Open AccessThe Incorporation of Field Portable Instrumentation Into Human Planetary Surface Exploration
Author(s) -
Young K. E.,
Bleacher J. E.,
Rogers A. D.,
Schmitt H. H.,
McAdam A. C.,
Garry W. B.,
Whelley P. L.,
Scheidt S. P.,
Ito G.,
Knudson C. A.,
Graff T. G.,
Bleacher L. V.,
Whelley N.,
Evans C. A.,
Hurtado J. M.,
Glotch T. D.
Publication year - 2018
Publication title -
earth and space science
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 0.843
H-Index - 23
ISSN - 2333-5084
DOI - 10.1029/2018ea000378
Subject(s) - instrumentation (computer programming) , timeline , software deployment , remote sensing , planetary exploration , scientific instrument , planetary surface , systems engineering , computer science , space exploration , aerospace engineering , software , earth science , geology , astrobiology , engineering , mars exploration program , physics , geography , software engineering , archaeology , quantum mechanics , programming language , operating system
Field portable instrumentation, such as in situ geochemical analyzers or broader field of view instruments like multispectral imagers or other imaging capabilities, has the potential to dramatically increase the science return of a planetary surface exploration mission. However, more work is needed to determine how emerging portable technologies should be designed and implemented into evolving mission architectures. This work summarizes the efforts of the RIS 4 E (Remote, In Situ and Synchrotron Studies for Science and Exploration) SSERVI (Solar System Exploration Research Virtual Institute) team in investigating how field portable instruments should be including into planning for future exploration EVAs (extravehicular activities). EVA crews of geologists and astronauts tested a variety of portable and handheld technologies at both the December 1974 lava flow, Kilauea Volcano, Hawai'i, and Kilbourne Hole, New Mexico, both of which are planetary analog sites. The timeline data gathered during instrument deployment were then mapped onto EVA timelines used in large‐scale NASA planetary surface exploration analog missions. Results and recommendations for future instrument hardware and software development are discussed, as is the operational framework necessary for incorporating in situ analytical capabilities into future planetary surface exploration.