Gamma Sagittarii

From Wikipedia, the free encyclopedia

The Bayer designation Gamma Sagittarii (γ Sgr / γ Sagittarii) is shared by two star systems in the constellation Sagittarius, γ1 Sagittarii and γ2 Sagittarii. They are separated by 0.86° on the sky, and can be resolved by the human eye.

[edit] γ¹ Sagittarii

γ¹ Sagittarii
Observation data
Epoch J2000.0
Constellation
(pronunciation)
Sagittarius
Right ascension 18h 05m 01.3s
Declination -29° 34' 48"
Apparent magnitude (V) +4.66 (mean)
Distance 2000 ± 1200 ly
(600 ± 370 pc)
Spectral type F4-G1Ib
Other designations
W Sagittarii, HR 6742,
HD 164975, SAO 186237,
HIP 88567, ADS 11029,
CCDM 18050-2935

Gamma-1 Sagittarii (γ¹ Sgr / γ¹ Sagittarii) is a cepheid variable star in the constellation Sagittarius. It is often referred to by its variable star designation, W Sagittarii.

This variable star changes in apparent magnitude from +4.3 to +5.1 with a period of 7.59 days. Its change in brightness is accompanied by a change in spectral classification, from G1 to F4. Based on its variablility, W Sagittarii has been estimated to be approximately 1500 light years from Earth.

W Sagittarii also shows evidence of being a close binary star, as well has having two more distant 13th magnitude companions, W Sagittarii B, and C separated by 33 and 48 arcseconds respectively.


[edit] γ² Sagittarii

γ² Sagittarii
Observation data
Epoch J2000.0
Constellation
(pronunciation)
Sagittarius
Right ascension 18h 05m 48.5s
Declination -30° 25' 27"
Apparent magnitude (V) +2.98
Distance 96.1 ± 2.5 ly
(29.5 ± 0.8 pc)
Spectral type K0III
Other designations
Alnasl, 10 Sagittarii,
HR 6746, HD 165135,
SAO 209696, HIP 88635

Gamma-2 Sagittarii (γ² Sgr / γ² Sagittarii) is a star in the constellation Sagittarius. It also has the traditional names Nash, Alnasl, Nasl, or El Nasl, which are derived from the Arabic النصل an-naşl meaning arrowhead.

Alnasl is a spectral type K0 giant, and has an apparent magnitude of +2.98. Alnasl is 96 light years from Earth.