List of star systems within 55–60 light-years
This is a list of star systems within 55-60 light years of Earth.
Star system | Median distance (ly) | Stars in system | Spectral type | Apparent magnitude (V) | Comments and references |
---|---|---|---|---|---|
HD 152391 | 55.2 ± 0.8 | 1 | GV | ||
Gliese 886 | 55.2 ± 3.4 | 2 | KV | ||
HR 6516 | 55.3 ± 0.8 | 2 | GV | ||
Gliese 565 | 55.3 ± 1 | 1 | KV | ||
WISE 0366-0143 | 55.4 | 1 | T | ||
WISE 1225-1013 | 55.4 | 1 | T6 | ||
WISE 1612-3420 | 55.4 | 1 | T6.5 | ||
WISE 1852+3537 | 55.4 | 1 | T7 | ||
HR 2997 | 55.6 ± 0.5 | 1 | GV | ||
Gliese 728 | 55.7 ± 1.5 | 1 | KV | ||
HD 76151 | 55.8 ± 0.8 | 1 | G3V | 6.00 | [1] |
HR 7232 | 56.0 ± 0.9 | 1 | GV | ||
HR 4864 | 56.0 ± 1 | 1 | GV | ||
WISE 0245-3450 | 56.1 | 1 | T8 | ||
WISE 1320+6034 | 56.1 | 1 | T6.5 | ||
Iota Horologii | 56.2 ± 0.5 | 1 | G0Vp | 5.40 | has 1 known planet[2][3] |
37 Geminorum | 56.3 ± 0.9 | 1 | G0V | 5.73 | [4][5] |
HD 3765 | 56.3 ± 1 | 1 | KV | ||
Gliese 3476 | 56.4 ± 0.6 | 1 | KV | ||
HIP 92444 | 56.4 ± 1.9 | 1 | KV | ||
Gliese 3222 | 56.4 ± 0.7 | 1 | KV | ||
ADS 9544 | 56.4 ± 0.8 | 2 | KV | ||
Gliese 727 | 56.4 ± 1 | 1 | KV | ||
Tau¹ Hydrae | 56.5 ± 2.2 | 2 | F6V | 4.59 | [6] |
Gliese 3833 | 56.5 ± 1 | 1 | KV | ||
DENIS-P J1058.7-1548 | 56.5 ± 1 | 1 | L3 | ||
q¹ Eridani | 56.6 ± 0.6 | 1 | F9V | 5.52 | has 1 known planet[7][8] |
HR 6748 | 56.6 ± 0.8 | 1 | GV | ||
HD 184467 | 56.6 ± 0.6 | 1 | KV | ||
Gliese 913 | 56.6 ± 2.9 | 1 | MV | ||
Xi Ophiuchi | 56.7 ± 0.9 | 2 | F2V | 4.39 | [9] |
10 Canum Venaticorum | 56.7 ± 0.6 | 1 | G0V | 5.95 | [10] |
BD +68 278 | 56.7 ± 2.8 | 3 | KV | ||
Rho Coronae Borealis | 56.8 ± 0.7 | 1 | G0V | 5.4 | has 1 known planet[11][12] |
WISE 1019+6529 | 56.8 | 1 | T9 | ||
Chi Eridani | 57.0 ± 0.6 | 1 | G8IV | 3.70 | [13][14] |
39 Serpentis | 57.0 ± 0.9 | 2 | GV | ||
Gliese 293.1 | 57.0 ± 1.5 | 2 | KV | ||
Gliese 397.1 | 57.0 ± 1.4 | 2 | MV | ||
g Lupi | 57.1 ± 0.7 | 1 | F5V | 4.64 | [15] |
Gliese 649.1 | 57.1 ± 0.7 | 3 | KV | ||
WISE 0247+3725 | 57.1 | 1 | T8 | ||
Xi Geminorum «Alzirr» | 57.2 ± 0.8 | 1 | F5IV | 3.35 | [16][17] |
58 Ophiuchi | 57.2 ± 0.8 | 1 | F5V | 4.87 | [18] |
Gliese 241 | 57.2 ± 1.4 | 1 | KV | ||
Gliese 3633 | 57.2 ± 1 | 1 | KV | ||
VVV BD001 | 57.2 +4.3 -3.8 | 1 | L | ||
59 Virginis | 57.3 ± 0.3 | 1 | G0V | 5.22 | has 1 known planet[19] |
HR 7783 | 57.3 ± 0.5 | 1 | GV | ||
HR 5384 | 57.4 ± 1.1 | 1 | GV | ||
HD 113194 | 57.4 ± 1.1 | 1 | KV | ||
Gliese 562 | 57.4 ± 1.3 | 1 | KV | ||
WISE 0528-3308 | 57.4 | 1 | T7 pec | ||
HD 1237 | 57.5 ± 0.5 | 1 | G6V | 6.59 | has 1 known planet[20] |
Gliese 1066 | 57.5 ± 0.9 | 1 | KV | ||
