List of star systems within 25–30 light-years
Appearance
(Redirected from SIPS J1259-4336)
This is a list of star systems within 25–30 light-years of Earth.
# | Visible to the unaided eye |
$ | Bright star (absolute magnitude of +8.5 or brighter) |
‡ | White dwarf |
§ | Brown dwarf or sub-brown dwarf |
* | Nearest in constellation |
System←→←→ | Star or (sub-) brown dwarf |
Distance (ly) | Constellation | Coordinates: RA, Dec (Ep J2000, Eq J2000) |
Stellar class |
Apparent magnitude (V) |
Parallax (mas) |
Notes and additional references |
---|---|---|---|---|---|---|---|---|
GJ 4248 (L 499-56) | 25.008±0.010 | Grus | 22h 02m 29.4s −37° 04′ 51″ |
M3.5 | 11.80 | 130.4186±0.0534[1] | ||
Mu Cassiopeiae (Gliese 53) | A$ | 25.033±0.084 | Cassiopeia | 01h 08m 16.4s +54° 55′ 13″ |
G5VIp | 5.14# | 130.2881±0.4348[1] | |
B | M5V | 11.45 | ||||||
Alpha Piscis Austrini | C (LP 876-10) | 25.0368±0.0062 | Aquarius | 22h 48m 04.5s −24° 22′ 08″ |
M4V | 12.624 | 130.2707±0.0325[1] | component C of triple system |
Vega (Alpha Lyrae)$ | 25.045 ± 0.069 | Lyra | 18h 36m 56.3s +38° 47′ 01″ |
A0Va | 0.03# | 130.23±0.36[2] | [3] | |
VX Arietis (Gliese 109) | 25.0513±0.0054 | Aries | 02h 44m 15.5s +25° 31′ 24″ |
M3.5V | 10.56 | 130.1956±0.0281[1] | flare star | |
Alpha Piscis Austrini | A (Fomalhaut)$ | 25.126±0.091 | Piscis Austrinus | 22h 57m 39.0s −29° 37′ 20″ |
A3V | 1.16# | 129.81±0.47[2] | [4][5] has 1 refuted planet, component A of triple system |
AN Sextantis (Gliese 382) | 25.1364±0.0049 | Sextans | 10h 12m 17.7s −03° 44′ 44″ |
M1V | 9.264 | 129.7544±0.0252[1] | [6] | |
Gliese 673 (HD 157881)$ | 25.1575±0.0034 | Ophiuchus | 17h 25m 45.2s +02° 06′ 41″ |
K7V | 7.492 | 129.6459±0.0175[1] | [7] | |
SIPS 1259-4336 | 25.200±0.012 | Centaurus | 12h 59m 04.7s −43° 36′ 24″ |
M7.5V | 18.01 | 129.4288±0.0620[1] | [8] | |
LHS 1070 (LP 881-64, GJ 2005) | A | 25.222±0.024 | Sculptor | 00h 24m 44.2s −27° 08′ 25″ |
M5.5-6V | 15.35 | 129.3167±0.1256[1] | [9] |
B | M8.5V | |||||||
C | M9-9.5V | |||||||
G 192-13 (GJ 3378) | 25.2245±0.0055 | Camelopardalis | 06h 01m 11.0s +59° 35′ 50″ |
M4.0Ve | 7.465 (J) | 129.3014±0.0283[1] | ||
Gliese 701 (HD 165222) | 25.2407±0.0050 | Serpens* | 18h 05m 07.6s −03° 01′ 53″ |
M1V | 9.9 | 129.2184±0.0256[1] | [10] | |
GJ 1093 (G 109-35) | 25.286±0.012 | Gemini | 06h 59m 28.8s +19° 20′ 56″ |
M5Ve | 128.9866±0.0607[1] | [11] | ||
LP 71-82 (G 227-22) | 25.4203±0.0063 | Draco | 18h 02m 16.6s +64° 15′ 44″ |
M5.0V | 13.51 | 128.3057±0.0319[1] | Very rapid star rotation | |
WISE 1800+0134§ | 25.47±0.10 | Ophiuchus | 18h 00m 26.5s +01° 34′ 57″ |
L7.5 | 14.30 (J) | 128.0546±0.5101[1] | [12][13] | |
Gliese 623 | A | 25.585±0.097 | Hercules | 16h 24m 09.3s +48° 21′ 11″ |
M3.0Ve | 127.4785±0.4818[14] | ||
B | M | |||||||
WISE J0005+3737§ | 25.70±0.43 | Andromeda | 00h 05m 17.5s +37° 37′ 21″ |
T9 | 126.9±2.1[13] | [13] | ||
Gliese 54 (CD-68 47) | A | 25.702±0.081 | Tucana* | 01h 10m 22.9s −67° 26′ 42″ |
M2.5V | 126.9±0.4[15] | [16] | |
B | M | |||||||
2MASS 0729-39§ | 25.82±1.82 | Puppis* | 07h 29m 00.0s −39° 54′ 04″ |
T8 | 126.3±8.3[17] | |||
GJ 1224 (G 154-44) | 25.9987±0.0063 | Serpens | 18h 07m 32.8s −15° 57′ 47″ |
M4Ve | 125.4509±0.0306[1] | [11] | ||
SCR J0740−4257 | 26.0295±0.0045 | Puppis | 07h 40m 11.8s −42° 57′ 40″ |
M4.5 | 13.81 | 125.3028±0.0215[1] | [18] | |
BB Capricorni (Wolf 922, Gliese 831) | A | 26.030±0.062 | Capricornus | 21h 31m 18.6s −09° 47′ 26″ |
