List of star systems within 30–35 light-years
This is a list of star systems within 30-35 light years of Earth.
Star system | Median distance (ly) | Stars in system | Spectral type | Apparent magnitude (V) | Comments and references |
---|---|---|---|---|---|
Gamma Pavonis | 30.1 ± 0.2 | 1 | F9V | 4.22 | [1][2] |
HD 102365 | 30.1 ± 0.2 | 2 | G2V + M4V | 4.88 + 15 | has 1 known planet[2][3][4][5] |
2MASS 1750-00 | 30.1 ± 0.7 | 1 | L | ||
Gliese 176 | 30.7 ± 0.7 | 1 | M2V | 9.95 | has 1 known planet[6] |
2MASS J11592743-5247188 | 30.9 ± 0.04 | 1 | M9V | [7]Brown Dwarf | |
2MASS 0034+0523 | 30.9 +2.4 -2.1 | 1 | T | ||
LHS 194 | 31.0 ± 0.8 | 1 | DQ | ||
61 Ursae Majoris | 31.1 ± 0.2 | 1 | G8V | 5.35 | [8][9] |
HR 4458 | 31.1 ± 0.2 | 2 | K0V + DC8 | 5.97 + 15 | [2][10][11] |
BPS CS 22898-0066 | 31.2 ± 7.1 | 1 | MV | ||
2MASS J11553952-3727350 | 31.2 ± 1.5 | 1 | L | ||
TYC 3251-1875-1 | 31.5 ± 5.9 | 1 | MV | ||
WISE J140533.32+835030.5 | 31.6 ± 5.5 | 1 | L | ||
CFBD J0059-01 | 31.6 ± 0.6 | 1 | T | ||
LHS 145 | 31.7 ± 0.3 | 1 | DA | ||
Gliese 638 | 31.9 ± 0.3 | 1 | K7V | 8.11 | [9] |
12 Ophiuchi | 31.9 ± 0.3 | 1 | K2V | 5.77 | [12] |
LP 655-48 | 32.0 ± 3.6 | 1 | MV | ||
WISE 0811-8051 | 32.0 | 1 | T9.5 | ||
2MASS J2139+0220 | 32.1 ± 0.6 | 1 | T | ||
AU Microscopii | 32.3 ± 0.3 | 3 | M1Ve | 8.73 | [13] |
HR 511 | 32.5 ± 0.2 | 1 | K0V | 5.63 | [10][14] |
WISE 1614+1739 | 32.6 | 1 | T9 | 19.08 | |
ULAS 1335+11 | 32.6 ± 0.5 | 1 | T | ||
Gliese 22 | 32.8 ± 0.7 | 3 | M2.5Ve + M3V | 10.29 + 12.19 + 13.2 | |
WISE 1150+6302 | 32.9 | 1 | T8 | 17.72 | |
WISE 1318-1758 | 32.9 | 1 | T9 | ||
WISE 1217+1626 | 32.9 +6.4 -4.6 | 2 | T9 | 17.83 | |
HR 5256 | 33.0 ± 0.2 | 1 | K3V | 6.520 | [15][16] |
Alpha Mensae | 33.1 ± 0.2 | 1 | G7V | 5.09 | [2][10] |
Gliese 453 | 33.2 ± 0.3 | 1 | KV | ||
Gliese 436 | 33.4 ± 0.8 | 1 | M2.5V | 10.67 | has 1 known planet[17] |
Gliese 127.1 | 33.4 ± 0.6 | 2 | DA3.0 | [18] | |
Gliese 3182 | 33.6 ± 1.3 | 1 | DAZ9 | [19] | |
Pollux | 33.7 ± 0.3 | 1 | K0III | 1.14 | has 1 known planet[20][21][22] |
Gliese 649 | 33.7 ± 0.5 | 1 | M1.5V | 9.62 | has 1 known planet[23] |
Gliese 339.1 | 33.7 ± 0.6 | 1 | DC7P | ||
2MASS 0559-1404 | 33.76 ± 0.35 | 1 | T | ||
HD 17925 | 33.9 ± 0.3 | 1 | K1V | 6.04 | [10][24] |
2MASS 1237+6526 | 33.9 ± 1.8 | 1 | T6.5V | 16.15 | [25] |
WISE 1322-2340 | 33.9 | 1 | T8 | 17.01 | |
WISE J2030+0749 | 34.2 ± 8.5 | 1 | T1.5 | [26] | |
Iota Persei | 34.4 ± 0.3 | 1 | G0V | 4.05 | |
2MASS 1047+2124 | 34.4 ± 1.4 | 1 | T | ||
2MASS J00501994−3322402 | 34.5 ± 0.9 | 1 | T | ||
