Double & Multiple Stars · Constellation Virgo

Porrima (Gamma Virginis / γ¹ & γ² Virginis)

Coordinates, Hipparcos distance (38.1 ly), 169-year eccentric F0V+F0V visual binary orbit (3.4″ in 2026), and observing guide for Porrima.

Right Ascension (J2000.0)12h 41m 39.64s
Declination (J2000.0)-01° 26′ 57.8″
Primary ClassificationVisual binary of two virtually identical F0 V main-sequence stars
Best Observing SeasonSpring (March–June)

Provenance-Backed Scientific Measurements

Every measurement below preserves its unit, uncertainty interval, observational method, reference epoch, quality status, and primary catalog source. See Uncertainty & Provenance for how competing measurements are handled.

Astrometric, Photometric, and Physical Parameters for Porrima (Gamma Virginis / γ¹ & γ² Virginis)
ParameterValueUncertaintyMethod & EpochQuality StatusSource Archive
Combined apparent visual magnitude (V)2.74 mag± 0.01 magJohnson UBV photometry (γ Vir A = 3.48 mag, γ Vir B = 3.50 mag)definitiveHipparcos New Reduction Catalog
Trigonometric parallax85.58 mas± 0.6 masHipparcos New Reduction + dynamical binary orbit (11.68 ± 0.08 pc / 38.1 ly) (J2000.0)definitiveHipparcos New Reduction Catalog
Visual binary orbital period61705 d± 75 dThree-century visual & speckle astrometric orbit (168.93 ± 0.20 yr, e = 0.8825)definitiveSIMBAD Astronomical Database (CDS)
Component stellar mass (γ Vir A & B each)1.4 M☉± 0.04 M☉3D astrometric + radial-velocity Keplerian orbit (A = 1.40 M☉, B = 1.39 M☉)definitiveSIMBAD Astronomical Database (CDS)
Visual angular separation (2026 epoch)0.057 arcmin± 0.002 arcminOrbital ephemeris (~3.4 arcseconds in 2026, widening from 0.36″ in 2005 toward 6.0″ in 2090)definitiveSIMBAD Astronomical Database (CDS)
Measurement Uncertainties & Competing Solutions: Because Porrima's orbit has a high eccentricity (e = 0.8825), its visual separation swings by a factor of 16 over its 168.93-year period—closing to just 0.36″ at periastron in May 2005 and now widening past 3.4″ in 2026.

J2000 Equatorial Sky Chart & Culmination Altitude

The chart below plots Porrima (Gamma Virginis Twin F0V Binary) at RA 12h 41m 39.64s, Dec -01° 26′ 57.8″ within Virgo, alongside peak meridian transit altitudes for 40°N and 30°S observers. Use the RA/Dec Coordinate Converter to compute exact culmination altitude for your latitude.

J2000 Equatorial Sky Position (Virgo) +90° 0° −90° 24h 12h RA 0h Peak Meridian Altitude 49° 40°N Lat 61° 30°S Lat RA: 12h 41m 39.64s Dec: -01° 26′ 57.8″ Epoch: J2000.0 · V = 2.74 mag First-party vector diagram derived from IAU / CDS SIMBAD / Gaia DR3 astrometry.

Astrophysical Context & Structure

Porrima (Gamma Virginis, named after the Roman goddess of prophecy) is the second-brightest star in Virgo at combined apparent magnitude 2.74, located just 11.68 ± 0.08 parsecs (38.1 light-years) from Earth and 1.4° north of the celestial equator. First resolved by Father Jean Richaud at Pondicherry, India, in 1689 and measured by James Bradley in 1718, Porrima is one of the most dynamic visual binaries accessible to amateur telescopes.

The system consists of two virtually identical twin F0 V yellow-white main-sequence stars: Gamma Virginis A (magnitude 3.48, 1.40 solar masses, 1.45 solar radii, 7,100 K) and Gamma Virginis B (magnitude 3.50, 1.39 solar masses, 1.43 solar radii). Orbiting their common center of mass every 168.93 years along a highly eccentric ellipse (eccentricity e = 0.8825), their true physical separation varies from 81 AU at apastron down to just 5.1 AU (Jupiter's distance from the Sun) at periastron.

When Porrima swept through periastron in May 2005 (repeating the 1836 close passage predicted by Sir John Herschel), its angular separation shrank to 0.36 arcseconds, rendering it a single elongated star in all but the largest professional apertures. Since 2005 the twins have rapidly separated, passing 2.0 arcseconds in 2013 and reaching ~3.4 arcseconds in 2026 on their way toward their 6.0-arcsecond maximum around 2090.

Practical Visual Observing Guide

Minimum InstrumentNaked eye; 60–80 mm telescope at 100×+ splits the 3.4″ twin pair
Recommended Magnification100×–160×
Best Evening SeasonSpring (March–June)
  • Located 15° northwest of Spica along the body of Virgo, Porrima is also the primary naked-eye landmark for hopping 4° southeast to the quasar 3C 273 or 8° north into the southern edge of the Virgo Galaxy Cluster.
  • In 2026 at ~3.4 arcseconds separation (position angle ~355°), any 60–80 mm telescope at 100×–150× splits Porrima cleanly into two identical, matched 3.5-magnitude creamy-white headlights.

Catalog Cross-Identifications & Aliases

Common Aliases: γ Virginis · Arich · HD 110379 / HD 110380 · HIP 61941 · 29 Virginis

Cross-Catalog Identifiers for Porrima (Gamma Virginis / γ¹ & γ² Virginis)
Catalog AuthorityIdentifier
HIPHIP 61941
HDHD 110379
SIMBAD* gam Vir
WIKIDATAQ13063
Related Object · Virgo

3C 273 (Brightest Quasar in Virgo)

Coordinates, redshift z = 0.1583 (~2.4 billion ly), magnitude 12.85, supermassive black hole accretion, and observing guide for quasar 3C 273.

Reference Guide

Angular Size, Separation & Field of View

How angular diameter (degrees, arcminutes, arcseconds), spherical angular separation, and small-angle physical diameter relate to telescope field of view.

Reference Guide

Trigonometric Parallax, Parsecs & Gaia DR3

How trigonometric parallax (d_pc = 1 / p_arcsec), the distance modulus equation, Hipparcos, and Gaia DR3 microarcsecond astrometry measure cosmic distances.

Scientific Sources & Dataset Provenance