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List of star systems within 200–250 light-years

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This is a list of star systems within 200–250 light years of Earth.[1][2][3]

Star system Median distance (ly) Stars in system Spectral type Apparent magnitude (V) Comments and references
HD 184010 200 1 KOIII-IV Has 3 exoplanets.
HD 38677 202 1 F8V Has 4 exoplanets.
Iota Antliae 202 ± 2 1 K1 III +4.60
12 Hydrae (D Hydrae) 202 ± 8 1 G8 IIIb CN-1 4.32
TOI-178 204.9 ± 0.6 1 K7V 11.95 Has 6 exoplanets.
Wolf 354 206.4 1 K3D
Gamma Pyxidis 207 1 K2.5III
Kepler-37 208.7 ± 0.1 1 G8V 9.710 Has 3 confirmed and 1 unconfirmed exoplanets.
HD 108236 210.6 ± 0.2 1 G5V 9.24 Has 5 exoplanets.
Omicron Cephei 211 ± 7 1 G8III+F6V 4.86+7.13
HD 80607 216.8 ± 0.5 1 G5 +9.090
K2-72 216.9 ± 0.4 1 M2.7 V Has 4 exoplanets.
HD 80606 217.2 ± 0.5 1 G5 +9.00 Has 1 exoplanet.
Kepler-138 218.9 ± 0.1 1 M1V 13.040±0.092 Has 3 confirmed and 1 unconfirmed exoplanets.
86 Aquarii (c¹ Aquarii) 220 ± 10 1 G8 III +4.47
K2-233 221 1 K3 Has 3 exoplanets.
Xi Andromedae (Adhil) 223 ± 2 1 K0IIIb 4.9
Alpha Cassiopeiae (Schedar) 228 ± 2 1 K0-IIIa 2.240
Sigma Sagittarii (Nunki) 228 ± 5 1 B2.5 V 2.05
Epsilon Boötis (Izar) 236 ± 8 2 K0 II-III+A2 V A binary star system.
TOI-1260 239.5 1 G Has 3 exoplanets.
HD 82785 239.9 ± 0.5 1 F2IV/V 6.43
Eta Andromedae 240 ± 10 2 G8III-IV + G8III-IV 4.403
Eta Aurigae (Haedus) 243 ± 4 1 B3 V 3.18
Epsilon Aquarii (Albali) 244 ± 7 2 A1 V + KV 3.77
LP 358-499 245.3 1 G Has 4 exoplanets.

See also

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References

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  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.