Alpha Microscopii

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Template:Short description

α Microscopii
Template:Location mark
Location of α Microscopii (circled)
Observation data
Epoch J2000.0      Equinox J2000.0 (ICRS)
Constellation Microscopium
Right ascension Template:RA[1]
Declination Template:DEC[1]
Apparent magnitude (V) 4.89±0.01[2]
Characteristics
Spectral type G7 III[3] or G8 III[4]
U−B Template:Engvar +0.73[5]
B−V Template:Engvar +1.00[5]
Astrometry
Radial velocity (Rv)−14.50±0.09[6] km/s
Proper motion (μ) RA: +15.057 mas/yr[1]
Dec.: −23.524 mas/yr[1]
Parallax (π)8.2508±0.1563 mas[7]
DistanceTemplate:Rnd ± Template:Rnd ly
(Template:Rnd ± Template:Rnd pc)
Absolute magnitude (MV)−0.45 ± 0.20[8]
Details[9]
Mass3.19±0.32 Template:Solar mass
Radius18.41±1.38 Template:Solar radius
Luminosity173±25 Template:Solar luminosity
Surface gravity (log g)2.27±0.11 cgs
Temperature4,881±43 K
Metallicity [Fe/H]−0.06±0.04 dex
Rotational velocity (v sin i)2.6±2[10] km/s
Age400[11] Myr
Metallicity [Fe/H]{{{metal_fe2}}} dex
Other designations
Template:Odlist[12][13]
Database references
SIMBADdata

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Alpha Microscopii (α Microscopii) is a star in the southern constellation of Microscopium.[13] It is visible to the naked eye with an apparent visual magnitude of 4.89.[2] Based upon an annual parallax shift of Script error: No such module "val". as seen from the Earth, it is located 395 light years from the Sun, give or take 7 light years. The star is moving nearer to the Sun with a heliocentric radial velocity of Script error: No such module "val".[6]

This is an evolved giant star of type G with a stellar classification of either G7 III[3] or G8 III[4] depending on the source. At the age of 400 million years, it has an estimated 3.19 times the mass of the Sun and has expanded to 18.4 times the Sun's radius.[9] The star is radiating 173 times the Sun's luminosity from its expanded photosphere at an effective temperature of Script error: No such module "val"., giving a yellow hue.[9]

This star has an optical visual companion, CCDM J20500-3347B, of apparent visual magnitude 10.0 approximately 20.4 arcseconds away at a position angle of 166°.[14] It has no physical connection to the star described above.[15] As for Alpha Microscopii, it was found to be a probable spectroscopic binary in 2014.[10]

References

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  1. a b c Template:Cite Gaia EDR3
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  3. a b Script error: No such module "Citation/CS1".
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  5. a b Script error: No such module "Citation/CS1".
  6. a b Script error: No such module "Citation/CS1".
  7. Template:Cite DR2
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  9. a b c Script error: No such module "Citation/CS1".
  10. a b Script error: No such module "Citation/CS1".
  11. Script error: No such module "Citation/CS1".
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  13. a b * alf Mic -- Star in double system, database entry, SIMBAD. Accessed on line September 4, 2008.
  14. Script error: No such module "Citation/CS1".
  15. Script error: No such module "citation/CS1".

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Template:Stars of Microscopium