alt=Rotating 3D image of the nearest stars|300px|thumb|upright=2|Animated 3D map of the nearest stars, centered on the Sun.
300px|thumb|upright=2|A radar map of all known stellar and [[substellar objects within 9 light years (ly), arranged clockwise in hours of right ascension, and marked by distance (▬) and position (◆). Distances are marked outward from the Sun (Sol), with concentric circles indicating the distance in one ly steps. Positions are marked inward from their distance markings, connected by lines according to their declinations (dotted when positive), representing the arcs of the declinations viewed edge-on. For within 12 ly see this map.]]
<!-- Current distances (first table) -->
This list covers all known stars, white dwarfs, brown dwarfs, and sub-brown dwarfs/rogue planets within of the Sun. So far, 131 such objects have been found. Only 22 are bright enough to be visible without a telescope, for which the star's visible light needs to reach or exceed the dimmest brightness visible to the naked eye from Earth, which is typically around 6.5 apparent magnitude.
The known 131 objects are bound in 94 stellar systems. Of those, 103 are main sequence stars: 80 red dwarfs and 23 "typical" stars having greater mass. Additionally, astronomers have found 6 white dwarfs (stars that have exhausted all fusible hydrogen), 21 brown dwarfs, as well as 1 sub-brown dwarf, WISE 0855−0714 (possibly a rogue planet). The closest system is Alpha Centauri, with Proxima Centauri as the closest star in that system, at 4.2465 light-years from Earth. The brightest, most massive and most luminous object among those 131 is Sirius A, which is also the brightest star in Earth's night sky; its white dwarf companion Sirius B is the hottest object among them. The largest object within 20 light-years is Procyon.
The Solar System, and the other stars/dwarfs listed here, are currently moving within (or near) the Local Interstellar Cloud, roughly across. The Local Interstellar Cloud is, in turn, contained inside the Local Bubble, a cavity in the interstellar medium about across. It contains Ursa Major and the Hyades star cluster, among others. The Local Bubble also contains the neighboring G-Cloud, which contains the stars Alpha Centauri and Altair. In the galactic context, the Local Bubble is a small part of the Orion Arm, which contains most stars that we can see without a telescope. The Orion Arm is one of the spiral arms of our Milky Way galaxy.
Astrometrics
<!-- Notes on methodology -->
The easiest way to determine stellar distance to the Sun for objects at these distances is parallax, which measures how much stars appear to move against background objects over the course of Earth's orbit around the Sun. As a parsec (parallax-second) is defined by the distance of an object that would appear to move exactly one second of arc against background objects, stars less than 5 parsecs away will have measured parallaxes of over 0.2 arcseconds, or 200 milliarcseconds. Determining past and future positions relies on accurate astrometric measurements of their parallax and total proper motions (how far they move across the sky due to their actual velocity relative to the Sun), along with spectroscopically determined radial velocities (their speed directly towards or away from us, which combined with proper motion defines their true movement through the sky relative to the Sun). Both of these measurements are subject to increasing and significant errors over very long time spans, especially over the several thousand-year time spans it takes for stars to noticeably move relative to each other.
<!-- Past/Future distances (second table) -->
Based on results from the Gaia telescope's second data release from April 2018, an estimated 694 stars will approach the Solar System to less than 5 parsecs in the next 15 million years. Of these, 26 have a good probability to come within and another 7 within . This number is likely much higher, due to the sheer number of stars needed to be surveyed; a star approaching the Solar System 10 million years ago, moving at a typical Sun-relative 20–200 kilometers per second, would be 600–6,000 light-years from the Sun at present day, with millions of stars closer to the Sun. The closest encounter to the Sun so far predicted is the low-mass orange dwarf star Gliese 710 / HIP 89825 with roughly 60% the mass of the Sun. It is currently predicted to pass ( au) from the Sun in million years from the present, close enough to significantly disturb the Solar System's Oort cloud.
thumb|upright=1.3|Stars within .
thumb|upright=1.3|Stars and star systems within .
thumb|upright=1.6|[[Hipparcos luminous stars distances map within . The number in square brackets is height above or below the galactic plane. The distance between stars is colour coded:
< 25 pc: green
< 50 pc: cyan
< 75 pc: yellow
< 100 pc: orange]]
List
<!--PLEASE NOTE: The various values for the stars, to preserve one's ability to sort various parts of the table, will be organized as such:
- /distance/system/star: no sort
stellar class: 3-digit 0-padded spectral type in intervals of 10: A0 = 000, A5 = 005, F5 = 015, etc.