15 Sagittae | 57.6 ± 0.6 | 2 | G0V + L4 | 5.8 | [21] |
83 Leonis | 57.6 ± 1.5 | 2 | K0IV + K2V | 6.49/7.57 | has 2 known planets[22] |
Gliese 819 | 57.6 ± 1.2 | 3 | KV | ||
Delta Leonis «Zosma» | 57.7 ± 0.9 | 1 | A4V | 2.56 | [23][24] |
Gliese 340 | 57.7 ± 1.1 | 2 | KV | ||
WISE 0138-0322 | 57.7 | 1 | T2 | ||
WISE 0611-0410 | 57.7 | 1 | T0 | ||
WISE 1122+2550 | 57.7 | 1 | T6 | ||
HR 7644 | 57.8 ± 0.8 | 1 | GV | has 1 known planet | |
Gliese 626 | 57.8 ± 1.4 | 1 | KV | ||
Iota Pavonis | 57.9 ± 0.7 | 1 | GV | ||
HD 35650 | 57.9 ± 1 | 1 | KV | ||
HD 82443 | 57.9 ± 0.9 | 2 | KV | ||
HR 5356 | 58.0 ± 1 | 2 | FV | ||
HR 4525 | 58.0 ± 0.8 | 1 | GV | ||
Gliese 365 | 58.0 ± 1.2 | 1 | KV | ||
HR 2401 | 58.2 ± 0.6 | 2 | FV | ||
V833 Tauri | 58.2 ± 1.3 | 3 | KV | ||
Alpha Comae Berenices «Diadem» | 58.3 ± 1.5 | 3 | F5V + F5V | 4.85/5.53 | [25][26] |
Eta Coronae Borealis | 58.3 ± 0.8 | 3 | G1V + G3V + L8 | 5.02 | [27][28] |
Gamma Coronae Australis | 58.4 ± 2.1 | 2 | F8V + F8V | 4.20 | |
WISE 0206+2640 | 58.4 | 1 | L9 pec | ||
Tau⁶ Eridani | 58.5 ± 0.7 | 1 | F5V | 4.20 | [29] |
HD 130948 | 58.5 ± 0.9 | 3 | G1V | 5.99 | [30] |
Gliese 1079 | 58.5 ± 0.8 | 1 | KV | ||
Gliese 787 | 58.5 ± 1.4 | 1 | KV | ||
Gliese 418 | 58.5 ± 1.4 | 1 | KV | ||
Iota Centauri «Alhakim» | 58.6 ± 0.8 | 1 | A2V | 2.73 | [31] |
Gliese 2037 | 58.6 ± 1 | 1 | KV | ||
Gliese 3317 | 58.7 ± 0.8 | 1 | KV | ||
Gliese 18 | 58.7 ± 1.2 | 1 | KV | ||
WISE 2213+0911 | 58.7 | 1 | T7 | ||
HR 4989 | 58.8 ± 0.7 | 2 | FIV | ||
HR 3079 | 58.8 ± 0.6 | 2 | FV | ||
Delta Geminorum «Wasat» | 58.8 ± 0.9 | 3 | F0IV | 3.53 | [31][32] |
Gliese 1240 | 58.8 ± 1 | 1 | KV | ||
Rho Geminorum | 58.9 ± 0.3 | 3 | F1V + M5 + K2.5V | 4.25/12.5/7.74 | [4][33] |
HD 154345 | 58.9 ± 0.6 | 1 | G8V | 6.74 | has 1 known planet[34] |
HD 40887 | 58.9 ± 1.9 | 3 | KV | ||
Gliese 830 | 58.9 ± 1.5 | 1 | KV | ||
HD 87883 | 58.9 ± 1 | 1 | K0V | 7.56 | has 1 known planet[35] |
HD 154088 | 59.0 ± 0.9 | 1 | K0V | 6.7258 | has 1 known planet[36] |
70 Virginis | 59.1 ± 0.8 | 1 | G2.5Va | 5.00 | has 1 known planet[37] |
HR 2208 | 59.1 ± 1 | 1 | GV | ||
Chi Cancri | 59.2 ± 1 | 1 | F6V | 5.14 | [31][38] |
14 Herculis | 59.2 ± 0.6 | 1 | K0V | 6.67 | has 2 known planets[39] |
Gliese 4008 | 59.3 ± 0.9 | 1 | KV | ||
Eta Corvi «Avis Satyra» | 59.4 ± 0.7 | 1 | F2V | 4.31 | [40] |
Pi Mensae | 59.4 ± 0.5 | 1 | G1IV | 5.67 | has 1 known planet[41] |
HIP 38939 | 59.4 ± 1.3 | 1 | KV | ||
Epsilon Reticuli | 59.5 ± 0.5 | 2 | K2IV + D | 4.44/12.5 | has 1 known planet[31][42][43] |
Beta Arietis «Sheratan» | 59.6 ± 0.8 | 2 | A5V | 2.655 | [44][45] |
Psi Velorum | 59.7 ± 1 | 2 | F3IV + F0V | 3.60 | |
