Субгиганты | Stellar Catalog

	Mass	Distance
Iota Hydri HD 21024, HIP 15201, iot Hyi, TIC 431380163, 2MASS J03155768-7723184, TYC 9366-741-1, HR 1025	F5IV-V	1.4 M☉	95.2 ly
HD 45588 LTT 2558, GJ 9212 B, IRAS 06251-2549, CCDM J06272-2551A, GJ 9212 A, 2MASS J06271136-2551232, CD -25 3237, HD 45588, NLTT 16540, UBV 6457, HIC 30711, PLX 1507, HIP 30711, PPM 250422, YZ 115 3638, GC 8368, HR 2349, SAO 171774, [RHG95] 1047	F8IV	1.3 M☉	95.9 ly
HD 22468 HR 1099	K1IV	1.5 M☉	96 ly
Theta Indi GJ 9733 A, Gliese 9733 A, HD 202730, CPD−53°10037, GC 29819, HIP 105319, HR 8140, HD 202730, SAO 246965, WDS J21199-5327AB	A5IV-V	1.8 M☉	96.1 ly
35 Leonis HD 89010, 35 Leo, HIP 50319	G1.5IV	1.3 M☉	96.6 ly
HD 145148	K1.5IV	-	96.7 ly
Alpheratz Alpheratz, Sirrah, Sirah, H 5 32A, α And, Alpha Andromedae, Alpha And, δ Pegasi, δ Peg, Delta Pegasi, Delta Peg, 21 Andromedae, 21 And, BD+28°4, FK5 1, GC 127, HD 358, HIP 677, HR 15, SAO 73765, PPM 89441, ADS 94 A, CCDM J00083+2905A, WDS 00084+2905A/Aa, LTT 10039, NLTT 346	B8IV-VHgMn	3.6 M☉	97 ly
51 Eridani c Eridani, BD−02° 963, HD 29391, HIC 21547, HIP 21547, HR 1474, SAO 131358, 2MASS J04373613-0228248, * 51 Eri	F0IV C	1.6 M☉	97.1 ly
HD 94510 u Car, u Carinae, NSV 5011, CPD−58°2834, GC 14980, HD 94510, HIP 53253, HR 4257, SAO 238574, CCDM J10535-5851	K0IV	1.9 M☉	97.3 ly
HD 196794	K2IV	-	97.7 ly
Rho Capricorni * rho Cap, ρ Cap, 11 Cap, BD−18°5689, GJ 791.1, GJ 9696, HD 194943, HIP 101027, HR 7822, SAO 163614, ADS 13887, WDS J20289-1749AB	F2 IV	1.5 M☉	97.9 ly
HD 138573	G5IV-V	-	97.9 ly
Kappa Coronae Borealis κ CrB, 11 CrB, kap CrB, HD 142091, HIC 77655, HIP 77655, HR 5901, SAO 64948, LTT 14702, FK5 1414, 2MASS J15511394+3539264, NLTT 41359, TIC 334753043, TYC 2578-1609-1, WISE J155113.91+353925.2	K1IVa B	1.3 M☉	98.1 ly
* kap CrB	K1IVa	-	98.2 ly
* alf Ind	K0III-IV	-	98.3 ly
HD 152311 BD-20 4572，SAO 184754，HR 6269	G2IV-V	-	98.8 ly
46 Leonis Minoris * 46 LMi, Praecipua, BD+34 2172, FK5 412, HD 94264, HIP 53229, HR 4247, SAO 62297	K0+III-IV	1.1 M☉	99.1 ly
HD 81809 HIP 46404, TIC 46802551, HR 3750	G1.5IV-V	0.87 M☉	101 ly
HD 221420	G2IV-V	1.7 M☉	102 ly
HD 37124 BD+20°1018, Gliese 209, GJ 209, HD 37124, HIC 26381, HIP 26381, SAO 77323, G 100-27	G4IV-V	0.81 M☉	103 ly

Имя звезды

Mass

Distance

Iota Hydri

HD 21024, HIP 15201, iot Hyi, TIC 431380163, 2MASS J03155768-7723184, TYC 9366-741-1, HR 1025

