List of stars with resolved images

Short description: none

The following is a list of stars with resolved images, that is, stars whose images have been resolved beyond a point source. Aside from the Sun, observed from Earth, stars are exceedingly small in apparent size, requiring the use of special high-resolution equipment and techniques to image. For example, Betelgeuse, the first star other than the Sun to be resolved, has an angular diameter of only 50 milliarcseconds (mas).[1]

## Contents

* 1 List
* 2 See also
* 3 Notes
* 4 References

## List

This list is incomplete; you can help by expanding it.

List of stars with resolved images  Star | Image  | Diameter  | Distance
(ly)  | First imager  | Year  | Notes

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Angular (mas)  | Geometric (R☉)
Sun | 50px  | 1930000±30000 | 1 | 0.0000158 | Louis Fizeau and Léon Foucault[2] | 1845 |
Altair
α Aql  | 50px  | 3.2 | 1.66±0.01 (polar)
2.02±0.01 (equator)  | 16.77±0.08 | CHARA array – MIRC[3] | 2006 |
Rasalhague
α Oph A  |  | 1.62±0.03 | 2.39±0.01 (polar)
2.87±0.02 (equator)  | 48.6±0.8 | CHARA array – MIRC[4] | 2006 |
Alderamin
α Cep  |  | 1.35±0.02 (polar)
1.75±0.03 (equator)  | 2.20±0.04 (polar)
2.74±0.04 (equator)  | 48.8±0.36 | CHARA array – MIRC[4] | 2006 |
Caph
β Cas  |  | 1.70±0.04 | 3.1±0.1 (polar)
3.8±0.1 (equator)  | 54.7±0.3 | CHARA array – MIRC[5] | 2007 |
Regulus
α Leo Aa  |  | 1.24±0.02 | 3.2±0.1 (polar)
4.2±0.1 (equator)  | 79.3±0.7 | CHARA array – MIRC[5] | 2008 |
Algol
β Per Aa1  | 50px
50px  | 0.88±0.05 | 4.13 | 93±2 | CHARA array – MIRC[6] | 2006 | stationary object in the animation
β Per Aa2  | 1.12±0.07 | 3 | orbiting object in the animation
β Per Ab  | 0.56±0.10 | 0.9 |  |  | Observed radius of Algol Ab is an instrumental artifact, caused by bandwidth smearing.
Actual radius is 1.73 ± 0.33 R☉.
Alkaid
η UMa  |  | 0.834±0.060 | 2.86±0.21 | 103.9±0.8 | CHARA array[7] | 2012 |
σ Gem A  |  | 2.425  | 10.1±0.4 | 126±2 | CHARA array/MIRC[8] | 2011  | The star contains starspots on its surface
Markab
α Peg  |  | 1.052±0.066 | 4.62±0.29 | 133±1 | CHARA array[7] | 2012 |
Elnath
β Tau  |  | 1.09±0.076 | 4.82±0.34 | 134±2 | CHARA array[7] | 2012 |
ζ And Aa  |  | 2.502±0.008 | 15.0±0.8 (polar)  | 189±3 | CFHT[9][10] | 1996 | First direct imaging of starspots on a star outside the Solar System.
R Dor |

