Constraints on the Gamma-Ray Emission from Small Solar System Bodies with the Fermi Large Area Telescope Data [PDF]
All known small solar system bodies have diameters between a few meters and a few thousands of kilometers. Based on the collisional evolution of solar system bodies, a larger number of asteroids with diameters down to ∼2 m is thought to exist.
S. De Gaetano +8 more
doaj +7 more sources
Small solar system bodies as granular systems [PDF]
Asteroids and other Small Solar System Bodies (SSSBs) are currently of great scientific and even industrial interest. Asteroids exist as the permanent record of the formation of the Solar System and therefore hold many clues to its understanding as a ...
Hestroffer Daniel +16 more
doaj +6 more sources
Performing Automated, High-Speed Photometry on Occulting, Small Outer Solar System Bodies
Monitoring stellar occultations provides a powerful means to measure the shapes and sizes of small Solar System bodies, but produces large quantities of image data which can be laborious to analyse.
Ben Attwood, James Robinson
doaj +5 more sources
Small Solar System Bodies as granular media [PDF]
Asteroids and other Small Solar System Bodies (SSSBs) are of high general and scientific interest in many aspects. The origin, formation, and evolution of our Solar System (and other planetary systems) can be better understood by analysing the ...
D. Hestroffer +14 more
exaly +5 more sources
Glycine amino acid transformation under impacts by small solar system bodies, simulated via high-pressure torsion method [PDF]
Impacts by small solar system bodies (meteoroids, asteroids, comets and transitional objects) are characterized by a combination of energy dynamics and chemical modification on both terrestrial and small solar system bodies.
Kaveh Edalati +3 more
doaj +2 more sources
The Moon: An Archive of Small Body Migration in the Solar System [PDF]
The Moon is an archive of impact cratering in the Solar System throughout the past 4.5 billion years. It preserves this record better than larger, more complex planets like the Earth, Mars and Venus, which have largely lost their ancient crusts through geological reprocessing and hydrospheric/atmospheric weathering.
K. H. Joy +5 more
openalex +5 more sources
Composition of Solar System Small Bodies [PDF]
The aim of the chapter is to summarize our understanding of the compositional distribution across the different reservoirs of small bodies (main belt asteroids, giant planet trojans, irregular satellites of the giant planets, TNOs, comets). We then use this information to i) discuss current dynamical models (Nice and Grand Tack models), ii) mention ...
Vernazza, Pierre, Beck, Pierre
openaire +4 more sources
Water in small bodies of the Solar System [PDF]
AbstractWater in form of ice or vapour is observed in comets, transneptunian objects and icy satellites formed in the outer regions of the Solar System, as well as in objects orbiting in the inner Solar System, such as dwarf planet Ceres. I will present an overview of the water content and properties in these objects and the implications in terms of ...
D. Bockelée–Morvan
openalex +3 more sources
Observation and research on small solar system bodies based on the Antarctic Tianmu Staring Observation Project [PDF]
The Antarctic Tianmu Staring Observation Project (ATSOP) entails the deployment of 30 small-aperture, wide-field optical telescopes in the Antarctic region.
JianChun Shi +10 more
doaj +2 more sources
Captured Small Solar System Bodies in the Ice Giant Region [PDF]
This white paper advocates for the inclusion of small, captured Outer Solar system objects, found in the Ice Giant region in the next Decadal Survey. These objects include the Trojans and Irregular satellite populations of Uranus and Neptune.
Timothy R. Holt +16 more
openalex +3 more sources

