WASP-5
| Observation data Epoch J2000.0 Equinox ICRS | |
|---|---|
| Constellation | Phoenix[1] |
| Right ascension | 23h 57m 23.75647s[2] |
| Declination | −41° 16′ 37.7437″[2] |
| Apparent magnitude (V) | 12.146[3] |
| Characteristics | |
| Evolutionary stage | Main sequence |
| Spectral type | G4V[4] |
| Apparent magnitude (B) | 12.808±0.02[3] |
| Apparent magnitude (V) | 12.146±0.01[3] |
| Apparent magnitude (J) | 10.949±0.022[3] |
| Apparent magnitude (H) | 10.650±0.025[3] |
| Apparent magnitude (K) | 10.598±0.023[3] |
| Astrometry | |
| Radial velocity (Rv) | 20.49±0.67[2] km/s |
| Proper motion (μ) | RA: 7.406(14) mas/yr[2] Dec.: −16.072(14) mas/yr[2] |
| Parallax (π) | 3.1883±0.0150 mas[2] |
| Distance | 1,023 ± 5 ly (314 ± 1 pc) |
| Details[5] | |
| Mass | 1.033±0.045 M☉ |
| Radius | 1.088±0.040 R☉ |
| Temperature | 5770±65 K |
| Metallicity [Fe/H] | 0.090±0.090 dex |
| Rotation | 16.20±0.40 d |
| Rotational velocity (v sin i) | 3.40±0.70 km/s |
| Age | 5.84±1.86[6] Gyr |
| Other designations | |
| TOI-250, TIC 184240683, WASP-5, GSC 08018-00199, 2MASS J23572375-4116377, DENIS J235723.7-411637, UCAC2 14323784[3] | |
| Database references | |
| SIMBAD | data |
| Exoplanet Archive | data |
WASP-5 is a magnitude 12 G-type main-sequence star located about 1,020 light-years (310 parsecs) away in the Phoenix constellation.[3] The star is likely older than the Sun, slightly enriched in heavy elements and is rotating rapidly, being spun up by the tides raised by the giant planet on a close orbit.[6]
Planetary system
[edit]This star has one exoplanet, WASP-5b, detected by the SuperWASP project in 2007.[4]
| Companion (in order from star) |
Mass | Semimajor axis (AU) |
Orbital period (days) |
Eccentricity | Inclination (°) |
Radius |
|---|---|---|---|---|---|---|
| b | 1.590+0.053 −0.052 MJ |
0.02739±0.00039 | 1.62842953(52) | <0.012 | 85.8±1.1 | 1.175±0.056 RJ |
See also
[edit]References
[edit]- ↑ Roman, Nancy G. (1987). "Identification of a constellation from a position". Publications of the Astronomical Society of the Pacific. 99 (617): 695. Bibcode:1987PASP...99..695R. doi:10.1086/132034. Constellation record for this object at VizieR.
- 1 2 3 4 5 6 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.
- 1 2 3 4 5 6 7 8 "WASP-5". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 14 December 2023.
- 1 2 Anderson, D.R.; Gillon, M.; Hellier, C.; Maxted, P. F. L.; Pepe, F.; Queloz, D.; Wilson, D. M.; Collier Cameron, A.; Smalley, B.; Lister, T. A.; Bentley, S. J.; Blecha, A.; Christian, D. J.; Enoch, B.; Hebb, L.; Horne, K.; Irwin, J.; Joshi, Y. C.; Kane, S. R.; Marmier, M.; Mayor, M.; Parley, N. R.; Pollacco, D. L.; Pont, F.; Ryans, R.; Ségransan, D.; Skillen, I.; Street, R. A.; Udry, S.; et al. (2008). "WASP-5b: a dense, very hot Jupiter transiting a 12th-mag Southern-hemisphere star". Monthly Notices of the Royal Astronomical Society: Letters. 387 (1): L4–L7. arXiv:0801.1685. Bibcode:2008MNRAS.387L...4A. doi:10.1111/j.1745-3933.2008.00465.x. S2CID 36741190.
- 1 2 Bonomo, 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. S2CID 118923163.
- 1 2 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
External links
[edit]- UK planet hunters announce three new finds (PDF)
- SuperWASP Homepage
- "WASP-5". Exoplanets. Archived from the original on 2016-03-03. Retrieved 2009-05-04.
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