Is this project an undergraduate, graduate, or faculty project?

Undergraduate

Project Type

individual

Campus

Daytona Beach

Authors' Class Standing

Aashman Gupta, Sophomore

Lead Presenter's Name

Aashman Gupta

Lead Presenter's College

DB College of Engineering

Faculty Mentor Name

Dr. Cagri Kilic

Abstract

This project evaluates the feasibility of sustained onboard AI autonomy for a solar-powered Mars rover by directly linking solar energy availability to achievable compute performance. While Mars solar irradiance and edge computing performance have been studied independently, no unified framework currently couples surface power generation to autonomy throughput in an experimentally validated manner. The project will begin with a simulation of solar power generation for a 1 m² rover-mounted array across a Martian sol, accounting for seasonal variation, dust opacity, and array configuration (fixed versus sun-tracking). The resulting power profile will then be coupled to representative compute platforms running autonomy workloads spanning high-, moderate-, and low-compute demand classes, including object detection, visual odometry, and terrain classification. Unlike purely theoretical studies, this work emphasizes hardware testing. Simulated power availability will be replicated in the laboratory using programmable benchtop power supplies to measure real computing throughput, duty cycle, and sustained power draw. The outcome will be a validated feasibility framework that future researchers can use as a baseline reference when designing AI-enabled Mars rover systems.

Did this research project receive funding support (Spark, SURF, Research Abroad, Student Internal Grants, Collaborative, Climbing, or Ignite Grants) from the Office of Undergraduate Research?

No

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Feasibility of High-Throughput Onboard AI for Mars Rovers Under Solar Constraints

This project evaluates the feasibility of sustained onboard AI autonomy for a solar-powered Mars rover by directly linking solar energy availability to achievable compute performance. While Mars solar irradiance and edge computing performance have been studied independently, no unified framework currently couples surface power generation to autonomy throughput in an experimentally validated manner. The project will begin with a simulation of solar power generation for a 1 m² rover-mounted array across a Martian sol, accounting for seasonal variation, dust opacity, and array configuration (fixed versus sun-tracking). The resulting power profile will then be coupled to representative compute platforms running autonomy workloads spanning high-, moderate-, and low-compute demand classes, including object detection, visual odometry, and terrain classification. Unlike purely theoretical studies, this work emphasizes hardware testing. Simulated power availability will be replicated in the laboratory using programmable benchtop power supplies to measure real computing throughput, duty cycle, and sustained power draw. The outcome will be a validated feasibility framework that future researchers can use as a baseline reference when designing AI-enabled Mars rover systems.

 

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