Maskelynite
Glassy material found in some meteorites and meteorite impact craters
title: "Maskelynite" type: doc version: 1 created: 2026-02-28 author: "Wikipedia contributors" status: active scope: public tags: ["minerals", "glass-in-nature", "impact-event-minerals", "meteorite-minerals"] description: "Glassy material found in some meteorites and meteorite impact craters" topic_path: "general/minerals" source: "https://en.wikipedia.org/wiki/Maskelynite" license: "CC BY-SA 4.0" wikipedia_page_id: 0 wikipedia_revision_id: 0
::summary Glassy material found in some meteorites and meteorite impact craters ::
::data[format=table title="infobox mineral"]
| Field | Value |
|---|---|
| name | Maskelynite (meteoritic glass) |
| image | NWA 1195, martian meteorite.jpg |
| caption | NWA 1195, a Martian meteorite composed largely of maskelynite |
| category | Glass |
| luster | Vitreous |
| :: |
| name = Maskelynite (meteoritic glass) | boxwidth = | boxbgcolor = | image = NWA 1195, martian meteorite.jpg | imagesize = | alt = | caption = NWA 1195, a Martian meteorite composed largely of maskelynite | category = Glass | formula = | strunz = | dana = | symmetry = | unit cell = | molweight = | color = | colour = | habit = | system = | twinning = | cleavage = | fracture = | tenacity = | mohs = | luster = Vitreous | streak = | diaphaneity = | gravity = | density = | polish = | opticalprop = | refractive = | birefringence = | pleochroism = | 2V = | dispersion = | extinction = | length fast/slow = | fluorescence = | absorption = | melt = | fusibility = | diagnostic = | solubility = | impurities = | alteration = | other = | prop1 = | prop1text = | references = Maskelynite is a glassy material found in some meteorites and meteorite impact craters. Typical samples are similar in composition to plagioclase feldspar, and revert to that mineral when melted and recrystallized. It was named after British geologist M.H.N. Story-Maskelyne.
Since maskelynite (like the volcanic glass obsidian) lacks an orderly arrangement of atoms, it is not considered a "mineral" by geologists, and is not listed as such by the Mineralogical Society of America.
History
The phase was first identified in the Shergotty meteorite by G. Tschermak (1872) as an isotropic glass of an unknown origin with near labradorite composition.{{cite conference | title = The Nature of "Maskelynite" in Shocked Meteorites: Not Diaplectic Glass but a Glass Quenched from Shock-Induced Dense Melt at High-Pressures | author = M. Chen |author2=A. El Goresy | book-title = Proceedings of the 62nd Annual Meteoritical Society Meeting | place = Johannesburg | number = 5047 | url = http://www.lpi.usra.edu/meetings/metsoc99/pdf/5047.pdf | date = 1999 | title = Maskelynite: Formation by Explosive Shock | author = Daniel J. Milton |author2=Paul S. de Carli | journal = Science | date = 1963 | volume = 140 | pages = 670–671 | doi = 10.1126/science.140.3567.670 | pmid = 17737107 | issue = 3567 |bibcode = 1963Sci...140..670M | s2cid = 39067336 | title = Natural Terrestrial Maskelynite | author = T.E. Bunch | author2 = Alvin J. Cohen | author3 = M. R. Dence | date = 1967 | journal = The American Mineralogist | volume = 52 | pages = 244–253 | url = http://www.minsocam.org/ammin/AM52/AM52_244.pdf
Origin
At first, maskelynite was believed to result from solid-state transformation of plagioclase into diaplectic glass by a relatively low-pressure shock wave (250 to 300 kilobars) and low-temperature (350°C), as in Milton and de Carli's experiment. Since 1997, this hypothesis has been challenged and now it is believed that the glass is formed by the quenching of dense mineral melts produced by higher-pressure shock waves.
References
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