Gliese 1106 | 59.7 +5.1 -4.4 | 1 | KV | ||
WISE 2239+1617 | 59.7 | 1 | T | ||
Gliese 1120 | 59.8 +3.7 -3.3 | 2 | KV | ||
Gliese 3488 | 59.8 ± 1.4 | 1 | KV | ||
LQ Hydrae | 59.8 ± 1.1 | 1 | KV | ||
Gliese 131 | 59.9 ± 1.5 | 1 | KV | ||
HR 8314 | 60.0 ± 0.9 | 2 | GV | ||
WISE 1436-1814 | 60.0 | 1 | T8 pec |
See also
References
- ↑ LTT 3283 -- High proper-motion Star, database entry, SIMBAD. Accessed on line January 20, 2011.
- ↑ "Iota Horologii". SolStation. Retrieved May 28, 2008.
- ↑ Zechmeister, M.; et al. (2013). "The planet search programme at the ESO CES and HARPS. IV. The search for Jupiter analogues around solar-like stars". Astronomy and Astrophysics. 552: A78. arXiv:1211.7263. Bibcode:2013A&A...552A..78Z. doi:10.1051/0004-6361/201116551.
- 1 2 Gray, R.O.; et al. (July 2006), "Contributions to the Nearby Stars (NStars) Project: spectroscopy of stars earlier than M0 within 40 pc-The Southern Sample", The Astronomical Journal, 132 (1): 161–170, arXiv:astro-ph/0603770, Bibcode:2006AJ....132..161G, doi:10.1086/504637.
- ↑ Mermilliod, J.-C. (1986), "Compilation of Eggen's UBV data, transformed to UBV (unpublished)", Catalogue of Eggen's UBV data, SIMBAD, Bibcode:1986EgUBV........0M.
- ↑ "HD 81997 -- Variable Star". SIMBAD Astronomical Database. Retrieved 2006-11-05.
- ↑ Marmier, M.; et al. (2013). "The CORALIE survey for southern extrasolar planets XVII. New and updated long period and massive planets". Astronomy and Astrophysics. 551. A90. arXiv:1211.6444. Bibcode:2013A&A...551A..90M. doi:10.1051/0004-6361/201219639.
- ↑ Decin, G.; et al. (November 2003), "Age Dependence of the Vega Phenomenon: Observations", The Astrophysical Journal, 598 (1): 636–644, arXiv:astro-ph/0308294, Bibcode:2003ApJ...598..636D, doi:10.1086/378800
- ↑ SIMBAD, LTT 6908 (accessed 27 December 2012)
- ↑ Maldonado, J.; et al. (May 2012), "Metallicity of solar-type stars with debris discs and planets", Astronomy and Astrophysics, 541, arXiv:1202.5884, Bibcode:2012A&A...541A..40M, doi:10.1051/0004-6361/201218800.
- ↑ Gerard T. van Belle & Kaspar von Braun (2009). "Directly Determined Linear Radii and Effective Temperatures of Exoplanet Host Stars" (abstract). The Astrophysical Journal. 694 (2): 1085–1098. arXiv:0901.1206. Bibcode:2009ApJ...694.1085V. doi:10.1088/0004-637X/694/2/1085.(web Preprint)
- ↑ Reffert, S.; Quirrenbach, A. (2011). "Mass constraints on substellar companion candidates from the re-reduced Hipparcos intermediate astrometric data: nine confirmed planets and two confirmed brown dwarfs". Astronomy & Astrophysics. 527. id.A140. arXiv:1101.2227. Bibcode:2011A&A...527A.140R. doi:10.1051/0004-6361/201015861.
