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Context. Jupiter-family comets (JFCs), which originate from the Kuiper belt and scattered disk, exhibit low-inclination and chaotic trajectories due to close encounters with Jupiter. Despite their typically short incursions into the inner…

地球与行星天体物理 · 物理学 2024-10-01 P. M. Shober , G. Tancredi , J. Vaubaillon , H. A. R. Devillepoix , S. Deam , S. Anghel , E. K. Sansom , F. Colas , S. Martino

We present the results of "snapshot" numerical integrations of test particles representing comet-like and asteroid-like objects in the inner solar system aimed at investigating the short-term dynamical evolution of objects close to the…

地球与行星天体物理 · 物理学 2016-05-25 Henry H. Hsieh , Nader Haghighipour

Evidence for cometary activity beyond Jupiter and Saturn's orbits -- such as that observed for Centaurs and long period comets -- suggests that the thermal processing of comet nuclei starts long before they enter the inner Solar System,…

地球与行星天体物理 · 物理学 2022-04-06 Anastasios Gkotsinas , Aurélie Guilbert-Lepoutre , Sean N. Raymond , David Nesvorný

The short period Jupiter family comets (JFCs) are thought to originate in the Kuiper Belt; specifically, a dynamical subclass of the Kuiper Belt known as the `scattered disk' is argued to be the dominant source of JFCs. However, the best…

天体物理学 · 物理学 2009-11-13 Kathryn Volk , Renu Malhotra

We explore the long-term evolution of a bias-free orbital representation of the cometary nuclei (with diameters above 2 km) of the Kuiper belt, using the so-called L7 synthetic model from CFEPS, which consists of three dynamical…

地球与行星天体物理 · 物理学 2019-10-23 Marco A. Muñoz-Gutiérrez , Antonio Peimbert , Bárbara Pichardo , Matthew J. Lehner , Shiang-Yu Wang

In an effort to understand the origin of the Main Belt Comets (MBCs) 7968 Elst-Pizzaro, 118401, and P/2005 U1, the dynamics of these three icy asteroids and a large number of hypothetical MBCs were studied. Results of extensive numerical…

地球与行星天体物理 · 物理学 2015-05-14 Nader Haghighipour

It has long been hypothesised that the Jupiter-family comets (JFCs) come from the scattered disc, an unstable planetesimal population beyond Neptune. This viewpoint has been widely accepted, but a few issues remain, the most prominent of…

地球与行星天体物理 · 物理学 2015-06-23 R. Brasser , J. -H. Wang

Jupiter family comets contribute a significant amount of debris to near-Earth space. However, telescopic observations of these objects seem to suggest they have short physical lifetimes. If this is true, the material generated will also be…

Themis family is one of the largest and oldest asteroid populations in the main-belt. Water-ice may widely exist on the parent body (24) Themis. In this work, we employ the Advanced Thermophysical Model as well as mid-infrared measurements…

地球与行星天体物理 · 物理学 2021-12-10 Haoxuan Jiang , Jianghui Ji

Centaurs--icy bodies orbiting beyond Jupiter and interior to Neptune--are believed to be dynamically related to Jupiter Family Comets (JFCs), which have aphelia near Jupiter's orbit and perihelia in the inner Solar System. Previous…

地球与行星天体物理 · 物理学 2019-10-23 Kevin R. Grazier , Jonathan Horner , Julie C. Castillo-Rogez

It was recently proposed that there exists a "gateway" in the orbital parameter space through which Centaurs transition to Jupiter-family Comets (JFCs). Further studies have implied that the majority of objects that eventually evolve into…

地球与行星天体物理 · 物理学 2023-01-25 Aurélie Guilbert-Lepoutre , Anastasios Gkotsinas , Sean N. Raymond , David Nesvorny

Jupiter-family comets (JFCs) are the evolutionary products of trans-Neptunian objects (TNOs) that evolve through the giant planet region as Centaurs and into the inner solar system. Through numerical orbital evolution calculations following…

地球与行星天体物理 · 物理学 2019-10-02 Gal Sarid , Kathryn Volk , Jordan Steckloff , Walter Harris , Maria Womack , Laura Woodney

We studied the orbital evolution of Jupiter-family comets (JFCs), Halley-type comets (HTCs), and long-period comets, and probabilities of their collisions with planets. In our runs the probability of a collision of one object with the Earth…

天体物理学 · 物理学 2010-12-01 S. I. Ipatov , J. C. Mather

Jupiter-family comets (JFCs) have orbital periods of less than 20 years and therefore undergo more frequent sublimation compared to other comet populations. The JFCs therefore represent the ideal dynamical population for investigating the…

地球与行星天体物理 · 物理学 2025-06-12 A. Fraser Gillan , Alan Fitzsimmons , Larry Denneau , Robert J. Siverd , Ken W. Smith , John L. Tonry , David R. Young

Rotational spin-up due to outgassing of comet nuclei has been identified as a possible mechanism for considerable mass-loss and splitting. We report a search for spin changes for three large Jupiter-family comets (JFCs): 14P/Wolf,…

地球与行星天体物理 · 物理学 2018-06-27 Rosita Kokotanekova , Colin Snodgrass , Pedro Lacerda , Simon F. Green , Plamen Nikolov , Tanyu Bonev

We estimate the total number and the slope of the size frequency distribution (SFD) of dormant Jupiter Family Comets (JFCs) by fitting a one-parameter model to the known population. We first select 61 Near Earth Objects (NEOs) that are…

天体物理学 · 物理学 2009-11-11 Kathryn Whitman , Alessandro Morbidelli , Robert Jedicke

From 1996 to 2015 sixteen main belt asteroids were discovered exhibiting cometary activity (less than one per year), all of them during searches at the telescope. In this work we will explore another way to discover them. We reduced 192016…

地球与行星天体物理 · 物理学 2017-03-30 I. Ferrin , M. Perez , J. Rendon

In this paper we apply different methods to examine the possibility that a small group of 24 asteroids dynamically linked to main-belt comet P/2006 VW139, recently discovered by the Pan-STARRS1 survey telescope, shares a common physical…

地球与行星天体物理 · 物理学 2012-07-17 Bojan Novakovic , Henry H. Hsieh , Alberto Cellino

We estimated the rate of comet and asteroid collisions with the terrestrial planets by calculating the orbits of 13000 Jupiter-crossing objects (JCOs) and 1300 resonant asteroids and computing the probabilities of collisions based on…

天体物理学 · 物理学 2007-05-23 S. I. Ipatov , J. C. Mather

We present a dynamical study of 39 active Centaurs and 17 high-perihelion (q$>$4.5 au) JFCs with a focus on investigating recent orbital changes as potential triggers for comet-like activity. We have identified a common feature in the…

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