EGU24-8912, updated on 08 Mar 2024
https://doi.org/10.5194/egusphere-egu24-8912
EGU General Assembly 2024
© Author(s) 2024. This work is distributed under
the Creative Commons Attribution 4.0 License.

Laser Ranging Interferometry for the next gravity missions

Vitali Müller1,2, Pallavi Bekal1,2, Malte Misfeldt1,2, Laura Müller1,2, Reshma Sudha1,2, Martin Weberpals1,2, Kolja Nicklaus3, Kai Voss3, and Gerhard Heinzel1,2
Vitali Müller et al.
  • 1Max-Planck-Institute for Gravitational Physics, Hannover, Germany (vitali.mueller@aei.mpg.de)
  • 2Institute for Gravitational Physics, Leibniz Universität Hannover, Germany
  • 3Spacetech GmbH, Immenstaad, Germany

The Laser Ranging Interferometer (LRI) on board the GRACE Follow-On spacecraft has successfully demonstrated for the first time interferometric laser ranging between satellites with a noise level below 1 nm/rtHz. In addition, the LRI’s steering mirror information provides attitude information that enable inter-comparisons with the conventional star cameras. Two new twin-satellite missions are now under development: the Next Generation Gravity Mission (NGGM) by ESA and the GRACE-C mission by a US-German partnership. Both missions rely on laser interferometry as the primary and only means of measuring the distance variations between the spacecraft.

In this presentation, we introduce the measurement concept and design principles, report on the current status of the ranging instruments and explain the changes to be implemented with respect to GRACE-FO, mainly related to redundancy and lessons learned.

How to cite: Müller, V., Bekal, P., Misfeldt, M., Müller, L., Sudha, R., Weberpals, M., Nicklaus, K., Voss, K., and Heinzel, G.: Laser Ranging Interferometry for the next gravity missions, EGU General Assembly 2024, Vienna, Austria, 14–19 Apr 2024, EGU24-8912, https://doi.org/10.5194/egusphere-egu24-8912, 2024.