Results 11 to 20 of about 208,051 (212)

Kuiper Belt Occultation Predictions [PDF]

open access: yesPublications of the Astronomical Society of the Pacific, 2013
Here we present observations of 7 large Kuiper Belt Objects. From these observations, we extract a point source catalog with $\sim0.01"$ precision, and astrometry of our target Kuiper Belt Objects with $0.04-0.08"$ precision within that catalog. We have developed a new technique to predict the future occurrence of stellar occultations by Kuiper Belt ...
Fraser, Wesley C.   +15 more
openaire   +6 more sources

The Trojan-like Colors of Low-perihelion Kuiper Belt Objects [PDF]

open access: yesThe Planetary Science Journal
An important testable prediction of dynamical instability models for the early evolution of the solar system is that Jupiter Trojans share a source population with the Kuiper Belt.
Matthew Belyakov   +2 more
doaj   +4 more sources

The Plane of the Kuiper Belt [PDF]

open access: yesThe Astronomical Journal, 2004
We present a robust method for measuring the effective plane of the Kuiper belt. The derived plane has an inclination with respect to the ecliptic of 1o.86 and an ascending node of 81o.6, with a 1 σ error in pole position of the plane of 0o.37. The plane of the Kuiper belt is inconsistent with the invariable plane, the plane of Jupiter, and the plane ...
Brown, Michael E., Pan, Margaret
openaire   +4 more sources

Mass of the Kuiper belt [PDF]

open access: yesCelestial Mechanics and Dynamical Astronomy, 2018
The Kuiper belt includes tens of thousands of large bodies and millions of smaller objects. The main part of the belt objects is located in the annular zone between 39.4 au and 47.8 au from the Sun, the boundaries correspond to the average distances for orbital resonances 3:2 and 2:1 with the motion of Neptune.
Pitjeva, E. V., Pitjev, N. P.
openaire   +2 more sources

QUAOAR: A ROCK IN THE KUIPER BELT [PDF]

open access: yesThe Astrophysical Journal, 2010
Here we report WFPC2 observations of the Quaoar-Weywot Kuiper belt binary. From these observations we find that Weywot is on an elliptical orbit with eccentricity of 0.14 {\pm} 0.04, period of 12.438 {\pm} 0.005 days, and a semi-major axis of 1.45 {\pm} 0.08 {\times} 104 km.
Fraser, Wesley C., Brown, Michael E.
openaire   +3 more sources

Dynamical Studies of the Kuiper Belt and the Centaurs

open access: yes, 2013
The Kuiper belt is a population of small bodies located outside Neptune's orbit. The observed Kuiper belt objects (KBOs) can be divided into several subclasses based on their dynamical structure.
Volk, Kathryn Margaret
core   +6 more sources

Population of the Scattered Kuiper Belt [PDF]

open access: yesThe Astrophysical Journal, 2000
15 pages, 3 ...
Trujillo, C. A.   +2 more
openaire   +3 more sources

Understanding the Origin of Planetary Systems: Studying the Kuiper Belt and the Dynamics of Planet Formation [PDF]

open access: yes, 2009
This thesis presents theoretical and observational studies pertaining to the early solar system, planet formation and extrasolar planets. First, we explore the dynamics of protoplanet formation. We find that the growth of protoplanets may be dominated
Schlichting, Hilke Elisabeth
core   +1 more source

Extrasolar Kuiper belts [PDF]

open access: yes, 2020
Chapter to be published in the book "The Trans-Neptunian Solar System" (D. Prialnik, M.A. Barucci and L. Young, eds.).
openaire   +2 more sources

Kuiper belt: Formation and evolution [PDF]

open access: yes, 2020
Review chapter to be published in the book "The Transneptunian Solar System", Dina Prialnik, Maria Antonietta Barucci, Leslie Young Eds ...
Morbidelli, Alessandro, Nesvorný, David
openaire   +3 more sources

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