By means of a varied-shape thermophysical model of Hanuš et al.(2015) that takes into
account asteroid shape and pole uncertainties, we analyze the thermal infrared data …

There are only a few known main belt (MB) asteroid families with ages greater than 2 Gyr
(Brož et al., 2013; Spoto et al., 2015). Estimates based on the family producing collision rate …

Eos family was created during a catastrophic impact about 1.3 Gyr ago. Rotation states of
individual family members contain information about the history of the whole population. We …

Forming the Flora Family: Implications for the Near-Earth Asteroid Population and Large
Terrestrial Planet Impactors - IOPscience This site uses cookies. By continuing to use this site …

Context. Asteroid (2579) Spartacus is a small V-type object located in the inner main belt.
This object shows spectral characteristics unusual for typical Vestoids, which may indicate …

Context. Most howardite-eucrite-diogenite (HED) meteorites (analogues to V-type asteroids)
are thought to originate from the asteroid (4) Vesta. However some HEDs show distinct …

SsoDNet.datacloud bibliographic references ABSTRACT Full list of bibliographic references
describing the methods used to determi Page 1 Draft version April 23, 2024 Typeset using …

Surveys are an important part of any science. In regard to asteroids, surveys can be used to
gather characteristics about as many asteroids as possible and then applied to models of …