List of star systems within 450–500 light-years
Appearance
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This is a list of star systems within 450-500 light years of Earth.[1][2][3]
List
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# | Visible to the unaided eye |
$ | Bright star (absolute magnitude of +8.5 or brighter) |
‡ | White dwarf |
§ | Brown dwarf or sub-brown dwarf |
* | Nearest in constellation |
System←→←→ | Star or (sub-) brown dwarf |
Distance (ly) | Constellation | Coordinates: RA, Dec (Ep J2000, Eq J2000) |
Stellar class |
Apparent magnitude (V) |
Parallax (mas) |
Notes and additional references |
---|---|---|---|---|---|---|---|---|
Gamma Circini | A | 450 | Circinus | B5 IV | 4.51 | |||
B | F8 V | |||||||
HL Tauri | 450 | Taurus | K9 | |||||
GG Tauri | A | 450 | Taurus | K7 | 12.25 ± 0.03 / 14.70 ± 0.06 + 17.11 ± 0.07 + 19.94 ± 0.08 | |||
B | M2 | |||||||
C | M3 | |||||||
D | M5 | |||||||
E | M7 | |||||||
1RXS J160929.1−210524 | 450 ± 1 | K7V | Has 1 confirmed exoplanet (1RXS J160929.1-210524 b). | |||||
Pleione (BU Tauri/28 Tauri) | 450 ± 8 | Taurus | B8Vne | 4.77 - 5.50 | Part of Pleiades Cluster (M45). | |||
V518 Carinae (HR 4196) | 450 ± 10 | Carina | B3/5V | 4.82 | Part of IC 2602 Open Cluster. | |||
Delta Antliae | A | 450 ± 10 | Antlia | B9.5 V | +5.55 | |||
B | F9 Ve | |||||||
38 Aquarii | 450 ± 20 | Aquarius | B5 III | 5.43 | ||||
V357 Carinae | 450 ± 20 | Carina | B2IV-V | +3.41 - 3.44 | ||||
Iota Aurigae (Hassaleh) | 450 ± 20 | Auriga | K3 II–III | 2.69 | ||||
V1400 Centauri (1SWASP J140747.93−394542.6/J1407) | 450.8 ± 0.9 | Centaurus | K5 IVe Li | 12.2–15.6 | ||||
HD 100655 (Formosa) | 451 ± 2 | G9 III | 6.45 | |||||
Rho Ophiuchi | A | 451±12 | Ophiuchus | B2/3V | 4.63 | Member of Rho Ophiuchi cloud complex. | ||
B | B2V | |||||||
18 Tauri | 452 ± 3 | Taurus | B8 V | 5.66 | Part of Pleiades Cluster (M45). | |||
K2-33 | 453 ± 1 | M2 | 14.3 | Has 1 exoplanet (K2-33b). | ||||
HD 96063 (Dingolay) | 454 ± 2 | K0 | 8.254 | Has one confirmed exoplanet (HD 96063b/Ramajay). | ||||
HD 28109 | 457 | G | Has three exoplanets. | |||||
Alruba | 457 ± 4 | A0V | 5.76 | |||||
HD 23853 | 459±4 | Taurus | B9.5V | 6.59 | Part of Pleiades Cluster (M45). | |||
IRAS 16293−2422 | A | 460 | G | |||||
B | G | |||||||
XZ Tauri | A | 460 | Taurus | M2.0 | 10.40 | |||
B | M3.5 | |||||||
Alpha Lupi (Uridim) | 460 ± 10 | Lupus | B1.5 III | 2.30 | One of the closest core-collapse supernova candidates to Earth. | |||
Theta Carinae | 460 ± 10 | Carina | B0.5 Vp | 2.76 | Part of IC 2602 Open Cluster. | |||
GY Andromedae | 460 ± 10 | Andromeda | B9 pe | 6.36 | ||||
Merope (23 Tauri) | 460 ± 20 | Taurus | B6IV(e) | 4.18 | Part of Pleiades Cluster (M45). | |||
HAT-P-12 (Komondor) | 463.0 ± 0.7 | K5 | 12.84 | Has one confirmed exoplanet (HAT-P-12b/Puli). | ||||
HAT-P-26 (Guahayona) | 466 ± 1 | K1V | 11.76 | |||||
2MASS J04442713+2512164 | 467 ± 4 | M7.25e±0.25 | 17.65±0.38 | Member of Taurus molecular cloud. | ||||
