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相关论文: Constraints on Comet 332P/Ikeya-Murakami

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During 2006 Mar - 2007 Jan, we used the IRAC and MIPS instruments on the Spitzer Space Telescope to study the infrared emission from the ensemble of fragments, meteoroids, and dust tails in the more than 3 degree wide…

地球与行星天体物理 · 物理学 2015-05-13 William T. Reach , Jeremie Vaubaillon , Michael S. Kelley , Carey M. Lisse , Mark V. Sykes

We investigated the physical properties of the comet-like objects 107P/(4015) Wilson--Harrington (4015WH) and P/2006 HR30 (Siding Spring; HR30) by applying a simple thermophysical model (TPM) to the near-infrared spectroscopy and broadband…

地球与行星天体物理 · 物理学 2024-01-15 Yoonsoo P. Bach , Masateru Ishiguro , Fumihiko Usui

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

This paper presents the past evolution of the orbital elements of comet 67P/Churyumov-Gerasimenko, target of the Rosetta spacecraft. The gravitational orbit of the comet is affected by the sublimation of ice from the nucleus that triggers…

地球与行星天体物理 · 物理学 2015-07-01 Lucie Maquet

Multiple outbursts of a Jupiter-family comet, 15P/Finlay, occurred from late 2014 to early 2015. We conducted an observation of the comet after the first outburst and subsequently witnessed another outburst on 2015 January 15.6-15.7. The…

We report results based on mid-infrared photometry of comet 103P/Hartley 2 taken during May 4-13, 2010 (when the comet was at a heliocentric distance of 2.3 AU, and an observer distance of 2.0 AU) by the Wide-field Infrared Survey Explorer…

The Rosetta spacecraft observations revealed that the nucleus of comet 67P/Churyumov-Gerasimenko consists of two similarly sized lobes connected by a narrow neck. Here we evaluate the possibility that 67P is a collapsed binary. We assume…

地球与行星天体物理 · 物理学 2018-06-06 David Nesvorny , Joel Parker , David Vokrouhlicky

The CN coma structure of the EPOXI mission target, comet 103P/Hartley 2, was observed during twenty nights from September to December 2010. These CN images probe the rotational state of the comet's nucleus and provide a ground-based…

地球与行星天体物理 · 物理学 2015-05-28 Nalin H. Samarasinha , Beatrice E. A. Mueller , Michael F. A'Hearn , Tony L. Farnham , Alan Gersch

Two papers recently reported the detection of gaseous nickel and iron in the comae of over 20 comets from observations collected over two decades, including interstellar comet 2I/Borisov. To evaluate the state of the laboratory data in…

地球与行星天体物理 · 物理学 2021-10-13 Steven Bromley , Brynna Neff , Stuart Loch , Joan Marler , Juraj Országh , Kumar Venkataramani , Dennis Bodewits

Anisotropic outgassing from comets exerts a torque sufficient to rapidly change the angular momentum of the nucleus, potentially leading to rotational instability. Here, we use empirical measures of spin changes in a sample of comets to…

地球与行星天体物理 · 物理学 2021-05-19 David Jewitt

We present a sensitive 3-sigma upper limit of 1.1% for the HNC/HCN abundance ratio in comet 73P/Schwassmann-Wachmann (Fragment B), obtained on May 10-11, 2006 using Caltech Submillimeter Observatory (CSO). This limit is a factor of ~7 lower…

天体物理学 · 物理学 2009-11-13 D. C. Lis , D. Bockelee-Morvan , J. Boissier , J. Crovisier , N. Biver , S. B. Charnley

Cometary activity is a manifestation of sublimation-driven processes at the surface of nuclei. However, cometary outbursts may arise from other processes that are not necessarily driven by volatiles. In order to fully understand nuclear…

We present an analysis of new and published data on P/2013 R3, the first asteroid detected while disintegrating. Thirteen discrete components are measured in the interval between UT 2013 October 01 and 2014 February 13. We determine a mean,…

地球与行星天体物理 · 物理学 2017-05-03 Dave Jewitt , Jessica Agarwal , Jing Li , Harold Weaver , Max Mutchler , Stephen Larson

Methods. We algorithmically tracked thousands of individual particles through four OSIRIS/NAC image sequences of 67P's near-nucleus coma. We then traced concentrated particle groups back to the nucleus surface, and estimated their potential…

地球与行星天体物理 · 物理学 2024-05-22 Marius Pfeifer , Jessica Agarwal , Raphael Marschall , Björn Grieger , Pablo Lemos

Comet 41P/Tuttle-Giacobini-Kresak (41P), a Jupiter family comet with three discoveries over about 100 years, is in a short-periodic orbit around the Sun with the perihelion close to the Earth distance. The 2017 apparition of 41P offered a…

地球与行星天体物理 · 物理学 2020-07-01 Hermann Boehnhardt , Arno Riffeser , Christoph Ries , Michael Schmidt , Ulrich Hopp

The first direct detection of the asteroidal YORP effect, a phenomenon that changes the spin states of small bodies due to thermal reemission of sunlight from their surfaces, was obtained for (54509) YORP 2000 PH5. Such an alteration can…

地球与行星天体物理 · 物理学 2017-11-16 C. de la Fuente Marcos , R. de la Fuente Marcos

We identify a sample of 27 long-period comets for which both non-gravitational accelerations and Lyman-alpha based gas production rates are available. Seven of the 27 comets (i.e. 25 percent) did not survive perihelion because of nucleus…

地球与行星天体物理 · 物理学 2022-10-05 David Jewitt

The near-Earth asteroid (196256) 2003 EH1 has been suggested to have a dynamical association with the Quadrantid meteoroid stream. We present photometric observations taken to investigate the physical character of this body and to explore…

地球与行星天体物理 · 物理学 2015-10-28 Toshihiro Kasuga , David Jewitt

We analyze a sample of 73 old long-period comets (LPCs) (orbital periods $200 < P < 1000$ yr) with perihelion distances $q < 2.5$ au, discovered in the period 1850-2014. We cloned the observed comets and also added fictitious LPCs with…

地球与行星天体物理 · 物理学 2016-07-27 Julio A. Fernández , Tabaré Gallardo , Juan D. Young

Spectropolarimetry is a powerful technique for investigating the physical properties of gas and solid materials in cometary comae without mutual contamination, but there have been few spectropolarimetric studies to extract each component.…