XO Telescope
The XO Project is an international team of amateur and professional astronomers tasked with identifying extrasolar planets. They are led by Peter R. McCullough of the Space Telescope Science Institute. It is primarily funded by NASA's Origins Program and the Director's Discretionary Fund of the Space Telescope Science Institute.
XO Telescope
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- United States
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wikidata · Q2610009 · wikipedia · XO Telescope
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Duties
Duties
Preliminary identification of possible star candidates starts at the Haleakala telescope in Hawaii by a team of professional astronomers. Once they identify a star that dims slightly from time to time (the transit method), the information is forwarded to a team of amateur astronomers who then investigate for additional evidence suggesting this dimming is caused by a transiting planet. Once enough data is collected, it is forwarded to the University of Texas McDonald Observatory to confirm the presence of a transiting planet by a second team of professional astronomers.
Equipment
Equipment
McCullough and his team employed a relatively inexpensive telescope called the XO Telescope, made from commercial equipment, to search for extrasolar planets. The construction of the one-of-a-kind telescope cost $60,000 for the hardware, and much more than that for the associated software. The telescope consists of two 200-millimeter telephoto camera lenses, and resembles binoculars in shape. It is similar to the TrES survey telescope. It stands on the summit of the Haleakalā volcano and 3,054 m (10,000 foot) in Hawaii. Their first discovery of a Jupiter-sized planet orbiting a Sun-like star 600 light-years from Earth in the constellation Corona Borealis—XO-1b—was reported May 16, 2006 on Newswise. In 2016 three similar double telescopes were operating, two in Spain and one in Utah.
Discoveries
Discoveries
The XO telescope has discovered six objects so far, five are hot Jupiter planets and one, XO-3b, may be a brown dwarf. • Star — Constellation — Right ascension — Declination — App. mag. — Distance (ly) — Spectral type — Planet — Mass — Radius — Orbital period (d) — Semimajor axis (AU) — Orbital eccentricity — Inclination (°) — Discovery year • Moldoveanu — Corona Borealis — 11.319 — 600 — G1V — Negoiu — 0.9 — 1.3 — 3.941534 — 0.0488 — 0 — 87.7 — 2006 • XO-2N — Lynx — 11.25 — 486 — K0V — XO-2Nb — 0.57 — 0.973 — 2.615838 — 0.0369 — 0 — 88.58 — 2007 • XO-3 — Camelopardalis — 9.91 — 850 — F5V — XO-3b — 11.79 — 1.217 — 3.1915239 — 0.0454 — 0.26 — 84.2 — 2007 • Koit — Lynx — 10.78 — 956 — F5V — Hämarik — 1.72 — 1.34 — 4.12502 — 0.0555 — 0.0024 — 88.7 — 2008 • Absolutno — Lynx — 12.1 — 881 — G8V — Makropulos — 1.15 — 1.15 — 4.187732 — 0.0508 — 0.0029 — 86.8 — 2008 • XO-6 — Camelopardalis — 10.28 — 760 — F5V — XO-6b — 4.4 — 2.07 — 3.76 — 0.082 — 0 — 86.0 — 2016 • XO-7 — Draco — 10.52 — 763 — G0V — XO-7b — 0.71 — 1.373 — 2.8641424 — 0.04421 — 0.038 — 83.45 — 2019
Other Ground-Based Transit Surveys
Other Ground-Based Transit Surveys
• Next-Generation Transit Survey • Trans-Atlantic Exoplanet Survey or TrES • HATNet Project or HAT • Kilodegree Extremely Little Telescope or KELT • SuperWASP or WASP
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- United States
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Licensing
Text attribution
Part of the biographical narrative on this page reuses licensed material. Its origin, revision and licence are recorded here.
The biographical narrative on this page is based on the Wikipedia article XO Project, revision 1318234544 (EN edition), by its contributors. VALÉORINE has edited that text and built its own documentary record around it. The reused material is available under CC BY-SA 4.0, and this page's reuse of it is offered under the same licence. Everything else on this page — the chronology, the holdings, the evidence, the plates and the connections — is VALÉORINE's own record. Sources and licences.
Notes from the source article
Cited by Wikipedia
Notes from the source article
These works are cited by the source article, in its own numbering. They are recorded as its citations, not as sources VALÉORINE has verified.
- 1.Astronomers Catch Planet By Unusual Means. www.spacedaily.com.
- 2.XO-3b: Supersized planet or oasis in the 'brown dwarf desert'?. EurekAlert!.
- 3.Astronomers Use Innovative Technique to Find Extrasolar Planet, HubbleSite
- 4.McCullough, P. R. The XO Project: Searching for Transiting Extrasolar Planet Candidates. Publications of the Astronomical Society of the Pacific. 117. 834. 783–795. 2005. 10.1086/432024.
- 5.Crouzet, N. Discovery of XO-6b: A Hot Jupiter Transiting a Fast Rotating F5 Star on an Oblique Orbit. The Astronomical Journal. 153. 3. 94. February 2017. 1538-3881.
- 6.McCullough, P. R. A Transiting Planet of a Sun-like Star. The Astrophysical Journal. 648. 2. 1228–1238. 2006. 10.1086/505651.
- 7.Burke, Christopher J. XO-2b: Transiting Hot Jupiter in a Metal-rich Common Proper Motion Binary. The Astrophysical Journal. 671. 2. 2115–2128. 2007. 10.1086/523087.
- 8.Johns-Krull, Christopher M. XO-3b: A Massive Planet in an Eccentric Orbit Transiting an F5V Star. The Astrophysical Journal. 677. 1. 657–670. 2008. 10.1086/528950.
- 9.McCullough, P. R. XO-4b: An Extrasolar Planet Transiting an F5V Star. 2008.
- 10.Burke, Christopher J. XO-5b: A Transiting Jupiter-sized Planet with a 4 day Period. The Astrophysical Journal. 686. 2. 1331–1340. 2008. 10.1086/591497.
- 11.Crouzet, N. Discovery of XO-6b: A Hot Jupiter Transiting a Fast Rotating F5 Star on an Oblique Orbit. The Astronomical Journal. 153. 3. 94. 2017. 10.3847/1538-3881/153/3/94.
References
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The Encyclopedia exists whether or not anything is for sale. Corrections are recorded rather than overwritten, and every version of this record is kept. Published 16 August 2026.
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