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 hav...
Ausführliche Beschreibung
Gespeichert in:
| Autor*in: |
Le Mouélic, S. [verfasserIn] Guenneguez, M. [verfasserIn] Schmitt, H.H. [verfasserIn] Macquet, L. [verfasserIn] Mangold, N. [verfasserIn] Caravaca, G. [verfasserIn] Seignovert, B. [verfasserIn] Le Menn, E. [verfasserIn] Lenta, L. [verfasserIn] |
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| Format: |
E-Artikel |
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| Sprache: |
Englisch |
| Erschienen: |
2023 |
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| Schlagwörter: |
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| Übergeordnetes Werk: |
Enthalten in: Planetary and space science - Kidlington [u.a.] : Elsevier Science, 1959, 240 |
|---|---|
| Übergeordnetes Werk: |
volume:240 |
| DOI / URN: |
10.1016/j.pss.2023.105813 |
|---|
| Katalog-ID: |
ELV066811198 |
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| 520 | |a 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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10.1016/j.pss.2023.105813 doi (DE-627)ELV066811198 (ELSEVIER)S0032-0633(23)00182-4 DE-627 ger DE-627 rda eng 620 VZ 39.00 bkl 50.93 bkl Le Mouélic, S. verfasserin aut Photogrammetric 3D reconstruction of Apollo 17 Station 6: From boulders to lunar rock samples integrated into virtual reality 2023 nicht spezifiziert zzz rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier 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. Moon Photogrammetry Lunar sample Apollo Geology Virtual reality Guenneguez, M. verfasserin aut Schmitt, H.H. verfasserin aut Macquet, L. verfasserin aut Mangold, N. verfasserin aut Caravaca, G. verfasserin aut Seignovert, B. verfasserin aut Le Menn, E. verfasserin aut Lenta, L. verfasserin aut Enthalten in Planetary and space science Kidlington [u.a.] : Elsevier Science, 1959 240 Online-Ressource (DE-627)320505650 (DE-600)2012795-9 (DE-576)255266839 1873-5088 nnns volume:240 GBV_USEFLAG_U GBV_ELV SYSFLAG_U SSG-OPC-GGO SSG-OPC-GEO SSG-OPC-AST GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_32 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_74 GBV_ILN_90 GBV_ILN_95 GBV_ILN_100 GBV_ILN_105 GBV_ILN_110 GBV_ILN_150 GBV_ILN_151 GBV_ILN_187 GBV_ILN_213 GBV_ILN_224 GBV_ILN_230 GBV_ILN_370 GBV_ILN_602 GBV_ILN_702 GBV_ILN_2001 GBV_ILN_2003 GBV_ILN_2004 GBV_ILN_2005 GBV_ILN_2007 GBV_ILN_2009 GBV_ILN_2010 GBV_ILN_2011 GBV_ILN_2014 GBV_ILN_2015 GBV_ILN_2020 GBV_ILN_2021 GBV_ILN_2025 GBV_ILN_2026 GBV_ILN_2027 GBV_ILN_2034 GBV_ILN_2044 GBV_ILN_2048 GBV_ILN_2049 GBV_ILN_2050 GBV_ILN_2055 GBV_ILN_2056 GBV_ILN_2059 GBV_ILN_2061 GBV_ILN_2064 GBV_ILN_2106 GBV_ILN_2110 GBV_ILN_2111 GBV_ILN_2112 GBV_ILN_2122 GBV_ILN_2129 GBV_ILN_2143 GBV_ILN_2152 GBV_ILN_2153 GBV_ILN_2190 GBV_ILN_2232 GBV_ILN_2336 GBV_ILN_2470 GBV_ILN_2507 GBV_ILN_4035 GBV_ILN_4037 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4242 GBV_ILN_4249 GBV_ILN_4251 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4326 GBV_ILN_4333 GBV_ILN_4334 GBV_ILN_4338 GBV_ILN_4393 GBV_ILN_4700 39.00 Astronomie: Allgemeines VZ 50.93 Weltraumforschung VZ AR 240 |
| spelling |