A0 = 000, F0 = 010, G0 = 020, K0 = 030, M0 = 040, L0 = 050, T0 = 060, Y0 = 070, D0 = 080
apparent magnitude/absolute magnitude: 2-digit 0-padded value.
-->
{| class="wikitable"
|+Key
|-
| style="background-color: lightblue"|
|Visible to the unaided eye (apparent magnitude of +6.5 or brighter)
|-
| style="background-color: lightgreen"|
|Luminous star (absolute magnitude of +8.5 or brighter)
|-
| style="background-color:#F5F5DC"|
|White dwarf
|-
| style="background-color:#D8BD98"| §
|Brown dwarf
|-
| style="background-color:#C67B30"|
|Sub-brown dwarf or rogue planet
|-
| style="background-color: pink"|
|Nearest in constellation
|}
The classes of the stars and brown dwarfs are shown in the color of their spectral types (these colors are derived from conventional names for the spectral types and do not necessarily represent the star's observed color). Many brown dwarfs are not listed by visual magnitude but are listed by near-infrared J band apparent magnitude due to how dim (and often invisible) they are in visible color bands (U, B or V). Absolute magnitude (with electromagnetic wave, 'light' band denoted in subscript) is a measurement at a 10-parsec distance across imaginary empty space devoid of all its sparse dust and gas. Some of the parallaxes and resultant distances are rough measurements.
{| class="wikitable mw-datatable sortable sort-under mw-collapsible sticky-header-multi" style="font-size:100%"
|+ Known systems within
! class="unsortable" colspan="2" | Designation
! rowspan="2" data-sort-type="number" | Distance|(ly)
! rowspan="2" | Constellation|
! rowspan="2" | RA/Dec(mas)
! rowspan="2" | Notes and additional references
|-
! class="unsortable" | System
! class="unsortable" | Name
! data-sort-type="number" | App.
! data-sort-type="number" | Abs.
|-
| Solar System
| style="background-color: lightgreen" | Sun (Sol)
| 0.0000158
|
|
| style="background: ;" | G2V
| flare star, two confirmed planets (b, 2016 and d, 2025) and a candidate planet (c, 2019)
|-
| style="background-color: lightgreen" | Rigil Kentaurus (A)
| rowspan="2" | 4.3441
|
| style="background: ;" | G2V
| one directly imaged habitable-zone planet candidate (Alpha Centauri Ab) (2021)
|-
| style="background-color: lightgreen" | Toliman (B)
|
| style="background: ;" | K1V four confirmed planets (d, b, c, and e)
|-
| rowspan="2" | Luhman 16(WISE 1049−5319)
| style="background: #D8BD98"| A§
| rowspan="2" | 6.5029
| rowspan="2" style="background-color: pink" | Vel
| rowspan="2" |
| style="background: ;" | L8±1
|0.032
| 10.7 J
| 14.2 J
| rowspan="2" | 501.557
| rowspan="2" | nearest brown dwarfs
|-
| style="background: #D8BD98" | B§
| style="background: ;" | T1±2
|-
| colspan="2" | Lalande 21185 (BD+36°2147, Gliese 411, HD 95735)
| 8.3044
| style="background-color: pink" | UMa
|
| style="background: ;" | M2.0V
|-
| rowspan="2" | Sirius (Alpha Canis Majoris)
| style="background-color: lightgreen" | A
| rowspan="2" | 8.7094
| rowspan="2" style="background-color: pink" | CMa
| rowspan="2" |
| style="background: " | A1V
|-
| B (UV Ceti)
| style="background: ;" | M6.0Ve
|0.100
| 12.99
| 15.85
|-
| colspan="2" | Ross 154 (V1216 Sagittarii)
| 9.7063
| style="background-color: pink" | Sgr
|
| style="background: ;" | M3.5Ve
|0.17
| 10.43
| 13.07
| 336.0266
| three circumstellar disks,one confirmed planet (AEgir, 2000) and one candidate (c, 2002)
|-
| colspan="2" | Lacaille 9352 (Gliese 887)
| 10.7241
| style="background-color: pink" | PsA
|
| style="background: ;" | M0.5V
|0.486
| 7.34
| 9.75
| 304.1354 four planets, b, c, d, and e with equivocal evidence for a fifth in the inner system as well as a possible outer giant.