M4.5V | 125.3±0.3[15] | ||
B | M | |||||||
Gliese 257 (CD-44 3045) | A | 26.2274±0.0084 | Puppis | 06h 57m 46.6s −44° 17′ 28″ |
M3.5V | 124.3569±0.0399[1] | ||
B | M | |||||||
GJ 1151 (G 122-49) | 26.231±0.012 | Ursa Major | 11h 50m 57.7s +48° 22′ 39″ |
M7 | 124.3378±0.0549[1] | [19] has 1 known planet | ||
Gliese 480.1 (L 399-68) | 26.2637±0.0062 | Centaurus | 12h 40m 46.3s +43° 33′ 59″ |
M3V | 124.1851±0.0295[1] | |||
Chi Draconis | A$ | 26.28±0.19 | Draco | 18h 21m 03.4s +72° 43′ 58″ |
F7V | 3.68# | 124.11±0.87[2] | |
B$ | K0V | 5.67# | ||||||
Pi3 Orionis (Tabit)$ | 26.316±0.036 | Orion | 04h 49m 50.4s +06° 57′ 41″ |
F6V | 3.16# | 123.94±0.17[2] | [20] | |
Gliese 486 (Wolf 437) | 26.3506±0.0070 | Virgo | 12h 47m 56.6s +09° 45′ 05″ |
M3.5Ve | 123.7756±0.0329[1] | has one known planet | ||
2MASS J21481628+4003593§ | 26.37±0.08 | Cygnus | 21h 48m 16.3s +40° 03′ 59″ |
L6.5pec (red) | 123.6752±0.3595[1] | [13] | ||
Gliese 793 (G 262-15) | 26.3764±0.0032 | Cepheus | 20h 30m 32.0s +65° 26′ 58″ |
M3V | 123.6547±0.0148[1] | |||
GJ 1154 (G 13-22) | 26.3789±0.0096 | Virgo | 12h 14m 16.5s +00° 37′ 26″ |
M4.5Ve | 123.6430±0.0449[1] | |||
Gliese 300 (L 674-15) | 26.4730±0.0051 | Puppis | 08h 12m 40.9s −21° 33′ 07″ |
M3.5V | 123.2033±0.0236[1] | [21] | ||
G 99-47 (EGGR 290, GJ 1087)‡ | 26.4740±0.0037 | Orion | 05h 56m 25.5s +05° 21′ 48″ |
DAP8.9 | 12.930 | 123.1989±0.0170[1] | [22][23] | |
Gliese 686 | 26.6132±0.0038 | Hercules | 17h 37m 53.3s +18° 35′ 30″ |
MV | 122.5546±0.0176[1] | has 1 known planet[24] | ||
L 97-12 (LAWD 26, Gliese 293)‡ | 26.6439±0.0025 | Volans* | 07h 53m 08.1s −67° 47′ 31″ |
DC8.8 | 12.726 (J) | 122.4130±0.0114[1] | [25][26] | |
UGPS J0521+3640§ | 26.69±0.35 | Auriga | 05h 21m 26.9s +36° 41′ 00″ |
T8.5 | 122.2±1.6[27] | [13] | ||
p Eridani (Gliese 66) | A$ | 26.7334±0.0070 | Eridanus | 01h 39m 47.6s −56° 11′ 47″ |
K2V | 5.82# | 122.0035±0.0319[1] | |
B$ | K2V | 5.95# | ||||||
L 173-19 | 26.7982±0.0070 | Eridanus | 02h 00m 38.3s −55° 58′ 05″ |
MV | 121.7084±0.0319[1] | |||
Gliese 884 (HD 217357)$ | 26.8502±0.0055 | Aquarius | 23h 00m 16.1s −22° 31′ 28″ |
K7+Vk | 7.88 | 121.4724±0.0249[1] | ||
Gliese 48 (Ross 318) | 26.8530±0.0035 | Cassiopeia | 01h 02m 32.2s +71° 40′ 47″ |
M3.0Ve | 121.4598±0.0158[1] | |||
WISEPC J115013.88+630240.7§ | 26.87±0.61 | Ursa Major | 11h 50m 13.9s +63° 02′ 42″ |
T8 | 121.4±2.7[13] | [13] | ||
Gliese 747 (G 207-16) | A | 27.134±0.045 | Lyra | 19h 07m 43.0s +32° 32′ 42″ |
M3V | 120.2±0.2[28] | ||
B | M | |||||||
2MASS 0348-6022§ | 27.16±0.41 | Reticulum | 03h 48m 07.7s −60° 22′ 27″ |
T7 | 120.1±1.8[27] | [13] | ||
WD 2359-434 (LAWD 96, Gliese 915)‡ | 27.176±0.0049 | Phoenix* | 00h 02m 10.7s −43° 09′ 55″ |
DAP5.8 | 120.0143±0.0215[1] | [29] | ||
Mu Herculis | Aa$ | 27.197±0.035 | Hercules | 17h 46m 27.5s +27° 43′ 15″ |
G5IV | 3.42# | 119.9248±0.1543[1] | |
Ab | M4V | |||||||
B | M3.5V | |||||||
C | M | |||||||
Wolf 489‡ | 27.2349±0.0069 | Virgo | 13h 36m 31.8s +03° 40′ 45″ |
DZ10.0 | 119.7566±0.0304[1] | |||
GJ 1227 (G 227-29) | 27.2360±0.0078 | Draco | 18h 22m 27.1s +62° 03′ 02″ |
M4.0V | 119.7519±0.0341[1] | |||
GJ 1289 (G 130-4) | 27.275±0.013 | Andromeda | 23h 43m 06.3s +36° 32′ 13″ |
MV | 119.5794±0.0563[1] | has 1 known planet[30] | ||
Gliese 185 (HD 32450) | A | 27.2766±0.0096 | Lepus | 05h 02m 28.5s −21° 15′ 24″ |
K7V | 119.5737±0.0420[1] | ||
B | M | |||||||