10.1016/j.pss.2023.105813 doi (DE-627)ELV066811198 (ELSEVIER)S0032-0633(23)00182-4 DE-627 ger DE-627 rda eng 620 VZ 39.00 bkl 50.93 bkl Le Mouélic, S. verfasserin aut Photogrammetric 3D reconstruction of Apollo 17 Station 6: From boulders to lunar rock samples integrated into virtual reality 2023 nicht spezifiziert zzz rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier 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. Moon Photogrammetry Lunar sample Apollo Geology Virtual reality Guenneguez, M. verfasserin aut Schmitt, H.H. verfasserin aut Macquet, L. verfasserin aut Mangold, N. verfasserin aut Caravaca, G. verfasserin aut Seignovert, B. verfasserin aut Le Menn, E. verfasserin aut Lenta, L. verfasserin aut Enthalten in Planetary and space science Kidlington [u.a.] : Elsevier Science, 1959 240 Online-Ressource (DE-627)320505650 (DE-600)2012795-9 (DE-576)255266839 1873-5088 nnns volume:240 GBV_USEFLAG_U GBV_ELV SYSFLAG_U SSG-OPC-GGO SSG-OPC-GEO SSG-OPC-AST GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_32 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_74 GBV_ILN_90 GBV_ILN_95 GBV_ILN_100 GBV_ILN_105 GBV_ILN_110 GBV_ILN_150 GBV_ILN_151 GBV_ILN_187 GBV_ILN_213 GBV_ILN_224 GBV_ILN_230 GBV_ILN_370 GBV_ILN_602 GBV_ILN_702 GBV_ILN_2001 GBV_ILN_2003 GBV_ILN_2004 GBV_ILN_2005 GBV_ILN_2007 GBV_ILN_2009 GBV_ILN_2010 GBV_ILN_2011 GBV_ILN_2014 GBV_ILN_2015 GBV_ILN_2020 GBV_ILN_2021 GBV_ILN_2025 GBV_ILN_2026 GBV_ILN_2027 GBV_ILN_2034 GBV_ILN_2044 GBV_ILN_2048 GBV_ILN_2049 GBV_ILN_2050 GBV_ILN_2055 GBV_ILN_2056 GBV_ILN_2059 GBV_ILN_2061 GBV_ILN_2064 GBV_ILN_2106 GBV_ILN_2110 GBV_ILN_2111 GBV_ILN_2112 GBV_ILN_2122 GBV_ILN_2129 GBV_ILN_2143 GBV_ILN_2152 GBV_ILN_2153 GBV_ILN_2190 GBV_ILN_2232 GBV_ILN_2336 GBV_ILN_2470 GBV_ILN_2507 GBV_ILN_4035 GBV_ILN_4037 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4242 GBV_ILN_4249 GBV_ILN_4251 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4326 GBV_ILN_4333 GBV_ILN_4334 GBV_ILN_4338 GBV_ILN_4393 GBV_ILN_4700 39.00 Astronomie: Allgemeines VZ 50.93 Weltraumforschung VZ AR 240 |
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10.1016/j.pss.2023.105813 doi (DE-627)ELV066811198 (ELSEVIER)S0032-0633(23)00182-4 DE-627 ger DE-627 rda eng 620 VZ 39.00 bkl 50.93 bkl Le Mouélic, S. verfasserin aut Photogrammetric 3D reconstruction of Apollo 17 Station 6: From boulders to lunar rock samples integrated into virtual reality 2023 nicht spezifiziert zzz rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier 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. Moon Photogrammetry Lunar sample Apollo Geology Virtual reality Guenneguez, M. verfasserin aut Schmitt, H.H. verfasserin aut Macquet, L. verfasserin aut Mangold, N. verfasserin aut Caravaca, G. verfasserin aut Seignovert, B. verfasserin aut Le Menn, E. verfasserin aut Lenta, L. verfasserin aut Enthalten in Planetary and space science Kidlington [u.a.] : Elsevier Science, 1959 240 Online-Ressource (DE-627)320505650 (DE-600)2012795-9 (DE-576)255266839 1873-5088 nnns volume:240 GBV_USEFLAG_U GBV_ELV SYSFLAG_U SSG-OPC-GGO SSG-OPC-GEO SSG-OPC-AST GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_32 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_74 GBV_ILN_90 GBV_ILN_95 GBV_ILN_100 GBV_ILN_105 GBV_ILN_110 GBV_ILN_150 GBV_ILN_151 GBV_ILN_187 GBV_ILN_213 GBV_ILN_224 GBV_ILN_230 GBV_ILN_370 GBV_ILN_602 GBV_ILN_702 GBV_ILN_2001 GBV_ILN_2003 GBV_ILN_2004 GBV_ILN_2005 GBV_ILN_2007 GBV_ILN_2009 GBV_ILN_2010 GBV_ILN_2011 GBV_ILN_2014 GBV_ILN_2015 GBV_ILN_2020 GBV_ILN_2021 GBV_ILN_2025 GBV_ILN_2026 GBV_ILN_2027 GBV_ILN_2034 GBV_ILN_2044 GBV_ILN_2048 GBV_ILN_2049 GBV_ILN_2050 GBV_ILN_2055 GBV_ILN_2056 GBV_ILN_2059 GBV_ILN_2061 GBV_ILN_2064 GBV_ILN_2106 GBV_ILN_2110 GBV_ILN_2111 GBV_ILN_2112 GBV_ILN_2122 GBV_ILN_2129 GBV_ILN_2143 GBV_ILN_2152 GBV_ILN_2153 GBV_ILN_2190 GBV_ILN_2232 GBV_ILN_2336 GBV_ILN_2470 GBV_ILN_2507 GBV_ILN_4035 GBV_ILN_4037 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4242 GBV_ILN_4249 GBV_ILN_4251 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4326 GBV_ILN_4333 GBV_ILN_4334 GBV_ILN_4338 GBV_ILN_4393 GBV_ILN_4700 39.00 Astronomie: Allgemeines VZ 50.93 Weltraumforschung VZ AR 240 |
