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WASP-3

Star in the constellation Lyra From Wikipedia, the free encyclopedia

WASP-3
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WASP-3 is a triple star system located about 753 light-years (231 parsecs) 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]

Quick Facts Observation data Epoch J2000.0 Equinox J2000.0, Apparent magnitude (V) ...
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Triple system

WASP-3 has been identified as a triple star system in a 2019 study of astrometry from the Gaia mission.[11]:5093 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]:1581 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 2900 K.[8]:11,13 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 300 AU.[8]:11,13 WASP-3B was first identified in observations from 2012 to 2013.[8]:14 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 4230 AU.[11]:5093 WASP-3C is about 0.77 times as massive as the Sun and has an effective temperature of about 4700 K.[6]

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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]

More information Companion (in order from star), Mass ...
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See also

References

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