Observation data Epoch J2000 Equinox J2000 | |
---|---|
Constellation | Aquarius |
Right ascension | 23h 41m 51.5301s[1] |
Declination | –05° 59′ 08.729″[1] |
Apparent magnitude (V) | 7.685±0.005[2] |
Characteristics | |
HD 222582A | |
Evolutionary stage | Main sequence |
Spectral type | G5V[3] |
B−V color index | 0.648±0.002[4] |
HD 222582B | |
Spectral type | M4.5V[5] |
Astrometry | |
Radial velocity (Rv) | +12.020±0.0004[6] km/s |
Proper motion (μ) | RA: −145.492(29) mas/yr[1] Dec.: −111.458(21) mas/yr[1] |
Parallax (π) | 23.7955 ± 0.0238 mas[1] |
Distance | 137.1 ± 0.1 ly (42.02 ± 0.04 pc) |
Absolute magnitude (MV) | 4.44±0.12[2] |
Position (relative to HD 222582A)[5] | |
Component | HD 222582B |
Epoch of observation | 2018 |
Angular distance | 109.56±0.18″ |
Position angle | 299.52±0.03° |
Projected separation | 4637±59 AU AU |
Details | |
A | |
Mass | 0.993±0.035[7] M☉ |
Radius | 1.137±0.017[7] R☉ |
Luminosity | 1.302+0.005 −0.004[8] L☉ |
Surface gravity (log g) | 4.370±0.009[4] cgs |
Temperature | 5,790±3[4] K |
Metallicity [Fe/H] | −0.005±0.003[4] dex |
Rotational velocity (v sin i) | 1.74±0.12[9] km/s |
Age | 6.7±0.3[4] Gyr |
Ba+Bb | |
Mass | 0.2[10] M☉ |
Other designations | |
Database references | |
SIMBAD | data |
Planet | |
HD 222582 b | Data Simbad |
Data ExoPlanet |
HD 222582 is a multiple star system in the equatorial constellation of Aquarius. It is invisible to the naked eye with an apparent visual magnitude of 7.7,[2] but can be viewed with binoculars or a small telescope.[12] The system is located at a distance of 137 light years from the Sun based on parallax,[1] and it is drifting further away with a radial velocity of +12 km/s.[6] It is located close enough to the ecliptic that it is subject to lunar occultations.[13]
The primary member of this system, designated component A, is an ordinary G-type main-sequence star with a stellar classification of G5V.[3] The physical properties of the star are similar enough to the Sun that it is considered a candidate solar twin.[14][4] It is about 6.5[9] billion years old with an inactive chromosphere[14] and is spinning with a low projected rotational velocity of 1.7 km/s.[9] The mass[7] and metallicity[4] of this star are essentially the same as the Sun. It has a 14% larger radius and is radiating 1.3 times the luminosity of the Sun from its photosphere at an effective temperature of 5,790 K.[4]
Component B of this system is a close binary[15][16] system with the components designated HD 222582 Ba and Bb. The pair have a combined class of M4.5 V+[5] and about 20% the mass of the Sun.[10]
Gaia DR3
was invoked but never defined (see the help page).mnras384_1_173
was invoked but never defined (see the help page).Houk_Swift_1999
was invoked but never defined (see the help page).Lorenzo-Oliveira_et_al_2018
was invoked but never defined (see the help page).Montes2018
was invoked but never defined (see the help page).Soubiran_et_al_2018
was invoked but never defined (see the help page).Soto_Jenkins_2018
was invoked but never defined (see the help page).Gaia DR2
was invoked but never defined (see the help page).dosSantos2016
was invoked but never defined (see the help page).oepc
was invoked but never defined (see the help page).SIMBAD
was invoked but never defined (see the help page).ICQ
was invoked but never defined (see the help page).Richichi2003
was invoked but never defined (see the help page).Reddy_Lambert_2017
was invoked but never defined (see the help page).Riddle2015
was invoked but never defined (see the help page).Raghavan2006
was invoked but never defined (see the help page).