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The following is a list of stars with resolved images, that is, stars whose images have been resolved beyond a point source.[clarification needed] 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 directly imaged, has an angular diameter of only 50 milliarcseconds (mas).[1]
List
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List of stars with resolved images
| Star
|
Image
|
Diameter
|
Distance (ly)
|
First imager
|
Year
|
Notes
|
| Angular (mas)
|
Geometric (Sun = 1)
|
| Sun
|
|
2000000
|
1
|
0.0000158
|
Louis Fizeau and Léon Foucault[2]
|
1845
|
|
Altair α Aql
|
|
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
|

|
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
|
|
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[8][9]
|
1996
|
First direct imaging of starspots on a star outside the Solar System.
|
| R Dor
|
|
57±5
|
370±50
|
204±9
|
New Technology Telescope[10]
|
1993
|
2nd largest known star by apparent diameter in Earth's sky, after the Sun.
|
Mira ο Cet A
|
|
50
|
up to 700
|
420
|
Hubble – FOC[11]
|
1997[citation needed]
|
|
| T Lep
|
|
5.8 15 for molecular layer
|
100
|
500
|
Very Large Telescope – VLTI[12]/AMBER[13]
|
2009[citation needed]
|
|
| π1 Gru
|
|
18.37[citation needed]
|
694
|
530
|
Very Large Telescope – VLTI/PIONIER[14]
|
2017[citation needed]
|
First directly observed granulation patterns on a star's surface outside the Solar System.
|
Antares α Sco A
|
|
41.3±0.1
|
700
|
620
|
Very Large Telescope – VLTI/AMBER[15]
|
2017[citation needed]
|
|
Betelgeuse α Ori
|
|
50
|
630
|
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[16]
|
2007
|
Both Aa1 and Aa2 are visible in the animation.
|
| θ1 Ori C
|
|
0.2
|
10.6±1.5
|
1400
|
Very Large Telescope – AMBER[17]
|
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[18]
|
2016[citation needed]
|
Almaaz ε Aur A
|
|
2.27
|
3.7±0.7
|
ca. 2000
|
CHARA array – MIRC[19]
|
2009
|
Supergiant with an eclipsing companion surrounded by a massive, opaque debris disk
|
| RW Cephei
|
|
2.45
|
900–1760
|
11000+4600 −2600–22000+5200 −3300
|
CHARA array – MIRC-X and MYSTIC[20]
|
2022
|
Hypergiant star currently undergoing a great dimming event
|
| HR 5171 Aa
|
|
4.1±0.8
|
1575±400
|
11740±1630
|
Very Large Telescope – VLTI/PIONIER[21]
|
2014
|
Eclipsing and potential contact binary yellow hypergiant
|
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 and brown dwarfs
References
- ↑ 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.
- ↑ "NASA – Sun–Earth Day – Technology Through Time". 2006. https://sunearthday.nasa.gov/2006/locations/firstphoto.php.
- ↑ 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.
- ↑ 4.0 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.
- ↑ 5.0 5.1 X. Che (2011). "Colder And Hotter: Interferometric Imaging Of Beta Cassiopeiae And ?lpha Leonis". The Astrophysical Journal 732 (2): 68. doi:10.1088/0004-637X/732/2/68. Bibcode: 2011ApJ...732...68C.
- ↑ 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.
- ↑ 7.0 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.
- ↑ 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.
- ↑ 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.
- ↑ "The Biggest Star in the Sky". ESO. March 11, 1997. http://www.eso.org/public/news/eso9706/. Retrieved 2010-06-26.
- ↑ "Hubble Separates Stars in the Mira Binary System". HubbleSite. 6 August 1997. http://hubblesite.org/news_release/news/1997-26. Retrieved 26 June 2017.
- ↑ "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.
- ↑ 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.
- ↑ "Giant Bubbles on Red Giant Star's Surface". European Southern Observatory. https://www.eso.org/public/news/eso1741/. Retrieved 22 December 2017.
- ↑ "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.
- ↑
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.
- ↑ "The orbit of Theta1 Orionis C". European Southern Observatory. 18 February 2009. https://www.eso.org/public/unitedkingdom/images/eso0906d/. Retrieved 26 June 2017.
- ↑ "First Light For Future Black Hole Probe". European Southern Observatory. 13 January 2016. https://www.eso.org/public/news/eso1601/. Retrieved 18 June 2023.
- ↑ 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.
- ↑ 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.
- ↑ 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.
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