List of nearest stars and brown dwarfs facts for kids
This list shows all the known stars, brown dwarfs, and sub-brown dwarfs that are within 20 light-years of our Sun. So far, scientists have found 131 such objects. Only 22 of these are bright enough to be seen without a telescope. For us to see a star without a telescope, its light must be brighter than a certain level (magnitude 6.5).
These 131 objects are part of 94 star systems. Most of them (103) are "main sequence stars." This group includes 80 red dwarfs and 23 "typical" stars that are more massive. Scientists have also found 6 white dwarfs (these are stars that have used up all their fuel), 21 brown dwarfs, and 1 sub-brown dwarf. This sub-brown dwarf, called WISE 0855−0714, might even be a planet floating freely in space.
The closest star system to us is Alpha Centauri. The closest star in that system is Proxima Centauri, which is about 4.25 light-years away from Earth. The brightest and most massive object on this list is Sirius A. It is also the brightest star we see in Earth's night sky. Its companion, Sirius B, is a white dwarf and the hottest object on this list. The largest object within 20 light-years is Procyon.
Our Solar System and the other stars on this list are moving within a cloud of gas and dust called the Local Interstellar Cloud. This cloud is about 30 light-years wide. The Local Interstellar Cloud is inside an even bigger empty space called the Local Bubble. This bubble is about 300 light-years across. It contains star groups like Ursa Major and the Hyades. The Local Bubble also holds the nearby G-Cloud, which includes stars like Alpha Centauri and Altair. Our Local Bubble is just a small part of the Orion Arm. This arm is where most of the stars we see without a telescope are located. The Orion arm is one of the spiral arms of our Milky Way galaxy.
Contents
Measuring Star Distances
The easiest way to measure how far away nearby stars are is by using something called parallax. This is how much a star seems to shift its position against more distant background objects as Earth moves around the Sun. Imagine holding your finger out and closing one eye, then the other. Your finger seems to jump! Stars do something similar.
A parsec is a unit of distance. It's based on how much a star's position appears to shift. If a star is less than 5 parsecs away, its shift will be easy to measure. To figure out where stars were in the past or will be in the future, scientists use very precise measurements. They look at parallax, how much stars move across the sky (called proper motion), and how fast they are moving directly towards or away from us (called radial velocities). Combining these measurements helps us understand a star's true movement in space. However, these predictions become less accurate over very long periods, like thousands of years.
Thanks to the Gaia telescope, scientists have estimated that about 694 stars will come within 5 parsecs (about 16 light-years) of our Solar System in the next 15 million years. Of these, 26 stars have a good chance of coming within 1 light-year. Another 7 might even come within half a light-year!
One star predicted to come very close to our Sun is a small orange dwarf star called Gliese 710. It is about half the size of our Sun. Scientists believe it will pass about 0.17 light-years away from the Sun in about 1.3 million years. This is close enough to stir up the Oort cloud, which is a huge cloud of icy objects far beyond our planets.
Stars and Brown Dwarfs Near Our Sun
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Visible to the unaided eye (apparent magnitude of +6.5 or brighter) |
$ | Luminous star (absolute magnitude of +8.5 or brighter) |
![]() |
White dwarf |
§ | Brown dwarf |
& | Sub-brown dwarf or rogue planet |
* | Nearest in constellation |
The "classes" of stars and brown dwarfs are shown with colors that match their type. Many brown dwarfs are too dim to be seen with regular light. So, their brightness is measured using infrared light (J band). "Absolute magnitude" tells us how bright a star would look if it were all the same distance away from us. Some of the distances listed are approximate.
