List of star systems within 40–45 light-years
This is a list of star systems within 40-45 light years of Earth.
Star system | Median distance (ly) | Stars in system | Spectral type | Apparent magnitude (V) | Comments and references |
---|---|---|---|---|---|
Gliese 179 | 40.1 +2.1 -1.9 | 1 | M4V | 11.96 | has 1 known planet[1] |
Beta Trianguli Australis | 40.2 ± 0.3 | 2 | F1V | 2.85 | [2][3] |
Gliese 806 | 40.2 ± 0.9 | 1 | M1.5V | 10.84 | |
Gliese 435 | 40.8 ± 0.5 | 1 | KV | ||
Gliese 4360 | 40.8 ± 0.7 | 2 | MV | ||
WISE J0457-0207 | 40.8 ± 10.1 | 1 | T | ||
WISE 1051-2138 | 40.8 | 1 | T9 | ||
Rho¹ (55) Cancri | 40.9 ± 0.4 | 2 | G8V + M4V | 5.95/13.15 | has 5 known planets[4] |
HD 69830 | 41.0 ± 0.4 | 1 | G8V | 5.98 | has 3 known planets[5][6][7] |
ULAS J0034-00 | 41.0 +2.1 -1.9 | 1 | Y0 | ||
WISE 1542+2230 | 41.1 | 1 | T9.5 | ||
HR 483 | 41.2 ± 0.4 | 2 | G1.5V + MV | 4.95/12.5 | |
Lambda Aurigae «Al Hurr» | 41.2 ± 0.5 | 2 | G1V | 4.71 | [8][9] |
Gliese 142 | 41.2 ± 1.2 | 1 | K3.5V | ||
HD 175224 | 41.2 ± 1.6 | 2 | MV | ||
Innes' star | 41.3 | 1 | MV | has 1 known planet | |
HD 14412 | 41.4 ± 0.4 | 1 | G8V | 6.33 | [10] |
Gliese 349 | 41.4 ± 0.6 | 1 | KV | ||
i (44) Boötis | 41.6 ± 0.3 | 3 | G0V + F | 4.75 | [6][11] |
HD 158633 | 41.7 ± 0.3 | 1 | K0V | 6.43 | [12] |
HD 40307 | 41.8 ± 0.3 | 1 | K2.5V | 7.17 | has 6 known planets[13][14] |
36 Ursae Majoris | 41.9 ± 0.4 | 3 | F8V | 4.82 | [9][15] |
Gliese 3707 | 41.9 ± 1.3 | 1 | MV | ||
HD 147513 | 42.0 ± 0.5 | 2 | G1V | 5.38 | has 1 known planet[2][6][16] |
Gliese 428 | 42.0 ± 1 | 2 | KV | ||
HD 104304 | 42.1 ± 0.4 | 1 | G8IV + M4V | 5.54 | [2][9][17] |
WISE 0857+5604 | 42.1 | 1 | T8 | ||
Capella | 42.2 ± 0.5 | 4 | G1III + K0III | 0.08 | [18][19] |
HD 166348 | 42.3 ± 0.7 | 1 | M0V | 8.38 | [20] |
Gliese 204 | 42.3 ± 0.5 | 1 | KV | ||
HD 172051 | 42.4 ± 0.5 | 1 | G5V | 5.85 | [10] |
Gliese 521 | 42.4 ± 0.9 | 1 | M1V | 10.26 | |
GRW +70 8247 | 42.4 +1.3 -1.2 | 1 | DA:w | 13.2 | [21] |
WISE 2019-1148 | 42.4 | 1 | T8.5 | ||
Gliese 167 | 42.7 ± 0.3 | 1 | K5V | 7.62 | |
WISE 2134-7137 | 42.7 | 1 | T9 | ||
WISE 2359-7335 | 42.7 | 1 | T5.5 | ||
HD 190007 | 42.8 ± 0.6 | 1 | K4V | 7.45 | |
SZ Crateris | 42.9 ± 1 | 2 | KV | 8.1 | |
HD 170657 | 43.1 ± 0.5 | 1 | K2V | 6.82 | [2] |
58 Eridani | 43.4 ± 0.5 | 1 | G1.5V | 5.49 | [2][22] |
Gliese 146 | 43.6 ± 0.5 | 1 | K6.5V | 8.64 | [2][6] |
Gliese 1267 | 43.6 ± 0.8 | 1 | KV | ||
Gliese 556 | 43.8 ± 0.4 | 1 | KV | ||
Gliese 69 | 43.8 ± 0.7 | 1 | K5V | 8.35 | |
Upsilon Andromedae | 43.9 ± 0.4 | 2 | F8V + M4.5V | 4.09 | has 4 known planets |
