List of stars with resolved images
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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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Star | Image | Diameter | Distance (ly) |
Imager | Notes | |
---|---|---|---|---|---|---|
Angular (mas) | Geometric (Sun = 1) | |||||
Sun | ![]() |
2×106 | 1 | 0.0000158 | Various | |
Altair | ![]() |
3.2 | 1.66±0.01 (polar) 2.02±0.01 (equator) |
16.77±0.08 | CHARA array - MIRC[2] | |
Rasalhague (Alpha Ophiuchi A) | 1.62±0.03 | 2.39±0.01 (polar) 2.87±0.02 (equator) |
48.6±0.8 | CHARA array - MIRC[3] | ||
Alderamin (Alpha Cephei) | 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[3] | ||
Caph (Beta Cassiopeiae) | 1.70±0.04 | 3.1±0.1 (polar) 3.8±0.1 (equator) |
54.7±0.3 | CHARA array - MIRC[4] | ||
Regulus (Alpha Leonis A) | 1.24±0.02 | 3.2±0.1 (polar) 4.2±0.1 (equator) |
79.3±0.7 | CHARA array - MIRC[4] | ||
Algol Aa1 (Beta Persei Aa1) (stationary object) |
![]() ![]() |
0.88±0.05 | 4.13 | 93±2 | CHARA array - MIRC[5] | |
Algol Aa2 (Beta Persei Aa2) (orbiting object) |
1.12±0.07 | 3 | ||||
Algol Ab (Beta Persei 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☉. | |||
Zeta Andromedae Aa | 2.502±0.008 | 15.0±0.8 (polar) | 189±3 | CHARA array - MIRC[6][7] | First direct imaging of starspots on a star outside the Solar System. | |
R Doradus | ![]() |
57±5 | 370±50 | 204±9 | New Technology Telescope[8] | 2nd largest known star by apparent diameter in Earth's sky, after the Sun. |
Mira (Omicron Ceti) | ![]() |
50 | up to 700 | 420 | Hubble - FOC[9] | |
T Leporis | ![]() |
5.8 15 for molecular layer |
100 | 500 | Very Large Telescope - VLTI[10]/AMBER[11] | |
Pi1 Gruis | ![]() |
18.37[citation needed] | 694 | 530 | Very Large Telescope - VLTI/PIONIER[12] | First directly observed granulation patterns on a star's surface outside the Solar System. |
Antares | ![]() |
41.3±0.1 | 700 | 620 | Very Large Telescope - VLTI/AMBER[13] | |
Betelgeuse | ![]() |
50 | 630 | 643±146 | ||
Sheliak A (Beta Lyrae A) | 0.46 | 6 | 960±50 | CHARA array - MIRC[17] | ||
Theta1 Orionis C | ![]() |
0.2 | 10.6±1.5 | 1400 | Very Large Telescope - AMBER[18], GRAVITY[19] |
|
Almaaz A (Epsilon Aurigae A) | 2.27 | 3.7±0.7 | ca. 2000 | CHARA array - MIRC[20] | Supergiant with an eclipsing companion surrounded by a massive, opaque debris disk | |
HR 5171 | ![]() |
4.1±0.8 | 1575±400 | 11740±1630 | Very Large Telescope - VLTI/PIONIER[21] | Eclipsing and potential contact binary yellow hypergiant |
β Tau (Beta Tauri) | 1.09±0.076 | 4.82±0.34 | 134±2 | CHARA array [22] | ||
η UMa (Eta Ursae Majoris) | 0.834±0.060 | 2.86±0.21 | 103.9±0.8 | CHARA array [22] | ||
α Peg (Alpha Pegasi) | 1.052±0.066 | 4.62±0.29 | 133±1 | CHARA array [22] |
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
- ^ a b 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. Bibcode:1998AJ....116.2501U. doi:10.1086/300596.
- ^ J.D. Monnier; et al. (2007). "Imaging the Surface of Altair". Science. 317 (5836): 342–5. arXiv:0706.0867. Bibcode:2007Sci...317..342M. doi:10.1126/science.1143205. PMID 17540860.
