Observation data Epoch J2000 Equinox J2000 | |
---|---|
Constellation | Ursa Major |
Right ascension | 10h 22m 43.5923s [1] |
Declination | +50° 07′ 42.062″ [1] |
Apparent magnitude (V) | 9.732 [2] |
Characteristics | |
Spectral type | G5V [3] |
B−V color index | 0.86 [3] |
Astrometry | |
Radial velocity (Rv) | 12.86(15) [1] km/s |
Proper motion (μ) |
RA: −26.110(14)
mas/
yr
[1] Dec.: 83.806(16) mas/ yr [1] |
Parallax (π) | 12.2731 ± 0.0155 mas [1] |
Distance | 265.7 ± 0.3
ly (81.5 ± 0.1 pc) |
Absolute magnitude (MV) | 5.22±0.14 [2] |
Details [3] | |
Mass | 0.936+0.028 −0.033 M☉ |
Radius | 1.062+0.046 −0.013 R☉ |
Luminosity | 0.77±0.09 [2] L☉ |
Surface gravity (log g) | 4.357+0.039 −0.005 cgs |
Temperature | 5,314±50 K |
Metallicity [Fe/H] | 0.30±0.09 dex |
Rotation | 28.7±0.4 d |
Rotational velocity (v sin i) | 1.65±0.26 km/s |
Age | 9.0+1.4 −2.2 Gyr [3] 12.4±2.6 [2] Gyr |
Other designations | |
Database references | |
SIMBAD | data |
HD 233731, or HAT-P-22, is a suspected multiple star system in the northern circumpolar constellation of Ursa Major. It is invisible to the naked eye, having an apparent visual magnitude of 9.732. [2] This system is located at a distance of 267 light years from the Sun based on parallax, and is drifting further away with a radial velocity of +13 km/s. [1]
The stellar classification of the primary is G5V, [3] matching an ordinary G-type main-sequence star. The star has a low level of stellar activity with an estimated age of 9 to 12 billion years old. Its metallicity is twice that of the Sun, unusual for its advanced age. [3] HD 233731 has a similar mass and radius as the Sun, and is spinning with a rotation period of 28.7 days. [3] It is radiating 77% [2] of the luminosity of the Sun from its photosphere at an effective temperature of 5314 K. [3]
A faint stellar companion (2MASS J10224397+5007504) with a red hue is located at an
angular separation of 9 arcseconds from the primary.
[2] In 2015, a spectroscopic stellar companion was reported with a
semimajor axis of less than 33
AU. This star has an effective temperature of 4,000+250
−400 K with a mass of 0.63+0.07
−0.17 M☉.
[5]
In 2010 a transiting hot Jupiter like planet was detected, designated HAT-P-22b. [2] It has an equilibrium temperature of 1,463±19 K, and planetary atmosphere is cloudy. [6] The measurement of Rossiter-McLaughlin effect in 2018 has allowed to detect what the planetary orbit is well aligned with the equatorial plane of the star, with a misalignment angle equal to 25°±18°. [3]
In 2017, analysis of additional HARPS data showed a long-term trend that suggested the presence of an additional orbiting companion, HAT-P-22c. [7]
Companion (in order from star) |
Mass |
Semimajor axis ( AU) |
Orbital period ( days) |
Eccentricity | Inclination | Radius |
---|---|---|---|---|---|---|
b | 2.192+0.073 −0.013 MJ |
0.04171+0.00042 −0.00050 |
3.21223328 | 0.016±0.009 | 86.46±0.41 ° | 1.060±0.048 RJ |
c (unconfirmed) | ≥3.0 MJ | — | ≥20.8 years | — | — | — |
{{
cite web}}
: CS1 maint: postscript (
link)