Stone Meteorites

Stone meteorites, the most common type found on Earth, are primarily composed of silicate minerals such as olivine and pyroxene. These meteorites are divided into two main groups: chondrites, which contain small, round chondrules formed from molten droplets in the early solar system, and achondrites, which lack chondrules and are rarer. Stony meteorites often resemble terrestrial rocks, but their extraterrestrial origin can be revealed through their mineral composition, fusion crust, and sometimes magnetic properties due to embedded iron-nickel alloys.

The study of stone meteorites provides valuable insights into the early history of our solar system, as many contain material that predates the formation of Earth itself. Some famous stony meteorites, like the Orgueil meteorite, have even been investigated for traces of organic compounds, fueling speculation about the origins of life. For anyone fascinated by planetary science or the search for our cosmic origins, stone meteorites are a gateway to understanding the building blocks of planets and the processes that shaped our world.

Here we are proud to offer a variety of stone meteorites from around the world including NWA's from Northwest Africa as well as a small collection of rare" Class L/LL 6 Stone Meteorites" named Holbrook Fall which we purchased from an estate in Holbrook, Arizona. Our inventory changes so check back from time to time.