HD 125072
HD 125072 is K3-IV class star in the constellation Centaurus. The components of the space velocity for this star are U=−18.5, V=−6.9 and W=−26.9 km/s. Based on the composition and kinematics of this star, it has an estimated age of about 10 billion years.[3]
References
- ↑ 1.0 1.1 1.2 1.3 1.4 1.5 1.6 1.7 "SIMBAD query result: LHS 2892 -- High proper-motion Star". Centre de Données astronomiques de Strasbourg. Retrieved 2008-04-09.
- ↑ 2.0 2.1 Perrin, M.-N.; Cayrel de Strobel, G.; Dennefeld, M. (1988). "High S/N detailed spectral analysis of four G and K dwarfs within 10 PC of the sun". Astronomy and Astrophysics 191 (2): 237–247. Bibcode:1988A&A...191..237P.
- ↑ 3.0 3.1 3.2 Lachaume, R.; Dominik, C.; Lanz, T.; Habing, H. J. (1999). "Age determinations of main-sequence stars: combining different methods". Astronomy and Astrophysics 348: 897–909. Bibcode:1999A&A...348..897L.
← Known celestial objects within 35–40 light-years → |
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| | Celestial objects by systems. Secondary members are listed in small print. |
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- 2MASS J16452211-1319516 (36.19±0.33 ly)
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- WISE 2313-0837 (~35.9 ly)
- WISE 0325+0831 (~36.5 ly)
- WISE 0038+2768 (~36.9 ly)
- WISE 0627-1114 (~37.2 ly)
- WISE 1959-3338 (~37.2 ly)
- WISE 0623-0456 (~37.5 ly)
- WISE 2325-4105 (~37.5 ly)
- WISE 2340-0745 (~37.8 ly)
- WISE 0759-4904 (~38.8 ly)
- WISE 0751-7634 (~39.1 ly)
- WISE 1653+4444 (~39.5 ly)
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| | Italic are systems without known trigonometric parallax. |
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