|-
| colspan="2" | Ross 128 (FI Virginis)
| 11.0074
| style="background-color: pink" | Vir
|
| style="background: ;" | M4.0Vn
|0.168
| 11.13
| 13.51
| 296.3053
|-
| rowspan="3" | EZ Aquarii(Gliese 866, Luyten 789-6)
| A
| rowspan="3" | 11.109
| rowspan="3" style="background-color: pink" | Aqr
| rowspan="3" |
| style="background: ;" | M5.0Ve
|0.11
| 13.33
| 15.64
| rowspan="3" | 293.60
| rowspan="3" | A & B flare stars
|-
| B
| style="background: ;" | M?
|0.11
| 13.27
| 15.58
|-
| C
| style="background: ;" | M?
|0.10
| 14.03
| 16.34
|-
| rowspan="2" | 61 Cygni
| style="background-color: lightgreen" | A (BD+38°4343)
| rowspan="2" | 11.4039
| rowspan="2" style="background-color: pink" | Cyg
|
| style="background: ;" | K5.0VB flare star, with possible planet or brown dwarf.Possible circumstellar disk.
|-
| style="background-color: lightgreen" | B (BD+38°4344)
|
| style="background: ;" | K7.0V
| rowspan="2" |
|-
| style="background: #F5F5DC" | B
| style="background: #F5F5DC" | DQZ
|-
| B (GQ Andromedae)
| style="background: ;" | M3.5V
|-
| style="background: #D8BD98"| Ba§
| rowspan="2" |
| style="background: ;" | T1.0V
|0.065
| 12.3 J
| 14.5 J
|
|-
| style="background: #D8BD98"| Bb§
| style="background: ;" | T6.0V
|0.050
| 13.2 J
|-
| colspan="2" | YZ Ceti (LHS 138)
| 12.1222
| Cet
|
| style="background: ;" | M4.5V
|-
| colspan="2" | Luyten's Star (BD+05°1668)
| 12.3485
| CMi
|
| style="background: ;" | M3.5Vn
|0.26
| 9.86
| 11.97
| 264.1269 and two suspected planets (d, e) (2019)
|-
| colspan="2" | Teegarden's Star (SO025300.5+165258)
| 12.4970
| style="background-color: pink" | Ari
|
| style="background: ;" | M6.5V
|0.08
| 15.14
| 17.22
| 260.9884
|-
| colspan="2" | Kapteyn's Star (CD−45°1841)
| 12.8308
| style="background-color: pink" | Pic
|
| style="background: ;" | M1.5VI
|-
| colspan="2" | Lacaille 8760 (AX Microscopii)
| 12.9472
| style="background-color: pink" | Mic
|
| style="background: ;" | M0.0V
|0.03
| rowspan="2" | B flare star
|-
| B (DO Cephei)
| style="background: ;" | M4.0V
|-
| rowspan="2" | Ross 614(V577 Monocerotis, Gliese 234)
| A (LHS 1849)
| rowspan="2" | 13.363
| rowspan="2" style="background-color: pink" | Mon
| rowspan="2" |
| style="background: ;" | M4.5V
| rowspan="2" | A flare star
|-
| B (LHS 1850)
| style="background: ;" | M5.5V
|0.111
| 14.23
| 16.17
|-
| colspan="2" style="background: #C67B30" |UGPS J0722-0540&
| 13.43
| Mon
|
| style="background: ;" | T9
| 18.45 J
| 242.8
|
|-
| colspan="2" | Wolf 1061 (Gliese 628, BD−12°4523)
| 14.0500
| Oph
|
| style="background: ;" | M3.0V
|-
| colspan="2" style="background: #F5F5DC" | Van Maanen's Star (Gliese 35, LHS 7)
| 14.0718
| style="background-color: pink" | Psc
|
| style="background: #F5F5DC" | DZ7
|-
| rowspan="2" | Wolf 424(FL Virginis, LHS 333, Gliese 473)
| A
| rowspan="2" | 14.595
| rowspan="2" | Vir
| rowspan="2" |
| style="background: ;" | M5.5Ve
|0.143
| 13.18
| 14.97
| rowspan="2" | 223.4775 and (c) (2020)