Designation | Distance (ly (±err))→→ |
Coordinates: RA, Dec (Ep J2000, Eq J2000) |
Stellar class |
Mass | Magnitude (mV or mJ) | Parallax (mas (±err)) |
Notes and additional references |
|||
---|---|---|---|---|---|---|---|---|---|---|
System | Star or (sub-) brown dwarf | M☉ | App. | Abs. | ||||||
Solar System | Sun (Sol)$ | 0.0000158 | N/A | N/A | G2V | 1 | −26.74![]() |
4.85 | N/A | eight recognized planets and more dwarf planets |
Alpha Centauri | Proxima Centauri (C, V645 Centauri) | 4.2465 +0.0003−{{{2}}} |
Cen* | 14h 29m 43.0s −62° 40′ 46″ |
M5.5Ve | 0.122 | 11.09 | 15.53 | 768.0665 +0.0499−{{{2}}} |
flare star, two confirmed planets (b, 2016, and d, 2022) and a third disputed planet (c, 2019) |
Rigil Kentaurus (A)$ | 4.3441 +0.0022−{{{2}}} |
14h 39m 36.5s −60° 50′ 02″ |
G2V | 1.079 | 0.01![]() |
4.38 | 750.81 +0.38−{{{2}}} |
one directly imaged habitable-zone planet candidate (Candidate 1) (2021) | ||
Toliman (B)$ | 14h 39m 35.1s −60° 50′ 14″ |
K1V | 0.909 | 1.34![]() |
5.71 | planet b refuted in 2015 | ||||
Barnard's Star (BD+04°3561a) | 5.9629 +0.0004−{{{2}}} |
Oph* | 17h 57m 48.5s +04° 41′ 36″ |
M4.0Ve | 0.144 | 9.53 | 13.22 | 546.9759 +0.0401−{{{2}}} |
flare star, largest-known proper motion, one refuted planet (b) | |
Luhman 16 (WISE 1049−5319) |
A§ | 6.5029 +0.0011−{{{2}}} |
Vel* | 10h 49m 18.9s −53° 19′ 10″ |
L8±1 | 0.032 | 10.7 J | 14.2 J | 501.557 +0.082−{{{2}}} |
nearest brown dwarfs |
B§ | T1±2 | 0.027 | ||||||||
WISE 0855−0714& | 7.430 +0.041−{{{2}}} |
Hya* | 08h 55m 10.8s -07° 14′ 43″ |
Y4 | 0.003-0.010 | 25.0 J | 28.2 J | 439.0 +2.4−{{{2}}} |
sub-brown dwarf | |
Wolf 359 (CN Leonis) | 7.8558 +0.0013−{{{2}}} |
Leo* | 10h 56m 29.2s +07° 00′ 53″ |
M6.0V | 0.090 | 13.44 | 16.55 | 415.1794 +0.0684−{{{2}}} |
flare star, has 1 candidate & 1 refuted planet | |
Lalande 21185 (BD+36°2147, Gliese 411, HD 95735) | 8.3044 +0.0007−{{{2}}} |
UMa* | 11h 03m 20.2s +35° 58′ 12″ |
M2.0V | 0.390 | 7.47 | 10.44 | 392.7529 +0.0321−{{{2}}} |
two known planets (2019, 2021) | |
Alpha Canis Majoris | Sirius (A)$ | 8.7094 +0.0054−{{{2}}} |
CMa* | 06h 45m 08.9s −16° 42′ 58″ |
A1V | 2.063 | −1.46![]() |
1.42 | 374.4896 +0.2313−{{{2}}} |
brightest star in the night sky |
B![]() |
DA2 | 1.018 | 8.44 | 11.34 | ||||||
Gliese 65 (Luyten 726–8) | A (BL Ceti) | 8.724 +0.012−{{{2}}} |
Cet* | 01h 39m 01.3s −17° 57′ 01″ |
M5.5Ve | 0.102 | 12.54 | 15.40 | 373.8443 +0.5009−{{{2}}} |
flare star (Archetypal member) |
B (UV Ceti) | M6.0Ve | 0.100 | 12.99 | 15.85 | ||||||
Ross 154 (V1216 Sagittarii) | 9.7063 +0.0009−{{{2}}} |
Sgr* | 18h 49m 49.4s −23° 50′ 10″ |
M3.5Ve | 0.17 | 10.43 | 13.07 | 336.0266 +0.0317−{{{2}}} |
flare star | |
Ross 248 (HH Andromedae) | 10.3057 +0.0014−{{{2}}} |
And* | 23h 41m 54.7s +44° 10′ 30″ |
M5.5Ve | 0.136 | 12.29 | 14.79 | 316.4812 +0.0444−{{{2}}} |
flare star | |
Ran (Epsilon Eridani)$ | 10.4749 +0.0037−{{{2}}} |
Eri* | 03h 32m 55.8s −09° 27′ 30″ |
K2V | 0.820 | 3.73![]() |
6.19 | 311.37 +0.11−{{{2}}} |
three circumstellar disks, one confirmed planet (AEgir, 2000) and one candidate (c, 2002) |
|
Lacaille 9352 (Gliese 887) | 10.7241 +0.0007−{{{2}}} |
PsA* | 23h 05m 52.0s −35° 51′ 11″ |
M0.5V | 0.486 | 7.34 | 9.75 | 304.1354 +0.0200−{{{2}}} |
two planets, b and c, with equivocal evidence for a third in the habitable zone (2020) | |
Ross 128 (FI Virginis) | 11.0074 +0.0011−{{{2}}} |
Vir* | 11h 47m 44.4s +00° 48′ 16″ |
M4.0Vn | 0.168 | 11.13 | 13.51 | 296.3053 +0.0302−{{{2}}} |
flare star, one planet (b) (2017) | |
EZ Aquarii (Gliese 866, Luyten 789-6) |
A | 11.109 +0.034−{{{2}}} |
Aqr* | 22h 38m 33.4s −15° 17′ 57″ |
M5.0Ve | 0.11 | 13.33 | 15.64 | 293.60 +0.9−{{{2}}} |
A & B flare stars |
B | M? | 0.11 | 13.27 | 15.58 | ||||||
C | M? | 0.10 | 14.03 | 16.34 | ||||||
Alpha Canis Minoris | Procyon (A)$ | 11.402 +0.032−{{{2}}} |
CMi* | 07h 39m 18.1s +05° 13′ 30″ |
F5IV–V | 1.499 | 0.38![]() |
2.66 | 286.05 +0.81−{{{2}}} |
|
B![]() |
DQZ | 0.602 | 10.70 | 12.98 | ||||||
61 Cygni | A (BD+38°4343)$ | 11.4039 +0.0012−{{{2}}} |
Cyg* | 21h 06m 53.9s +38° 44′ 58″ |
K5.0V | 0.70 | 5.21![]() |
7.49 | 286.0054 +0.0289−{{{2}}} |
First star (besides Sun) to have measured distance. B flare star, with possible planet or brown dwarf. Possible circumstellar disk. |