| 57±5 | 370±50 | 204±9 | New Technology Telescope[11] | 1993 | 2nd largest known star by apparent diameter in Earth's sky, after the Sun.
Mira
ο Cet A  | 50px  | 28.9–34.9[12] | 332–402[12] | 420 | Hubble – FOC[13] | 1997 |
Polaris
α UMi Aa  | Template:Cssic | 3.143±0.027 | 46.27±0.42 | 446±1 | CHARA array[14] | 2024  |
T Lep | 50px  | 5.8
15 for molecular layer | 100 | 500 | Very Large Telescope – VLTI[15]/AMBER[16] | 2009 |
π1 Gru | 50px  | 21[17] | 370[17] | 535[17] | Very Large Telescope – VLTI/PIONIER[18] | 2017 | First directly observed granulation patterns on a star's surface outside the Solar System.
Antares
α Sco A  | 50px  | 41.3±0.1 | 680[19] | 553[20] | Very Large Telescope – VLTI/AMBER[21][22] | 2017 |
R Car |  | 10.23±0.05–13.77±0.14 | 400–540  | 590±40 | Very Large Telescope – PIONIER[23] | 2014[lower-alpha 1] |
Betelgeuse
α Ori  | 50px  | 50 | 640[24]–764[25] | 643±146 | Hubble – GHRS[1] | 1995 | First star with a resolved image outside the Solar System.
Sheliak
β Lyr Aa  |  | 0.46 | 6 | 960±50 | CHARA array – MIRC[26] | 2007 | Both Aa1 and Aa2 are visible in the animation.
R Scl | 50px  | 8.9±0.3 | 355±55 | 1180±140 | Very Large Telescope – AMBER[27] | 2017  |
θ1 Ori C | 50px  | 0.2 | 10.6±1.5 | 1400 | Very Large Telescope – AMBER[28] | 2009 | In the image, the right inset is θ1 Ori C and the left inset is θ1 Ori F.
θ1 Ori F |  |  |  | Very Large Telescope – VLTI/GRAVITY[29] | 2016
ε Aur |  | 2.22±0.10[30] | 143–358[30] | 2000–4800[30] | CHARA array – MIRC[31] | 2009 | Supergiant with an eclipsing companion surrounded by a massive, opaque debris disk
AZ Cyg |  | 4.05±0.01 | 911+57
−50 | 6820+420
−380 | CHARA array – MIRC[32] | 2011[lower-alpha 2] |
SU Per |  | 3.53±0.09[33] | 1044+31
−21–1139+34
−23[34] | 7,250+470−420[35] | CHARA array[33] | 2015  |
ρ Cas | Template:Cssic | 2.09±0.02 | 564-700  | 8150±1630 | CHARA array[36] | 2024  |
RW Cep | 50px  | 2.45 | 1100±44 [37] | 11000+4600
−2600–22000+5200
−3300 | CHARA array – MIRC-X and MYSTIC[38] | 2022 | Hypergiant star currently undergoing a great dimming event
HR 5171 Aa | 50px  | 4.1±0.8 | 1060–1160[39] | 11740±1630 | Very Large Telescope – VLTI/PIONIER[40] | 2014 | Eclipsing and potential contact binary yellow hypergiant
WOH G64 | 50px  |  | 800[41] | ca. 160 000 | Very Large Telescope – VLTI/GRAVITY[42] | 2024  | Star is in the Large Magellanic Cloud. First resolved image of star outside of the Milky Way.
V602 Carinae |  |  | 1,015[43] |  | Very Large Telescope – VLTI/PIONIER[44] | 2022  |

## See also

* Doppler imaging which produces maps of the surfaces of stars
* Zeeman–Doppler imaging which maps the magnetic fields of stars
* List of directly imaged exoplanets
* Angular resolution
* Angular diameter
* List of nearest stars

## Notes

1. ↑ Published 2024 based on observations from 2014 and 2020
2. ↑ First peer-reviewed publication in 2021, based on observations from 2011-2016