|-
| colspan="2" | Gliese 674 (LHS 449)
| 14.8492
| style="background-color: pink" | Ara
|
| style="background: ;" | M3.0V
|-
| colspan="2" | LHS 292 (LP 731-58)
| 14.8706
| style="background-color: pink" | Sex
|
| style="background: ;" | M6.5V
|
|-
| colspan="2" | Gliese 876 (Ross 780)
| 15.2382
| Aqr
|
| style="background: ;" | M3.5V
|-
| colspan="2" style="background: #D8BD98" | WISE 1639−6847§
| 15.336
| style="background-color: pink" | TrA
|
| style="background: ;" | Y0.5
|
| 20.57 J
| 22.10 J
| 212.67
|
|-
| colspan="2" | LHS 288 (Luyten 143-23)
| 15.7586
| style="background-color: pink" | Car
|
| style="background: ;" | M5.5V
|-
| colspan="2" style="background: #D8BD98" | DENIS 0255−4700§
| 15.877
| Eri
|
| style="background: ;" | L7.5V
|-
| colspan="2" | Gliese 832
| 16.2005
| style="background-color: pink" | Gru
|
| style="background: ;" | M1.5 V and the other now refuted (c (2014))
|-
| colspan = '2' | Gliese 682 (CD-44 11909)
| 16.3328
| style="background-color: pink" | Sco
|
| style="background: ;" | M4 V
| 0.27
| 10.95
| 12.45
| 199.6944
| rowspan="2" |
|-
| style="background-color: lightgreen" | B
|
| style="background: ;" | K5 V
| 0.70
| style="background: lightblue;" | 6.01
| 7.46
|-
| colspan = '2' style="background-color: lightgreen" | Altair (Alpha Aquilae)
| 16.730
| style="background-color: pink" | Aql
|
| style="background: " | A7 IV-Vn
| 1.79
| style="background: lightblue;" | 0.77
| 2.22
| 194.95
|
|-
| rowspan='2' | EI Cancri (GJ 1116, )
| A
| rowspan='2' | 16.800
| rowspan='2' | Cnc
| rowspan='2' |
| style="background: ;" | M5.5 V
| 0.12
| 14.06
| 15.50
| rowspan='2' | 194.1443
| rowspan='2' | binary brown dwarf
|-
| style="background: #D8BD98" | B§
| style="background: ;" | T8 V
| 0.019–0.038
|
|
|-
| colspan = '2' | GJ 3323 (LHS 1723, )
| 17.5309
| Eri
|
| style="background: ;" | M4 V
| 0.1705
| 12.22
| 13.57
| 186.0466
|
|-
| colspan = '2' | Gliese 251 (Wolf 294, HD 265866)
| 18.2146
| style="background-color: pink" | Gem
|
| style="background: ;" | M3 V
| 0.360
| 10.02
| 11.29
| 179.0629
|-
| style="background: #D8BD98" | Ba§
| style="background: ;" | T7
| 0.036
| rowspan=2 | 14.01 J
| rowspan=2 | 15.21 J
|-
| style="background: #D8BD98" | Bb§
| style="background: ;" | T8
| 0.033
|-
| colspan = '2' style="background-color: lightgreen" | Alsafi (Sigma Draconis)
| 18.7993
| Dra
|
| style="background: ;" | K0 V
| 0.85
| style="background: lightblue;" | 4.67
| 5.87
| 173.4939
| rowspan="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
| style="background: ;" | M V
| 0.112
| 14.02
| 15.13
|-
| rowspan='2' | HR 7703 (279 G. Sagittarii, HD 191408, Gliese 783, )
| style="background-color: lightgreen" | A
| rowspan='2' | 19.609
| rowspan='2' | Sgr
| rowspan='2' |
| style="background: ;" | K2.5 V
| 0.65
| style="background: lightblue;" | 5.31
| 6.41
| rowspan='2' | 166.3272
|
|- class="unsortable"
! System
! Name
! rowspan="2" | Distance(ly
! rowspan="2" | Cons.
