Wide binary star system in the constellation Boötes
HAT-P-4
Observation dataEpoch 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/sProper 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/sProper 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 : BD 36°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.)
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 .
The star exhibits an infrared excess noise of unknown origin.[ 12]
The 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]
The companion star is located at a distance of 28446 astronomical units and therefore has an orbital period that is extremely long.[ 5]
^ 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 .