List of star systems within 60–65 light-years

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This is a list of star systems within 60-65 light years of Earth.

Star systemMedian distance (ly)Stars in system Spectral type Apparent magnitude (V)Comments and references
Delta Equulei 60.0 ± 1.02F5V + G04.49/5.4 [1]
HD 53143 60.0 ± 0.61K9V6.80 [2] [3]
15 Leonis Minoris 60.1 ± 0.81G0V5.12 [4] [5]
Gliese 339 60.1 ± 1.32KV
Gliese 161 60.2 ± 0.91GV
Gliese 2102 60.2 ± 1.21KV
Gliese 4134 60.4 +9.0
−6.9		1KV
Gliese 315 60.4 ± 1.21KV
Gliese 509 60.4 ± 2.52KV
HD 156985 60.4 ± 0.81KV
G 185-32 60.4 +3.5
−3.2		1DA4.013.00 [6] [7]
Gliese 610 60.5 ± 1.51KV
Gliese 106 60.5 ± 2.81KV
HR 244 60.6 ± 0.71F9V4.82 [8]
Theta Cygni 60.7 ± 0.52F3V + M3V4.490/13.03 [9] [10] [11] [12]
Gliese 499 60.7 ± 2.22KV
WISE 2301+0216 60.71T6.5
Gliese 254 60.8 ± 2.01KV
Theta Centauri (Menkent)60.9 ± 0.91K0III2.06 [4] [13]
Mu Virginis 60.9 ± 1.11F2IV3.88 [4] [5]
HD 152606 60.9 ± 1.01KV
Gliese 902.1 60.9 ± 1.31KV
Kelu-1 60.9 ± 2.33L2 + L4 [14]
Gliese 1094 61.0 ± 2.31KV
HR 8061 61.1 ± 2.63FV
Tau Piscis Austrini 61.1 ± 1.01F6V4.94
HR 8148 61.1 ± 1.32GV
HD 206804 61.1 ± 1.92KV
Gliese 715 61.2 ± 1.21KV
WISE 0150+3827 61.31T0
HD 4747 61.4 ± 1.22G8V7.30
Gliese 249 61.4 ± 1.41KV
Gliese 296 61.5 ± 9.71KV
HD 170573 61.5 ± 9.71KV
Gliese 1054 61.55 ± 0.851M1Ve
6 Ceti 61.6 ± 0.91F8V4.89 [15]
HR 7683 61.6 ± 0.62GIV
Gliese 583 61.6 ± 1.81KV
Gliese 4287 61.6 ± 2.32KV
Gliese 773 61.6 ± 1.82KV
WISE 2157+2659 61.61T7
Gliese 100 61.7 ± 2.33KV
Eta Serpentis «Tang»61.8 ± 0.91K0IV3.260 [16] [17]
Gliese 689 62.0 ± 0.91KV
WISE 1711+3500 62.0 ± 9.82T8
HD 139477 62.2 ± 0.91KV
110 Herculis 62.3 ± 0.81F6V4.20 [18]
HR 2643 62.3 ± 1.01GV
WISE 1721+1117 62.31T6
HR 3625 62.4 ± 1.11FV
Gliese 646 62.4 ± 2.43KV
Gliese 576 62.6 ± 2.51KV
Gliese 1246 62.6 ± 1.41KV
ADS 10075 62.6 ± 1.42KV
WISE 0049+0441 62.61L9
Rho Puppis «Tureis»62.7 ± 0.81F2mF5IIp2.78 [19] [20]
HD 25457 62.7 ± 0.91FV
Gliese 292.2 62.7 ± 2.31GV
Gliese 825.3 62.7 ± 1.51KV
Gliese 3546 62.7 +11.4
−8.4		1KV
1 Centauri 62.8 ± 0.91F3IV4.23
Gliese 1283 62.8 ± 1.41KV
HD 189733 62.8 ± 1.12K1.5V + M7.676has 1 known planet [21] [22] [23]
Beta Pictoris 62.9 ± 0.61A6V3.861has 1 known planet [4] [24] [25]
WISE 0032-4946 62.91T8.5
HD 43587 63.0 ± 1.04G0V + M0V + M3.5V + M5V5.70 [26] [27] [28]
Gliese 710 63.0 ± 1.81K7V9.69 [4] [29]
Gliese 900 63.0 ± 2.23KV
WD 0806-661 63.0 ± 2.02DQ4.2 + Y13.71 [30] [31] [32]
Gliese 775.1 63.1 ± 1.01GV
Gliese 1126 63.1 ± 1.12KV
Gliese 45 63.1 ± 1.31KV
Gliese 816.1 63.2 ± 0.92KV
Omicron Aquilae 63.3 ± 0.93F8V + M3V5.11 [33] [34]
Gliese 790 63.3 ± 1.01GV
Gliese 9126 63.3 +36.4
−16.9		1KV
HD 274255 63.3 +4.9
−4.3		1MV
Alpha Chamaeleontis 63.5 ± 0.61F5V4.066 [35]
HR 6465 63.5 ± 1.11GV
Gliese 894.5 63.5 ± 1.61KV
Gliese 59 63.6 ± 1.12KV
Gliese 571.1 63.6 ± 2.31KV
WISE 0812+4021 63.61T8
HD 130004 63.7 ± 1.21KV
c Ursae Majoris 63.8 ± 0.92G0V5.20 [5] [36]
Gliese 204.1 63.8 ± 0.61GV
HIP 38594 63.8 ± 2.01MV
Gliese 3859 63.9 ± 0.71GV
74 Orionis 64.0 ± 1.11FV
Gliese 3383 64.0 +8.5
−6.7		1GV
Alpha Trianguli (Mothallah)64.1 ± 1.02F5III-F6IV + M3.42 [13] [37] [38] [39]
Eta Crucis 64.2 ± 0.62F2III4.14 [40]
Gliese 3867 64.2 ± 1.31GV
HD 59747 64.2 ± 1.71GV
Gliese 906 64.2 ± 2.11KV
45 Boötis 64.3 ± 1.02F5V4.93 [41]
HD 217107 64.3 ± 1.01G8IV6.17has 2 known planets [42]
Gliese 81.2 64.3 ± 1.01KV
HD 220140 64.4 ± 0.81GV
Gliese 140.1 64.4 ± 2.32KV
Gliese 3678 64.4 ± 1.51KV
EQ Virginis 64.5 ± 1.31K5Ve9.31
Gliese 3634 64.5 +2.0
−1.9		1M2.511.95has 1 known planet [43]
DENIS-P J020529.0-115925 64.5 +2.0
−1.9		3L5.517.3
Nu² Canis Majoris 64.7 ± 0.91K1III3.95has 1 known planet [44]
Gliese 586 64.8 ± 1.53KV
Gliese 1164 64.8 +4.4
−3.9		2KV
LHS 1678 64.8±0.032M3.5V12.6Primary component is orbited by three exoplanets. [45]
22 Lyncis 64.9 ± 1.12FV
HD 192263 64.9 ± 1.51K2V7.79has 1 known planet [46]
HD 35112 64.9 ± 2.01KV
WISE 0612-3036 64.91T6
WISE 0929+0409 64.91T6.5
HR 3430 65.0 ± 1.32GV
Gliese 530 65.0 ± 1.11GV
HD 216520 65.0 ± 0.81KV

