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 34.013166s[1] |
| Declination | +33° 13′ 19.078368″[1] |
| Apparent magnitude (V) | 6.36[2] |
| Characteristics | |
| Spectral type | G8V[3]+T7[4] |
| U−B color index | +0.455[2] |
| B−V color index | +0.799[2] |
| Astrometry | |
| Radial velocity (Rv) | −21.62±0.12[1] km/s |
| Proper motion ( | RA: 81.966±0.013 mas/yr[1] Dec.: 160.158±0.016 mas/yr[1] |
| Parallax ( | 64.0703 ± 0.0154 mas[1] |
| Distance | 50.91 ± 0.01 ly (15.608 ± 0.004 pc) |
| Absolute magnitude (MV) | 5.37[5] |
| Orbit[6] | |
| Primary | Gliese 758 A |
| Companion | Gliese 758 B |
| Period (P) | 131.276+15.078 −12.080 yr |
| Semi-major axis (a) | 25.409+1.944 −1.626 |
| Eccentricity (e) | 0.365+0.079 −0.082 |
| Inclination (i) | 38.080+5.438 −4.808° |
| Longitude of the node ( | 349.680+5.776 −6.263° |
| Periastron epoch (T) | 2,421,289.845+3,708.120 −4,680.545 |
| Argument of periastron ( (secondary) | 175.102+11.951 −14.709° |
| Semi-amplitude (K1) (primary) | 0.139318+0.009603 −0.008036 km/s |
| Details | |
| Gliese 758 A | |
| Mass | 0.93±0.03[6] M☉ |
| Radius | 0.88[7] R☉ |
| Surface gravity (log g) | 4.55[7] cgs |
| Temperature | 5305[1] K |
| Metallicity [Fe/H] | 0.18[3] dex |
| Age | 7.7–8.7[8] Gyr |
| Gliese 758 B | |
| Mass | 36.387+1.210 −1.081[6] MJup |
| Surface gravity (log g) | 4.3 ±0.5[4] cgs |
| Temperature | 741 ±25[4] K |
| Other designations | |
| Database references | |
| SIMBAD | A |
| B | |
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 50.9 light-years (15.6 parsecs) from Earth.
Properties
[edit]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 5,425 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]
Companion
[edit]In November 2009, a team using the HiCIAO instrument of the Subaru Telescope imaged a substellar companion orbiting the star. This brown dwarf, designated Gliese 758 B, was estimated to be of approximately 10 to 40 Jupiter masses. A second candidate object was also detected, which was given the designation Gliese 758 C.[10][11][12] Follow-up studies of the system refined 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.[13] On the other hand, a younger age was suggested from the kinematic stellar grouping.
The most recent parameters for Gliese 758 B as of 2022 come from a combination of data from radial velocity, astrometry, and imaging,[14][15][6] showing that it is about 36 times the mass of Jupiter, and on an eccentric orbit with a semi-major axis of about 25.4 astronomical units and an orbital period of about 131 years.[6]
First near-infrared spectroscopy was published in 2017. This team used the Hale Telescope at Palomar Observatory to obtain a low-resolution spectrum. Comparison with archived IRTF/SpeX spectra of brown dwarfs resulted in a best fit to a spectral type of T7.0 ±1.0. The modelling of the spectrum indicates a temperature of 741 ± 25 K, which is slightly hotter than previously thought. A later spectral type and lower temperature is not excluded.[4]
See also
[edit]References
[edit]- ^ a b c d e f Vallenari, A.; et al. (Gaia collaboration) (2023). "Gaia Data Release 3. Summary of the content and survey properties". Astronomy and Astrophysics. 674: A1. arXiv:2208.00211. Bibcode:2023A&A...674A...1G. doi:10.1051/0004-6361/202243940. S2CID 244398875. Gaia DR3 record for this source at VizieR.
- ^ a b c 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
- ^ a b c d e 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. S2CID 16602121.
- ^ a b c d Nilsson, R.; Veicht, A.; Giorla Godfrey, P. A.; Rice, E. L.; Aguilar, J.; Pueyo, L.; Roberts, L. C., Jr.; Oppenheimer, R.; Brenner, D.; Luszcz-Cook, S. H.; Bacchus, E.; Beichman, C.; Burruss, R.; Cady, E.; Dekany, R. (2017-03-01). "Project 1640 Observations of Brown Dwarf GJ 758 B: Near-infrared Spectrum and Atmospheric Modeling". The Astrophysical Journal. 838: 64. arXiv:1703.01023. Bibcode:2017ApJ...838...64N. doi:10.3847/1538-4357/aa643c. ISSN 0004-637X.
{{cite journal}}: CS1 maint: multiple names: authors list (link) CS1 maint: unflagged free DOI (link) - ^ 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, S2CID 118577511
- ^ a b c d e Feng, Fabo; Butler, R. Paul; et al. (August 2022). "3D Selection of 167 Substellar Companions to Nearby Stars". The Astrophysical Journal Supplement Series. 262 (21): 21. arXiv:2208.12720. Bibcode:2022ApJS..262...21F. doi:10.3847/1538-4365/ac7e57. S2CID 251864022.
- ^ a b c 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, S2CID 18775378
- ^ a b 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, S2CID 27151456
- ^ "HD 182488". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 2009-12-13.
- ^ 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, S2CID 116823073
- ^ "Possible Planet Around a G-class Star". Centauri Dreams. 2009-12-04. Archived from the original on 2016-01-29. Retrieved 2009-12-04.
- ^ "Discovery of an Exoplanet Candidate Orbiting a Sun-Like Star: Inaugural Observations with Subaru's New Instrument HiCIAO", Subaru Telescope, 2009-12-03, archived from the original on 2012-06-21, retrieved 2009-12-04
- ^ Janson, M.; Carson, J.; Thalmann, C.; McElwain, M. W.; Goto, M.; Crepp, J.; Wisniewski, J.; Abe, L.; Brandner, W.; Burrows, Adam; Egner, S.; Feldt, M.; Grady, C. A.; Golota, T.; Guyon, Olivier; 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): 85, arXiv:1011.5505, Bibcode:2011ApJ...728...85J, doi:10.1088/0004-637X/728/2/85, S2CID 119296265
- ^ Bowler, Brendan P.; et al. (2018). "Orbit and Dynamical Mass of the Late-T Dwarf GL 758 B". The Astronomical Journal. 155 (4): 159. arXiv:1802.10126. Bibcode:2018AJ....155..159B. doi:10.3847/1538-3881/aab2a6. S2CID 54816662.
- ^ Brandt, G. Mirek; Dupuy, Trent J.; et al. (December 2021). "Improved Dynamical Masses for Six Brown Dwarf Companions Using Hipparcos and Gaia EDR3". The Astronomical Journal. 162 (6): 301. arXiv:2109.07525. Bibcode:2021AJ....162..301B. doi:10.3847/1538-3881/ac273e. S2CID 237532125.
External links
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