To install click the Add extension button. That's it.

The source code for the WIKI 2 extension is being checked by specialists of the Mozilla Foundation, Google, and Apple. You could also do it yourself at any point in time.

4,5
Kelly Slayton
Congratulations on this excellent venture… what a great idea!
Alexander Grigorievskiy
I use WIKI 2 every day and almost forgot how the original Wikipedia looks like.
Live Statistics
English Articles
Improved in 24 Hours
Added in 24 Hours
What we do. Every page goes through several hundred of perfecting techniques; in live mode. Quite the same Wikipedia. Just better.
.
Leo
Newton
Brights
Milds

From Wikipedia, the free encyclopedia

HAT-P-4
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
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]
Distance1,050 ± 5 ly
(322 ± 2 pc)
HAT-P-4B
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]
Distance1,060 ± 5 ly
(325 ± 2 pc)
Details
HAT-P-4A
Mass1.260+0.043
−0.042
[7] M
Radius1.573±0.015[7] R
Luminosity0.41 L
Surface gravity (log g)4.145±0.015[7] cgs
Temperature5927+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
Temperature6037±37[8] K
Metallicity [Fe/H]0.175±0.006[8] dex
Position (relative to HAT-P-4A)[5]
ComponentHAT-P-4B
Epoch of observation1999/02/07
Angular distance91.760±0.099
Position angle163.97±0.06°
Observed separation
(projected)
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
SIMBADdata
Extrasolar Planets
Encyclopaedia
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]

YouTube Encyclopedic

  • 1/5
    Views:
    2 082
    373
    2 008
    829 989 142
    50 497 305
  • This rain could kill you (HAT-P-7b) 💵 #planets #didyouknow #facts
  • Find Minimum Sample Size to Estimate Population Proportion, p hat unknown Math 160 Stats Final 4
  • Math 14 HW 8.2.7 and 8.2.9
  • Put On Your Shoes | Clothing Song for Kids
  • Five Little Elves | Christmas Song For Kids | Super Simple Songs

Transcription

Planetary System

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]

Binary companion

The companion star is located at a distance of 28446 astronomical units and therefore has an orbital period that is extremely long.[5]

The HAT-P-4A planetary system[13][14]
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

References

  1. ^ 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 
  2. ^ a b c d 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.
  3. ^ 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
  4. ^ a b c d 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.
  5. ^ 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.
  6. ^ 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.
  7. ^ 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.
  8. ^ 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.
  9. ^ 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.
  10. ^ "BD+36 2593". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 2023-02-24.
  11. ^ "TYC 2569-744-1". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 2023-02-24.
  12. ^ 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
  13. ^ 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.
  14. ^ 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



This page was last edited on 26 November 2023, at 03:21
Basis of this page is in Wikipedia. Text is available under the CC BY-SA 3.0 Unported License. Non-text media are available under their specified licenses. Wikipedia® is a registered trademark of the Wikimedia Foundation, Inc. WIKI 2 is an independent company and has no affiliation with Wikimedia Foundation.