- ^ a b M. Zhao; et al. (2009). "Imaging And Modeling Rapidly Rotating Stars: Alpha Cephei And Alpha Ophiuchi". The Astrophysical Journal. 701 (1): 209–224. arXiv:0906.2241. Bibcode:2009ApJ...701..209Z. doi:10.1088/0004-637X/701/1/209.
- ^ a b X. Che; et al. (2011). "Colder And Hotter: Interferometric Imaging Of Beta Cassiopeiae And ?lpha Leonis". The Astrophysical Journal. 732 (2): 68. arXiv:1105.0740. Bibcode:2011ApJ...732...68C. doi:10.1088/0004-637X/732/2/68.
- ^ Baron, F.; Monnier, J.; Pedretti, E.; Zhao, M.; Schaefer, G.; Parks, R.; Che, X.; Thureau, N.; ten Brummelaar, T. A.; McAlister, H. A.; Ridgway, S. T.; Farrington, C.; Sturmann, J.; Sturmann, L.; Turner, N. (2012). "Imaging the Algol Triple System in the H Band with the CHARA Interferometer". The Astrophysical Journal. 752 (1): 20. arXiv:1205.0754. Bibcode:2012ApJ...752...20B. doi:10.1088/0004-637X/752/1/20.
- ^ 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. arXiv:1301.0445. Bibcode:2007A&A...463.1071K. doi:10.1051/0004-6361:20065982.
- ^ Roettenbacher, R.M.; Monnier, J.D.; Korhonen, H.; Aarnio, A.N.; Baron, F.; Che, X.; Harmon, R.O.; Kővári, Zs.; Kraus, S.; Schaefer, G.H.; Torres, G.; Zhao, M.; Ten Brummelaar, T.A.; Sturmann, J.; Sturmann, L. (2016). "No Sun-like dynamo on the active star ζ Andromedae from starspot asymmetry". Nature. 533 (7602): 217–220. arXiv:1709.10107. Bibcode:2016Natur.533..217R. doi:10.1038/nature17444. PMID 27144357.
- ^ "The Biggest Star in the Sky". ESO. March 11, 1997. Retrieved 2010-06-26.
- ^ "Hubble Separates Stars in the Mira Binary System". HubbleSite. 6 August 1997. Retrieved 26 June 2017.
- ^ "Hundred metre virtual telescope captures unique detailed colour image". European Southern Observatory. 18 February 2009. 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". www.eso.org. Retrieved 22 December 2017.
- ^ "Astronomers Capture Best-Ever Image of Alien Star". Scientific American. 24 August 2017. Retrieved 27 August 2017.
- ^ "Betelgeuse captured by ALMA". European Southern Observatory. 26 June 2017. Retrieved 26 June 2017.
- ^ "Sharpest views of Betelgeuse reveal how supergiant stars lose mass". European Southern Observatory. 29 July 2009. Retrieved 26 June 2017.
- ^ "The Flames of Betelgeuse". European Southern Observatory. 23 June 2011. Retrieved 26 June 2017.
- ^ M. Zhao; et al. (2008). "First Resolved Images Of The Eclipsing And Interacting Binary Beta Lyrae". The Astrophysical Journal. 684 (2): L95–L98. arXiv:0808.0932. Bibcode:2008ApJ...684L..95Z. doi:10.1086/592146.
- ^ "The orbit of Theta1 Orionis C". European Southern Observatory. 18 February 2009. Retrieved 26 June 2017.
- ^ "GRAVITY discovers new double star in Orion Trapezium cluster". European Southern Observatory. 13 January 2016. Retrieved 26 June 2017.
- ^ B. Kloppenborg; et al. (2010). "Infrared images of the transiting disk in the Epsilon Aurigae system". Nature. 464 (7290): 370–2. arXiv:1004.2464. Bibcode:2010Natur.464..870K. doi:10.1038/nature08968. PMID 20376144.
- ^ Wittkowski, M; Abellan, F. J; Arroyo-Torres, B; Chiavassa, A; Guirado, J. C; Marcaide, J. M; Alberdi, A; De Wit, W. J; Hofmann, K.-H; Meilland, A; Millour, F; Mohamed, S; Sanchez-Bermudez, J (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. arXiv:1709.09430. Bibcode:2017A&A...606L...1W. doi:10.1051/0004-6361/201731569. S2CID 54740936.
- ^ a b c 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. eISSN 1538-4357.
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