Jbilet Winselwan meteorite

Jbilet Winselwan was reported in early June 2013 by a meteorite hunter from Smara, Western Sahara. Due to inherent delays in communication from the desert, the official date of the find is earlier than the initial reports. The accessibility of the strewn field, being only 7 miles south of Smara, led to a large number of meteorite hunters visiting the area from the summer of 2013 onward. The majority of specimens range from 3 to 200 grams with a few larger samples occurring, the largest being ~900g. Samples reached the market quickly and the official classification was approved by The Meteoritical Society on 12 August 2013.[1]

Jbilet Winselwan was classified as CM-type carbonaceous chondrite at The National Museum of Natural History, France, and The University of Hassan II Casablanca based on its oxygen-isotopic composition, petrography, and mineral compositions. The meteorite contains CAIs and both type I and type II chondrules ranging up to 1.2mm, with the majority around 200 μm. X-ray diffraction used in classification showed strong peaks for serpentines, broad but weaker peaks for smectites, and a weak broad peak for tochilinite. Major silicate compositions are olivine (Fa_0.98±0.44 and Fa_25-40) and pyroxene (Fs_2.6±1.5 and Fs_40-61). Rare kamacite with 5.8 wt% Ni was identified. The oxygen isotopic compositions were measured for two fragments for identification, at δ¹⁸O 3.811±0.09 and 5.851±0.016, δ¹⁷O -2.446±0.040 and -0.601±0.026, respectively. The isotope values plot well inside the CM chondrite region.[1][5]

As a result of its pristinity and relative ease to obtain, Jbilet Winselwan has been extensively studied for a northwest Africa find. The earliest studies identified its extreme degree of brecciation,[1][3][5] showing that it likely represents the outermost portion of its parent asteroid; the regolith. This regolith context has been of particular interest, as two missions are currently underway to collect asteroid regolith, Hayabusa2 and OSIRIS-REx. Jbilet Winselwan has specifically been identified as an analog for Hayabusa2, as the mission is targeting a C-type asteroid, the same class as its likely parent body.[2] In this context, the meteorite was further characterized in its major and minor elements,[2] alteration textures,[2] hydrocarbons,[6] and thermal metamorphism.[6]

The extremely brecciated characteristics of Jbilet Winselwan have also led people to use it as an indicator of the thermal and hydration history of its parent body. A single thin section will contain multiple lithologies ranging from typically-hydrated CM chondrite material with tightly packed chondrules to significantly more dehydrated material with few, poorly preserved chondrules. It has been suggested that some Jbilet Winselwan lithologies represent prime examples of post-shock aqueous alteration,[3] including some regions which have formed as a result of cyclical events.[4]