B (BD+38°4344)$ | 21h 06m 55.3s +38° 44′ 31″ |
K7.0V | 0.63 | 6.03![]() |
8.31 | |||||
Struve 2398 (Gliese 725, BD+59°1915) |
A (HD 173739) | 11.4908 +0.0009−{{{2}}} |
Dra* | 18h 42m 46.7s +59° 37′ 49″ |
M3.0V | 0.334 | 8.90 | 11.16 | 283.8401 +0.0220−{{{2}}} |
flare stars, star B has 2 candidate planets |
B (HD 173740) | 18h 42m 46.9s +59° 37′ 37″ |
M3.5V | 0.248 | 9.69 | 11.95 | |||||
Groombridge 34 (Gliese 15) |
A (GX Andromedae) | 11.6191 +0.0008−{{{2}}} |
And | 00h 18m 22.9s +44° 01′ 23″ |
M1.5V | 0.38 | 8.08 | 10.32 | 280.7068 +0.0203−{{{2}}} |
flare star, two known planets (Ab, 2014, and Ac, 2018) |
B (GQ Andromedae) | M3.5V | 0.15 | 11.06 | 13.30 | flare star | |||||
DX Cancri (G 51-15) | 11.6797 +0.0027−{{{2}}} |
Cnc* | 08h 29m 49.5s +26° 46′ 37″ |
M6.5Ve | 0.09 | 14.78 | 16.98 | 279.2496 +0.0637−{{{2}}} |
flare star | |
Epsilon Indi (CPD−57°10015) |
A$ | 11.8670 +0.0041−{{{2}}} |
Ind* | 22h 03m 21.7s −56° 47′ 10″ |
K5Ve | 0.754 | 4.69![]() |
6.89 | 274.8431 +0.0956−{{{2}}} |
one planet (Ab) (2018) |
Ba§ | 22h 04m 10.5s −56° 46′ 58″ |
T1.0V | 0.065 | 12.3 J | 14.5 J | |||||
Bb§ | T6.0V | 0.050 | 13.2 J | 15.4 J | ||||||
Tau Ceti (BD−16°295)$ | 11.9118 +0.0074−{{{2}}} |
Cet | 01h 44m 04.1s −15° 56′ 15″ |
G8.5Vp | 0.783 | 3.49![]() |
5.68 | 273.8097 +0.1701−{{{2}}} |
one debris disk four confirmed planets (e, f, g, and h) (2012, 2017), four candidate planets (b, c, d, and "i") (2012, 2019) |
|
Gliese 1061 (LHS 1565) | 11.9839 +0.0014−{{{2}}} |
Hor* | 03h 35m 59.7s −44° 30′ 45″ |
M5.5V | 0.113 | 13.09 | 15.26 | 272.1615 +0.0316−{{{2}}} |
has 3 known planets (2019) | |
YZ Ceti (LHS 138) | 12.1222 +0.0015−{{{2}}} |
Cet | 01h 12m 30.6s −16° 59′ 56″ |
M4.5V | 0.130 | 12.02 | 14.17 | 269.0573 +0.0337−{{{2}}} |
flare star, three planets (b, c, and d) (2017) | |
Luyten's Star (BD+05°1668) | 12.3485 +0.0019−{{{2}}} |
CMi | 07h 27m 24.5s +05° 13′ 33″ |
M3.5Vn | 0.26 | 9.86 | 11.97 | 264.1269 +0.0413−{{{2}}} |
two planets (b, c) (2017) and two suspected planets (d, e) (2019) | |
Teegarden's Star (SO025300.5+165258) | 12.4970 +0.0045−{{{2}}} |
Ari* | 02h 53m 00.9s +16° 52′ 53″ |
M6.5V | 0.08 | 15.14 | 17.22 | 260.9884 +0.0934−{{{2}}} |
has 2 known planets (2019) | |
Kapteyn's Star (CD−45°1841) | 12.8308 +0.0008−{{{2}}} |
Pic* | 05h 11m 40.6s −45° 01′ 06″ |
M1.5VI | 0.281 | 8.84 | 10.87 | 254.1986 +0.0168−{{{2}}} |
two refuted planets (b and c) (2014) | |
Lacaille 8760 (AX Microscopii) | 12.9472 +0.0018−{{{2}}} |
Mic* | 21h 17m 15.3s −38° 52′ 03″ |
M0.0V | 0.60 | 6.67 | 8.69 | 251.9124 +0.0352−{{{2}}} |
brightest M dwarf star in night sky, flare star | |
SCR 1845−6357 | A | 13.0638 +0.0070−{{{2}}} |
Pav* | 18h 45m 05.3s −63° 57′ 48″ |
M8.5V | 0.07 | 17.39 | 19.41 | 249.6651 +0.1330−{{{2}}} |
|
B§ | 18h 45m 02.6s −63° 57′ 52″ |
T6 | 0.03 | 13.3 J | 15.3 J | |||||
Kruger 60 (BD+56°2783) |
A | 13.0724 +0.0052−{{{2}}} |
Cep* | 22h 27m 59.5s +57° 41′ 45″ |
M3.0V | 0.271 | 9.79 | 11.76 | 249.5 +0.1−{{{2}}} |
B flare star |
B (DO Cephei) | M4.0V | 0.176 | 11.41 | 13.38 | ||||||
DEN 1048-3956 | 13.1932 +0.0027−{{{2}}} |
Ant* | 10h 48m 14.7s −39° 56′ 06″ |
M8.5V | 0.08 | 17.39 | 19.37 | 247.2156 +0.0512−{{{2}}} |
||
Ross 614 (V577 Monocerotis, Gliese 234) |
A (LHS 1849) | 13.363 +0.040−{{{2}}} |
Mon* | 06h 29m 23.4s −02° 48′ 50″ |
M4.5V | 0.223 | 11.15 | 13.09 | 244.07 +0.73−{{{2}}} |
A flare star |
B (LHS 1850) | M5.5V | 0.111 | 14.23 | 16.17 | ||||||
UGPS J0722-0540§ | 13.43 +0.13−{{{2}}} |
Mon | 07h 22m 27.3s –05° 40′ 30″ |
T9 | 0.010-0.025 | 16.52 J | 18.45 J | 242.8 +2.4−{{{2}}} |
||
Wolf 1061 (Gliese 628, BD−12°4523) | 14.0500 +0.0016−{{{2}}} |
Oph | 16h 30m 18.1s −12° 39′ 45″ |
M3.0V | 0.294 | 10.07 | 11.93 | 232.1390 +0.0268−{{{2}}} |
three planets (b, c, and d) (2015) | |
Van Maanen's star (Gliese 35, LHS 7)![]() |
14.0718 +0.0011−{{{2}}} |
Psc* | 00h 49m 09.9s +05° 23′ 19″ |
DZ7 | 0.67 | 12.38 | 14.21 | 231.7800 +0.0183−{{{2}}} |
closest-known free-floating white dwarf, third-known white dwarf possible debris disk (1917) |
|
Gliese 1 (CD−37°15492) | 14.1747 +0.0022−{{{2}}} |
Scl* | 00h 05m 24.4s −37° 21′ 27″ |
M1.5 V | 0.45-0.48 | 8.55 | 10.35 | 230.0970 +0.0362−{{{2}}} |
