The Radio-wave Observations at the Lunar Surface of the Photoelectron Sheath (ROLSES) instrument onboard the Intuitive Machines-1 Mission to the Moon

The Radio-wave Observations at the Lunar Surface of the photoElectron Sheath (ROLSES) instrument is a radio telescope system designed to characterize the radio and plasma wave environment of the near-side lunar surface at frequencies between 2 kHz and 30 MHz. The ROLSES sensor consists of a set of four 2.5 meter radio monopole antennas onboard the Intuitive Machines-(IM-1) lander, Odysseus. The antennas were stowed during launch to be deployed after landing on the lunar surface using a frangibolt mechanism. The frequency range is well suited to observing radio waves at frequencies below 15 MHz that cannot be observed from Earth due to the ionospheric cutoff. The higher frequencies are helpful in cross-calibrating with ground-based observations. Radio waves from the Sun, the Milky Way galaxy, Jupiter, Earths auroral region, and ground-based radio transmitters were expected to be present on the lunar surface. In addition, local plasma fluctuations and lunar/interplanetary dust were expected to produce detectable radio signals. Radio data from each of the 4 antennas, after passing through an isolating pre-amp and signal conditioning analog electronics, are digitized to 14 bits at 120 mega samples per second and then digitally processed by a Field Programmable Gate Array (FPGA) that performs onboard spectral analysis via a Fast Fourier Transform (FFT). Time-averaged spectral values are then stored and returned. ROLSES science data are sent to the lander at ~ 16 kb/s and subsequently downlinked for further processing. Also telemetered to Earth are raw waveforms (unprocessed time sequence data) that are useful in studying dust impact on ROLSES antennas. ROLSES data are sent to the lander and subsequently downlinked for further processing. ROLSES is part of NASA's Commercial Lunar Payload Services (CLPS) program. Odysseus landed close to the south pole at Malapert A (~80S). This paper describes the complete design and operations of the ROLSES instrument and presents initial observations. Despite the tilted landing of Odysseus, we were able to successfully command, deploy the antennas, and operate the instrument in transit and on the lunar surface. We also describe an enhanced version of this instrument (ROLSES 2) currently under development.

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Publication Details

Journal
Journal of Astronomical Instrumentation
Published
2026-07-24
DOI
https://doi.org/10.1142/s2251171726500078
Primary Topic
Planetary Science and Exploration
Type
article
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article

The Radio-wave Observations at the Lunar Surface of the Photoelectron Sheath (ROLSES) instrument onboard the Intuitive Machines-1 Mission to the Moon

Igor Kleyner, Joshua J. Hibbard, Pietro A. Sparacino, S. Yashiro et al.
Journal of Astronomical Instrumentation
Planetary Science and Exploration
article

The Radio-wave Observations at the Lunar Surface of the Photoelectron Sheath (ROLSES) instrument onboard the Intuitive Machines-1 Mission to the Moon

Igor Kleyner, Joshua J. Hibbard, Pietro A. Sparacino, S. Yashiro, Damon Bradley, W. M. Farrell, N. Gopalswamy, Scott D. Murphy, Richard B. Katz, Michael Choi, Pertti Makela, Robert J. MacDowall, Thomas M. Schluszas, Richard C. Mills, Victor Gonzalez-Leon, Jack O. Burns, Chimaobi Onyeachu, Scott A. Boardsen
article en

Abstract

The Radio-wave Observations at the Lunar Surface of the photoElectron Sheath (ROLSES) instrument is a radio telescope system designed to characterize the radio and plasma wave environment of the near-side lunar surface at frequencies between 2 kHz and 30 MHz. The ROLSES sensor consists of a set of four 2.5 meter radio monopole antennas onboard the Intuitive Machines-(IM-1) lander, Odysseus. The antennas were stowed during launch to be deployed after landing on the lunar surface using a frangibolt mechanism. The frequency range is well suited to observing radio waves at frequencies below 15 MHz that cannot be observed from Earth due to the ionospheric cutoff. The higher frequencies are helpful in cross-calibrating with ground-based observations. Radio waves from the Sun, the Milky Way galaxy, Jupiter, Earths auroral region, and ground-based radio transmitters were expected to be present on the lunar surface. In addition, local plasma fluctuations and lunar/interplanetary dust were expected to produce detectable radio signals. Radio data from each of the 4 antennas, after passing through an isolating pre-amp and signal conditioning analog electronics, are digitized to 14 bits at 120 mega samples per second and then digitally processed by a Field Programmable Gate Array (FPGA) that performs onboard spectral analysis via a Fast Fourier Transform (FFT). Time-averaged spectral values are then stored and returned. ROLSES science data are sent to the lander at ~ 16 kb/s and subsequently downlinked for further processing. Also telemetered to Earth are raw waveforms (unprocessed time sequence data) that are useful in studying dust impact on ROLSES antennas. ROLSES data are sent to the lander and subsequently downlinked for further processing. ROLSES is part of NASA's Commercial Lunar Payload Services (CLPS) program. Odysseus landed close to the south pole at Malapert A (~80S). This paper describes the complete design and operations of the ROLSES instrument and presents initial observations. Despite the tilted landing of Odysseus, we were able to successfully command, deploy the antennas, and operate the instrument in transit and on the lunar surface. We also describe an enhanced version of this instrument (ROLSES 2) currently under development.

Journal of Astronomical Instrumentation
Openalex Percentile: Top 10%
Planetary Science and Exploration
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