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Mitigation of the threat from airbursting asteroids requires an understanding of the potential risk they pose for the ground. How asteroids release their kinetic energy in the atmosphere is not well understood due to the rarity of…

Earth and Planetary Astrophysics · Physics 2025-09-17 Auriane Egal , Denis Vida , François Colas , Brigitte Zanda , Sylvain Bouley , Asma Steinhausser , Pierre Vernazza , Ludovic Ferrière , Jérôme Gattacceca , Mirel Birlan , Jérémie Vaubaillon , Karl Antier , Simon Anghel , Josselin Desmars , Kévin Baillié , Lucie Maquet , Sébastien Bouquillon , Adrien Malgoyre , Simon Jeanne , Jiři Borovička , Pavel Spurný , Hadrien A. R. Devillepoix , Marco Micheli , Davide Farnocchia , Shantanu Naidu , Peter Brown , Paul Wiegert , Krisztián Sárneczky , András Pál , Nick Moskovitz , Theodore Kareta , Toni Santana-Ros , Alexis Le Pichon , Gilles Mazet-Roux , Julien Vergoz , Luke McFadden , Jelle Assink , Läslo Evers , Daniela Krietsch , Henner Busemann , Colin Maden , Lisa Maria Eckart , Jean-Alix Barrat , Pavel Povinec , Ivan Sykora , Ivan Kontul' , Oscar Marchhart , Martin Martschini , Silke Merchel , Alexander Wieser , Matthieu Gounelle , Sylvain Pont , Pierre Sans-Jofre , Sebastiaan de Vet , Ioannis Baziotis , Miroslav Brož , Michaël Marsset , Jérôme Vergne , Josef Hanuš , Maxime Devogèle , Luca Conversi , Francisco Ocaña , Luca Buzzi , Dan Alin Nedelcu , Adrian Sonka , Florent Losse , Philippe Dupouy , Korado Korlević , Dieter Husar , Jost Jahn , Damir Šegon , Mark McIntyre , Ralf Neubert , Pierre Beck , Patrick Shober , Anthony Lagain , Josep Maria Trigo-Rodriguez , Enrique Herrero , Jim Rowe , Andrew R. D. Smedley , Ashley King , Salma Sylla , Daniele Gardiol , Dario Barghini , Hervé Lamy , Emmanuel Jehin , Detlef Koschny , Bjorn Poppe , Andrés Jordán , Rene A. Mendez , Katherine Vieira , Hebe Cremades , Hasnaa Chennaoui Aoudjehane , Zouhair Benkhaldoun , Olivier Hernandez , Darrel Robertson , Peter Jenniskens

Imminent impactors are natural bodies discovered in space before impacting the Earth. They provide a rare opportunity to characterize individual near-Earth objects (NEOs) in great detail as asteroids in space, meteors in Earth's atmosphere…

Earth and Planetary Astrophysics · Physics 2026-04-09 Ian Chow , Mario Jurić , R. Lynne Jones , Kathleen Kiker , Joachim Moeyens , Peter G. Brown , Aren N. Heinze , Jacob A. Kurlander

We present a new space mission concept that is capable of finding, detecting, and tracking 90% of near-Earth objects (NEO) with H magnitude of $\rm H\leq22$ (i.e., $\sim$140 m in size) that are potentially hazardous to the Earth. The new…

Instrumentation and Methods for Astrophysics · Physics 2017-07-24 Michael Shao , Slava G. Turyshev , Sara Spangelo , Thomas Werne , Chengxing Zhai

Numerous decameter-sized asteroids have been observed impacting Earth as fireballs. These objects can have impact energies equivalent to hundreds of kilotons of TNT, posing a hazard if they impact populated areas. Previous estimates of…

Earth and Planetary Astrophysics · Physics 2025-01-08 Ian Chow , Peter G. Brown

We estimated the rate of comet and asteroid collisions with the terrestrial planets by calculating the orbits of 13000 Jupiter-crossing objects (JCOs) and 1300 resonant asteroids and computing the probabilities of collisions based on…