See also

Related Research Articles

Zeta Trianguli Australis is a spectroscopic binary in the constellation Triangulum Australe. It is approximately 39.5 light years from Earth.

<span class="mw-page-title-main">Omicron Aquilae</span> Star in the constellation Aquila

Omicron Aquilae is the Bayer designation for a double star in the equatorial constellation of Aquila. The brighter component has an apparent visual magnitude of +5.11, which means it is faintly visible to the naked eye in dark suburban skies. The annual parallax shift of this star is 52.11 mas, which is equivalent to a physical distance of 62.6 light-years from Earth.

<span class="mw-page-title-main">Theta Boötis</span> Star in the northern constellation of Boötes

Theta Boötis, Latinized from θ Boötis, is a star in the northern constellation of Boötes the herdsman, forming a corner of the upraised left hand of this asterism. It has the traditional name Asellus Primus and the Flamsteed designation 23 Boötis. Faintly visible to the naked eye, this star has a yellow-white hue with an apparent visual magnitude of 4.05. It is located at a distance of 47 light years from the Sun based on parallax, but is drifting closer with a radial velocity of −10.6 km/s.

<span class="mw-page-title-main">44 Boötis</span> Triple star system in the constellation Boötes

44 Boötis or i Boötis is a triple star system in the constellation Boötes. It is approximately 41.6 light years from Earth.

