HAT-P-21

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HAT-P-21 / Mazalaai
Observation data
Epoch J2000      Equinox J2000
Constellation Ursa Major
Right ascension 11h 25m 05.9859s[1]
Declination +41° 01′ 40.665″[1]
Apparent magnitude (V) 11.46[2]
Characteristics
Spectral type G3V
Distance
927 ± 6 ly
(284 ± 2 pc)
Details
Gyr
TYC 3013-1229-1, GSC 03013-01229, 2MASS J11250598+4101406[2]
Database references
SIMBADdata

HAT-P-21 is a G-type main-sequence star about 927 light-years away. The star has amount of metals similar to solar abundance. The survey in 2015 has failed to detect any stellar companions.[6] The star is rotating rapidly, being spun up by the tides of giant planet on close orbit.[4]

Naming

In 2019, the HAT-P-21 star received the proper name Mazalaai while its planet

HAT-P-21b received the name Bambaruush at an international NameExoWorlds contest.[7] These names refer to the Mongolian name for the endangered Gobi bear
subspecies, and the Mongolian term for 'bear cub', respectively.

Planetary system

In 2010 a

HAT-P-21b are known with better precision.[5]

The planetary orbit is likely aligned with the equatorial plane of the star, misalignment equal to 25±16 degrees.[9]

Size comparison of HAT-P-21 b and Jupiter
The HAT-P-21 planetary system[8][10]
Companion
(in order from star)
Mass Semimajor axis
(AU)
Orbital period
(days)
Eccentricity Inclination Radius
b (Bambaruush)
4.063±0.161 MJ 0.0494±0.0007 4.124481±0.000007 0.228±0.016 88.6° 1.08±0.18 RJ

References