Active seismic exploration along a human lunar mission traverse analogue in the San Francisco volcanic field

Author:

Bell Ernest12,Schmerr Nicholas1,Porter Ryan3,Bleacher Jacob4,Young Kelsey2,Huang Mong-Han1,Lekic Vedran1,Pettit Donald5

Affiliation:

1. University of Maryland, College Park, Maryland, USA..

2. NASA, Goddard Spaceflight Center, Greenbelt, Maryland, USA..

3. Northern Arizona University, School of Earth Sciences and Environmental Sustainability, Flagstaff, Arizona, USA..

4. NASA, Washington D.C., USA..

5. NASA, Johnson Space Center, Houston, Texas, USA..

Abstract

Lunar surface activities during Apollo and terrestrial analogue lunar mission simulations have commonly focused on traverses that prioritize surface observations and sample collection activities. Along the way, geophysical measurements are often made. However, they are not necessarily made in a way that optimizes information about the physical subsurface properties, which is something that geophysics can provide. In 2010, NASA simulated a high-quality multiweek human lunar rover traverse analogue mission in the San Francisco volcanic field in Arizona. The traverse route and associated science station locations were selected based on addressing surface observation and sampling tasks. Geophysical studies were not included in the simulation. We returned to the same field area and obtained data on 19 active seismic refraction geophone lines from the science station locations accessed during the simulation. We analyzed the data to calculate 1D seismic velocity profiles for each of the lines. Results revealed up to seven distinct seismically defined material types, including a nearly ubiquitous veneer of regolith of variable thickness at the surface. Results also provided depth and thickness of the seven material types in the first 60 m of the subsurface at each of the science station locations. These cannot be obtained by geologic observations of the outcrops. Systematic interpretation of the area's overall subsurface stratigraphy was not feasible due to the geophysically nonsystematic nature of the original traverse's prioritization of the science station locations. The added geophysical understanding of a region could drive additional geologic investigations to locate samples of otherwise unknown material through the location of surface exposures or coring. This emphasizes the importance of synchronizing geologic and geophysical research requirements during lunar traverse planning and execution to optimize addressing scientific and utilization questions.

Funder

NASA PSTAR

NASA SSERVI GEODES

Publisher

Society of Exploration Geophysicists

Subject

Geology,Geophysics

Reference41 articles.

1. K–Ar Study of the S.P. Flow

2. Bell, E., N. C. Schmerr, J. E. Bleacher, R. C. Porter, K. Young, J. A. Richardson, J. D. West, S. Rees, and D. R. Pettit, 2018, Using earth analogs of the moon to study volcanic fields and prepare for human lunar geophysical exploration: Presented at the Fall Meeting, AGU.

3. Bleacher, J. E., D. B. Eppler, D. H. Needham, C. A. Evans, J. A. Skinner, and W. Feng, 2015, Geologic investigations spurred by analog testing at the 7504 Cone-SP Mountain area of the San Francisco volcanic field: Presented at the Fall Meeting, AGU.

4. Recurrence rates of basaltic volcanism in SP cluster, San Francisco volcanic field, Arizona

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