The past decade has seen an astonishing array of advances across a wide spectrum of
important inputs to the problem and mystery of asteroid interiors. These include the …

Our photometric observations of Asteroid (99942) Apophis from December 2012 to April
2013 revealed it to be in a state of non-principal axis rotation (tumbling). We constructed its …

We studied a sample of 93 asteroid pairs, ie, pairs of genetically related asteroids that are on
highly similar heliocentric orbits. We estimated times elapsed since separation of pair …

The discovery of 1I/2017 U1 (1I/'Oumuamua) has provided the first glimpse of a planetesimal
born in another planetary system. This interloper exhibits a variable colour within a range …

This is a study of the collisional history of the asteroids in the main asteroid belt. Over the∼
4.5 Byr of the belt existence, every asteroid collided with others a multitude of times …

In the past decade, hundreds of asteroid shape models have been derived using the
lightcurve inversion method. At the same time, a new framework of three-dimensional shape …

We consider the effect of an asteroid's approach to a planet on its rotational dynamics by
means of comprehensive numerical experiments. For a number of asteroids experiencing …

We present V-band photometry of the 20 000 brightest asteroids using data from the All-Sky
Automated Survey for Supernovae (ASAS-SN) between 2012 and 2018. We were able to …

Asteroid-sized bodies are predicted to have been scattered throughout the solar system
following gravitational interactions with the giant planets. This process could have delivered …

We propose and analyze a new mechanism for the formation of the wide asynchronous
binary population. These binary asteroids have wide semimajor axes relative to most near …