Eduardo A. Lima

TL;DR: It is shown that dusty olivine-bearing chondrules from the Semarkona meteorite were magnetized in a nebular field of 54 ± 21 microteslas, which implies that background magnetic fields in the terrestrial planet-forming region were likely 5 to 54 microtesla, which is sufficient to account for measured rates of mass and angular momentum transport in protoplanetary disks.

TL;DR: The Planetary Major Equipment Program (NNX15AH72G) as discussed by the authors is a program of the U.S. National Aeronautics and Space Administration (NOAASA).

TL;DR: P paleomagnetic analysis of three angrites found that they record a past magnetic field of ∼10 microteslas on the angrite parent body extending from 4564 to at least 4558 million years ago, extending beyond the expected lifetime of the early circumstellar disk.

TL;DR: It is shown that remanent magnetization in the eucrite meteorite Allan Hills A81001 formed during cooling on Vesta 3.69 billion years ago in a surface magnetic field of at least 2 microteslas, suggesting that Vesta formed an advecting liquid metallic core.

TL;DR: In this article, high resolution maps of the magnetic field of Martian meteorite ALH 84001 have been presented, which suggest that the local paleofield was within an order of magnitude of that of the present-day Earth.