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List of star systems within 70–75 light-years

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This is a list of star systems within 70–75 light years of Earth.

Star system Median distance (ly) Stars in system Spectral type Apparent magnitude (V) Comments and references
GJ 4268 70.0 ± 1.0 2 KV
GJ 3071 70.0 ± 2.5 1 KV
HIP 88976 70.0 2 MV
HD 215152 70.39 ± 0.04 1 K3 V 8.13 Has 4 exoplanets.
HD 90089 70.1 2 F2V 5.25 [1]The temperature of the dust is around 30K.
Gliese 694.2 70.1 2 MV
Gliese 799.1 70.2 1 DA3
HD 16673 70.3 1 FV
HIP 65083 70.3 3 MV
HD 329868 70.3 2 MV
GJ 1170 70.3 2 MV
Epsilon Serpentis 70.4 1 A2Vm 3.71 [2]
GJ 3059 70.4 2 MV
Zeta Leporis 70.5 1 A2IV 3.524 [3][4]
84 Ceti 70.5 2 F7V + K2V 5.709 [5][6][7]
HIP 15332 70.5 2 MV
Sigma Coronae Borealis 70.7 5 F9V + G0V 5.64 [8]
WISE 2327-2730 70.8 1 L9
Gliese 747.4 70.9 2 MV
Theta Sculptoris 71.1 1 F5V 5.236 [9]
Alpha Hydri 71.3 2 F0IV 2.90 [10]
Lambda Arae 71.3 1 F4V 4.77 [3][11]
HD 91324 71.3 2 F9V + M5 4.89 [12][13]
Eta Scorpii 71.6 1 F5IV 3.33 [3][14]
HD 108954 71.6 1 FV
HD 164922 71.69 ± 0.03 1 G9V +6.99 Has 4 exoplanets.
Gamma Tucanae 71.8 ± 0.8 2 F1III 3.99 [15]
WISE 0031-3840 71.8 1 L2 pec
Psi1 Draconis 71.9 2 F5V + F8V 4.59/5.81 has 1 known planet[16]
WISE 0952+1955 72.1 1 T6
WISE 1517+0529 72.4 1 T8
WISE 0836-1859 72.4 1 T8 pec
VHS J1256-1257 72.4 3 M7.5+M7.5+L7.0
WISE 1717+6129 72.7 1 T8
Epsilon Cygni 72.7 ± 0.2 2 K0III 2.48
94 Ceti 73.0 2 F8V + M3V 5.07 has 1 known planet[5][17]
HD 63433 73.035 1 G5V 6.92 [18] Has three known exoplanets
Mu Cygni 73.1 3 F6V + G2V 4.50 [19][20]
WISE 0221+3842 73.1 1 T6.5
18 Puppis 73.3 4 FV
HR 4657 73.6 1 FV
HD 139461/139460 73.8 2 FV
HD 167425 73.8 1 FV
Alpha Serpentis 74 ± 0.3 2 K2 IIIb CN1 2.623 [21][22]
EZ Ceti 74 ± 5 2 G3V 6.75 [23]
Zeta Virginis 74.1 3 A3V + M4V-M7V 3.40 [24]
39 Leonis 74.1 2 F6V + M1 5.81/11.40 [25][26][27]
Upsilon Aquarii 74.2 ± 1.2 1 F5V 5.21 [3][11]
Alpha1 Librae 74.9 ± 0.7 4 F3V 5.15
WISE 1809+3838 74.4 1 T8

See also

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References

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  3. ^ a b c d Gray, R. O.; et al. (July 2006), "Contributions to the Nearby Stars (NStars) Project: spectroscopy of stars earlier than M0 within 40 pc-The Southern Sample", The Astronomical Journal, 132 (1): 161–170, arXiv:astro-ph/0603770, Bibcode:2006AJ....132..161G, doi:10.1086/504637, S2CID 119476992
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  6. ^ Raghavan, Deepak; et al. (September 2010), "A Survey of Stellar Families: Multiplicity of Solar-type Stars", The Astrophysical Journal Supplement, 190 (1): 1–42, arXiv:1007.0414, Bibcode:2010ApJS..190....1R, doi:10.1088/0067-0049/190/1/1, S2CID 368553. For the adopted physical separation, see Table 13 in the appendix.
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  14. ^ Bok, B. J.; Bok, P. F.; Miller, E. W. (November 1972), "Photometric standards for the southern hemisphere. II", Astronomical Journal, 77: 733, Bibcode:1972AJ.....77..733B, doi:10.1086/111346
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  22. ^ Gutierrez-Moreno, A.; et al. (1966). "A system of photometric standards". Publications of the Department of Astronomy University of Chile. 1: 1. Bibcode:1966PDAUC...1....1G.
  23. ^ Houk, N.; Swift, C. (1999). "Michigan catalogue of two-dimensional spectral types for the HD Stars, Vol. 5". Michigan Spectral Survey. 05: 0. Bibcode:1999MSS...C05....0H.
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  26. ^ Woolf, Vincent M.; Wallerstein, George (February 2006), "Calibrating M Dwarf Metallicities Using Molecular Indices", The Publications of the Astronomical Society of the Pacific, 118 (840): 218–226, arXiv:astro-ph/0510148, Bibcode:2006PASP..118..218W, doi:10.1086/498459, S2CID 119340035.
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