## References

1. ↑ 1.0 1.1 H.Uitenbroek; Dupree, A. K.; Gilliland, R. L. (1998). "Spatially Resolved Hubble Space Telescope Spectra of the Chromosphere of alpha Orionis". Astronomical Journal 116 (5): 2501. doi:10.1086/300596. Bibcode: 1998AJ....116.2501U.
2. ↑ "NASA – Sun–Earth Day – Technology Through Time". 2006. https://sunearthday.nasa.gov/2006/locations/firstphoto.php.
3. ↑ J.D. Monnier (2007). "Imaging the Surface of Altair". Science 317 (5836): 342–5. doi:10.1126/science.1143205. PMID 17540860. Bibcode: 2007Sci...317..342M.
4. ↑ 4.0 4.1 M. Zhao (2009). "Imaging And Modeling Rapidly Rotating Stars: Alpha Cephei And Alpha Ophiuchi". The Astrophysical Journal 701 (1): 209–224. doi:10.1088/0004-637X/701/1/209. Bibcode: 2009ApJ...701..209Z.
5. ↑ 5.0 5.1 X. Che (2011). "Colder And Hotter: Interferometric Imaging Of Beta Cassiopeiae And Alpha Leonis". The Astrophysical Journal 732 (2): 68. doi:10.1088/0004-637X/732/2/68. Bibcode: 2011ApJ...732...68C.
6. ↑ Baron, F.; Monnier, J.; Pedretti, E.; Zhao, M.; Schaefer, G.; Parks, R.; Che, X.; Thureau, N. et al. (2012). "Imaging the Algol Triple System in the H Band with the CHARA Interferometer". The Astrophysical Journal 752 (1): 20. doi:10.1088/0004-637X/752/1/20. Bibcode: 2012ApJ...752...20B.
7. ↑ 7.0 7.1 7.2 Gordon, Kathryn D.; Gies, Douglas R.; Schaefer, Gail H.; Huber, Daniel; Ireland, Michael (7 March 2019). "Angular Sizes, Radii, and Effective Temperatures of B-type Stars from Optical Interferometry with the CHARA Array". The Astrophysical Journal 873 (1): 91. doi:10.3847/1538-4357/ab04b2. Bibcode: 2019ApJ...873...91G.
8. ↑ Roettenbacher, Rachael M.; Monnier, John D.; Korhonen, Heidi; Harmon, Robert O.; Baron, Fabien; Hackman, Thomas; Henry, Gregory W.; Schaefer, Gail H. et al. (2017-11-01). "Contemporaneous Imaging Comparisons of the Spotted Giant σ Geminorum Using Interferometric, Spectroscopic, and Photometric Data". The Astrophysical Journal 849 (2): 120. doi:10.3847/1538-4357/aa8ef7. ISSN 0004-637X. Bibcode: 2017ApJ...849..120R.
9. ↑ Kővári, Zs.; Bartus, J.; Strassmeier, K. G.; Oláh, K.; Weber, M.; Rice, J. B.; Washuettl, A. (2007). "Doppler imaging of stellar surface structure. XXIII. The ellipsoidal K giant binary ζ Andromedae". Astronomy and Astrophysics 463 (3): 1071. doi:10.1051/0004-6361:20065982. Bibcode: 2007A&A...463.1071K.
10. ↑ Roettenbacher, R.M.; Monnier, J.D.; Korhonen, H.; Aarnio, A.N.; Baron, F.; Che, X.; Harmon, R.O.; Kővári, Zs. et al. (2016). "No Sun-like dynamo on the active star ζ Andromedae from starspot asymmetry". Nature 533 (7602): 217–220. doi:10.1038/nature17444. PMID 27144357. Bibcode: 2016Natur.533..217R.
11. ↑ "The Biggest Star in the Sky". ESO. March 11, 1997. http://www.eso.org/public/news/eso9706/. Retrieved 2010-06-26.
12. ↑ 12.0 12.1 Woodruff, H. C.; Eberhardt, M.; Driebe, T.; Hofmann, K.-H. et al. (2004). "Interferometric observations of the Mira star o Ceti with the VLTI/VINCI instrument in the near-infrared". Astronomy & Astrophysics 421 (2): 703–714. doi:10.1051/0004-6361:20035826. Bibcode: 2004A&A...421..703W.
