Podobři | Stellar Catalog

	Mass	Distance
HD 136064	F9IV	-	82.5 ly
94 Aquarii Aa BD−14 6448, GJ 894.2, Gliese 894.2, HD 219834, HIP 115126, HR 8866, SAO 165625	G8.5IV	1.2 M☉	82.8 ly
HD 138763 BD-05 4100，SAO 140613，HD 138763，HR 5779	F9IV-V	-	83.1 ly
HD 187237 TYC 2147-3301-1, HIP 97420	G2IV-V	-	83.2 ly
HD 13825 TYC 1765-1368-1, HIP 10505	G5IV-V	-	84 ly
Lambda Andromedae lam And, λ And, 16 Andromedae, BD+45°4283, FK5 890, GJ 9832, HD 222107, HIP 116584, HR 8961, SAO 53204, PPM 64456, LTT 16964, NLTT 57442	G8 III-IVk	1.2 M☉	84.6 ly
HD 144009 TYC 9277-3005-1, USNO-A2 0150-16093262, HIP 79143	G8IV-VFe+0.5	-	84.6 ly
HD 136834 LHS 3067, GJ 1192, Gliese 1192, 2MASS J15224254+0125069, WISEA J152242.30+012503.3, TYC 337-615-1	K3IV-V	-	84.7 ly
HD 128356 LTT 5787, CD-25 10441, HIC 71481, HIP 71481, 2MASS J14370489-2548087, SAO 182707, TIC 16855, TYC 6749-785-1	K2.5IV C	0.65 M☉	85 ly
18 Boötis 18 Boo, BD+13°2782, FK5 1372, GJ 3841, HD 125451, HIP 69989, HR 5365, SAO 100975, WDS J14193+1300	F5IV	1.3 M☉	85.1 ly
HD 30562 BD–05°1044, GJ 177.1, Gliese 177.1, HD 30562, HIC 22336, HIP 22336, HR 1536, SAO 131504, PPM 187358, NLTT 13980, GCRV 2828, LTT 2093, 2MASS J04483633-0540258, TIC 176379354, TYC 4748-1630-1, WISEA J044836.62-054028.9	G2IV C	1.3 M☉	85.3 ly
Zeta Aquilae Okab (primary), Zeta Aql, ζ Aql, 17 Aql, BD+13 3899, FK5 716, GJ 4095, Gliese 4095, HD 177724, HIP 93747, HR 7235, SAO 104461, WDS J19054+1352A, zet Aql	A0IV-Vnn	2.4 M☉	85.3 ly
23 Librae CD−24° 11928, Gliese 579.4, GJ 579.4, HD 134987, HIC 74500, HIP 74500, HR 5657, SAO 183275	G6IV-V C	1.1 M☉	85.4 ly
Epsilon Cephei ε Cephei, 23 Cephei, BD+56 2741, HD 211336, HIP 109857, HR 8494, SAO 34227	F0 IV	1.6 M☉	85.5 ly
HD 60532 108 G. Puppis, BD–21° 2007, GC 10134, HIC 36795, HIP 36795, HR 2906, GJ 279, Gliese 279, SAO 174009, 2MASS J07340317-2217457, FK5 288, TIC 456871289, TYC 5991-217-1	F6IV-V C	1.4 M☉	85.5 ly
Delta Corvi 7 Crv, del Crv, BD−15 3482, FK5 465, HD 108767, HIP 60965, HR 4757, SAO 157323	A0IV(n)kB9	-	85.7 ly
Gamma Boötis Aa Seginus, Haris, Ceginus, Segin, Gam Boo, 27 Boötis, BD+38°2565, FK5 535, HD 127762, HIP 71075, HR 5435, SAO 64203, WDS J14321+3818A, BU 616, gam Boo	A7IV+(n)	2.1 M☉	86 ly
HD 205905	G1.5IV-V	-	86.1 ly
V1688 Aquilae V1688 Aql, HD 180263, TYC 1049-315-1, USNO-A2 0975-14436832, HIP 94650	K2IV-V	-	86.1 ly
HD 114174	G5 IV-V	1.1 M☉	86.1 ly

Název hvězdy

Mass

Distance

HD 136064

F9IV

82.5 ly

94 Aquarii Aa

BD−14 6448, GJ 894.2, Gliese 894.2, HD 219834, HIP 115126, HR 8866, SAO 165625

G8.5IV

1.2 M☉

82.8 ly

HD 138763

BD-05 4100，SAO 140613，HD 138763，HR 5779

F9IV-V

83.1 ly

HD 187237

TYC 2147-3301-1, HIP 97420

G2IV-V

83.2 ly

HD 13825

TYC 1765-1368-1, HIP 10505

G5IV-V

84 ly

Lambda Andromedae

lam And, λ And, 16 Andromedae, BD+45°4283, FK5 890, GJ 9832, HD 222107, HIP 116584, HR 8961, SAO 53204, PPM 64456, LTT 16964, NLTT 57442

G8 III-IVk

1.2 M☉

84.6 ly

HD 144009

TYC 9277-3005-1, USNO-A2 0150-16093262, HIP 79143

G8IV-VFe+0.5

84.6 ly

HD 136834

LHS 3067, GJ 1192, Gliese 1192, 2MASS J15224254+0125069, WISEA J152242.30+012503.3, TYC 337-615-1

