Results 51 to 60 of about 15,689 (250)
The Trojan-like Colors of Low-perihelion Kuiper Belt Objects
The Planetary Science JournalAn 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 +1 more source
Observed Binary Fraction Sets Limits on the Extent of Collisional Grinding in the Kuiper Belt
, 2011 The size distribution in the cold classical Kuiper belt can be approximated by two idealized power laws: one with steep slope for radii R>R* and one with shallow slope for ...
Benavidez +29 more
core +1 more source
A Possible Divot in the Size Distribution of the Kuiper Belt's Scattering Objects [PDF]
, 2013 Via joint analysis of a calibrated telescopic survey, which found scattering Kuiper Belt objects, and models of their expected orbital distribution, we measure the form of the scattering object's size distribution.
Gladman, B. +4 more
core +3 more sources
Scandinavian Journal of Medicine &Science in Sports, Volume 36, Issue 3, March 2026.ABSTRACT The study aimed to investigate the effects of 5 weeks of post‐exercise cold‐water immersion (CWI) following high‐intensity interval training (HIIT) sessions on the satellite cell pool, muscle content of inflammatory markers, muscle expression of peroxisome proliferator‐activated receptor‐γ coactivator 1‐α (PGC‐1α), maximal oxygen uptake (V ...
Elvis S. Malta +6 more
wiley +1 more source
Dynamics of the Kuiper Belt [PDF]
, 1999 Our current knowledge of the dynamical structure of the Kuiper Belt is reviewed here. Numerical results on long term orbital evolution and dynamical mechanisms underlying the transport of objects out of the Kuiper Belt are discussed.
Duncan, M., Levison, H., Malhotra, R.
core +1 more source
The Challenge of Icy Sample Return Begins With Artemis
Geophysical Research Letters, Volume 53, Issue 4, 28 February 2026.Abstract Throughout the Solar System, volatiles are found as solid ices. Returning ices to Earth for scientific analysis is critical to understanding the formation of a Solar System that bears life. This challenge begins with the Artemis missions to the lunar south polar region, where the coldest lunar regolith is enriched in H2O and other ices—systems
D. L. Gilbertson +7 more
wiley +1 more source
Orbital Evolution of Scattered Planets [PDF]
, 2001 A simple dynamical model is employed to study the possible orbital evolution of scattered planets and phase plane analysis is used to classify the parameter space and solutions.
Jiang, Ing-Guey, Yeh, Li-Chin
core +2 more sources
WATER ICE IN THE KUIPER BELT [PDF]
The Astronomical Journal, 2012 We examine a large collection of low resolution near-infrared spectra of Kuiper belt objects and centaurs in an attempt to understand the presence of water ice in the Kuiper belt. We find that water ice on the surface of these objects occurs in three separate manners: (1) Haumea family members uniquely show surfaces of nearly pure water ice, presumably
Brown, M. E. +2 more
openaire +3 more sources
The Dynamic Inducing Magnetic Field Signal at Triton
Geophysical Research Letters, Volume 53, Issue 4, 28 February 2026.Abstract Triton, Neptune's largest moon, is suspected of harboring a subsurface ocean. Detecting sub‐surface oceans requires measuring the ocean's induced magnetic field, typically exploiting common frequencies at which the field environment of the moon changes, in this case Triton's path through Neptune's magnetosphere.
L. Wivell, M. K. Dougherty, A. Masters
wiley +1 more source
The Collisional Divot in the Kuiper belt Size Distribution [PDF]
, 2009 This paper presents the results of collisional evolution calculations for the Kuiper belt starting from an initial size distribution similar to that produced by accretion simulations of that region - a steep power-law large object size distribution that ...
Bernstein +19 more
core +3 more sources