SCR 1138-7721 | 27.3296±0.0070 | Chamaeleon* | 11h 38m 16.8s −77° 21′ 49″ |
MV | 119.3419±0.0305[1] | [21] | ||
SCR J1546−5534 | A | 27.39±0.16 | Norma | 15h 46m 41.7s −55° 34′ 47″ |
M7.5 | 119.0962±0.7032[14] | ||
B§ | T8 | |||||||
2MASS J00345157+0523050§ | 27.45±0.64 | Pisces | 00h 34m 51.6s +05° 23′ 05″ |
T6.5 | 118.8±2.7[13] | [13] | ||
TYC 3980-1081-1 | A (IRAS 21500+5903) | 27.604±0.0036 | Cepheus | 21h 51m 38.3s +59° 17′ 40″ |
M3.5V | 118.1551±0.0155[1] | ||
B (UCAC4 747-070768)‡ | DAH | |||||||
Beta Canum Venaticorum (Chara)$ | 27.634±0.036 | Canes Venatici* | 12h 33m 44.5s +41° 21′ 27″ |
G0V | 4.24# | 118.0266±0.1530[1] | ||
Gliese 232 (Ross 64) | 27.7046±0.0065 | Gemini | 06h 24m 41.3s +23° 25′ 59″ |
M4V | 117.7263±0.0278[1] | |||
Gliese 618 (CD-37 10765) | A | 27.7647±0.0069 | Scorpius | 16h 20m 03.5s −37° 31′ 44″ |
M3V | 117.4716±0.0291[1] | ||
B | M5 | |||||||
Gliese 318 (CD-32 5613, LAWD 28)‡ | 27.7826±0.0049 | Pyxis* | 08h 41m 32.4s −32° 56′ 33″ |
DA5.5 | 117.3961±0.0205[1] | suspected double white dwarf | ||
61 Virginis$ | 27.836±0.035 | Virgo | 13h 18m 24.3s −18° 18′ 40″ |
G7V | 4.74# | 117.1726±0.1456[1] | has 3 known planets | |
GJ 1276 (EGGR 453)‡ | 27.8436±0.0081 | Aquarius | 22h 53m 53.3s −06° 46′ 54″ |
DZ | 117.1388±0.0341[1] | [29] | ||
Gliese 493.1 (Wolf 461) | 27.869±0.015 | Virgo | 13h 00m 33.5s +05° 41′ 08″ |
M4.5Ve | 117.0327±0.0613[1] | |||
GJ 3454 (G 89-32) | A | 27.97±0.23 | Canis Minor | 07h 36m 25.1s +07° 04′ 43″ |
M4.5V | 116.6±0.97[31] | ||
B | M | |||||||
CWISEP 0402-2651§ | 28.02+5.99 −4.20 |
Eridanus | 02h 02m 16.2s +10° 20′ 14″ |
Y1 | 116.4±20.5[13] | [13] | ||
Gliese 877 (L 49-19) | 28.0412±0.0041 | Octans* | 22h 55m 45.5s −75° 27′ 31″ |
M3V | 10.377 | 116.3134±0.0168[1] | ||
CD Ceti (GJ 1057) | 28.052±0.010 | Cetus | 03h 13m 22.9s +04° 46′ 29″ |
M4.5Ve | 116.2678±0.0427[1] | has 1 known planet[32] | ||
Zeta Tucanae$ | 28.073±0.032 | Tucana | 00h 20m 04.3s −64° 52′ 29″ |
F9.5V | 4.23# | 116.1826±0.1334[1] | ||
LP 502-56 (NLTT 40406) | 28.107±0.011 | Serpens | 15h 30m 30.3s +09° 26′ 01″ |
M5.5V | 116.0425±0.0435[1] | |||
WISE 1647+5632§ | 28.12+9.37 −5.62 |
Draco | 16h 47m 15.8s +56° 32′ 06″ |
T6 | 16.59 | 116±29[33] | ||
CWISE 0617+1945 | A§ | 28.2±5.7[34] | Orion | 06h 17m 41.8s +19° 45′ 13″ |
L2 | parallax uncertain,[13][34] brown dwarfs are separated by about 37 AU[34] | ||
B§ | L4 | |||||||
GJ 3517 (LP 666-9) | 28.242±0.018 | Hydra | 08h 53m 36.2s −03° 29′ 32″ |
M9V | 18.959 | 115.4876±0.0726[1] | [35] | |
Chi1 Orionis | A$ | 28.256±0.066 | Orion | 05h 54m 23.0s +20° 16′ 34″ |
G0V | 4.39# | 115.43±0.27[2] | |
B | ||||||||
AP Columbae | 28.2636±0.0073 | Columba* | 06h 04m 32.2s −34° 33′ 36″ |
M4.5Ve | 12.96 | 115.3982±0.0298[1] | ||
SIPS J1141-3624 (PM J11413-3624) | 28.3408±0.0088 | Centaurus | 11h 41m 21.5s −36° 24′ 35″ |
M5 | 13.105 | 115.0835±0.0359[1] | ||
GJ 1207 (G 19-7) | 28.3822±0.0062 | Ophiuchus | 16h 57m 05.7s −04° 20′ 56″ |
M3.5Ve | 12.25 | 114.9158±0.0252[1] | ||
LP 991-84 | 28.459±0.010 | Phoenix | 39h 54m 21.7s −39° 36′ 09″ |
M4.5V | 14.403 | 114.604±0.0402[1] | ||
Xi Ursae Majoris | Aa (Alula Australis)$ | 28.49±0.11 | Ursa Major | 11h 18m 10.9s +31° 31′ 45″ |
F8.5:V | 4.41# | 114.4867±0.4316[14] | |
Ab | M | |||||||
Ba$ | G2V | 4.87# | ||||||
Bb | M | |||||||
WISE J1118+3125§ | T8.5 | |||||||
2MASS 0036+1821 (LSPM J0036+1821)§ | 28.492±0.034 | Pisces | 00h 36m 16.17s 18° +21′ 10.4″ |
L3.5 | 114.4735±0.1381[1] | [13] | ||
