Gamma Microscopii

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Gamma Microscopii
Diagram showing star positions and boundaries of the Microscopium constellation and its surroundings
Cercle rouge 100%.svg

Location of γ Microscopii (circled)
Observation data
Epoch J2000.0      Equinox J2000.0 (ICRS)
Constellation Microscopium
Right ascension 21h 01m 17.46047s[1]
Declination −32° 15′ 27.9574″[1]
Apparent magnitude (V) 4.680[2]
Characteristics
Spectral type G6 III[3]
U−B color index +0.575[2]
B−V color index +0.882[2]
R−I color index +0.32[4]
Astrometry
Radial velocity (Rv) +17.6[5] km/s
Proper motion (μ) RA: −1.73[1] mas/yr
Dec.: +0.41[1] mas/yr
Parallax (π) 14.24 ± 0.26[1] mas
Distance 229 ± 4 ly
(70 ± 1 pc)
Absolute magnitude (MV) 0.49[6]
Details
Mass 2.5[7] M
Radius 10[7] R
Luminosity 64[7] L
Surface gravity (log g) 3.34[8] cgs
Temperature 5,050[8] K
Metallicity [Fe/H] –0.22 ± 0.11[9] dex
Age 620[7] Myr
Other designations
Gamma Microscopii, Gamma Mic, γ Mic, CD−32 16353, CPD−32 6269, FK5 1550, GC 29331, HD 199951, HIP 103738, HR 8039, SAO 212636, WDS 21013-3215A.[10][11]
Database references
SIMBAD data

Gamma Microscopii (γ Microscopii, γ Mic) is the brightest star in the faint southern constellation of Microscopium.[7] It has an apparent visual magnitude of 4.68,[2] which is too dim to be viewed from city skies. The distance to this star has been determined using parallax measurements made during the Hipparcos mission, which place it around 229 light-years (70 parsecs) away with a 2% margin of error.[1]

Based upon a stellar classification of G6 III,[3] this is a G-type giant star. It is a core helium fusing star that is classified as a member of the red clump evolutionary branch, although the metallicity of this star—meaning the abundance of elements other than hydrogen and helium—is anomalously low for a member of this group.[9] The effective temperature of the star's outer envelope is 5,050 K,[8] giving it the yellow-hued glow typical of G-type stars.[12]

In the galactic coordinate system, this star has space velocity components of [U, V, W] = [+13.75, +3.47, –10.50] km s−1. The peculiar velocity of this star, relative to its neighbors, is 1.2 km s−1. It has been listed as likely member of the Ursa Major Moving Group of stars that share a similar location and a common trajectory through space.[6] Backwards extrapolation of the motion of γ Microscopii has shown that approximately 3.8 million years ago, it was only around 6 light-years from the Sun.[13] It would then have had an apparent magnitude of −3 and have been brighter than Sirius is now.[7]

Gamma Microscopii has a visual companion, CCDM J21013-3215B at an angular separation of 26 arcseconds along a position angle of 94°, with an apparent visual magnitude of approximately 13.7.[11] Most likely this star is not gravitationally bound to γ Microscopii, but is merely a line of sight companion.[7][14]

Gamma Microscopii was a later designation of 1 Piscis Austrini.[15]

References

  1. 1.0 1.1 1.2 1.3 1.4 1.5 Lua error in package.lua at line 80: module 'strict' not found.
  2. 2.0 2.1 2.2 2.3 Lua error in package.lua at line 80: module 'strict' not found.
  3. 3.0 3.1 Lua error in package.lua at line 80: module 'strict' not found.
  4. HR 8039, database entry, The Bright Star Catalogue, 5th Revised Ed. (Preliminary Version), D. Hoffleit and W. H. Warren, Jr., CDS ID V/50. Accessed on line November 20, 2008.
  5. Lua error in package.lua at line 80: module 'strict' not found.
  6. 6.0 6.1 Lua error in package.lua at line 80: module 'strict' not found.
  7. 7.0 7.1 7.2 7.3 7.4 7.5 7.6 Gamma Mic, Stars, Jim Kaler. Accessed on line March 19, 2015.
  8. 8.0 8.1 8.2 Lua error in package.lua at line 80: module 'strict' not found.
  9. 9.0 9.1 Lua error in package.lua at line 80: module 'strict' not found.
  10. * gam Mic -- Star in double system, database entry, SIMBAD. Accessed on line November 20, 2008.
  11. 11.0 11.1 Entry 21013-3215, The Washington Double Star Catalog, United States Naval Observatory. Accessed on line November 20, 2008.
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