WD 0821-669 | 34.7 ± 0.4 | 1 | DA9 | ||
2MASS 2228-4310 | 34.7 +2.8 -2.4 | 1 | T | ||
Zeta Herculis | 34.8 ± 0.2 | 2 | F9IV + G7V | 2.81 | [27][28] |
Gliese 617 | 34.8 ± 0.4 | 2 | MV | ||
2MASS J08251968+2115521 | 34.8 ± 0.4 | 1 | L | ||
2MASS 0243-2453 | 34.8 ± 1.4 | 1 | T6 | [25] | |
HD 160346 | 34.9 ± 0.5 | 1 | KV | ||
WISE 0734-7157 | 34.9 | 1 | Y0 | 20.41 | [29] |
See also
References
- ↑ Jehin, E.; et al. (January 1999), "Abundance correlations in mildly metal-poor stars", Astronomy and Astrophysics, 341: 241–255, arXiv:astro-ph/9809405, Bibcode:1999A&A...341..241J
- 1 2 3 4 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
- ↑ Poveda, A.; et al. (April 1994), "Statistical studies of visual double and multiple stars. II. A catalogue of nearby wide binary and multiple systems", Revista Mexicana de Astronomía y Astrofísica, 28 (1): 43–89, Bibcode:1994RMxAA..28...43P
- ↑ Feinstein, A. (1966), "Photoelectric observations of Southern late-type stars", The Information Bulletin for the Southern Hemisphere, 8: 30, Bibcode:1966IBSH....8...30F
- ↑ Raghavan, Deepak; et al. (September 2010), "A Survey of Stellar Families: Multiplicity of Solar-type Stars", The Astrophysical Journal Supplement, 190 (1): 1–42, arXiv:1007.0414, Bibcode:2010ApJS..190....1R, doi:10.1088/0067-0049/190/1/1 For the adopted physical separation, see Table 11 in the appendix.
- ↑ Forveille, T.; et al. (January 2009). "The HARPS search for southern extra-solar planets. XIV. Gl 176b, a super-Earth rather than a Neptune, and at a different period". Astronomy and Astrophysics. 493 (2): 645–650. arXiv:0809.0750. Bibcode:2009A&A...493..645F. doi:10.1051/0004-6361:200810557.
- ↑ http://simbad.u-strasbg.fr/simbad/sim-id?Ident=2MASS+J11592743-5247188
- ↑ Cornide, M.; Rego, M. (October 1984). "Iron abundances in G dwarfs". Astrophysics and Space Science. 105 (1): 55–65. Bibcode:1984Ap&SS.105...55C. doi:10.1007/BF00651207.
- 1 2 Wilson, O. C. (November 1962). "Relationship Between Colors and Spectra of Late Main-Sequence Stars". Astrophysical Journal. 136: 793. Bibcode:1962ApJ...136..793W. doi:10.1086/147437.
- 1 2 3 4 Mermilliod, J.-C. (1986). "Compilation of Eggen's UBV data, transformed to UBV (unpublished)". Catalogue of Eggen's UBV data. Bibcode:1986EgUBV........0M.
- ↑ Holberg, J. B.; et al. (November 2013). "Where are all the Sirius-like binary systems?". Monthly Notices of the Royal Astronomical Society. 435 (3): 2077–2091. arXiv:1307.8047. Bibcode:2013MNRAS.435.2077H. doi:10.1093/mnras/stt1433.
