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Related papers: Reconstructing the Chelyabinsk event: pre-impact o…

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There are several differences between the planetary entry of space vehicles and that of asteroids. In this work we do investigate the applicability of classical methods and approaches developed for debris analysis to asteroid entry. In…

Earth and Planetary Astrophysics · Physics 2013-04-10 Cristina Parigini , Juan Luis Cano , Rodrigo Haya-Ramos

We explored the statistical and compositional link between Chelyabinsk meteoroid and potentially hazardous asteroid (86039) 1999 NC43 to investigate their proposed relation proposed by Borovi\v{c}ka et al. (2013). Using detailed computation…

The Chelyabinsk meteorite is a highly shocked, low porosity, ordinary chondrite, probably similar to S- or Q-type asteroids. Therefore, nanoindentation experiments on this meteorite allow us to obtain key data to understand the physical…

This letter presents a new solution for the Tunguska event of June 30th, 1908. The solution has been obtained starting from seismic data, is in fair agreement with the observational evidence, and supports the asteroidal hypothesis for the…

Astrophysics · Physics 2007-05-23 Luigi Foschini

This paper describes briefly a mathematical model that relates the parameters of celestial bodies motion in the spheres of activity of the Sun and the Earth with mass-energy characteristics of these celestial bodies and their explosion…

Earth and Planetary Astrophysics · Physics 2014-04-01 Yu. I. Lobanovsky

The well-known Tunguska-1908 phenomenon (TP) problems (the fast transfer of the kinetic energy of the meteoroid W~10-50 Mt TNT to air, with its heating to T>10^4 K at an altitude of 5-10 km, the final turn of the smoothly sloping, ~0-20^o…

Earth and Planetary Astrophysics · Physics 2009-03-20 Edward M. Drobyshevski

Tunguska and Chelyabinsk impact events occurred inside a geographical area of only 3.4\% of the Earth's surface. Although two events hardly constitute a statistically significant demonstration of a geographical pattern of impacts, their…

Earth and Planetary Astrophysics · Physics 2018-05-16 Jorge I. Zuluaga , Mario Sucerquia

Earth is constantly being bombarded with material from space. Most of the natural material end up being dust grains that litter the surface of Earth, but larger bodies are known to impact every few decades. The most recent large impact was…

Instrumentation and Methods for Astrophysics · Physics 2019-09-05 Ravi teja Nallapu , Jekan Thangavelautham

When a space body enters Earth's atmosphere, its surface is exposed to high pressure and temperatures. The airflow tears off small droplets from the meteoroid forming a cloud of meteorite dust. Can new materials be synthesized in these…

Asteroid 2009 FD could impact Earth between 2185 and 2196. The long term propagation to the possible impacts and the intervening planetary encounters make 2009 FD one of the most challenging asteroids in terms of hazard assessment. To…

Earth and Planetary Astrophysics · Physics 2015-06-22 F. Spoto , A. Milani , D. Farnocchia , S. R. Chesley , M. Micheli , G. B. Valsecchi , D. Perna , O. Hainaut

The population of Earth-impacting meteoroids and its size-dependent orbital elements are key to understanding the origin of meteorites and informing on planetary defence efforts. Outstanding questions include the role of collisions in…

Apollo meteoroid 2018 LA has become only the third natural object ever to be discovered prior to causing a meteor airburst and just the second one to have its meteorites recovered (at Botswana's Central Kalahari Game Reserve). Here, we use…

Earth and Planetary Astrophysics · Physics 2018-07-30 C. de la Fuente Marcos , R. de la Fuente Marcos

Here we show an example of a young asteroid cluster located in a dynamically stable region, which was produced by partial disruption of a primitive body about 30 km in size. We estimate its age to be only 1.9 +/- 0.3 Myr, thus its…

Earth and Planetary Astrophysics · Physics 2012-07-10 Bojan Novakovic , Aldo Dell'Oro , Alberto Cellino , Zoran Knezevic

We have developed a statistical framework that uses collisional evolution models, shock physics modeling and scaling laws to determine the range of plausible collisional histories for individual meteorite parent bodies. It is likely that…

Earth and Planetary Astrophysics · Physics 2013-09-11 Thomas M Davison , David P O'Brien , Fred J Ciesla , Gareth S Collins

This monograph presents a study of the nature and origin of meteorites, asteroids and comets; and of the consequences of encounters of these cosmic objects with the Earth. The purpose of this monograph is mainly of divulgation for…

Earth and Planetary Astrophysics · Physics 2021-07-13 Carlos A. Olano

The collision history of asteroids is an important archive of inner Solar System evolution. Evidence for these collisions is brought to Earth by meteorites, which can preserve impact-reset radioisotope mineral ages. However, as meteorites…

Earth and Planetary Astrophysics · Physics 2022-01-28 Craig R. Walton , Oliver Shorttle , Sen Hu , Auriol S. P. Rae , Ji Jianglong , Ana Černok , Helen Williams , Yu Liu , Guoqiang Tang , Qiuli Li , Mahesh Anand

The article provides an open discussion and a critical feedback to the comments of Haack et al. (2015) and emphasizes a significance of the first macroscopic evidence for a candidate meteorite of a new type: planetary-origin meteorite…

Earth and Planetary Astrophysics · Physics 2016-09-23 Yana Anfinogenova , John Anfinogenov , Larisa Budaeva , Dmitry Kuznetsov

The potentially hazardous asteroid (101955) 1999 RQ36 has the possibility of collision with the Earth in the latter half of the 22nd century, well beyond the traditional 100-year time horizon for routine impact monitoring. The probabilities…

Earth and Planetary Astrophysics · Physics 2009-09-02 Andrea Milani , Steven R. Chesley , Maria Eugenia Sansaturio , Fabrizio Bernardi , Giovanni B. Valsecchi , Oscar Arratia

This paper presents the analysis of ionospheric effects in the region close to the Chelyabinsk meteorite explosion at 03:20UT 2013 February 15 from the Institute of Solar-Terrestrial Physics of Siberian Branch of Russian Academy of Sciences…

Shock-induced changes in ordinary chondrite meteorites related to impacts or planetary collisions are known to be capable of altering their optical properties. Thus, one can hypothesize that a significant portion of the ordinary chondrite…