Gliese 250 (HD 50281) | A$ | 28.5373±0.0055 | Monoceros | 06h 52m 18.1s −05° 10′ 25″ |
K3V | 6.58 | 114.2911±0.0219[1] | |
Ba | M2.5V | |||||||
Bb | ||||||||
Gliese 450 (MCC 135) | 28.5888±0.0048 | Ursa Major | 11h 51m 07.3s +35° 16′ 19″ |
M1.5V | 114.0854±0.0191[1] | |||
WISENF 1936+0408§ | 28.64±0.99 | Aquila | 19h 36m 56.1s +04° 08′ 01″ |
Y0 | 113.9±3.8[13] | spectral type is uncertain[13] | ||
41 G. Arae | Aa$ | 28.673±0.018 | Ara | 17h 19m 03.8s −46° 38′ 10″ |
G8V | 5.55# | 113.7513±0.0725[1] | [36] |
Bb | ||||||||
B | M0V | |||||||
? | ? | |||||||
HD 192310 (5 G. Capricorni, HR 7722, Gliese 785)$ | 28.739±0.013 | Capricornus | 20h 15m 17.4s −27° 01′ 59″ |
K2+V | 5.73# | 113.4872±0.0516[1] | has 2 known planets | |
Gliese 849 | 28.7503±0.0076 | Aquarius | 22h 09m 40.3s –04° 38′ 27″ |
M3.5V | 113.4447±0.0300[1] | has 2 known planets | ||
HU Delphini (Gliese 791.2) | A | 28.762±0.051 | Delphinus | 20h 29m 48.3s +09° 41′ 20″ |
M4.5V | 113.4±0.2[16] | [16] | |
B | M | |||||||
Gliese 745 | A (Ross 730) | 28.8066±0.0049 | Sagitta* | 19h 07m 05.6s +20° 53′ 17″ |
M2.0V | 113.2228±0.0192[1] | ||
B (HD 349726) | M2V | |||||||
IRAS 06355-7535 (LDS 169) | A (L 32-9) | 28.8301±0.0043 | Mensa* | 06h 33m 47.0s −75° 37′ 46″ |
M2V | 10.484 | 113.1304±0.0169[1] | |
B (L 32-8) | M3V | 11.419 | ||||||
HR 1614 (284 G. Eridani, HD 32147, Gliese 183)$ | 28.8451±0.0057 | Eridanus | 05h 00m 49.0s −05° 45′ 13″ |
K3V | 6.22# | 113.0715±0.0222[1] | ||
GJ 1105 (G 111-47) | 28.8653±0.0066 | Lynx* | 07h 58m 12.7s +41° 18′ 13″ |
M3.5Ve | 112.9927±0.0259[1] | [19] | ||
Gliese 867 | A (FK Aquarii) | 28.8668±0.0099 | Aquarius | 22h 38m 45.6s −20° 37′ 16″ |
M0Vep | 112.9867±0.0387[1] | ||
B (FL Aquarii) | M3.5V | |||||||
C | ||||||||
D | ||||||||
Ross 695 (Gliese 465) | 28.9469±0.0062 | Corvus* | 12h 24m 52.5s −18° 14′ 32″ |
M2 | 11.272 | 112.6740±0.0241[1] | ||
SCR J0630-7643 | A | 28.951±0.024 | Mensa | 06h 30m 46.6s −76° 43′ 09″ |
M6.0 | 112.6584±0.0934[1] | [21] | |
B | M | |||||||
DENIS 0334-49 (LEHPM 3396) | 28.963±0.014 | Horologium | 03h 34m 12.2s −49° 53′ 32″ |
M9V | 112.6100±0.0557[1] | [37] | ||
2MASS 0727+1710§ | 28.99±0.23 | Gemini | 07h 27m 18.2s +17° 10′ 01″ |
T7 | 112.5±0.9[38] | [13] | ||
Gamma Leporis | A$ | 29.0004±0.0058 | Lepus | 05h 44m 27.8s −22° 26′ 54″ |
F6V | 3.59# | 112.4661±0.0225[1] | |
B (AK Leporis)$ | K2V | 6.17# | ||||||
C | M3.5V | |||||||
WISE1810§ | 29.03+2.28 −1.95 |
Serpens | 18h 10m 06.18s −10° 10′ 00.5″ |
esdT8-esdT9[39] | 112.5+8.1 −8.0[39] |
closest extreme metal-poor brown dwarf[39] | ||
GJ 2066 (G 113-20) | 29.1550±0.0059 | Hydra | 08h 16m 08.0s +01° 18′ 09″ |
M2.0V | 10.091 | 111.8698±0.0228[1] | ||
LHS 224 (G 193-27, GJ 3421) | A | 29.43±0.19 | Lynx | 07h 03m 55.7s +52° 42′ 07″ |
M5.0Ve | 110.8263±0.6945[1] | ||
B | M | |||||||
SZ Ursae Majoris | A | 29.588±0.0045 | Ursa Major | 11h 20m 04.8s +65° 50′ 47″ |
M2V | 110.2305±0.0166[1] | ||
B | ||||||||
Gliese 433 | 29.6045±0.0055 | Hydra | 11h 35m 26.9s −32° 32′ 24″ |
M2V | 110.1711±0.0204[1] | has 3 known planets | ||
Delta Eridani («Rana»)$ | 29.644±0.052 | Eridanus | 03h 43m 14.9s –09° 45′ 48″ |
KIV | 3.52# | 110.0254±0.1944[1] | ||
Gliese 508 (HD 115953) | Aa | 29.65±0.23 | Canes Venatici | 13h 19m 45.5s +47° 46′ 41″ |
M2V | 8.54 | 109.9837±0.8292[14] | |
Ab | ||||||||
B | ||||||||
GJ 3146 (LP 469-206) | 29.664±0.019 | Aries | 02h 16m 30.0s +13° 35′ 13″ |
M5.0Ve | 109.9500±0.0704[1] | |||
