This is a list of star systems within 450–500 light years of Earth.[1][2][3]
| Star system←→←→ | Median distance (ly) | Stars in system | Spectral type | Apparent magnitude (V) | Comments and references |
|---|---|---|---|---|---|
| HD 28109 | 457 | 1 | G | Has three exoplanets. | |
| Alpha Lupi | 460 ± 10 | 1 | B1.5 III | 2.30 | One of the closest supernova candidates. |
| Theta Carinae | 460 ± 10 | 2 | B0.5 Vp | 2.76 | |
| Kepler-68 | 470.7 ± 0.7 | 1 | G1V | 10.08 | Has three confirmed and one unconfirmed exoplanets. |
| Kappa Scorpii | 480 ± 10 | 1 | B1.5 III | 2.41 - 2.42 | |
| Lambda Tauri | 480 ± 10 | 3 | B3 V + A4 IV | +3.37 | |
| XO-2S | 489 ± 1 | 2 | K0V + K0V | 11.12±0.03 | Has four exoplanets. |
| XO-2N | 490 ± 1 | 2 | K0V + K0V | 11.18±0.03 | Has four exoplanets. |
| Beta Canis Majoris (Mirzam) | 490 ± 20 | 1 | B1 II-III | 1.985 | One of the closest supernova candidates. |
| Omicron Velorum | 490 ± 30 | 1 | B3/5(V) | +3.60 | |
| Kepler-411B | 496 ± 4 | 1 | M | 12.55 | Has five exoplanets. |
| R Coronae Australis | 498.6 | possibly 3 | B5IIIpe | +11.91 | [4] |
| Kepler-411A | 499.4 ± 0.6 | 1 | K3V | 12.55 | Has five exoplanets. |
See also
editReferences
edit- ^ Brown, A. G. A.; et al. (Gaia collaboration) (August 2018). "Gaia Data Release 2: Summary of the contents and survey properties". Astronomy & Astrophysics. 616. A1. arXiv:1804.09365. Bibcode:2018A&A...616A...1G. doi:10.1051/0004-6361/201833051. Gaia DR2 record for this source at VizieR.
- ^ Barry, Don C. (January 1970), "Spectral Classification of a and F Stars", Astrophysical Journal Supplement, 19: 281, Bibcode:1970ApJS...19..281B, doi:10.1086/190209.
- ^ Frost, E. B. (December 1924), "Fourteen spectroscopic binaries", Astrophysical Journal, 60: 319–320, Bibcode:1924ApJ....60..319F, doi:10.1086/142868.
- ^ Sissa, E.; Gratton, R.; Alcala, J. M.; Desidera, S.; Messina, S.; Mesa, D.; D'Orazi, V.; Rigliaco, E. (2019-10). "The origin of R CrA variability: A complex triple system hosting a disk". Astronomy & Astrophysics. 630: A132. doi:10.1051/0004-6361/201936101. ISSN 0004-6361.
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