||
TZ Arietis (Gliese 83.1, L 1159–16) | 14.5780 +0.0046−{{{2}}} |
Ari | 02h 00m 13.2s +13° 03′ 08″ |
M4.5V | 0.14 | 12.27 | 14.03 | 223.7321 +0.0699−{{{2}}} |
flare star, has one confirmed planet (b) | |
Wolf 424 (FL Virginis, LHS 333, Gliese 473) |
A | 14.595 +0.031−{{{2}}} |
Vir | 12h 33m 17.2s +09° 01′ 15″ |
M5.5Ve | 0.143 | 13.18 | 14.97 | 223.4775 +0.4665−{{{2}}} |
flare stars |
B | M7Ve | 0.131 | 13.17 | 14.96 | ||||||
Gliese 687 (LHS 450, BD+68°946) | 14.8395 +0.0014−{{{2}}} |
Dra | 17h 36m 25.9s +68° 20′ 21″ |
M3.0V | 0.401 | 9.17 | 10.89 | 219.7898 +0.0210−{{{2}}} |
possible flare star, two planets (b) (2014) and (c) (2020) | |
Gliese 674 (LHS 449) | 14.8492 +0.0018−{{{2}}} |
Ara* | 17h 28m 39.9s −46° 53′ 43″ |
M3.0V | 0.35 | 9.38 | 11.09 | 219.6463 +0.0262−{{{2}}} |
one planet (b) (2007) | |
LHS 292 (LP 731-58) | 14.8706 +0.0041−{{{2}}} |
Sex* | 10h 48m 12.6s −11° 20′ 14″ |
M6.5V | 0.08 | 15.60 | 17.32 | 219.3302 +0.0602−{{{2}}} |
flare star | |
Gliese 440 (WD 1142-645, LP 145-141)![]() |
15.1226 +0.0013−{{{2}}} |
Mus* | 11h 45m 42.9s −64° 50′ 29″ |
DQ6 | 0.75 | 11.50 | 13.18 | 215.6753 +0.0181−{{{2}}} |
||
Gliese 1245 | A (G 208-44 A) | 15.2001 +0.0034−{{{2}}} |
Cyg | 19h 53m 54.2s +44° 24′ 55″ |
M5.5V | 0.11 | 13.46 | 15.17 | 214.5745 +0.0476−{{{2}}} |
flare stars |
B (G 208-45) | 19h 53m 55.2s +44° 24′ 56″ |
M6.0V | 0.10 | 14.01 | 15.72 | |||||
C (G 208-44 B) | 19h 53m 54.2s +44° 24′ 55″ |
M5.5 | 0.07 | 16.75 | 18.46 | |||||
WISE 1741+2553§ | 15.22 +0.20−{{{2}}} |
Her* | 17h 41m 24.2s +25° 53′ 19″ |
T9 | 16.53 J | 18.18 J | 214.3 +2.8−{{{2}}} |
|||
Gliese 876 (Ross 780) | 15.2382 +0.0025−{{{2}}} |
Aqr | 22h 53m 16.7s −14° 15′ 49″ |
M3.5V | 0.37 | 10.17 | 11.81 | 214.0380 +0.0356−{{{2}}} |
four planets (d (2005), c (2001), b (1998), and e (2010)) | |
WISE 1639-6847§ | 15.450 +0.041−{{{2}}} |
TrA* | 16h 39m 40.9s -68° 47′ 46″ |
Y0.5 | 20.57 J | 22.10 J | 211.11 +0.56−{{{2}}} |
|||
LHS 288 (Luyten 143-23) | 15.7586 +0.0034−{{{2}}} |
Car | 10h 44m 21.2s −61° 12′ 36″ |
M5.5V | 0.11 | 13.90 | 15.51 | 206.9698 +0.0448−{{{2}}} |
||
Gliese 1002 | 15.8060 +0.0036−{{{2}}} |
Cet | 00h 06m 43.8s −07° 32′ 22″ |
M5.5V | 0.11 | 13.76 | 15.40 | 206.3500 +0.0474−{{{2}}} |
two known planets (b & c, 2022) | |
DEN 0255-4700§ | 15.877 +0.014−{{{2}}} |
Eri | 02h 55m 03.7s −47° 00′ 52″ |
L7.5V | 0.025-0.065 | 22.92 | 24.44 | 205.4251 +0.1857−{{{2}}} |
||
Groombridge 1618 (Gliese 380)$ | 15.8857 +0.0017−{{{2}}} |
UMa | 10h 11m 22.1s +49° 27′ 15″ |
K7.0V | 0.67 | 6.59 | 8.16 | 205.3148 +0.0224−{{{2}}} |
flare star, one suspected debris disk | |
Gliese 412 | A | 15.9969 +0.0026−{{{2}}} |
UMa | 11h 05m 28.6s +43° 31′ 36″ |
M1.0V | 0.48 | 8.77 | 10.34 | 203.8876 +0.0332−{{{2}}} |
|
B (WX Ursae Majoris) | 11h 05m 30.4s +43° 31′ 18″ |
M5.5V | 0.10 | 14.48 | 16.05 | flare star | ||||
AD Leonis | 16.1939 +0.0024−{{{2}}} |
Leo | 10h 19m 36.4s +19° 52′ 10″ |
M3.0V | 0.39-0.42 | 9.32 | 10.87 | 201.4064 +0.0296−{{{2}}} |
flare star, 1 refuted planet (b in 2020) | |
Gliese 832 | 16.2005 +0.0019−{{{2}}} |
Gru* | 21h 33m 34.0s −49° 00′ 32″ |
M1.5 V | 0.45 | 8.66 | 10.20 | 201.3252 +0.0237−{{{2}}} |
possible flare star, two planets; one confirmed (b (2008)), and the other now refuted (c (2014)) | |
Gliese 682 (CD-44 11909) | 16.3328 +0.0026−{{{2}}} |
Sco* | 17h 37m 03.7s –44° 19′ 09″ |
M4 V | 0.27 | 10.95 | 12.45 | 199.6944 +0.0312−{{{2}}} |
has 2 disputed planets | |
Omicron2 Eridani (40 Eridani, Gliese 166) |
Keid (A)$ | 16.3330 +0.0042−{{{2}}} |
Eri | 04h 15m 16.3s -07° 39′ 10″ |
K0.5 V | 0.84 | 4.43![]() |
5.93 | 199.6911 +0.0512−{{{2}}} |
has 1 known planet |
B![]() |
04h 15m 21.8s −07° 39′ 29″ |
DA4 | 0.573 | 9.52 | 11.02 | |||||
C | 04h 15m 21.5s −07° 39′ 22″ |
M4 V | 0.2036 | 11.24 | 12.74 | |||||
EV Lacertae | 16.4761 +0.0018−{{{2}}} |
Lac* | 22h 46m 49.7s +44° 20′ 02″ |
M3.5 V | 0.35 | 10.22 | 11.70 | 197.9573 +0.0220−{{{2}}} |
record setting stellar flare observed | |
70 Ophiuchi (Gliese 702) | A$ | 16.7074 +0.0087−{{{2}}} |
Oph | 18h 05m 27.4s +02° 29′ 59″ |
K0 V | 0.90 | 4.21![]() |
5.66 | 195.2166 +0.1012−{{{2}}} |
|
B$ | 18h 05m 27.5s +02° 29′ 56″ |
K5 V | 0.70 | 6.01![]() |
7.46 | |||||
