Results 51 to 60 of about 163 (159)
Giga-year evolution of Jupiter Trojans and the asymmetry problem [PDF]
We present a series of numerical integrations of observed and fictitious Jupiter Trojan asteroids, under the gravitational effects of the four outer planets, for time-spans comparable with the age of the Solar System. From these results we calculate the escape rate from each Lagrange point, and construct dynamical maps of "permanence" time in different
Di Sisto, Romina Paula +2 more
openaire +4 more sources
The impact history and prolonged magmatism of the angrite parent body
Abstract As some of the oldest differentiated materials in our solar system, angrite meteorites can provide unique insights into the earliest stages of planetary evolution. However, the timing of planetary mixing, as evidenced by oxygen isotope variations in the quenched angrites, and the extent of magmatism on the angrite parent body (APB) remain ...
B. G. Rider‐Stokes +8 more
wiley +1 more source
The Distribution of Highly Red-sloped Asteroids in the Middle and Outer Main Belt
Red ( S > 10%/0.1 μ m) spectral slopes are common among Centaurs and trans-Neptunian objects (TNOs) in the outer solar system. Interior to and co-orbital with Jupiter, the red ( S ∼ 10%/0.1 μ m) slopes of D-type main-belt and Jupiter Trojan asteroids are
Oriel A. Humes +2 more
doaj +1 more source
Prospects of a New L5 Trojan Flyby Target for the Lucy Mission
NASA’s Lucy spacecraft is en route to conduct the first close encounter with Jupiter’s Trojans. While most scheduled flybys lie in the L _4 cloud, the only L _5 target is the Patroclus–Menoetius binary. Since each flyby offers unique insights into target
Luis E. Salazar Manzano +8 more
doaj +1 more source
Collisional Evolution of Jupiter Trojans
Jupiter Trojans (JT) are asteroids that populate the Sun-Jupiter Lagrangian regions, L4 and L5, at a mean distance of about 5.2 au from the Sun. These asteroids are believed to be leftovers from the Solar System's early days and have been in stable orbits around Jupiter for billions of years.
openaire +1 more source
Jupiter’s Metastable Companions
Jovian co-orbitals share Jupiter’s orbit and exhibit 1:1 mean-motion resonance with the planet. This includes >10,000 so-called Trojan asteroids surrounding the leading (L4) and trailing (L5) Lagrange points, viewed as stable groups dating back to planet
Sarah Greenstreet +2 more
doaj +1 more source
Size and Shape of Jupiter Trojan (2207) Antenor from Stellar Occultations
Librating around the Lagrange L5, the Jupiter’s Trojan (2207) Antenor has been observed in recent years and its rotational light curve suggests it to be a very likely binary asteroid candidate.
F. S. Ferreira +36 more
doaj +1 more source
Lucy Mission Search Plans for Activity around Its Jovian Trojan Flyby Targets
Activity in small bodies, defined here as the episodic or continuous release of material, was long thought to be exclusively a behavior of comets, but it has since been discovered in some centaurs, main-belt asteroids, and near-Earth asteroids.
S. Alan Stern +11 more
doaj +1 more source
Lucy L′Ralph In-flight Calibration and Results at (152830) Dinkinesh
The L’Ralph instrument is a key component of NASA’s Lucy mission, intended to provide spectral image data of multiple Jupiter Trojans. The instrument operates from ∼0.35 to 4 μ m using two focal plane assemblies: a 350–950 nm multispectral imager, Multi ...
Amy A. Simon +14 more
doaj +1 more source
The NSF-DOE Vera C. Rubin Observatory is a new 8m-class survey facility presently being commissioned in Chile, expected to begin the 10 yr long Legacy Survey of Space and Time (LSST) by the end of 2025.
Jacob A. Kurlander +20 more
doaj +1 more source

