Meteorite**Ksar Ghilane 022, Achon. Ung.**26.287 gram, Planet Mercury Candidate For Sale

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Meteorite**Ksar Ghilane 022, Achon. Ung.**26.287 gram, Planet Mercury Candidate:
$5800.00

Ksar Ghilane 022, classified as an \"Achondrite (ungrouped, Mg-rich clinopyroxenite)\", is a rare and intriguing meteorite that is speculated to be a strong candidate for originating from the planet Mercury. The presence of sulfide spherules, along with exotic sulfides like oldhamite, suggest a possible connection to planets like Mercury or Venus due to the long periods of heating that likely formed these unique features.

This particular slice of Ksar Ghilane 022 weighs 26.287 grams and boasts a flawless polish on one side, making it a desirable piece for collectors and enthusiasts. The meteorite\'s uncommon composition and potential link to inner solar system planets such as Mercury make it a fascinating specimen for study and admiration.

Based on the petrography and geochemistry information provided, the presence of almost end-member augite and enstatite, along with accessory minerals such as Cr-troilite, daubreelite, and an Mn-Fe oxide phase, are indicative of a unique composition that could potentially be associated with a meteorite from the planet Mercury. The presence of minerals like enstatite and sulfides, coupled with the specific oxygen isotope ratios found, could provide evidence supporting a possible origin from Mercury.

Ksar Ghilane 022 (KG 022) 32.559°N, 9.508°E

Tatawin, Tunisia

Purchased: 2023

Classification: Ungrouped achondrite

History: Found in Tunisia in 2023. Purchased by Adam Aaronson in February and November 2023 from a Libyan dealer. Portions of the material were subsequently provided to Craig Zlimen at the Tucson Gem and Mineral Show in February 2024, and in turn acquired by Robert Ward, Brian Caress and Ben Hoefnagels.

Physical characteristics: A single large stone (25 kg) and many smaller pieces found with it. Most of the stones lack fusion crust and have mottled, dark and light gray granular exteriors. However, several pieces are partly coated by black fusion crust. The interiors of the stones have the appearance of equigranular aggregates of light gray and whitish grains.

Petrography: (A. Irving, UWS, and P. Carpenter, WUSL) The specimen is composed predominantly (>90 vol.%) of almost end-member augite (mostly as equant grains, mean grainsize ~1.5 mm) accompanied by minor enstatite and accessory Cr-troilite, daubreelite, alabandite and an Mn-Fe oxide phase. Enstatite occurs as small irregular inclusions or sparse fine lamellae within augite grains, and different macroscopic colors of the augite grains apparently reflect differing concentrations of sulfide inclusions. Some secondary calcite veins are present throughout.

Geochemistry: Augite (Fs0.0-0.1Wo39.4-42.3, N = 3), enstatite (Fs0.1±0.0Wo0.9-3.6, N = 3). Oxygen isotopes (K. Ziegler, UNM): analyses of acid-washed subsamples by laser fluorination gave, respectively, δ17O 3.018, 2.926; δ18O 5.781, 5.559; Δ17O -0.034, -0.009 per mil (all data linearized, TFL slope = 0.528).

Classification: Achondrite (ungrouped, Mg-rich clinopyroxenite). This meteorite is texturally and mineralogically very similar to ungrouped augite-rich achondrite NWA 15915. but does not exhibit the same degree of irrational exsolution of enstatite from the dominant constituent augite. Terrestrial pairing is further excluded by the different physical appearance of these two meteorites, different degree of weathering, and the fact that their purported find sites are hundreds of kilometers apart. Both of these meteorites may have some affinities to aubrites, but differ in being composed predominantly of almost Fe-free augite rather than enstatite.

Meteorite**Ksar Ghilane 022, Achon. Ung.**26.287 gram, Planet Mercury Candidate

$5800.00

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