Canon EOS 5D Mark IV
ƒ/10
65 mm
1/100
25600

Vesta is the largest and brightest asteroid in the asteroid belt and the second largest body overall (after the dwarf planet Ceres), with an average diameter of about 525 km (326 miles). That is pretty close to the size of the State of Colorado.

A couple of billion years ago two massive impacts ejected part of Vesta’s mass and some of that material landed here on Earth as HED (howardite, eucrite, and diogenite) meteorites. It’s astonishing to consider that when you look at photographs of Vesta, or eve through a powerful telescope, the actual craters from which the HED meteorites were blasted out can easily be seen, such as Rheasilvia which is over 300 miles wide.

From the Meteorite Bulletin for NWA 7831:

History: Found buried in the ground near Chouichiyat in the Western Sahara on March 3, 2013, and excavated by a team of local people.

Physical characteristics: composed of translucent yellow-green crystals of orthopyroxene with pale orange weathering products along numerous fractures. Much of the material disintegrated into fragments upon excavation.

3 responses to “NWA 7831 Olivine DIogenite — 5x Macro #3”

  1. Diogenite comes from deep in the mantle of Vesta, We have never drilled that deep on Earth, but it might look somewhat similar. New work on exposed mantle in Maryland give us a sense of what it looks like. From National Geographic:

    "While this layer of rock is usually found between the planet’s crust and core, a segment peeks out of the scrubby Maryland forest, offering scientists a rare chance to study Earth’s innards up close. Even more intriguing, the rock’s unusual chemical makeup suggests that this piece of mantle, along with chunks of lower crust scattered around Baltimore, was once part of the seafloor of a now-vanished ocean.
    Over the roughly 490 million years since their formation, these hunks of Earth were smashed by shifting tectonic plates and broiled by searing hot fluids rushing through cracks, altering both their composition and sheen. Mantle rock is generally full of sparkly green crystals of the mineral olivine, but the rock in my hand was surprisingly unremarkable to look at: mottled yellow-brown stone occasionally flecked with black.
    “Those rocks have had a tough life,” says George Guice, a mineralogist at the Smithsonian’s National Museum of Natural History.

    THE LURE OF GREEN SPARKLE
    Guice has long chased after sparkly green rocks, known to geologists as ultramafic. They’re rich in magnesium and make up the majority of our planet as the mantle. But pieces of the mantle are rare at the surface, and ultramafic rocks can form in several different ways, including in large crystallizing magma chambers. They’re also devilishly difficult to study.

    Ultramafic rocks form deep underground at high temperatures and pressures, so their minerals are not stable near Earth’s surface. In this shallow environment, they’re often exposed to hot fluids rushing through cracks, transforming their mineral makeup, as seen in the rocks strewn around Baltimore. Understanding the rock’s history through these changes, Guice says, is like looking through thick fog."

    Meteorites offer a preserved time capsule from these depths, albeit from an alien world.

  2. New research related to the anorthite contained in some rare Vestian meteorites, like mine here: Meteorite suggests asteroid Vesta may once have had magma lake just like the early moon, say Chinese scientists: "The researchers said that while Vesta is much smaller than the moon and other planets, the “planetary embryo” has a similar evolutionary history to the moon. Anorthosites are formed when magma oceans solidify and the only ones that have previously been found have come from the Earth or the moon."

Leave a Reply to jurvetson Cancel reply

Your email address will not be published. Required fields are marked *