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相关论文: The Persistent Activity of Jupiter-Family Comets a…

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We performed a monitoring observation of a Jupiter-Family comet, 17P/Holmes, during its 2014 perihelion passage to investigate its secular change in activity. The comet has drawn the attention of astronomers since its historic outburst in…

Jupiter-family Comets (JFCs) exhibit a wide range of activity levels and mass-loss over their orbits. We analyzed high-cadence observations of 42 active JFCs with the wide-field Asteroid Terrestrial-impact Last Alert System (ATLAS) survey…

地球与行星天体物理 · 物理学 2023-12-13 A. Fraser Gillan , Alan Fitzsimmons , Larry Denneau , Robert J. Siverd , Ken W. Smith , John L. Tonry , David R. Young

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

Aims. In this work, we present an extended study of the dust environment of a sample of short period comets and their dynamical history. With this aim, we characterized the dust tails when the comets are active, and we made a statistical…

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

We review the composition of Jupiter-family comet dust as inferred from infrared spectroscopy. We find that Jupiter-family comets have 10 micron silicate emission features with fluxes roughly 20-25% over the dust continuum (emission…

天体物理学 · 物理学 2015-05-13 Michael S. Kelley , Diane H. Wooden

Periodic comets of different dynamical groups with orbits at 2 - 5 AU still occasionally active. The observed dust activity of such objects can be connected with processes of water ice sublimation (MBCs) or crystallization of amorphous…

地球与行星天体物理 · 物理学 2020-05-18 E. Musiichuk , S. Borysenko

We observed 34 comets using the 24 micron camera on the Spitzer Space Telescope. Each image contains the nucleus and covers at least 10^6 km of each comet's orbit. Debris trails due to mm-sized or larger particles were found along the…

天体物理学 · 物理学 2024-10-31 William T. Reach , Michael S. Kelley , Mark V. Sykes

Jupiter co-orbital comets have orbits that are not long-term stable. They may experience flybys with Jupiter close enough to trigger tidal disruptions like the one suffered by comet Shoemaker-Levy 9. Our aim was to study the activity and…

Jupiter-family comet (JFC) P/2021 HS (PANSTARRS) only exhibits a coma within a few weeks of its perihelion passage at 0.8~au, which is atypical for a comet. Here we present an investigation into the underlying cause using serendipitous…

Comet 7P/Pons-Winnecke was observed from the Calar Alto Observatory (Spain) for four months during the 2021 inbound apparition. Broad-band visible images were taken between 1.71 and 1.25 AU pre-perihelion, while long-slit spectrophotometric…

地球与行星天体物理 · 物理学 2025-03-18 Irene Mariblanca-Escalona , Luisa M. Lara , Fernando Moreno , Pedro J. Gutiérrez , Marçal Evangelista-Santana

Current wide-field surveys discover ~15 Jupiter-family comets (JFCs) each year, typically identified via visual detection of a dust coma or tail. The same surveys also discover many asteroids that have distant JFC-like orbits, but with no…

地球与行星天体物理 · 物理学 2025-12-15 A. Fraser Gillan , Alan Fitzsimmons , Colin Orion Chandler , Colin Snodgrass , Joseph Murtagh

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…

Through photometry and spectroscopy, we studied the evolution of the activity and chemical composition of comet 67P during its 2025 and 2021 perihelion passages and of comet 103P during its 2010 and 2023 passages. For each comet, we aim to…

地球与行星天体物理 · 物理学 2026-05-07 E. Hemmen , M. Vander Donckt , E. Jehin , S. Hmiddouch , K. Aravind , J. Manfroid , Z. Benkhaldoun , A. Jabiri , S. Ganesh

As comets journey into the inner solar system, they deliver particulates and volatile gases into their comae that reveal the most primitive materials in the solar system. Cometary dust particles provide crucial information for assessing the…

地球与行星天体物理 · 物理学 2023-09-28 David E. Harker , Diane H. Wooden , Michael S. P. Kelley , Charles E. Woodward

We report new lightcurves and phase functions for nine Jupiter-family comets (JFCs). They were observed in the period 2004-2015 with various ground telescopes as part of the Survey of Ensemble Physical Properties of Cometary Nuclei…

地球与行星天体物理 · 物理学 2017-08-23 R. Kokotanekova , C. Snodgrass , P. Lacerda , S. F. Green , S. C. Lowry , Y. R. Fernandez , C. Tubiana , A. Fitzsimmons , H. H. Hsieh

Radio observations from decimetric to submillimetric wavelengths are now a basic tool for the investigation of comets. Spectroscopic observations allow us i) to monitor the gas production rate of the comets, by directly observing the water…

天体物理学 · 物理学 2015-05-13 J. Crovisier , N. Biver , D. Bockelée-Morvan , P. Colom

We present results from SEPPCoN, an on-going Survey of the Ensemble Physical Properties of Cometary Nuclei. In this report we discuss mid-infrared measurements of the thermal emission from 89 nuclei of Jupiter-family comets (JFCs). All data…

We report the discovery of recurrent activity on quasi-Hilda comet (QHC) 362P/(457175) 2008 GO98. The first activity epoch was discovered during the perihelion passage of 362P. The first activity epoch was discovered during the perihelion…

Photometric and spectroscopic observations of five nearly parabolic comets with eccentricity larger than 0.99 at heliocentric distances greater than 4 AU were performed. No molecular emission was observed for any studied comet and the…

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