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相关论文: Destruction of Long-Period Comets

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As an Oort Cloud object with a record small perihelion distance of 2.7 Rsun and discovered more than a year before its encounter with the Sun, comet C/2012 S1 is a subject of considerable scientific interest. Its activity along the orbit's…

地球与行星天体物理 · 物理学 2015-06-04 Zdenek Sekanina , Rainer Kracht

We introduce a new technique to estimate the comet nuclear size frequency distribution (SFD) that combines a cometary activity model with a survey simulation and apply it to 150 long period comets (LPC) detected by the Pan-STARRS1…

The third macroscopic interstellar object detected in the solar system recently passed through perihelion, with the best-fitting models of its trajectory now featuring non-gravitational accelerations. We assess how much mass loss is…

地球与行星天体物理 · 物理学 2025-12-23 John C. Forbes , Harvey Butler

Context: Increasingly, Oort Cloud comets are being discovered at great distances from the Sun and tracked over ever wider ranges of heliocentric distances as observational equipment improves. Aims: To investigate in detail how the original…

地球与行星天体物理 · 物理学 2023-10-18 Małgorzata Królikowska , Luke Dones

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

A numerical simulation of the Oort cloud is used to explain the observed orbital distributions and numbers of Jupiter-family and Halley-type short-period comets. Comets are given initial orbits with perihelion distances between 5 and 36 AU,…

地球与行星天体物理 · 物理学 2014-02-07 V. V. Emel'yanenko , D. J. Asher , M. E. Bailey

Comet 73P/Schwassmann-Wachmann 3 has been observed to fragment on several occasions, yet the cause of its fragmentation remains poorly understood. We use previously unpublished archival Hubble Space Telescope data taken in 2006 to study the…

地球与行星天体物理 · 物理学 2019-09-04 Ariel Graykowski , David Jewitt

Near-Sun Comet C/2019 Y4 (ATLAS) is the first member of a long-period comet group observed to disintegrate well before perihelion. Here we present our investigation into this disintegration event using images obtained in a 3-day {\it Hubble…

Comet disintegration proceeds both through sublimation and discrete splitting events. The cross-sectional area of material ejected by a comet may, within days, become many times greater than that of the Earth, making encounters with such…

地球与行星天体物理 · 物理学 2020-04-07 W. M. Napier

On 2013 November 28 Comet ISON (C/2012 S1) will pass by the Sun with a perihelion distance of 2.7 solar radii. Understanding the possible outcomes for the comet's response to such a close passage by the Sun is important for planning…

地球与行星天体物理 · 物理学 2015-06-17 Matthew M. Knight , Kevin J. Walsh

So-called 'dark comets' are small, morphologically inactive near-Earth objects (NEOs) that exhibit nongravitational accelerations inconsistent with radiative effects. These objects exhibit short rotational periods (minutes to hours), where…

We show that if comets (or any small icy planetesimals such as Kuiper belt objects) are composed of pebble piles, their internal radiogenic as well as geochemical heating results in considerably different evolutionary outcomes compared to…

地球与行星天体物理 · 物理学 2022-06-03 Uri Malamud , Wolf A. Landeck , Dorothea Bischoff , Christopher Kreuzig , Hagai B. Perets , Bastian Gundlach , Jurgen Blum

We investigated three comets, which are active at large heliocentric distances, using observations obtained at the 6-m BTA telescope (SAO RAS, Russia) in the photometric mode of the focal reducer SCORPIO. The three comets,…

地球与行星天体物理 · 物理学 2021-02-10 Oleksandra Ivanova , Yury Skorov , Pavlo Korsun , Viktor Afanasiev , Jürgen Blum

Cometary outgassing can produce torques that change the spin state of the nucleus, influencing the evolution and lifetimes of comets (1,2). If these torques spin up the rotation to the point that centripetal forces exceed the material…

地球与行星天体物理 · 物理学 2018-01-12 Dennis Bodewits , Tony L. Farnham , Michael S. P. Kelley , Matthew M. Knight

Remote investigations of the ancient solar system matter has been traditionally carried out through the observations of long-period (LP) comets that are less affected by solar irradiation than the short-period counterparts orbiting much…

地球与行星天体物理 · 物理学 2016-12-14 K. Sarneczky , Gy. M. Szabo , B. Csak , J. Kelemen , G. Marschalko , A. Pal , R. Szakats , T. Szalai , E. Szegedi-Elek , P. Szekely , K. Vida , J. Vinko , L. L. Kiss

Some asteroids eject dust, unexpectedly producing transient, comet-like comae and tails. First ascribed to the sublimation of near-surface water ice, mass losing asteroids (also called "main-belt comets") can in fact be driven by a…

地球与行星天体物理 · 物理学 2015-06-03 Dave Jewitt

Dynamics of a complete sample of 22 small perihelion distance near-parabolic comets discovered in the years 2006 - 2010 is studied. First, osculating orbits are obtained after a careful positional data inspection and processing, including…

地球与行星天体物理 · 物理学 2015-06-16 Malgorzata Krolikowska , Piotr A. Dybczynski

We examine the rise and sudden demise of comet C/2010 X1 (Elenin) on its approach to perihelion. Discovered inbound at 4.2 AU, this long-period comet was predicted to become very bright when near perihelion, at 0.48 AU on 2011 September 10.…

地球与行星天体物理 · 物理学 2015-06-24 Jing Li , David Jewitt

We present results from a wide-field imaging campaign at the Canada-France-Hawaii Telescope to study the spectacular outburst of comet 17P/Holmes in late 2007. Using image-processing techniques we probe inside the spherical dust coma and…

地球与行星天体物理 · 物理学 2015-05-18 Rachel Stevenson , Jan Kleyna , David Jewitt

We analyse the population of near-Earth Long-Period Comets (LPCs) (perihelion distances q < 1.3 AU and orbital periods P > 10^3 yr). We have considered the sample of LPCs discovered during the period 1900-2009 and their estimated absolute…

地球与行星天体物理 · 物理学 2015-06-04 Julio A. Fernández , Andrea Sosa