13. ↑ "Hubble Separates Stars in the Mira Binary System". HubbleSite. 6 August 1997. https://hubblesite.org/contents/news-releases/1997/news-1997-26.html. Retrieved 26 June 2017.
14. ↑ Evans, Nancy Remage; Schaefer, Gail H.; Gallenne, Alexandre; Torres, Guillermo; Horch, Elliott P.; Anderson, Richard I.; Monnier, John D.; Roettenbacher, Rachael M. et al. (2024-08-01). "The Orbit and Dynamical Mass of Polaris: Observations with the CHARA Array". The Astrophysical Journal 971 (2): 190. doi:10.3847/1538-4357/ad5e7a. ISSN 0004-637X. Bibcode: 2024ApJ...971..190E.
15. ↑ "Hundred metre virtual telescope captures unique detailed colour image". European Southern Observatory. 18 February 2009. http://www.eso.org/public/unitedkingdom/news/eso0906/. Retrieved 26 June 2017.
16. ↑ J.-B. Le Bouquin, S. Lacour, S. Renard, E. Thiébaut, A. Merand, T. Verhoelst, Pre-maximum spectro-imaging of the Mira star T Leporis with AMBER/VLTI, Astronomy and Astrophysics Volume 496, Number 1, March II 2009, L1–L4.
17. ↑ 17.0 17.1 17.2 Wallstrom, S. H. J.; Danilovich, T.; Muller, H. S. P.; Gottlieb, C. A.; Maes, S.; Van de Sande, M.; Decin, L.; Richards, A. M. S. et al. (December 6, 2023). "ATOMIUM: Molecular inventory of 17 oxygen-rich evolved stars observed with ALMA". Astronomy & Astrophysics 681: A50. doi:10.1051/0004-6361/202347632. ISSN 0004-6361.
18. ↑ "Giant Bubbles on Red Giant Star's Surface". European Southern Observatory. https://www.eso.org/public/news/eso1741/. Retrieved 22 December 2017.
19. ↑ Ohnaka, K; Hofmann, K.-H; Schertl, D; Weigelt, G; Baffa, C; Chelli, A; Petrov, R; Robbe-Dubois, S (2013). "High spectral resolution imaging of the dynamical atmosphere of the red supergiant Antares in the CO first overtone lines with VLTI/AMBER". Astronomy & Astrophysics 555: A24. doi:10.1051/0004-6361/201321063. Bibcode: 2013A&A...555A..24O.
20. ↑ van Leeuwen, F. (November 2007). "Validation of the new Hipparcos reduction". Astronomy and Astrophysics 474 (2): 653–664. doi:10.1051/0004-6361:20078357. Bibcode: 2007A&A...474..653V.
21. ↑ "Astronomers Capture Best-Ever Image of Alien Star". Scientific American. 24 August 2017. https://www.scientificamerican.com/article/astronomers-capture-best-ever-image-of-alien-star. Retrieved 27 August 2017.
22. ↑ "VLTI reconstructed view of the surface of Antares". https://www.eso.org/public/ireland/images/eso1726a/?lang.
23. ↑ Rosales-Guzmán, A. et al. (August 2024). "A new dimension in the variability of AGB stars: Convection patterns size changes with pulsation". Astronomy & Astrophysics 688: A124. doi:10.1051/0004-6361/202349112. Bibcode: 2024A&A...688A.124R.
24. ↑ Mittag, M.; Schröder, K.-P.; Perdelwitz, V.; Jack, D.; Schmitt, J. H. M. M. (2023-01-01). "Chromospheric activity and photospheric variation of α Ori during the great dimming event in 2020" (in en). Astronomy & Astrophysics 669: A9. doi:10.1051/0004-6361/202244924. ISSN 0004-6361. Bibcode: 2023A&A...669A...9M. https://www.aanda.org/articles/aa/full_html/2023/01/aa44924-22/aa44924-22.html.