LHS 1126 (GJ 2012, EGGR 246)‡ | 29.6701±0.0055 | Cetus | 00h 41m 26.0s −22° 21′ 02″ |
DQ9 | 109.9276±0.0202[1] | [29] | ||
V374 Pegasi | 29.6898±0.0070 | Pegasus | 22h 01m 13.1s +28° 18′ 25″ |
M3.5Ve | 109.8548±0.0259[1] | |||
2MASSI J0652307+471034§ | 29.714±0.076 | Auriga | 06h 52m 30.7s +47° 10′ 35″ |
L4.5 | 109.7651±0.2782[1] | [13] | ||
WT 460 | A | 29.723±0.063 | Centaurus | 14h 11m 59.9s −41° 32′ 22″ |
M5.5e | 109.7323±0.2316[1] | ||
B | ||||||||
Gliese 283 (L 745-46) | A (LP 783-3, LAWD 25)‡ | 29.8285±0.0049 | Puppis | 07h 40m 20.8s −17° 24′ 49″ |
DAZ6 | 13.061 | 109.3440±0.0181[1] | [29] |
B (LP 783-2) | M6.5V | 16.696 | ||||||
WISE 0713−2917§ | 29.84±0.58 | Canis Major | 07h 13m 22.6s −29° 17′ 52″ |
Y0 | 109.3±2.1[13] | [13] | ||
2MASS J03552337+1133437§ | 29.88±0.13 | Taurus | 03h 55m 23.4s +11° 33′ 44″ |
L5γ | 109.1381±0.4833[1] | |||
WISEP J213456.73-713743.6§ | 29.90±1.05 | Indus | 21h 34m 56.7s −71° 37′ 45″ |
T9pec | 109.1±3.7[40] | |||
Groombridge 1830 (CF Ursae Majoris, HD 103095)$ | 29.9145±0.0054 | Ursa Major | 11h 52m 58.8s +37° 43′ 07″ |
G8VIp | 6.42# | 109.0296±0.0197[1] | ||
GJ 3801 (Ross 1015) | 29.980±0.012 | Canes Venatici | 13h 42m 43.3s +33° 17′ 24″ |
M4V | 13.896 | 108.7903±0.0440[1] | [41] | |
Beta Comae Berenices$ | 29.998±0.045 | Coma Berenices* | 13h 11m 52.4s +27° 52′ 41″ |
G0V | 4.23# | 108.7250±0.1645[1] | ||
System | Star or (sub-) brown dwarf |
Distance (ly) | Constellation | Coordinates: RA, Dec (Ep J2000, Eq J2000) |
Stellar class |
Apparent magnitude (V) |
Parallax (mas) |
Notes and additional references |
See also
[edit]- List of nearest stars
- List of star systems within 20–25 light-years
- List of star systems within 30–35 light-years
- Lists of stars
- List of nearest bright stars
- Spherical shell
References
[edit]- ^ a b c d e f g h i j k l m n o p q r s t u v w x y z aa ab ac ad ae af ag ah ai aj ak al am an ao ap aq ar as at au av aw ax ay az ba bb bc bd be bf bg bh bi bj bk bl bm bn bo bp bq br bs bt bu bv bw bx by bz ca cb cc cd ce cf Brown, A. G. A.; et al. (Gaia collaboration) (2021). "Gaia Early Data Release 3: Summary of the contents and survey properties". Astronomy & Astrophysics. 649: A1. arXiv:2012.01533. Bibcode:2021A&A...649A...1G. doi:10.1051/0004-6361/202039657. S2CID 227254300. (Erratum: doi:10.1051/0004-6361/202039657e).
- ^ a b c d e van Leeuwen, F. (November 2007), "Validation of the new Hipparcos reduction", Astronomy and Astrophysics, 474 (2): 653–664, arXiv:0708.1752, Bibcode:2007A&A...474..653V, doi:10.1051/0004-6361:20078357, S2CID 18759600
- ^ Staff. "V* alf Lyr – Variable Star". SIMBAD. Centre de Données astronomiques de Strasbourg. Retrieved 2007-10-30.—use the "display all measurements" option to show additional parameters.
- ^ Ducati, J. R. (2002). "VizieR Online Data Catalog: Catalogue of Stellar Photometry in Johnson's 11-color system". CDS/ADC Collection of Electronic Catalogues. 2237: 0. Bibcode:2002yCat.2237....0D.
- ^ "LP 876-10 -- Double or multiple star". SIMBAD. Centre de Données astronomiques de Strasbourg. Retrieved 2014-07-30.
- ^ Houdebine, E. R.; Butler, C. J.; Garcia-Alvarez, D.; Telting, J. (2012). "Observation and modelling of main-sequence star chromospheres - XIX. FIES and FEROS observations of dM1 stars". Monthly Notices of the Royal Astronomical Society. 426 (2): 1591. Bibcode:2012MNRAS.426.1591H. doi:10.1111/j.1365-2966.2012.21787.x.
