Mercury, the innermost planet of our solar system, was named after the swift Roman messenger god, reflecting its rapid orbit around the Sun. Long associated with mystery and extremes, Mercury endures intense heat and violent impacts, preserving an ancient surface that records the earliest history of planetary formation. Yet unlike the Moon or Mars, no meteorite has ever been definitively confirmed to originate from Mercury, making candidate specimens of extraordinary scientific importance.
KG 022 is one such remarkable meteorite. Recovered from the deserts of Tunisia, its highly unusual mineral composition differs from typical meteorites and closely resembles surface materials measured on Mercury by spacecraft missions. These rare chemical characteristics, formed under highly reducing conditions, have led some researchers to propose that KG 022 may represent material ejected from Mercury’s surface by a massive impact billions of years ago.
Although its Mercurian origin cannot be confirmed with certainty, KG 022 remains one of the most compelling candidates identified to date. As an ungrouped achondrite of extreme rarity, it represents a fragment of a planetary body formed at the dawn of the solar system, offering a rare and tangible connection to one of its most elusive worlds.