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14 Sagittae
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Binary star system in the constellation Aquila
J2000
Aquila
20 03 30.01476
+16 01 52.5083
5.89
main sequence
B9p HgMn
−0.06
−0.44
−21.7
+5.420
−8.189
4.9546
0.0550
−0.72
61.541 d
0.49
2440799.01 JD
345
4.2
14 Sge A
291.53
13,200
3.60
7.0 0.5
14 Sge +15°4033 190229 98754 7664 105615 27812
14+Sge
14 Sagittae is a binary star system in the equatorial constellation of Aquila. 14 Sagittae is the Flamsteed designation. It appears as a sixth magnitude star, near the lower limit of visibility to the naked eye, having an apparent visual magnitude of 5.89. The system is located 658 light years away, as determined from its annual parallax shift of 4.95 mas. It is moving closer to the Earth with a heliocentric radial velocity of –22 km/s.
This is a single-lined spectroscopic binary with an orbital period of 61.5 days and an eccentricity of 0.49. The visible component is a chemically peculiar mercury-manganese star with a stellar classification of B9p HgMn. It is narrow-lined with a projected rotational velocity of 7 km/s. The star is radiating 292 times the Sun's luminosity from its photosphere at an effective temperature of 13,200 K.
John Flamsteed labelled this star as y Sagittae, but the designation was dropped by later authors and is now largely unknown.
References
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Wilson Ralph Elmer
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Carnegie Institute Washington D.C. Publication
Carnegie Institution of Washington
Washington 1953
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Astronomy and Astrophysics
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Elemental abundance analyses with DAO spectrograms: XL
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External links
HR 7664
Image 14 Sagittae
Category:Mercury-manganese stars
Category:Spectroscopic binaries
Category:Aquila (constellation)
BD+15 4033
Sagittae, 14
190229
098754
7664
Category:B-type giants
Category:B9 stars