- ^ Koen, C.; et al. (April 2010). "UBV(RI)C JHK observations of Hipparcos-selected nearby stars". Monthly Notices of the Royal Astronomical Society. 403 (4): 1949–1968. Bibcode:2010MNRAS.403.1949K. doi:10.1111/j.1365-2966.2009.16182.x.
- ^ Henry, Todd J.; Jao, Wei-Chun; Winters, Jennifer G.; Dieterich, Sergio B.; Finch, Charlie T.; Ianna, Philip A.; Riedel, Adric R.; Silverstein, Michele L.; Subasavage, John P.; Vrijmoet, Eliot Halley (2018), "The Solar Neighborhood XLIV: RECONS Discoveries within 10 parsecs", The Astronomical Journal, 155 (6): 265, arXiv:1804.07377, Bibcode:2018AJ....155..265H, doi:10.3847/1538-3881/aac262, S2CID 53983430
- ^ Köhler, R.; Ratzka, T.; Leinert, Ch. (2012). "Orbits and masses in the multiple system LHS 1070". Astronomy & Astrophysics. 541: A29. arXiv:1203.6270. Bibcode:2012A&A...541A..29K. doi:10.1051/0004-6361/201118707. S2CID 119241128.
- ^ Chavez, Joy; Lambert, David L. (2009). "Isotopic Titanium Abundances in Local M Dwarfs". The Astrophysical Journal. 699 (2): 1906–1918. arXiv:0905.2762. Bibcode:2009ApJ...699.1906C. doi:10.1088/0004-637X/699/2/1906. S2CID 16637036.
- ^ a b Davison, Cassy L.; White, R. J.; Henry, T. J.; Riedel, A. R.; Jao, W-C.; Bailey Iii, J. I.; Quinn, S. N.; Cantrell, J. R.; Subasavage, J. P.; Winters, J. G. (2015). "A 3D Search for Companions to 12 Nearby M Dwarfs". The Astronomical Journal. 149 (3): 106. arXiv:1501.05012. Bibcode:2015AJ....149..106D. doi:10.1088/0004-6256/149/3/106. S2CID 9719725.
- ^ Gizis, John E.; Burgasser, Adam J.; Faherty, Jacqueline K.; Castro, Philip J; Shara, Michael M. (2011). "WISEP J180026.60+013453.1: A nearby late-L Dwarf near the Galactic Plane". The Astronomical Journal. 142 (5): 171. arXiv:1109.0054. Bibcode:2011AJ....142..171G. doi:10.1088/0004-6256/142/5/171. S2CID 118596629.
- ^ a b c d e f g h i j k l m n o p q r s t Kirkpatrick, J. Davy; Gelino, Christopher R.; Faherty, Jacqueline K.; Meisner, Aaron M.; Caselden, Dan; Schneider, Adam C.; Marocco, Federico; Cayago, Alfred J.; Smart, R. L.; Eisenhardt, Peter R.; Kuchner, Marc J. (2021). "The Field Substellar Mass Function Based on the Full-sky 20 pc Census of 525 L, T, and y Dwarfs". The Astrophysical Journal Supplement Series. 253 (1): 7. arXiv:2011.11616. Bibcode:2021ApJS..253....7K. doi:10.3847/1538-4365/abd107. S2CID 227126954.
- ^ a b c d Brown, A. G. A.; et al. (Gaia collaboration) (August 2018). "Gaia Data Release 2: Summary of the contents and survey properties". Astronomy & Astrophysics. 616. A1. arXiv:1804.09365. Bibcode:2018A&A...616A...1G. doi:10.1051/0004-6361/201833051.
- ^ a b Benedict, G. F.; Henry, T. J.; Franz, O. G.; McArthur, B. E.; Wasserman, L. H.; Jao, Wei-Chun; Cargile, P. A.; Dieterich, S. B.; Bradley, A. J.; Nelan, E. P.; Whipple, A. L. (2016). "The Solar Neighborhood. XXXVII. The Mass–Luminosity Relation for Main-Sequence M Dwarfs". The Astronomical Journal. 152 (5): 141. arXiv:1608.04775. Bibcode:2016AJ....152..141B. doi:10.3847/0004-6256/152/5/141. S2CID 54029447.
- ^ a b c Benedict, G. F.; Henry, T. J.; Franz, O. G.; McArthur, B. E.; Wasserman, L. H.; Jao, Wei-Chun; Cargile, P. A.; Dieterich, S. B.; Bradley, A. J.; Nelan, E. P.; Whipple, A. L. (2016). "The Solar Neighborhood. Xxxvii. The Mass–Luminosity Relation for Main-Sequence M Dwarfs". The Astronomical Journal. 152 (5): 141. arXiv:1608.04775. Bibcode:2016AJ....152..141B. doi:10.3847/0004-6256/152/5/141. ISSN 1538-3881. S2CID 54029447.
- ^ Faherty, Jacqueline K.; Burgasser, Adam J.; Walter, Frederick M.; Van Der Bliek, Nicole; Shara, Michael M.; Cruz, Kelle L.; West, Andrew A.; Vrba, Frederick J.; Anglada-Escudé, Guillem (2012). "The Brown Dwarf Kinematics Project (BDKP). III. Parallaxes for 70 Ultracool Dwarfs". The Astrophysical Journal. 752 (1): 56. arXiv:1203.5543. Bibcode:2012ApJ...752...56F. doi:10.1088/0004-637X/752/1/56. S2CID 18160586.
