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PreprintCC BY 4.0arXiv

Solar System Surface Technosignatures: Searching for Signs of Artificial Design on Extraterrestrial Terrain

Abstract

Artificial radio emissions have historically been a major focus of technosignature searches. Here, we apply an anthropological lens to expand this scope to surface technosignatures: non-random, intentional patterning on planetary terrain, similar to long-lasting human-made landscapes and monuments on Earth. On geologically inactive bodies such as the Moon and Mars, artificial traces and patterns could potentially remain visible for hundreds of millions of years. We discuss two recent developments that make this search timely: high-resolution imaging datasets, such as those produced by the HiRISE camera on the Mars Reconnaissance Orbiter (MRO), and ML-based anomaly-detection methods. Finally, we list two possible approaches to developing a model capable of searching for these surface technosignatures: a supervised and an unsupervised one. Complemented by LiDAR, ground-penetrating radar, and reflectance spectroscopy, these methods would enable the first quantitative upper limits on surface technosignatures while yielding ancillary benefits for planetary science.

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BibTeX
@misc{henrique2026solar,
  title = {{Solar System Surface Technosignatures: Searching for Signs of Artificial Design on Extraterrestrial Terrain}},
  author = {Ana Henrique and Sofia Sheikh and Benjamin Fields},
  howpublished = {arXiv},
  year = {2026},
  month = oct,
  doi = {10.48550/arxiv.2610.28687},
  eprint = {2610.28687},
  archivePrefix = {arXiv},
  url = {https://arxiv.org/abs/2610.28687},
  note = {CC BY 4.0},
}
RIS
TY  - UNPB
TI  - Solar System Surface Technosignatures: Searching for Signs of Artificial Design on Extraterrestrial Terrain
AU  - Ana Henrique
AU  - Sofia Sheikh
AU  - Benjamin Fields
PY  - 2026
DA  - 2026/10/20
PB  - arXiv
DO  - 10.48550/arxiv.2610.28687
UR  - https://arxiv.org/abs/2610.28687
AB  - Artificial radio emissions have historically been a major focus of technosignature searches. Here, we apply an anthropological lens to expand this scope to surface technosignatures: non-random, intentional patterning on planetary terrain, similar to long-lasting human-made landscapes and monuments on Earth. On geologically inactive bodies such as the Moon and Mars, artificial traces and patterns could potentially remain visible for hundreds of millions of years. We discuss two recent developments that make this search timely: high-resolution imaging datasets, such as those produced by the HiRISE camera on the Mars Reconnaissance Orbiter (MRO), and ML-based anomaly-detection methods. Finally, we list two possible approaches to developing a model capable of searching for these surface technosignatures: a supervised and an unsupervised one. Complemented by LiDAR, ground-penetrating radar, and reflectance spectroscopy, these methods would enable the first quantitative upper limits on surface technosignatures while yielding ancillary benefits for planetary science.
ER  -