Delta1 Chamaeleontis

Star in the constellation Chamaeleon From Wikipedia, the free encyclopedia

Delta1 Chamaeleontis is a close double star located in the constellation Chamaeleon. Its name is a Bayer designation that is Latinized from δ1 Chamaeleontis, and abbreviated Delta1 Cha or δ1 Cha. They have a combined apparent visual magnitude of 5.47,[3] which is just bright enough to be faintly visible to the naked eye as a point of light on a dark rural night. With an annual parallax shift of 9.36 mas,[2] it is located around 350 light-years (110 pc) 350 light years from the Sun.

Right ascension10h 45m 16.31446s[2]
Declination−80° 28 10.5409[2]
Apparentmagnitude(V)5.47[3] (6.266 + 6.503)[4]
Quick facts Constellation, Right ascension ...
δ1 Chamaeleontis
Location of δ1 Chamaeleontis (circled in red)
Observation data
Epoch J2000.0      Equinox J2000.0 (ICRS)
Constellation Chamaeleon[1]
Right ascension 10h 45m 16.31446s[2]
Declination −80° 28 10.5409[2]
Apparent magnitude (V) 5.47[3] (6.266 + 6.503)[4]
Characteristics
Spectral type K0 III[5]
U−B color index +0.74[3]
B−V color index +0.95[3]
Astrometry
Radial velocity (Rv)+10.7[6] km/s
Proper motion (μ) RA: −17.28[2] mas/yr
Dec.: −29.25[2] mas/yr
Parallax (π)9.36±0.45 mas[2]
Distance350 ± 20 ly
(107 ± 5 pc)
Absolute magnitude (MV)+0.32[1]
Details
Luminosity76[7] L
Temperature5,052[7] K
Other designations
δ1 Cha, CPD−79°554, HD 93779, HIP 52595, HR 4231, SAO 258592, WDS J10453-8028[8]
Database references
SIMBADdata
Close

This pair is one of two stars named Delta Chamaeleontis, the other being the slightly brighter Delta2 Chamaeleontis located about 6 arcminutes away.[9] Delta Chamaeleontis forms the southernmost component of the constellation's "dipper" or bowl. Together with Gamma Chamaeleontis, they point to a spot that is within 2° of the south celestial pole.[10]

The two components of Delta1 Chamaeleontis have visual magnitudes of 6.3 and 6.5. As of 2000, the pair had an angular separation of 0.783 arcseconds along a position angle of 83.8°.[4] They can be visually separated using a 7.9 in (20 cm) aperture telescope.[9] The pair is a source of X-ray emission with a flux of 27.4×10−17 W/m2.[11] The stellar classification of Delta1 Chamaeleontis is K0 III,[5] which matches an evolved K-type giant star.

References

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