This is a list of star systems within 35-40 light years of Earth.
Star system | Median distance (ly) | Stars in system | Spectral type | Apparent magnitude (V) | Comments and references |
---|---|---|---|---|---|
AT Microscopii | 35 ± 1 | 2 | M4Ve + M4.5Ve | 11.0/11.1 | |
TVLM513-46546 | 35.1 ± 0.09 | 1 | M8.5V | ||
Gliese 203 | 35.11 ± 0.92 | 1 | M3.5Ve | ||
Gliese 3820 | 35.12 ± 0.32 | 1 | M4.5V | ||
SCR J0838-5855 | 35.16 ± 0.22 | 2 | M6.0 | [1] | |
HR 9038 | 35.2 ± 0.2 | 3 | K3V + M2 | 6.40/11.4 | [2][3][4] |
Gliese 488 | 35.2 ± 0.4 | 1 | MV | ||
Delta Trianguli | 35.4 ± 0.3 | 2 | G0V + K | 4.865 | [5][6] |
L 34-26 | 35.52 ± 0.06 | 1 | M3 | 11.28 | has one known planet, closest directly imaged exoplanet (as of July 2021)[7] |
GJ 4063 | 35.5292 | 1 | M4V | 11.75 | |
Beta Virginis «Zavijava» | 35.6 ± 0.3 | 1 | F9V | 3.604 | [8][9] |
Gliese 86 | 35.6 ± 0.2 | 2 | K1V | has 1 known planet[3][10] | |
SCR J1214-2345 | 35.69 ± 0.60 | 1 | M4.5 + T1 | [11] | |
G 239-25 | 35.77 ± 0.12 | 1 | M3V | ||
HD 160346 | 35.88 ± 0.27 | 2 | K3V | ||
2MASS J19513587-3510375 | 35.88 ± 6.52 | 1 | M4 | ||
WISE 2313-0837 | 35.9 | 1 | T8 | ||
Gliese 438 | 35.94 ± 0.19 | 1 | MV | ||
L 369-44 | 36.168 | 2 | M5+M | 12.67 | |
2MASS J16452211-1319516 | 36.19 ± 0.33 | 1 | L1.5 | ||
Denebola | 36.2 ± 0.4 | 1 | A3V | 2.113 | [12][13] |
HR 6806 | 36.2 ± 0.2 | 1 | K2V | 6.40 | [2][3] |
54 Piscium | 36.2 ± 0.3 | 2 | K0V + T7.5V | 5.88 | has 1 known planet[14][15][16] |
HIP 57050 | 36.2 ± 1.1 | 1 | MV | has 1 known planet [17] | |
Gamma Serpentis | 36.3 ± 0.3 | 1 | F6V | 3.85 | [18] |
HD 74576 | 36.3 ± 0.2 | 1 | KV | ||
HD 85512 | 36.4 ± 0.3 | 1 | K5V | 7.66 | has 1 known planet[19] |
Gliese 325 | 36.4 +1.5 −1.4 | 2 | KV | ||
11 Leonis Minoris | 36.5 ± 0.3 | 2 | G8V + M5V | 4.80/12.50 | [20] |
WISE 0325+0831 | 36.5 | 1 | T7 | ||
Theta Persei | 36.6 ± 0.3 | 2 | F7V + M1V | 4.12/10 | |
HD 115404 | 36.6 ± 0.4 | 2 | K2V + M1V | 6.61 | |
Arcturus | 36.7 ± 0.3 | 1 | K0III | -0.05 | [3][21] |
ADS 48 | 36.7 ± 0.6 | 3 | KV | 8.83/9.00/9.97 | [22][23][24] |
G 107-69/70 | 36.76 ± 0.01 | 4 | M4.5+DA+DA | 13.2 | |
WISE 0038+2768 | 36.9 | 1 | T9 | ||
Eta Boötis «Muphrid» | 37.0 ± 0.3 | 2 | G0IV | 2.680 | [5][25] |
Gliese 208 | 37.1 ± 0.6 | 1 | M0.0 Ve | 8.9 | |
Gliese 902 | 37.2 ± 0.3 | 1 | KV | ||
WISE 0627-1114 | 37.2 | 1 | T6 | ||
WISE 1959-3338 | 37.2 | 1 | T8 | ||
Gliese 169 | 37.4 ± 0.5 | 1 | KV | ||
WISE 0623-0456 | 37.5 | 1 | T8 | ||
WISE 2325-4105 | 37.5 | 1 | T9pec | ||
HR 5553 | 37.6 ± 0.4 | 2 | K0V | 6.00 | [2][26] |
WISE 2340-0745 | 37.8 | 1 | T7 | ||
Gliese 3417 | 37.88 ± 0.96 | 1 | M4.5V | ||
