XO Project

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Template:Short description 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.[1] It is primarily funded by NASA's Origins Program and the Director's Discretionary Fund of the Space Telescope Science Institute.[2][3]

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.[2]

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.[4] 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.[1] 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.[5]

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
(MJ) 		Radius
(RJ) 		Orbital
period
(d) 		Semimajor
axis
(AU) 		Orbital
eccentricity 		Inclination
(°) 		Discovery
year
Moldoveanu[6] Corona Borealis Template:RA Template:DEC 11.319 600 G1V Negoiu 0.9 1.3 3.941534 0.0488 0 87.7 2006
XO-2N[7] Lynx Template:RA Template:DEC 11.25 486 K0V XO-2Nb 0.57 0.973 2.615838 0.0369 0 88.58 2007
XO-3[8] Camelopardalis Template:RA Template:DEC 9.91 850 F5V XO-3b 11.79 1.217 3.1915239 0.0454 0.26 84.2 2007
Koit[9] Lynx Template:RA Template:DEC 10.78 956 F5V Hämarik 1.72 1.34 4.12502 0.0555 0.0024 88.7 2008
Absolutno[10] Lynx Template:RA Template:DEC 12.1 881 G8V Makropulos 1.15 1.15 4.187732 0.0508 0.0029 86.8 2008
XO-6[11] Camelopardalis Template:RA Template:DEC 10.28 760 F5V XO-6b 4.4 2.07 3.76 0.082 0 86.0 2016
XO-7 Draco Template:RA Template:DEC 10.52 763 G0V XO-7b 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

References

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  1. ^ a b Page Module:Citation/CS1/styles.css has no content."Astronomers Catch Planet By Unusual Means". www.spacedaily.com. Retrieved 2024-12-31.
  2. ^ a b Page Module:Citation/CS1/styles.css has no content."XO-3b: Supersized planet or oasis in the 'brown dwarf desert'?". EurekAlert!. Archived from the original on 2021-03-30. Retrieved 2024-12-31.
  3. ^ Astronomers Use Innovative Technique to Find Extrasolar Planet, HubbleSite
  4. ^ Page Module:Citation/CS1/styles.css has no content.McCullough, P. R.; et al. (2005). "The XO Project: Searching for Transiting Extrasolar Planet Candidates". Publications of the Astronomical Society of the Pacific. 117 (834): 783–795. arXiv:astro-ph/0505560. Bibcode:2005PASP..117..783M. doi:10.1086/432024. S2CID 16972795.
  5. ^ Page Module:Citation/CS1/styles.css has no content.Crouzet, N.; McCullough, P. R.; Long, D.; Rodriguez, P. Montanes; Etangs, A. Lecavelier des; Ribas, I.; Bourrier, V.; Hébrard, G.; Vilardell, F. (February 2017). "Discovery of XO-6b: A Hot Jupiter Transiting a Fast Rotating F5 Star on an Oblique Orbit". The Astronomical Journal. 153 (3): 94. arXiv:1612.02776. Bibcode:2017AJ....153...94C. doi:10.3847/1538-3881/153/3/94. ISSN 1538-3881.
  6. ^ Page Module:Citation/CS1/styles.css has no content.McCullough, P. R.; et al. (2006). "A Transiting Planet of a Sun-like Star". The Astrophysical Journal. 648 (2): 1228–1238. arXiv:astro-ph/0605414. Bibcode:2006ApJ...648.1228M. doi:10.1086/505651. S2CID 8100425.
  7. ^ Page Module:Citation/CS1/styles.css has no content.Burke, Christopher J.; et al. (2007). "XO-2b: Transiting Hot Jupiter in a Metal-rich Common Proper Motion Binary". The Astrophysical Journal. 671 (2): 2115–2128. arXiv:0705.0003. Bibcode:2007ApJ...671.2115B. doi:10.1086/523087. S2CID 13468914.
  8. ^ Page Module:Citation/CS1/styles.css has no content.Johns-Krull, Christopher M.; et al. (2008). "XO-3b: A Massive Planet in an Eccentric Orbit Transiting an F5V Star". The Astrophysical Journal. 677 (1): 657–670. arXiv:0712.4283. Bibcode:2008ApJ...677..657J. doi:10.1086/528950. S2CID 15342571.
  9. ^ Page Module:Citation/CS1/styles.css has no content.McCullough, P. R.; et al. (2008). "XO-4b: An Extrasolar Planet Transiting an F5V Star". arXiv:0805.2921 [astro-ph].
  10. ^ Page Module:Citation/CS1/styles.css has no content.Burke, Christopher J.; et al. (2008). "XO-5b: A Transiting Jupiter-sized Planet with a 4 day Period". The Astrophysical Journal. 686 (2): 1331–1340. arXiv:0805.2399. Bibcode:2008ApJ...686.1331B. doi:10.1086/591497. S2CID 14043772.
  11. ^ Page Module:Citation/CS1/styles.css has no content.Crouzet, N.; et al. (2017). "Discovery of XO-6b: A Hot Jupiter Transiting a Fast Rotating F5 Star on an Oblique Orbit". The Astronomical Journal. 153 (3). 94. arXiv:1612.02776. Bibcode:2017AJ....153...94C. doi:10.3847/1538-3881/153/3/94. S2CID 119082666.


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