25. ↑ Joyce, Meridith; Leung, Shing-Chi; Molnár, László; Ireland, Michael; Kobayashi, Chiaki; Nomoto, Ken’ichi (2020-10-01). "Standing on the Shoulders of Giants: New Mass and Distance Estimates for Betelgeuse through Combined Evolutionary, Asteroseismic, and Hydrodynamic Simulations with MESA". The Astrophysical Journal 902 (1): 63. doi:10.3847/1538-4357/abb8db. ISSN 0004-637X. Bibcode: 2020ApJ...902...63J.
26. ↑ M. Zhao (2008). "First Resolved Images Of The Eclipsing And Interacting Binary Beta Lyrae". The Astrophysical Journal 684 (2): L95–L98. doi:10.1086/592146. Bibcode: 2008ApJ...684L..95Z.
27. ↑ Wittkowski, M. et al. (May 2017). "Aperture synthesis imaging of the carbon AGB star R Sculptoris. Detection of a complex structure and a dominating spot on the stellar disk". Astronomy & Astrophysics 601: A3. doi:10.1051/0004-6361/201630214. Bibcode: 2017A&A...601A...3W.
28. ↑ "The orbit of Theta1 Orionis C". European Southern Observatory. 18 February 2009. https://www.eso.org/public/unitedkingdom/images/eso0906d/. Retrieved 26 June 2017.
29. ↑ "First Light For Future Black Hole Probe". European Southern Observatory. 13 January 2016. https://www.eso.org/public/news/eso1601/. Retrieved 18 June 2023.
30. ↑ 30.0 30.1 30.2 Kloppenborg, B. K.; Stencel, R. E.; Monnier, J. D.; Schaefer, G. H.; Baron, F.; Tycner, C.; Zavala, R. T.; Hutter, D. et al. (2015). "Interferometry of ɛ Aurigae: Characterization of the Asymmetric Eclipsing Disk". The Astrophysical Journal Supplement Series 220 (1): 14. doi:10.1088/0067-0049/220/1/14. Bibcode: 2015ApJS..220...14K.
31. ↑ B. Kloppenborg (2010). "Infrared images of the transiting disk in the Epsilon Aurigae system". Nature 464 (7290): 370–2. doi:10.1038/nature08968. PMID 20376144. Bibcode: 2010Natur.464..870K.
32. ↑ Norris, Ryan P. et al. (October 2021). "Long Term Evolution of Surface Features on the Red Supergiant AZ Cyg". The Astrophysical Journal 919 (2): 124. doi:10.3847/1538-4357/ac0c7e. Bibcode: 2021ApJ...919..124N.
33. ↑ 33.0 33.1 Norris, Ryan (2023). "Student Science at NMT: Learning Optical Interferometry Through Projects on Evolved Stars". CHARA. https://www.chara.gsu.edu/files/2023Meeting/Norris_NMT_Students_2023.pdf.
34. ↑ Norris, Ryan (2019). Seeing Stars Like Never Before: A Long-term Interferometric Imaging Survey of Red Supergiants (PhD thesis). Georgia State University. doi:10.57709/15009706.
35. ↑ Bailer-Jones, C. A. L.; Rybizki, J.; Fouesneau, M.; Demleitner, M.; Andrae, R. (2021). "Estimating Distances from Parallaxes. V. Geometric and Photogeometric Distances to 1.47 Billion Stars in Gaia Early Data Release 3". The Astronomical Journal 161 (3): 147. doi:10.3847/1538-3881/abd806. Bibcode: 2021AJ....161..147B. SU Persei's database entry at VizieR.
36. ↑ Anugu, Narsireddy et al. (October 2024). "CHARA Near-infrared Imaging of the Yellow Hypergiant Star ρ Cassiopeiae: Convection Cells and Circumstellar Envelope". The Astrophysical Journal 974 (1): 113. doi:10.3847/1538-4357/ad6b2b. Bibcode: 2024ApJ...974..113A.
