Neural 3D Reconstruction of Planetary Surfaces from Descent-Phase Wide-Angle Imagery

arXiv cs.CV / 4/16/2026

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Key Points

  • The paper addresses the challenge of generating accurate 3D digital elevation models of planetary surfaces using wide-angle imagery captured during spacecraft descent, where radial distortion is strong and parallax is limited.
  • It proposes a “first study” of applying modern neural reconstruction methods specifically to descent-phase planetary imaging, motivated by the shortcomings of conventional multi-view stereo in this setting.
  • The approach introduces an explicit neural height-field representation that encodes domain priors, leveraging the typical continuity, smoothness, solidity, and lack of floating objects on planetary surfaces.
  • Experiments on simulated lunar and Mars descent sequences show improved spatial coverage while retaining satisfactory depth/accuracy compared with traditional multi-view stereo baselines.
  • Overall, the work argues that neural methods can serve as a competitive, potentially low-cost alternative to standard MVS pipelines for planetary terrain reconstruction.

Abstract

Digital elevation modeling of planetary surfaces is essential for studying past and ongoing geological processes. Wide-angle imagery acquired during spacecraft descent promises to offer a low-cost option for high-resolution terrain reconstruction. However, accurate 3D reconstruction from such imagery is challenging due to strong radial distortion and limited parallax from vertically descending, predominantly nadir-facing cameras. Conventional multi-view stereo exhibits limited depth range and reduced fidelity under these conditions and also lacks domain-specific priors. We present the first study of modern neural reconstruction methods for planetary descent imaging. We also develop a novel approach that incorporates an explicit neural height field representation, which provides a strong prior since planetary surfaces are generally continuous, smooth, solid, and free from floating objects. This study demonstrates that neural approaches offer a strong and competitive alternative to traditional multi-view stereo (MVS) methods. Experiments on simulated descent sequences over high-fidelity lunar and Mars terrains demonstrate that the proposed approach achieves increased spatial coverage while maintaining satisfactory estimation accuracy.