diogenite


Also found in: Wikipedia.

diogenite

[dī′ä·jə‚nīt]
(mineralogy)
An achondritic stony meteorite composed essentially of iron-rich pyroxene minerals. Also known as rodite.
Mentioned in ?
References in periodicals archive ?
The slice on the right comes from a diogenite meteorite named GRA 98108, recovered from Graves Nunatak, Antarctica.
The new findings solidly confirm the connection between Vesta and a class of meteorites found on Earth called the Howardite, Eucrite and Diogenite meteorites, which have the same ratios for these elements.
In addition, samples of howardite and diogenite meteorites were used for comparison.
He simply wanted to take a close look at a meteorite that researchers had classified as a diogenite. This type of rock is believed to have come from a well-studied asteroid, 4 Vesta.
Scientists have several theories about why this is the case and the research team-which included lead author James Day of Scripps Institution of Oceanography and Richard Walker of the University of Maryland-set out to explore these theories by looking at diogenite meteorites.
This basin appears to have excavated into the mantle of Vesta, exposing material spectrally similar to diogenite meteorites; Vesta's crust is spectrally similar to eucrite and howardite meteorites, thus confirming that Vesta and its family of asteroids are the source of the howardite-eucrite-diogenite (HED) family of basaltic achondrite meteorites.
Although Vesta and its family are located between Mars and Jupiter, smaller pieces of these asteroids can be found in meteorite collections on Earth, including most eucrite, howardite and diogenite meteorites.
For nearly a decade the stone was considered a diogenite, a class of igneous meteorites believed to be chips of the asteroid Vesta.
ALH84001 masqueraded for almost a decade as a diogenite, thought to be a chip off the asteroid 4 Vesta.
Scientists noticed that Vesta's infrared spectrum is remarkably similar to the spectra of a class of meteorites called the HEDs (Howardites, Eucrites, and Diogenites), ancient samples of which apparently started out as volcanic rocks within the crust or mantle of a large terrestrial planet or protoplanet and that were later transported to Earth by impacts.
The three meteorite types -- the eucrites, howardites and diogenites -- came from an asteroid big enough for its surface rock to melt, possibly from the heat of radioactive elements inside it, concludes a team headed by Dale P.
Vesta's spectra match those of a class of meteorites called the HEDs (for "Howardites, Eucrites, and Diogenites").