Zeta Sagittarii

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

Location of ζ Sagittarii (circled) near the center
Observation data
Epoch J2000.0      Equinox J2000.0
Constellation Sagittarius
Right ascension 19h 02m 36.73024s[1]
Declination –29° 52′ 48.2279″[1]
Apparent magnitude (V) +2.59[2] (3.27/3.48)[3]
Characteristics
Spectral type A2.5 Va[4]
U−B color index +0.05[2]
B−V color index +0.08[2]
Astrometry
Radial velocity (Rv) +22[5] km/s
Proper motion (μ) RA: +10.79[1] mas/yr
Dec.: +21.11[1] mas/yr
Parallax (π) 36.98 ± 0.87[1] mas
Distance 88 ± 2 ly
(27.0 ± 0.6 pc)
Absolute magnitude (MV) 1.11/1.32[3]
Orbit[3]
Period (P) 21.00 ± 0.01 years
Semi-major axis (a) 0.489 ± 0.001"
Eccentricity (e) 0.211 ± 0.001
Inclination (i) 111.1 ± 0.1°
Longitude of the node (Ω) 74.0 ± 0.1°
Periastron epoch (T) 2005.99 ± 0.03
Argument of periastron (ω)
(secondary)
7.2 ± 0.6°
Details
Surface gravity (log g) 3.90[6] cgs
Temperature 8,799[6] K
Rotational velocity (v sin i) 77[7] km/s
Other designations
Ascella, ζ Sagittarii, ζ Sgr, Zeta Sgr, 38 Sagittarii, CCDM J19026-2953AB, CPD-30  5798, GC 26161, HD 176687, HIP 93506, HR 7194, IDS 18562-3001 AB, PPM 269230, SAO 187600, WDS J19026-2953AB.[4]

Zeta Sagittarii (Zeta Sgr, ζ Sagittarii, ζ Sgr) is the third brightest star system in the constellation Sagittarius, with an apparent visual magnitude of +2.59.[2] It has the traditional name Ascella. Based upon parallax measurements, the distance to Ascella is about 88 ly (27 pc).[1] Ascella is moving away from the Solar System with a radial velocity of 22 km s−1.[5] Some 1.0–1.4 million years ago, this system came within 7.5 ± 1.8 ly (2.30 ± 0.55 pc) of the Sun.[8]

This is a binary star system, with the two components orbiting each other over a period of 21 years at an eccentricity of 0.211. The combined mass of the system is 5.26 ± 0.37 times the mass of the Sun[3] and their blended stellar classification is A2.5 Va.[4]

The system consists of a spectral class A2 giant with an apparent magnitude of +3.27, and an A4 subgiant with apparent magnitude of +3.48. The pair have a mean separation of 13.4 astronomical units (AU).[9] Ascella has a faint, 10th magnitude companion, separated from the primary by a distance of 75 arcseconds.

Name and etymology

Namesakes

References

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  11. skywatchers[dead link]
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  14. (Chinese) AEEA (Activities of Exhibition and Education in Astronomy) 天文教育資訊網 2006 年 5 月 11 日