HD 121228
HD 121228 is a blue supergiant star located in the constellation Centaurus. The star is noted for its close visual proximity to the planetary nebula SuWt 2.[5][6]
Observation data Epoch J2000 Equinox J2000 | |
---|---|
Constellation | Centaurus |
Right ascension | 13h 55m 52.322s[1] |
Declination | −59° 22′ 16.45″[1] |
Apparent magnitude (V) | 7.86[2] |
Characteristics | |
Spectral type | B1 Ib |
Apparent magnitude (U) | 7.34 |
Apparent magnitude (B) | 8.00 |
Apparent magnitude (V) | 7.86 |
Apparent magnitude (R) | 8.88 |
Apparent magnitude (G) | 7.7591 |
Apparent magnitude (J) | 7.428 |
Apparent magnitude (H) | 7.426 |
Apparent magnitude (K) | 7.385 |
Astrometry | |
Parallax (π) | 0.6538 ± 0.0435[1] mas |
Distance | 5,000 ± 300 ly (1,500 ± 100 pc) |
Absolute magnitude (MV) | -5.778[3] |
Details | |
Mass | 7.0[4] M☉ |
Temperature | 26,424[3] K |
Age | 31.6[4] Myr |
Other designations | |
Database references | |
SIMBAD | data |
References
- Brown, A. G. A.; et al. (Gaia collaboration) (August 2018). "Gaia Data Release 2: Summary of the contents and survey properties". Astronomy & Astrophysics. 616. A1. arXiv:1804.09365. Bibcode:2018A&A...616A...1G. doi:10.1051/0004-6361/201833051. Gaia DR2 record for this source at VizieR.
- Zacharias, N.; Finch, C. T.; Girard, T. M.; Henden, A.; Bartlett, J. L.; Monet, D. G.; Zacharias, M. I. (2012). "VizieR Online Data Catalog: UCAC4 Catalogue (Zacharias+, 2012)". VizieR On-line Data Catalog. Bibcode:2012yCat.1322....0Z.
- Westin, T. N. G. (1985). "The local system of early type stars. Spatial extent and kinematics". Astronomy and Astrophysics Supplement Series. 60: 99. Bibcode:1985A&AS...60...99W.
- Tetzlaff, N.; Neuhäuser, R.; Hohle, M. M. (2011). "A catalogue of young runaway Hipparcos stars within 3 kpc from the Sun". Monthly Notices of the Royal Astronomical Society. 410 (1): 190. arXiv:1007.4883. Bibcode:2011MNRAS.410..190T. doi:10.1111/j.1365-2966.2010.17434.x.
- "HD 121228". SIMBAD. Retrieved November 26, 2018.
- "PN SuWt 2". SIMBAD. Retrieved November 26, 2018.
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