Nu Sagittarii

Nu Sagittarii

The Bayer designation Nu Sagittarii (ν Sgr, ν Sagittarii) is shared by two star systems, ν¹ Sagittarii and ν² Sagittarii, in the constellation Sagittarius. The two stars are separated by 0.23° in the sky. Nu Sagittarii also has the traditional name Ain al Rami, from the Arabic عين الرامي cain ar-rāmī meaning eye of the archer[1].

Nu Sagittarii is often cited as one of the earliest identified double stars. In the Almagest, Ptolemy describes the star as "nebulous and double", referring to the double nature of the star, as well as the nearby globular cluster NGC 6717.[citation needed][clarification needed]

ν¹ Sagittarii

ν¹ Sagittarii
Observation data
Epoch J2000.0      Equinox J2000.0
Constellation Sagittarius
Right ascension 18h 54m 10.2s
Declination -22° 44' 42"
Apparent magnitude (V) +4.86
Distance 1850 ± 900 ly
(570 ± 270 pc)
Spectral type K2I+B9V:
Other designations
32 Sagittarii, HR 7116,
HD 174974, SAO 187426,
HIP 92761, ADS 11794,
CCDM 18542-2245

Nu-1 Sagittarii is a triple star system lying approximately 1850 light years from Earth. The primary component, Nu-1 Sagittarii A, is a spectral type K1 bright giant which has an apparent magnitude of +4.86. It is orbited by two magnitude +10.8 companions: Nu-1 Sagittarii B at a distance of 2.5 arcseconds from the primary, and Nu-1 Sagittarii C at a distance of 28.2 arcseconds.


ν² Sagittarii

ν² Sagittarii
Observation data
Epoch J2000.0      Equinox J2000.0
Constellation Sagittarius
Right ascension 18h 55m 07.1s
Declination -22° 40' 17"
Apparent magnitude (V) +5.00
Distance 270 ± 21 ly
(83 ± 6 pc)
Spectral type K1Ib/II
Other designations
35 Sagittarii, HR 7120,
HD 175190, SAO 187445,
HIP 92845

Nu-2 Sagittarii A is a spectral type K1 supergiant which has an apparent magnitude of +5.00. It is approximately 270 light years from Earth.


References