阿波罗17号空间站的摄影测量3D重建:从巨石到月球岩石样本集成到虚拟现实中

IF 1.8 4区 物理与天体物理 Q3 ASTRONOMY & ASTROPHYSICS
S. Le Mouélic , M. Guenneguez , H.H. Schmitt , L. Macquet , N. Mangold , G. Caravaca , B. Seignovert , E. Le Menn , L. Lenta
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引用次数: 0

摘要

1972年,阿波罗17号宇航员花了三天时间探索月球上的金牛座利特罗山谷。在他们的第三次舱外活动中,他们在6号站呆了1个多小时,6号站是一个地质航路点,由一块从北地块滚下来的巨石的三个大碎片和两个小碎片组成。我们使用了宇航员在6号空间站拍摄的所有可用的扫描数字阿波罗照片来计算一个全面的探索区域的3D模型。我们使用了动态摄影测量的结构,利用它们的重叠来自动导出154张可用图像中的每一张的位置。所有图像都在一个单独的摄影测量项目中对齐,这一方面允许在他们的调查过程中自动可视化宇航员的位置,另一方面可以在3D中重建三个主要的巨石,因此限制了它们各自的大小和方向。除了巨石外,我们还表明,通过摄影测量的3D重建也可以应用于巨石本身的岩石样本。这些样本在70年代被带回地球时,在LPI从多个角度系统地拍摄了下来。为了进行重建,我们使用16个立体对的扫描存档图像,计算样品76015、76215、76315和76275的三维模型。这些模型可能起到保存的作用,因为一些样品,后锯为分析,不再以其原始形式存在。然后,可以在一个基于网络的平台上对巨石和岩石样本的3D模型进行操作和可视化。3D模型也被集成到虚拟现实场景中,以便以沉浸式和协作的方式全面调查其属性。例如,直接了解样品在其环境中的位置和方向可能为更好地理解微陨石撞击和太阳风粒子引起的空间风化变化等过程提供额外的限制。利用漫游者和/或宇航员拍摄的图像进行三维摄影测量重建,可能是即将到来的月球任务中考虑的基本技术之一,以最大限度地提高他们的科学、教育和外展回报。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Photogrammetric 3D reconstruction of Apollo 17 Station 6: From boulders to lunar rock samples integrated into virtual reality

Apollo 17 astronauts spent three days exploring the Taurus Littrow Valley on the Moon in 1972. During their third Extravehicular Activity, they spent more than 1 h at Station 6, a geologic waypoint consisting of three big and two small fragments of a boulder that rolled down the North massif. We have used all the available scanned digital Apollo photos taken by the astronauts at this Station 6 to compute a comprehensive 3D model of the explored area. We used Structure From Motion photogrammetry to automatically derive the position of each of the 154 available images using their overlap. All images were aligned in a single photogrammetric project, which allows on one hand to automatically visualize the astronaut positions during their investigations, and on the other hand to reconstruct in 3D the three main pieces of boulders, therefore constraining their respective size and orientation. In addition to the boulders, we show that the 3D reconstruction by photogrammetry can also be applied to the rock samples taken from the boulders themselves. These samples were systematically photographed from multiple angles at the LPI during the 70s when brought back to Earth. For the reconstruction, we used scanned archived images representing 16 stereoscopic pairs, to compute 3D models of samples 76015, 76215, 76315 and 76275. These models might play a role in preservation as some of the samples, latter sawed for analysis, do not exist anymore in their pristine form. 3D models of the boulders and rock samples can then be manipulated and visualized on a web-based platform. 3D models have also been integrated into a virtual reality scene in order to provide the possibility to investigate their properties at full scale in an immersive and collaborative way. The knowledge of the samples position and orientation directly in their context might for example provide additional constrains to better understand processes such as the space weathering alteration due to micrometeorite impacts and solar wind particle. 3D photogrammetric reconstructions using images taken by rovers and/or astronauts might be one of the basic techniques to consider in forthcoming lunar missions in order to maximize their scientific, educational and outreach return.

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来源期刊
Planetary and Space Science
Planetary and Space Science 地学天文-天文与天体物理
CiteScore
5.40
自引率
4.20%
发文量
126
审稿时长
15 weeks
期刊介绍: Planetary and Space Science publishes original articles as well as short communications (letters). Ground-based and space-borne instrumentation and laboratory simulation of solar system processes are included. The following fields of planetary and solar system research are covered: • Celestial mechanics, including dynamical evolution of the solar system, gravitational captures and resonances, relativistic effects, tracking and dynamics • Cosmochemistry and origin, including all aspects of the formation and initial physical and chemical evolution of the solar system • Terrestrial planets and satellites, including the physics of the interiors, geology and morphology of the surfaces, tectonics, mineralogy and dating • Outer planets and satellites, including formation and evolution, remote sensing at all wavelengths and in situ measurements • Planetary atmospheres, including formation and evolution, circulation and meteorology, boundary layers, remote sensing and laboratory simulation • Planetary magnetospheres and ionospheres, including origin of magnetic fields, magnetospheric plasma and radiation belts, and their interaction with the sun, the solar wind and satellites • Small bodies, dust and rings, including asteroids, comets and zodiacal light and their interaction with the solar radiation and the solar wind • Exobiology, including origin of life, detection of planetary ecosystems and pre-biological phenomena in the solar system and laboratory simulations • Extrasolar systems, including the detection and/or the detectability of exoplanets and planetary systems, their formation and evolution, the physical and chemical properties of the exoplanets • History of planetary and space research
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