<span class="mw-page-title-main">Tau Centauri</span> White-hued star in the constellation Centaurus

Tau Centauri, Latinized from τ Centauri, is a solitary star in the southern constellation of Centaurus. It is visible to the naked eye with an apparent visual magnitude of +3.86. The distance to this star, based upon an annual parallax shift of 24.85 mas, is 131 light years. There is a 98% chance that it is a co-moving companion of Gamma Centauri; the two stars have an estimated separation of 1.7 ly (0.53 pc).

HD 187923 is a suspected variable star in the equatorial constellation of Aquila. It is a dim star that is just visible to the naked eye, having an apparent visual magnitude of 6.148. Based upon an annual parallax shift of 37.04 mas, it is located 88 light years away. The star is moving closer to the Earth with a heliocentric radial velocity of −20.7 km/s. It has a relatively high proper motion, traversing the celestial sphere at the rate of 0.480″ per year.

HD 24496 is a binary star system in the equatorial constellation of Taurus. The combined apparent visual magnitude of the pair is 6.81, which is too faint to be readily visible to the normal human eye. The system is located at a distance of 66.8 light years from the Sun based on parallax, and is drifting further away with a radial velocity of +19 km/s. It is traversing the celestial sphere with a proper motion of 0.276″ per year.

Tau6 Eridani, Latinized from τ6 Eridani, is a single star in the equatorial constellation of Eridanus, located near the constellation border with Fornax. It has a yellow-white hue with an apparent visual magnitude of 4.22, which is bright enough to be seen with the naked eye. Based upon parallax measurements, the distance to this star is around 57.5 light years. It is drifting further away with a radial velocity of +8 km/s.

Tau1 Eridani, Latinized from τ1 Eridani, is a binary star system in the constellation Eridanus. It has an apparent magnitude of 4.46, making it visible to the naked eye in suitably dark conditions. This a spectroscopic binary with an orbital period of 958 days. It is located about 46 light years from the Earth. At present, the system is moving away from the Sun with a radial velocity of +26 km/s. About 305,000 years ago, it made perihelion passage at an estimated distance of 30.5 ly (9.35 pc).

Nu1 Lupi (ν1 Lup) is a solitary star in the southern constellation of Lupus. It is visible to the naked eye with an apparent visual magnitude of 5.01. It is a high proper motion star with an annual parallax shift of 27.89 mas as seen from Earth, yielding a distance estimate of 117 light years from the Sun.

<span class="mw-page-title-main">50 Persei</span> Star in the constellation Perseus

50 Persei is a star in the constellation Perseus. Its apparent magnitude is 5.52, which is bright enough to be seen with the naked eye. Located around 21.00 parsecs (68.5 ly) distant, it is a White main-sequence star of spectral type F7V, a star that is currently fusing its core hydrogen. In 1998 the star was named a candidate Gamma Doradus variable with a period of 3.05 days, which would means it displays variations in luminosity due to non-radial pulsations in the photosphere. Subsequently, it was classified as a RS Canum Venaticorum and BY Draconis variable by an automated program.

ω Leonis, is a star system located in the zodiac constellation of Leo. It is visible to the naked eye in the absence of light pollution, with an apparent visual magnitude of about 5.4. The distance to this star, as determined using parallax measurements, is around 108 light years from the Sun. Because of its location close to the ecliptic, it is subject to being obscured by the Moon, and potentially by planets.

HD 126053 is the Henry Draper Catalogue designation for a star in the equatorial constellation of Virgo. It has an apparent magnitude of 6.25, which means it is faintly visible to the naked eye. According to the Bortle scale, it requires dark suburban or rural skies to view. Parallax measurements made by the Hipparcos spacecraft provide an estimated distance of 57 light years to this star. It is drifting closer with a heliocentric radial velocity of −19.2 km/s.

Lambda Crateris, Latinized from λ Crateris, is the Bayer designation for a suspected binary star system in the southern constellation of Crater. With an annual parallax shift of 23.32 milliarcsecond as observed from Earth, it is located around 140 light years from the Sun. It is faintly visible to the naked eye with an apparent visual magnitude of 5.08.

HD 119124 is a wide binary star system in the circumpolar constellation of Ursa Major. With an apparent visual magnitude of 6.3, it lies below the normal brightness limit of stars that are visible with the naked eye under most viewing conditions. An annual parallax shift of 39.24 mas for the A component provides a distance estimate of 83 light years. The pair are candidate members of the Castor Moving Group, which implies a relatively youthful age of around 200 million years. HD 119124 is moving closer to the Sun with a radial velocity of −12 km/s.

References

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