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We present observations and models of the dust environment of activated asteroid P/2013 P5 (PANSTARRS). The object displayed a complex morphology during the observations, with the presence of multiple tails. We combined our own…

地球与行星天体物理 · 物理学 2015-06-18 F. Moreno. , J. Licandro , C. Álvarez-Iglesias , A. Cabrera-Lavers , F. Pozuelos

This is an overview of recent research on meteors and the parent bodies from which they are produced. While many meteor showers result from material ejected by comets, two out of the three strongest annual showers (the Geminids and the…

地球与行星天体物理 · 物理学 2022-09-21 Toshihiro Kasuga , David Jewitt

The aim of this study is to estimate the rotational characteristics of meteoroids after their release from a comet during normal activity. The results can serve as initial conditions for further analyses of subsequent evolution of rotation…

地球与行星天体物理 · 物理学 2015-06-19 David Capek

The recent close approach of the NEA (3200) Phaethon offered a rare opportunity to obtain high-quality observational data. We used the newly obtained optical light curves to improve the spin and shape model of Phaethon and to determine its…

We have performed detailed dynamical modeling of the structure of a faint dust band observed in coadded IRAS data at an ecliptic latitude of 17$^{\circ}$ that convincingly demonstrates that it is the result of a relatively recent…

地球与行星天体物理 · 物理学 2015-10-07 A. J. Espy Kehoe , T. J. J. Kehoe , J. E. Colwell , S. F. Dermott

We report new observations of the active asteroid P/2010 A2 taken when it made its closest approach to the Earth (1.06 au in 2017 January) after its first discovery in 2010. Despite a crucial role of the rotational period in clarifying its…

地球与行星天体物理 · 物理学 2017-06-28 Yoonyoung Kim , Masateru Ishiguro , Myung Gyoon Lee

[Abridged] Asteroid mining is not necessarily a distant prospect. Hayabusa2 and OSIRIS-REx have recently rendezvoused with near-Earth asteroids and will return samples to Earth. While there is significant science motivation for these…

地球与行星天体物理 · 物理学 2019-12-02 Logan Fladeland , Aaron C. Boley , Michael Byers

The under-abundance of asteroids on orbits with small perihelion distances suggests that thermally-driven disruption may be an important process in the removal of rocky bodies in the Solar System. Here we report our study of how the debris…

地球与行星天体物理 · 物理学 2019-03-20 Quanzhi Ye , Mikael Granvik

The $\sim$4 km diameter main belt asteroid 6478 Gault has ejected dust intermittently since at least 2013. The character of the emission, including its episodic nature and the low speed of the ejected particles ($V \sim $ 0.15 m s$^{-1}$),…

地球与行星天体物理 · 物理学 2021-04-14 J. X. Luu , D. C. Jewitt , M. Mutchler , J. Agarwal , Y. Kim , J. Li , H. Weaver

Based on telescopic observations of Jupiter-family comets (JFCs), there is predicted to be a paucity of objects at sub-kilometre sizes. However, several bright fireballs and some meteorites have been tenuously linked to the JFC population,…

By using an array of high-sensitivity CCD video devices and spectrographs, the activity of meteor events from the poorly-known $\rho$-Geminid meteoroid stream has been monitored during January 2012 and 2013. As a result of this research,…

地球与行星天体物理 · 物理学 2015-06-23 Jose M. Madiedo

Context. Rotational instability of rubble-pile asteroids can trigger mass shedding, forming transient debris clouds that may provide the initial conditions for secondary formation in binary systems. Aims. We investigate the dynamical and…

地球与行星天体物理 · 物理学 2025-12-16 Yutian Wu , Xiaojing Zhang , Chenyang Huang , Yang Yu

More than a half of asteroids in the main belt have irregular shapes with the ratios of the minor to major axis lengths less than 0.6. One of the mechanisms to create such shapes is collisions between asteroids. The relationship between…

地球与行星天体物理 · 物理学 2018-12-12 Keisuke Sugiura , Hiroshi Kobayashi , Shu-ichiro Inutsuka

The solar system is dusty, and would become dustier over time as asteroids collide and comets disintegrate, except that small debris particles in interplanetary space do not last long. They can be ejected from the solar system by Jupiter,…

地球与行星天体物理 · 物理学 2015-05-30 David Nesvorny , Diego Janches , David Vokrouhlicky , Petr Pokorny , William F. Bottke , Peter Jenniskens

The JAXA/ISAS spacecraft DESTINY$^+$ will be launched to the active asteroid (3200) Phaethon in 2022. Among the proposed core payload is the DESTINY+ Dust Analyzer (DDA) which is an upgrade of the Cosmic Dust Analyzer flown on the Cassini…

Material arriving at our solar system from the Galaxy may be detected at Earth in the form of meteors ablating in our atmosphere. Here we report on a search for interstellar meteors within the highest-quality events in the Global Meteor…

地球与行星天体物理 · 物理学 2025-03-26 Paul Wiegert , Vanessa Tran , Cole Gregg , Denis Vida , Peter Brown

We report an instrumental observation of the very exceptional Geminid fireball which was observed in scope of the Czech part of the European Fireball Network (EN) on 13 December 2012 at 4h12m59.4s UT. The uniqueness of this Geminid fireball…

地球与行星天体物理 · 物理学 2026-03-25 Pavel Spurný , Jiří Borovička

We present an analysis of asteroid (3200) Phaethon using coronagraphic observations from 2008 to 2022 by the COR2 cameras onboard the twin Solar TErrestrial RElations Observatory (STEREO) spacecraft. Although undetected in individual…

地球与行星天体物理 · 物理学 2023-02-15 Man-To Hui

Context. Dynamically linking a meteor shower with its parent body is challenging, and chaos in the dynamics of meteoroid streams may be one of the reasons. For a robust identification of parent bodies, it is therefore necessary to quantify…

地球与行星天体物理 · 物理学 2024-01-24 Ariane Courtot , Melaine Saillenfest , Jérémie Vaubaillon , Marc Fouchard

The Martian Moons Exploration (MMX) spacecraft is a JAXA mission to Mars and its moons Phobos and Deimos. MMX will carry the Circum-Martian Dust Monitor (CMDM) which is a newly developed light-weight ($\mathrm{650\,g}$) large area…