Movatterモバイル変換


[0]ホーム

URL:


Jump to content
WikipediaThe Free Encyclopedia
Search

WASP-4

Coordinates:Sky map23h 34m 15.06s, −42° 03′ 41.1″
From Wikipedia, the free encyclopedia
G-type main sequence star in the constellation Phoenix
WASP-4

Artistic rendering of WASP-4 b
Observation data
Epoch J2000.0      Equinox J2000.0
ConstellationPhoenix[1]
Right ascension23h 34m 15.0857s[2]
Declination−42° 03′ 41.048″[2]
Apparent magnitude (V)12.468±0.025[3]
Characteristics
Evolutionary stageMain sequence
Spectral typeG7V[4]
Apparent magnitude (V)12.468±0.025[3]
Apparent magnitude (B)13.216±0.020[3]
Variable typePlanetary transit variable[4]
Astrometry
Radial velocity (Rv)57.61±0.76[2] km/s
Proper motion (μ)RA: 9.950(12)mas/yr[2]
Dec.: −87.620(10)mas/yr[2]
Parallax (π)3.6623±0.0147 mas[2]
Distance891 ± 4 ly
(273 ± 1 pc)
Details[5]
Mass0.89±0.01 M
Radius0.920±0.060 R
Surface gravity (log g)4.484+0.037
−0.047
[6] cgs
Temperature5436±34 K
Metallicity [Fe/H]−0.050±0.040 dex
Rotation22.2±3.3 d
Rotational velocity (v sin i)2.2+0.6
−1.0
 km/s
Age7.0±2.9 Gyr
Other designations
1SWASP J233415.06-420341.1,TOI-232,TIC 402026209,WASP-4,TYC 8017-108-1,2MASS J23341508-4203411[7]
Database references
SIMBADdata

WASP-4 is aG-type main-sequence star approximately 891light-years away in theconstellation ofPhoenix.[4][1][2] Despite its advanced age, the star is rotating rapidly, being spun up by the tides raised by a giant planet on a close orbit.[8]

Planetary system

[edit]

In 2007 theexoplanetWASP-4b was discovered orbiting this star. With an orbital period of just 1.3 days it is classified as ahot Jupiter.[4] The planet's orbital period appears to be decreasing at a rate of7.33±0.71 milliseconds per year, suggesting that its orbit is decaying, with a decay timescale of 15.77±1.57 million years. Anothersuperjovian planet in the system is suspected.[9]

The WASP-4 planetary system[9]
Companion
(in order from star)
MassSemimajor axis
(AU)
Orbital period
(days)
EccentricityInclinationRadius
b1.164±0.082 MJ0.02239±0.000841.338231587(22)<0.0033[5]88.02±0.69°1.312±0.045 RJ
c(unconfirmed)≥5.47±0.44MJ6.82±0.257001.0±6.6

See also

[edit]

References

[edit]
  1. ^abRoman, 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. ^abcdefVallenari, 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 atVizieR.
  3. ^abcHenden, 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
  4. ^abcdWilson, D. M.; et al. (2008)."WASP-4b: A 12th Magnitude Transiting Hot Jupiter in the Southern Hemisphere".The Astrophysical Journal Letters.675 (2):L113 –L116.arXiv:0801.1509.Bibcode:2008ApJ...675L.113W.doi:10.1086/586735.S2CID 10823235.
  5. ^abBonomo, A. S.; Desidera, S.; et al. (June 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 & Astrophysics.602: A107.arXiv:1704.00373.Bibcode:2017A&A...602A.107B.doi:10.1051/0004-6361/201629882.
  6. ^Dragomir, Diana; Kane, Stephen R.; Pilyavsky, Genady;Mahadevan, Suvrath; Ciardi, David R.; Zachary Gazak, J.; Gelino, Dawn M.; Payne, Alan; Rabus, Markus; Ramirez, Solange V.; von Braun, Kaspar; Wright, Jason T.; Wyatt, Pamela (2011). "Terms Photometry of Known Transiting Exoplanets".The Astronomical Journal.142 (4): 115.arXiv:1108.2308.Bibcode:2011AJ....142..115D.doi:10.1088/0004-6256/142/4/115.S2CID 118606598.
  7. ^"WASP-4".SIMBAD.Centre de données astronomiques de Strasbourg. Retrieved2018-09-22.
  8. ^Maxted, P. F. L.; Serenelli, A. M.; Southworth, J. (2015), "A comparison of gyrochronological and isochronal age estimates for transiting exoplanet host stars",Astronomy & Astrophysics,577: A90,arXiv:1503.09111,Bibcode:2015A&A...577A..90M,doi:10.1051/0004-6361/201525774,S2CID 53324330
  9. ^abTurner, Jake D.; Flagg, Laura; Ridden-Harper, Andrew; Jayawardhana, Ray (2022), "Characterizing the WASP-4 System with TESS and Radial Velocity Data: Constraints on the Cause of the Hot Jupiter's Changing Orbit and Evidence of an Outer Planet",The Astronomical Journal,163 (6): 281,arXiv:2112.09621,Bibcode:2022AJ....163..281T,doi:10.3847/1538-3881/ac686f,S2CID 245329747

External links

[edit]


Stars
Bayer
Variable
HR
HD
Other
Exoplanets
Galaxies
NGC
Other
Galaxy clusters
Stub icon

This variable star–related article is astub. You can help Wikipedia byexpanding it.

Retrieved from "https://en.wikipedia.org/w/index.php?title=WASP-4&oldid=1189322711"
Categories:
Hidden categories:

[8]ページ先頭

©2009-2025 Movatter.jp