63 Ophiuchi

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63 Ophiuchi
Diagram showing star positions and boundaries of the Sagittarius constellation and its surroundings
Cercle rouge 100%.svg

The location of 63 Ophiuchi (circled) in the constellation Sagittarius
Observation data
Epoch J2000.0      Equinox J2000.0 (ICRS)
Constellation Sagittarius
Right ascension 17h 54m 54.04380s[1]
Declination −24° 53′ 13.5413″[1]
Apparent magnitude (V) 6.20[2]
Characteristics
Spectral type O8II((f))[3]
U−B color index –0.89[4]
B−V color index +0.04[4]
Astrometry
Radial velocity (Rv) –11[5] km/s
Proper motion (μ) RA: 1.66[1] mas/yr
Dec.: –2.63[1] mas/yr
Parallax (π) −0.77 ± 0.40[1] mas
Absolute magnitude (MV) −6.0[6]
Details
Surface gravity (log g) 3.5[7] cgs
Temperature 34,000[7] K
Rotational velocity (v sin i) 35[7]-86[8] km/s
Other designations
63 Oph, HR 6672, HD 162978, HIP 87706, SAO 185928
Database references
SIMBAD data

63 Ophiuchi is an O-type giant star in the constellation Sagittarius, despite its name. During a 2009 survey for companions of massive stars, it was observed using speckle interferometry but no companion was found.[9] Uncertain negative parallax measurements of –0.77 ± 0.40 mas suggest that this extremely luminous star may be located about 4000 light-years away. An estimate of the distance based on the strength of the Ca II line yields a more modest value of 2,605 ly (799 pc).[10] The star lies only 0.3° north of the galactic plane.

In 1983, astronomers from the Sternberg Astronomical Institute in Moscow, Russia identified a faint, shell-shaped nebula surrounding the star that was being excited by the star's energy. Named Sharpless 22, this ring-shaped nebula has a double-shell structure with an inner envelope spanning 45–50 (9–18 pc), surrounded by a diffuse envelope some 65–80′ (14–29 pc) across. At an estimated mass loss rate of (6–8) × 10−6 M/yr, it would take the star about (1–5) × 105 years to produce such a nebula from the outflow of its stellar wind.[11]

References

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