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The first solar system minerals

Mineralogists so far have discovered the following 11 minerals in presolar grains.
Yellow-octahedral-crystal
Diamond is the hardest mineral known. This 1.19-carat yellow octahedral crystal measures 0.6 centimeter across. It originated in the Premier Mine, Cullinan, Pretoria, Gauteng Province, South Africa. David J. Eicher collection
In the November 2012 issue of Astronomy, world-renowned mineralogist Jolyon Ralph wrote, “Did life change Earth’s geology?” The author talked about the first minerals that formed within grains of material that predate the solar system’s formation. But didn’t have room for a list of these minerals in the magazine.

Mineralogists so far have discovered the following 11 minerals in presolar grains (material from outside our solar system that formed when massive stars exploded or were part of the outflows of red giant stars) contained within chondrite meteorites:

Corundum (Al2O3) — This mineral, also known as alumina, is chemically and structurally the same as ruby and sapphire.

Diamond (C) — Scientists found nanometer-sized grains (around 2.6nm in diameter) possibly formed by vapor deposition.

Graphite (C) — The most stable form of carbon, graphite exists in presolar grains as particles and layered particles, some with graphene (an atomic-scale honeycomb lattice made of carbon atoms) cores.

Hibonite ([Ca, Ce]Al12O19) — This calcium aluminum oxide also contains some cerium and often titanium and magnesium.

Corundum
Corundum is another mineral found in presolar grains. It manifests in several varieties. The one shown here, ruby, measures 5 centimeters across. It comes from the Jagdalak Ruby Mine, Sorobi District, Konar Province, Afghanistan. David J. Eicher collection
Moissanite (SiC) — Mineralogists first found this in rock samples from Barringer Meteorite Crater, Arizona.

Nierite (Si3N4) — Silicon nitride is a hard ceramic used in high-temperature applications such as bearings in the main engines of NASA’s space shuttles; mineralogists found it in the 1990s in presolar grains.

Olivine ([Mg, Fe]2SiO4) — Researchers have detected olivine on the Moon and Mars, in meteorites, in comets, and raining down on a protostar known as HOPS-68.

Pyroxene ([Mg, Fe]SiO3) — This forms a group of minerals; enstatites are magnesium-rich and ferrosilites are iron-rich. Both are common in meteorites. Astronomers have observed enstatite around the planetary nebula NGC 6302.

Spinel (MgAl2O4) — This magnesium aluminum oxide is common in the calcium-aluminum-rich inclusions of chondrites.

Titanium carbide (TiC) — This extremely hard ceramic occurs with other carbides and within grains of diamond, graphite, and Mossanite.

Titanium oxide (TiO2) — Three mineral forms of titanium oxide occur: rutile, anatase, and brookite. Each is TiO2 but crystallizes in a different way. TiO2 exists in the atmospheres of M-class stars, which are cool enough for the molecules to form.

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