List of star systems within 50–55 light-years

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This is a list of star systems within 50-55 light years of Earth.

Star systemMedian distance (ly)Stars in system Spectral type Apparent magnitude (V)Comments and references
Delta Aquilae 50.1 ± 0.63F0IV + K3.365 [1] [2] [3]
51 Pegasi 50.1 ± 0.61G5V5.49has 1 known planet [4] [5] [6]
HR 159 50.2 ± 0.82G8V + G8V
WISE 0614+3912 50.21T6
WISE 1617+1807 50.21T8
WISE 1627+3255 50.21T6
Gliese 156 50.3 ± 0.91K7V9.02
Phi² Ceti 50.4 ± 0.81F7V5.172 [7] [8]
Sigma Boötis «Hemelein Secunda»50.4 ± 0.61F2V4.46
Gliese 862 50.4 ± 0.81KV
Gliese 227 50.4 ± 0.71KV
99 Herculis 50.5 ± 0.62F7V + K4V5.10/8.45 [9] [10] [11]
Gliese 758/B 50.5 ± 0.52G8V6.36
WISE 0542-1628 50.61T6.5
WISE 1124-0421 50.61T7
WISE 2015+6646 50.61T8
Gliese 3685/3686 50.7 +11.8
−8.0
2MV
HD 38858 50.8 ± 0.91G4V5.97has 1 known planet [9] [12] [13]
HD 135599 50.8 ± 0.81KV
Gliese 778 50.8 ± 0.71KV
Tau Boötis 50.9 ± 0.62F6IV4.50has 1 known planet [14] [15]
Gliese 1175 50.9 ± 0.61KV
WISE 1519+7009 50.91T8
HD 207129 51.0 ± 0.61G2V5.58 [16]
Gliese 782 51.1 ± 1.21KV
Gliese 397 51.1 ± 1.01KVhas 1 known planet [17]
HD 113538 51.2 ± 1.11K9V9.057has 2 known planets [7] [18]
WISE 0325-3854 51.21T9
WISE 2342+0856 51.21T6.5
HD 139763 51.3 ± 1.11KV
Gliese 157 51.4 ± 1.73KV
WISE 0614+0951 51.51T7
WISE 0750+2725 51.51T8.5
WISE 0906+4735 51.51T8
WISE 1906+4508 51.51T6
Gliese 3929 51.541M3.5V12.675 [19] Has two confirmed exoplanets
Castor 51.6 ± 1.06A1V + Am + dM1e1.93/2.97/9.833 pairs of stars [lower-alpha 1] [20] [21]
Chi Herculis 51.7 ± 0.41F8Ve4.62
104 Tauri 51.8 ± 0.81G4V4.92 [22] [23]
Gliese 777 51.8 ± 0.53G6IV + M4.5V5.71/14.40has 2 known planets [24]
Ross 640 51.84 ± 0.021DZA5.513.83 [25]
Gliese 619 51.9 ± 0.71KV
Gliese 112.1 51.9 ± 1.31KV
Gliese 156.2 52.1 ± 0.71KV
Gliese 462 52.2 ± 1.11KV
Gliese 3 52.2 ± 0.71KV
WISE 1457+5815 52.21T7
WISE 2319-1844 52.21T7.5
WISE 1622-0959 52.2 ± 6.51T6
Gliese 3781 52.3 ± 1.22G8/K0V7.06
Gliese 32 52.3 ± 1.42KV
Gliese 1062 52.3 ± 2.91MV
HD 179930 52.5 ± 1.72MV
Gliese 1264 52.6 ± 2.11MV
HR 3138 52.8 ± 0.43G0V5.60
Gliese 472 52.8 ± 0.51KV
Gliese 824 52.8 ± 0.91KV
I Carinae 52.9 ± 0.41F2IV3.99
Gliese 152 52.9 ± 0.61KV
Xi Pegasi 53.0 ± 0.72F6V + M3.54.195/11.70 [26] [27] [28] [29]
10 Ursae Majoris 53.0 ± 0.92F4V3.96 [30]
WISE 1042-3842 53.21T6.5
HR 6516 53.3 ± 0.82G9IV-V5.31
9 Puppis 53.4 ± 0.82G2V5.16
Gliese 143 53.4 ± 1.31KV
Gliese 1177 53.4 ± 2.72KVhas 1 known planet [17]
Gliese 826.1 53.4 ± 1.21KV
HD 40887 53.4 ± 0.93K3V
Alpha Circini 53.5 ± 0.51A7 Vp SrCrE3.18-3.21Variable [7] [31]
Gliese 247 53.5 ± 1.21KV
BPM 37093 53.5 +9.7
−7.1
1DAV4.414.0Variable [32] [33]
WISE 2237-0614 53.51T517.40
BY Draconis 53.6 ± 0.61K6Ve8.07 [34]
Gliese 531 53.6 ± 0.81KV
Gliese 676 53.7 ± 1.52M0V + M3V9.59has 4 known planets [35] [36]
Gliese 322 53.8 ± 1.31KV
WISE 0241-3653 53.81T7
Psi⁵ Aurigae 53.9 ± 0.61G0V5.25 [37] [38]
HD 53705/53706/53680 53.9 ± 0.94GV
Gliese 553 53.9 ± 1.41KV
Gliese 1049 53.9 ± 1.21MV
HD 128311 54.0 ± 0.91K0V7.51has 2 known planets [39]
HR 5273 54.1 ± 0.72GV
WISE 0656+4205 54.11T3
WISE 2348-1028 54.11T7
Gliese 3839 54.36 ± 1.921M4.5V
WISE 1804+3117 54.4 +12.2
−8.4
1T9.5
WISE 0148-7202 54.4 +19.8
−11.4
1T9.5
Gliese 633 54.47 ± 0.981M2.5V
Beta Cassiopeiae «Caph»54.5 ± 0.52F2III2.28 [7] [40]
HR 2225 54.5 ± 0.71GV
Gliese 795 54.5 ± 2.02KV
39 Tauri 54.6 ± 0.82G5V5.90 [41] [42]
A 2329 54.6 ± 1.12KV
Gliese 295 54.8 ± 0.71G8V6.98
Gliese 1181 54.8 ± 2.52KV
Gliese 786 54.8 ± 0.71KV
WISE 0333-5856 54.81T3
WISE 2357+1227 54.81T6
HD 7924 54.9 ± 0.51K0V7.185has 3 known planets [43]
HR 2721 55.0 ± 0.61G0V5.54
Gliese 895.4 55.0 ± 0.61KV
Gliese 200 55.0 ± 1.62KV
  1. Each main star has a dM1e companion

See also

Related Research Articles

<span class="mw-page-title-main">Gliese 876</span> Star in the constellation Aquarius

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.

<span class="mw-page-title-main">DX Cancri</span> Red dwarf star in the constellation Cancer

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.

<span class="mw-page-title-main">Zeta Tucanae</span> Star in the constellation Tucana

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.

<span class="mw-page-title-main">Theta Persei</span> Star system in the constellation Perseus

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.

<span class="mw-page-title-main">HD 114613</span> Star in the constellation Centaurus

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.

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