Most, but by not all meteorites contain iron.
They are classified into three main types: stony, iron, and stony-iron meteorites.
The presence of iron in meteorites is significant for understanding the formation and differentiation of planetary bodies. Iron meteorites provide insights into the core formation processes, while stony meteorites help scientists study the early solar system's conditions. Research from institutions like the University of Arizona's Lunar and Planetary Laboratory and publications in journals such as 'Meteoritics & Planetary Science' offer detailed analyses of meteorite compositions and their implications for planetary science.
In summary, while not all meteorites contain iron, those that do offer valuable information about the solar system's history and the processes that shaped planetary bodies. Understanding the diverse compositions of meteorites is crucial for advancing our knowledge of planetary formation and evolution.