Bibcode: 2013A&A...549A.109B. 

External links

Coordinates: Sky map 22h 09m 40.3460s, −4° 38′ 26.624″



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