This is a list of star systems within 50-55 light years of Earth.
Star system | Median distance (ly) | Stars in system | Spectral type | Apparent magnitude (V) | Comments and references |
---|---|---|---|---|---|
Delta Aquilae | 50.1 ± 0.6 | 3 | F0IV + K | 3.365 | [1] [2] [3] |
51 Pegasi | 50.1 ± 0.6 | 1 | G5V | 5.49 | has 1 known planet [4] [5] [6] |
HR 159 | 50.2 ± 0.8 | 2 | G8V + G8V | ||
WISE 0614+3912 | 50.2 | 1 | T6 | ||
WISE 1617+1807 | 50.2 | 1 | T8 | ||
WISE 1627+3255 | 50.2 | 1 | T6 | ||
Gliese 156 | 50.3 ± 0.9 | 1 | K7V | 9.02 | |
Phi² Ceti | 50.4 ± 0.8 | 1 | F7V | 5.172 | [7] [8] |
Sigma Boötis «Hemelein Secunda» | 50.4 ± 0.6 | 1 | F2V | 4.46 | |
Gliese 862 | 50.4 ± 0.8 | 1 | KV | ||
Gliese 227 | 50.4 ± 0.7 | 1 | KV | ||
99 Herculis | 50.5 ± 0.6 | 2 | F7V + K4V | 5.10/8.45 | [9] [10] [11] |
Gliese 758/B | 50.5 ± 0.5 | 2 | G8V | 6.36 | |
WISE 0542-1628 | 50.6 | 1 | T6.5 | ||
WISE 1124-0421 | 50.6 | 1 | T7 | ||
WISE 2015+6646 | 50.6 | 1 | T8 | ||
Gliese 3685/3686 | 50.7 +11.8 −8.0 | 2 | MV | ||
HD 38858 | 50.8 ± 0.9 | 1 | G4V | 5.97 | has 1 known planet [9] [12] [13] |
HD 135599 | 50.8 ± 0.8 | 1 | KV | ||
Gliese 778 | 50.8 ± 0.7 | 1 | KV | ||
Tau Boötis | 50.9 ± 0.6 | 2 | F6IV | 4.50 | has 1 known planet [14] [15] |
Gliese 1175 | 50.9 ± 0.6 | 1 | KV | ||
WISE 1519+7009 | 50.9 | 1 | T8 | ||
HD 207129 | 51.0 ± 0.6 | 1 | G2V | 5.58 | [16] |
Gliese 782 | 51.1 ± 1.2 | 1 | KV | ||
Gliese 397 | 51.1 ± 1.0 | 1 | KV | has 1 known planet [17] | |
HD 113538 | 51.2 ± 1.1 | 1 | K9V | 9.057 | has 2 known planets [7] [18] |
WISE 0325-3854 | 51.2 | 1 | T9 | ||
WISE 2342+0856 | 51.2 | 1 | T6.5 | ||
HD 139763 | 51.3 ± 1.1 | 1 | KV | ||
Gliese 157 | 51.4 ± 1.7 | 3 | KV | ||
WISE 0614+0951 | 51.5 | 1 | T7 | ||
WISE 0750+2725 | 51.5 | 1 | T8.5 | ||
WISE 0906+4735 | 51.5 | 1 | T8 | ||
WISE 1906+4508 | 51.5 | 1 | T6 | ||
Gliese 3929 | 51.54 | 1 | M3.5V | 12.675 | [19] Has two confirmed exoplanets |
Castor | 51.6 ± 1.0 | 6 | A1V + Am + dM1e | 1.93/2.97/9.83 | 3 pairs of stars [lower-alpha 1] [20] [21] |
Chi Herculis | 51.7 ± 0.4 | 1 | F8Ve | 4.62 | |
104 Tauri | 51.8 ± 0.8 | 1 | G4V | 4.92 | [22] [23] |
Gliese 777 | 51.8 ± 0.5 | 3 | G6IV + M4.5V | 5.71/14.40 | has 2 known planets [24] |
Ross 640 | 51.84 ± 0.02 | 1 | DZA5.5 | 13.83 | [25] |
Gliese 619 | 51.9 ± 0.7 | 1 | KV | ||
Gliese 112.1 | 51.9 ± 1.3 | 1 | KV | ||
Gliese 156.2 | 52.1 ± 0.7 | 1 | KV | ||
Gliese 462 | 52.2 ± 1.1 | 1 | KV | ||
Gliese 3 | 52.2 ± 0.7 | 1 | KV | ||
WISE 1457+5815 | 52.2 | 1 | T7 | ||
WISE 2319-1844 | 52.2 | 1 | T7.5 | ||
WISE 1622-0959 | 52.2 ± 6.5 | 1 | T6 | ||
Gliese 3781 | 52.3 ± 1.2 | 2 | G8/K0V | 7.06 | |
Gliese 32 | 52.3 ± 1.4 | 2 | KV | ||
Gliese 1062 | 52.3 ± 2.9 | 1 | MV | ||
HD 179930 | 52.5 ± 1.7 | 2 | MV | ||
Gliese 1264 | 52.6 ± 2.1 | 1 | MV | ||
HR 3138 | 52.8 ± 0.4 | 3 | G0V | 5.60 | |
Gliese 472 | 52.8 ± 0.5 | 1 | KV | ||
Gliese 824 | 52.8 ± 0.9 | 1 | KV | ||
I Carinae | 52.9 ± 0.4 | 1 | F2IV | 3.99 | |
Gliese 152 | 52.9 ± 0.6 | 1 | KV | ||
Xi Pegasi | 53.0 ± 0.7 | 2 | F6V + M3.5 | 4.195/11.70 | [26] [27] [28] [29] |
