30 Arietis

30 Arietis (abbreviated 30 Ari) is a 6th-apparent-magnitude multiple star system in the constellation of Aries. 30 Arietis is the Flamsteed designation. 30 Arietis A and B are separated by 38.1″ or about 1,500 AU at a distance of 130 light years away. The main components of both systems are both binaries with a composite spectra belonging to F-type main-sequence stars, meaning they are fusing hydrogen in their cores. The 30 Arietis system is 910 million years old, one fifth the age of the Sun.

30 Arietis

30 Arietis star system hierarchy
Observation data
Epoch J2000      Equinox J2000
Constellation Aries
30 Arietis A
Right ascension 02h 37m 00.5235s
Declination +24° 38 49.9880
30 Arietis B
Right ascension 02h 36m 57.7449s
Declination +24° 38 53.0026
Characteristics
Spectral type F5 V / F6 V
B−V color index 0.410 / 0.510
Astrometry
30 Arietis A
Proper motion (μ) RA: 136.862±0.137 mas/yr
Dec.: −15.188±0.141 mas/yr
Parallax (π)22.1261 ± 0.0726 mas
Distance147.4 ± 0.5 ly
(45.2 ± 0.1 pc)
30 Arietis B
Proper motion (μ) RA: 141.411±0.083 mas/yr
Dec.: −10.677±0.086 mas/yr
Parallax (π)22.3641 ± 0.0516 mas
Distance145.8 ± 0.3 ly
(44.7 ± 0.1 pc)
Orbit
Primary30 Arietis A
Companion30 Arietis BC
Period (P)34000 yr
Semi-major axis (a)40"
(1670 AU)
Orbit
Primary30 Arietis B
Companion30 Arietis C
Period (P)80 yr
Semi-major axis (a)22.3 AU
Orbit
Primary30 Arietis B
Companion30 Arietis Bb
Period (P)335.1 ± 2.5 d
(0.917 ± 0.007 yr)
Semi-major axis (a)0.995 ± 0.012 AU
Eccentricity (e)0.289 ± 0.092
Inclination (i)4.14+0.96
−0.90
°°
Details
30 Arietis A
Mass1.31 ± 0.04 M
Radius1.37 ± 0.03 R
Age860±630 Myr
30 Arietis Ba
Mass1.16 ± 0.04 M
Radius1.13 ± 0.03 R
Age910±830 Myr
Details
30 Arietis Bb
Mass147+41
−29
 MJup
Other designations
CCDM 02370+2439, WDS 02370+2439

30 Arietis A
BD+24°376, HD 16246, HIP 12189, HR 765, SAO 75471

30 Arietis B
BD+24°375, HD 16232, HIP 12184, HR 764, SAO 75470
Database references
SIMBADA
B
Exoplanet Archivedata
Data sources:
Hipparcos Catalogue,
CCDM (2002),
Bright Star Catalogue (5th rev. ed.)
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