HAT-P-9b

HAT-P-9b, formally named Alef,[1] is an exoplanet approximately 1500 light years away in the constellation Auriga. This planet was found by the transit method on June 26, 2008. It has a mass 78% that of Jupiter and a radius 140% that of Jupiter. As with most transiting planets, this planet is a hot Jupiter, meaning this Jupiter-like planet orbits extremely close to its parent star, taking only 3.92 days to orbit.[2]

HAT-P-9b
Size comparison of HAT-P-9b with Jupiter.
Discovery
Discovered byShporer et al.
Discovery siteCambridge, Massachusetts
Discovery dateJune 26, 2008
Transit (SuperWASP)
Orbital characteristics
0.0528 ± 0.002 AU (7,900,000 ± 300,000 km)
Eccentricity~0.0012
3.92289 ± 0.00004 d
StarHAT-P-9
Physical characteristics
Mean radius
1.4 ± 0.06 RJ
Mass0.78 ± 0.09 MJ
Mean density
380 kg/m3 (640 lb/cu yd)
10.3 m/s2 (34 ft/s2)
1.05 g

    The study in 2012, utilizing a Rossiter–McLaughlin effect, have determined the planetary orbit is mildly misaligned with the rotational axis of the star, misalignment equal to -16±8°.[3]

    The name Alef was selected in the NameExoWorlds campaign by Israel, during the 100th anniversary of the IAU. Alef is the first letter in the Hebrew alphabet and also means bull.[1]

    References
    1. "Approved names". NameExoworlds. Retrieved 2020-01-02.
    2. Shporer, Avi; et al. (2009). "HAT-P-9b: A Low-Density Planet Transiting a Moderately Faint F Star". The Astrophysical Journal. 690 (2): 1393–1400. arXiv:0806.4008. Bibcode:2009ApJ...690.1393S. doi:10.1088/0004-637X/690/2/1393. S2CID 930937.
    3. Albrecht, Simon; Winn, Joshua N.; Johnson, John A.; Howard, Andrew W.; Marcy, Geoffrey W.; Butler, R. Paul; Arriagada, Pamela; Crane, Jeffrey D.; Shectman, Stephen A.; Thompson, Ian B.; Hirano, Teruyuki; Bakos, Gaspar; Hartman, Joel D. (2012), "Obliquities of Hot Jupiter host stars: Evidence for tidal interactions and primordial misalignments", The Astrophysical Journal, 757: 18, arXiv:1206.6105, doi:10.1088/0004-637X/757/1/18, S2CID 17174530

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