- ↑ Torres, C. A. O.; et al. (December 2006). "Search for associations containing young stars (SACY). I. Sample and searching method". Astronomy and Astrophysics. 460 (3): 695–708. arXiv:astro-ph/0609258. Bibcode:2006A&A...460..695T. doi:10.1051/0004-6361:20065602.
- ↑ "Chi Eridani". SIMBAD Astronomical Database. Centre de Données astronomiques de Strasbourg. Retrieved 12 July 2015.
- ↑ LTT 6256 -- High proper-motion Star, database entry, SIMBAD. Accessed on line February 4, 2011.
- ↑ "ksi Gem -- Variable Star", SIMBAD, Centre de Données astronomiques de Strasbourg, retrieved 2012-01-20
- ↑ Wielen, R.; et al. (1999), Sixth Catalogue of Fundamental Stars (FK6). Part I. Basic fundamental stars with direct solutions (35), Astronomisches Rechen-Institut Heidelberg, Bibcode:1999VeARI..35....1W
- ↑ SIMBAD, 58 Ophiuchi (accessed 30 December 2012)
- ↑ Kuzuhara, M.; et al. (2013). "Direct Imaging of a Cold Jovian Exoplanet in Orbit around the Sun-like Star GJ 504". The Astrophysical Journal. 774 (1). 11. arXiv:1307.2886. Bibcode:2013ApJ...774...11K. doi:10.1088/0004-637X/774/1/11.
- ↑ Naef, D.; et al. (2001). "The CORALIE survey for southern extrasolar planets V. 3 new extrasolar planets". Astronomy and Astrophysics. 375 (1): 205–218. arXiv:astro-ph/0106255. Bibcode:2001A&A...375..205N. doi:10.1051/0004-6361:20010841.
- ↑ Crepp, Justin R.; et al. (2012). "The Dynamical Mass and Three-Dimensional Orbit of HR7672B: A Benchmark Brown Dwarf with High Eccentricity". arXiv:1112.1725. Bibcode:2012ApJ...751...97C. doi:10.1088/0004-637X/751/2/97.
- ↑ Stefano Meschiari; Gregory Laughlin; Steven S. Vogt; R. Paul Butler; Eugenio J. Rivera; Nader Haghighipour; Peter Jalowiczor (2011). "The Lick-Carnegie Survey: Four New Exoplanet Candidates". The Astrophysical Journal. 727 (2). article id. 117. arXiv:1011.4068. Bibcode:2011ApJ...727..117M. doi:10.1088/0004-637X/727/2/117.
- ↑ Cowley, A.; et al. (April 1969), "A study of the bright A stars. I. A catalogue of spectral classifications", Astronomical Journal, 74: 375–406, Bibcode:1969AJ.....74..375C, doi:10.1086/110819
- ↑ Wielen, R.; et al. (1999), Sixth Catalogue of Fundamental Stars (FK6). Part I. Basic fundamental stars with direct solutions (35), Astronomisches Rechen-Institut Heidelberg, Bibcode:1999VeARI..35....1W
- ↑ Diadem, Jim Kaler, Stars. Accessed on line September 3, 2008.
- ↑ Entry 13100+1732, Sixth Catalog of Orbits of Visual Binary Stars, United States Naval Observatory. Accessed on line September 3, 2008.
- ↑ Edwards, T. W. (1976). "MK classification for visual binary components". Bibcode:1976AJ.....81..245E. doi:10.1086/111879.
- ↑ Kirkpatrick, J. Davy; Dahn, Conard C.; Monet, David G.; Reid, I. Neill; et al. (2001). "Brown Dwarf Companions to G-Type Stars. I. Gliese 417B and Gliese 584C.". arXiv:astro-ph/0103218. Bibcode:2001AJ....121.3235K. doi:10.1086/321085.
- ↑ SIMBAD, LHS 1591 (accessed 11 September 2012)
- ↑ Chen, Y. Q.; Nissen, P. E.; Zhao, G.; Zhang, H. W.; Benoni, T. (February 2000). "Chemical composition of 90 F and G disk dwarfs". Astronomy and Astrophysics Supplement. 141: 491–506. arXiv:astro-ph/9912342. Bibcode:2000A&AS..141..491C. doi:10.1051/aas:2000124.
