Abstract
The objective of the Psyche Magnetometry Investigation is to test the
hypothesis that asteroid (16) Psyche formed from the core of a
differentiated planetesimal. To address this, the Psyche Magnetometer
will measure the magnetic field around the asteroid to search for
evidence of remanent magnetization. Paleomagnetic measurements of
meteorites and dynamo theory indicate that a diversity of planetesimals
once generated dynamo magnetic fields in their metallic cores. Likewise,
the detection of a strong magnetic moment (>2×1014 Am2)
at Psyche would likely indicate that the body once generated a core
dynamo, implying that it formed by igneous differentiation. The Psyche
Magnetometer consists of two three-axis fluxgate Sensor Units (SUs)
mounted 0.7 m apart along a 2.15-m long boom and connected to two
Electronics Units (EUs) located within the spacecraft bus. The
Magnetometer samples at up to 50 Hz, has a range of ±80,000 nT, and an instrument noise of 39 pTaxis−13σ
integrated over 0.1 to 1 Hz. The two pairs of SUs and EUs provide
redundancy and enable gradiometry measurements to suppress noise from
flight system magnetic fields. The Magnetometer will be powered on soon
after launch and acquire data for the full duration of the mission. The
ground data system processes the Magnetometer measurements to obtain an
estimate of Psyche’s dipole moment.
Original language | English |
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Article number | 22 |
Journal | Space Science Reviews |
Volume | 219 |
Issue number | 22 |
Number of pages | 47 |
ISSN | 0038-6308 |
DOIs | |
Publication status | Published - 2023 |