ADS 16402
Observation data Epoch J2000.0 Equinox J2000.0 | |
---|---|
Constellation | Lacerta[1] |
ADS 16402 A | |
Right ascension | 22h 57m 45.9211s[2] |
Declination | +38° 40′ 27.198″[2] |
Apparent magnitude (V) | +10.0[3] |
ADS 16402 B (HAT-P-1) | |
Right ascension | 22h 57m 46.8443s[2] |
Declination | +38° 40′ 30.355″[2] |
Apparent magnitude (V) | +10.4[3] |
Characteristics | |
ADS 16402 A | |
Spectral type | F8[3]/G0V[4] |
Apparent magnitude (J) | 8.670±0.021[5] |
Apparent magnitude (H) | 8.467±0.044[5] |
Apparent magnitude (K) | 8.405±0.020[5] |
ADS 16402 B (HAT-P-1) | |
Spectral type | F8[3]/G0V[4] |
Apparent magnitude (J) | 9.156±0.026[5] |
Apparent magnitude (H) | 8.923±0.030[5] |
Apparent magnitude (K) | 8.858±0.018[5] |
Astrometry | |
ADS 16402 A | |
Radial velocity (Rv) | −3.43 ± 0.32[4] km/s |
Proper motion (μ) | RA: 32.128±0.042[2] mas/yr Dec.: −41.969±0.044[2] mas/yr |
Parallax (π) | 6.1989 ± 0.0387 mas[2] |
Distance | 526 ± 3 ly (161 ± 1 pc) |
Absolute magnitude (MV) | 3.4 ± 0.3[4] |
ADS 16402 B (HAT-P-1) | |
Radial velocity (Rv) | −2.94 ± 0.56[4] km/s |
Proper motion (μ) | RA: 32.384±0.041[2] mas/yr Dec.: −41.751±0.044[2] mas/yr |
Parallax (π) | 6.2615 ± 0.0381 mas[2] |
Distance | 521 ± 3 ly (159.7 ± 1.0 pc) |
Absolute magnitude (MV) | 3.7 ± 0.3[4] |
Details | |
ADS 16402 A | |
Mass | 1.16 ± 0.11[4] M☉ |
Radius | 1.123 +0.14 −0.10[4] R☉ |
Luminosity | 1.82 +0.75 −0.53[4] L☉ |
Surface gravity (log g) | 4.36 ± 0.03[6] cgs |
Temperature | 6251 ± 17[6] K |
Metallicity [Fe/H] | 0.146 ± 0.014[6] dex |
Rotational velocity (v sin i) | 7.1 ± 0.3[4] km/s |
Age | 1.9 ± 0.6[7] Gyr |
ADS 16402 B (HAT-P-1) | |
Mass | 1.151 +0.052 −0.051[8] M☉ |
Radius | 1.174 +0.026 −0.027[8] R☉ |
Luminosity | 1.585 +0.099 −0.094[8] L☉ |
Surface gravity (log g) | 4.43 ± 0.02[6] cgs |
Temperature | 6049 ± 8[6] K |
Metallicity [Fe/H] | 0.155 ± 0.007[6] dex |
Rotational velocity (v sin i) | 2.2 ± 0.2[4] km/s |
Age | 1.9 ± 0.6[7] Gyr |
Position (relative to ADS 16402 A) | |
Angular distance | 11.26 ± 0.03″ [9] |
Other designations | |
ADS 16402 A: BD+37 4734p, PPM 88381[3] | |
ADS 16402 B: HAT-P-1, BD+37° 4734s, PPM 88382[3] | |
Database references | |
SIMBAD | ADS 16402 |
ADS 16402 A | |
HAT-P-1 |
ADS 16402 is a binary star system, composed of two sun-like stars located approximately 525 light-years away in the constellation Lacerta. It was first identified by John Herschel in 1831.[4] The two stars are separated by 11.26 arcseconds which leads to a projected separation of roughly 1500 astronomical units at the distance of ADS 16402. The star system is estimated to be 1.9 ± 0.6 billion years old.[7] The secondary star ADS 16402 B is also designated HAT-P-1.
