NASA STTR 2019-I Solicitation

Proposal Summary

 19-1- T4.01-2855
 Information Technologies for Intelligent and Adaptive Space Robotics
 Planetary-Scale Surface Feature Detection and Mapping for Future Exploration Missions
Name:  New Rights Group, Inc. DBA Development Seed
Name:  Arizona State University
Street:  1226 9th Street Northwest, Second Floor
Street:  PO Box 876004
City:  Washington
City:  Tempe
State/Zip:  DC 20001-4202
State/Zip:  AZ 85286-6004
PHONE:  (202) 207-0485
PHONE:  (480) 965-7591

Principal Investigator (Name, E-mail, Mail Address, City/State/Zip, Phone)

Tanya Harrison
PO Box 876004 Tempe, AZ 85286 - 6004
(480) 965-7591

Business Official (Name, E-mail, Mail Address, City/State/Zip, Phone)

Dr. Mark Wronkiewicz
1226 9th Street NW, Second Floor Washington, DC 20001 - 4202
(573) 578-1453
Estimated Technology Readiness Level (TRL) :
Begin: 3
End: 8
Technical Abstract (Limit 2000 characters, approximately 200 words)

Accurate navigation is a crucial part of both robotic and crewed exploration of other worlds. For missions to the surfaces of Mars and the Moon, mission planners will require increasingly autonomous guidance systems that support fast, efficient, and agile surface route planning. These navigation systems will rely on access to accurate and regularly updated maps of surface landmarks. In a recent pilot study (Wronkiewicz et al. (2018)), we presented a technique using machine learning to autonomously map surface features (specifically, craters) using satellite images from the Mars Reconnaissance Orbiter (MRO) ConteXt Camera (CTX). Our method could generate accurate crater maps five orders of magnitude faster and at 10x better resolution than the best manual identification efforts. This result suggests we should further explore methods of autonomously generating surface feature maps as a way to reduce the amount of manual effort needed to chart other bodies in the solar system.

We propose building the tools to efficiently map surface features across both the Moon and Mars. Specifically, we will achieve two main technical objectives: (1) create an open-source, cloud-based, reusable software product that can rapidly apply ML algorithms across large image datasets (e.g., satellite images covering the Moon and Mars) and (2) generate publicly available impact crater maps encompassing the entire surface of Mars and the Moon at ten times better resolution than is provided by existing catalogs. We will open source both the software and data products to encourage future research applying ML for planetary-scale mapping. These maps, and the software used to rapidly generate them, will undergird safe and efficient planetary navigation in a manner that exhibits “higher performance and autonomy than currently possible” (NASA STTR T4.01).

Potential NASA Applications (Limit 1500 characters, approximately 150 words)

The two technical objectives proposed are immediately usable by NASA. The proposed software product will help NASA leverage machine learning on the cloud to analyze planetary satellite image datasets (e.g., within the PDS). The proposed map products will provide mission planners with initial global martian and lunar maps. Using these as a foundation, NASA can better explore the mapping of additional surface features and investigate automated navigation systems for future robotic and crewed missions.

Potential Non-NASA Applications (Limit 1500 characters, approximately 150 words)

Machine learning models to detect surface features are applicable to Earth for uses such as monitoring surface changes over time (both natural and anthropogenic). Our model's ability to ingest global datasets and create maps from them could potentially also be applied to map notable features in satellite images of Earth to aid in resource exploration, urban planning, farming. and more.

Duration: 6

Form Generated on 06/16/2019 22:59:53