Phi Sagittarii

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

Location of φ Sagittarii (circled)
Observation data
Epoch J2000      Equinox J2000
Constellation Sagittarius
Right ascension 18h 45m 39.38610s[1]
Declination –26° 59′ 26.7944″[1]
Apparent magnitude (V) 3.17[2]
Characteristics
Spectral type B8.5 III[3] to B7 IV[4]
U−B color index –0.36[5]
B−V color index –0.11[5]
Astrometry
Radial velocity (Rv) +21.5[2] km/s
Proper motion (μ) RA: +50.61[1] mas/yr
Dec.: +1.22[1] mas/yr
Parallax (π) 13.63 ± 0.19[1] mas
Distance 239 ± 3 ly
(73 ± 1 pc)
Details
Mass 4–4.2[6] M
Radius 4.8[6] R
Luminosity 475[6] L
Temperature 14,990[4] K
Rotational velocity (v sin i) 35[7] km/s
Age 1.65 × 108[6] years
Other designations
φ Sagittarii, φ Sgr, Phi Sgr, 27 Sagittarii, 27 Sagittarii, CPD-27  5241, FK5 1487, GC 25661, HD 173300, HIP 92041, HR 7039, PPM 297231, SAO 268859.[8]

Phi Sagittarii (Phi Sgr, φ Sagittarii, φ Sgr) is a star in the southern constellation of Sagittarius. With an apparent visual magnitude of 3.17,[2] it is the ninth brightest star in the constellation and is readily visible to the naked eye. Parallax measurements place it at a distance of roughly 239 light-years (73 pc) from the Earth.[1]

The stellar classification of this star has been rated at B8.5 III[3] and B7 IV,[4] with a luminosity class of III indicating it is a giant star, while a class of IV suggests it is still a subgiant star. Both represent stages in the evolution of a star after it has exhausted the hydrogen at its core. This energy is being radiated from the star's outer envelope at an effective temperature of 14,990 K,[4] which produces the blue-white hue typical of B-type stars.[9]

In the past, this star catalogued as a spectroscopic binary and a companion was apparently detected through lunar occultation.[10] However, it is most likely a solitary star[6][11] and any nearby stars are merely optical companions.

Name and etymology

References

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  13. skywatchers Archived May 17, 2007 at the Wayback Machine
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  15. Jack W. Rhoads - Technical Memorandum 33-507-A Reduced Star Catalog Containing 537 Named Stars, Jet Propulsion Laboratory, California Institute of Technology; November 15, 1971
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  17. (Chinese) AEEA (Activities of Exhibition and Education in Astronomy) 天文教育資訊網 2006 年 5 月 11 日