CHARA array

The CHARA (Center for High Angular Resolution Astronomy) array is an optical interferometer, located on Mount Wilson, California. The array consists of six 1-metre (40 in) telescopes operating as an astronomical interferometer. Construction was completed in 2003. CHARA is owned by Georgia State University (GSU).

CHARA array
CHARA 1497.jpg
Alternative namesCHARA Edit this at Wikidata
Coordinates34°13′29″N 118°03′26″W / 34.22469°N 118.05712°W / 34.22469; -118.05712Coordinates: 34°13′29″N 118°03′26″W / 34.22469°N 118.05712°W / 34.22469; -118.05712 Edit this at Wikidata
OrganizationGeorgia State University Edit this on Wikidata
Telescope styleoptical telescope Edit this on Wikidata Edit this at Wikidata
CHARA array is located in the United States
CHARA array
Location of CHARA array


CHARA’s six telescopes each have a one-meter diameter mirror to reflect light. They are spread across Mount Wilson to increase the angular resolution of the array. Each of the six telescopes provides a different image, to combine it into one image the light from each telescope is transported through vacuum tubes and fed into a single beam, where they are matched up to within one micron. This process is called interferometry, and allows the array to have the same resolving power as a telescope with a 330-meter mirror, and an angular resolution of 200 micro-arcseconds.[1][2]


In 1984 CHARA was founded, and with financial support from the National Science Foundation (NSF), in 1985 planning for the array began. Construction for the array started on July 13, 1996, and with $6.3 million awarded to GSU by the NSF, and the same amount matched by GSU, going towards the effort. In July 1998, GSU was awarded another $1.5 million by W.M. Keck Foundation, which allowed for a sixth telescope to be added to the previously planned five. With a final gift of $574,000 from David and Lucile Packard Foundation, the funding for the array was completed in October 1998.[3]

After another five years of construction, the CHARA array was completed in 2003. In April of the same year, CHARA was awarded a 3-year grant to support scientific programs at the center, which was renewed in 2006.[3] In 2013 another grant from the NSF worth 3.6 million was given to the Center.[4]

Observatories throughout the world have come to CHARA to test beam combining technology.[5]


Animation showing the Beta Lyrae eclipsing binary, using images from the CHARA array

On January 15, 2007, the diameter of an exoplanet was measured directly, using CHARA. This was achieved by using the observed angular diameter of the star that the planet orbited, and the already known distance of the star from Earth, to get the diameter of the star. With this they could calculate the diameter of the exoplanet when comparing its size to the star when it passed in front of it. This was the first time the diameter of an exoplanet was directly measured, and returned a value slightly different than that obtained from indirect, more conventional methods.[6]

In 2013 CHARA was used to capture images showing the starspots on Zeta Andromedae, a star 181 light years away. This was the first time that images of starspots on stars other than our Sun has been taken.[7][8]

CHARA directly observed binary stars, such as Beta Lyrae and Algol.[9][10] CHARA directly imaged multiple stars, such as Regulus, Rasalhague, Altair, Alderamin and Beta Cassiopeiae to measure the flattened shape of these rapidly rotating stars. Because the equator is further from the center of the star, it will appear cooler than the poles, an effect called gravity darkening.[11]

The CHARA array can also resolve the circumstellar disks around Be-stars and measure the disk precession variations.[12]


CHARA holds annual science meetings where recent advancements in science and technologies relevant to the array are discussed. The center also gives access to the array to the astronomical community using the National Optical Astronomy Observatory peer review system for around 50 nights per year. They also have periodic community workshops.

See alsoEdit

  1. ^ "About". Retrieved 2017-10-26.
  2. ^ Hand, Eric (2010-04-07). "Telescope arrays give fine view of stars". Nature News. 464 (7290): 820–821. Bibcode:2010Natur.464..820H. doi:10.1038/464820a. PMID 20376117.
  3. ^ a b Baron, Fabien. "History of CHARA". Retrieved 2017-10-26.
  4. ^ "CHARA Array awarded $3.9 million to provide telescope access to scientists across the nation". EurekAlert!. Retrieved 2017-10-26.
  5. ^ Leverington, David (2016-11-24). Observatories and Telescopes of Modern Times: Ground-Based Optical and Radio Astronomy Facilities since 1945. Cambridge University Press. ISBN 9781316841815.
  6. ^ "CHARA measures an exoplanet". Retrieved 2017-10-26.
  7. ^ "'Starspot' Images that Give Insight into Early Sun Captured by University's CHARA Telescope Array - News Hub -". News Hub. 2016-05-04. Retrieved 2017-10-26.
  8. ^ "Seeing Stars |". Discover Magazine. Retrieved 2017-10-26.
  9. ^ Zhao, M.; Gies, D.; Monnier, J. D.; Thureau, N.; Pedretti, E.; Baron, F.; Merand, A.; ten Brummelaar, T.; McAlister, H.; Ridgway, S. T.; Turner, N. (September 2008). "First Resolved Images of the Eclipsing and Interacting Binary β Lyrae". ApJL. 684 (2): L95. arXiv:0808.0932. Bibcode:2008ApJ...684L..95Z. doi:10.1086/592146. ISSN 0004-637X.
  10. ^ Baron, F.; Monnier, J. D.; Pedretti, E.; Zhao, M.; Schaefer, G.; Parks, R.; Che, X.; Thureau, N.; ten Brummelaar, T. A.; McAlister, H. A.; Ridgway, S. T. (June 2012). "Imaging the Algol Triple System in the H Band with the CHARA Interferometer". ApJ. 752 (1): 20. Bibcode:2012ApJ...752...20B. doi:10.1088/0004-637X/752/1/20. hdl:2027.42/98563. ISSN 0004-637X.
  11. ^ "CHARA - Rapid Rotators". Retrieved 2020-01-24.
  12. ^ "CHARA - Be Stars". Retrieved 2020-01-24.