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Sterne 1-20
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Sternname 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

EK Chamaeleontis
V* EK Cha, UCAC2 410939, TIC 323292535, Gaia DR3 5209037736474704512, ASAS J084235-7858.1, UCAC3 23-14912, WISEA J084226.98-785747.6, Gaia DR2 5209037736474704512, 2MASS J08422710-7857479, UCAC4 056-006819, WISE J084227.02-785747.7, RECX 5, USNO-A2.0 0075-01721570
M4.5 0.11 M☉ 321 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
Sterne 1-20
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Protoplanet candidate EK Chamaeleontis b identified around a young red dwarf star
icon9. 10. 2026
iconSterne | Exoplaneten | Junge Sternobjekte
Image: Protoplanet candidate EK Chamaeleontis b identified around a young red dwarf star
The search for planets in the very early stages of their formation, known as protoplanets, remains a significant challenge in space observation. A new candidate, designated as EK Cha b, has been observed around the young red dwarf star EK Cha. This object is notable because it provides a rare opportunity to study planetary development within a gas-rich environment. While large gas planets are less common around red dwarf stars compared to larger stars, these cool, small stars represent a common ...
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Inclined planet in the protoplanetary disc of HD 139614 creates shifting shadows
icon6. 10. 2026
iconSterne | Exoplaneten | Junge Sternobjekte
Image: Inclined planet in the protoplanetary disc of HD 139614 creates shifting shadows
An inclined planet orbiting HD 139614 is warping its protoplanetary disc, casting large shadows across the outer regions. New models confirm these shadows and a spiral structure are evidence of the planet's gravitational influence on the surrounding dust....
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Mass measurements of infant planets orbiting the young star V1298 Tau
icon26. 9. 2026
iconSterne | Exoplaneten | Junge Sternobjekte
Image: Mass measurements of infant planets orbiting the young star V1298 Tau
New mass measurements of the infant planets orbiting V1298 Tau reveal that planets b and e are likely gas giants. These findings, based on long-term radial velocity monitoring, suggest higher masses than previously estimated from transit timing observations....
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study iconResearch in Junge Sternobjekte

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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.
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exoplanet iconStellarGuide: Sterne

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Sterne
Sterne sind riesige Kugeln aus heißem Gas, die durch Kernfusion in ihrem Inneren Energie erzeugen und dadurch leuchten. Die meisten Sterne bestehen hauptsächlich aus Wasserstoff und Helium. Im Zentrum eines Sterns verschmelzen Wasserstoffatome aufgrund des hohen Drucks und der Temperatur zu Helium, wobei eine enorme Menge Energie in Form von Licht und Wärme freigesetzt wird.
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