31.9: The Nearest Stars, Brown Dwarfs, and White Dwarfs (Appendix I)
- Page ID
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\(\newcommand{\avec}{\mathbf a}\) \(\newcommand{\bvec}{\mathbf b}\) \(\newcommand{\cvec}{\mathbf c}\) \(\newcommand{\dvec}{\mathbf d}\) \(\newcommand{\dtil}{\widetilde{\mathbf d}}\) \(\newcommand{\evec}{\mathbf e}\) \(\newcommand{\fvec}{\mathbf f}\) \(\newcommand{\nvec}{\mathbf n}\) \(\newcommand{\pvec}{\mathbf p}\) \(\newcommand{\qvec}{\mathbf q}\) \(\newcommand{\svec}{\mathbf s}\) \(\newcommand{\tvec}{\mathbf t}\) \(\newcommand{\uvec}{\mathbf u}\) \(\newcommand{\vvec}{\mathbf v}\) \(\newcommand{\wvec}{\mathbf w}\) \(\newcommand{\xvec}{\mathbf x}\) \(\newcommand{\yvec}{\mathbf y}\) \(\newcommand{\zvec}{\mathbf z}\) \(\newcommand{\rvec}{\mathbf r}\) \(\newcommand{\mvec}{\mathbf m}\) \(\newcommand{\zerovec}{\mathbf 0}\) \(\newcommand{\onevec}{\mathbf 1}\) \(\newcommand{\real}{\mathbb R}\) \(\newcommand{\twovec}[2]{\left[\begin{array}{r}#1 \\ #2 \end{array}\right]}\) \(\newcommand{\ctwovec}[2]{\left[\begin{array}{c}#1 \\ #2 \end{array}\right]}\) \(\newcommand{\threevec}[3]{\left[\begin{array}{r}#1 \\ #2 \\ #3 \end{array}\right]}\) \(\newcommand{\cthreevec}[3]{\left[\begin{array}{c}#1 \\ #2 \\ #3 \end{array}\right]}\) \(\newcommand{\fourvec}[4]{\left[\begin{array}{r}#1 \\ #2 \\ #3 \\ #4 \end{array}\right]}\) \(\newcommand{\cfourvec}[4]{\left[\begin{array}{c}#1 \\ #2 \\ #3 \\ #4 \end{array}\right]}\) \(\newcommand{\fivevec}[5]{\left[\begin{array}{r}#1 \\ #2 \\ #3 \\ #4 \\ #5 \\ \end{array}\right]}\) \(\newcommand{\cfivevec}[5]{\left[\begin{array}{c}#1 \\ #2 \\ #3 \\ #4 \\ #5 \\ \end{array}\right]}\) \(\newcommand{\mattwo}[4]{\left[\begin{array}{rr}#1 \amp #2 \\ #3 \amp #4 \\ \end{array}\right]}\) \(\newcommand{\laspan}[1]{\text{Span}\{#1\}}\) \(\newcommand{\bcal}{\cal B}\) \(\newcommand{\ccal}{\cal C}\) \(\newcommand{\scal}{\cal S}\) \(\newcommand{\wcal}{\cal W}\) \(\newcommand{\ecal}{\cal E}\) \(\newcommand{\coords}[2]{\left\{#1\right\}_{#2}}\) \(\newcommand{\gray}[1]{\color{gray}{#1}}\) \(\newcommand{\lgray}[1]{\color{lightgray}{#1}}\) \(\newcommand{\rank}{\operatorname{rank}}\) \(\newcommand{\row}{\text{Row}}\) \(\newcommand{\col}{\text{Col}}\) \(\renewcommand{\row}{\text{Row}}\) \(\newcommand{\nul}{\text{Nul}}\) \(\newcommand{\var}{\text{Var}}\) \(\newcommand{\corr}{\text{corr}}\) \(\newcommand{\len}[1]{\left|#1\right|}\) \(\newcommand{\bbar}{\overline{\bvec}}\) \(\newcommand{\bhat}{\widehat{\bvec}}\) \(\newcommand{\bperp}{\bvec^\perp}\) \(\newcommand{\xhat}{\widehat{\xvec}}\) \(\newcommand{\vhat}{\widehat{\vvec}}\) \(\newcommand{\uhat}{\widehat{\uvec}}\) \(\newcommand{\what}{\widehat{\wvec}}\) \(\newcommand{\Sighat}{\widehat{\Sigma}}\) \(\newcommand{\lt}{<}\) \(\newcommand{\gt}{>}\) \(\newcommand{\amp}{&}\) \(\definecolor{fillinmathshade}{gray}{0.9}\)Star | System | Discovery Name | Distance (light-year) | Spectral Type | Location: RA1 | Location: Dec2 | Luminosity (Sun = 1) |
