Peter Lehner, Ryosuke Sakagami, W. Boerdijk, Andreas Dömel, M. Durner, Giacomo Franchini, A. Prince, Kristin Lakatos, David Lennart Risch, Lukas Meyer, B. Vodermayer, E. Dietz, S. Frohmann, F. Seel, Susanne Schröder, H. Hübers, A. Albu-Schäffer, A. Wedler
{"title":"行星探测用激光诱导击穿光谱仪的移动操作","authors":"Peter Lehner, Ryosuke Sakagami, W. Boerdijk, Andreas Dömel, M. Durner, Giacomo Franchini, A. Prince, Kristin Lakatos, David Lennart Risch, Lukas Meyer, B. Vodermayer, E. Dietz, S. Frohmann, F. Seel, Susanne Schröder, H. Hübers, A. Albu-Schäffer, A. Wedler","doi":"10.1109/AERO55745.2023.10115597","DOIUrl":null,"url":null,"abstract":"Laser-induced Breakdown Spectroscopy(LIBS) is an established analytical technique to measure the elemental composition of rocks and other matter on the Martian surface. We propose an autonomous in-contact sampling method based on an attachable LIBS instrument, designed to measure the composition of samples on the surface of planets andmoons. Thespectrometer module is picked up by our LightweightRover Unit(LRU) at the landing site and transported to the sampling location, where the manipulator establishes a solid contact be-tween the instrument and the sample. The rover commands the instrument to trigger the measurement, which in turn releases a laser-pulse and captures the spectrum of the resulting plasma. The in-contact deployment ensures a suitable focus distance for the spectrometer, without a focusing system that would add to the instrument's volume and weight, and allows for flexible deployment of the instrument. The autonomous software com-putes all necessary manipulation operations on-board the rover and requires almost no supervision from mission control. We tested the LRU and the LIBS instrument at the moon analogue test site on Mt. Etna, Sicily and successfully demonstrated multiple LIBS measurements, in which the rover automatically deployed the instrument on a rock sample, recorded a measure-ment and sent the data to mission control, with sufficient quality to distinguish the major elements of the recorded sample.","PeriodicalId":344285,"journal":{"name":"2023 IEEE Aerospace Conference","volume":"33 7-8 1","pages":"0"},"PeriodicalIF":0.0000,"publicationDate":"2023-03-04","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"2","resultStr":"{\"title\":\"Mobile Manipulation of a Laser-induced Breakdown Spectrometer for Planetary Exploration\",\"authors\":\"Peter Lehner, Ryosuke Sakagami, W. Boerdijk, Andreas Dömel, M. Durner, Giacomo Franchini, A. Prince, Kristin Lakatos, David Lennart Risch, Lukas Meyer, B. Vodermayer, E. Dietz, S. Frohmann, F. Seel, Susanne Schröder, H. Hübers, A. Albu-Schäffer, A. 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Mobile Manipulation of a Laser-induced Breakdown Spectrometer for Planetary Exploration
Laser-induced Breakdown Spectroscopy(LIBS) is an established analytical technique to measure the elemental composition of rocks and other matter on the Martian surface. We propose an autonomous in-contact sampling method based on an attachable LIBS instrument, designed to measure the composition of samples on the surface of planets andmoons. Thespectrometer module is picked up by our LightweightRover Unit(LRU) at the landing site and transported to the sampling location, where the manipulator establishes a solid contact be-tween the instrument and the sample. The rover commands the instrument to trigger the measurement, which in turn releases a laser-pulse and captures the spectrum of the resulting plasma. The in-contact deployment ensures a suitable focus distance for the spectrometer, without a focusing system that would add to the instrument's volume and weight, and allows for flexible deployment of the instrument. The autonomous software com-putes all necessary manipulation operations on-board the rover and requires almost no supervision from mission control. We tested the LRU and the LIBS instrument at the moon analogue test site on Mt. Etna, Sicily and successfully demonstrated multiple LIBS measurements, in which the rover automatically deployed the instrument on a rock sample, recorded a measure-ment and sent the data to mission control, with sufficient quality to distinguish the major elements of the recorded sample.