Identifying meteorite droppers among the population of bright 'sporadic'bolides imaged by the Spanish Meteor Network during the spring of 2022

E Peña-Asensio, JM Trigo-Rodríguez… - Monthly Notices of …, 2023 - academic.oup.com
The extraordinary weather conditions available between February and March 2022 over
Spain have allowed us to analyse the brightest fireballs recorded by the monitoring stations …

Small near-Earth asteroids as a source of meteorites

J Borovička, P Spurný, P Brown - Asteroids IV, 2015 - books.google.com
Small asteroids intersecting Earth's orbit can deliver extraterrestrial rocks to Earth, called
meteorites. This process is accompanied by a luminous phenomena in the atmosphere …

Near-Earth stream decoherence revisited: the limits of orbital similarity

PM Shober, A Courtot, J Vaubaillon - Astronomy & Astrophysics, 2025 - aanda.org
Context. Orbital similarity measures, such as the D values, have been extensively used in
meteor science to identify meteoroid streams and associate meteorite falls with near-Earth …

Influence of planetary encounters on the magnitude of the Yarkovsky effect in asteroid dynamics

AA Martyusheva, AV Melnikov - Solar System Research, 2023 - Springer
The influence of the solar radiation pressure and the Yarkovsky effect on the long-term
orbital dynamics is estimated for a number of asteroids experiencing successive planetary …

All-sky Meteor Orbit System AMOS and preliminary analysis of three unusual meteor showers

J Tóth, L Kornoš, P Zigo, Š Gajdoš, D Kalmančok… - Planetary and space …, 2015 - Elsevier
Abstract All-sky Meteor Orbit System (AMOS) is a semi-autonomous video observatory for
detection of transient events on the sky, mostly the meteors. Its hardware and software …

Asteroid 2013 ND15: Trojan companion to Venus, PHA to the Earth

C De la Fuente Marcos… - Monthly Notices of the …, 2014 - academic.oup.com
Venus has three known co-orbitals:(322756) 2001 CK32, 2002 VE68 and 2012 XE133. The
first two have absolute magnitudes 18< H< 21. The third one, significantly smaller at H= 23.4 …

Properties and evolution of NEO families created by tidal disruption at Earth

E Schunová, R Jedicke, KJ Walsh, M Granvik… - Icarus, 2014 - Elsevier
We have calculated the coherence and detectable lifetimes of synthetic near-Earth object
(NEO) families created by catastrophic disruption of a progenitor as it suffers a very close …

101955 Bennu and 162173 Ryugu: Dynamical modelling of ejected particles to the Earth

M Kováčová, R Nagy, L Kornoš, J Tóth - Planetary and Space Science, 2020 - Elsevier
Apollo-type asteroids Bennu and Ryugu are currently targets of sample-return missions. The
goal of OSIRIS-REx mission (NASA) is to explore asteroid Bennu and Ryugu is being …

The coupling orbit–attitude–structure evolution of rubble-pile asteroid with Earth flyby in the restricted three-body problem

X Zeng, C Feng, T Wen, Q Gan - Aerospace, 2022 - mdpi.com
Some asteroids flying close to Earth may pose a threat of impact. Among them, the structural
and dynamical characteristics of rubble-pile asteroids can be changed because of the tidal …

[HTML][HTML] Fragments of Late Eocene Earth-impacting asteroids linked to disturbance of asteroid belt

B Schmitz, S Boschi, A Cronholm, PR Heck… - Earth and Planetary …, 2015 - Elsevier
The onset of Earth's present icehouse climate in the Late Eocene coincides with
astronomical events of enigmatic causation. At∼ 36 Ma ago the 90–100 km large Popigai …