Nu Scorpii (Jabbah) | A | 470 | Scorpius | B3V | 4.349 + 6.60 + 6.30 | |||
B | B9III | |||||||
B | B9III | |||||||
Winnecke 4B (M40) | 470 ± 1 | G0 V | 10.11 | |||||
Rho Scorpii (Iklil) | 470 ± 10 | Scorpius | B2 IV | 3.86 | ||||
Epsilon Cassiopeiae (Segin) | 470 ± 10 | Cassiopeia | B3 V | 3.37 | ||||
Gamma Pegasi (Algenib) | 470 ± 30 | Pegasus | B2 IV | +2.78 to 2.89 | ||||
Tau Scorpii (Paikauhale) | 470 ± 40 | Scorpius | B0.2 V | +2.82 | ||||
Kepler-68 | 470.7 ± 0.7 | G1V | 10.08 | Has three confirmed and one unconfirmed exoplanets. | ||||
T Tauri | 471 ± 4 | Taurus | K0IV/Ve | 9.3 - 13.5 | ||||
UScoCTIO 108 | A | 473 ± 6 | M7 | 13.6 | has a brown dwarf or an extrasolar planet. | |||
B | M9.5 III | |||||||
Mu² Scorpii (Pipirima) | 474 ± 8 | Scorpius | B2 IV | 3.56 | ||||
WD 1145+017 (EPIC 201563164) | 476 ± 6 | DB | 17.24±0.02 | Has 1 Confirmed exoplanet (WD 1145+017 b). | ||||
Kappa Scorpii (Girtab) | 480 ± 10 | Scorpius | B1.5 III | 2.41 - 2.42 | ||||
Lambda Tauri | A | 480 ± 10 | Taurus | B3 V | +3.37 | |||
B | A4 IV | |||||||
BL Crucis | 480 ± 10 | Crux | M4-5III | 5.38 | ||||
PP Carinae | 480 ± 30 | Carina | B4 Vne | 3.22 - 3.55 | Part of IC 2602 Open Cluster. | |||
HD 206610 (Bosona) | 482 ± 2 | K0III | 8.34 | |||||
Gamma Ursae Minoris (Pherkad) | 487 ± 8 | Ursa Minor | A2 III | |||||
XO-2 | S | 489 ± 1 | K0V | 11.12±0.03 | Has four exoplanets. | |||
N | 490 ± 1 | K0V | 11.18±0.03 | |||||
89 Aquarii (c³ Aquarii) | A | 489.2 | Aquarius | G3 II | +4.69 | |||
B | A2 V | |||||||
HD 93194 | 490 ± 10 | B3/5Vn | Part of IC 2602 Open Cluster. | |||||
Beta Canis Majoris (Mirzam)$ | 490 ± 20 | Canis Major | B1 II-III | 1.985# | ||||
Omicron Velorum | 490 ± 30 | Vela | B3/5(V) | +3.60 | Member of IC 2391 Cluster. | |||
HD 93607 | 491 ± 5 | B4V | 4.87 | Part of IC 2602 Open Cluster. | ||||
8 Leonis Minoris | 492 ± 2 | Leo Minor | M1 IIIab | 5.37 | ||||
HD 108530 | 494 | K2III | ||||||
GQ Lupi | A | 495 ± 4 | Lupus | K7V | 11.40 | Has one confirmed exoplanet (GQ Lupi b). | ||
B | M4 | |||||||
Kepler-411B | 496 ± 4 | M | 12.55 | Orbits a star with 5 planets | ||||
Alpha Apodis (Paradys) | 498 ± 9 | Apus | K3IIICN0.5 | 3.83 | ||||
R Coronae Australis | A | 498.6 | Corona Australis | B5IIIpe | +11.91 | [4] | ||
B | M | |||||||
Kepler-411A | 499.4 ± 0.6 | K3V | 12.55 | Has five exoplanets. | ||||
System | Star or (sub-) brown dwarf |
Distance (ly) | Constellation | Coordinates: RA, Dec (Ep J2000, Eq J2000) |
Stellar class |
Apparent magnitude (V) |
Parallax (mas) |
Notes and additional references |
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.
- ^ Sissa, E.; Gratton, R.; Alcala, J. M.; Desidera, S.; Messina, S.; Mesa, D.; D'Orazi, V.; Rigliaco, E. (October 2019). "The origin of R CrA variability: A complex triple system hosting a disk". Astronomy & Astrophysics. 630: A132. arXiv:1908.07256. doi:10.1051/0004-6361/201936101. ISSN 0004-6361.