List of nearest bright stars

Last updated August 03, 2024

This list of nearest bright stars is a table of stars found within 15 parsecs (48.9 light-years) of the nearest star, the Sun, that have an absolute magnitude of +8.5 or brighter, which is approximately comparable to a listing of stars more luminous than a red dwarf. Right ascension and declination coordinates are for the epoch J2000. The distance measurements are based on the Hipparcos Catalogue and other astrometric data. In the event of a spectroscopic binary, the combined spectral type and absolute magnitude are listed in italics.

Stars within 10 parsecs

These stars are estimated to be within 32.6 light-years of the Sun.

Star Designation		Stellar Class	Magnitude		Right Ascension (J2000)	Declination (J2000)	Distance (Light-years)
Star Designation		Stellar Class	Apparent	Absolute	Right Ascension (J2000)	Declination (J2000)	Distance (Light-years)
Sun		G2V	−26.74	4.80	—	—	0
α Centauri	A	G2V	−0.01	4.34	14^h 39^m 36.50^s	−60° 50′ 02.3″	4.34
α Centauri	B	K1V	1.35	5.71	14^h 39^m 35.08^s	−60° 50′ 13.8″	4.34
Sirius (α Canis Majoris)		A1V	−1.44	1.45	06^h 45^m 08.92^s	−16° 42′ 58.0″	8.60
ε Eridani		K2V	3.72	6.18	03^h 32^m 55.84^s	−09° 27′ 29.7″	10.5
61 Cygni	A	K5.0V	5.20	7.49	21^h 06^m 53.94^s	+38° 44′ 57.9″	11.4
61 Cygni	B	K7.0V	6.05	8.33	21^h 06^m 53.94^s	+38° 44′ 57.9″	11.4
Procyon (α Canis Minoris)	A	F5IV-V	0.40	2.68	07^h 39^m 18.12^s	+05° 13′ 30.0″	11.5
ε Indi		K5Ve	4.69	6.90	22^h 03^m 21.66^s	−56° 47′ 09.5″	11.9
τ Ceti		G8Vp	3.49	5.68	01^h 44^m 04.08^s	−15° 56′ 14.9″	11.9
Groombridge 1618 (in Ursa Major)		K7.0V	6.60	8.16	10^h 11^m 22.14^s	+49° 27′ 15.3″	15.9
ο² Eridani	A	K1Ve	4.43	5.92	04^h 15^m 16.32^s	−07° 39′ 10.3″	16.3
70 Ophiuchi	A	K1Ve	4.24	5.71	18^h 05^m 27.29^s	+02° 30′ 00.4″	16.7
70 Ophiuchi	B	K5Ve	6.01	7.48	18^h 05^m 27.29^s	+02° 30′ 00.4″	16.7
Altair (α Aquilae)		A7Vn	0.76	2.21	19^h 50^m 47.00^s	+08° 52′ 06.0″	16.7
σ Draconis		G9V	4.67	5.87	19^h 32^m 21.59^s	+69° 39′ 40.2″	18.8
Gliese 570 (in Libra)	A	K5Ve	5.72	6.86	14^h 57^m 28.00^s	−21° 24′ 55.7″	19.2
η Cassiopeiae	A	G3V	3.46	4.59	00^h 49^m 06.29^s	+57° 48′ 54.7″	19.3
36 Ophiuchi	A	K1Ve	5.07	6.18	17^h 15^m 20.98^s	−26° 36′ 10.2″	19.4
	B	K1Ve	5.11	6.22	17^h 15^m 20.98^s	−26° 36′ 10.2″
	C	K5Ve	6.33	7.45	17^h 16^m 13.36^s	−26° 32′ 46.1″
HR 7703 (in Sagittarius)	A	K3V	5.32	6.42	20^h 11^m 11.94^s	−36° 06′ 04.4″	19.6
82 G. Eridani		G8V	4.26	5.35	03^h 19^m 55.65^s	−43° 04′ 11.2″	19.7
δ Pavonis		G7IV	3.55	4.62	20^h 08^m 42.61^s	−66° 10′ 55.4″	19.9
HD 219134 / Gliese 892 (in Cassiopeia)		K3V	5.57	6.49	23^h 13^m 16.98^s	+57° 10′ 06.1″	21.3
ξ Boötis	A	G8Ve	4.72	5.59	14^h 51^m 23.38^s	+19° 06′ 01.7″	22.0
ξ Boötis	B	K4Ve	6.97	7.84	14^h 51^m 23.38^s	+19° 06′ 01.7″	22.0
Gliese 667 (in Scorpius)	A	K3V	6.29	7.07	17^h 18^m 57.18^s	−34° 59′ 23.3″	23.2