- ^ Winters, Jennifer G.; Henry, Todd J.; Lurie, John C.; Hambly, Nigel C.; Jao, Wei-Chun; Bartlett, Jennifer L.; Boyd, Mark R.; Dieterich, Sergio B.; Finch, Charlie T.; Hosey, Altonio D. (2015). "The Solar Neighborhood. XXXV. Distances to 1404 M Dwarf Systems within 25 Pc in the Southern Sky". The Astronomical Journal. 149 (1): 5. arXiv:1401.0722. Bibcode:2015AJ....149....5W. doi:10.1088/0004-6256/149/1/5. S2CID 16953825.
- ^ a b Dittmann, Jason A.; Irwin, Jonathan M.; Charbonneau, David; Berta-Thompson, Zachory K. (2014). "Trigonometric Parallaxes for 1507 Nearby Mid-To-Late M Dwarfs". The Astrophysical Journal. 784 (2): 156. arXiv:1312.3241. Bibcode:2014ApJ...784..156D. doi:10.1088/0004-637X/784/2/156. ISSN 0004-637X. S2CID 18789867.
- ^ Johnson, H. L.; Morgan, W. W. (1953). "Fundamental stellar photometry for standards of spectral type on the revised system of the Yerkes spectral atlas". Astrophysical Journal. 117: 313–352. Bibcode:1953ApJ...117..313J. doi:10.1086/145697.
- ^ a b c Winters, Jennifer G.; Henry, Todd J.; Lurie, John C.; Hambly, Nigel C.; Jao, Wei-Chun; Bartlett, Jennifer L.; Boyd, Mark R.; Dieterich, Sergio B.; Finch, Charlie T.; Hosey, Altonio D. (2015). "The Solar Neighborhood. XXXV. Distances to 1404 M Dwarf Systems within 25 Pc in the Southern Sky". The Astronomical Journal. 149 (1): 5. arXiv:1401.0722. Bibcode:2015AJ....149....5W. doi:10.1088/0004-6256/149/1/5. S2CID 16953825.
- ^ Sion, Edward M.; Holberg; Oswalt; McCook; Wasatonic (2009). "The White Dwarfs within 20 Parsecs of the Sun: Kinematics and Statistics". The Astronomical Journal. 138 (6): 1681–1689. arXiv:0910.1288. Bibcode:2009AJ....138.1681S. doi:10.1088/0004-6256/138/6/1681. S2CID 119284418.
- ^ "V* V1201 Ori -- White Dwarf". Centre de Données astronomiques de Strasbourg. Retrieved 2011-11-01.
- ^ Affer, L.; Damasso, M.; Micela, G.; Poretti, E.; Scandariato, G.; Maldonado, J.; Lanza, A. F.; Covino, E.; Garrido Rubio, A.; González Hernández, J. I.; Gratton, R.; Leto, G.; Maggio, A.; Perger, M.; Sozzetti, A.; Suárez Mascareño, A.; Bonomo, A. S.; Borsa, F.; Claudi, R.; Cosentino, R.; Desidera, S.; Giacobbe, P.; Molinari, E.; Pedani, M.; Pinamonti, M.; Rebolo, R.; Ribas, I.; Toledo-Padrón, B. (2019). "HADES RV program with HARPS-N at the TNG". Astronomy & Astrophysics. 622: A193. arXiv:1901.05338. doi:10.1051/0004-6361/201834868. S2CID 118863481.
- ^ "GJ 293 -- White Dwarf". Centre de Données astronomiques de Strasbourg. Retrieved 2011-10-30.
- ^ Holberg, J. B.; Sion; Oswalt; McCook; Foran; Subasavage (2008). "A New Look at the Local White Dwarf Population". The Astronomical Journal. 135 (4): 1225–1238. Bibcode:2008AJ....135.1225H. doi:10.1088/0004-6256/135/4/1225. S2CID 122855486.
- ^ a b Kirkpatrick, J. Davy; Martin, Emily C.; Smart, Richard L.; Cayago, Alfred J.; Beichman, Charles A.; Marocco, Federico; et al. (February 2019). "Preliminary Trigonometric Parallaxes of 184 Late-T and Y Dwarfs and an Analysis of the Field Substellar Mass Function into the "Planetary" Mass Regime". The Astrophysical Journal Supplement Series. 240 (2): 69. arXiv:1812.01208. Bibcode:2019ApJS..240...19K. doi:10.3847/1538-4365/aaf6af. 19.
- ^ Torres, G.; Andersen, J.; Giménez, A. (2010). "Accurate masses and radii of normal stars: modern results and applications". The Astronomy & Astrophysics Review. 18 (1–2): 67–126. arXiv:0908.2624. Bibcode:2010A&ARv..18...67T. doi:10.1007/s00159-009-0025-1. S2CID 14006009.
- ^ a b c d Subasavage, John P.; Jao, Wei-Chun; Henry, Todd J.; Harris, Hugh C.; Dahn, Conard C.; Bergeron, P.; Dufour, P.; Dunlap, Bart H.; Barlow, Brad N.; Ianna, Philip A.; Lépine, Sébastien; Margheim, Steven J. (2017). "The Solar Neighborhood. XXXIX. Parallax Results from the CTIOPI and NOFS Programs: 50 New Members of the 25 parsec White Dwarf Sample". The Astronomical Journal. 154 (1): 32. arXiv:1706.00709. Bibcode:2017AJ....154...32S. doi:10.3847/1538-3881/aa76e0. S2CID 119189852.
- ^ Moutou, C.; Ould-Elhkim, M.; et al. (June 2024). "Characterizing planetary systems with SPIRou: a temperate sub-Neptune exoplanet orbiting the nearby fully-convective star GJ 1289 and a candidate around GJ 3378". Astronomy & Astrophysics. arXiv:2406.10384.