Altair (Alpha Aquilae)$ | 16.730 +0.049−{{{2}}} |
Aql* | 19h 50m 47.0s +08° 52′ 06″ |
A7 IV-Vn | 1.79 | 0.77![]() |
2.22 | 194.95 +0.57−{{{2}}} |
||
EI Cancri (GJ 1116, G 9-38) | A | 16.800 +0.011−{{{2}}} |
Cnc | 08h 58m 15.2s +19° 45′ 47″ |
M5.5 V | 0.12 | 14.06 | 15.50 | 194.1443 +0.1228−{{{2}}} |
|
B | M V | 0.10 | 14.92 | 16.36 | ||||||
WISE J150649.97+702736.1§ | 16.856 +0.052−{{{2}}} |
UMi* | 15h 06m 52.4s +70° 27′ 25″ |
T6 | 13.74 J | 15.17 J | 193.5 +0.6−{{{2}}} |
|||
GJ 3379 (G 99-49) | 16.9861 +0.0027−{{{2}}} |
Ori* | 06h 00m 03.5s +02° 42′ 24″ |
M3.5 V | 0.2312 | 11.31 | 12.73 | 192.0135 +0.0310−{{{2}}} |
||
DENIS J081730.0-615520§ | 17.002 +0.037−{{{2}}} |
Car | 08h 17m 30.1s −61° 55′ 16″ |
T6 | 0.015 | 13.61 J | 15.03 J | 191.8362 +0.4186−{{{2}}} |
||
Gliese 445 (LHS 2459, G 254-29) | 17.1368 +0.0017−{{{2}}} |
Cam* | 11h 47m 41.4s +78° 41′ 28″ |
M3.5 V | 0.14 | 10.79 | 12.19 | 190.3251 +0.0194−{{{2}}} |
||
2MASS J15404342−5101357 | 17.3738 +0.0046−{{{2}}} |
Nor* | 15h 40m 43.5s -51° 01′ 36″ |
M7 V | 0.090 | 15.26 | 16.63 | 187.7290 +0.0496−{{{2}}} |
||
2MASS 0939−2448 | A§ | 17.41 +0.44−{{{2}}} |
Ant | 09h 39m 35.5s −24° 48′ 28″ |
T8 V | 0.019–0.048 | 15.61 J | 16.97 J | 187.3 +4.6−{{{2}}} |
binary brown dwarf |
B§ | T8 V | 0.019–0.038 | ||||||||
Gliese 3323 (LHS 1723, LP 656-38) | 17.5309 +0.0026−{{{2}}} |
Eri | 05h 01m 57.4s −06° 56′ 46″ |
M4 V | 0.1705 | 12.22 | 13.57 | 186.0466 +0.0277−{{{2}}} |
has 2 known planets | |
Gliese 526 (Wolf 498, HD 119850) | 17.7263 +0.0024−{{{2}}} |
Boo* | 13h 45m 43.8s +14° 53′ 29″ |
M1 V | 0.28 | 8.46 | 9.78 | 183.9962 +0.0253−{{{2}}} |
||
Stein 2051 (Gliese 169.1, G 175-34) | A | 17.9925 +0.0020−{{{2}}} |
Cam | 04h 31m 11.5s +58° 58′ 37″ |
M4 V | 0.252 | 11.04 | 12.33 | 181.2730 +0.0203−{{{2}}} |
|
B![]() |
04h 31m 12.6s +58° 58′ 41″ |
DC5 | 0.675 | 12.43 | 13.72 | |||||
WISEP J111448.80-261828.2§ | 18.20 +0.14−{{{2}}} |
Hya | 11h 14m 51.3s −26° 18′ 24″ |
T7.5 | 0.029–0.048 | 15.86 J | 17.12 J | 179.2 +1.4−{{{2}}} |
||
Gliese 251 (Wolf 294, HD 265866) | 18.2146 +0.0028−{{{2}}} |
Gem* | 06h 54m 49.0s +33° 16′ 05″ |
M3 V | 0.360 | 10.02 | 11.29 | 179.0629 +0.0280−{{{2}}} |
has 1 known planet | |
LP 816-60 | 18.3305 +0.0038−{{{2}}} |
Cap* | 20h 52m 33.0s -16° 58′ 29″ |
M3.5 V | 0.224 | 11.50 | 12.75 | 177.9312 +0.0365−{{{2}}} |
||
WISE 0350−5658§ | 18.49 +0.24−{{{2}}} |
Ret* | 03h 50m 00.3s -56° 58′ 30″ |
Y1 | 22.47 J | 23.70 J | 176.4 +2.3−{{{2}}} |
|||
WISEA J183537.82+325945.4 | 18.5534 +0.0049−{{{2}}} |
Lyr* | 18h 35m 37.9s +32° 59′ 55″ |
M8.5 V | 0.053 | 18.27 | 19.50 | 175.7930 +0.0468−{{{2}}} |
||
Gliese 205 (Wolf 1453, HD 36395) | 18.6042 +0.0022−{{{2}}} |
Ori | 05h 31m 27.4s −03° 40′ 38″ |
M1 V | 0.556 | 7.95 | 9.17 | 175.3131 +0.0204−{{{2}}} |
has 2 candidate planets | |
WISE J041521.21-093500.6§ | 18.62 +0.18−{{{2}}} |
Eri | 04h 15m 19.5s −09° 35′ 07″ |
T8 | 0.03 | 15.34 J | 16.56 J | 175.2 +1.7−{{{2}}} |
||
Gliese 229 (HD 42581) | A | 18.7906 +0.0018−{{{2}}} |
Lep* | 06h 10m 34.6s −21° 51′ 53″ |
M1.5 V | 0.579 | 8.14 | 9.34 | 173.5740 +0.0170−{{{2}}} |
has 2 known planets |
B§ | T6 V | 0.058 | 14.01 J | 15.21 J | ||||||
Alsafi (Sigma Draconis)$ | 18.7993 +0.0081−{{{2}}} |
Dra | 19h 32m 21.6s +69° 39′ 40″ |
G9 V | 0.85 | 4.67![]() |
5.87 | 173.4939 +0.0748−{{{2}}} |
||
Ross 47 (Gliese 213) | 18.8883 +0.0031−{{{2}}} |
Ori | 05h 42m 09.3s +12° 29′ 21″ |
M4 V | 0.35 | 11.57 | 12.76 | 172.6762 +0.0286−{{{2}}} |
||
Gliese 570 (Lalande 27173, 33 G. Librae) |
A$ | 19.1987 +0.0074−{{{2}}} |
Lib* | 14h 57m 28.0s -21° 24′ 56″ |
K4 V | 0.802 | 5.64![]() |
6.79 | 169.8843 +0.0653−{{{2}}} |
|
B | M1.5 V | 0.55 | 8.30 | 9.45 | ||||||
C | M | 0.35 | 9.96 | 11.11 | ||||||
D§ | T7.5 | 0.05 | 15.32 J | 16.47 J | ||||||
Gliese 693 (Luyten 205–128) | 19.2078 +0.0053−{{{2}}} |
Pav | 17h 46m 32.4s -57° 19′ 09″ |
M3 V | 0.26 | 10.76 | 11.91 | 169.8042 +0.0465−{{{2}}} |
||
Gliese 754 (Luyten 347–14) | 19.2724 +0.0067−{{{2}}} |
Tel* | 19h 20m 48.0s −45° 33′ 30″ |
M4 V | 0.173 | 12.23 | 13.37 | 169.2351 +0.0588−{{{2}}} |
has 1 candidate planet | |
Gliese 908 (Lalande 46650, BR Piscium) | 19.2745 +0.0032−{{{2}}} |
Psc | 23h 49m 12.5s +02° 24′ 04″ |
M1 V | 0.37 | 8.98 | 10.12 | 169.2163 +0.0281−{{{2}}} |