Gliese 667 (in Scorpius)	B	K5V	7.24	8.02	17^h 18^m 57.18^s	−34° 59′ 23.3″	23.2
Gliese 105 (in Cetus)	A	K3V	5.79	6.50	02^h 36^m 04.89^s	+06° 53′ 12.7″	23.4
HD 4628 (in Pisces)		K2V	5.74	6.38	00^h 48^m 22.98^s	+05° 16′ 50.2″	24.3
β Hydri		G2IV	2.82	3.46	00^h 25^m 45.07^s	−77° 15′ 15.2″	24.3
107 Piscium		K1V	5.24	5.86	01^h 42^m 29.76^s	+20° 16′ 06.6″	24.4
μ Cassiopeiae	A	G5VI	5.17	5.78	01^h 08^m 16.39^s	+54° 55′ 13.2″	24.6
TW Piscis Austrini	B	K5Ve	6.48	7.07	22^h 56^m 24.05^s	−31° 33′ 56.0″	24.8
Vega (α Lyrae)		A0Va	0.03	0.58	18^h 36^m 56.34^s	+38° 47′ 01.3″	25.0
Fomalhaut (α Piscis Austrini/α PsA)	A	A3V	1.17	1.74	22^h 57^m 39.05^s	−29° 37′ 20.1″	25.1
Gliese 673 (in Ophiuchus)		K7V	7.54	8.10	17^h 25^m 45.23^s	+02° 06′ 41.1″	25.1
p Eridani	A	K0V	5.82	6.27	01^h 39^m 47.54^s	−56° 11′ 47.0″	25.5
p Eridani	B	K5V	5.95	6.40	01^h 39^m 47.54^s	−56° 11′ 47.0″	25.5
π³ Orionis		F6V	3.19	3.67	04^h 49^m 50.41^s	+06° 57′ 40.6″	26.3
χ Draconis	A	F7V	3.68	4.15	18^h 21^m 03.38^s	+72° 43′ 58.2″	26.3
χ Draconis	B	K0V	5.67	6.14	18^h 21^m 03.38^s	+72° 43′ 58.2″	26.3
Gliese 884 (in Aquarius)		K5	7.88	8.33	23^h 00^m 16.12^s	−22° 31′ 27.6″	26.6
μ Herculis		G5IV	3.42	3.80	17^h 46^m 27.53^s	+27° 43′ 14.4″	27.1
β Canum Venaticorum		G0V	4.24	4.63	12^h 33^m 44.54^s	+41° 21′ 26.9″	27.5
61 Virginis		G5V	4.74	5.09	13^h 18^m 24.31^s	−18° 18′ 40.3″	27.9
ζ Tucanae		F9V	4.23	4.56	00^h 20^m 04.26^s	−64° 52′ 29.2″	28.0
χ¹ Orionis	A	G0V	4.39	4.70	05^h 54^m 22.98^s	+20° 16′ 34.2″	28.3
HD 50281 (in Monoceros)	A	K3V	6.58	6.88	06^h 52^m 18.05^s	−05° 10′ 25.4″	28.4
HR 1614 (284 G. Eridani)	A	K3V	6.22	6.49	05^h 00^m 49.00^s	−05° 45′ 13.2″	28.4
41 G. Arae	A	G8V	5.55	5.83	17^h 19^m 03.83^s	−46° 38′ 10.4″	28.7
ξ Ursae Majoris	A	G0V	4.41	4.25	11^h 18^m 11^s	+31° 31′ 45″	28.8
ξ Ursae Majoris	B	G5V	4.87	5.07	11^h 18^m 11^s	+31° 31′ 45″	28.8
HD 192310/Gliese 785 (5 G. Capricorni)		K2+V	5.73	6.00	20^h 15^m 7.39^s	−27° 01′ 58.7″	29.1
γ Leporis	A	F7V	3.59	3.83	05^h 44^m 27.79^s	−22° 26′ 54.2″	29.3
γ Leporis	B	K2V	6.17	6.41	05^h 44^m 27.79^s	−22° 26′ 54.2″	29.3
δ Eridani		K0IV	3.52	3.74	03^h 43^m 14.90^s	−09° 45′ 48.2″	29.5
Groombridge 1830 (in Ursa Major)		G8Vp	6.42	6.61	11^h 52^m 58.77^s	+37° 43′ 07.2″	29.7
β Comae Berenices		G0V	4.23	4.42	13^h 11^m 52.39^s	+27° 52′ 41.5″	29.8
κ¹ Ceti		G5V	4.84	5.03	03^h 19^m 21.70^s	+03° 22′ 12.7″	29.8
HD 102365 (in Centaurus)	A	G3V	4.89	5.06	11^h 46^m 31.07^s	−40° 30′ 01.3″	30.1
γ Pavonis		F6V	4.21	4.39	21^h 26^m 26.61^s	−65° 21′ 58.3″	30.2
61 Ursae Majoris		G8V	5.31	5.41	11^h 41^m 03.02^s	+34° 12′ 05.9″	31.1
HR 4458 (in Hydra)	A	K0V	5.96	6.06	11^h 34^m 29.49^s	−32° 49′ 52.8″	31.2
12 Ophiuchi		K2V	5.77	5.82	16^h 36^m 21.45^s	−02° 19′ 28.5″	31.8
Gliese 638 (in Hercules)		K7V	8.10	8.15	16^h 45^m 06.35^s	+33° 30′ 33.2″	31.9

Stars between 10 and 13 parsecs

These stars are estimated to be from 32.7 to 42.4 light years distant from the Sun.

