17 citations · 17 across the 1 of their papers we have counts for
8 papers
Scattering V-type asteroids during the giant planets instability: A step for Jupiter, a leap for basalt
Pedro Brasil, Fernando Roig, David Nesvorný +1
V-type asteroids are a taxonomic class whose surface is associated to a basaltic composition. The only known source of V-type asteroids in the Main Asteroid Belt is (4) Vesta, that…
Detection of the YORP Effect for Small Asteroids in the Karin Cluster
Valerio Carruba, David Nesvorný, David Vokrouhlický
The Karin cluster is a young asteroid family thought to have formed only ~My ago. The young age can be demonstrated by numerically integrating the orbits of Karin clus…
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…
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…
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…
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…