Beta Reticuli
Observation data ICRS )
| ||
---|---|---|
Constellation | Reticulum
| |
Right ascension | 03h 44m 11.97587s[1] | |
Declination | −64° 48′ 24.8610″[1] | |
Apparent magnitude (V) | +3.84[2] | |
Characteristics | ||
Spectral type | K0IV SB[3] | |
U−B color index | +1.11[2] | |
B−V color index | +1.13[2] | |
Absolute magnitude (MV) | +1.46±0.03[3] | |
Semi-amplitude (K1)(primary) | 5.1235±0.0025 km/s | |
Details | ||
β Ret A | ||
Gyr | ||
β Ret B | ||
Mass | 0.4±0.1[3] M☉ | |
Database references | ||
SIMBAD | data |
Beta Reticuli (Beta Ret, β Reticuli, β Ret) is
This is a single-lined
During the mid-20th century, the Dutch-American astronomer Willem Jacob Luyten proposed that the G3V star HD 24293 formed a third component of this system, based upon similar proper motions. However, this was subsequently ruled out based on more accurate measurements, since their actual distances, radial velocities, and proper motions do not match.[7]
Beta Reticuli is moving through the Galaxy at a speed of 69.2 km/s relative to the Sun. Its projected Galactic orbit carries it between 10,100 and 24,200 light years from the center of the Galaxy.[8] Beta Reticuli came closest to the Sun 319,000 years ago when it had brightened to magnitude 2.98 from a distance of 67 light years.[8]
Naming
In Chinese caused by adaptation of the European southern hemisphere constellations into the Chinese system, 蛇首 (Shé Shǒu), meaning Snake's Head, refers to an asterism consisting of β Reticuli and α Hydri. Consequently, β Reticuli itself is known as 蛇首二 (Shé Shǒu èr, English: the Second Star of Snake's Head.)[9]
References
- ^ S2CID 18759600.
- ^ Bibcode:1986EgUBV........0M.
- ^ .
- S2CID 59451347, A61.
- ^ "* bet Ret". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 2017-02-13.
- S2CID 14878976.
- S2CID 118194112.
- ^ a b Beta Reticuli (HIP 17440) Archived January 2, 2013, at the Wayback Machine
- ^ (in Chinese) AEEA (Activities of Exhibition and Education in Astronomy) 天文教育資訊網 2006 年 7 月 27 日