Results 31 to 40 of about 214,518 (270)
VLT/SPHERE imaging survey of the largest main-belt asteroids: Final results and synthesis
Context. Until recently, the 3D shape, and therefore density (when combining the volume estimate with available mass estimates), and surface topography of the vast majority of the largest (D ≥ 100 km) main-belt asteroids have remained poorly constrained.
P. Vernazza+66 more
semanticscholar +1 more source
Size and Albedo Constraints for (152830) Dinkinesh Using WISE Data
Probing small main-belt asteroids provides insight into their formation and evolution through multiple dynamical and collisional processes. These asteroids also overlap in size with the potentially hazardous near-Earth object population and supply the ...
Kiana D. McFadden+9 more
doaj +1 more source
Taxonomic Analysis of Asteroids with Artificial Neural Networks
We study the surface composition of asteroids with visible and/or infrared spectroscopy. For example, asteroid taxonomy is based on the spectral features or multiple color indices in visible and near-infrared wavelengths.
Nanping Luo+5 more
doaj +1 more source
CASTAway: An asteroid main belt tour and survey [PDF]
CASTAway is a mission concept to explore our Solar System's main asteroid belt. Asteroids and comets provide a window into the formation and evolution of our Solar System and the composition of these objects can be inferred from space-based remote sensing using spectroscopic techniques.
S. B. Calcutt+45 more
openaire +15 more sources
On the oldest asteroid families in the main belt [PDF]
Asteroid families are groups of minor bodies produced by high-velocity collisions. After the initial dispersions of the parent bodies fragments, their orbits evolve because of several gravitational and non-gravitational effects,such as diffusion in mean-motion resonances, Yarkovsky and YORP effects, close encounters of collisions, etc.
R. C. Domingos+6 more
openaire +7 more sources
The distribution of basaltic asteroids in the Main Belt [PDF]
We present the observational results of a survey designed to target and detect asteroids whose colors are similar to those of Vesta family members and thus may be considered as candidates for having a basaltic composition. Fifty basaltic candidates were selected with orbital elements that lie outside of the Vesta dynamical family.
Ronald Fevig+7 more
openaire +3 more sources
Determining the Pyroxene Mineralogies of Vestoids
Bulk pyroxene compositions were calculated for a number of V-type asteroid spectra using formulae derived by Burbine et al. These formulae were derived by analyzing HED (howardite, eucrite, and diogenite) meteorites and calculate bulk Fs (mol%) and Wo ...
T. H. Burbine+3 more
doaj +1 more source
The Challenge of Measuring Asteroid Masses with Gaia DR2 Astrometry
The Gaia second data release (DR2) contains high-accuracy astrometric measurements of thousands of solar system bodies. These measurements raise the possibility of determining asteroid masses by modeling scattering events between massive objects observed
Zachary Murray
doaj +1 more source
The Flux Distribution and Sky Density of 25th Magnitude Main Belt Asteroids [PDF]
Digital tracking enables telescopes to detect asteroids several times fainter than conventional techniques. We describe our optimized methodology to acquire, process, and interpret digital tracking observations, and we apply it to probe the apparent ...
A. Heinze, Joseph Trollo, S. Metchev
semanticscholar +1 more source
The Mid-plane of the Main Asteroid Belt [PDF]
Abstract We measure the mid-plane of the main asteroid belt by using the observational data of a nearly complete and unbiased sample of asteroids and find that it has inclination and longitude of ascending node
Saverio Cambioni, Renu Malhotra
openaire +3 more sources