Although Mars today does not have a core dynamo, magnetizations in the
Martian crust and meteorites suggest a magnetic field was present prior
to 3.7 billion years (Ga) ago. However, the lack of ancient, oriented
Martian bedrock samples available on Earth has prevented accurate
estimates of the dynamo’s intensity, lifetime, and direction.
Constraining the nature and lifetime of the dynamo are vital to
understanding the evolution of the Martian interior and the potential
habitability of the planet. The Perseverance rover, which is exploring
Jezero crater, is providing an unprecedented opportunity to address this
gap by acquiring absolutely oriented bedrock samples with estimated ages
from ~2.3 to > 4.1 Ga. As a first step in
establishing whether these samples could contain records of Martian
paleomagnetism, it is important to determine their ferromagnetic
mineralogy, the grain sizes of the phases, and the form of any natural
remanent magnetization. Here, we synthesize data from various
Perseverance instruments to achieve those goals and discuss the
implications for future laboratory paleomagnetic analyses. Using the
rover’s instrument payload, we find that cored samples likely contain
iron oxides enriched in Cr and Ti. The relative proportions of Fe, Ti,
and Cr indicate that the phases may be titanomagnetite or Fe-Ti-Cr
spinels that are ferromagnetic at room temperature, but we cannot rule
out the presence of non-ferromagnetic ulvöspinel, ilmenite, and chromite
due to signal mixing. Importantly, the inferred abundance of iron oxides
in the samples suggests that even <1 mm-sized samples will be
easily measurable by present-day magnetometers.