HD 84117
From Wikipedia, the free encyclopedia
HD 84117 is a F-type main sequence star in the constellation of Hydra.[1] It has an apparent visual magnitude of approximately 4.94.[1]
References
- ↑ 1.0 1.1 1.2 1.3 1.4 1.5 1.6 1.7 1.8 1.9 1.10 LTT 3558 -- High proper-motion Star, database entry, SIMBAD. Accessed on line January 20, 2011.
- ↑ 2.0 2.1 2.2 HR 3862, database entry, The Bright Star Catalogue, 5th Revised Ed. (Preliminary Version), D. Hoffleit and W. H. Warren, Jr., CDS ID V/50. Accessed on line January 20, 2011.
- ↑ From apparent magnitude and parallax.
- ↑ 4.0 4.1 4.2 4.3 4.4 HD 84117, database entry, The Geneva-Copenhagen Survey of Solar neighbourhood, J. Holmberg et al., 2007, CDS ID V/117A. Accessed on line January 20, 2011.
- ↑ HD 84117, database entry, Catalog of Apparent Diameters and Absolute Radii of Stars (CADARS), 3rd edition, L. E. Pasinetti-Fracassini, L. Pastori, S. Covino, and A. Pozzi, CDS ID II/224. Accessed on line January 20, 2011.
← Star systems within 45–50 light-years → |
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G (Yellow) |
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| V |
- 18 Scorpii (45.7 ± 0.6 ly; 1 star)
- 47 Ursae Majoris (45.9 ± 0.4 ly; 1 star, 3 planets: b
- c
- d)
- 26 Draconis (45.9 ± 0.3 ly; 3 stars)
- Pi¹ Ursae Majoris (46.6 ± 0.5 ly; 1 star)
- Gliese 611 (46.9 ± 0.4 ly; 2 stars)
- 72 Herculis (46.9 ± 0.4 ly; 1 star)
- Nu² Lupi (47.5 ± 0.5 ly; 1 star, 3 planets: b
- c
- d)
- HR 7898 (47.8 ± 0.6 ly; 1 star)
- Psi Serpentis (47.9 ± 0.6 ly; 2 stars)
- 20 Leonis Minoris «Cor» (48.6 ± 0.6 ly; 1 star)
- HR 209 (48.7 ± 0.5 ly; 2 stars)
- HD 176051 (48.9 ± 0.4 ly; 2 stars, 1 planet: b)
- 171 G. Puppis (49.6 ± 0.4 ly; 2 stars)
- HR 5864 (49.7 ± 0.6 ly; 2 stars)
- Mu Arae (49.8 ± 0.6 ly; 1 star, 4 planets: d
- e
- b
- c)
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K (Orange) |
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| V |
- Gliese 898/897 (45.5 ± 0.9 ly; 4 stars)
- Gliese 532 (45.7 ± 0.6 ly; 1 star)
- HD 23356 (45.8 ± 0.6 ly; 1 star)
- Gliese 42 (45.9 ± 0.5 ly; 1 star)
- Gliese 726 (46.1 ± 0.8 ly; 1 star)
- Gliese 529 (46.3 ± 0.7 ly; 1 star)
- Gliese 282 (46.3 ± 0.6 ly; 2 stars)
- HR 7578 (46.4 ± 0.5 ly; 2 stars)
- Gliese 481 (46.6 ± 0.7 ly; 1 star)
- Gliese 613 (46.8 ± 0.6 ly; 1 star)
- HD 150689 (46.9 ± 0.7 ly; 1 star)
- Gliese 546 (47.0 ± 0.7 ly; 1 star)
- Gliese 259 (47.7 ± 0.5 ly; 1 star)
- OU Geminorum (47.8 ± 0.8 ly; 2 stars)
- Gliese 604 (47.8 ± 0.7 ly; 1 star)
- Gliese 420 (47.9 ± 0.8 ly; 2 stars)
- Gliese 833 (48.1 ± 0.6 ly; 1 star)
- Gliese 269 (48.2 ± 0.6 ly; 2 stars)
- Gliese 818 (48.4 ± 1.0 ly; 1 star)
- AB Doradus (48.7 ± 0.4 ly; 2 stars)
- Gliese 14 (48.9 ± 0.8 ly; 1 star)
- Gliese 52 (49.1 ± 0.9 ly; 1 star)
- Gliese 483 (49.1 ± 0.6 ly; 1 star)
- GJ 1279 (49.2 ± 0.7 ly; 1 star)
- Gliese 141 (49.3 ± 0.7 ly; 1 star)
- Gliese 40 (49.6 ± 1.1 ly; 2 stars)
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- Gliese 400 (46.0 ± 1.6 ly; 2 stars)
- HIP 79431 (47.0+2.2
−2.0 ly; 1 star, 1 planet: b)
- CM Draconis (47.1 ± 1.8 ly; 2 stars, 0 (1?) planets: b?)
- GJ 1214 (47.5 ± 0.4 ly; 1 star, 1 planet: b)
- Gliese 123 (48.8 ± 1.3 ly; 1 star)
- Gliese 163 (48.9+1.4
−1.3 ly; 1 star, 3 (5?) planets: b
- e?
- c
- f?
- d)
- Gliese 317 (49.9 ± 0.4 ly; 1 star, 2 planets: b
- c)
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L |
- WISEP J004701.06+680352.1 (48.9 ± 16.3 ly; 1 brown dwarf)
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| T |
- WISE 0323-6025 (~45.3 ly; 1 brown dwarf)
- WISE 0335+4310 (~45.7 ly; 1 brown dwarf)
- WISE 0723+3403 (~45.7 ly; 1 brown dwarf)
- WISE 0819-0335 (~46.0 ly; 1 brown dwarf)
- WISE 2209-2734 (~46.0 ly; 1 brown dwarf)
- WISE 2237+7228 (~46.0 ly; 1 brown dwarf)
- WISE 2344+1034 (~46.0 ly; 1 brown dwarf)
- WISE 0458+6434 (46.6+17.4
−9.9 ly; 2 brown dwarfs)
- WISE 0223-2932 (~47.0 ly; 1 brown dwarf)
- WISE 0500-1223 (~47.0 ly; 1 brown dwarf)
- WISE 1812+2721 (~47.0 ly; 1 brown dwarf)
- VHS J125804.89-441232.4 (47.1 ± 5.9 ly; 1 brown dwarf)
- WISEPA J074457.15+562821.8 (~47.3 ly; 1 brown dwarf)
- WISE 1309-1600 (~47.3 ly; 1 brown dwarf)
- WISE 0040+0900 (~47.6 ly; 1 brown dwarf)
- WISE 1018-2445 (~47.6 ly; 1 brown dwarf)
- WISE 2018-7423 (~47.9 ly; 1 brown dwarf)
- WISE 0015-4615 (~48.6 ly; 1 brown dwarf)
- WISE 2343-7418 (~48.6 ly; 1 brown dwarf)
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In left column are stellar classes of primary members of star systems. Bold are systems containing at least one component with absolute magnitude of +8.5 or brighter. Italic are systems without known trigonometric parallax. |
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