Mapping olivine abundance on asteroid (25143) Itokawa from Hayabusa/NIRS data
L Nardi, E Palomba, A Longobardo, A Galiano, F Dirri - Icarus, 2019 - Elsevier
Olivine is one of the main abundant mineral in the Solar System, and the determination of its
abundance on a surface may give fundamental information about its evolution. The study of …
abundance on a surface may give fundamental information about its evolution. The study of …
Round up the unusual suspects: Near-Earth Asteroid 17274 (2000 LC16) a plausible D-type parent body of the Tagish Lake meteorite
GM Gartrelle, PS Hardersen, MRM Izawa, MC Nowinski - Icarus, 2021 - Elsevier
Asteroids are the origin point for most meteorites impacting Earth. Terrestrial meteorite
samples provide evidence of what actually occurred in the early solar system at the …
samples provide evidence of what actually occurred in the early solar system at the …
[PDF][PDF] Deriving global Olivine distribution on Hayabusa's target (25143) Itokawa using Near-Infrared Spectrometer data
L Nardi, E Palomba… - European …, 2017 - meetingorganizer.copernicus.org
In 2005 Hayabusa spacecraft visited asteroid Itokawa, bringing back surface samples to
Earth in 2010. Near-Infrared spectra acquired by NIRS and samples analysis confirmed …
Earth in 2010. Near-Infrared spectra acquired by NIRS and samples analysis confirmed …
[图书][B] Spectral Variations of D-Type Asteroids at Different Heliocentric Distances
GM Gartrelle - 2019 - search.proquest.com
D-type asteroids represent a complex mystery related to the history, compositional
chemistry, and dynamical migration of Outer Solar System objects. These spectrally …
chemistry, and dynamical migration of Outer Solar System objects. These spectrally …