10 Ursae Majoris | 53.0 ± 0.9 | 2 | F4V | 3.96 | [30] |
WISE 1042-3842 | 53.2 | 1 | T6.5 | ||
HR 6516 | 53.3 ± 0.8 | 2 | G9IV-V | 5.31 | |
9 Puppis | 53.4 ± 0.8 | 2 | G2V | 5.16 | |
Gliese 143 | 53.4 ± 1.3 | 1 | KV | ||
Gliese 1177 | 53.4 ± 2.7 | 2 | KV | has 1 known planet [17] | |
Gliese 826.1 | 53.4 ± 1.2 | 1 | KV | ||
HD 40887 | 53.4 ± 0.9 | 3 | K3V | ||
Alpha Circini | 53.5 ± 0.5 | 1 | A7 Vp SrCrE | 3.18-3.21 | Variable [7] [31] |
Gliese 247 | 53.5 ± 1.2 | 1 | KV | ||
BPM 37093 | 53.5 +9.7 −7.1 | 1 | DAV4.4 | 14.0 | Variable [32] [33] |
WISE 2237-0614 | 53.5 | 1 | T5 | 17.40 | |
BY Draconis | 53.6 ± 0.6 | 1 | K6Ve | 8.07 | [34] |
Gliese 531 | 53.6 ± 0.8 | 1 | KV | ||
Gliese 676 | 53.7 ± 1.5 | 2 | M0V + M3V | 9.59 | has 4 known planets [35] [36] |
Gliese 322 | 53.8 ± 1.3 | 1 | KV | ||
WISE 0241-3653 | 53.8 | 1 | T7 | ||
Psi⁵ Aurigae | 53.9 ± 0.6 | 1 | G0V | 5.25 | [37] [38] |
HD 53705/53706/53680 | 53.9 ± 0.9 | 4 | GV | ||
Gliese 553 | 53.9 ± 1.4 | 1 | KV | ||
Gliese 1049 | 53.9 ± 1.2 | 1 | MV | ||
HD 128311 | 54.0 ± 0.9 | 1 | K0V | 7.51 | has 2 known planets [39] |
HR 5273 | 54.1 ± 0.7 | 2 | GV | ||
WISE 0656+4205 | 54.1 | 1 | T3 | ||
WISE 2348-1028 | 54.1 | 1 | T7 | ||
Gliese 3839 | 54.36 ± 1.92 | 1 | M4.5V | ||
WISE 1804+3117 | 54.4 +12.2 −8.4 | 1 | T9.5 | ||
WISE 0148-7202 | 54.4 +19.8 −11.4 | 1 | T9.5 | ||
Gliese 633 | 54.47 ± 0.98 | 1 | M2.5V | ||
Beta Cassiopeiae «Caph» | 54.5 ± 0.5 | 2 | F2III | 2.28 | [7] [40] |
HR 2225 | 54.5 ± 0.7 | 1 | GV | ||
Gliese 795 | 54.5 ± 2.0 | 2 | KV | ||
39 Tauri | 54.6 ± 0.8 | 2 | G5V | 5.90 | [41] [42] |
A 2329 | 54.6 ± 1.1 | 2 | KV | ||
Gliese 295 | 54.8 ± 0.7 | 1 | G8V | 6.98 | |
Gliese 1181 | 54.8 ± 2.5 | 2 | KV | ||
Gliese 786 | 54.8 ± 0.7 | 1 | KV | ||
WISE 0333-5856 | 54.8 | 1 | T3 | ||
WISE 2357+1227 | 54.8 | 1 | T6 | ||
HD 7924 | 54.9 ± 0.5 | 1 | K0V | 7.185 | has 3 known planets [43] |
HR 2721 | 55.0 ± 0.6 | 1 | G0V | 5.54 | |
Gliese 895.4 | 55.0 ± 0.6 | 1 | KV | ||
Gliese 200 | 55.0 ± 1.6 | 2 | KV |
Gliese 876 is a red dwarf star 15.2 light-years away from Earth in the constellation of Aquarius. It is one of the closest known stars to the Sun confirmed to possess a planetary system with more than two planets, after GJ 1061, YZ Ceti, Tau Ceti, and Wolf 1061; as of 2018, four extrasolar planets have been found to orbit the star. The planetary system is also notable for the orbital properties of its planets. It is the only known system of orbital companions to exhibit a near-triple conjunction in the rare phenomenon of Laplace resonance. It is also the first extrasolar system around a normal star with measured coplanarity. While planets b and c are located in the system's habitable zone, they are giant planets believed to be analogous to Jupiter.
HD 210277 is a single star in the equatorial constellation of Aquarius. It has an apparent visual magnitude of 6.54, which makes it a challenge to view with the naked eye, but it is easily visible in binoculars. The star is located at a distance of 69.6 light years from the Sun based on parallax, but is drifting closer with a radial velocity of −20.9 km/s.
