The surface gravity on Mars is smaller than the surface gravity on Earth, resulting in longer falling times. This effect can be simulated on Earth by taking advantage of air resistance and buoyancy, which cause low density objects to fall slowly enough to approximate objects falling on the surface of Mars. We describe a computer simulation based on an experiment that approximates Martian gravity, and verify our numerical results by performing the experiment.
@article{arxiv.1602.06858,
title = {Demonstrating Martian Gravity},
author = {Patrik Pirkola and Patrick B. Hall},
journal= {arXiv preprint arXiv:1602.06858},
year = {2016}
}