K3IV-V

84.7 ly

HD 128356

LTT 5787, CD-25 10441, HIC 71481, HIP 71481, 2MASS J14370489-2548087, SAO 182707, TIC 16855, TYC 6749-785-1

K2.5IV C

0.65 M☉

85 ly

18 Boötis

18 Boo, BD+13°2782, FK5 1372, GJ 3841, HD 125451, HIP 69989, HR 5365, SAO 100975, WDS J14193+1300

F5IV

1.3 M☉

85.1 ly

HD 30562

BD–05°1044, GJ 177.1, Gliese 177.1, HD 30562, HIC 22336, HIP 22336, HR 1536, SAO 131504, PPM 187358, NLTT 13980, GCRV 2828, LTT 2093, 2MASS J04483633-0540258, TIC 176379354, TYC 4748-1630-1, WISEA J044836.62-054028.9

G2IV C

1.3 M☉

85.3 ly

Zeta Aquilae

Okab (primary), Zeta Aql, ζ Aql, 17 Aql, BD+13 3899, FK5 716, GJ 4095, Gliese 4095, HD 177724, HIP 93747, HR 7235, SAO 104461, WDS J19054+1352A, zet Aql

A0IV-Vnn

2.4 M☉

85.3 ly

23 Librae

CD−24° 11928, Gliese 579.4, GJ 579.4, HD 134987, HIC 74500, HIP 74500, HR 5657, SAO 183275

G6IV-V C

1.1 M☉

85.4 ly

Epsilon Cephei

ε Cephei, 23 Cephei, BD+56 2741, HD 211336, HIP 109857, HR 8494, SAO 34227

F0 IV

1.6 M☉

85.5 ly

HD 60532

108 G. Puppis, BD–21° 2007, GC 10134, HIC 36795, HIP 36795, HR 2906, GJ 279, Gliese 279, SAO 174009, 2MASS J07340317-2217457, FK5 288, TIC 456871289, TYC 5991-217-1

F6IV-V C

1.4 M☉

85.5 ly

Delta Corvi

7 Crv, del Crv, BD−15 3482, FK5 465, HD 108767, HIP 60965, HR 4757, SAO 157323

A0IV(n)kB9

85.7 ly

Gamma Boötis Aa

Seginus, Haris, Ceginus, Segin, Gam Boo, 27 Boötis, BD+38°2565, FK5 535, HD 127762, HIP 71075, HR 5435, SAO 64203, WDS J14321+3818A, BU 616, gam Boo

A7IV+(n)

2.1 M☉

86 ly

HD 205905

G1.5IV-V

86.1 ly

V1688 Aquilae

V1688 Aql, HD 180263, TYC 1049-315-1, USNO-A2 0975-14436832, HIP 94650

K2IV-V

86.1 ly

HD 114174

G5 IV-V

1.1 M☉

86.1 ly

Frequently Asked Questions about nearby stars

What is the nearest star?

Nearest star is Proxima Centauri, located approximately 4.24 light-years (1.30 parsecs) from the Sun. It is part of the Alpha Centauri star system, which also includes Alpha Centauri A and Alpha Centauri B.

What are the nearest stars to Earth?

Nearest stars to Earth include the Alpha Centauri system (Alpha Centauri A, Alpha Centauri B, and Proxima Centauri), Barnard's Star, and Wolf 359. There are also brown dwarfs Luhman 16 and WISE 0855−0714.

What is the solar neighborhood?

Solar neighborhood (also Local Interstellar Cloud) is the region of interstellar space that surrounds the Sun with diameter about 15 light years. Stellar Catalog database includes all stars contained within this region.

How do astronomers measure distances to stars?

Astronomers use methods like parallax, standard candles, and redshift to measure distances to stars. Parallax is especially useful for nearby stars in our solar neighborhood, while other techniques help map the universe beyond.

Are there any exoplanets orbiting the nearest stars?

Yes, several exoplanets have been discovered orbiting the nearest stars. For example, Proxima Centauri has an exoplanet called Proxima Centauri b, which is located in the star's habitable zone and is the closest known exoplanet to Earth.

Why are the nearest stars important for astronomy and physics?

The nearest stars provide valuable laboratories for studying stellar evolution, space environments, and the fundamental physics of stars. Observing these stars helps astronomers understand the structure of our galaxy and the broader universe.

Hvězdy

Hvězdy jsou obrovské koule horkého plynu, které září díky energii vznikající jadernou fúzí v jejich jádru. Většina hvězd se skládá převážně z vodíku a helia. V centru hvězdy dochází díky vysokému tlaku a teplotě k přeměně vodíku na helium, přičemž se uvolňuje obrovské množství energie ve formě světla a tepla.

More about Hvězdy

Random terms

Pozice hvězdy Zářivost hvězdy Teplota hvězdy Hmotnost hvězdy Velikost hvězdy Stáří hvězdy

Seznam nejbližších Podobři

Frequently Asked Questions about nearby stars

What is the nearest star?

What are the nearest stars to Earth?

What is the solar neighborhood?

How do astronomers measure distances to stars?

Are there any exoplanets orbiting the nearest stars?

Why are the nearest stars important for astronomy and physics?

StellarGuide: Hvězdy