Astrophysics · Physics 2010-12-01 S. I. Ipatov , J. C. Mather

We present a practical and effective method of planetary defense that allows for extremely short mitigation time scales if required as well as long time scale mitigation. This one system allows for virtually any required defense mode. In…

Earth and Planetary Astrophysics · Physics 2025-06-27 Philip Lubin

We consider synchronized trains of sub-picosecond pulses generated by mode-locked lasers applied to deflection of near Earth objects (NEO) on collision course with Earth. Our method is designed to avoid a predicted collision of the NEO with…

Space Physics · Physics 2013-09-13 Richard Fork , Spencer Cole , Luke Burgess , Grant Bergstue

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…

Earth and Planetary Astrophysics · Physics 2021-08-04 Athanasia Toliou , Mikael Granvik , Georgios Tsirvoulis

Determining the size and orbital distribution of the population of near-Earth asteroids (NEAs) is the focus of intense research, with the most recent models converging to a population of approximately $1000$ NEAs larger than 1 km and up to…

Earth and Planetary Astrophysics · Physics 2016-12-21 Pasquale Tricarico

The number of known Near Earth Asteroids (NEAs) and Potentially Hazardous Asteroids (PHAs) has continued to grow in the last decade. Follow-up and recovery of newly discovered objects, as well as new astrometry at second or third…

Astrophysics · Physics 2007-05-23 Ovidiu Vaduvescu , Mirel Birlan

We study the time evolution of the impact probability for synthetic but realistic impacting and close approaching asteroids detected in a simulated all-sky survey. We use the impact probability to calculate the impact warning time as the…

Earth and Planetary Astrophysics · Physics 2015-08-26 Peter Vereš , Davide Farnocchia , Robert Jedicke , Federica Spoto

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…

Summary: In the past decade both scientists and laymen have probably heard at least once through the newspapers, TV and Internet that a new asteroid has been discovered with non-zero (sometimes "high") probability of collision with the…

Space Physics · Physics 2013-04-29 Germano D'Abramo

Among the currently known Near Earth Objects (NEOs), roughly 1400 are classified as being potentially hazardous asteroids. The recent Chelyabinsk event has shown that these objects can pose a real threat to mankind. We illustrate that high…

Instrumentation and Methods for Astrophysics · Physics 2013-11-19 Siegfried Eggl , Anatoliy Ivantsov , Daniel Hestroffer , Davide Perna , David Bancelin , William Thuillot

Recent observations of asteroidal surfaces indicate the presence of materials that do not match the bulk lithology of the body. A possible explanation for the presence of these exogenous materials is that they are products of inter-asteroid…

Earth and Planetary Astrophysics · Physics 2016-01-27 C. Avdellidou , M. C. Price , M. Delbo , P. Ioannidis , M. J. Cole

We integrated the orbital evolution of 30,000 Jupiter-family comets, 1300 resonant asteroids, and 7000 asteroidal, trans-Neptunian, and cometary dust particles. For initial orbital elements of bodies close to those of Comets 2P, 10P, 44P,…

Astrophysics · Physics 2010-11-29 S. I. Ipatov , J. C. Mather

Dynamical models of the asteroid delivery from the main belt suggest that the current impact flux of diameter D>10 km asteroids on the Earth is 0.5-1 per Gyr. Studies of the Near-Earth Asteroid (NEA) population find a much higher flux, with…

Earth and Planetary Astrophysics · Physics 2018-01-10 D. Nesvorny , F. Roig

Given a primary interest in "mitigation of the potential hazard" of near-Earth objects impacting the Earth, the subject of characterization takes on an aspect not normally present when considering asteroids as abstract bodies. Many…

Space Physics · Physics 2007-05-23 Russell Schweickart , Clark Chapman , Dan Durda , Bill Bottke , David Nesvorny , Piet Hut

Asteroid discoveries are essential for planetary-defense efforts aiming to prevent impacts with Earth, including the more frequent megaton explosions from decameter impactors. While large asteroids ($\geq$100 km) have remained in the main…

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