Zeta Doradus | 38.0 ± 0.2 | 2 | F7V + K7V | 4.82/9.02 | [27] |
SCR J0640-0552 | 38.04 ± 1.27 | 1 | M2 | [1] | |
SSSPM J0829-1309 | 38.128 ± 0.077 | 1 | L2 | [28] | |
Iota Pegasi | 38.3 ± 0.3 | 2 | F5V + G8V | 3.84/6.68 | [29][30] |
Lambda Serpentis | 38.3 ± 0.4 | 1 | G0V | 4.43 | [31][32] |
Gliese 773.6 | 38.5 ± 5.8 | 1 | KV | ||
Delta Capricorni «Deneb Algedi» | 38.6 ± 0.4 | 2 | A7mIII | 2.81 | [33] |
HD 125072 | 38.6 ± 0.4 | 1 | K3IV | 6.637 | [3][5] |
L 43-72 | 38.66 ± 0.71 | 2 | M4.5 | [1] | |
Gamma Virginis «Porrima» | 38.7 ± 0.4 | 2 | F0V + F0V | 2.74 | [34] |
L 449-1 | 38.7 ± 0.6 | 2 | MV | ||
WISE 0759-4904 | 38.8 | 1 | T8 | ||
Gliese 414 B | 38.70[35] | 2 | M2V[36] | 9.98[lower-alpha 1] | |
Gliese 414 A | 38.76[35] | K7V[36] | 9.24[lower-alpha 2] | Has two known exoplanets (b and c) | |
WISE 0751-7634 | 39.1 | 1 | T9 | ||
G 180-060 | 39.20 ± 1.19 | 1 | M6V | ||
Zeta Reticuli | 39.4 ± 0.3 | 2 | G3V + G2V | 5.22 | [37][38] |
Zeta Trianguli Australis | 39.5 ± 0.3 | 2 | F9V | 4.90 | [2][3] |
85 Pegasi | 39.5 ± 0.4 | 3 | G5Vb + K7V | 5.75/8.89 | |
Gliese 798 | 39.5 ± 0.6 | 1 | KV | ||
Gliese 180 | 39.5 +1.2 −1.1 | 1 | MV | 10.894 | has 2 known planets |
TRAPPIST-1 | 39.5 ± 1.3 | 1 | M8.2V | 18.80 | has 7 known planets |
WISE 1653+4444 | 39.5 | 1 | T8 | ||
Gliese 3304 | 39.53 ± 1.43 | 1 | M4.5V | ||
HR 3384 | 39.7 ± 0.3 | 1 | G9V | 6.38 | [3][39] |
V538 Aurigae | 39.9 ± 0.4 | 1 | K1V | 6.25 | [2][40] |
See also
Notelist
- ↑ Calculated using an absolute magnitude of 9.6[36] in the equation: Mapp = Mabs-5+5log(distance (light-years)/3.26
- ↑ Calculated using an absolute magnitude of 8.864[36] in the equation: Mapp = Mabs-5+5log(distance (light-years)/3.26
References
- 1 2 3 Winters, Jennifer G.; Sevrinsky, R. Andrew; Jao, Wei-Chun; Henry, Todd J.; Riedel, Adric R.; Subasavage, John P.; Lurie, John C.; Ianna, Philip A.; Finch, Charlie T. (2016). "The Solar Neighborhood XXXVIII. Results from the CTIO/SMARTS 0.9m: Trigonometric Parallaxes for 151 Nearby M Dwarf Systems". The Astronomical Journal. 153 (1): 14. arXiv:1610.07552. Bibcode:2017AJ....153...14W. doi:10.3847/1538-3881/153/1/14. ISSN 1538-3881. S2CID 6136017.
- 1 2 3 4 5 Mermilliod, J.-C. (1986), "Compilation of Eggen's UBV data, transformed to UBV (unpublished)", Catalogue of Eggen's UBV Data. SIMBAD: 0, Bibcode:1986EgUBV........0M.
- 1 2 3 4 5 6 7 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. S2CID 119476992.
- ↑ Malkov, O. Yu.; et al. (2012), "Dynamical masses of a selected sample of orbital binaries", Astronomy & Astrophysics, 546: 5, Bibcode:2012A&A...546A..69M, doi:10.1051/0004-6361/201219774, A69.
