XO Project
{{Short description|International team of astronomers}}
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.{{Cite web |title=Astronomers Catch Planet By Unusual Means |url=https://www.spacedaily.com/reports/Astronomers_Catch_Planet_By_Unusual_Means.html |access-date=2024-12-31 |website=www.spacedaily.com}} It is primarily funded by NASA's Origins Program and the Director's Discretionary Fund of the Space Telescope Science Institute.{{Cite web |title=XO-3b: Supersized planet or oasis in the 'brown dwarf desert'? |url=http://www.eurekalert.org/pub_releases/2007-05/ru-xsp052507.php |archive-url=http://web.archive.org/web/20210330143231/https://www.eurekalert.org/pub_releases/2007-05/ru-xsp052507.php |archive-date=2021-03-30 |access-date=2024-12-31 |website=EurekAlert! |language=en}}[http://hubblesite.org/newscenter/archive/releases/2006/22/full/ Astronomers Use Innovative Technique to Find Extrasolar Planet, HubbleSite]
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
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 [http://www.newswise.com/articles/view/520570/ on Newswise].
In 2016 three similar double telescopes were operating, two in Spain and one in Utah.{{Cite journal|last1=Crouzet|first1=N.|last2=McCullough|first2=P. R.|last3=Long|first3=D.|last4=Rodriguez|first4=P. Montanes|last5=Etangs|first5=A. Lecavelier des|last6=Ribas|first6=I.|last7=Bourrier|first7=V.|last8=Hébrard|first8=G.|last9=Vilardell|first9=F.|date=February 2017|title=Discovery of XO-6b: A Hot Jupiter Transiting a Fast Rotating F5 Star on an Oblique Orbit|journal=The Astronomical Journal|volume=153|issue=3|pages=94|doi=10.3847/1538-3881/153/3/94|issn=1538-3881|arxiv=1612.02776|bibcode=2017AJ....153...94C |doi-access=free }}
Discoveries
The XO telescope has discovered six objects so far, five are hot Jupiter planets and one, XO-3b, may be a brown dwarf.
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! Star ! App. ! Planet ! Mass ! Radius ! Orbital ! Semimajor ! Inclination ! Discovery | ||||||||||||||
XO-1 | Corona Borealis | {{RA|16|02|12}} | {{DEC|+28|10|11}} | 11.319 | 600 | G1V
| XO-1b | 0.9 | 1.3 | 3.941534 | 0.0488 | 0 | 87.7 | 2006 | |
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| XO-2N | Lynx | {{RA|07|48|07}} | {{DEC|+50|13|33}} | 11.25 | 486 | K0V
| XO-2Nb | 0.57 | 0.973 | 2.615838 | 0.0369 | 0 | 88.58 | 2007 | |
XO-3 | Camelopardalis | {{RA|04|21|53}} | {{DEC|+57|49|01}} | 9.91 | 850 | F5V
| XO-3b | 11.79 | 1.217 | 3.1915239 | 0.0454 | 0.26 | 84.2 | 2007 | |
XO-4 | Lynx | {{RA|07|21|33.1657}} | {{DEC|+58|16|05.005}} | 10.78 | 956 | F5V
| XO-4b | 1.72 | 1.34 | 4.12502 | 0.0555 | 0.0024 | 88.7 | 2008 | |
XO-5 | Lynx | {{RA|07|46|51.959}} | {{DEC|+39|05|40.47}} | 12.1 | 881 | G8V
| XO-5b | 1.15 | 1.15 | 4.187732 | 0.0508 | 0.0029 | 86.8 | 2008 | |
XO-6 | Camelopardalis | {{RA|6|19|10.31}} | {{DEC|+73|49|39.24}} | 10.28 | 760 | F5V | XO-6b | 4.4 | 2.07 | 3.76 | 0.082 | 0 | 86.0 | 2016 |
XO-7
|{{RA|18|29|52.30}} |{{DEC|85|13|59.58}} |10.52 |763 |G0V |0.71 |1.373 |2.8641424 |0.04421 |0.038 |83.45 |2019 |
See also
A subset of XO light curves are available at the NASA Exoplanet Archive.
=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
References
{{Reflist|refs=
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External links
- [http://www.stsci.edu/~pmcc/xo/ The XO Project website]
- [http://www.stsci.edu/~pmcc/xo/ The XO Project website]
- [http://www.spacedaily.com/reports/Astronomers_Catch_Planet_By_Unusual_Means.html Astronomers Catch Planet By Unusual Means] (SpaceDaily) May 19, 2006
{{Exoplanet search projects}}