WASP-3
| Observation data Epoch J2000.0 Equinox J2000.0 | |
|---|---|
| Constellation | Lyra[2] |
| WASP-3A | |
| Right ascension | Template:RA[3] |
| Declination | Template:DEC[3] |
| Apparent magnitude (V) | Script error: No such module "val".[4] |
| WASP-3C | |
| Right ascension | Template:RA[5][6] |
| Declination | Template:DEC[5][6] |
| Characteristics | |
| WASP-3A | |
| Evolutionary stage | main-sequence star |
| Spectral type | F7V[4] |
| Apparent magnitude (B) | Script error: No such module "val".[4] |
| Apparent magnitude (G) | Script error: No such module "val".[4][6] |
| Apparent magnitude (J) | Script error: No such module "val".[4] |
| Apparent magnitude (H) | Script error: No such module "val".[4] |
| Apparent magnitude (K) | Script error: No such module "val".[4] |
| Variable type | planetary transit[7] |
| WASP-3B | |
| Apparent magnitude (J) | Script error: No such module "val".[8] |
| Apparent magnitude (H) | Script error: No such module "val".[8] |
| Apparent magnitude (K) | Script error: No such module "val".[8] |
| Astrometry | |
| WASP-3A | |
| Radial velocity (Rv) | Script error: No such module "val".[9] km/s |
| Proper motion (μ) | RA: Script error: No such module "val". mas/yr[3] Dec.: Script error: No such module "val". mas/yr[3] |
| Parallax (π) | 4.3338±0.0120 mas[3] |
| Distance | Template:Rnd ± Template:Rnd ly (Template:Rnd ± Template:Rnd pc) |
| Details | |
| WASP-3A | |
| Mass | Script error: No such module "val".[9]Template:Rp Template:Solar mass |
| Radius | Script error: No such module "val".[10] Template:Solar radius |
| Surface gravity (log g) | Script error: No such module "val".[9]Template:Rp cgs |
| Temperature | Script error: No such module "val".[9]Template:Rp K |
| Metallicity | Script error: No such module "val".[9]Template:Rp |
| Rotational velocity (v sin i) | Script error: No such module "val".[10] km/s |
| Age | Script error: No such module "val".[10] Gyr |
| WASP-3B | |
| Mass | Script error: No such module "val".[8]Template:Rp Template:Solar mass |
| Surface gravity (log g) | ~5.22[8]Template:Rp cgs |
| Temperature | ~2900[8]Template:Rp K |
| Metallicity [Fe/H] | {{{metal_fe2}}} dex |
| Position (relative to WASP-3A)[8]Template:Rp | |
| Component | WASP-3B |
| Epoch of observation | 2012–2013 |
| Angular distance | ~1.19″ |
| Position angle | ~87.1° |
| Projected separation | Script error: No such module "val". AU |
| Position (relative to WASP-3A)[6] | |
| Component | WASP-3C |
| Angular distance | Script error: No such module "val".″ |
| Position angle | Script error: No such module "val".° |
| Projected separation | 4230 AU |
| Other designations | |
| Template:Odlist, USNO-B1.0 1256-00285133, 1SWASP J183431.62+353941.4[4] | |
| Database references | |
| SIMBAD | data |
| Exoplanet Archive | data |
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WASP-3 is a triple star system located about Script error: No such module "convert". away from the Sun in the constellation Lyra. The system has an apparent magnitude of 10. The brightest and most massive star of this system is WASP-3A, an F-type main sequence star which has one known transiting hot Jupiter exoplanet, WASP-3b. Since the planet transits the star, the star is classified as a planetary transit variable and has received the variable star designation V838 Lyrae.[7]
Triple system
WASP-3 has been identified as a triple star system in a 2019 study of astrometry from the Gaia mission.[11]Template:Rp The brightest and most massive component of the system is WASP-3A, an F-type main sequence star that is 1.24 times as massive as the Sun and 1.31 times as large as the Sun in radius.[9]Template:Rp WASP-3A appears to be a variable star; observations between 2007 and 2010 show that the star's chromospheric activity had increased during that time period.[12] The second companion, WASP-3B, is a low-mass star about 0.11 times as massive as the Sun and has an effective temperature of about Script error: No such module "val"..[8]Template:Rp WASP-3B is separated eastward from WASP-3A at an angular separation of approximately 1.19 arcseconds, corresponding to a projected separation distance of about Script error: No such module "val"..[8]Template:Rp WASP-3B was first identified in observations from 2012 to 2013.[8]Template:Rp The third companion, WASP-3C, is much more distant with an angular separation of approximately 18.3 arcseconds from WASP-3A, corresponding to a projected separation distance of Script error: No such module "val"..[11]Template:Rp WASP-3C is about 0.77 times as massive as the Sun and has an effective temperature of about Script error: No such module "val"..[6]
Planetary system
WASP-3A has one known transiting hot Jupiter extrasolar planet, WASP-3b, which was detected by the SuperWASP project in 2007.[9] It was confirmed in 2008 by observations from the William Herschel Telescope.
In 2010, researchers proposed a second planet orbiting WASP-3A due to transit timing variations in WASP-3b.[13][14] But in 2012 this proposal was refuted.[12]
Template:OrbitboxPlanet begin Template:OrbitboxPlanet
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See also
References
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- ↑ Script error: No such module "citation/CS1".
- ↑ Template:Cite constellation
- ↑ a b c d Template:Cite Gaia DR3
- ↑ a b c d e f g h Template:Cite simbad
- ↑ a b Template:Cite simbad
- ↑ a b c d e Script error: No such module "Citation/CS1".
- ↑ a b Script error: No such module "citation/CS1".
- ↑ a b c d e f g h i j Script error: No such module "Citation/CS1".
- ↑ a b c d e f g Script error: No such module "Citation/CS1".
- ↑ a b c Script error: No such module "Citation/CS1".
- ↑ a b Script error: No such module "Citation/CS1".
- ↑ a b Script error: No such module "Citation/CS1".
- ↑ Planet found tugging on transits Template:Webarchive, Astronomy Now, 9 July 2010
- ↑ Script error: No such module "Citation/CS1".
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External links
- Script error: No such module "citation/CS1".
- Pages with script errors
- Pages with broken file links
- Lyra
- F-type main-sequence stars
- Triple star systems
- Planetary transit variables
- Planetary systems with one confirmed planet
- Wide Angle Search for Planets
- 2MASS objects
- Objects with variable star designations
- Durchmusterung objects
- TESS Objects of Interest
- TIC objects