Results 1 to 10 of about 22,696,219 (287)
Methodology for the Observations of Stellar Occultations by Small Bodies of the Solar System
The observation of stellar occultations constitutes one of the most important techniques for determining the dimensions and establishing the physical parameters of small Solar System bodies.
Luis E. Salazar-Manzano +1 more
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SMALL VELOCITIES OF METEOROIDS: INTERRELATION OF SOLAR SYSTEM SMALL BODIES
Reality and dynamical connection of meteoroids with small velocities are discussed.
V. V. Andreev
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Regolith dynamics on small bodies in the Solar System [PDF]
Many small bodies in the Solar System, such as near-Earth asteroids, are believed to be granular aggregates - rubble piles – held together mainly by low self-gravity, typically of the order of mms−2.
Gaurav Kumar +2 more
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. In the framework of UkrVO national project the new methods of plate digital image processing are developed. The photographic material of the UkrVO Joint Digital Archive (JDA – http://gua.db.ukr-vo.org/vo-mao/DB/archivespecial.php) is used for the ...
I. Vavilova +8 more
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Metal Pollution of the Solar White Dwarf by Solar System Small Bodies
Abstract White dwarfs (WDs) often show metal lines in their spectra, indicating accretion of asteroidal material. Our Sun is to become a WD in several gigayears. Here, we examine how the solar WD accretes from the three major small body populations: the main belt asteroids (MBAs), Jovian Trojan asteroids (JTAs), and trans-Neptunian ...
Daohai Li +2 more
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Three Fast-spinning Medium-sized Hilda Asteroids Uncovered by TESS
Hilda asteroids, which orbit in a 3:2 resonance with Jupiter, serve as key indicators of dynamical processes in the early solar system. Their spin rates, an important probe of these mechanisms, can constrain their density and collisional evolution ...
Nóra Takács +10 more
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Orbital and Absolute Magnitude Distribution of Jupiter Trojans
Jupiter Trojans (JTs) librate about the Lagrangian stationary centers L4 and L5 associated with this planet on typically small-eccentricity and moderate-inclination heliocentric orbits.
David Vokrouhlický +6 more
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Meteorites and cosmic dust: Interstellar heritage and nebular processes in the early solar system
Small solar system bodies like asteroids and comets have escaped planetary accretion. They are the oldest and best preserved witnesses of the formation of the solar system.
Engrand C.
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We present here the design, architecture, and first data release for the Solar System Notification Alert Processing System (SNAPS). SNAPS is a solar system broker that ingests alert data from all-sky surveys.
David E. Trilling +6 more
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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 ...
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