Gliese 758

Gliese 758 is a star in the northern constellation of Lyra. At about magnitude 6 it is a challenge to view with the naked eye even in good seeing conditions, but can be easily seen through a small telescope or binoculars. Parallax measurements from the Hipparcos mission give it an estimated distance of around 51.4 light-years (15.8 parsecs) from Earth.

Gliese 758

Discovery image of Gliese 758 b, taken with Subaru HiCIAO in the near infrared.
Observation data
Epoch J2000.0      Equinox J2000.0
Constellation Lyra
Right ascension 19h 23m 34.01358s[1]
Declination +33° 13′ 19.0725″[1]
Apparent magnitude (V) 6.36[2]
Characteristics
Spectral type G8V[3]
U−B color index +0.455[2]
B−V color index +0.799[2]
Astrometry
Radial velocity (Rv)-21.6[4] km/s
Proper motion (μ) RA: 81.80[4] mas/yr
Dec.: 160.39[4] mas/yr
Parallax (π)64.06 ± 0.02[4] mas
Distance50.91 ± 0.02 ly
(15.610 ± 0.005 pc)
Absolute magnitude (MV)5.37[5]
Orbit[6]
PrimaryGliese 758 A
CompanionGliese 758 B
Period (P)96+21
−9 yr
Semi-major axis (a)21.1+2.7
−1.3 AU
Eccentricity (e)0.58+0.07
−0.11
Inclination (i)28+12
−10°
Longitude of the node (Ω)175±5°
Periastron epoch (T)2465800+2000
−800
Argument of periastron (ω)
(secondary)		184+8
−9°
Details
Mass0.966[7] M☉
Radius0.88[7] R☉
Surface gravity (log g)4.55[7] cgs
Temperature5404[4] K
Metallicity [Fe/H]0.18[3] dex
Age7.7–8.7[8] Gyr
Other designations
GJ 758, BD+32 3411, HD 182488, HIP 95319, HR 7368, PPM 82821, SAO 68239.[9]
Database references
SIMBADdata
Extrasolar Planets
Encyclopaedia		data

Properties

This is a Sun-like star with 97% of the Sun's mass and 88% of the radius of the Sun. The spectrum matches a stellar classification of G8V,[3] identifying it as a G-type main sequence star that is generating energy through the nuclear fusion of hydrogen at its core. It is radiating this energy into space from its outer envelope at an effective temperature of 5425 K.[3] Estimates of its age put it at about 7.7–8.7 billion years old,[8] although some measurements give it an age as low as 720 million years.[7] The abundance of elements other than hydrogen and helium, what astronomers term the star's metallicity, are 51% higher than in the Sun.[3]

System

In November 2009, a team using the HiCIAO instrument of the Subaru Telescope imaged a substellar companion orbiting the star. This object, designated Gliese 758 B, was estimated to be of approximately 10-40 Jupiter masses. A second candidate object was also detected, which was given the designation Gliese 758 C.[10][11] Follow-up studies of the system suggested the mass range of Gliese 758 B, indicating it to be a companion with approximately 30 to 40 Jupiter masses and revealed that Gliese 758 C is a background star which is not physically associated with the Gliese 758 system.[12] On the other hand, a younger age was suggested from the kinematic stellar grouping.

Orbit

Gliese 758 B is on an eccentric orbit with a semimajor axis of 21.1+2.7
−1.3 Astronomical units and an orbital period of 96+21
−9 years, which takes it within 9 astronomical units of its host star at its closest approach.[6]

See also

References
  1. 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.
  2. Breger, M. (March 1968), "UBV and narrow-band UVBY photometry of bright stars", Astronomical Journal, 73: 84–85, Bibcode:1968AJ.....73...84B, doi:10.1086/110602
  3. Soubiran, C.; et al. (2008). "Vertical distribution of Galactic disk stars. IV. AMR and AVR from clump giants". Astronomy and Astrophysics. 480 (1): 91–101. arXiv:0712.1370. Bibcode:2008A&A...480...91S. doi:10.1051/0004-6361:20078788.
  4. Gaia Collaboration; et al., "Gaia Data Release 2.", Astronomy and Astrophysics, in press (Special Issue), arXiv:1804.09365v2
  5. Holmberg, J.; Nordström, B.; Andersen, J. (July 2009), "The Geneva-Copenhagen survey of the solar neighbourhood. III. Improved distances, ages, and kinematics", Astronomy and Astrophysics, 501 (3): 941–947, arXiv:0811.3982, Bibcode:2009A&A...501..941H, doi:10.1051/0004-6361/200811191
  6. Bowler, Brendan P.; et al. (2018). "Orbit and Dynamical Mass of the Late-T Dwarf Gl 758 B". arXiv:1802.10126.
  7. Takeda, Genya; et al. (February 2007), "Structure and Evolution of Nearby Stars with Planets. II. Physical Properties of ~1000 Cool Stars from the SPOCS Catalog", The Astrophysical Journal Supplement Series, 168 (2): 297–318, arXiv:astro-ph/0607235, Bibcode:2007ApJS..168..297T, doi:10.1086/509763
  8. Mamajek, Eric E.; Hillenbrand, Lynne A. (November 2008), "Improved Age Estimation for Solar-Type Dwarfs Using Activity-Rotation Diagnostics", The Astrophysical Journal, 687 (2): 1264–1293, arXiv:0807.1686, Bibcode:2008ApJ...687.1264M, doi:10.1086/591785
  9. "HD 182488". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 2009-12-13.
  10. Thalmann, C.; et al. (2009), "Discovery of the Coldest Imaged Companion of a Sun-Like Star", The Astrophysical Journal Letters, 707 (2): L123–L127, arXiv:0911.1127, Bibcode:2009ApJ...707L.123T, doi:10.1088/0004-637X/707/2/L123
  11. "Discovery of an Exoplanet Candidate Orbiting a Sun-Like Star: Inaugural Observations with Subaru's New Instrument HiCIAO", Subaru Telescope, 2009-12-03, retrieved 2009-12-04
  12. Janson, M.; Carson, J.; Thalmann, C.; McElwain, M. W.; Goto, M.; Crepp, J.; Wisniewski, J.; Abe, L.; Brandner, W.; Burrows, A.; Egner, S.; Feldt, M.; Grady, C. A.; Golota, T.; Guyon, O.; Hashimoto, J.; Hayano, Y.; Hayashi, M.; Hayashi, S.; Henning, T.; Hodapp, K. W.; Ishii, M.; Iye, M.; Kandori, R.; Knapp, G. R.; Kudo, T.; Kusakabe, N.; Kuzuhara, M.; Matsuo, T.; Mayama, S.; Miyama, S.; Morino, J.-I.; Moro-Martín, A.; Nishimura, T.; Pyo, T.-S.; Serabyn, E.; Suto, H.; Suzuki, R.; Takami, M.; Takato, N.; Terada, H.; Tofflemire, B.; Tomono, D.; Turner, E. L.; Watanabe, M.; Yamada, T.; Takami, H.; Usuda, T.; Tamura, M. (2011), "Near-infrared Multi-band Photometry of the Substellar Companion GJ 758 B", The Astrophysical Journal, 728 (2), arXiv:1011.5505, Bibcode:2011ApJ...728...85J, doi:10.1088/0004-637X/728/2/85

This article is issued from Wikipedia. The text is licensed under Creative Commons - Attribution - Sharealike. Additional terms may apply for the media files.