Star Designation		Stellar Class	Magnitude		Right Ascension (J2000)	Declination (J2000)	Distance (Light-years)
Star Designation		Stellar Class	Apparent	Absolute	Right Ascension (J2000)	Declination (J2000)	Distance (Light-years)
HR 511		K0V	5.63	5.61	01^h 47^m 44.83^s	+63° 51′ 09.0″	32.8
HR 5256		K3V	6.49	6.47	13^h 57^m 32.06^s	+61° 29′ 34.3″	33.0
α Mensae		G5V	5.08	5.05	06^h 10^m 13.93^s	−74° 45′ 11.0″	33.1
Gliese 453		K4V	6.99	6.95	11^h 57^m 57.63^s	−27° 42′ 25.4″	33.2
Pollux		K0IIIb	1.16	1.09	07^h 45^m 18.95^s	+28° 01′ 34.3″	33.7
HD 17925 (32 G. Eridani)		K1V	6.05	5.97	02^h 52^m 31.65^s	−12° 46′ 11.0″	33.9
ι Persei		G0V	4.05	3.94	03^h 09^m 04.02^s	+49° 36′ 47.8″	34.4
Wolf 635	A	K7 V	7.70	7.54	17^h 05^m 04.47^s	−05° 03′ 59.4″	35.1
HR 9038	A	K3V	6.36	6.19	23^h 52^m 25.32^s	+75° 32′ 40.5″	35.2
ζ Herculis	A	F9IV	2.91	2.74	16^h 41^m 17.16^s	+31° 36′ 09.8″	35.2
ζ Herculis	B	G7V	5.43	5.26	16^h 41^m 17.16^s	+31° 36′ 09.8″	35.2
δ Trianguli		G0V	4.84	4.66	02^h 17^m 03.23^s	+34° 13′ 27.2″	35.4
β Virginis		F8V	3.59	3.40	11^h 50^m 41.72^s	+01° 45′ 53.0″	35.6
Gliese 86	A	K0V	6.12	5.93	02^h 10^m 22.07^s	−50° 49′ 25.4″	35.6
Gliese 688	A	K3V	6.53	6.38	17^h 39^m 16.92^s	+03° 33′ 18.9″	35.9
HR 6806		K2V	6.38	6.15	18^h 09^m 37.42^s	+38° 27′ 28.0″	36.0
Gliese 505	A	K1V	6.52	6.27	13^h 16^m 51.05^s	+17° 01′ 01.8″	36.1
Denebola		A3Vvar	2.14	1.92	11^h 49^m 03.58^s	+14° 34′ 19.4″	36.2
54 Piscium		K0V	5.88	5.65	00^h 39^m 21.81^s	+21° 15′ 01.7″	36.2
γ Serpentis		F6V	3.85	3.62	15^h 56^m 27.18^s	+15° 39′ 41.8″	36.3
Gliese 320		K2V	6.58	6.35	08^h 43^m 18.48^s	−38° 52′ 56.6″	36.3
Gliese 370		K5V	7.67	7.43	09^h 51^m 06.31^s	−43° 30′ 10.0″	36.4
11 Leonis Minoris	A	G8V	5.40	5.16	09^h 35^m 39.50^s	+35° 48′ 36.5″	36.5
θ Persei	A	F7V	4.10	3.85	02^h 44^m 11.99^s	+49° 13′ 42.4″	36.6
Arcturus (α Boötis)		K1.5III	−0.05	−0.31	14^h 15^m 39.67^s	+19° 10′ 56.7″	36.7
η Boötis	A/B	G0IV	2.68	2.41	13^h 54^m 41.08^s	+18° 23′ 51.8″	37.0
Gliese 902		K3V	7.09	6.81	23^h 39^m 36.83^s	−72° 43′ 19.8″	37.2
Gliese 169		K7V	8.30	8.00	04^h 29^m 00.12^s	+21° 55′ 21.7″	37.4
HR 5553	A/B	K2V	6.00	5.69	14^h 53^m 23.77^s	+19° 09′ 10.1″	37.6
ζ Doradus	A	F7V	4.71	4.38	05^h 05^m 30.72^s	−57° 28′ 21.7″	38.0
λ Serpentis		G0Vvar	4.42	4.07	15^h 46^m 26.61^s	+07° 21′ 11.1″	38.3
ι Pegasi	A/B	F5V	3.77	3.42	22^h 07^m 00.67^s	+25° 20′ 42.4″	38.3
δ Capricorni	A	A5IV	2.73–2.93	2.37	21^h 47^m 02.13^s	−16° 07′ 38.2″	38.6
γ Virginis	A	F0V	3.46	3.10	12^h 41^m 40.36^s	−01° 26′ 57.7″	38.6
γ Virginis	B	F0V	3.52	3.16	12^h 41^m 40.36^s	−01° 26′ 57.7″	38.6
Gliese 542		K3V	6.66	6.29	14^h 19^m 05.88^s	−59° 22′ 44.5″	38.6
Gliese 414 (nl)	A	K7V	8.30	7.92	11^h 11^m 05.2^s	+30° 26′ 45.6″	38.9
ζ² Reticuli		G1V	5.24	4.83	03^h 18^m 09.45^s	−62° 30′ 22.9″	39.4
ζ Trianguli Australis		F9V	4.91	4.50	16^h 28^m 27.46^s	−70° 05′ 03.8″	39.5
ζ¹ Reticuli		G2V	5.53	5.11	03^h 17^m 42.77^s	−62° 34′ 31.2″	39.5
Gliese 798		K7 V	8.83	8.41	20^h 42^m 18.72^s	−52° 41′ 57.1″	39.5
HR 3384		G9V	6.38	5.95	08^h 32^m 52.91^s	−31° 30′ 03.1″	39.8
V538 Aurigae		K1Ve	6.21	5.77	05^h 41^m 20.33^s	+53° 28′ 51.8″	39.9
β Trianguli Australis	A	F2III	2.83	2.38	15^h 55^m 08.92^s	−63° 25′ 50.6″	40.1
85 Pegasi	A	G3V	5.81	5.34	00^h 02^m 10.10^s	+27° 04′ 56.1″	40.5
85 Pegasi	B	K6V	8.88	8.41	00^h 02^m 10.10^s	+27° 04′ 56.1″	40.5
Gliese 435 (es)		K5V	7.77	7.28	11^h 41^m 03.55^s	−44° 24′ 18.7″	40.8
ρ¹ Cancri	A	G8V	5.96	5.47	08^h 52^m 35.85^s	+28° 19′ 50.9″	40.9
HD 69830 (285 G. Puppis)		K0V	5.95	5.45	08^h 18^m 23.62^s	−12° 37′ 55.8″	41.0
Gliese 67	A	G1.5V	4.95	4.30	01^h 41^m 47.1^s	+42° 36′ 48.1″	41.2
λ Aurigae		G0V	4.69	4.18	05^h 19^m 08.38^s	+40° 05′ 56.6″	41.2
HD 14412 (22 G. Fornacis)		G8V	6.33	5.81	02^h 18^m 58.77^s	−25° 56′ 44.5″	41.3
HD 104304 (24 G. Virginis)		K0IV	5.54	4.99	12^h 00^m 44.28^s	−10° 26′ 45.7″	41.6
44 Boötis	A	F9V	5.20	4.67	15^h 03^m 47.43^s	+47° 39′ 14.6″	41.6
44 Boötis	B/C	G2V	5.97	5.44	15^h 03^m 47.43^s	+47° 39′ 14.6″	41.6
Gliese 675		K0V	6.44	5.90	17^h 25^m 00.59^s	+67° 18′ 24.1″	41.7
Gliese 2046		K3V	7.17	6.63	05^h 54^m 04.33^s	−60° 01′ 24.5″	41.8
36 Ursae Majoris	A	F8V	4.82	4.28	10^h 30^m 37.66^s	+55° 58′ 49.9″	41.9
HD 147513 (62 G. Scorpii)		G3V	5.37	4.82	16^h 24^m 01.19^s	−39° 11′ 34.7″	42.0
Gliese 428 (it)	A	K7V	7.51	6.96	11^h 24^m 41.24^s	−61° 38′ 51.2″	42.0
Gliese 428 (it)	B	M0Ve	8.82	8.27	11^h 24^m 41.24^s	−61° 38′ 51.2″	42.0
Gliese 349 (es)		K3V	7.20	6.68	09^h 29^m 54.82^s	+05° 39′ 18.5″	42.1