HR 7703 is a binary star system in the constellation of Sagittarius. The brighter component has an apparent visual magnitude of 5.31, which means it is visible from suburban skies at night. The two stars are separated by an angle of 7.10″, which corresponds to an estimated semimajor axis of 56.30 AU for their orbit.
DX Cancri is a variable star in the northern zodiac constellation of Cancer. With an apparent visual magnitude of 14.81, it is much too faint to be seen with the naked eye. Visually viewing this star requires a telescope with a minimum aperture of 16 in (41 cm). Based upon parallax measurements, DX Cancri is located at a distance of 11.8 light-years from Earth. This makes it the 18th closest star to the Sun.
Zeta Tucanae, Latinized from ζ Tucanae, is a star in the constellation Tucana. It is a spectral class F9.5 main sequence star with an apparent magnitude of +4.23. Despite having a slightly lower mass, this star is more luminous than the Sun. Based upon parallax measurements by the Hipparcos spacecraft, it is approximately 28.0 light years from Earth. This is one of the least variable stars observed during the Hipparcos mission.
HD 142 is a wide binary star system in the southern constellation of Phoenix. The main component has a yellow-white hue and is dimly visible to the naked eye with an apparent visual magnitude of 5.7. The system is located at a distance of 85.5 light years from the Sun based on parallax measurements, and is drifting further away with a radial velocity of +6 km/s.
94 Ceti is a trinary star system approximately 73 light-years away in the constellation Cetus.
Theta Persei is a star system 37 light years away from Earth, in the constellation Perseus. It is one of the closest naked-eye stars.
Gliese 86 is a K-type main-sequence star approximately 35 light-years away in the constellation of Eridanus. It has been confirmed that a white dwarf orbits the primary star. In 1998 the European Southern Observatory announced that an extrasolar planet was orbiting the star.
36 Ursae Majoris is a double star in the northern constellation of Ursa Major. With an apparent visual magnitude of 4.8, it can be seen with the naked eye in suitable dark skies. Based upon parallax measurements, this binary lies at a distance of 42 light-years from Earth.
HD 114613 is a fifth magnitude yellow subgiant that lies 66.7 light-years away in the constellation of Centaurus. The star may be host to a long-period giant planet.
Xi Pegasi is the Bayer designation for a double star in the northern constellation of Pegasus, the winged horse. Located in the horse's neck, the primary component is an F-type main sequence star that is visible to the naked eye with an apparent visual magnitude of 4.2. It is 86% larger and 17% more massive that the Sun, radiating 4.5 times the solar luminosity. Based upon parallax measurements taken with the Hipparcos spacecraft, it is located 53.2 ± 0.2 light years from the Sun.