Planetary system
On September 14, 2006 the HATNet Project announced their first extrasolar planet discovery HAT-P-1b, a hot jupiter type gas giant in orbit around the secondary star ADS 16402B. Following the designation scheme used by the HATNet Project, the secondary star is known as HAT-P-1, and the planet itself designated HAT-P-1b.[4][10]
Companion (in order from star) |
Mass | Semimajor axis (AU) |
Orbital period (days) |
Eccentricity | Inclination | Radius |
---|---|---|---|---|---|---|
b | 0.529 ± 0.020 MJ | 0.05561 ± 0.00083 | 4.4652968 ± 0.0000018 | 0 | 85.634 ± 0.056° | 1.319 ± 0.019 RJ |
See also
- HATNet Project or HAT
References
- ^ 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 f g h i j Brown, A. G. A.; et al. (Gaia collaboration) (August 2018). "Gaia Data Release 2: Summary of the contents and survey properties". Astronomy & Astrophysics. 616. A1. arXiv:1804.09365. Bibcode:2018A&A...616A...1G. doi:10.1051/0004-6361/201833051. Gaia Data Release 2 catalog entry for ADS 16402 A Gaia Data Release 2 catalog entry for ADS 16402 B
- ^ a b c d e f g "ADS16402". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 2009-05-10.
- ^ a b c d e f g h i j k l m Bakos, G. Á.; et al. (2007). "HAT-P-1b: A Large-Radius, Low-Density Exoplanet Transiting One Member of a Stellar Binary". The Astrophysical Journal. 656 (1): 552–559. arXiv:astro-ph/0609369. Bibcode:2007ApJ...656..552B. doi:10.1086/509874.
- ^ a b c d e f Skrutskie, M. F.; et al. (2006). "The Two Micron All Sky Survey (2MASS)". The Astronomical Journal. 131 (2): 1163–1183. Bibcode:2006AJ....131.1163S. doi:10.1086/498708.Vizier catalog entry for AVizier catalog entry for B
- ^ a b c d e f Liu, F.; et al. (2014). "A high-precision chemical abundance analysis of the HAT-P-1 stellar binary: constraints on planet formation". Monthly Notices of the Royal Astronomical Society. 442 (1): L51–L55. arXiv:1404.2112. Bibcode:2014MNRAS.442L..51L. doi:10.1093/mnrasl/slu055.
- ^ a b c Bonfanti, A.; et al. (2015). "Revising the ages of planet-hosting stars". Astronomy and Astrophysics. 575. A18. arXiv:1411.4302. Bibcode:2015A&A...575A..18B. doi:10.1051/0004-6361/201424951.
- ^ a b c d Nikolov, N.; et al. (2014). "Hubble Space Telescope hot Jupiter transmission spectral survey: a detection of Na and strong optical absorption in HAT-P-1b". Monthly Notices of the Royal Astronomical Society. 437 (1): 46–66. arXiv:1310.0083. Bibcode:2014MNRAS.437...46N. doi:10.1093/mnras/stt1859.
- ^ Faedi, F.; et al. (2013). "Lucky imaging of transiting planet host stars with LuckyCam". Monthly Notices of the Royal Astronomical Society. 433 (3): 2097–2106. arXiv:1305.3795. Bibcode:2013MNRAS.433.2097F. doi:10.1093/mnras/stt885.
- ^ Aguilar, David A.; Pulliam, Christine (September 14, 2006). "Strange New Planet Baffles Astronomers" (Press release). Cambridge, Massachusetts: Harvard–Smithsonian Center for Astrophysics. Retrieved November 18, 2016.
- ^ Turner, Jake D.; et al. (2016). "Ground-based near-UV observations of 15 transiting exoplanets: constraints on their atmospheres and no evidence for asymmetrical transits". Monthly Notices of the Royal Astronomical Society. 459 (1): 789–819. arXiv:1603.02587. Bibcode:2016MNRAS.459..789T. doi:10.1093/mnras/stw574.
External links
- "Planet HAT-P-1 b". The Extrasolar Planets Encyclopaedia. Retrieved 2018-05-06.