||
Gliese 752 (Wolf 1055, HD 180617) | A | 19.2922 +0.0027−{{{2}}} |
Aql | 19h 16m 55.3s +05° 10′ 08″ |
M2.5 V | 0.46 | 9.10 | 10.24 | 169.0615 +0.0239−{{{2}}} |
has 1 known planet |
B (VB 10) | 19h 16m 57.6s +05° 09′ 02″ |
M8 V | 0.075 | 17.45 | 18.59 | very small and very dim red dwarf | ||||
Gliese 588 (CD-40 9712) | 19.2996 +0.0031−{{{2}}} |
Lup* | 15h 32m 12.9s -41° 16′ 32″ |
M2.5 V | 0.43 | 9.31 | 10.45 | 168.9965 +0.0270−{{{2}}} |
has 2 candidate planets | |
Eta Cassiopeiae (Gliese 34) | Achird (A)$ | 19.3314 +0.0025−{{{2}}} |
Cas* | 00h 49m 06.3s +57° 48′ 55″ |
G3 V | 0.972 | 3.46![]() |
4.60 | 168.7186 +0.0216−{{{2}}} |
|
B | K7 V | 0.57 | 7.51 | 8.65 | ||||||
36 Ophiuchi (Gliese 663) | Guniibuu (A)$ | 19.4185 +0.0036−{{{2}}} |
Oph | 17h 15m 20.9s -26° 36′ 09″ |
K1.5 V | 0.85 | 5.07![]() |
6.20 | 167.9617 +0.0311−{{{2}}} |
|
B$ | 17h 15m 21.0s -26° 36′ 10″ |
K1 V | 0.85 | 5.08![]() |
6.21 | |||||
C$ | 17h 16m 13.4s -26° 32′ 46″ |
K5 V | 0.71 | 6.32![]() |
7.45 | |||||
YZ Canis Minoris (Ross 882, Gliese 285) | 19.5330 +0.0040−{{{2}}} |
CMi | 07h 44m 40.2s +03° 33′ 09″ |
M4 V | 0.308 | 11.19 | 12.30 | 166.9769 +0.0343−{{{2}}} |
||
WISE 1541−2250§ | 19.54 +0.24−{{{2}}} |
Lib | 15h 41m 51.6s −22° 50′ 25″ |
Y0.5 | 0.011 | 20.99 J | 22.10 J | 166.9 +2.0−{{{2}}} |
||
GJ 1005 (Luyten 722-22, G 158-50) | A | 19.577 +0.035−{{{2}}} |
Cet | 00h 15m 28.1s -16° 08′ 02″ |
M3.5 V | 0.179 | 11.60 | 12.71 | 166.6 +0.3−{{{2}}} |
distance uncertain: 16.28±0.75, 17.91±0.67, 17.0±1.5, 16.26±0.76, 17.26, 19.695±0.095 ly |
B | M V | 0.112 | 14.02 | 15.13 | ||||||
HR 7703 (279 G. Sagittarii, HD 191408, Gliese 783, IRAS 20079-3614) | A$ | 19.609 +0.013−{{{2}}} |
Sgr | 20h 11m 11.93s –36° 06′ 04″ |
K2.5 V | 0.65 | 5.31![]() |
6.41 | 166.3272 +0.1065−{{{2}}} |
|
B | M4 V | 0.24 | 11.50 | 12.60 | ||||||
82 G. Eridani (e Eridani, Gliese 139, HD 20794)$ | 19.7045 +0.0093−{{{2}}} |
Eri | 03h 19m 55.7s −43° 04′ 11″ |
G8 V | 0.70 | 4.26![]() |
5.35 | 165.5242 +0.0784−{{{2}}} |
has 3 confirmed planets, 3 candidate planets, hot and cold dust disks | |
Gliese 268 (Ross 986, QY Aurigae) | A | 19.7414 +0.0076−{{{2}}} |
Aur* | 07h 10m 01.8s 38° 31′ 46″ |
M4.5 V | 0.226 | 12.05 | 13.14 | 165.2147 +0.0636−{{{2}}} |
|
B | M V | 0.192 | 12.45 | 13.54 | ||||||
Delta Pavonis$ | 19.893 +0.015−{{{2}}} |
Pav | 20h 08m 43.6s −66° 10′ 55″ |
G8 IV | 1.051 | 3.55![]() |
4.62 | 163.9544 +0.1222−{{{2}}} |
has 1 candidate planet | |
SIMP0136§ | 19.955 +0.057−{{{2}}} |
Psc | 01h 36m 56.5s +09° 33′ 47″ |
T2.5 | 0.012 | 13.25 J | 14.32 J | 163.4478 +0.4629−{{{2}}} |
rogue planet, 12.7 MJ | |
2MASS 0937+2931§ | 19.96 +0.22−{{{2}}} |
Leo | 09h 37m 34.9s 29° 31′ 41″ |
T7 | 0.040 | 14.65 J | 15.71 J | 163.39 +1.76−{{{2}}} |
||
System | Star or (sub-) brown dwarf | Distance (ly (±err)) |
Coordinates: RA, Dec (Ep J2000, Eq J2000) |
Stellar class |
Mass M☉ |
App. | Abs. | Parallax (mas (±err)) |
Notes and additional references |
|
Designation | Magnitude (mV or mJ) |
Stars Visiting Our Neighborhood
Over long periods, stars slowly move through space. This changes their positions and distances from our Sun. Scientists can predict these movements using very precise measurements. They use how much a star seems to shift (parallax), how much it moves across the sky (proper motion), and how fast it moves towards or away from us (radial velocities). While these predictions are helpful, they become less accurate over extremely long times.
One star that is known to have come very close to the Sun is Gliese 710. This star is about half the size of our Sun. It is currently 62 light-years away. In 1999, data from the Hipparcos satellite first showed that it would pass less than 1.3 light-years from the Sun in about 1.4 million years. More recent observations from the Gaia telescope have made this prediction even more precise. It's now thought that Gliese 710 will pass much closer, about 0.178 light-years away. This is close enough to significantly disturb the Oort cloud, which is a huge, distant cloud of icy objects surrounding our Solar System.
The latest data from the Gaia telescope has given us updated information for many of the stars listed below.
