List of stars with resolved images
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 directly imaged, has an angular diameter of only 50 milliarcseconds (mas).[1]
List
Star | Image | Diameter | Distance (ly) |
Imager | Notes | |
---|---|---|---|---|---|---|
Angular (mas) | Geometric (Sun = 1) | |||||
The Sun | 1 930 000 | 1 | 0.000 015 8 (1 AU) |
Resolvable with the naked eye; see also solar telescope. |
Closest, brightest, and largest star by apparent diameter. | |
Proxima Centauri | 1.02 ± 0.08 | 0.141 ± 0.007 | 4.246 ± 0.006 | Very Large Telescope | 2nd closest star. | |
Rigil Kentaurus (Alpha Centauri A) | 8.511 ± 0.020 | 1.224 ± 0.003 | 4.37 | Very Large Telescope - VINCI/VLTI[2] | ||
Toliman (Alpha Centauri B) | 6.001 ± 0.034 | 0.863 ± 0.005 | ||||
Altair | 3.2 | 1.66 ± 0.01 (polar) 2.02 ± 0.01 (equator) |
16.77 ± 0.08 | CHARA array - MIRC[3] | ||
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[4] | ||
Alderamin (Alpha Cephei) | 1.35 ± 0.02 (polar) 1.75 ± 0.03 (equatorial) |
2.20 ± 0.04 (polar) 2.74 ± 0.04 (equator) |
48.8 ± 0.36 | CHARA array - MIRC[4] | ||
Caph (Beta Cassiopeiae) | 1.70 ± 0.04 | 3.1 ± 0.1 (polar) 3.8 ± 0.1 (equator) |
54.7 ± 0.3 | CHARA array - MIRC[5] | ||
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[5] | ||
Algol Aa1 (Beta Persei Aa1) (stationary object) |
0.88 ± 0.05 | 4.13 | 93 ± 2 | CHARA array - MIRC[6] | ||
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[7][8] | First direct imaging of starspots on a star outside the Solar System. | |
R Doradus | 57 ± 5 | 370 ± 50 | 204 ± 9 | New Technology Telescope[9] | 2nd largest known star by apparent diameter in Earth's sky, after the Sun. | |
Mira (Omicron Ceti) | 50 | up to 700 | 420 | Hubble - FOC[10] | ||
T Leporis | 5.8 15 for molecular layer |
100 | 500 | Very Large Telescope - VLTI[11]/AMBER[12] | ||
Pi1 Gruis | 18.37 | 694 | 530 | Very Large Telescope - PIONIER[13] | 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[14] | ||
Betelgeuse | 50 | 630 | 643 ± 146 | |||
Sheliak A (Beta Lyrae A) | 0.46 | 6 | 960 ± 50 | CHARA array - MIRC[18] | ||
Theta1 Orionis C | 0.2 | 10.6 ± 1.5 | 1400 | Very Large Telescope - AMBER[19], GRAVITY[20] |
||
Almaaz A (Epsilon Aurigae A) | 2.27 | 3.7 ± 0.7 | ca. 2000 | CHARA array - MIRC[21] | ||
Almaaz B (Epsilon Aurigae B) | 5.9 ± 0.1 | |||||
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
References
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- P. Kervella, F. Thevenin, D. Segransan, G. Berthomieu, B. Lopez, P. Morel, J. Provost, The diameters of Alpha Centauri A and B - A comparison of the asteroseismic and VINCI/VLTI views, Astronomy and Astrophysics 404 3 (2003) 1087–1097.
- 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.
- 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.
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- "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.
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