Published August 7, 2024 | Version v1
Journal article Open

Feasibility of keeping Mars warm with nanoparticles

  • 1. Northwestern University
  • 2. University of Chicago
  • 3. University of Central Florida

Description

One-third of Mars' surface has shallow-buried H2O, but it is currently too cold for use by life. Proposals to warm Mars using greenhouse gases require a large mass of ingredients that are rare on Mars' surface. However, we show here that artificial aerosols made from materials that are readily available at Mars—for example, conductive nanorods that are ~9 micrometers long—could warm Mars >5 × 103 time smore effectively than the best gases. Such nanoparticles forward-scatter sunlight and efficiently block upwelling thermal infrared. Like the natural dust of Mars, they are swept high into Mars' atmosphere, allowing delivery from the near-surface. For a 10-year particle lifetime, two climate models indicate that sustained release at 30 liters per second would globally warm Mars by ≳30 kelvin and start to melt the ice. Therefore, if nanoparticles can be made at scale on (or delivered to) Mars, then the barrier to warming of Mars appears to be less high than previously thought.

Data availability

All data needed to evaluate the conclusions in the paper are present in the paper and/or the Supplementary Materials. Additional data, for example, full 3D climate model output files, are stored at Zenodo (doi: 10.5281/zenodo.8352416). FDTD: 3D Electromagnetic Simulator is commercial code (Lumerical). The MarsWRF source code can be made available by Aeolis Research pending scientific review and a completed Rules of the Road agreement. Requests for the MarsWRF source code should be submitted to mir@aeolisresearch.com.

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Additional details

Identifiers

DOI
10.1126/sciadv.adn4650
Other
oai:uchicago.tind.io:13094

UChicago Information

Division(s)
Physical Sciences Division
Department(s)
Geophysical Sciences