---|---|---|---|---|---|---|---|
Sun | — | G2 V | — | — | 1 | ||
1 | 1 | Proxima Centauri | 4.2 | M5.5 V | 14 29 | −62 40 | 5 × 10−5 |
2 | 2 | Alpha Centauri A | 4.4 | G2 V | 14 39 | −60 50 | 1.5 |
3 | Alpha Centauri B | 4.4 | K2 IV | 14 39 | −60 50 | 0.5 | |
4 | 3 | Barnard’s Star | 6.0 | M4 V | 17 57 | +04 42 | 4.4 × 10−4 |
5 | 4 | Luhman 16A | 6.5 | L8 | 10 49 | –53 19 | |
6 | Luhman 16B | 6.5 | T1 | 10 40 | –53 19 | ||
7 | 5 | WISE 0855-0714 | 7.3 | Y2 | 08 55 | –07 15 | |
8 | 4 | Wolf 359 | 7.8 | M6 V | 10 56 | +07 00 | 2 × 10−5 |
9 | 5 | Lalande 21 185 | 8.3 | M2 V | 11 03 | +35 58 | 5.7 × 10−3 |
10 | 6 | Sirius A | 8.6 | A1 V | 06 45 | −16 42 | 23.1 |
11 | Sirius B | 8.6 | DA23 | 06 45 | −16 43 | 2.5 × 10−3 | |
12 | 7 | Luyten 726-8 A | 8.7 | M5.5 V | 01 39 | −17 57 | 6 × 10−5 |
13 | Luyten 726-8 B (UV Ceti) | 8.7 | M6 V | 01 39 | −17 57 | 4 × 10−5 | |
14 | 8 | Ross 154 | 9.7 | M3.5 V | 18 49 | −23 50 | 5 × 10−4 |
15 | 9 | Ross 248 (HH Andromedae) | 10.3 | M5.5 V | 23 41 | +44 10 | 1.0 × 10−4 |
16 | 10 | Epsilon Eridani | 10.5 | K2 V | 03 32 | −09 27 | 0.29 |
17 | 11 | Lacaille 9352 | 10.7 | M0.5 V | 23 05 | −35 51 | 0.011 |
18 | 12 | Ross 128 (FI Virginis) | 10.9 | M4 V | 11 47 | +00 48 | 3.4 × 10−4 |
19 | 13 | Luyten 789-6 A (EZ Aquarii A) | 11.3 | M5 V | 22 38 | −15 17 | 5 × 10−5 |
20 | Luyten 789-6 B (EZ Aquarii B) | 11.3 | M5.5 V | 22 38 | −15 15 | 5 × 10−5 | |
21 | Luyten 789-6 C (EZ Aquarii C) | 11.3 | M6.5 V | 22 38 | −15 17 | 2 × 10−5 | |
22 | 14 | 61 Cygni A | 11.4 | K5 V | 21 06 | +38 44 | 0.086 |
23 | 61 Cygni B | 11.4 | K7 V | 21 06 | +38 44 | 0.041 | |
24 | 15 | Procyon A | 11.4 | F5 IV | 07 39 | +05 13 | 7.38 |
25 | Procyon B | 11.4 | wd4 | 07 39 | +05 13 | 5.5 × 10−4 | |
26 | 16 | Sigma 2398 A | 11.5 | M3 V | 18 42 | +59 37 | 0.003 |
27 | Sigma 2398 B | 11.5 | M3.5 V | 18 42 | +59 37 | 1.4 × 10−3 | |
28 | 17 | Groombridge 34 A (GX Andromedae) | 11.6 | M1.5 V | 00 18 | +44 01 | 6.4 × 10−3 |
29 | Groombridge 34 B (GQ Andromedae) | 11.6 | M3.5 V | 00 18 | +44 01 | 4.1 × 10−4 | |
30 | 18 | Epsilon Indi A | 11.8 | K5 V | 22 03 | −56 46 | 0.150 |
31 | Epsilon Indi Ba | 11.7 | T15 | 22 04 | −56 46 | — | |
32 | Epsilon Indi Bb | 11.7 | T66 | 22 04 | −56 46 | — | |
33 | 19 | G 51-15 (DX Cancri) | 11.8 | M6.5 V | 08 29 | +26 46 | 1 × 10−5 |
34 | 20 | Tau Ceti | 11.9 | G8.5 V | 01 44 | −15 56 | 0.458 |
35 | 21 | Luyten 372-58 | 12.0 | M5 V | 03 35 | −44 30 | 7 × 10−5 |
36 | 22 | Luyten 725-32 (YZ Ceti) | 12.1 | M4.5 V | 01 12 | −16 59 | 1.8 × 10−4 |
37 | 23 | Luyten’s Star | 12.4 | M3.5 V | 07 27 | +05 13 | 1.4 × 10−3 |
38 | 24 | SCR J184-6357 A | 12.6 | M8.5 V | 18 45 | −63 57 | 1 × 10−6 |
39 | SCR J184-6357 B | 12.7 | T67 | 18 45 | −63 57 | — | |
40 | 25 | Teegarden’s Star | 12.5 | M6 V | 02 53 | +16 52 | 1 × 10−5 |
41 | 26 | Kapteyn’s Star | 12.8 | M1 V | 05 11 | −45 01 | 3.8 × 10−3 |
42 | 27 | Lacaille 8760 (AX Microscopium) | 12.9 | K7 V | 21 17 | −38 52 | 0.029 |