non-chondritic

the meteorite's non-chondritic nature suggested an unusual origin.

scientists analyzed the non-chondritic material to understand early solar system processes.

non-chondritic meteorites often contain refractory inclusions rich in calcium and aluminum.

identifying non-chondritic samples is crucial for understanding planetary formation.

the team focused on non-chondritic inclusions within the larger meteorite.

several non-chondritic types have been classified based on their mineralogy.

the non-chondritic composition differed significantly from typical chondrites.

researchers compared the non-chondritic material to known planetary compositions.

the presence of non-chondritic material supports a complex formation history.

geochronology of non-chondritic samples provides insights into early solar system events.

the study highlighted the importance of non-chondritic meteorites for research.