Stars between 13 and 15 parsecs

These stars are estimated to be from 42.5 to 48.9 light years distant from the Sun. A value of 48.9 light years corresponds to a minimum parallax of 66.7 mas.

Star Designation		Stellar Class	Magnitude		Right Ascension (J2000)	Declination (J2000)	Distance (Light-years)
Star Designation		Stellar Class	Apparent	Absolute	Right Ascension (J2000)	Declination (J2000)	Distance (Light-years)
HD 36003 (it)		K5V	7.65	7.08	05^h 28^m 26^s	−03° 29′ 58″	42.5
HD 172051 (86 G. Sagittarii)		G5V	5.85	5.28	18^h 38^m 53.49^s	−21° 03′ 06.7″	42.6
HD 166348 [ it ]		K7V	8.23	7.65	18^h 12^m 21^s	−43° 26′ 41″	42.6
Gliese 167		K5V	7.62	7.03	04^h 15^m 57^s	−53° 18′ 35″	42.8
Capella	Aa	G5III	0.76	0.20	05^h 16^m 41.34^s	+45° 59′ 52.8″	42.9
Capella	Ab	G1III	0.91	0.35	05^h 16^m 41.34^s	+45° 59′ 52.8″	42.9
SZ Crateris	A	K5V	8.61	8.0	11^h 21^m 27^s	−20° 27′ 14″	42.9
Gliese 716		K2V	6.81	6.21	18^h 31^m 19^s	−18° 54′ 30″	43.1
Gliese 146		K5V	8.95	8.34	03^h 35^m 01^s	−48° 25′ 09″	43.1
V1654 Aquilae		K4V	7.45	6.84	20^h 02^m 47^s	+03° 19′ 34″	43.1
Gliese 69		K5V	8.35	7.74	01^h 43^m 41^s	+63° 49′ 24″	43.1
58 Eridani		G1V	5.63	5.01	04^h 47^m 36^s	−16° 56′ 04″	43.4
Gliese 528 [ it ]	A	K4V	7.96	7.32	13^h 49^m 04^s	+26° 58′ 47″	43.7
Gliese 528 [ it ]	B	K6V	8.35	7.71	13^h 49^m 04^s	+26° 58′ 47″	43.7
υ Andromedae	A	F8V	4.10	4.63	01^h 36^m 48^s	+41° 24′ 20″	43.7
Gliese 556 [ it ]		K3V	7.32	6.67	14^h 33^m 29^s	+52° 54′ 32″	44.0
θ Ursae Majoris		F6IV	3.02	2.37	09^h 32^m 52^s	+51° 40′ 43″	44.0
LHS 3508 [ it ]		K5V	7.91	7.24	20^h 02^m 35^s	−50° 03′ 06″	44.3
V834 Tau		K3V	8.03	7.36	04^h 41^m 19^s	+20° 54′ 05″	44.4
Gliese 853	A	G1-3V	5.33	4.66	22^h 18^m 15^s	−53° 37′ 32″	44.4
Gliese 868		K5V	7.93	7.25	22^h 40^m 43^s	−29° 40′ 28″	44.5
Gliese 5		G8V	5.92	5.23	00^h 06^m 37^s	+29° 01′ 19″	44.7
β Aquilae	A	G8IV	3.75	3.06	19^h 55^m 19^s	+06° 24′ 29″	44.7
10 Tauri		F9V	4.29	3.60	03^h 36^m 53^s	+00° 24′ 10″	44.7
Gliese 656		K0V	7.28	6.58	17^h 10^m 10^s	−60° 43′ 44″	44.9
ι Piscium		F7V	4.06	3.36	23^h 39^m 57^s	+05° 37′ 38″	45.0
γ Cephei	A	K1IV	2.94	2.24	23^h 39^m 21^s	+77° 37′ 56″	45.0
Gliese 615		K0V	7.36	6.66	16^h 13^m 49^s	−57° 34′ 14″	45.1
Gliese 898		K5/M0V	8.38	7.68	23^h 32^m 49^s	−16° 50′ 44″	45.1
36 Ursae Majoris	B	K7Ve	8.77	8.06	10^h 30^m 25^s	+56° 00′ 00″	45.2
18 Scorpii		G1V	5.50	4.76	16^h 15^m 37^s	−08° 22′ 06″	45.3
HD 23356 [ nl ]		K2V	7.1	6.4	03^h 43^m 56^s	−19° 06′ 42″	45.5
τ¹ Eridani	A/B	F5/F6V	4.47	3.74	02^h 45^m 06^s	−18° 34′ 22″	45.5
Gliese 529		K5.5Vk	8.36	7.62	13^h 49^m 45^s	−22° 06′ 40″	45.9
Gliese 726		K5	8.91	8.17	18^h 47^m 27^s	−03° 38′ 23″	45.9
Gliese 282	A	K2V	7.26	6.52	07^h 39^m 59^s	−03° 35′ 51″	45.9
Gliese 282	B	K5	9.02	8.28	07^h 39^m 59^s	−03° 35′ 51″	45.9
