Description
Polished Stony Magnetic Meteorite from Morocco
This specimen is a polished stony magnetic meteorite of the H chondrite classification, sourced from Morocco. With its metallic inclusions and fine-grained silicate structure, this meteorite offers a remarkable opportunity to own a genuine fragment of space rock. Its polished surface reveals the internal texture and mineral composition that make these meteorites so scientifically and visually fascinating.
Every specimen is a 100% genuine meteorite and comes complete with a Certificate of Authenticity. The photographs show an example of the type and quality you will receive, with a 1cm scale cube included for accurate sizing. Each meteorite has been carefully chosen and prepared to display its natural features to best effect.
Geological and Cosmic Origin
H chondrites are part of the ordinary chondrite group, the most common type of meteorites to fall to Earth, making up approximately 40% of observed meteorite falls. They are believed to have originated from the asteroid belt between Mars and Jupiter, likely from parent bodies that underwent significant heating and differentiation early in the solar system’s history, over 4.5 billion years ago.
The “H” in H chondrite stands for High Iron, a defining characteristic of this type. These meteorites are rich in metallic iron-nickel, which accounts for their magnetic properties. Their composition provides vital insights into the formation of the early solar nebula and the processes that shaped planetesimals before the planets fully formed.
Classification and Composition
- Type: Ordinary Chondrite
- Group: H (High Iron)
- Structure: Chondritic texture, with visible chondrules under magnification
- Minerals Present: Olivine, pyroxene, troilite, and abundant iron-nickel metal
- Magnetic Properties: Strongly magnetic due to high metal content
The polished surface enhances the contrast between the silicate-rich matrix and the reflective metallic grains, making the specimen ideal for both scientific appreciation and display.
Morphological Features
H chondrites are characterised by their chondrules, small spherical inclusions formed from molten droplets in the solar nebula. These are set within a fine-grained matrix containing metallic flakes and veins of iron-nickel alloy. The high iron content gives these meteorites a distinctive weight and density compared to terrestrial rocks.
This polished Moroccan specimen highlights:
- Bright metallic inclusions with strong reflective luster
- A dense, compact structure typical of H chondrites
- A fine balance of silicate minerals and iron-rich phases
Scientific and Collector Importance
H chondrites are crucial for understanding early solar system history. They preserve evidence of the conditions present during planetary formation and are used by planetary scientists to study thermal metamorphism and differentiation in small celestial bodies.
For collectors, polished meteorites are especially desirable as they reveal internal details not visible on natural surfaces. The magnetic properties make them interactive and engaging specimens, while their extraterrestrial origin ensures that each piece is a direct connection to the early solar system.
Display and Aesthetic Value
This Moroccan H chondrite meteorite, polished to a smooth finish, is an eye-catching display piece as well as a scientifically valuable sample. Its reflective metallic grains and dense, stony matrix give it a striking appearance that appeals to enthusiasts, educators, and interior decorators alike.
Each specimen measures within the 30–60mm range, making it perfect for handling, study, or placing in a collection cabinet. Its rarity as a natural space rock ensures that every piece is unique, carrying the history of billions of years from space to Earth.
Owning a polished H chondrite meteorite is more than adding a mineral specimen to a collection—it is possessing a fragment of cosmic history forged in the earliest days of the solar system.
Reviews
There are no reviews yet.