Spacek, J., Alpern, H., Dineen, T., Petkowski, J.J., Rizzo, G., Benner, S.A., Lui, M., Cockell, C., Eubanks, M., Schulze-Makuch, D., Temby, C., Richburg, M.
Astrobiology (2026) PMID: 42489219, doi: 10.1177/15311074261471218
The International Mars Prospecting Ride-Share System (IMPRESS) is
presented here as a scalable, democratized, and low-cost mission
architecture for distributed measurements on the martian surface and in
the shallow subsurface. IMPRESS is intended to prospect on Mars in
advance of sample return and human exploration. Its primary objective is
to survey Mars for extant life, but it also supports geophysical, soil
chemistry, resource, and landing-site risk assessments. Instead of
relying on soft landers and drilling systems, IMPRESS deploys swarms of
planetary penetrators that use descent kinetic energy to emplace
instruments 0.2-1 m below the surface. This architecture provides
spatial coverage, measurement replication, and mission redundancy. This
increases the chance of detecting unevenly distributed biosignatures and
gives negative results stronger context. Small penetrator platforms
with standardized design, power, and communication interfaces lower the
cost per experiment. The probes operate as independent nodes within a
network, which enables time-correlated atmospheric, seismic, and
environmental measurements that support the broader Mars exploration
campaign. Repeatable mission deployments can range from small rideshare
implementations with tens of penetrators to larger dedicated campaigns
with hundreds or more. We describe the IMPRESS mission architecture,
penetrator platforms, compatible payload classes, and how distributed
shallow-subsurface surveys reduce scientific and operational uncertainty
before future Mars surface activities.