47 Ursae Majoris		G0V	5.03	4.29	10^h 59^m 28^s	+40° 25′ 48″	45.9
Gliese 532 [ it ]		K5	8.99	8.24	13^h 52^m 00^s	+49° 57′ 03″	46.0
26 Draconis	A	F9V	5.06	4.31	17^h 34^m 60^s	+61° 52′ 30″	46.0
26 Draconis	B	K3V	7.95	7.20	17^h 34^m 60^s	+61° 52′ 30″	46.0
α Fornacis	A	F7IV	3.80	3.05	03^h 12^m 04^s	−28° 59′ 21″	46.0
α Fornacis	B	G7V	6.73	5.98	03^h 12^m 04^s	−28° 59′ 21″	46.0
Gliese 42		K2V	7.48	6.72	00^h 53^m 01^s	−30° 21′ 25″	46.2
Gliese 481 [ it ]		K4V	7.91	7.13	12^h 41^m 06^s	+15° 22′ 36″	46.2
Gliese 611 [ it ]	A	G8V	6.71	5.94	16^h 04^m 57^s	+39° 09′ 23″	46.4
HD 150689 [ nl ]		K2V	7.39	6.62	16^h 44^m 14^s	−38° 56′ 36″	46.4
HR 7578		K3V	6.23	5.46	19^h 54^m 18^s	−23° 56′ 28″	46.4
π¹ Ursae Majoris		G1V	5.63	4.86	08^h 39^m 12^s	+65° 01′ 15″	46.6
Ras Alhague	A	A5III	2.08	1.30	17^h 34^m 56^s	+12° 33′ 36″	46.7
η Cephei		K0IV	3.42	2.63	20^h 45^m 17^s	+61° 50′ 20″	46.8
Gliese 613		K3V	7.12	6.33	16^h 09^m 43^s	−56° 26′ 46″	46.8
72 Herculis		G0V	5.38	4.59	17^h 20^m 39^s	+32° 28′ 13″	46.9
Gliese 796		G8V	6.37	5.58	20^h 40^m 12^s	−23° 46′ 24″	46.9
Gliese 481		K2	7.86	7.07	12^h 41^m 06^s	+15° 22′ 36″	47.0
Gliese 546 [ nl ]		K5V	8.37	7.57	14^h 21^m 57^s	+29° 37′ 47″	47.1
Gliese 420 [ nl ]		dK5	8.06	7.26	11^h 15^m 12^s	+73° 28′ 31″	47.1
ν² Lupi		G2V	5.66	4.84	15^h 21^m 48^s	−48° 19′ 04″	47.5
θ Boötis	A	F7V	4.10	3.28	14^h 25^m 12^s	+51° 51′ 06″	47.5
Gliese 269 [ it ]	A	K2V	8.08	7.26	07^h 17^m 30^s	−46° 58′ 45″	47.6
Gliese 833 [ it ]		K2V	7.31	6.48	21^h 36^m 41^s	−50° 50′ 43″	47.7
ι Ursae Majoris	A	A7V	3.23	2.40	08^h 59^m 13^s	+48° 02′ 32″	47.7
Gliese 259 [ nl ]		K1V	6.88	6.05	07^h 01^m 14^s	−25° 56′ 55″	47.7
111 Tauri	A	F8V	5.00	4.17	05^h 24^m 25^s	+17° 23′ 00″	47.8
111 Tauri	B	dK5e	7.83	7.00	05^h 23^m 38^s	+17° 19′ 27″	47.8
ψ Serpentis		G5V	5.86	5.03	15^h 44^m 02^s	+02° 30′ 55″	47.8
Gliese 604 [ nl ]		K5V	8.05	7.22	15^h 57^m 41^s	−42° 37′ 27″	47.8
ψ Capricorni		F5V	4.14	3.30	20^h 46^m 06^s	−25° 16′ 14″	47.9
HD 97584	A	K4V	7.68	6.85	11^h 15^m 12^s	+73° 28′ 31″	47.9
HD 19305		M0V	9.05	8.21	03^h 06^m 27^s	+01° 57′ 55″	48
OU Geminorum		K2Ve	6.76	5.91	06^h 26^m 10^s	+18° 45′ 25″	48.2
α Corvi		F2V	4.02	3.17	12^h 08^m 25^s	−24° 43′ 44″	48.2
20 Leonis Minoris	A	G3Va	5.40	4.50	10^h 01^m 01^s	+31° 55′ 25″	48.6
AB Doradus	A	K1Vp	6.98	−	05^h 28^m 45^s	−65° 26′ 55″	48.7
ν Phoenicis		F8V	4.57	3.70	01^h 15^m 11^s	−45° 31′ 54″	48.7
Gliese 1021		G5V	5.80	4.93	00^h 45^m 45^s	−47° 33′ 06″	48.7
Gliese 52 [ nl ]		K7V	8.98	8.10	01^h 07^m 09^s	+63° 56′ 30″	48.8
Gliese 1279 [ nl ]		K5V	8.50	7.62	23^h 09^m 41^s	−67° 44′ 00″	48.8
Alderamin		A7IV-V	2.45	1.58	21^h 18^m 35^s	+62° 35′ 08″	48.8
Gliese 738	A	G0V	6.22	5.34	18^h 57^m 02^s	+32° 54′ 05″	48.9
Gliese 738	B	K1V	7.53	6.65	18^h 57^m 02^s	+32° 54′ 05″	48.9

