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This paper presents a robust linear method for impact probability estimation of near-Earth asteroids with the Earth. This method is a significantly modified and improved method, which uses a special curvilinear coordinate system associated…

地球与行星天体物理 · 物理学 2020-01-08 Dmitrii E. Vavilov

(99942) Apophis is a potentially hazardous asteroid that will closely approach the Earth on April 13, 2029. Although the likelihood of an impact has been ruled out, this close encounter represents a unique opportunity for planetary science…

地球与行星天体物理 · 物理学 2023-09-04 Andrea C. Morelli , Alessandra Mannocchi , Carmine Giordano , Fabio Ferrari , Francesco Topputo

Asteroid (99942) Apophis' close approach in 2029 will be one of the most significant small-body encounter events in the near future and offers a good opportunity for in situ exploration to determine the asteroid's surface properties and…

地球与行星天体物理 · 物理学 2014-08-04 Yang Yu , Derek C. Richardson , Patrick Michel , Stephen R. Schwartz , Ronald-Louis Ballouz

An asteroid impact is a low probability event with potentially devastating consequences. The Asteroid Risk Mitigation Optimization and Research (ARMOR) software tool calculates whether a colliding asteroid experiences an airburst or surface…

空间物理 · 物理学 2017-02-21 Clemens M. Rumpf , Hugh G. Lewis , Peter M. Atkinson

Asteroid 99942 Apophis will pass near the Earth in April 2029. Expected to miss our planet by a safe margin, that could change if Apophis' path was perturbed by a collision with another asteroid in the interim. Though the statistical chance…

地球与行星天体物理 · 物理学 2024-03-04 Paul Wiegert , Ben Hyatt

In this work, we investigate the surface thermophysical properties (thermal emissivity, thermal inertia, roughness fraction and geometric albedo) of asteroid (99942) Apophis, using the currently available thermal infrared observations of…

地球与行星天体物理 · 物理学 2017-09-20 LiangLiang Yu , Jianghui Ji , Wing-Huen Ip

The potentially hazardous asteroid (PHA) (99942) Apophis is one of the most remarkable near-Earth asteroids (NEA) in terms of impact hazard. A good determination of its surface thermal inertia is very important in order to evaluate the…

地球与行星天体物理 · 物理学 2016-08-07 J. Licandro , T. Müller , C. Alvarez , V. Alí-Lagoa , M. Delbò

Asteroids can be eclipsed by other bodies in the Solar System, but no direct observation of an asteroid eclipse has been reported to date. We describe a statistical method to predict an eclipse for an asteroid based on the analysis of the…

天体物理学 · 物理学 2007-05-23 P. Tricarico , N. C. Hearn , G. Lake , G. Worthey

Asteroids that could collide with the Earth are listed on the publicly available Near-Earth object (NEO) hazard web sites maintained by the US and European space agencies (NASA and ESA). The impact probability distribution of 69 potentially…

地球与行星天体物理 · 物理学 2017-02-21 Clemens Rumpf , Hugh G. Lewis , Peter M. Atkinson

We present an updated set of near-Earth asteroids with a Yarkovsky-related semimajor axis drift detected from the orbital fit to the astrometry. We find 87 reliable detections after filtering for the signal-to-noise ratio of the Yarkovsky…

地球与行星天体物理 · 物理学 2018-09-19 Alessio Del Vigna , Laura Faggioli , Andrea Milani , Federica Spoto , Davide Farnocchia , Benoit Carry

The asteroid belt is a unique source of information on some of the most important questions facing solar system science. These questions include the sizes, numbers, types and orbital distributions of the planetesimals that formed the…

地球与行星天体物理 · 物理学 2024-11-20 Stanley F. Dermott , Dan Li , Apostolos A. Christou

The majority of existing probabilistic model checking case studies are based on well understood theoretical models and distributions. However, real-life probabilistic systems usually involve distribution parameters whose values are obtained…

软件工程 · 计算机科学 2013-08-29 Guoxin Su , David S. Rosenblum

Potentially impacting asteroids were analysed for their impact risk on the Earth. To this end, the Asteroid Risk Mitigation Optimization and Research (ARMOR) tool is currently being developed. The tool's modules are described and their…

空间物理 · 物理学 2015-02-23 Clemens Rumpf

Orbit-determination programs find the orbit solution that best fits a set of observations by minimizing the RMS of the residuals of the fit. For near-Earth asteroids, the uncertainty of the orbit solution may be compatible with trajectories…

地球与行星天体物理 · 物理学 2021-08-09 Javier Roa , Davide Farnocchia , Steven R. Chesley

On April 13, 2029, near-Earth asteroid (NEA) (99942) Apophis will pass at a distance of 6 Earth radii from Earth. This event will provide researchers with a unique opportunity to study the effects of tidal forces experienced by an asteroid…

Hazardous asteroid has been one of the concerns for humankind as fallen asteroid on earth could cost a huge impact on the society.Monitoring these objects could help predict future impact events, but such efforts are hindered by the large…

地球与行星天体物理 · 物理学 2024-09-05 Thai Duy Quy , Alvin Buana , Josh Lee , Rakha Asyrofi

We seek evidence of the Yarkovsky effect among Near Earth Asteroids (NEAs) by measuring the Yarkovsky-related orbital drift from the orbital fit. To prevent the occurrence of unreliable detections we employ a high precision dynamical model,…

地球与行星天体物理 · 物理学 2015-06-12 D. Farnocchia , S. R. Chesley , D. Vokrouhlicky , A. Milani , F. Spoto

This paper develops a measure-theoretic framework establishing when and how a possibilistic representation of incomplete knowledge contracts into a probabilistic representation of intrinsic stochastic variability. Epistemic uncertainty is…

人工智能 · 计算机科学 2026-04-14 Moriba Kemessia Jah

On April 13, 2029, the asteroid Apophis will pass near Earth at a geocentric distance of about 38,000 km. Numerical models have suggested that the post-encounter spin state will critically depend on the orientation of Apophis during the…

Epistemic uncertainty in probabilistic seismic hazard assessment (PSHA) is commonly addressed through a logic-tree framework that combines weighted alternative models to characterize the range of plausible hazard outcomes. Implicit in this…

地球物理 · 物理学 2026-03-03 Davide Zaccagnino , Didier Sornette