- ^ Henry, Todd J.; Jao, Wei-Chun; Subasavage, John P.; Beaulieu, Thomas D.; Ianna, Philip A.; Costa, Edgardo; Méndez, René A. (January 2006). "The Solar Neighborhood. XVII. Parallax Results from the CTIOPI 0.9 m Program: 20 New Members of the RECONS 10 Parsec Sample" (PDF). The Astronomical Journal. 132 (6): 2360–2371. arXiv:astro-ph/0608230. Bibcode:2006AJ....132.2360H. doi:10.1086/508233. S2CID 15002841.
- ^ Bauer, F. F.; Zechmeister, M.; et al. (August 2020). "The CARMENES search for exoplanets around M dwarfs. Measuring precise radial velocities in the near infrared: The example of the super-Earth CD Cet b". Astronomy & Astrophysics. 640: A50. arXiv:2006.01684. Bibcode:2020A&A...640A..50B. doi:10.1051/0004-6361/202038031.
- ^ Kirkpatrick, J. Davy; Cushing, Michael C.; Gelino, Christopher R.; Griffith, Roger L.; Skrutskie, Michael F.; Marsh, Kenneth A.; Wright, Edward L.; Mainzer, Amy K.; Eisenhardt, Peter R.; McLean, Ian S.; Thompson, Maggie A.; Bauer, James M.; Benford, Dominic J.; Bridge, Carrie R.; Lake, Sean E.; Petty, Sara M.; Stanford, Spencer Adam; Tsai, Chao-Wei; Bailey, Vanessa; Beichman, Charles A.; Bloom, Joshua S.; Bochanski, John J.; Burgasser, Adam J.; Capak, Peter L.; Cruz, Kelle L.; Hinz, Philip M.; Kartaltepe, Jeyhan S.; Knox, Russell P.; Manohar, Swarnima; Masters, Daniel; Morales-Calderon, Maria; Prato, Lisa A.; Rodigas, Timothy J.; Salvato, Mara; Schurr, Steven D.; Scoville, Nicholas Z.; Simcoe, Robert A.; Stapelfeldt, Karl R.; Stern, Daniel; Stock, Nathan D.; Vacca, William D. (2011). "The First Hundred Brown Dwarfs Discovered by the Wide-field Infrared Survey Explorer (WISE)". The Astrophysical Journal Supplement. 197 (2): 19. arXiv:1108.4677v1. Bibcode:2011ApJS..197...19K. doi:10.1088/0067-0049/197/2/19. S2CID 16850733.
- ^ a b c Humphreys, Austin; Meisner, Aaron M.; Burgasser, Adam J.; Hsu, Chih-Chun; Schneider, Adam C.; Theissen, Christopher A.; Aganze, Christian; Gerasimov, Roman; Schapera, Noah; Kirkpatrick, J. Davy; Marocco, Federico; Faherty, Jacqueline K.; Caselden, Dan; Kuchner, Marc J.; Cushing, Michael C. (August 2023). "Spectroscopic Confirmation of the Nearby, Wide-separation L Dwarf Pair CWISE J061741.79+194512.8AB". Research Notes of the AAS. 7 (8): 184. doi:10.3847/2515-5172/acf4a0. ISSN 2515-5172.
- ^ "Gliese 3517".
- ^ Jenkins, J. S.; Díaz, M.; Jones, H. R. A.; Butler, R. P.; Tinney, C. G.; O'Toole, S. J.; Carter, B. D.; Wittenmyer, R. A.; Pinfield, D. J. (2015). "The observed distribution of spectroscopic binaries from the Anglo-Australian Planet Search". Monthly Notices of the Royal Astronomical Society. 453 (2): 1439–1457. arXiv:1507.04749. Bibcode:2015MNRAS.453.1439J. doi:10.1093/mnras/stv1596. ISSN 0035-8711. S2CID 53350848.
{{cite journal}}
: CS1 maint: unflagged free DOI (link) - ^ Discovery of a nearby M9 dwarf: DENIS 0334-49. 2006.
- ^ Dupuy, Trent J.; Liu, Michael C. (2012). "The Hawaii Infrared Parallax Program. I. Ultracool Binaries and the L/T Transition". The Astrophysical Journal Supplement. 201 (2): 19. arXiv:1201.2465. Bibcode:2012ApJS..201...19D. doi:10.1088/0067-0049/201/2/19. S2CID 119256363.
- ^ a b c Lodieu, N.; Zapatero Osorio, M. R.; Martin, E. L.; Rebolo Lopez, R.; Gauza, B. (2022-06-01). "Physical properties and trigonometric distance of the peculiar dwarf WISE J181005.5$-$101002.3". Astronomy & Astrophysics. 663. arXiv:2206.13097. Bibcode:2022A&A...663A..84L. doi:10.1051/0004-6361/202243516. S2CID 249836684.
- ^ Tinney, C. G.; Faherty, Jacqueline K.; Kirkpatrick, J. Davy; Cushing, Mike; Morley, Caroline V.; Wright, Edward L. (2014). "The Luminosities of the Coldest Brown Dwarfs". The Astrophysical Journal. 796 (1): 39. arXiv:1410.0746. Bibcode:2014ApJ...796...39T. doi:10.1088/0004-637X/796/1/39. S2CID 9038276.
- ^ Jao (饒惟君), Wei-Chun; Henry, Todd J.; Riedel, Adric R.; Winters, Jennifer G.; Slatten, Kenneth J.; Gies, Douglas R. (2016). "Distance-Dependent Offsets Between Parallaxes for Nearby Stars and Gaia Dr1 Parallaxes". The Astrophysical Journal. 832 (1): L18. arXiv:1611.00656. Bibcode:2016ApJ...832L..18J. doi:10.3847/2041-8205/832/1/L18. ISSN 2041-8213. S2CID 27256626.