activity
20102024
most citedChelyabinsk meteorite explains unusual spectral properties of Baptistina Asteroid Family

75 citations · 290 across the 21 of their papers we have counts for

collaborators

21 papers

astro-ph.EP2024

Origin of Asteroid (101955) Bennu and its Connection to the New Polana Family

Driss Takir, Joshua P. Emery, William F. Bottke +1

The asteroid (142) Polana is classified as a B-type asteroid located in the inner Main Belt. This asteroid is the parent of the New Polana family, which has been proposed to be the…

astro-ph.EP202441 cited

A Contact Binary Satellite of the Asteroid (152830) Dinkinesh

Harold F. Levison, Simone Marchi, Keith S. Noll +3

Asteroids with diameters less than about 5 km have complex histories because they are small enough for radiative torques, YORP, to be a notable factor in their evolution. (152830)…

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.EP2024

The population of small near-Earth objects: composition, source regions and rotational properties

Juan A. Sanchez, Vishnu Reddy, Audrey Thirouin +7

The study of small (300 m) near-Earth objects (NEOs) is important because they are more closely related than larger objects to the precursors of meteorites that fall on Earth. C…

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…