F5IV-V

1.4 M☉

95.2 ly

HD 45588

LTT 2558, GJ 9212 B, IRAS 06251-2549, CCDM J06272-2551A, GJ 9212 A, 2MASS J06271136-2551232, CD -25 3237, HD 45588, NLTT 16540, UBV 6457, HIC 30711, PLX 1507, HIP 30711, PPM 250422, YZ 115 3638, GC 8368, HR 2349, SAO 171774, [RHG95] 1047

F8IV

1.3 M☉

95.9 ly

HD 22468

HR 1099

K1IV

1.5 M☉

96 ly

Theta Indi

GJ 9733 A, Gliese 9733 A, HD 202730, CPD−53°10037, GC 29819, HIP 105319, HR 8140, HD 202730, SAO 246965, WDS J21199-5327AB

A5IV-V

1.8 M☉

96.1 ly

35 Leonis

HD 89010, 35 Leo, HIP 50319

G1.5IV

1.3 M☉

96.6 ly

HD 145148

K1.5IV

96.7 ly

Alpheratz

Alpheratz, Sirrah, Sirah, H 5 32A, α And, Alpha Andromedae, Alpha And, δ Pegasi, δ Peg, Delta Pegasi, Delta Peg, 21 Andromedae, 21 And, BD+28°4, FK5 1, GC 127, HD 358, HIP 677, HR 15, SAO 73765, PPM 89441, ADS 94 A, CCDM J00083+2905A, WDS 00084+2905A/Aa, LTT 10039, NLTT 346

B8IV-VHgMn

3.6 M☉

97 ly

51 Eridani

c Eridani, BD−02° 963, HD 29391, HIC 21547, HIP 21547, HR 1474, SAO 131358, 2MASS J04373613-0228248, * 51 Eri

F0IV C

1.6 M☉

97.1 ly

HD 94510

u Car, u Carinae, NSV 5011, CPD−58°2834, GC 14980, HD 94510, HIP 53253, HR 4257, SAO 238574, CCDM J10535-5851

K0IV

1.9 M☉

97.3 ly

HD 196794

K2IV

97.7 ly

Rho Capricorni

* rho Cap, ρ Cap, 11 Cap, BD−18°5689, GJ 791.1, GJ 9696, HD 194943, HIP 101027, HR 7822, SAO 163614, ADS 13887, WDS J20289-1749AB

F2 IV

1.5 M☉

97.9 ly

HD 138573

G5IV-V

97.9 ly

Kappa Coronae Borealis

κ CrB, 11 CrB, kap CrB, HD 142091, HIC 77655, HIP 77655, HR 5901, SAO 64948, LTT 14702, FK5 1414, 2MASS J15511394+3539264, NLTT 41359, TIC 334753043, TYC 2578-1609-1, WISE J155113.91+353925.2

K1IVa B

1.3 M☉

98.1 ly

* kap CrB

K1IVa

98.2 ly

* alf Ind

K0III-IV

98.3 ly

HD 152311

BD-20 4572，SAO 184754，HR 6269

G2IV-V

98.8 ly

46 Leonis Minoris

* 46 LMi, Praecipua, BD+34 2172, FK5 412, HD 94264, HIP 53229, HR 4247, SAO 62297

K0+III-IV

1.1 M☉

99.1 ly

HD 81809

HIP 46404, TIC 46802551, HR 3750

G1.5IV-V

0.87 M☉

101 ly

HD 221420

G2IV-V

1.7 M☉

102 ly

HD 37124

BD+20°1018, Gliese 209, GJ 209, HD 37124, HIC 26381, HIP 26381, SAO 77323, G 100-27

G4IV-V

0.81 M☉

103 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.

Звезды

Звёзды — это огромные шары раскалённого газа, которые светятся благодаря выработке энергии в процессе ядерного синтеза в их ядрах. Большинство звёзд состоит в основном из водорода и гелия. В центре звезды из-за высокого давления и температуры атомы водорода сливаются в гелий, высвобождая огромное количество энергии в виде света и тепла.

More about Звезды

Random terms

Позиция звезды Светимость Температура звезд Масса звезды Размер звезды Звездный возраст

Список Субгиганты

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: Звезды