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Gamma Virginis

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Gamma Virginis A/B
Observation data
Epoch J2000      Equinox J2000
Constellation Virgo
Right ascension 12h 41m 39.6s
Declination -1° 26′ 58″
Apparent magnitude (V) 2.74 (3.48/3.50)
Characteristics
Spectral type F0 V/F0 V
U−B color index -0.05
B−V color index 0.36
Variable type ?
Astrometry
Radial velocity (Rv)-20 km/s
Proper motion (μ) RA: -616.66 mas/yr
Dec.: 60.66 mas/yr
Parallax (π)84.53 ± 1.18 mas
Distance38.6 ± 0.5 ly
(11.8 ± 0.2 pc)
Absolute magnitude (MV)2.38 (3.12/3.14)
Orbit
CompanionGamma Virginis B
Period (P)171.37 yr
Semi-major axis (a)3.746″
Eccentricity (e)0.881
Inclination (i)146.05°
Longitude of the node (Ω)31.78°
Periastron epoch (T)1836.433
Other designations
Porrima, Arich, 29 Virginis, Gl 482 A/B, HR 4825/4826, BD -00°2601, HD 110379/110380, LHS 2604, LTT 4843/4844, GCTP 2924.00, SAO 138917, GC 17270, ADS 8630, CCDM 12417-0127, LFT 937/938, HIP 61941.

Gamma Virginis (γ Vir / γ Virginis) is a star in the constellation Virgo. It also has the traditional name Porrima.

Gamma Virginis is a binary star, consisting of two stars of approximately equal apparent magnitudes 3.48 and 3.50, and of spectral type F0V. With an orbital period of 168.68 years (calculated by Heintz at Sproul Observatory in 1990) until the beginning of the 1990s it was an easy object for amateur astronomers, but now the smaller apparent distance between the stars requires a larger telescope. The last time they were at periapsis was in 1836. The distance will again be wide enough in 2020 to view with a small telescope. The star system has a combined apparent magnitude of 2.9. The system is 32 light years away from the Sun.

As Gamma Virginis is close to the ecliptic, it can be occulted by the Moon and (extremely rarely) by planets.

Changes of distance and position angle

This table shows the apparent distance between the two stars and their relative position angle: first three columns show data predicted from an orbit calculated in 1937, the next three columns show observations reported by the Hanwell Community Observatory.

Predicted from 1937 Strand orbit Observations 2003 to 2005
Year distance position angle Date distance position angle
1995 2.5" 280
2000 1.8" 267
2002 1.5" 259
2003 2003 Dec. 0.6 arcsec. 219°
2004 1.2" 246 2004 Dec. 0.4 arcsec. 177°
2005 2005 April 0.27-0.29" 161±0.6°
2006 0.8" 221
2008 0.4" 126
2010 0.9" 44

External links