Star name | HIP number |
Minimum distance (light-years) |
Date of approach in thousands of years |
Current distance (light-years) |
Stellar classification | Mass in M☉ | Current apparent magnitude |
Current Constellation | Current Right ascension |
Current Declination |
---|---|---|---|---|---|---|---|---|---|---|
Gliese 710 | 89825 | 0.167±0.012 | 1296+24 −23 |
62.248±0.020 | K7V | 0.4–0.6 | 9.6 | Serpens | 18h 19m 50.843s | −01° 56′ 18.98″ |
HD 7977 | N/A | 0.478+0.104 −0.078 |
−2764+28 −29 |
246.74±0.60 | G0V | ~1.2 | 9.04 | Cassiopeia | 01h 20m 31.597s | +61° 52′ 57.08″ |
Scholz's Star and companion brown dwarf | N/A | 0.82+0.37 −0.22 |
−78.5±0.7 | 22.2±0.2 | A: M9V B: T5 |
A: 0.095 B: 0.063 |
18.3 | Monoceros | 07h 20m 03.20s | -08° 46′ 51.2″ |
2MASS J0628+1845 | N/A | 1.61+0.28 −0.24 |
1720+150 −130 |
272.28±0.80 | M2.5V | 0.28 | 16.2 | Gemini | 06h 28m 11.593s | +18° 45′ 12.91″ |
2MASS J0805+4624 | N/A | 1.610+0.099 −0.092 |
−363+13 −14 |
238.1±1.0 | M3V | 0.25 | 17.0 | Lynx | 08h 05m 29.038s | +46° 24′ 51.78″ |
CD-69 2001 | N/A | 1.616+0.070 −0.068 |
−1907±10 | 332.61±0.55 | K4V | 0.61 | 11.13 | Indus | 21h 40m 31.514s | -69° 25′ 14.58″ |
HD 49995 | N/A | 1.70+0.23 −0.20 |
−4034+94 −98 |
439.74±0.59 | A: F3V B: M1V |
A: 1.48 B: 0.49 |
8.78 | Canis Major | 06h 50m 20.810s | -18° 37′ 30.58″ |
2MASS J0621-0101 | N/A | 1.71+0.46 −0.39 |
−3206+68 −66 |
428.8±3.1 | G5V | 0.96 | 11.9 | Orion | 06h 21m 34.807s | -01° 01′ 55.01″ |
LSPM J2146+3813 | N/A | 1.8557±0.0048 | 84.59±0.19 | 22.9858±0.0034 | M5V | ~0.15 | 10.82 | Cygnus | 21h 46m 22.285s | +38° 13′ 03.12″ |
2MASS J0455+1144 | N/A | 1.94+0.16 −0.15 |
1702+58 −54 |
349.50±0.80 | M0V | 0.50 | 15.3 | Orion | 04h 55m 21.427s | +11° 44′ 41.25″ |
2MASS J0734-0637 | N/A | 1.950±0.021 | −554.6±3.3 | 130.66±0.12 | M0V | 0.50 | 12.9 | Monoceros | 07h 34m 39.097s | -06° 37′ 12.21″ |
2MASS J1151-0313 | N/A | 1.98+0.20 −0.18 |
1017+60 −54 |
125.88±0.41 | M3.5V | 0.23 | 15.3 | Virgo | 11h 51m 37.434s | -03° 13′ 45.24″ |
UCAC4 076–006432 | N/A | 2.042+0.034 −0.033 |
−893.8+7.9 −8.0 |
212.41±0.15 | mid K | ~0.6 | 12.69 | Mensa | 06h 34m 29.385s | -74° 49′ 47.12″ |
2MASS J0120+4739 | N/A | 2.25+0.17 −0.15 |
473+27 −25 |
237.56±0.66 | M3.5V | 0.25 | 16.5 | Andromeda | 01h 20m 04.561s | +47° 39′ 46.56″ |
TYC 6760–1510–1 | N/A | 2.46+0.19 −0.18 |
−1708+44 −47 |
102.89±0.16 | M1.5V | 0.58 | 11.5 | Hydra | 15h 00m 09.536s | -29° 05′ 27.67″ |
UCAC2 15719371 | N/A | 2.46±0.10 | −4282+70 −73 |
280.80±0.26 | K4V | 0.66 | 12.58 | Antlia | 09h 44m 09.884s | -37° 45′ 31.09″ |
TYC 1662–1962–1 | N/A | 2.637+0.055 −0.054 |
−1536.6+9.0 −9.1 |
286.51±0.40 | Early K | ~0.8 | 10.95 | Vulpecula | 21h 14m 32.911s | +21° 53′ 32.76″ |
HD 179939 | 94512 | 2.65±0.17 | 3020±25 | 334.32±0.88 | A3V | 1.7 | 7.23 | Aquila | 19h 14m 10.043s | +07° 45′ 50.72″ |
BD-21 1529 | N/A | 2.701+0.059 −0.058 |
−1660.1±6.3 | 368.48±0.56 | G5V | ~0.95 | 9.67 | Canis Major | 06h 37m 48.004s | -21° 22′ 21.94″ |
2MASS J1310-1307 | N/A | 2.79+0.59 −0.47 |
−1520+150 −190 |
433.0±2.6 | M2.5V | 0.34 | 16.3 | Virgo | 13h 10m 30.804s | -13° 07′ 33.55″ |
UPM J1121-5549 | N/A | 2.803±0.020 | −282.5+1.6 −1.7 |
72.498±0.029 | M3V | 0.29 | 13.5 | Centaurus | 11h 21m 18.136s | -55° 49′ 17.77″ |
UCAC4 464–006057 | N/A | 2.812+0.052 −0.051 |
932±11 | 101.570±0.086 | Early M | ~0.4 | 11.73 | Taurus | 04h 09m 02.050s | +02° 45′ 38.32″ |
UCAC4 213–008644 | N/A | 2.91+0.13 −0.12 |
−306+12 −13 |
80.987±0.048 | M5.0 | 0.17 | 16.4 | Puppis | 06h 21m 54.714s | -47° 25′ 31.33″ |
Gliese 3649 | N/A | 3.016±0.024 | −520.4±3.1 | 54.435±0.023 | M1 | 0.49 | 10.85 | Leo | 11h 12m 38.97s | +18° 56′ 05.4″ |
Ross 248 | N/A | 3.0446±0.0077 | 38.500±0.096 | 10.3057±0.0014 | M6V | 0.136 | 12.29 | Andromeda | 23h 41m 54.99s | +44° 10′ 40.8″ |
2MASS J1921-1244 | N/A | 3.08+0.21 −0.19 |
−3490+120 −130 |
376.46±0.73 | K6V | 0.69 | 12.46 | Sagittarius | 19h 21m 58.124s | -12° 43′ 58.61″ |
Proxima Centauri | 70890 | 3.123±0.015 | 28.65±0.27 | 4.24646±0.00028 | M5Ve | 0.15 | 11.05 | Centaurus | 14h 29m 42.949s | −62° 40′ 46.14″ |
