Results 1 to 10 of about 163 (159)
A Crater Chronology for the Jupiter’s Trojan Asteroids
We present a new crater chronology for Jupiter’s Trojan asteroids. This tool can be used to interpret the collisional history of the bodies observed by NASA’s Lucy mission. The Lucy mission will visit a total of six Trojan asteroids: Eurybates, Polymele,
S. Marchi +4 more
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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
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Orbital and Absolute Magnitude Distribution of Jupiter Trojans
Jupiter Trojans (JTs) librate about the Lagrangian stationary centers L4 and L5 associated with this planet on typically small-eccentricity and moderate-inclination heliocentric orbits.
David Vokrouhlický +6 more
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Apsidal asymmetric-alignment of Jupiter Trojans [PDF]
ABSTRACT The most distant Kuiper belt objects exhibit the clustering in their orbits, and this anomalous architecture could be caused by Planet 9 with large eccentricity and high inclination. We then suppose that the orbital clustering of minor planets may be observed somewhere else in the Solar system.
Jian Li, Hanlun Lei, Zhihong J Xia
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CAPTURE OF TROJANS BY JUMPING JUPITER [PDF]
Jupiter Trojans are thought to be survivors of a much larger population of planetesimals that existed in the planetary region when planets formed. They can provide important constraints on the mass and properties of the planetesimal disk, and its dispersal during planet migration.
Nesvorny, David +2 more
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Broadband linear polarization of Jupiter Trojans [PDF]
Accepted for publication on A& ...
Bagnulo, S. +4 more
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Origin and Evolution of Jupiter’s Trojan Asteroids
AbstractThe origin of the Jupiter Trojan asteroids has long been a mystery. Dynamically, the population, which is considerably smaller than the main asteroid belt, librates around Jupiter’s stable L4 and L5 Lagrange points, 60 deg ahead and behind Jupiter.
William F. Bottke +3 more
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Collisional families offer a unique window into the interior composition of asteroid populations. Previous dynamical studies of the Jupiter Trojans have uncovered a handful of potential collisional families, two of which have been subsequently confirmed ...
Ian Wong, Michael E. Brown
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FOSSIL. I. The Spin Rate Limit of Jupiter Trojans [PDF]
Abstract Rotation periods of 53 small (diameters 2 km < D < 40 km) Jupiter Trojans (JTs) were derived using the high-cadence lightcurves obtained by the FOSSIL phase I survey, a Subaru/Hyper Suprime-Cam intensive program. These are the first reported periods measured for JTs with D < 10 km. We found a lower limit of the rotation
Chang, Chan-Kao +27 more
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The tumultuous early era of outer solar system evolution culminated when Neptune migrated across the primordial Kuiper Belt (PKB) and triggered a dynamical instability among the giant planets.
William F. Bottke +8 more
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