Results 41 to 50 of about 1,958 (128)
Brownian Motion in Planetary Migration [PDF]
A residual planetesimal disk of mass 10-100 Earth masses remained in the outer solar system following the birth of the giant planets, as implied by the existence of the Oort cloud, coagulation requirements for Pluto, and inefficiencies in planet ...
Eugene I. Chiang +4 more
core +2 more sources
The long-term evolution of the outer solar system is subject to the influence of the giant planets, however, perturbations from other massive bodies located in the region imprint secular signatures, which are discernible in long-term simulations. In this
Marco A. Muñoz-Gutiérrez +2 more
doaj +1 more source
Inner solar system dynamical analogs for plutinos [PDF]
By studying orbits of near-Earth asteroids potentially in 2:3 mean motion resonance with Earth, Venus, and Mars, we have found plutino analogs. We identify 23 objects in the inner solar system dynamically protected from encounter through this resonance ...
Brasser, Ramon +3 more
core
The dynamics of Plutinos [PDF]
Plutinos are Kuiper-belt objects that share the 3:2 Neptune resonance with Pluto. The long-term stability of Plutino orbits depends on their eccentricity. Plutinos with eccentricities close to Pluto (fractional eccentricity difference |e-e_p|/e_p=0.3 can
Tremaine, Scott, Yu, Qingjuan
core +3 more sources
Estimating Solar Wind Charge Exchange Generated Soft X‐Rays in the Jovian Magnetosheath
Abstract Solar Wind Charge eXchange (SWCX) generated soft x‐rays are used extensively to study the interfaces between charged and neutral particles throughout the solar system. This paper outlines the development of a model of Jupiter's magnetosheath using magnetohydrodynamic derived boundary equations and a combination of in situ Juno measurements and
Fenn Leppard +8 more
wiley +1 more source
UEG Week 2022 Poster Presentations
United European Gastroenterology Journal, Volume 10, Issue S8, Page 473-1092, October 2022.
wiley +1 more source
LiDO: Exploring the Stable Plutino Parameter Space
We present a publicly available, high-resolution, filled-parameter-space synthetic distribution of the plutinos, trans-Neptunian objects (TNOs) librating in the 3:2 mean-motion resonance with Neptune, with particular focus on the plutinos simultaneously ...
Samantha M. Lawler +9 more
doaj +1 more source
A study of the high-inclination population in the Kuiper belt - II. The Twotinos [PDF]
As the second part of our study, in this paper we proceed to explore the dynamics of the high-inclination Twotinos in the 1:2 Neptune mean motion resonance (NMMR).
Li, Jian, Sun, Yi-Sui, Zhou, Li-Yong
core +1 more source
Review of asteroid, meteor, and meteorite‐type links
Abstract With the goal to determine the origin of our meteorites in the asteroid belt, video and photographic observations of meteors have now tracked 75 meteorite falls. Six years ago, there were just hints that different meteorite types arrived on different orbits, but now, the number of orbits (N) is high enough for distinct patterns to emerge.
Peter Jenniskens +1 more
wiley +1 more source
Review of Jupiter-Trojan asteroids research
Jupiter-Trojan asteroids, as fossils of planet formation, orbiting the Sun in Jupiter's stable Lagrange points, provide a unique and critical insight into planetary origins, the sources of volatiles and organics on the terrestrial planets, and the ...
Haitao Huang, Yunzhao Wu
doaj +1 more source