! rowspan="2" | RA/Dec(Ep. & Eq. J2000)
! rowspan="2" | Stellarclass
! rowspan="2" | Mass(<var>M</var><sub>☉</sub>)
! data-sort-type="number" | App.
! data-sort-type="number" | Abs.
! rowspan="2" | Parallax(mas)
! rowspan="2" | Notes and additionalreferences
|- class="unsortable"
! colspan="2" | Designation
! colspan="2" | Magnitude ()
|}
Distant future and past encounters
right|thumb|350px|alt=Graph of the distances of various stars from the Sun during the past 20,000 to future 80,000 years.|Distances of the nearest stars from 20,000 years ago until 80,000 years in the future
thumb|350px|Visualisation of the [[orbit of the Sun (yellow dot and white curve) around the Galactic Center (GC) in the last galactic year. The red dots correspond to the positions of the stars studied by the European Southern Observatory in a monitoring programme.]]
Over long periods of time, the slow independent motion of stars change in both relative position and in their distance from the observer. This can cause other currently distant stars to fall within a stated range, which may be readily calculated and predicted using accurate astrometric measurements of parallax and total proper motions, along with spectroscopically determined radial velocities. Although extrapolations can be made into the past or future, they are subject to increasingly significant cumulative errors over very long periods.
One of the first stars known to approach the Sun particularly close is Gliese 710. The star, whose mass is roughly half that of the Sun, is currently 62 light-years from the Solar System. It was first noticed in 1999 using data from the Hipparcos satellite, and was estimated to pass less than from the Sun in 1.4 million years. With the release of Gaias observations of the star, it has since been refined to a much closer , close enough to significantly disturb objects in the hypothetical Oort cloud, which is thought to extend from the Sun.
Gaia third data release has provided updated values for many of the candidates in the table below.
