Mu Fornacis

Star in the constellation Fornax From Wikipedia, the free encyclopedia

μ Fornacis (Latinised as Mu Fornacis) is a star in the southern constellation of Fornax. With an apparent visual magnitude of 5.27,[3] it is visible to the naked eye. The distance to this star, as determined by its annual parallax shift of 10.18 mas,[2] is around 320 light years.

Right ascension02h 12m 54.46962s[2]
Declination−30° 43 25.7732[2]
Quick facts Constellation, Right ascension ...
Mu Fornacis
Observation data
Epoch J2000.0      Equinox J2000.0 (ICRS)
Constellation Fornax[1]
Right ascension 02h 12m 54.46962s[2]
Declination −30° 43 25.7732[2]
Apparent magnitude (V) 5.27[3]
Characteristics
Evolutionary stage main sequence[4]
Spectral type A0 V[5]
U−B color index −0.06[3]
B−V color index −0.02[3]
Astrometry
Radial velocity (Rv)10.0±3.7[6] km/s
Proper motion (μ) RA: +14.10[2] mas/yr
Dec.: +6.85[2] mas/yr
Parallax (π)10.18±0.24 mas[2]
Distance320 ± 8 ly
(98 ± 2 pc)
Absolute magnitude (MV)+0.31[1]
Details[7]
Mass2.55±0.34 M
Radius2.9±0.1 R
Luminosity75±4 L
Surface gravity (log g)3.92±0.06 cgs
Temperature9,977±136 K
Rotational velocity (v sin i)320[5] km/s
Age188[8] Myr
Other designations
μ For, CD−31°882, FK5 78, GJ 89, HD 13709, HIP 10320, HR 652, SAO 193573[9]
Database references
SIMBADdata
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This is an A-type main sequence star with a stellar classification of A0 V.[5] It is a Be star that displays "central quasi emission" (CQE) bumps in its spectrum due to a surrounding shell of material.[10] The star has an estimated 2.6 times the mass of the Sun and 2.9 times the Sun's radius.[7] Mu Fornacis is spinning rapidly with a projected rotational velocity of 320 km/s[5] and is around 188 million years old.[8] It radiates 75 times the solar luminosity from its outer atmosphere at an effective temperature of 9,977 K.[7]

Mu Fornacis appears to be emitting an infrared excess at a wavelength of 22 μm, which could be due to an orbiting debris disk.[11]

References

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