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The observed near-Earth asteroid population contains very few objects with small perihelion distances, say, q<=0.2 au. NEAs that currently have orbits with larger q might be hiding a past evolution during which they have approached closer…

地球与行星天体物理 · 物理学 2021-08-04 Athanasia Toliou , Mikael Granvik , Georgios Tsirvoulis

From Jan. 6, 2019 to Feb. 18, 2019, OSIRIS-REx observed asteroid (101955) Bennu ejecting 11 plumes of dust, of which part is escaping and another part is re-captured by the asteroid. The relative magnitudes of the typical forces acting on…

地球与行星天体物理 · 物理学 2020-10-21 Yu Jiang , Jürgen Schmidt

Aims. Based on measurements by the Ulysses spacecraft and high-resolution modelling of the motion of interstellar dust (ISD) through the heliosphere we predict the ISD flow in the inner planetary system and on to the Earth. This is the…

地球与行星天体物理 · 物理学 2019-01-09 Peter Strub , Veerle J. Sterken , Rachel Soja , Harald Krüger , Eberhard Grün , Ralf Srama

To deflect impact-trajectory of massive km^3 and spinning asteroid by a few terrestrial radius one need a large momentum exchange. The dragging of huge spinning bodies in space by external engine seems difficult or impossible. Our solution…

天体物理学 · 物理学 2008-03-11 D. Fargion

We analyze a sample of 139 near-Earth asteroids (NEAs), defined as those that reach perihelion distances $q < 1.3$ au, and that also fulfill the conditions of approaching or crossing Jupiter's orbit (aphelion distances $Q > 4.8$ au), having…

地球与行星天体物理 · 物理学 2014-05-08 Julio A. Fernández , Andrea Sosa , Tabaré Gallardo , Jorge N. Gutiérrez

In 2029, the near-Earth asteroid (99942) Apophis approaches the Earth within six Earth radii. This opportunity is one of the rarest natural experiments that we can use to better characterize a small body through telescopic observations and…

地球与行星天体物理 · 物理学 2025-07-24 Masatoshi Hirabayashi

Containing only a few percent the mass of the moon, the current asteroid belt is around three to four orders of magnitude smaller that its primordial mass inferred from disk models. Yet dynamical studies have shown that the asteroid belt…

地球与行星天体物理 · 物理学 2019-01-16 Matthew S. Clement , Sean N. Raymond , Nathan A. Kaib

Strange-looking dust cloud around asteroid (596) Scheila was discovered on 2010 December 11.44-11.47. Unlike normal cometary tails, it consisted of three tails and faded within two months. We constructed a model to reproduce the morphology…

The G-ring arc of Saturn, confined by the 7:6 corotation eccentric resonance with Mimas, is primarily composed of micrometric particles. These particles, significantly influenced by the solar radiation pressure, are subject to rapid…

地球与行星天体物理 · 物理学 2025-01-23 V. Lattari , R. Sfair , P. B. Siqueira , C. M. Schäfer

The irregular satellites of Jupiter produce dust particles through the impact of interplanetary micrometeoroids. In this paper, the dynamics of these particles is studied by both high-accuracy numerical simulation and analytical theory, in…

地球与行星天体物理 · 物理学 2024-02-07 Zhenghan Chen , Kun Yang , Xiaodong Liu

Context. The existence of meteor clusters has long since been a subject of speculation and so far only seven events have been reported, among which two involve less than five meteors, and three were seen during the Leonid storms. Aims. The…

Micrometeoroids (cosmic dust with size between a few $\mu$m and $\sim$1 mm) dominate the annual extraterrestrial mass flux to the Earth. We investigate the range of physical processes occurring when micrometeoroids traverse the atmosphere.…

地球与行星天体物理 · 物理学 2015-06-15 G. Briani , E. Pace , S. N. Shore , G. Pupillo , A. Passaro , S. Aiello

Aims. A new mechanism of dust accumulation and planetesimal formation in a gravitationally unstable disk with suppressed magnetorotational instability is studied and compared with the classical dead zone in a layered disk model. Methods. We…

地球与行星天体物理 · 物理学 2024-07-17 Eduard I. Vorobyov , Aleksandr M. Skliarevskii , Manuel Guedel , Tamara Molyarova

This paper presents an analysis of optimal impact strategies to deflect potentially dangerous asteroids. To compute the increase in the minimum orbit intersection distance of the asteroid due to an impact with a spacecraft, simple…

最优化与控制 · 数学 2011-05-02 Massimiliano Vasile , Camilla Colombo

We analyze lunar impact flashes recorded by our team during runs in December 2007, 2011, 2013 and 2014. In total, 12 impact flashes with magnitudes ranging between 7.1 and 9.3 in V band were identified. From these, 9 events could be linked…

地球与行星天体物理 · 物理学 2015-11-24 Jose L. Ortiz , Jose M. Madiedo , Nicolas Morales , Pablo Santos-Sanz , Francisco J. Aceituno

We develop a first-principles formalism, based on the transport equation in the line-of-sight approximation, to link the expected number of muons at neutrino telescopes to the flux of neutrinos at the Earth's surface. We compute the…

高能物理 - 唯象学 · 物理学 2025-08-01 Stefano Palmisano , Diego Redigolo , Michele Tammaro , Andrea Tesi

Meteor showers and their outbursts are the dominant source of meteoroid impact risk to spacecraft on short time scales. Meteor shower prediction models depend on historical observations to produce accurate forecasts. However, the current…

Potential microbial contamination of Martian moons, Phobos and Deimos, which can be brought about by transportation of Mars ejecta produced by meteoroid impacts on the Martian surface, has been comprehensively assessed in a statistical…

One of the most energetic bolide events in recent decades was detected by the US Government sensors (USGS) over remote areas of the Bering Sea on December 18, 2018, 23:48 UT. No ground-based optical observations exist. Using the satellite…

地球与行星天体物理 · 物理学 2021-01-04 J. Borovicka , M. Setvak , H. Roesli , J. K. Kerkmann

A new meteor shower $\lambda$-Sculptorids produced by the comet 46P/Wirtanen was forecast for December 12, 2023. The predicted activity was highly uncertain, but generally considered to be low. Observations in Australia, New Zealand, and…

地球与行星天体物理 · 物理学 2024-02-13 D. Vida , J. M. Scott , A. Egal , J. Vaubaillon , Q. -Z. Ye , D. Rollinson , M. Sato , D. E. Moser