Related Research Articles

HR 7703 is a binary star system in the constellation of Sagittarius. The brighter component has an apparent visual magnitude of 5.31, which means it is visible from suburban skies at night. The two stars are separated by an angle of 7.10″, which corresponds to an estimated semimajor axis of 56.30 AU for their orbit.

<span class="mw-page-title-main">DX Cancri</span> Red dwarf star in the constellation Cancer

DX Cancri is a variable star in the northern zodiac constellation of Cancer. With an apparent visual magnitude of 14.81, it is much too faint to be seen with the naked eye. Visually viewing this star requires a telescope with a minimum aperture of 16 in (41 cm). Based upon parallax measurements, DX Cancri is located at a distance of 11.8 light-years from Earth. This makes it the 18th closest star to the Sun.

<span class="mw-page-title-main">Lacaille 8760</span> Star in the constellation Microscopium

Lacaille 8760 is a red dwarf star in the constellation Microscopium. It is one of the nearest stars to the Sun at about 12.9 light-years' distance, and the brightest M-class main-sequence star in Earth's night sky, although it is generally too faint to be seen without a telescope. At an apparent magnitude of +6.7, it may only be visible to the unaided eye under exceptionally good viewing conditions, under dark skies.

HD 28185 is a yellow dwarf star similar to the Sun located 128 light-years away from Earth in the constellation Eridanus. The designation HD 28185 refers to its entry in the Henry Draper catalogue. The star is known to possess one long-period extrasolar planet.