37. ↑ Anugu, Narsireddy; Gies, Douglas R.; Roettenbacher, Rachael M.; Monnier, John D.; Montargés, Miguel; Mérand, Antoine; Baron, Fabien; Schaefer, Gail H. et al. (September 2024). "Time Evolution Images of the Hypergiant RW Cephei during the Rebrightening Phase Following the Great Dimming" (in en). The Astrophysical Journal Letters 973 (1): L5. doi:10.3847/2041-8213/ad736c. ISSN 2041-8205. Bibcode: 2024ApJ...973L...5A.
38. ↑ Anugu, Narsireddy; Baron, Fabien; Gies, Douglas R.; Lanthermann, Cyprien; Schaefer, Gail H.; Shepard, Katherine A.; ten Brummelaar, Theo; Monnier, John D. et al. (July 2023). "The Great Dimming of the hypergiant star RW Cephei: CHARA Array images and spectral analysis". The Astronomical Journal 166 (2): 78. doi:10.3847/1538-3881/ace59d. Bibcode: 2023AJ....166...78A.
39. ↑ van Genderen, A. M.; Lobel, A.; Nieuwenhuijzen, H.; Henry, G. W.; de Jager, C.; Blown, E.; Di Scala, G.; van Ballegoij, E. J. (2019-11-01). "Pulsations, eruptions, and evolution of four yellow hypergiants". Astronomy and Astrophysics 631: A48. doi:10.1051/0004-6361/201834358. ISSN 0004-6361. Bibcode: 2019A&A...631A..48V. https://ui.adsabs.harvard.edu/abs/2019A&A...631A..48V/abstract.
40. ↑ Wittkowski, M; Abellan, F. J; Arroyo-Torres, B; Chiavassa, A; Guirado, J. C; Marcaide, J. M; Alberdi, A; De Wit, W. J et al. (28 September 2017). "Multi-epoch VLTI-PIONIER imaging of the supergiant V766 Cen: Image of the close companion in front of the primary". Astronomy & Astrophysics 1709: L1. doi:10.1051/0004-6361/201731569. Bibcode: 2017A&A...606L...1W.
41. ↑ Munoz-Sanchez, G.; Kalitsounaki, M.; Wit, S. de; Antoniadis, K.; Bonanos, A. Z.; Zapartas, E.; Boutsia, K.; Christodoulou, E. et al. (2024-12-02), The dramatic transition of the extreme Red Supergiant WOH G64 to a Yellow Hypergiant
42. ↑ Ohnaka, K.; Hofmann, K.-H.; Weigelt, G.; Loon, J. Th van; Schertl, D.; Goldman, S. R. (2024-11-01). "Imaging the innermost circumstellar environment of the red supergiant WOH G64 in the Large Magellanic Cloud" (in en). Astronomy & Astrophysics 691: L15. doi:10.1051/0004-6361/202451820. ISSN 0004-6361. Bibcode: 2024A&A...691L..15O. https://www.aanda.org/articles/aa/full_html/2024/11/aa51820-24/aa51820-24.html.
43. ↑ González-Torà, G.; Wittkowski, M.; Davies, B.; Plez, B. (2023-12-19), "The effect of winds on atmospheric layers of red supergiants II. Modelling VLTI/GRAVITY and MATISSE observations of AH Sco, KW SGR, V602 Car, CK Car, and V460 Car", Astronomy & Astrophysics 683: A19, doi:10.1051/0004-6361/202348047, http://arxiv.org/abs/2312.12521, retrieved 2025-12-03
44. ↑ Climent, J. B.; Wittkowski, M.; Chiavassa, A.; Baron, F.; Marcaide, J. M.; Guirado, J. C.; Freytag, B.; Höfner, S. et al. (2020-02-21), "VLTI-PIONIER imaging of the red supergiant V602 Carinae", Astronomy & Astrophysics 635: A160, doi:10.1051/0004-6361/201936734, Bibcode: 2020A&A...635A.160C, http://arxiv.org/abs/2002.09243, retrieved 2025-10-25

