Abstract Lava tubes, a common volcanic feature on terrestrial planets, offer critical insights into lava flow processes and may serve as future potential habitats for space crews and other facilities on the Moon and Mars. Seismic detection of these features is challenging as the irregular morphology and rough cave ceilings and walls generate complex seismic wavefields dominated by strong scattering and reverberation rather than pure reflections. Here we present observations of enhanced backscattering in seismic data collected above terrestrial lava tubes. We show that the spatial and frequency characteristics of wavefield intensity can be related to the dimensions of the lava tubes. Our findings suggest that, when geological indicators such as collapse pits are present, this method would enable mapping lava tubes on Earth and, by proxy, on the Moon and Mars, and that the approach is readily adaptable for future planetary exploration.
Observations from the Little Bunker
Last updated: October 16, 2025 02:57 AM
Atmospheric CO₂
424.4 ppm
+18.2
ppm/year
Atmospheric CH₄
1933.54 ppb
+12.29
ppb/year
Global Temperature
+1.48 °C
Peak: +1.73°C
World Population
8.1 billion
+67
million/year