- 1 2 3 4 Johnson, H. L.; et al. (1966). "UBVRIJKL photometry of the bright stars". Communications of the Lunar and Planetary Laboratory. 4 (99). Bibcode:1966CoLPL...4...99J.
- ↑ "Delta Geminorum (Wasat)", SIMBAD, Centre de Données astronomiques de Strasbourg, retrieved 2011-06-03
- ↑ Tokovinin, A. A. (1997). "MSC - a catalogue of physical multiple stars". Astronomy and Astrophysics Supplement Series. 124 (1): 75–84. Bibcode:1997A&AS..124...75T. doi:10.1051/aas:1997181. ISSN 0365-0138.
- ↑ Wright, J. T.; et al. (2008). "The Jupiter Twin HD 154345b". The Astrophysical Journal Letters. 683 (1): L63–L66. arXiv:0802.1731. Bibcode:2008ApJ...683L..63W. doi:10.1086/587461.
- ↑ Fischer, Debra; et al. (2009). "Five planets and an independent confirmation of HD 196885 Ab from Lick Observatory". The Astrophysical Journal. 703 (2): 1545–1556. arXiv:0908.1596. Bibcode:2009ApJ...703.1545F. doi:10.1088/0004-637X/703/2/1545.
- ↑ Mayor, M.; et al. (2011). "The HARPS search for southern extra-solar planets XXXIV. Occurrence, mass distribution and orbital properties of super-Earths and Neptune-mass planets". arXiv:1109.2497. Bibcode:2011arXiv1109.2497M.
- ↑ Butler, R. P.; et al. (2006). "Catalog of Nearby Exoplanets". The Astrophysical Journal. 646 (1): 505–522. arXiv:astro-ph/0607493. Bibcode:2006ApJ...646..505B. doi:10.1086/504701.
- ↑ Boyajian, Tabetha S.; et al. (July 2013), "Stellar Diameters and Temperatures. III. Main-sequence A, F, G, and K Stars: Additional High-precision Measurements and Empirical Relations", The Astrophysical Journal, 771 (1): 40, arXiv:1306.2974, Bibcode:2013ApJ...771...40B, doi:10.1088/0004-637X/771/1/40.
- ↑ Wittenmyer, Robert A.; et al. (January 2007). "Long-Period Objects in the Extrasolar Planetary Systems 47 Ursae Majoris and 14 Herculis". The Astrophysical Journal. 654 (1): 625–632. arXiv:astro-ph/0609117. Bibcode:2007ApJ...654..625W. doi:10.1086/509110.
- ↑ "SIMBAD query result: NSV 5690 -- Variable Star". Centre de données astronomiques de Strasbourg. Retrieved 2008-11-19.
- ↑ Jones; et al. (2002). "A probable planetary companion to HD 39091 from Anglo-Australian Planet Search". Monthly Notices of the Royal Astronomical Society. 333 (4): 871–875. arXiv:astro-ph/0112084. Bibcode:2002MNRAS.333..871J. doi:10.1046/j.1365-8711.2002.05459.x. (web Preprint)
- ↑ Chauvin, G.; Lagrange, A.-M.; Udry, S.; Mayor, M. (2007), "Characterization of the long-period companions of the exoplanet host stars: HD 196885, HD 1237 and HD 27442", Astronomy and Astrophysics, 475 (2): 723–727, arXiv:0710.5918, Bibcode:2007A&A...475..723C, doi:10.1051/0004-6361:20067046.
- ↑ Butler, R. P.; et al. (2001). "Two New Planets from the Anglo-Australian Planet Search". The Astrophysical Journal. 555 (1): 410–417. Bibcode:2001ApJ...555..410B. doi:10.1086/321467.
- ↑ Trilling, D. E.; et al. (April 2007), "Debris disks in main-sequence binary systems", The Astrophysical Journal, 658 (2): 1264–1288, arXiv:astro-ph/0612029, Bibcode:2007ApJ...658.1289T, doi:10.1086/511668
- ↑ Gutierrez-Moreno, Adelina; et al. (1966). "A System of photometric standards". 1. Publicaciones Universidad de Chile, Department de Astronomy: 1–17. Bibcode:1966PDAUC...1....1G.
This article is issued from Wikipedia - version of the 10/2/2016. The text is available under the Creative Commons Attribution/Share Alike but additional terms may apply for the media files.