Tektites and impactites are not classified in the same way as meteorites. Meteorites are categorized based on their composition and origin, such as stony, iron, or stony-iron, and further subdivided into groups like chondrites and achondrites (McSween, 1999, "Meteorites and Their Parent Planets").
Tektites, on the other hand, are natural glass objects formed from terrestrial debris ejected during meteorite impacts. They are classified based on their geographic location and physical characteristics, such as splash-form or layered tektites (Koeberl, 1994, "Tektites and Impact Glasses"). Impactites are rocks created or altered by the impact of a meteorite, including shocked rocks and breccias, and are classified based on their formation process and mineralogical changes (French, 1998, "Traces of Catastrophe: A Handbook of Shock-Metamorphic Effects in Terrestrial Meteorite Impact Structures"). While meteorites are primarily studied for their extraterrestrial origin, tektites and impactites are examined for insights into impact processes and Earth's geological history (Melosh, 1989, "Impact Cratering: A Geologic Process"). Understanding these differences is crucial for geologists and planetary scientists in unraveling the complexities of planetary impacts and their effects on Earth's surface.
