This is a list of star systems within 400–450 light years of Earth.
Star system←→←→ | Median distance (ly) | Stars in system | Spectral type | Apparent magnitude (V) | Comments and references |
---|---|---|---|---|---|
400 | 1 | N | 25.6 | The closest Neutron Star to Earth. | |
400 | 1 | F6V | 9.43 | Has 1 potential exoplanet. | |
Delta Scorpii (Dschubba) | 400 | 2 | B0.3 IV + B1-3V | 1.59 - 2.32 | |
Electra (17 Tauri) | 400 ± 10 | 1 | B6 IIIe | 3.70 | Part of Pleiades Cluster (M45). |
Beta Scorpii (Acrab) | 400 ± 40 | 3 | B1V+B2V | ||
401 ± 2 | 1 | M4V | 18.19 | Has 4 exoplanets. | |
HD 61248 (Q Carinae) | 402 ± 7 | 1 | K3 III | 4.93 | |
HD 30442 (HR 1527) | 403 ± 5 | 1 | M3 IIIab | 5.47±0.01 | |
404 | 1 | B5V | |||
407 | 1 | K7V | Has 3 exoplanets. | ||
Betelgeuse (Alpha Orionis) | 1 | M1–M2 Ia–ab | +0.50 | The closest red supergiant star an one of the closest supernova candidates to Earth. | |
416 | 1 | G5III | |||
420 ± 10 | 1 | B9 Vn | 5.44 | Part of Pleiades Cluster (M45). | |
430 | 1 | A8 Vm + G7 III | 4.79 | ||
Celaeno (16 Tauri) | 430 | 1 | B7IV | +5.448 | Part of Pleiades Cluster (M45). |
430 ± 20 | 1 | B9Vn | 5.36 + 8.40 | ||
430 ± 20 | 1 | K2.5III | 3.825 | ||
430 ± 30 | 1 | B1 III | +2.30 | ||
Epsilon Canis Majoris (Adhara) | 430 ± 30 | 1 | B2 II | 1.50 | One of the closest supernova candidates to Earth. |
21 Tauri (Asterope) | 431 ± 8 | 1 | B8 V[|| 5.76 ||Part of [[Pleiades Cluster]] (M45).|- | Atlas (27 Tauri) || 431 ± 13 || 1 || style="background: ;" | B8III || 3.63 ||Part of Pleiades Cluster (M45).|- | Alcyone (Eta Tauri)|| 440 || 1 || style="background: ;" | B5IIIe || 2.87 ||Part of Pleiades Cluster (M45).|-| Taygeta (19 Tauri) || 440 || 2 || style="background: ;" | B6IV || 4.30 ||Part of Pleiades Cluster (M45).|- | Gamma Canis Majoris (Muliphein)|| 440 ± 10 || 1 || style="background: ;" | B8II || +4.10 |||-| Omicron Aquarii || 440 ± 10 || 1 || style="background: ;" | B7 IVe || +4.71 |||-| Zeta Ophiuchi || 440 ± 40 || 1 || style="background: ;" | O9.5 V || 2.56 – 2.58 || The closest O-type star and one of the closest supernova candidates to Earth.|-| RS Canum Venaticorum || 444 ± 1 || 2 || style="background: ;" | F6IV+G8IV || 7.93 to 9.14 |||-| 22 Tauri || 444 ± 6 || 1 || style="background: ;" | A0 Vn || 6.43 ||Part of Pleiades Cluster (M45).|- | 18 Tauri || 444 ± 7 || 1 || style="background: ;" | B8 V || 5.66 ||Part of Pleiades Cluster (M45).|- | HIP 78530 || || 1 || style="background: ;" | B9V || 7.1691±0.0459 ||Has 1 exoplanet.|- |} See alsoReferences |
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