List of star systems within 350–400 light-years
Appearance
This is a list of star systems within 350–400 light years of Earth.[1][2][3]
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Star system←→←→ | Median distance (ly) | Stars in system | Spectral type | Apparent magnitude (V) | Comments and references |
---|---|---|---|---|---|
Kepler-102 | 352.5 ± 0.4 | 1 | K3V | 12.07 | Has 5 exoplanets. |
V1298 Tauri | 354 ± 2 | 1 | K0-K1.5 | 10.31 - 10.43 | Has 4 exoplanets. |
K2-302 | 359.3 | 1 | G | Has 3 exoplanets. | |
K2-198 | 362 | 1 | G | Has 3 exoplanets. | |
TOI-125 | 363 | 1 | G | Has 3 Confirmed and 2 unconfirmed exoplanets. | |
H Centauri | 370 ± 10 | 3 | B7V + B8.5V + B | 5.163 | |
HIP 41378 | 345.7 ± 0.8 | 1 | F8 | 8.92 | Has 5 Confirmed and 2 unconfirmed exoplanets. |
AR Scorpii | 384 ± 2 | 2 | M5+D | It is the first "white dwarf-pulsar" to be discovered. | |
Gamma Andromedae | 390 | 1 | K2+IIb | 2.27 | |
Beta Centauri (Hadar) | 390 ± 20 | 3 | B1 III+B1 III+B1V | 0.61 | |
Alpha Trianguli Australis (Atria) | 391 ± 7 | 1 | K2Ib-IIa | 1.91 | |
Kepler-446 | 391 | 1 | M4V | Has 3 exoplanets. | |
HD 33142 | 394.3 | 1 | G | Has 3 exoplanets. |
See also
[edit]References
[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.