Results 31 to 40 of about 1,643,192 (137)
On the Dynamics of Resonant Kuiper Belt Objects
, 2007 published in the proceedings of the 9th APRIM ...
Jiang, Ing-Guey, Yeh, Li-Chin
openaire +2 more sources
How the formation of Neptune shapes the Kuiper belt
, 2021 Hydrodynamical simulations predict the inward migration of giant planets during the gas phase of the protoplanetary disc. This phenomenon is also invoked to explain resonant and near-resonant exoplanetary system structures. The early inward migration may
Simona Pirani +5 more
core +1 more source
The Trojan-like Colors of Low-perihelion Kuiper Belt Objects [PDF]
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
core +3 more sources
The shape distribution of Kuiper belt objects
, 2003 . If we assume that the periodic brightness variations in a Kuiper Belt lightcurve are determined only by their aspherical shapes and the observing geome-try, the fraction of detectable Kuiper Belt lightcurves and the lightcurve amplitude distribution ...
Pedro Lacerda, Jane Luu
core +1 more source
A Search for Bright Kuiper Belt Objects
, 1998 Since 1992, 60 large Kuiper Belt objects have been detected by ground-based telescopes. Previous surveys which have detected objects have searched approximately 60□° and detected objects with magnitudes 20·6 < mR < 25·0.
R. L. Webster, Michael J. I. Brown
core +1 more source
Satellites and Small Bodies With ALMA: Insights Into Solar System Formation and Evolution
AGU Advances, Volume 6, Issue 6, December 2025.Abstract Our understanding of the formation and evolution of planetary systems has made major advances in the past decade. This progress has been driven in large part by the Atacama Large Millimeter/submillimeter Array (ALMA), which has given us an unprecedented view of solar system bodies themselves, and of the structure and chemistry of forming ...
Katherine de Kleer +3 more
wiley +1 more source
The Planetary Science JournalBeing one of the most populated mean motion resonances (MMRs) with Neptune and lying close to the inner boundary of the present-day cold classical disk, observations of the orbital and surface class distributions of the plutinos in the 3:2 MMR provide ...
Cameron Collyer +8 more
doaj +1 more source
Reassessing the Relationship Between Meteor Radio Afterglows and Optical Persistent Trains
Journal of Geophysical Research: Space Physics, Volume 130, Issue 9, September 2025.Abstract Meteor radio afterglows (MRAs) and optical persistent trains (PTs) are two types of long‐lived phenomena which are occasionally observed following the occurrence of a meteor. Both phenomena are thought to be produced by intrinsic emission mechanisms; PTs have been associated with chemiluminescent reactions between meteoric metals and ...
L. E. Cordonnier +5 more
wiley +1 more source
UEG Week 2023 Poster Presentations
, 2023 United European Gastroenterology Journal, Volume 11, Issue S8, Page 535-1498, October 2023.
wiley +1 more source
LiDO: Discovery of a 10:1 Resonator with a Novel Libration State
The Planetary Science JournalThe Large inclination Distant Objects (L i DO) survey has discovered the first securely classified object in the 10:1 mean motion resonance of Neptune.
Rosemary E. Pike +11 more
doaj +1 more source