<!--Comment: These examples are all from one source Matthews (1994). This section does require more source references-->
{| class="wikitable sortable sort-under sticky-header-multi defaultcenter"
|+Stars that are known to have passed or will pass within 5 light-years of the Sun in the past or future
! Star name
! Minimum distance<br>(light-years)
! Date of approach<br>in thousands of years<!--this is the date of approach. NOT how many years away. Barnard's star will approach us in 9,700 years, not 11,700.-->
! Current distance<br>(light-years)
! Stellar
! Mass in M<sub>☉</sub>
! Current<br>apparent
! Current Constellation|
! Current<br>Right ascension
! data-sort-type="number" | Current<br>Declination
|-
| Gliese 710
|
|
|
| K7V
| 0.4–0.6
|
| Serpens
|
|
|-<!--OMITTED FOR HUGE RV
| WD 0810-353
|
|
|
| WD
| 0.65
|
| Puppis
|
| -->
|-
| HD 7977
|
|
|
| G0V
| ~1.2
|
| Cassiopeia
|
|
|-<!--STARS MEASURED BY BAILER-JONES+ (2018) MAY BE FALSE POSITIVES. FALSE POSITIVE STARS ARE OMITTED-->
| Scholz's Star and companion brown dwarf
|
|
|
| A: M9V<br/>B: T5
| A: 0.095<br>B: 0.063
|
| Monoceros
|
| <!--2MASS J0610-4246 (AKA Gaia DR2 5571232118090082816) is not included despite appearing in several papers, because it has a low-mass companion with a much higher proper motion that averages to a much more distant approach-->
|-
| 2MASS J0628+1845
|
|
|
| M2.5V
| 0.28
|
| Gemini
|
|
|-
| 2MASS J0805+4624
|
|
|
| M3V
| 0.25
|
| Lynx
|
|
|-
| CD-69 2001
|
|
|
| K4V
| 0.61
|
| Indus
|
|
|-
| HD 49995
|
|
|
| A: F3V<br/>B: M1V
| A: 1.48<br/>B: 0.49
| 8.78
| Canis Major
|
|
|-
| 2MASS J0621-0101
|
|
|
| G5V
| 0.96
| 11.9
| Orion
|
|
|-<!-- the object at 17 40 14.405 -23 37 53.28 is in a highly contaminated part of the galactic center and isn't included, with an approach of 1.75 +0.26 -0.23 LY-->
| LSPM J2146+3813
|
|
|
| M5V
| ~0.15
|
| Cygnus
|
|
|-
| 2MASS J0455+1144
|
|
|
| M0V
| 0.50
|
| Orion
|
|
|-
| 2MASS J0734-0637
|
|
|
| M0V
| 0.50
|
| Monoceros
|
|
|-
| 2MASS J1151-0313
|
|
|
| M3.5V
| 0.23
|
| Virgo
|
|
|-
| UCAC4 076–006432
|
|
|
| mid K
| ~0.6
|
| Mensa
|
|
|-<!--UCAC4 574-064555 is not included despite giving a close approach of 2.15 +0.84 -0.74 due to having a highly uncertain solution in Gaia eDR3 which might change-->
| 2MASS J0120+4739
|
|
|
| M3.5V
| 0.25
|
| Andromeda
|
|
|-
| TYC 6760–1510–1
|
|
|
| M1.5V
| 0.58
|
| Hydra
|
|
|-
| UCAC2 15719371
|
|
|
| K4V
| 0.66
|
| Antlia
|
|
|-<!-- EGGR 290 at 2.514 +0.065 -0.062 is omitted for unreasonable RV-->
| TYC 1662–1962–1
|
|
|
| Early K
| ~0.8
|
| Vulpecula
|
|
|-
| HD 179939
|
|
|
| A3V
| 1.7
|
| Aquila
|
|
|-
| BD-21 1529
|
|
|
| G5V
| ~0.95
|
| Canis Major
|
|
|-
| 2MASS J1310-1307
|
|
|
| M2.5V
| 0.34
|
| Virgo
|
|
|-
| UPM J1121-5549
|
|
|
| M3V
| 0.29
|
| Centaurus
|
|
|-
| UCAC4 464–006057
|
|
|
| Early M
| ~0.4
|
| Taurus
|
|
|-<!-- 10 15 33.832 -23 40 14.02 (approach 2.815 +0.101 -0.096) was omitted for an impossible RV of over 700 km/s-->
| UCAC4 213–008644
|
|
|
| M5.0
| 0.17
|
| Puppis
|
|
|-
| GJ 3649
|
|
|
| M1
| 0.49
|
| Leo
|
|
|-
| Ross 248
|
|
|
| M6V
| 0.136
|
| Andromeda
|
|
|-
| 2MASS J1921-1244
|
|
|
| K6V
| 0.69
|
| Sagittarius
|
|
|-
| Proxima Centauri
|
|
|
| M5Ve
| 0.15
|
| Centaurus
|
|
|-
| TYC 9387–2515–1
|
|
|
| K1V
| 0.86
|
| Mensa
|
|
|-
| Alpha Centauri AB
|
|
|
| A: G2V<br>B: K1V
| A: 1.100<br>B: 0.907
| A: -0.01<br>B: +1.33
| Centaurus
|
|
|-
| Gliese 445
|
|
|
| M4
| 0.15?
