activity
20242026
most citedCatastrophic disruption of asteroid 2023 CX1 and implications for planetary defense

14 citations · 27 across the 11 of their papers we have counts for

collaborators

12 papers

astro-ph.EP2026

The Non-Principal-Axis Rotation and Convex Shape Model of Earth Quasi-Satellite and the Target of China's Tianwen-2 Mission (469219) Kamo`oalewa

Xiaoyu Sun, Zhijun Song, Hanjie Tan +8

(469219) Kamo`oalewa is the most stable Earth quasi-satellite and the target of China's Tianwen-2 asteroid sample return mission. Due to its small size, fast rotation, and the limi…

astro-ph.EP2026

Dynamic Trajectory Analysis of Meteoroids Showing Minimal Deceleration

Thomas Stevenson, Ellie Sansom, Hadrien Devillepoix +8

Meteoroids decelerate and ablate as they descend through the atmosphere, however a portion of instrumentally observed meteors show little measurable deceleration and remain poorly…

astro-ph.EP2026

Unmasking (44) Nysa: Evidence for a trilobate structure

Kate Minker, Anthony Berdeu, Gianluca Li Causi +16

Context. (44) Nysa is one of the largest known E-type asteroids. Light curve inversion models have indicated that it may have an elongated shape commonly found in large binary syst…

astro-ph.EP2026

A Machine Learning Approach to Meteor Classification

Samantha Hemmelgarn, Nicholas Moskovitz, Denis Vida

We use machine learning to develop a framework for classifying meteoroids based on 13 directly observed parameters from the Global Meteor Network. This method adds depth to the $K_…

astro-ph.EP2026

NEO Colors from The Mission Accessible Near-Earth Object Survey (MANOS)

Nicholas Moskovitz, Theodore Kareta, Samantha Hemmelgarn +13

We present spectro-photometric griz colors for 189 near-Earth objects (NEOs) collected by the Mission Accessible Near-Earth Object Survey (MANOS). Data acquisition involved non-sim…

astro-ph.EP2026★ 4 cited

Astrometric follow-up of near-Earth asteroid 2024 YR4 during a Torino scale level 3 alert

Marco Micheli, Maxime Devogèle, Larry Denneau +38

The discovery of 2024 YR4 presented the planetary defense community with the most significant impact threat in almost two decades, reaching level 3 on the Torino scale. The communi…

astro-ph.EP2025★ 3 cited

Rapid-response characterization of near-Earth asteroid 2024 YR4 during a Torino Scale 3 alert

Maxime Devogèle, Olivier R. Hainaut, Marco Micheli +32

On 27 December 2024, near-Earth object (NEO) 2024 YR was discovered by the ATLAS survey and identified as a virtual impactor. A few weeks later, it eventually reached level 3 o…

astro-ph.EP2025★ 14 cited

Catastrophic disruption of asteroid 2023 CX1 and implications for planetary defense

Auriane Egal, Denis Vida, François Colas +94

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 atmo…

astro-ph.EP2024

On The Lunar Origin of Near-Earth Asteroid 2024 PT5

Theodore Kareta, Oscar Fuentes-Muñoz, Nicholas Moskovitz +2

The Near-Earth Asteroid (NEA) 2024 PT5 is on an Earth-like orbit which remained in Earth's immediate vicinity for several months at the end of 2024. PT5's orbit is challenging to p…

astro-ph.EP2024★ 1 cited

Telescope-to-Fireball Characterization of Earth Impactor 2022 WJ1

Theodore Kareta, Denis Vida, Marco Micheli +10

Comparing how an asteroid appears in space to its ablation behavior during atmospheric passage and finally to the properties of associated meteorites represents the ultimate probe…

astro-ph.EP2024

How Meteor Showers Can Guide the Search for Long Period Comets

Samantha Hemmelgarn, Nicholas Moskovitz, Stuart Pilorz +1

With orbital periods longer than 200 years, most long-period comets (LPCs) remain undiscovered until they are in-bound towards perihelion. The comets that pass close to Earth's orb…

astro-ph.EP2024★ 5 cited

Properties of outer solar system pebbles during planetesimal formation from meteor observations

Peter Jenniskens, Paul R. Estrada, Stuart Pilorz +42

In the late stages of accretion leading up to the formation of planetesimals, particles grew to pebbles the size of 1-mm to tens of cm. That is the same size range that dominates t…