Jump to content

List of star systems within 350–400 light-years

From Wikipedia, the free encyclopedia

This is a list of star systems within 350–400 light years of Earth.[1][2][3]

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]
  1. ^ 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.
  2. ^ 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.
  3. ^ Frost, E. B. (December 1924), "Fourteen spectroscopic binaries", Astrophysical Journal, 60: 319–320, Bibcode:1924ApJ....60..319F, doi:10.1086/142868.