Mu Arietis

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μ Arietis
Observation data
Epoch J2000      Equinox J2000
Constellation Aries
Right ascension 02h 42m 21.9397s
Declination +20° 00′ 41.274″
Apparent magnitude (V) 5.738
Characteristics
Spectral type A0V
U-B color index -0.03
B-V color index -0.02
Astrometry
Radial velocity (Rv) -7 km/s
Proper motion (μ) RA: 27.49 mas/yr
Dec.: -46.08 mas/yr
Parallax (π) 9.64 ± 0.88 mas
Distance 340 ± 30 ly
(104 ± 9 pc)
Absolute magnitude (MV) 5.72
Details
Mass 3,1 M
Radius 2,1 R
Luminosity 40 L
Temperature 7,500–10,000 K
Rotation 195 Km/s
0,00149474 Year
Orbit
Companion CCDM 02424+2001 B
Semimajor axis (a) 0,1"
Inclination (i) 100°
Orbit
Companion CCDM 02424+2001 C
Semimajor axis (a) 19.1"
Inclination (i) 264°
Other designations
34 Arietis, HR 793,
HD 16811, BD+19°403,
HIP 12640, SAO 93062,
GC 3256, ADS 2062,
CCDM 02424+2001
Database references
SIMBAD data
Data sources:
Hipparcos Catalogue,
CCDM (2002),
Bright Star Catalogue (5th rev. ed.)
Database references
SIMBAD data

Mu Arietis (μ Ari / μ Arietis) is a triple star system in the constellation Aries. It is approximately 338 light years from Earth.

The primary component, μ Arietis A, is a spectroscopic binary which is classified as a white A-type main sequence dwarf with an apparent magnitude of +5.74. The two components are separated by 0.05 arcseconds and have an orbital period of 8.8 years. The third component, μ Arietis B, is 19.1 arcseconds distant and has an apparent magnitude of +12.1.

Aries Constellation

[edit] References


[edit] Components

NAME Right ascension Declination Apparent magnitude (V) Spectral type Database references
ADS 2062 B (BD+19 403B) 02h 42m 20.4s +20° 00' 41 12.2 Simbad
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