- 1 2 3 Holmberg, J.; Nordström, B.; Andersen, J. (July 2009), "The Geneva-Copenhagen survey of the solar neighbourhood. III. Improved distances, ages, and kinematics", Astronomy and Astrophysics, 501 (3): 941–947, arXiv:0811.3982, Bibcode:2009A&A...501..941H, doi:10.1051/0004-6361/200811191, S2CID 118577511
- ↑ Kim, Jinyoung Serena; et al. (October 2005), "Formation and Evolution of Planetary Systems: Cold Outer Disks Associated with Sun-like Stars", The Astrophysical Journal (Submitted manuscript), 632 (1): 659–669, arXiv:astro-ph/0506434, Bibcode:2005ApJ...632..659K, doi:10.1086/432863, S2CID 7324203
- ↑ Zhang, Zhoujian; Liu, Michael C.; Claytor, Zachary R.; Best, William M. J.; Dupuy, Trent J.; Siverd, Robert J. (2021-07-01). "The Second Discovery from the COCONUTS Program: A Cold Wide-orbit Exoplanet around a Young Field M Dwarf at 10.9 pc". The Astrophysical Journal Letters. 916 (2): L11. arXiv:2107.02805. Bibcode:2021ApJ...916L..11Z. doi:10.3847/2041-8213/ac1123. S2CID 236464073.
- ↑ Gutierrez-Moreno, Adelina; Moreno, Hugo (June 1968), "A photometric investigation of the Scorpio-Centaurus association", Astrophysical Journal Supplement, 15: 459, Bibcode:1968ApJS...15..459G, doi:10.1086/190168
- ↑ Morgan, W. W.; Keenan, P. C. (1973), "Spectral Classification", Annual Review of Astronomy and Astrophysics, 11 (1): 29–50, Bibcode:1973ARA&A..11...29M, doi:10.1146/annurev.aa.11.090173.000333
- ↑ "Extrasolar Planet in Double Star System Discovered from La Silla" (Press release). Garching, Germany: European Southern Observatory. November 24, 1998. Retrieved December 29, 2012.
- ↑ Scholz, Ralf-Dieter (2021). "Gaia EDR3 Confirms a Red Dwarf Companion of the nearby F1 Star HD 105452 and Reveals a New Brown Dwarf Companion of the M4.5 Dwarf SCR J1214-2345". Research Notes of the AAS. 5 (3): 40. arXiv:2103.00144. Bibcode:2021RNAAS...5...40S. doi:10.3847/2515-5172/abea23. S2CID 232075955. 40.
- ↑ Akeson, R. L.; Chen, X.; Ciardi, D.; Crane, M.; Good, J.; Harbut, M.; Jackson, E.; Kane, S. R.; Laity, A. C.; Leifer, S.; Lynn, M.; McElroy, D. L.; Papin, M.; Plavchan, P.; Ramírez, S. V.; Rey, R.; von Braun, K.; Wittman, M.; Abajian, M.; Ali, B.; Beichman, C.; Beekley, A.; Berriman, G. B.; Berukoff, S.; Bryden, G.; Chan, B.; Groom, S.; Lau, C.; Payne, A. N.; et al. (2013). "The NASA Exoplanet Archive: Data and Tools for Exoplanet Research". Publications of the Astronomical Society of the Pacific. 125 (930): 989–999. arXiv:1307.2944. Bibcode:2013PASP..125..989A. doi:10.1086/672273. S2CID 119223465.
- ↑ Gutierrez-Moreno, Adelina; et al. (1966), "A System of photometric standards", Publ. Dept. Astron. Univ. Chile, 1: 1–17, Bibcode:1966PDAUC...1....1G
- ↑ van Belle, Gerard T.; von Braun, Kaspar (2009). "Directly Determined Linear Radii and Effective Temperatures of Exoplanet Host Stars". The Astrophysical Journal (abstract). 694 (2): 1085–1098. arXiv:0901.1206. Bibcode:2009ApJ...694.1085V. doi:10.1088/0004-637X/694/2/1085. S2CID 18370219.
- ↑ Johnson, H. L.; et al. (1966). "UBVRIJKL photometry of the bright stars". Communications of the Lunar and Planetary Laboratory. 4 (99): 99. Bibcode:1966CoLPL...4...99J.
- ↑ Fischer, Debra A.; et al. (2003). "A Sub-Saturn Mass Planet Orbiting HD 3651". The Astrophysical Journal. 590 (2): 1081–1087. Bibcode:2003ApJ...590.1081F. CiteSeerX 10.1.1.582.3920. doi:10.1086/375027. S2CID 18090744.
- ↑ Haghighipour, Nader; Vogt, Steven S.; Paul Butler, R.; Rivera, Eugenio J.; Laughlin, Greg; Meschiari, Stefano; Henry, Gregory W. (20 May 2010). "The Lick-Carnegie Exoplanet Survey: A Saturn-Mass Planet In The Habitable Zone Of The Nearby M4v Star Hip 57050". The Astrophysical Journal. 715 (1): 271–276. arXiv:1004.4608. Bibcode:2010ApJ...715..271H. doi:10.1088/0004-637X/715/1/271. S2CID 12681412.
