Список Молодые звездные объекты

Больше о Молодые звездные объекты

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Звезды 1-20

		Mass	Distance
RX J0506.2+0439 2MASS J05061292+0439272, TIC 455029978	M4.5V	-	90.1 ly
Gliese 3305 2MASS J04373746-0229282, GJ 3305, TIC 298812498, StKM 1-497	M1.1V C	0.67 M☉	90.6 ly
CE Antliae , TYC 7190-2111-1, TWA 7, CE Ant, 2MASS J10423011-3340162, TIC 54147487, WISE J104230.01-334016.4, ASAS J104230-3340.3, GSC 07190-02111, RX J104230.3-334014	M2Ve	0.46 M☉	111 ly
TWA 30	M5	0.12 M☉	155 ly
TWA 30 B	M4	-	155 ly
HL Tauri	K9	-	185 ly
TW Hydrae TWA 1, TW Hya, CD−34° 7151, HIP 53911	K6	0.9 M☉	196 ly
MP Musca MP Mus, PDS 66, CPD-68 1894, Hen 3-892, TYC 9246-971-1	K1Ve	1.3 M☉	319 ly
T Chamaeleontis T Cha, HIP 58285, TYC 9419-1187-1, GSC 09419-01187, 2MASS J11571348-7921313	K0e	0.65 M☉	335 ly
HD 44179		-	347 ly
HD 44179 B		-	347 ly
DX Chamaeleontis HD 104237, DX Cha, CD−77°528, GC 16412, HD 104237, HIP 58520, SAO 256895, PPM 371328, WDS J11596-7813C	A8Ve	2.2 M☉	348 ly
DX Chamaeleontis B		1.4 M☉	348 ly
V1298 Tauri V 1298 Tau, K2-309, 2MASS J04051959+2009256, BD+19 656, EPIC 210818897, RX J0405.3+2009, 1SWASP J040519.59+200925.5	K0-K1.5	1.1 M☉	352 ly
PDS 70 V1032 Cen, 2MASS J14081015-4123525, IRAS 14050−4109, CD-40 8434, DENIS J140810.1-412352, TIC 179413040, WISE J140810.13-412352.7	K7IVe C	0.76 M☉	370 ly
GG Tauri Aa GG Tau, WDS J04325+1732, TYC 1270-897-1	K7	0.78 M☉	380 ly
GG Tauri Ab	M0.5	-	380 ly
GG Tauri Ba	M5	0.12 M☉	380 ly
GG Tauri Bb	M7	0.04 M☉	380 ly
GG Tauri Ac		-	380 ly

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Звезды 1-20

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Research in Молодые звездные объекты

Просмотрите последние научные исследования звезд и экзопланет в нашей галактике. Откройте для себя новейшие исследования в области астрофизики и звездной астрономии.

Текущее исследование

	HL Tauri 185 ly			Nonthermal Velocity Dispersion in the Outer Disk of HL Tau 7. 4. 2026
	DX Chamaeleontis 348 ly			The Arc in the DX Cha Circumbinary System: Evidence For a Retrograde Circumbinary Disk 23. 3. 2026
	HD 34282 1007 ly			Multi-wavelength ALMA Imaging of HD 34282: Dust-trapping Signatures of a Vortex Candidate 10. 3. 2026
	HL Tauri 185 ly			Hunting for methanol in the water rich, planet forming disk around HL Tauri 5. 3. 2026
	CE Antliae 111 ly			Dynamics of the TWA 7 planetary system and possibility of an additional planet 4. 3. 2026

Старые публикации

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.

StellarGuide: Звезды

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.

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Позиция звезды Светимость Температура звезд Масса звезды Размер звезды Звездный возраст