EDUCATION
Find a Meteorite: Explore Meteorites - Achondrites
Achondrites: Meteorites from asteroids that melted
When asteroids became hot enough to melt the rock and metal portions found in the chondritic type, material separated to form different types of meteorites. The rock portion of the bodies became a type of stony meteorite called the achondrites (meteorites without chondrules). These are actually igneous rocks from magmas that formed on asteroids. These asteroids became hot enough to melt from radioactive elements just after the Solar System formed (4.6 billion years ago).
Igneous Rocks (formed from melts)
|
|
During melting, the denser metal separated in these asteroids to form iron meteorites. The Iron meteorites are composed mainly of iron alloyed with nickel and they often contain a sulfide mineral called troilite (FeS) (something like fools gold or pyrite found on the Earth). Irons are the meteorites that are most easy to identify because they are heavier than most rocks, are magnetic, and are made of iron and nickel metal. Just like the Earth which has an iron-nickel core, the composition of irons indicates that they represent the cores of their parent asteroids.
The stony-iron meteorites or stony-irons are composed of both rocky material that formed from a magma and metallic iron-nickel. If an asteroid, contains a core, mantle, and crust, like the Earth does; then, the irons would be from the core, the stones from the crust or mantle, and the stony-irons from in-between the core and mantle. The asteroid Vesta is thought to have melted and may contain achondrite materials. The optical and infrared spectral signatures of the rocks on Vesta observed by telescopes match some of the achondrite meteorites, which suggests that some of these meteorite types (Howardites, Eucrites, and Diogenites) might come from Vesta!
Stony-irons and iron meteorites
|
|
|
- Back to Explore Meteorites
- More about asteroids that didn't melt
- More about asteroids that melted
- More about meteorites
- Dawn Dictionary



