activity
20142023
most citedPlanetesimal rings as the cause of the Solar System's planetary architecture

124 citations · 383 across the 8 of their papers we have counts for

collaborators

16 papers

astro-ph.EP2024

The Debiased Near-Earth Object Population from ATLAS Telescopes

Rogerio Deienno, Larry Denneau, David Nesvorný +7

This work is dedicated to debias the Near-Earth Objects (NEO) population based on observations from the Asteroid Terrestrial-impact Last Alert System (ATLAS) telescopes. We have ap…

astro-ph.EP2024

NEOMOD 3: The Debiased Size Distribution of Near Earth Objects

David Nesvorny, David Vokrouhlicky, Frank Shelly +9

Our previous model (NEOMOD2) for the orbital and absolute magnitude distribution of Near Earth Objects (NEOs) was calibrated on the Catalina Sky Survey observations between 2013 an…

astro-ph.EP20241 cited

Implantation of asteroids from the terrestrial planet region: The effect of the timing of the giant planet instability

Andre Izidoro, Rogerio Deienno, Sean N. Raymond +1

The dynamical architecture and compositional diversity of the asteroid belt strongly constrain planet formation models. Recent Solar System formation models have shown that the ast…

astro-ph.EP2024

The link between Athor and EL meteorites does not constrain the timing of the giant planet instability

Andre Izidoro, Rogerio Deienno, Sean N. Raymond +1

The asteroid Athor, residing today in the inner main asteroid belt, has been recently associated as the source of EL enstatite meteorites to Earth. It has been argued that Athor fo…

astro-ph.EP2024

Accretion and Uneven Depletion of the Main Asteroid Belt

Rogerio Deienno, David Nesvorny, Matthew S. Clement +3

The main asteroid belt (MAB) is known to be primarily composed of objects from two distinct taxonomic classes, generically defined here as S- and C-complex. The former probably ori…

astro-ph.EP2024

Orbital and absolute magnitude distribution of Jupiter Trojans

David Vokrouhlický, David Nesvorný, Miroslav Brož +4

Jupiter Trojans (JTs) librate about the Lagrangian stationary centers L4 and L5 associated with this planet on a typically small-eccentricity and moderate-inclination heliocentric…