Results 121 to 130 of about 15,403 (216)
M-type asteroids are historically thought to be exposed metallic cores of differentiated planets with a composition dominated by pure iron and nickel. However, recent spectral and radar observations reveal an insufficient number of M-type asteroids in ...
Tian Zhang +7 more
doaj +1 more source
Asteroid Collisions: Expected Visibility and Rate
Asteroid collisions are one of the main processes responsible for the evolution of bodies in the main belt. Using observations of the Dimorphos impact by the DART spacecraft, we estimate how asteroid collisions in the main belt may look in the first ...
Eran O. Ofek +11 more
doaj +1 more source
Speckle interferometry of asteroids [PDF]
This final report for NASA Contract NAGw-867 consists of abstracts of the first three papers in a series of four appearing in Icarus that were funded by the preceding contract NAGw-224: (1) Speckle Interferometry of Asteroids I.
Drummond, Jack
core +1 more source
Asteroid size distributions for the main belt and for asteroid families [PDF]
A. Kazantzev, L. Kazantzeva
openaire +1 more source
Terrestrial planet and asteroid belt formation by Jupiter-Saturn chaotic excitation. [PDF]
Lykawka PS, Ito T.
europepmc +1 more source
Shape, size and multiplicity of main-belt asteroids I. Keck Adaptive Optics survey. [PDF]
Marchis F +7 more
europepmc +1 more source
Spectroscopic identification of water emission from a main-belt comet. [PDF]
Kelley MSP +6 more
europepmc +1 more source
Tests of HgCdTe Photodetectors Performances for Implementation on the MIST-A Instrument. [PDF]
Cencia C +25 more
europepmc +1 more source

