𝔖 Bobbio Scriptorium
✦   LIBER   ✦

An Overview on the Kuiper Belt and on the Origin of Jupiter-family Comets

✍ Scribed by Alessandro Morbidelli


Book ID
110262065
Publisher
Springer Netherlands
Year
1998
Tongue
English
Weight
1014 KB
Volume
72
Category
Article
ISSN
1572-9478

No coin nor oath required. For personal study only.


πŸ“œ SIMILAR VOLUMES


From the Kuiper Belt to Jupiter-Family C
✍ Harold F. Levison; Martin J. Duncan πŸ“‚ Article πŸ“… 1997 πŸ› Elsevier Science 🌐 English βš– 770 KB

the first discovered on an unstable planet-crossing orbit that lies entirely in the outer Solar System. Since that time, We present numerical orbital integrations of thousands of massless particles as they evolve from Neptune-encountering a total of six objects on similar giant plant-crossing orbit

Considerations on the magnitude distribu
✍ Alessandro Morbidelli; Harold F. Levison; William F. Bottke; Luke Dones; David N πŸ“‚ Article πŸ“… 2009 πŸ› Elsevier Science 🌐 English βš– 416 KB

By examining the absolute magnitude (H) distributions (hereafter HD) of the cold and hot populations in the Kuiper belt and of the Trojans of Jupiter, we find evidence that the Trojans have been captured from the outer part of the primordial trans-neptunian planetesimal disk. We develop a sketch mod

Chaotic Diffusion and the Origin of Come
✍ Alessandro Morbidelli πŸ“‚ Article πŸ“… 1997 πŸ› Elsevier Science 🌐 English βš– 628 KB

2/3 resonance). We have also confirmed the importance of these resonances through the numerical integration of The dynamical structure of the 2 / 3 resonance at small inclination is explored using numerical integrations of test particles both fictitious and ''real'' objects. to compute the evolutio

Collision Rates in the Present-Day Kuipe
✍ Daniel D. Durda; S.Alan Stern πŸ“‚ Article πŸ“… 2000 πŸ› Elsevier Science 🌐 English βš– 202 KB

We present results from our model of collision rates in the presentday Edgeworth-Kuiper Belt and Centaur region. We have updated previous results to allow for new estimates of the total disk population in order to examine surface activation and modification time scales due to cratering impacts. We e

On the population, physical decay and or
✍ Romina P. Di Sisto; Julio A. FernΓ‘ndez; AdriΓ‘n Brunini πŸ“‚ Article πŸ“… 2009 πŸ› Elsevier Science 🌐 English βš– 833 KB

We study the Jupiter family comet (JFC) population assumed to come from the Scattered Disk and transferred to the Jupiter's zone through gravitational interactions with the Jovian planets. We shall define as JFCs those with orbital periods P < 20 yr and Tisserand parameters in the range 2 < T K 3:1,