Zeta Tucanae, Latinized from ζ Tucanae, is a star in the constellation Tucana. It is a spectral class F9.5 main sequence star with an apparent magnitude of +4.23. Despite having a slightly lower mass, this star is more luminous than the Sun. Based upon parallax measurements by the Hipparcos spacecraft, it is approximately 28.0 light years from Earth. This is one of the least variable stars observed during the Hipparcos mission.

Pi¹ Ursae Minoris is a common proper motion binary star system in the northern circumpolar constellation of Ursa Minor. The pair have apparent visual magnitudes of +6.58 and +7.31, with a combined magnitude of 6.1. They are located about 71 light years from the Sun. The two have an angular separation of 31.4 arc seconds, which corresponds to a physical separation of about 680 AU, and orbit each other with a period of about 13,100 years.

Beta Comae Berenices is a main sequence dwarf star in the northern constellation of Coma Berenices. It is located at a distance of about 29.95 light-years from Earth. The Greek letter beta (β) usually indicates that the star has the second highest visual magnitude in the constellation. However, with an apparent visual magnitude of 4.3, this star is actually slightly brighter than α Comae Berenices. It can be seen with the naked eye, but may be too dim to be viewed from a built-up urban area.

9 Aurigae is a star system in Auriga (constellation). It has an apparent magnitude of about 5, making it visible to the naked eye in many suburban skies. Parallax estimates made by the Hipparcos spacecraft put it at about 86 light-years from the solar system, although individual Gaia Data Release 3 parallaxes place all three components at 88 light years.

Psi⁵ Aurigae is a star in the northern constellation of Auriga. It is faintly visible to the naked eye with an apparent visual magnitude of 5.25. Based upon parallax measurements made during the Hipparcos mission, this star is approximately 53.9 light-years distant from Earth. There is an optical companion which is 36 arcseconds away and has an apparent magnitude of +8.4.

HR 4458 is a binary star system in the equatorial constellation of Hydra. It has the Gould designation 289 G. Hydrae; HR 4458 is the Bright Star Catalogue designation. At a distance of 31.13 light years, it is the closest star system to the Solar System within this constellation. This object is visible to the naked eye as a dim, orange-hued star with an apparent visual magnitude of 5.97. It is moving closer to the Earth with a heliocentric radial velocity of −22 km/s.

Gliese 412 is a pair of stars that share a common proper motion through space and are thought to form a binary star system. The pair have an angular separation of 31.4″ at a position angle of 126.1°. They are located 15.8 light-years distant from the Sun in the constellation Ursa Major. Both components are relatively dim red dwarf stars.

HD 176051 is a spectroscopic binary star system approximately 49 light years away from Earth in the constellation Lyra. The pair orbit with a period of 22,423 days and an eccentricity of 0.25. Compared to the Sun, they have a somewhat lower proportion of elements more massive than helium. Their individual masses are estimated at 1.07 and 0.71 solar masses (M_☉). The system is moving closer to the Sun with a radial velocity of −47 km/s and will reach perihelion in about 269,000 years when it comes within roughly 17 ly (5.1 pc) of the Sun.

HD 115404 is a binary star system located in the constellation Coma Berenices. Parallax measurements made by Hipparcos put the system at 36 light-years, or 11 parsecs, away. The combined apparent magnitude of the system is 6.52, with the magnitudes of the components being 6.66 and 9.50.

Zeta Doradus, Latinized from ζ Doradus, is a young star system that lies approximately 38 light-years away. The system consists of two widely separated stars, with the primary being bright enough to be observed with the naked eye but the secondary being much a much fainter star that requires telescopic equipment to be observed.

HR 3384 is solitary star in the southern constellation of Pyxis. It has an apparent magnitude of 6.38, indicating it is faintly visible to the naked eye. Based on the Bortle scale, the star can be viewed from dark rural skies. Astrometric measurements of the star by the Hipparcos spacecraft, give an estimated distance of about 40 light-years from Earth. It is moving away from the Sun with a radial velocity of +81.91.

Mu Ceti is a star in the constellation Cetus. The combined apparent magnitude of the system is +4.27, and it is located 84 light-years from the Sun.

Gliese 251, also known as HIP 33226 or HD 265866, is a star located about 18 light years away from the Solar System. Located in the constellation of Gemini, it is the nearest star in this constellation. It is located near the boundary with Auriga, 49 arcminutes away from the bright star Theta Geminorum; due to its apparent magnitude of +9.89 it cannot be observed with the naked eye. The closest star to Gliese 251 is QY Aurigae, which is located 3.5 light years away.

<span class="mw-page-title-main">Gliese 402</span> Star in the constellation Leo

Gliese 402 is a star located 22.7 light years from the Solar System. Located in the constellation of Leo, it is also known as Wolf 358 from its entry in Max Wolf's star catalogue. The stars nearest to Gliese 402 are Gliese 393, at 3.43 light years, Gliese 408, at 6.26 light years, and Gliese 382 at 6.66 light years.