Theta Ursae Majoris «Alhaud» | 44.0 ± 0.4 | 3 | F6IV | 3.166 | [26][27] |
HD 29697 | 44.0 ± 0.8 | 1 | K3V | 8.00 | [6][28] |
Gliese 868 | 44.2 ± 0.7 | 1 | K5V | 7.93 | |
HD 211415 | 44.4 ± 0.4 | 2 | G0V + MV | 5.33/9.9 | [2][6][29] |
Gliese 528 | 44.4 ± 0.7 | 2 | K4V + dK6 | 7.96/8.35 | |
G 29-38 | 44.4 +2.6 -2.3 | 1 | DAV4.4 | 13.03 | Variable[30] |
WISE 1311+0122 | 44.4 | 1 | T9 | ||
WISE 1952+7240 | 44.4 | 1 | T | ||
HD 154577 | 44.6 ± 0.6 | 1 | K2.5Vk | 7.385 | [2][31] |
Beta Aquilae «Alshain» | 44.7 ± 0.5 | 2 | G8IV | 3.71/11.4 | |
HD 166 | 44.7 ± 0.5 | 2 | G8V | 6.09 | [6][32] |
Gliese 215 | 44.7 ± 0.7 | 1 | MV | ||
WISE 0513+0608 | 44.7 | 1 | T6.5 | ||
WISE 2255-3118 | 44.7 | 1 | T | ||
10 Tauri | 44.8 ± 0.5 | 2 | F8V | 4.28 | [33] |
Gliese 615 | 44.8 ± 0.5 | 1 | KV | ||
Iota Piscium | 45.0 ± 0.5 | 1 | F7V | 4.13 | [11] |
Gamma Cephei «Errai» | 45.0 ± 0.3 | 2 | K1IVe | 3.22 | has 1 known planet |
WISE 2226+0440 | 45.0 | 1 | T8 |
See also
References
- ↑ Howard, Andrew W.; et al. (2010). "The California Planet Survey. I. Four New Giant Exoplanets". The Astrophysical Journal. 721 (2): 1467–1481. arXiv:1003.3488. Bibcode:2010ApJ...721.1467H. doi:10.1088/0004-637X/721/2/1467.
- 1 2 3 4 5 6 7 8 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
- ↑ Nicolet, B. (October 1978). "Photoelectric photometric Catalogue of homogeneous measurements in the UBV System". Astronomy and Astrophysics Supplement Series. 34: 1–49. Bibcode:1978A&AS...34....1N.
- ↑ "Astronomers Discover Record Fifth Planet Around Nearby Star 55 Cancri". Sciencedaily.com. November 6, 2007. Archived from the original on 26 September 2008. Retrieved 2008-09-14.
- ↑ Tanner, Angelle; et al. (February 2015), "Stellar Parameters for HD 69830, a Nearby Star with Three Neptune Mass Planets and an Asteroid Belt", The Astrophysical Journal, 800 (2): 5, arXiv:1412.5251, Bibcode:2015ApJ...800..115T, doi:10.1088/0004-637X/800/2/115, 115.
- 1 2 3 4 5 6 7 Mermilliod, J.-C. (1986), "Compilation of Eggen's UBV data, transformed to UBV (unpublished)", Catalogue of Eggen's UBV data. SIMBAD, Bibcode:1986EgUBV........0M.
- ↑ Lovis, Christophe; et al. (2006). "An extrasolar planetary system with three Neptune-mass planets" (PDF). Nature. 441 (7091): 305–309. arXiv:astro-ph/0703024. Bibcode:2006Natur.441..305L. doi:10.1038/nature04828. PMID 16710412.
- ↑ 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.
- 1 2 3 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.
- 1 2 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.
