HD 111968, also known by the Bayer designation n Centauri (n Cen), is a star in the constellation Centaurus.
Observation data Epoch J2000.0 Equinox J2000.0 | |
---|---|
Constellation | Centaurus |
Right ascension | 12h 53m 26.20svan Leeuwen, Floor (13 August 2007). "Validation of the new Hipparcos reduction". Astronomy & Astrophysics. 474 (2): 653–664. arXiv:0708.1752. Bibcode:2007A&A...474..653V. doi:10.1051/0004-6361:20078357. eISSN 1432-0746. ISSN 0004-6361. |
Declination | −40° 10′ 43.9″[1] |
Apparent magnitude (V) | +4.25 |
Characteristics | |
Spectral type | A7III |
U−B color index | +0.12 |
B−V color index | +0.22[2] |
Variable type | none |
Astrometry | |
Proper motion (μ) | RA: +70.84±0.14[1] mas/yr Dec.: −22.54±0.10[1] mas/yr |
Parallax (π) | 21.95 ± 0.19 mas[1] |
Distance | 149 ± 1 ly (45.6 ± 0.4 pc) |
Absolute magnitude (MV) | +0.86[2] |
Details | |
Temperature | 7,648[2] K |
Rotational velocity (v sin i) | 92.4±4.6[2] km/s |
Other designations | |
Database references | |
SIMBAD | data |
n Centauri is a white A-type giant with an apparent magnitude of +4.25. It is approximately 149 light years from Earth.
References
- ^ a b c d van Leeuwen, F. (2007). "Validation of the new Hipparcos reduction". Astronomy and Astrophysics. 474 (2): 653–664. arXiv:0708.1752. Bibcode:2007A&A...474..653V. doi:10.1051/0004-6361:20078357. Vizier catalog entry
- ^ a b c d Ammler-von Eiff, M.; Reiners, A. (June 2012), "New measurements of rotation and differential rotation in A-F stars: are there two populations of differentially rotating stars?", Astronomy & Astrophysics, 542: A116, arXiv:1204.2459, Bibcode:2012A&A...542A.116A, doi:10.1051/0004-6361/201118724.