orbit determination of 2001 QW 322 , a Kuiper Belt binary with a very large separation whose properties challenge binary-formation and evolution theories. Six years of tracking indicate that the binary's mutual orbit period is ≈25-30 years, that the orbit pole is retrograde and inclined 50-62 • from the ecliptic plane, and, most surprisingly,...
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October 17, 2008 (v1)Journal articleUploaded on: December 4, 2022
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2006 (v1)Journal article
Icarus, 185, pp. 508-522, http://dx.doi.org./10.1016/j.icarus..07.024
Uploaded on: December 3, 2022 -
December 2006 (v1)Journal article
International audience
Uploaded on: February 22, 2023 -
December 2006 (v1)Journal article
International audience
Uploaded on: December 4, 2022 -
2006 (v1)Journal article
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Uploaded on: February 28, 2023 -
July 28, 2011 (v1)Publication
We report the orbital distribution of the trans-neptunian objects (TNOs) discovered during the Canada-France Ecliptic Plane Survey (CFEPS), whose discovery phase ran from early 2003 until early 2007. We obtained characterized observations of 321 sq.deg. of sky to depths in the range g ~23.5 - 24.4 AB mag. We provide a database of 169 TNOs with...
Uploaded on: December 4, 2022 -
October 1, 2011 (v1)Journal article
We report the orbital distribution of the trans-Neptunian objects (TNOs) discovered during the Canada-France Ecliptic Plane Survey (CFEPS), whose discovery phase ran from early 2003 until early 2007. The follow-up observations started just after the first discoveries and extended until late 2009. We obtained characterized observations of 321...
Uploaded on: December 4, 2022 -
June 1, 2009 (v1)Journal article
Astronomical Journal, 137, pp. 4917-4935 (2009)
Uploaded on: December 4, 2022 -
2008 (v1)Journal articleThe Canada-France Ecliptic Plan Survey: L3 Data Release and the Orbital Structure of the Kuiper Belt
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Uploaded on: November 25, 2023 -
2009 (v1)Journal article
International audience
Uploaded on: December 3, 2022 -
2024 (v1)Journal article
Asteroids smaller than 10 km are thought to be rubble piles formed from the reaccumulation of fragments produced in the catastrophic disruption of parent bodies. Ground-based observations reveal that some of these asteroids are today binary systems, in which a smaller secondary orbits a larger primary asteroid. However, how these asteroids...
Uploaded on: August 7, 2024