References

Allende Prieto, C.; et al. (June 2004), "S⁴N: A spectroscopic survey of stars in the solar neighborhood. The Nearest 15 pc", Astronomy and Astrophysics, 420: 183–205, arXiv: astro-ph/0403108 , Bibcode:2004A&A...420..183A, doi:10.1051/0004-6361:20035801
Anderson, E.; Francis, Ch. (2012), "XHIP: An extended hipparcos compilation", Astronomy Letters, 38 (5): 331, arXiv: 1108.4971 , Bibcode:2012AstL...38..331A, doi:10.1134/S1063773712050015.
Butler, R. P.; et al. (July 2006). "Catalog of Nearby Exoplanets". The Astrophysical Journal. 646 (1): 505–522. arXiv: astro-ph/0607493 . Bibcode:2006ApJ...646..505B. doi:10.1086/504701.
de Mello, G. F. Porto; del Peloso, E. F. & Ghezzi, L. (April 2006). "Astrobiologically interesting stars within 10 parsecs of the Sun". Astrobiology. 6 (2): 308–331. arXiv: astro-ph/0511180 . Bibcode:2006AsBio...6..308P. doi:10.1089/ast.2006.6.308. PMID 16689649.
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.
Henry, Todd J. (1 October 2006). "The One Hundred Nearest Star Systems". Research Consortium on Nearby Stars. Archived from the original on 28 November 2006. Retrieved 11 December 2006.
Holmberg, J.; Nordström, B.; Andersen, J. (July 2009). "The Geneva-Copenhagen survey of the solar neighbourhood. III. Improved distances, ages, and kinematics". Astronomy and Astrophysics Supplement Series. 501 (3): 941–947. arXiv: 0811.3982 . Bibcode:2009A&A...501..941H. doi:10.1051/0004-6361/200811191.Note: see VizieR catalogue V/130.
Mamajek, Eric E.; Hillenbrand, Lynne A. (November 2008). "Improved Age Estimation for Solar-Type Dwarfs Using Activity-Rotation Diagnostics". The Astrophysical Journal. 687 (2): 1264–1293. arXiv: 0807.1686 . Bibcode:2008ApJ...687.1264M. doi:10.1086/591785.Note: this is a "volume-limited" sample of stars within 16 parsecs of the Sun.
Pasinetti Fracassini, L. E.; Pastori, L.; Covino, S.; Pozzi, A. (February 2001). "Catalogue of Apparent Diameters and Absolute Radii of Stars (CADARS)". Astronomy and Astrophysics. 367 (Third ed.): 521–524. arXiv: astro-ph/0012289 . Bibcode:2001A&A...367..521P. doi:10.1051/0004-6361:20000451.Note: see VizieR catalogue J/A+A/367/521.
Perryman, Michael (2010), "The Making of History's Greatest Star Map", Astronomers' Universe, Heidelberg: Springer-Verlag, Bibcode:2010mhgs.book.....P, doi:10.1007/978-3-642-11602-5, ISBN 978-3-642-11601-8
Perryman, M. A. C.; et al. (1997), "The Hipparcos Catalogue", Astronomy & Astrophysics, 323: L49–L52, Bibcode:1997A&A...323L..49P
Takeda, G.; et al. (2007). "Stellar parameters of nearby cool stars. II. Physical properties of ~1000 cool stars from the SPOCS catalog". Astrophysical Journal Supplement Series. 168 (2): 297–318. arXiv: astro-ph/0607235 . Bibcode:2007ApJS..168..297T. doi:10.1086/509763.Note: see VizieR catalogue J/ApJS/168/297.
Valenti, Jeff A.; Fischer, Debra A. (July 2005). "Spectroscopic Properties of Cool Stars (SPOCS). I. 1040 F, G, and K Dwarfs from Keck, Lick, and AAT Planet Search Programs". The Astrophysical Journal Supplement Series. 159 (1): 141–166. Bibcode:2005ApJS..159..141V. doi: 10.1086/430500 .Note: see VizieR catalogie J/ApJS/159/141 Archived 6 August 2016 at the Wayback Machine .
van Leeuwen, Floor (2007). Hipparcos, the new Reduction of the Raw data. Astrophysics and Space Science Library. Vol. 350. pp. 653–664. arXiv: 0708.1752 . Bibcode:2007A&A...474..653V. doi:10.1051/0004-6361:20078357. ISBN 978-1-4020-6341-1.{{cite book}}: |journal= ignored (help)Note: see VizieR catalogue I/311.

External links

"SIMBAD Astronomical Database". Centre de Données astronomiques de Strasbourg. Retrieved 5 August 2006.
"NStars database". NASA. Archived from the original on 1 November 2005. Retrieved 24 October 2005.
"ARICNS". Astronomisches Rechen-Institut. Archived from the original on 14 October 2005. Retrieved 24 October 2005.
"Notable Nearby Stars". SolStation. Retrieved 24 October 2005.
"What color are the stars?". Mitchell Charity. Retrieved 24 October 2005.

This page is based on this Wikipedia article
Text is available under the CC BY-SA 4.0 license; additional terms may apply.
Images, videos and audio are available under their respective licenses.