Identification of Magnetite in B-type Asteroids

TL;DR

This study uses infrared spectroscopy to identify magnetite and phyllosilicates in B-type asteroids, indicating past aqueous alteration and water incorporation in these rare objects.

Contribution

It provides the first spectroscopic evidence linking magnetite and hydrated minerals to B-type asteroids, suggesting aqueous alteration history.

Findings

Detection of a 1-micron absorption band matching magnetite.

Observation of a 2.9-micron feature indicating phyllosilicates.

Evidence that some B-type asteroids contain water-related minerals.

Abstract

Spectrally blue (B-type) asteroids are rare, with the second discovered asteroid Pallas being the largest and most famous example. We conducted a focused, infrared spectroscopic survey of B-type asteroids to search for water-related features in these objects. Our results show that the negative optical spectral slope of some B-type asteroids is due to the presence of a broad absorption band centered near 1.0 micron. The 1-micron band can be matched in position and shape using magnetite (Fe3O4), which is an important indicator of past aqueous alteration in the parent body. Furthermore, our observations of B-type asteroid (335) Roberta in the 3-micron region reveal an absorption feature centered at 2.9 micron, which is consistent with the absorption due to phyllosilicates (another hydration product) observed in CI chondrites. The new observations suggest that at least some B-type asteroids are likely to have incorporated significant amounts of water ice and to have experienced intensive aqueous alteration.