* v
* t
* e

Stars

Formation|

* Accretion
* Molecular cloud
* Bok globule
* Young stellar object
* Protostar
* Pre-main-sequence
* Herbig Ae/Be
* T Tauri
* FU Orionis
* Herbig–Haro object
* Hayashi track
* Henyey track

Evolution|

* Main sequence
* Red-giant branch
* Horizontal branch
* Red clump
* Asymptotic giant branch
* Blue loop
* Protoplanetary nebula
* Planetary nebula
* PG1159
* Dredge-up
* Instability strip
* Luminous blue variable
* Blue straggler
* Stellar population
* Supernova
* Superluminous supernova / Hypernova

Spectral
classification|

* Early
* Late
* Main sequence
* O
* B
* A
* F
* G
* K
* M
* Brown dwarf
* WR
* OB
* Subdwarf
* O
* B
* Subgiant
* Giant
* Blue
* Red
* Yellow
* Bright giant
* Supergiant
* Blue
* Red
* Yellow
* Hypergiant
* Yellow
* Carbon
* S
* CN
* CH
* White dwarf
* Chemically peculiar
* Am
* Ap/Bp
* HgMn
* Helium-weak
* Barium
* Extreme helium
* Lambda Boötis
* Lead
* Technetium
* Be
* Shell
* B[e]

Remnants|

* White dwarf
* Helium planet
* Black dwarf
* Neutron
* Radio-quiet
* Pulsar
* Binary
* X-ray
* Magnetar
* Stellar black hole
* X-ray binary
* Burster

Hypothetical|

* Blue dwarf
* Green
* Black dwarf
* Exotic
* Boson
* Electroweak
* Strange
* Preon
* Planck
* Dark
* Dark-energy
* Quark
* Q
* Black
* Gravastar
* Frozen
* Quasi-star
* Thorne–Żytkow object
* Iron
* Blitzar

Stellar
nucleosynthesis|

* Deuterium burning
* Lithium burning
* Proton–proton chain
* CNO cycle
* Helium flash
* Triple-alpha process
* Alpha process
* Carbon burning
* Neon burning
* Oxygen burning
* Silicon burning
* S-process
* R-process
* Fusor
* Nova
* Symbiotic
* Remnant
* Luminous red nova

Structure|

* Core
* Convection zone
* Microturbulence
* Oscillations
* Radiation zone
* Atmosphere
* Photosphere
* Starspot
* Chromosphere
* Corona
* Stellar wind
* Bubble
* Bipolar outflow
* Accretion disk
* Asteroseismology
* Helioseismology
* Eddington luminosity
* Kelvin–Helmholtz mechanism

Properties|

* Designation
* Dynamics
* Effective temperature
* Luminosity
* Kinematics
* Magnetic field
* Absolute magnitude
* Mass
* Metallicity
* Rotation
* Starlight
* Variable
* Photometric system
* Color index
* Hertzsprung–Russell diagram
* Color–color diagram

Star systems|

* Binary
* Contact
* Common envelope
* Eclipsing
* Symbiotic
* Multiple
* Cluster
* Open
* Globular
* Super
* Planetary system

Earth-centric
observations|

* Sun
* Solar System
* Sunlight
* Pole star
* Circumpolar
* Constellation
* Asterism
* Magnitude
* Apparent
* Extinction
* Photographic
* Radial velocity
* Proper motion
* Parallax
* Photometric-standard

Lists|

* Proper names
* Arabic
* Chinese
* Extremes
* Most massive
* Highest temperature
* Largest volume
* Smallest volume
* Brightest
* Historical
* Most luminous
* Nearest
* Nearest bright
* With exoplanets
* Brown dwarfs
* White dwarfs
* Milky Way novae
* Supernovae
* Candidates
* Remnants
* Planetary nebulae
* Timeline of stellar astronomy

Related articles|

* Substellar object
* Brown dwarf
* Sub-brown dwarf
* Planet
* Galactic year
* Galaxy
* Guest
* Gravity
* Intergalactic
* Starfield
* Tidal disruption event

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