20 Leonis Minoris
20 Leonis Minoris
Observation data Epoch J2000 Equinox J2000 |
Constellation |
Leo Minor |
Right ascension |
10h 01m 00.66s[1] |
Declination |
+31° 55′ 25.2″[1] |
Apparent magnitude (V) |
5.40
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Characteristics |
Spectral type |
G3 Va/M6.5 |
U−B color index |
0.27 |
B−V color index |
0.65 |
Astrometry |
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Radial velocity (Rv) | +56.0 km/s |
Proper motion (μ) | RA: -527.63 ± 0.30[1] mas/yr Dec.: -429.42 ± 0.18[1] mas/yr |
Parallax (π) | 66.46 ± 0.32[1] mas |
Distance | 49.1 ± 0.2 ly (15.05 ± 0.07 pc) |
Absolute magnitude (MV) | 4.53 |
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Details |
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Radius | 1.247 ± 0.021[2] R☉ |
Luminosity | 1.378 ± 0.027[2] L☉ |
Temperature | 5735 ± 5.6[3] K |
Age | 6.2–7.7[4] Gyr |
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Other designations |
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20 LMi, GJ 376, HR 3951, BD +32°1964, HD 86728, LHS 2216, LTT 12671, GCTP 2366.00, SAO 61808, FK5 1258, HIP 49081. [5] |
20 Leonis Minoris is a binary star system in the constellation Leo Minor. It has a relatively high proper motion. The companion is an old, active red dwarf star that has a relatively high metallicity.[6] The two stars are currently separated by 14.5 arc seconds.
References
- ↑ 1.0 1.1 1.2 1.3 1.4 van Leeuwen, F. (2007), "HIP 49081", Hipparcos, the New Reduction, retrieved 2009-12-18
- ↑ 2.0 2.1 Boyajian, Tabetha S. et al. (February 2012), "Stellar Diameters and Temperatures. I. Main-sequence A, F, and G Stars", The Astrophysical Journal 746 (1): 101, arXiv:1112.3316, Bibcode:2012ApJ...746..101B, doi:10.1088/0004-637X/746/1/101 . See Table 10.
- ↑ Kovtyukh; Soubiran, C.; Belik, S. I.; Gorlova, N. I. (2003), "High precision effective temperatures for 181 F-K dwarfs from line-depth ratios", Astronomy and Astrophysics 411 (3): 559–564, arXiv:astro-ph/0308429, Bibcode:2003A&A...411..559K, doi:10.1051/0004-6361:20031378
- ↑ Mamajek, Eric E.; Hillenbrand, Lynne A. (November 2008), "Improved Age Estimation for Solar-Type Dwarfs Using Activity-Rotation Diagnostics", The Astrophysical Journal 687 (2): 1264–1293, arXiv:0807.1686, Bibcode:2008ApJ...687.1264M, doi:10.1086/591785
- ↑ "HD 86728 -- High proper-motion Star", Simbad Astronomical Object Database, retrieved 2006-07-31
- ↑ Gizis, J. E. et al. (2000), "Two Nearby M Dwarf Binaries from 2MASS" (ABSTRACT PAGE), Monthly Notices of the Royal Astronomical Society 311 (2): 385, Bibcode:2000MNRAS.311..385G, doi:10.1046/j.1365-8711.2000.03060.x
External links
← Known celestial objects within 45–50 light-years → |
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| | Celestial objects by systems. Secondary members are listed in small print. |
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- GJ 898 (45.5±0.9 ly)
- 2 red dwarfs: GJ 897 A
- B
- Gliese 532 (45.7±0.6 ly)
- HD 23356 (45.8±0.6 ly)
- Gliese 42 (45.9±0.5 ly)
- Gliese 726 (46.1±0.8 ly)
- Gliese 529 (46.3±0.7 ly)
- Gliese 282 (46.3±0.6 ly)
- K-type main-sequence star B
- HR 7578 (46.4±0.5 ly)
- red dwarf B
- Gliese 481 (46.6±0.7 ly)
- Gliese 613 (46.8±0.6 ly)
- HD 150689 (46.9±0.7 ly)
- Gliese 546 (47.0±0.7 ly)
- Gliese 259 (47.7±0.5 ly)
- OU Geminorum (47.8±0.8 ly)
- star B
- Gliese 604 (47.8±0.7 ly)
- Gliese 420 (47.9±0.8 ly)
- red dwarf B
- Gliese 833 (48.1±0.6 ly)
- Gliese 269 (48.2±0.6 ly)
- K-type main-sequence star B
- Gliese 818 (48.4±1.0 ly)
- AB Doradus (48.7±0.4 ly)
- 2 red dwarfs: C
- B
- Gliese 14 (48.9±0.8 ly)
- Gliese 52 (49.1±0.9 ly)
- Gliese 483 (49.1±0.6 ly)
- GJ 1279 (49.2±0.7 ly)
- Gliese 141 (49.3±0.7 ly)
- Gliese 40 (49.6±1.1 ly)
- red dwarf B
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- WISEP J004701.06+680352.1 (48.9±16.3 ly)
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- WISE 0323-6025 (~45.3 ly)
- WISE 0335+4310 (~45.7 ly)
- WISE 0723+3403 (~45.7 ly)
- WISE 0819-0335 (~46.0 ly)
- WISE 2209-2734 (~46.0 ly)
- WISE 2237+7228 (~46.0 ly)
- WISE 2344+1034 (~46.0 ly)
- WISE 0458+6434 (46.6+17.4
−9.9 ly)
- T-type brown dwarf B
- WISE 0223-2932 (~47.0 ly)
- WISE 0500-1223 (~47.0 ly)
- WISE 1812+2721 (~47.0 ly)
- VHS J125804.89-441232.4 (47.1±5.9 ly)
- WISE 0744+5628 (~47.3 ly)
- WISE 1309-1600 (~47.3 ly)
- WISE 0040+0900 (~47.6 ly)
- WISE 1018-2445 (~47.6 ly)
- WISE 2018-7423 (~47.9 ly)
- WISE 0015-4615 (~48.6 ly)
- WISE 2343-7418 (~48.6 ly)
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| | | | Italic are systems without known trigonometric parallax. |
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