Huckitta is a famous Australian Pallasite from the Northern Territory, officially classified as Pallasite, PMG-an. A small mass was first found near Alice Springs in 1924, with the much larger main mass recovered at Huckitta Station in 1937. As a Pallasite, Huckitta represents Stony-Iron material containing both iron-nickel metal and olivine, formed over 4.5 billion years ago within an early differentiated asteroid. Its anomalous Main Group classification adds further scientific interest, separating it from more typical PMG Pallasites.

Huckitta specimens are known for their strongly weathered character, with much of the original metal altered during long terrestrial exposure in the Australian environment. Prepared pieces can show a mixture of oxidised metal and olivine-rich material, giving Huckitta a more ancient and earthy appearance than fresher Pallasites. Rather than the bright translucent olivine in clean metal seen in specimens such as Sericho or Esquel, Huckitta often preserves ghostly olivine forms within weathered iron oxides.

Studying Huckitta provides insight into Pallasite formation, core-mantle boundary material, and the long-term weathering of Stony-Iron meteorites on Earth. Its large recovered mass, Australian provenance, and PMG-an classification make it an important and recognisable Pallasite. For collectors, Huckitta offers a classic and historically significant meteorite with a distinctive preservation style and strong scientific appeal. Each specimen represents ancient asteroid material, altered over time into one of the most characteristic weathered Pallasites.