HAT-P-4 is a wide binary star consisting of a pair of G-type main-sequence stars[5] in the constellation of Boötes.[1] It is also designated BD+36°2593.
| Observation data Epoch J2000 Equinox J2000 | |
|---|---|
| Constellation | Boötes[1] |
| HAT-P-4A | |
| Right ascension | 15h 19m 57.9204s[2] |
| Declination | +36° 13′ 46.738″[2] |
| Apparent magnitude (V) | 11.159±0.010[3] |
| HAT-P-4B | |
| Right ascension | 15h 20m 00.0127s[4] |
| Declination | +36° 12′ 18.520″[4] |
| Apparent magnitude (V) | 11.534±0.01[3] |
| Characteristics | |
| HAT-P-4A | |
| Spectral type | G0V[5] |
| B−V color index | 0.771 |
| Variable type | planetary transit[6] |
| HAT-P-4B | |
| Spectral type | G2V[5] |
| Astrometry | |
| HAT-P-4A | |
| Radial velocity (Rv) | −1.13(37)[2] km/s |
| Proper motion (μ) | RA: −21.513(13) mas/yr[2] Dec.: −24.255(19) mas/yr[2] |
| Parallax (π) | 3.1071 ± 0.0154 mas[2] |
| Distance | 1,050 ± 5 ly (322 ± 2 pc) |
| HAT-P-4B | |
| Radial velocity (Rv) | −1.31(35)[4] km/s |
| Proper motion (μ) | RA: −21.424(13) mas/yr[4] Dec.: −24.182(20) mas/yr[4] |
| Parallax (π) | 3.0777 ± 0.0155 mas[4] |
| Distance | 1,060 ± 5 ly (325 ± 2 pc) |
| Details | |
| HAT-P-4A | |
| Mass | 1.260+0.043 −0.042[7] M☉ |
| Radius | 1.573±0.015[7] R☉ |
| Luminosity | 0.41 L☉ |
| Surface gravity (log g) | 4.145±0.015[7] cgs |
| Temperature | 5927+57 −47[7] K |
| Metallicity [Fe/H] | 0.277±0.007[8] dex |
| Rotational velocity (v sin i) | 5.6 ± 0.9[9] km/s |
| Age | ~4.2 Gyr |
| HAT-P-4B | |
| Surface gravity (log g) | 4.38±0.14[8] cgs |
| Temperature | 6037±37[8] K |
| Metallicity [Fe/H] | 0.175±0.006[8] dex |
| Position (relative to HAT-P-4A)[5] | |
| Component | HAT-P-4B |
| Epoch of observation | 1999/02/07 |
| Angular distance | 91.760±0.099″ |
| Position angle | 163.97±0.06° |
| Projected separation | 28446 AU |
| Other designations | |
| HAT-P-4A: BD36°2593, Gaia DR3 1291120362349158016, SAO 64638, TYC 2569-1599-1, GSC 02569-01599, 2MASS J15195792+3613467[10] | |
| HAT-P-4B: Gaia DR3 1291119606434912384, TYC 2569-744-1, 2MASS J15200001+3612185[11] | |
| Database references | |
| SIMBAD | data |
| Data sources: | |
| Hipparcos Catalogue, CCDM (2002), Bright Star Catalogue (5th rev. ed.) | |
The star exhibits an infrared excess noise of unknown origin.[12]
Planetary System
editThe primary star is home to the transiting extrasolar planet HAT-P-4b.[6] This planet is a fairly typical hot Jupiter type planet in a 3-day orbit.[6]
Binary companion
editThe companion star is located at a distance of 28446 astronomical units and therefore has an orbital period that is extremely long.[5]
| Companion (in order from star) |
Mass | Semimajor axis (AU) |
Orbital period (days) |
Eccentricity | Inclination | Radius |
|---|---|---|---|---|---|---|
| b | 0.651+0.033 −0.037 MJ |
0.04449+0.00083 −0.0012 |
3.0565254±0.0000012 | <0.0073 | — | 1.28+0.016 −0.015[7] RJ |
See also
editReferences
edit- ^ 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 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 for component A Vizier catalog entry for component B
- ^ 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 d e Mugrauer, M.; Ginski, C.; Seeliger, M. (2014). "New wide stellar companions of exoplanet host stars". Monthly Notices of the Royal Astronomical Society. 439 (1): 1063–1070. Bibcode:2014MNRAS.439.1063M. doi:10.1093/mnras/stu044.
- ^ a b c Kovács, G.; et al. (2007). "HAT-P-4b: A Metal-rich Low-Density Transiting Hot Jupiter". The Astrophysical Journal Letters. 670 (1): L41–L44. arXiv:0710.0602. Bibcode:2007ApJ...670L..41K. doi:10.1086/524058. S2CID 14966730.
- ^ a b c d e Wang, Xian-Yu; et al. (1 July 2021). "Transiting Exoplanet Monitoring Project (TEMP). VI. The Homogeneous Refinement of System Parameters for 39 Transiting Hot Jupiters with 127 New Light Curves". The Astrophysical Journal Supplement Series. 255 (1). 15. arXiv:2105.14851. Bibcode:2021ApJS..255...15W. doi:10.3847/1538-4365/ac0835. S2CID 235253975.
- ^ a b c d Saffe, C.; et al. (2017). "Signatures of rocky planet engulfment in HAT-P-4. Implications for chemical tagging studies". Astronomy and Astrophysics Letters. 604. L4. arXiv:1707.02180. Bibcode:2017A&A...604L...4S. doi:10.1051/0004-6361/201731430. S2CID 119204481.
- ^ Torres, Guillermo; et al. (2012). "Improved Spectroscopic Parameters for Transiting Planet Hosts". The Astrophysical Journal. 757 (2). 161. arXiv:1208.1268. Bibcode:2012ApJ...757..161T. doi:10.1088/0004-637X/757/2/161. S2CID 16580774.
- ^ "BD+36 2593". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 2023-02-24.
- ^ "TYC 2569-744-1". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 2023-02-24.
- ^ Sada, Pedro V.; Deming, Drake; Jennings, Donald E.; Jackson, Brian k.; Hamilton, Catrina M.; Fraine, Jonathan; Peterson, Steven W.; Haase, Flynn; Bays, Kevin; Lunsford, Allen; o'Gorman, Eamon (2012), "Extrasolar Planet Transits Observed at Kitt Peak National Observatory", Publications of the Astronomical Society of the Pacific, 124 (913): 212–229, arXiv:1202.2799, Bibcode:2012PASP..124..212S, doi:10.1086/665043, S2CID 29665395
- ^ 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.
- ^ Sada, Pedro V.; et al. (2012). "Extrasolar Planet Transits Observed at Kitt Peak National Observatory". Publications of the Astronomical Society of the Pacific. 124 (913): 212–229. arXiv:1202.2799. Bibcode:2012PASP..124..212S. doi:10.1086/665043. S2CID 29665395.
External links
edit- Image HAT-P-4
- "HAT-P-4". Exoplanets. Archived from the original on 2016-03-03. Retrieved 2009-05-10.
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