GSC 02652-01324 is an orange dwarf main sequence star approximately 521 light-years away in the constellation of Lyra (the Lyre).[5][2][3]
Observation data Epoch J2000.0 Equinox J2000.0 | |
---|---|
Constellation | Lyra[2] |
Right ascension | 19h 04m 09.8516s[3] |
Declination | +36° 37′ 57.447″[3] |
Apparent magnitude (V) | +11.806[4] |
Characteristics | |
Spectral type | K0V[5] |
Apparent magnitude (B) | 12.405±0.005[4] |
Apparent magnitude (V) | 11.806[4] |
Apparent magnitude (J) | 10.294±0.022[6] |
Apparent magnitude (H) | 9.887±0.021[6] |
Apparent magnitude (K) | 9.819±0.019[6] |
Variable type | Planetary transit variable[5] |
Astrometry | |
Proper motion (μ) | RA: −32.168(12) mas/yr[3] Dec.: −20.463(13) mas/yr[3] |
Parallax (π) | 6.2648 ± 0.0111 mas[3] |
Distance | 520.6 ± 0.9 ly (159.6 ± 0.3 pc) |
Absolute magnitude (MV) | +5.81[citation needed] |
Details[citation needed] | |
Mass | 0.87 ± 0.03 M☉ |
Radius | 0.82 ±0.02 R☉ |
Luminosity | 0.49 L☉ |
Temperature | 5250 K |
Metallicity | 0.001 ± 0.004 |
Age | 2.5±1.4 Gyr |
Other designations | |
Database references | |
SIMBAD | data |
Planetary system
editIn 2004 the extrasolar planet TrES-1b was found to be orbiting this star by the Trans-Atlantic Exoplanet Survey using the transit method. The planet was detected crossing its parent star using a small 4-inch-diameter (100 mm) telescope. The discovery was confirmed by the Keck Observatory using the radial velocity method, allowing its mass to be determined.[5][8]
Additional planets in the systems are suspected due to transit timing variations of TrES-1b.[9]
Companion (in order from star) |
Mass | Semimajor axis (AU) |
Orbital period (days) |
Eccentricity | Inclination | Radius |
---|---|---|---|---|---|---|
b | 0.697+0.028 −0.027 MJ |
0.03926+0.00058 −0.00060 |
3.0300689±0.0000007[9] | <0.012 | 90+0 −1.1° |
1.067+0.021 −0.022 RJ |
See also
editReferences
edit- ^ Winn, Joshua N.; Holman, Matthew J.; Roussanova, Anna (10 March 2007). "The Transit Light Curve Project. III. Tres Transits of TrES-1". The Astrophysical Journal. 657 (2): 1098–1106. doi:10.1086/510834. Retrieved 31 August 2024.
- ^ a b Roman, Nancy G. (1987). "Identification of a Constellation From a Position". Publications of the Astronomical Society of the Pacific. 99 (617): 695–699. Bibcode:1987PASP...99..695R. doi:10.1086/132034. Vizier query form
- ^ a b c d e 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 Henden, A. A.; et al. (2016). "VizieR Online Data Catalog: AAVSO Photometric All Sky Survey (APASS) DR9 (Henden+, 2016)". VizieR On-line Data Catalog: II/336. Originally Published in: 2015AAS...22533616H. 2336. Bibcode:2016yCat.2336....0H.Vizier catalog entry
- ^ a b c d Alonso, Roi; et al. (2004). "TrES-1: The Transiting Planet of a Bright K0V Star". The Astrophysical Journal Letters. 613 (2): L153–L156. arXiv:astro-ph/0408421. Bibcode:2004ApJ...613L.153A. doi:10.1086/425256. S2CID 8940599.
- ^ a b c Skrutskie, Michael F.; Cutri, Roc M.; Stiening, Rae; Weinberg, Martin D.; Schneider, Stephen E.; Carpenter, John M.; Beichman, Charles A.; Capps, Richard W.; Chester, Thomas; Elias, Jonathan H.; Huchra, John P.; Liebert, James W.; Lonsdale, Carol J.; Monet, David G.; Price, Stephan; Seitzer, Patrick; Jarrett, Thomas H.; Kirkpatrick, J. Davy; Gizis, John E.; Howard, Elizabeth V.; Evans, Tracey E.; Fowler, John W.; Fullmer, Linda; Hurt, Robert L.; Light, Robert M.; Kopan, Eugene L.; Marsh, Kenneth A.; McCallon, Howard L.; Tam, Robert; Van Dyk, Schuyler D.; Wheelock, Sherry L. (1 February 2006). "The Two Micron All Sky Survey (2MASS)". The Astronomical Journal. 131 (2): 1163–1183. Bibcode:2006AJ....131.1163S. doi:10.1086/498708. ISSN 0004-6256. S2CID 18913331. Vizier catalog entry
- ^ "TrES-1 Parent Star". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 2018-02-01.
- ^ "Keck confirms transit planet" (Press release). Kamuela, Hawaii: W. M. Keck Observatory. August 24, 2004. Retrieved August 14, 2019.
- ^ a b Yeung, Paige; Perian, Quinn; Robertson, Peyton; Fitzgerald, Michael; Fowler, Martin; Sienkiewicz, Frank; Tock, Kalee (2022), "Searching for Transit Timing Variations and Fitting a New Ephemeris to Transits of Tres-1 B", Journal of the Korean Astronomical Society, 55 (4): 111, arXiv:2207.01559, Bibcode:2022JKAS...55..111Y, doi:10.5303/JKAS.2022.55.4.111, S2CID 250264173
- ^ Bonomo, A. S.; et al. (2017). "The GAPS Programme with HARPS-N at TNG . XIV. Investigating giant planet migration history via improved eccentricity and mass determination for 231 transiting planets". Astronomy and Astrophysics. 602. A107. arXiv:1704.00373. Bibcode:2017A&A...602A.107B. doi:10.1051/0004-6361/201629882. S2CID 118923163.
- ^ Baluev, Roman V.; et al. (2015). "Benchmarking the power of amateur observatories for TTV exoplanets detection". Monthly Notices of the Royal Astronomical Society. 450 (3): 3101–3113. arXiv:1501.06748. Bibcode:2015MNRAS.450.3101B. doi:10.1093/mnras/stv788. S2CID 15420110.
- ^ Torres, Guilermo; et al. (2008). "Improved Parameters for Extrasolar Transiting Planets". Astrophysical Journal. 677 (2): 1324–1342. arXiv:0801.1841. Bibcode:2008ApJ...677.1324T. doi:10.1086/529429. S2CID 12899134.
External links
edit- "Planet TRES-1 b". Extrasolar Planets Encyclopaedia. Retrieved 2018-11-28.