- ↑ Fuhrmann, Klaus (February 2008), "Nearby stars of the Galactic disc and halo - IV", Monthly Notices of the Royal Astronomical Society, 384 (1): 173–224, Bibcode:2008MNRAS.384..173F, doi:10.1111/j.1365-2966.2007.12671.x
- ↑ 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
- ↑ White, Russel J.; Gabor, Jared M.; Hillenbrand, Lynne A. (June 2007), "High-Dispersion Optical Spectra of Nearby Stars Younger Than the Sun", The Astronomical Journal, 133 (6): 2524–2536, arXiv:0706.0542, Bibcode:2007AJ....133.2524W, doi:10.1086/514336.
- ↑ Oja, T. (August 1991). "UBV photometry of stars whose positions are accurately known. VI". Astronomy and Astrophysics Supplement Series. 89 (2): 415–419. Bibcode:1991A&AS...89..415O.
- ↑ Marrese, P. M.; Boschi, F.; Munari, U. (August 2003). "High resolution spectroscopy over lambda lambda 8500-8750 Å for GAIA. IV. Extending the cool MK stars sample". Astronomy and Astrophysics. 406: 995–999. Bibcode:2003A&A...406..995M. doi:10.1051/0004-6361:20030647.
- ↑ Butler, R. Paul; et al. (2004). "A Neptune-Mass Planet Orbiting the Nearby M Dwarf GJ 436". The Astrophysical Journal. 617 (1): 580–588. arXiv:astro-ph/0408587. Bibcode:2004ApJ...617..580B. doi:10.1086/425173. Retrieved 2009-12-26.
- ↑ http://simbad.u-strasbg.fr/simbad/sim-id?Ident=LB+3303
- ↑ http://simbad.u-strasbg.fr/simbad/sim-id?Ident=Gliese++3182
- ↑ Ducati, J. R. (2002). "VizieR Online Data Catalog: Catalogue of Stellar Photometry in Johnson's 11-color system". CDS/ADC Collection of Electronic Catalogues. 2237: 0. Bibcode:2002yCat.2237....0D.
- ↑ Morgan, W. W.; Keenan, P. C. (1973), "Spectral Classification", Annual Review of Astronomy and Astrophysics, 11: 29, Bibcode:1973ARA&A..11...29M, doi:10.1146/annurev.aa.11.090173.000333
- ↑ Hatzes, A. P.; et al. (2006), "Confirmation of the planet hypothesis for the long-period radial velocity variations of β Geminorum", Astronomy and Astrophysics, 457: 335–341, arXiv:astro-ph/0606517, Bibcode:2006A&A...457..335H, doi:10.1051/0004-6361:20065445
- ↑ Johnson, John Asher; et al. (2010). "The California Planet Survey II. A Saturn-Mass Planet Orbiting the M Dwarf Gl649". The Publications of the Astronomical Society of the Pacific. 122 (888): 149–155. arXiv:0912.2730. Bibcode:2010PASP..122..149J. doi:10.1086/651007.
- ↑ Montes, D.; et al. (2001), "Late-type members of young stellar kinematic groups - I. Single stars", Monthly Notices of the Royal Astronomical Society, 328 (1): 45–63, arXiv:astro-ph/0106537, Bibcode:2001MNRAS.328...45M, doi:10.1046/j.1365-8711.2001.04781.x.
- ↑ Bihain, Gabriel; Scholz, Ralf-Dieter; Storm, Jesper; Schnurr, Olivier (2013). "An overlooked brown dwarf neighbour (T7.5 at d~5pc) of the Sun and two additional T dwarfs at about 10pc". arXiv:1307.2722.
- ↑ Edwards, T. W. (April 1976), "MK classification for visual binary components", Astronomical Journal, 81: 245–249, Bibcode:1976AJ.....81..245E, doi:10.1086/111879
- ↑ 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
- ↑ Kirkpatrick, J. D.; Gelino, C. R.; Cushing, M. C.; Mace, G. N.; Griffith, R. L.; Skrutskie, M. F.; Marsh, K. A.; Wright, E. L.; Eisenhardt, P. R.; McLean, I. S.; Mainzer, A. K.; Burgasser, A. J.; Tinney, C. G.; Parker, S.; Salter, G. (2012). "Further Defining Spectral Type "Y" and Exploring the Low-mass End of the Field Brown Dwarf Mass Function". The Astrophysical Journal. 753 (2): 156. arXiv:1205.2122. Bibcode:2012ApJ...753..156K. doi:10.1088/0004-637X/753/2/156.
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