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10.1016/j.pss.2023.105813 doi (DE-627)ELV066811198 (ELSEVIER)S0032-0633(23)00182-4 DE-627 ger DE-627 rda eng 620 VZ 39.00 bkl 50.93 bkl Le Mouélic, S. verfasserin aut Photogrammetric 3D reconstruction of Apollo 17 Station 6: From boulders to lunar rock samples integrated into virtual reality 2023 nicht spezifiziert zzz rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier 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. Moon Photogrammetry Lunar sample Apollo Geology Virtual reality Guenneguez, M. verfasserin aut Schmitt, H.H. verfasserin aut Macquet, L. verfasserin aut Mangold, N. verfasserin aut Caravaca, G. verfasserin aut Seignovert, B. verfasserin aut Le Menn, E. verfasserin aut Lenta, L. verfasserin aut Enthalten in Planetary and space science Kidlington [u.a.] : Elsevier Science, 1959 240 Online-Ressource (DE-627)320505650 (DE-600)2012795-9 (DE-576)255266839 1873-5088 nnns volume:240 GBV_USEFLAG_U GBV_ELV SYSFLAG_U SSG-OPC-GGO SSG-OPC-GEO SSG-OPC-AST GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_32 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_74 GBV_ILN_90 GBV_ILN_95 GBV_ILN_100 GBV_ILN_105 GBV_ILN_110 GBV_ILN_150 GBV_ILN_151 GBV_ILN_187 GBV_ILN_213 GBV_ILN_224 GBV_ILN_230 GBV_ILN_370 GBV_ILN_602 GBV_ILN_702 GBV_ILN_2001 GBV_ILN_2003 GBV_ILN_2004 GBV_ILN_2005 GBV_ILN_2007 GBV_ILN_2009 GBV_ILN_2010 GBV_ILN_2011 GBV_ILN_2014 GBV_ILN_2015 GBV_ILN_2020 GBV_ILN_2021 GBV_ILN_2025 GBV_ILN_2026 GBV_ILN_2027 GBV_ILN_2034 GBV_ILN_2044 GBV_ILN_2048 GBV_ILN_2049 GBV_ILN_2050 GBV_ILN_2055 GBV_ILN_2056 GBV_ILN_2059 GBV_ILN_2061 GBV_ILN_2064 GBV_ILN_2106 GBV_ILN_2110 GBV_ILN_2111 GBV_ILN_2112 GBV_ILN_2122 GBV_ILN_2129 GBV_ILN_2143 GBV_ILN_2152 GBV_ILN_2153 GBV_ILN_2190 GBV_ILN_2232 GBV_ILN_2336 GBV_ILN_2470 GBV_ILN_2507 GBV_ILN_4035 GBV_ILN_4037 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4242 GBV_ILN_4249 GBV_ILN_4251 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4326 GBV_ILN_4333 GBV_ILN_4334 GBV_ILN_4338 GBV_ILN_4393 GBV_ILN_4700 39.00 Astronomie: Allgemeines VZ 50.93 Weltraumforschung VZ AR 240 |
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Le Mouélic, S. @@aut@@ Guenneguez, M. @@aut@@ Schmitt, H.H. @@aut@@ Macquet, L. @@aut@@ Mangold, N. @@aut@@ Caravaca, G. @@aut@@ Seignovert, B. @@aut@@ Le Menn, E. @@aut@@ Lenta, L. @@aut@@ |
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Le Mouélic, S. |
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photogrammetric 3d reconstruction of apollo 17 station 6: from boulders to lunar rock samples integrated into virtual reality |
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Photogrammetric 3D reconstruction of Apollo 17 Station 6: From boulders to lunar rock samples integrated into virtual reality |
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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. |
| abstractGer |
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. |
| abstract_unstemmed |
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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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.</subfield></datafield><datafield tag="650" ind1=" " ind2="4"><subfield code="a">Moon</subfield></datafield><datafield tag="650" ind1=" " ind2="4"><subfield code="a">Photogrammetry</subfield></datafield><datafield tag="650" ind1=" " ind2="4"><subfield code="a">Lunar sample</subfield></datafield><datafield tag="650" ind1=" " ind2="4"><subfield code="a">Apollo</subfield></datafield><datafield tag="650" ind1=" " ind2="4"><subfield code="a">Geology</subfield></datafield><datafield tag="650" ind1=" " 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