- 1 2 Gray, R. O.; Napier, M. G.; Winkler, L. I. (April 2001), "The Physical Basis of Luminosity Classification in the Late A-, F-, and Early G-Type Stars. I. Precise Spectral Types for 372 Stars", The Astronomical Journal, 121 (4): 2148–2158, Bibcode:2001AJ....121.2148G, doi:10.1086/319956.
- ↑ "LHS 3287 -- High proper-motion Star". SIMBAD. Centre de Données astronomiques de Strasbourg. Retrieved 2009-04-14.
- ↑ HD 40307, entry, SIMBAD. Accessed online June 18, 2008.
- ↑ Tuomi, M.; Anglada-Escudé, G.; Gerlach, E.; Jones, H. R. A.; Reiners, A.; Rivera, E. J.; Vogt, S. S.; Butler, R. P. (17 December 2012). "Habitable-zone super-Earth candidate in a six-planet system around the K2.5V star HD 40307". Astronomy & Astrophysics. 549: A48. doi:10.1051/0004-6361/201220268.
- ↑ "HR 4112 -- Star in double system", SIMBAD, Centre de Données astronomiques de Strasbourg, retrieved 2012-01-30
- ↑ Mayor, M.; Udry, S.; Naef, D.; Pepe, F.; Queloz, D.; Santos, N. C.; Burnet, M. (February 2004). "The CORALIE survey for southern extra-solar planets". Astronomy and Astrophysics. 415 (1): 391–402. doi:10.1051/0004-6361:20034250.
- ↑ Schnupp, C.; et al. (June 2010), "Discovery of a stellar companion to the nearby solar-analogue HD 104304", Astronomy and Astrophysics, 516: A21, arXiv:1005.0620, Bibcode:2010A&A...516A..21S, doi:10.1051/0004-6361/201014740
- ↑ Strassmeier, K. G.; Fekel, F. C. (1990). "The spectral classification of chromospherically active binary stars with composite spectra". Astronomy and Astrophysics. 230: 389. Bibcode:1990A&A...230..389S.
- ↑ Hoffleit, Dorrit; Jaschek, Carlos (1991). "The Bright star catalogue". New Haven, Conn.: Yale University Observatory, 5th rev.ed. Bibcode:1991bsc..book.....H.
- ↑ LTT 7224 -- High proper-motion Star, database entry, SIMBAD. Accessed on line January 20, 2011.
- ↑ Gliese 742, entry in SIMBAD. Accessed on line November 5, 2007.
- ↑ Cousins, A. W. J. (1973), "UBV photometry of some southern stars", Monthly Notes of the Astronomical Society of Southern Africa, 32: 11, Bibcode:1973MNSSA..32...11C.
- ↑ Lowrance, Patrick J.; Kirkpatrick, J. Davy; Beichman, Charles A. (2002). "A Distant Stellar Companion in the υ Andromedae System". The Astrophysical Journal Letters. 572 (1): L79–L81. arXiv:astro-ph/0205277. Bibcode:2002ApJ...572L..79L. doi:10.1086/341554.
- ↑ "NLTT 5367 -- High proper-motion Star". SIMBAD Astronomical Object Database. Centre de Données astronomiques de Strasbourg. Retrieved 2009-05-20.
- ↑ Wright, J. T.; et al. (2009). "Ten New and Updated Multi-planet Systems, and a Survey of Exoplanetary Systems". The Astrophysical Journal. 693 (2): 1084–1099. arXiv:0812.1582. Bibcode:2009ApJ...693.1084W. doi:10.1088/0004-637X/693/2/1084.
- ↑ Mallik, Sushma V. (December 1999), "Lithium abundance and mass", Astronomy and Astrophysics, 352: 495–507, Bibcode:1999A&A...352..495M
- ↑ 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
- ↑ 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
- ↑ 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. See pp. 80–81.
- ↑ The general catalogue of trigonometric parallaxes, W. F. van Altena, J. T. Lee, E. D. Hoffleit, New Haven, CT: Yale University Observatory, c1995, 4th ed., completely revised and enlarged. CDS ID I/238A.
- ↑ 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 Supplement Series. 501 (3): 941–947. arXiv:0811.3982. Bibcode:2009A&A...501..941H. doi:10.1051/0004-6361/200811191. Note: see VizieR catalogue V/130.
- ↑ 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.
- ↑ Internet Stellar Database Retrieved 2011-11-16.
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