|
| Camelopardalis|
|
|
|-
| 2MASS J1638-6355
|
|
|
| K2V
| 0.82
|
| Triangulum Australe
|
|
|-
| 2MASS J0542+3217
|
|
|
| A: G4V<br/>B: K0V
| A: 1.01<br/>B: 0.85
|
| Auriga
|
|
|-
| 2MASS J0625-2408
|
|
|
| K/M
| ~0.5
|
| Canis Major
|
|
|-
| Barnard's Star
|
|
|
| sdM4
| 0.144
|
| Ophiuchus
|
|
|-
| BD+05 1792
|
|
|
| G2V
| 1.07
|
| Gemini
|
|
|-
| 2MASS J2241-2759
|
|
|
| K7V
| ~0.5
|
| Piscis Austrinus
|
|
|-
| 2MASS J1724-0522
|
|
|
| K0V
| 0.86
|
| Ophiuchus
|
|
|-
| StKM 1–554
|
|
|
| M0V
| 0.65
|
| Orion
|
|
|-
| GJ 3379
|
|
|
| M3.5V
| 0.19
|
| Orion
|
|
|-
| 2MASS J1936+3627
|
|
|
| G5.5V
| 0.95
| 12.2
| Cygnus
|
|
|-
| 2MASS J0710+5228
|
|
|
| M3V
| 0.33
|
| Lynx
|
|
|-
| HD 146248
|
|
|
| G2/3IV
| 1.23
|
| Triangulum Australe
|
|
|-
| 2MASS J1724+0355
|
|
|
| G8V
| 0.85
|
| Ophiuchus
|
|
|-
| StKM 1–1456
|
|
|
| A: K5V<br/>B: M8V
| A: 0.81<br/>B: 0.09
|
| Hercules
|
|
|-
| Zeta Leporis
|
|
|
| A2Vann
| 2.0
|
| Lepus
|
|
|-
| Lalande 21185
|
|
|
| M2V
| 0.39
|
| Ursa Major
|
|
|-
| HD 68814
|
|
|
| G6V
| 0.98
|
| Hydra
|
|
|-
| 2MASS J1941-4602
|
|
|
| M4-M6
| ~0.15
|
| Telescopium
|
|
|-<!--Gaia DR2 5828371157273738368 is not included because of a potential white dwarf companion with high proper motion uncertainty influencing the total system motion-->
|}
See also
- Interstellar travel
- Location of Earth
- The Magnificent Seven
- Nearby Stars Database
- Solar System#Galactic position
- Stars 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 star systems within 50–55 light-years
- List of star systems within 55–60 light-years
- List of star systems within 60–65 light-years
- List of star systems within 65–70 light-years
- List of star systems within 70–75 light-years
- List of star systems within 75–80 light-years
- List of star systems within 80–85 light-years
- List of star systems within 85–90 light-years
- List of star systems within 90–95 light-years
- List of star systems within 95–100 light-years
- List of star systems within 100–150 light-years
- List of star systems within 150–200 light-years
- List of star systems within 200–250 light-years
- List of star systems within 250–300 light-years
- List of star systems within 300–350 light-years
- List of star systems within 350–400 light-years
- List of star systems within 400–450 light-years
- List of star systems within 450–500 light-years
- List of nearest giant stars
- List of nearest supergiants
- List of nearest hypergiants
- List of nearest bright stars
- Historical brightest stars
- List of nearest exoplanets
- List of nearest terrestrial exoplanet candidates
- List of nearest stars by spectral type
- 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
Notes
References
External links
- "The 100 nearest star systems", Research Consortium on Nearby Stars
- The dynamics of the closest stars
- Table 4 "The Census of Stars and Brown Dwarfs within 8 Parsecs of the Sun" in
- 3D radar map of stars within 9 lys, free online interactive 3D model of nearest stars