It is of great significance to apply the object detection methods to automatically detect
boulders from planetary images and analyze their distribution. This contributes to the …

We manually mapped particles ranging in longest axis from 0.3 cm to 95 m on (101955)
Bennu for the Origins, Spectral Interpretation, Resource Identification, and Security–Regolith …

Boulders form from a variety of geological processes, which their size, shape, and
orientation may help us better understand. Furthermore, they represent potential hazards to …

Abstract The Orbiter High Resolution Camera (OHRC) is a very high spatial resolution
panchromatic camera (0.45–0.70 μm) on-board Chandrayaan-2 orbiter. Its spatial resolution …

Like many airless planetary surfaces, the surface of the Moon is scattered by populations of
blocks and smaller boulders. These features decrease in abundance with increasing …

Dawn's framing camera observed boulders on the surface of Vesta when the spacecraftwas
in its lowest orbit (Low Altitude Mapping Orbit, LAMO). We identified, measured, and …

Abstract Orbiter High Resolution Camera (OHRC) on-board Chandrayaan-2 had acquired a
high-resolution image (∼ 0.26 m) covering Apollo 11 landing site, showing the Lander …

We focus on a young (~ 4.5 Ma), 3.4 km long landslide located in the floor of Simud Vallis,
Oxia Palus Quadrangle of Mars. By making use of a 2 m-scale HiRISE DEM we reconstruct …

We study the size frequency distribution of the blocks located in the deeply fractured,
geologically active Enceladus South Polar Terrain with the aim to suggest their formative …

Boulder occurrence at the southern polar regions of the Moon was analysed to see
connections between optical, radio, spectral, and topography-related roughness datasets …