- ↑ Malagnini, M. L.; Morossi, C. (November 1990), "Accurate absolute luminosities, effective temperatures, radii, masses and surface gravities for a selected sample of field stars", Astronomy and Astrophysics Supplement Series, 85 (3): 1015–1019, Bibcode:1990A&AS...85.1015M
- ↑ Pepe, F.; et al. (2011). "The HARPS search for Earth-like planets in the habitable zone. I. Very low-mass planets around HD 20794, HD 85512, and HD 192310". Astronomy and Astrophysics. 534. A58. arXiv:1108.3447. Bibcode:2011A&A...534A..58P. doi:10.1051/0004-6361/201117055. S2CID 15088852.
- ↑ Malkov, O. Yu.; et al. (2012), "Dynamical masses of a selected sample of orbital binaries", Astronomy & Astrophysics, 546: 5, Bibcode:2012A&A...546A..69M, doi:10.1051/0004-6361/201219774, A69
- ↑ 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.
- ↑ GJ 4 A – Star in double system, database entry, SIMBAD. Accessed 13 July 2013
- ↑ GJ 4 B – Star in double system, database entry, SIMBAD. Accessed 13 July 2013
- ↑ GJ 2 – Star in double system, database entry, SIMBAD. Accessed 13 July 2013.
- ↑ Thévenin, F.; et al. (June 2005), "VLTI/VINCI diameter constraints on the evolutionary status of δ Eri, ξ Hya, η Boo", Astronomy and Astrophysics, 436 (1): 253–262, arXiv:astro-ph/0501420, Bibcode:2005A&A...436..253T, doi:10.1051/0004-6361:20042075, S2CID 118169489
- ↑ Kennedy, Grant M. (February 2015), "Nature or nurture of coplanar Tatooines: the aligned circumbinary Kuiper belt analogue around HD 131511", Monthly Notices of the Royal Astronomical Society: Letters, 447 (1): L75–L79, arXiv:1412.0674, Bibcode:2015MNRAS.447L..75K, doi:10.1093/mnrasl/slu190.
- ↑ van Leeuwen, F. (2007). "Validation of the new Hipparcos reduction". Astronomy and Astrophysics. 474 (2): 653–664. arXiv:0708.1752. Bibcode:2007A&A...474..653V. doi:10.1051/0004-6361:20078357. S2CID 18759600. Archived from the original on 2016-04-02.
- ↑ "SSSPM J0829-1309". sim-id. Retrieved 2019-11-20.
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value (help) - ↑ Konacki, Maciej; et al. (2010). "High-precision Orbital and Physical Parameters of Double-lined Spectroscopic Binary Stars—HD78418, HD123999, HD160922, HD200077, and HD210027". The Astrophysical Journal. 719 (2): 1293–1314. arXiv:0910.4482. Bibcode:2010ApJ...719.1293K. doi:10.1088/0004-637X/719/2/1293. S2CID 119253596.
- ↑ 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
- ↑ "lam Ser -- Spectroscopic binary". SIMBAD. Centre de Données astronomiques de Strasbourg. Retrieved 2010-12-15.
- ↑ Johnson, H. L.; Morgan, W. W. (1953). "Fundamental stellar photometry for standards of spectral type on the revised system of the Yerkes spectral atlas". Astrophysical Journal. 117: 313–352. Bibcode:1953ApJ...117..313J. doi:10.1086/145697. S2CID 18072563.
- ↑ Malkov, O. Yu.; et al. (February 2006), "A catalogue of eclipsing variables", Astronomy and Astrophysics, 446 (2): 785–789, Bibcode:2006A&A...446..785M, doi:10.1051/0004-6361:20053137
- ↑ Cayrel de Strobel, G.; Soubiran, C.; Ralite, N. (July 2001), "Catalogue of [Fe/H] determinations for FGK stars: 2001 edition", Astronomy and Astrophysics, 373: 159–163, arXiv:astro-ph/0106438, Bibcode:2001A&A...373..159C, doi:10.1051/0004-6361:20010525, S2CID 17519049
- 1 2 https://exoplanetarchive.ipac.caltech.edu/overview/GJ%20414
- 1 2 3 4 https://ui.adsabs.harvard.edu/abs/2021AJ....161...86D
- ↑ del Peloso, E. F.; da Silva, L.; Porto de Mello, G. F. (June 2000). "zeta1 and zeta2 Reticuli and the existence of the zeta Herculis group". Astronomy and Astrophysics. 358: 233–241. Bibcode:2000A&A...358..233D.
- ↑ Feinstein, A. (1966), "Photoelectric observations of Southern late-type stars", Informational Bulletin of the Southern Hemisphere, 8: 30, Bibcode:1966IBSH....8...30F
- ↑ 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, S2CID 27151456
- ↑ Montes, D.; et al. (November 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, S2CID 55727428.
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