EGU24-13552, updated on 09 Mar 2024
https://doi.org/10.5194/egusphere-egu24-13552
EGU General Assembly 2024
© Author(s) 2024. This work is distributed under
the Creative Commons Attribution 4.0 License.

Ground magnetic survey on Mars from theZhurong rover

Aimin Du, Yasong Ge, Huapei Wang, Ying Zhang, and Hao Luo
Aimin Du et al.
  • Institute of Geology and Geophysics, Chinese Academy of Sciences, Beijing, China, Space physics, Beijing, China (amdu@mail.iggcas.ac.cn)

Mars’ magnetic field has been measured at large scale by orbiting spacecraft and at very small scale via Martian meteorites. Here we report on a ground magnetic survey on metre to kilometre scales. The Zhurong rover made vector measurements at 16 sites along a 1,089 m track in the Utopia Basin on Mars. It recorded an extremely weak magnetic field, with an order of the average intensity less than that inferred from orbit, in contrast to the large magnetic field in Elysium Planitia measured by InSight. A spacecraft measurement samples an area with radius comparable to its altitude, while a ground measurement samples an area with radius comparable to the depth of the magnetized body. The weak magnetic field measured by Zhurong indicates no magnetization anomalies for a depth of many kilometres around and below the rover’s traverse. We suggest two possible explanations for the weak magnetic field: the entire Utopia Basin may have remained unmagnetized since its formation about 4 billion years ago or that the 5-km-radius ghost crater where Zhurong landed may have been been demagnetized by impact.

How to cite: Du, A., Ge, Y., Wang, H., Zhang, Y., and Luo, H.: Ground magnetic survey on Mars from theZhurong rover, EGU General Assembly 2024, Vienna, Austria, 14–19 Apr 2024, EGU24-13552, https://doi.org/10.5194/egusphere-egu24-13552, 2024.