activity
20082021
most citedIdentification and Dynamical Properties of Asteroid Families

177 citations · 1.3k across the 38 of their papers we have counts for

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Showing 2016Show all

7 papers · 1 filter

astro-ph.EP2016★ 25 cited

Hektor - an exceptional D-type family among Jovian Trojans

Jakub Rozehnal, Miroslav Brož, David Nesvorný +4

In this work, we analyze Jovian Trojans in the space of suitable resonant elements and we identify clusters of possible collisional origin by two independent methods: the hierarchi…

astro-ph.EP2016★ 127 cited

Dynamical Evidence for a Late Formation of Saturn's Moons

Matija Ćuk, Luke Dones, David Nesvorný

We explore the past evolution of Saturn's moons using direct numerical integrations. We find that the past Tethys-Dione 3:2 orbital resonance predicted in standard models likely di…

astro-ph.EP2016★ 30 cited

Jumping Jupiter can explain Mercury's orbit

Fernando Roig, David Nesvorný, Sandro Ricardo DeSouza

The orbit of Mercury has large values of eccentricity and inclination that cannot be easily explained if this planet formed on a circular and coplanar orbit. Here, we study the evo…

astro-ph.EP2016★ 21 cited

On the oldest asteroid families in the main belt

V. Carruba, D. Nesvorný, S. Aljbaae +2

Asteroid families are groups of minor bodies produced by high-velocity collisions. After the initial dispersions of the parent bodies fragments, their orbits evolve because of seve…

astro-ph.EP2016★ 21 cited

Footprints of a possible Ceres asteroid paleo-family

V. Carruba, D. Nesvorný, S. Marchi +1

Ceres is the largest and most massive body in the asteroid main belt. Observational data from the Dawn spacecraft reveal the presence of at least two impact craters about 280~km in…

astro-ph.EP2016★ 17 cited

Characterizing the original ejection velocity field of the Koronis family

Valerio Carruba, David Nesvorný, Safwan Aljbaae

An asteroid family forms as a result of a collision between an impactor and a parent body. The fragments with ejection speeds higher than the escape velocity from the parent body c…

astro-ph.EP2016★ 43 cited

Constraints on the original ejection velocity fields of asteroid families

Valerio Carruba, David Nesvorný

Asteroid families form as a result of large-scale collisions among main belt asteroids. The orbital distribution of fragments after a family-forming impact could inform us about th…