Free Access

Fig. 4

thumbnail

Asteroid spectra and the best two matches derived from a comparison with laboratory spectra: a) spectrum of Kourakuen and the spectrum of a sample from Pavlovka; b) spectrum of Kourakuen and the spectrum of a mixture of pyroxene hypersthene plagioclase bytownite ilmenite; c) spectrum of Apophis and the spectrum of a simulant Lunar soil; d) spectrum of Apophis and the spectrum of a particulate sample from the Hamlet meteorite; e) de-reddened spectrum of Apophis and the spectrum of a particulate sample from the Cherokee Springs meteorite; f) de-reddened spectrum of Apophis and the spectrum of a particulate sample from the Cat Mountain meteorite; g) spectrum of 1996 FG3 and the spectrum of a sample from the meteorite Sete Lagoas; and h) spectrum of 1996 FG3 and the spectrum of a sample from the Murchison meteorite heated to 1000 °C.

This figure is made of several images, please see below:

Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.

Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.

Initial download of the metrics may take a while.