TYC 9387–2515–1 | N/A | 3.220+0.081 −0.079 |
−1509.1+8.6 −8.7 |
401.96±0.54 | K1V | 0.86 | 11.45 | Mensa | 06h 18m 54.643s | -80° 19′ 16.54″ |
Alpha Centauri AB | A: 71683 B: 71685 |
3.242±0.060 | 29.63+1.00 −0.98 |
4.321±0.024 | A: G2V B: K1V |
A: 1.100 B: 0.907 |
A: -0.01 B: +1.33 |
Centaurus | 14h 39m 36.495s | −60° 50′ 02.31″ |
Gliese 445 | 57544 | 3.3400±0.0051 | 46.341±0.065 | 17.1368±0.0017 | M4 | 0.15? | 10.8 | Camelopardalis | 11h 47m 41.377s | +78° 41′ 28.18″ |
2MASS J1638-6355 | N/A | 3.37+0.29 −0.28 |
−1428+21 −22 |
468.5±4.2 | K2V | 0.82 | 12.44 | Triangulum Australe | 16h 38m 21.759s | -63° 55′ 13.16″ |
2MASS J0542+3217 | N/A | 3.43+0.75 −0.71 |
5823+89 −87 |
884.6±2.4 | A: G4V B: K0V |
A: 1.01 B: 0.85 |
12.80 | Auriga | 05h 42m 38.349s | +32° 17′ 29.85″ |
2MASS J0625-2408 | N/A | 3.700+0.082 −0.080 |
−1874±14 | 534.88±0.93 | K/M | ~0.5 | 12.91 | Canis Major | 06h 25m 42.744s | -24° 08′ 35.02″ |
Barnard's Star | 87937 | 3.7682±0.0031 | 11.735±0.013 | 5.96290±0.00044 | sdM4 | 0.144 | 9.54 | Ophiuchus | 17h 57m 48.498s | +04° 41′ 36.25″ |
BD+05 1792 | N/A | 3.965±0.040 | −962.7±3.0 | 239.73±0.33 | G2V | 1.07 | 8.58 | Gemini | 07h 48m 07.037s | +05° 27′ 22.51″ |
2MASS J2241-2759 | N/A | 4.05±0.16 | −2810+37 −38 |
411.06±0.76 | K7V | ~0.5 | 12.28 | Piscis Austrinus | 22h 41m 50.996s | -27° 59′ 47.04″ |
2MASS J1724-0522 | N/A | 4.15+0.26 −0.25 |
3058+54 −52 |
489.5±1.3 | K0V | 0.86 | 12.73 | Ophiuchus | 17h 24m 55.056s | -05° 22′ 11.45″ |
StKM 1–554 | N/A | 4.217+0.036 −0.035 |
−549.9+2.9 −3.0 |
151.97±0.19 | M0V | 0.65 | 12.17 | Orion | 05h 14m 01.871s | +05° 22′ 56.26″ |
Gliese 3379 | N/A | 4.227±0.024 | −157.43+0.93 −0.94 |
16.9861±0.0027 | M3.5V | 0.19 | 11.31 | Orion | 06h 00m 03.824s | +02° 42′ 22.97″ |
2MASS J1936+3627 | N/A | 4.23+0.62 −0.57 |
3830+120 −110 |
671.6±3.4 | G5.5V | 0.95 | 12.2 | Cygnus | 19h 36m 57.294s | +36° 27′ 57.71″ |
2MASS J0710+5228 | N/A | 4.303±0.039 | 507.6+3.8 −3.7 |
90.949±0.050 | M3V | 0.33 | 12.52 | Lynx | 07h 10m 52.167s | +52° 28′ 18.49″ |
HD 146248 | N/A | 4.341+0.040 −0.039 |
−1141.5±3.7 | 334.87±0.47 | G2/3IV | 1.23 | 9.47 | Triangulum Australe | 16h 19m 27.875s | -64° 50′ 34.38″ |
2MASS J1724+0355 | N/A | 4.37±0.12 | 1991+38 −37 |
254.99±0.26 | G8V | 0.85 | 12.54 | Ophiuchus | 17h 24m 34.633s | +03° 55′ 26.75″ |
StKM 1–1456 | N/A | 4.396±0.043 | 1240.2+6.9 −6.8 |
144.934±0.095 | A: K5V B: M8V |
A: 0.81 B: 0.09 |
10.58 | Hercules | 17h 17m 31.118s | +15° 34′ 55.35″ |
Zeta Leporis | 27288 | 4.43+0.33 −0.30 |
−878+42 −46 |
72.81±0.40 | A2Vann | 2.0 | 3.55 | Lepus | 05h 46m 57.341s | −14° 49′ 19.02″ |
Lalande 21185 | 54035 | 4.6807±0.0055 | 21.973±0.033 | 8.30437±0.00068 | M2V | 0.39 | 7.52 | Ursa Major | 11h 03m 20.194s | +35° 58′ 11.55″ |
HD 68814 | 40317 | 4.724+0.090 −0.089 |
−2242±13 | 259.85±0.30 | G6V | 0.98 | 9.57 | Hydra | 08h 13m 57.112s | -04° 03′ 12.56″ |
2MASS J1941-4602 | N/A | 4.814+0.050 −0.049 |
−456.5+4.1 −4.2 |
66.848±0.033 | M4-M6 | ~0.15 | 12.4 | Telescopium | 19h 41m 53.18s | -46° 02′ 31.4″ |
Images for kids
See also
In Spanish: Anexo:Estrellas más cercanas para niños
- Interstellar travel
- Location of Earth
- The Magnificent Seven
- Nearby Stars Database
- Solar System#Galactic context
- Stars and planetary systems in fiction
Related lists
- List of stars with resolved images
- List of brightest stars
- List of star systems within 20–25 light-years
- List of star systems within 25–30 light-years
- List of star systems within 30–35 light-years
- List of star systems within 35–40 light-years
- List of star systems within 40–45 light-years
- List of star systems within 45–50 light-years
- List of nearest bright stars
- Historical brightest stars
- List of nearest exoplanets
- List of nearest terrestrial exoplanet candidates
- List of nearest free floating planetary mass objects
- List of nearby stellar associations and moving groups
- List of star-forming regions in the Local Group
- Lists of stars
- List of Solar System objects by greatest aphelion
- List of trans-Neptunian objects
- List of nearest known black holes