Jia Wang
Current Organizations / Institutes
The organizations/institutes from the scholar's latest article
Research Subjects
Jia Wang has a total of 125 co-authors. Here are the top co-authors by number of shared publications:
- Kaichang Di
Chinese Academy of Sciences
7 shared publications - Yexin Wang
State Key Laboratory of Remote Sensing and Digital Earth, Aerospace Information Research Institute, Chinese Academy of Sciences, Beijing 100101, China
6 shared publications - Bin Liu
State Key Laboratory of Remote Sensing and Digital Earth, Aerospace Information Research Institute, Chinese Academy of Sciences, Beijing 100101, China
5 shared publications Wenhui Wan
State Key Laboratory of Remote Sensing Science, Aerospace Information Research Institute, Chinese Academy of Sciences, Beijing, China
4 shared publications- Haibo Gao
Harbin Institute of Technology
3 shared publications - Huaiguang Yang
National Key Laboratory of Aerospace Mechanism, Harbin Institute of Technology, Harbin, China
3 shared publications
Latest Publications
- Open Access
- 28 July 2025
- Published by Copernicus GmbH in The International Archives of the Photogrammetry, Remote Sensing and Spatial Information Sciences
- Vol. XLVIII-G-2, 383-388
Landing Site Mapping and Lander Localization for Chang’e-5 and Chang’e-6 Lunar Sample Return Missions
Chang’e-5 and Chang’e-6 are lunar sample return missions in China’s lunar exploration program. In these missions, high-resolution landing site mapping and lander localization were performed to support mission operations and scientific investigations of the landing sites. The mapping and lander localization results also provided key information to provenance analysis of the samples. This paper presents a review of the landing site mapping and lander localization techniques and results in the two missions, including landing site topographic mapping using orbital images before landing, landing site topographic mapping using descent images after landing, lander localization, crater mapping and scientific applications, such as surface age determination, lunar chronology function update, and regolith thickness estimation.
- 28 July 2025
- Published by Copernicus GmbH in The International Archives of the Photogrammetry, Remote Sensing and Spatial Information Sciences
- Vol. XLVIII-G-2, 383-388
Open AccessLanding Site Mapping and Lander Localization for Chang’e-5 and Chang’e-6 Lunar Sample Return Missions
Chang’e-5 and Chang’e-6 are lunar sample return missions in China’s lunar exploration program. In these missions, high-resolution landing site mapping and lander localization were performed to support mission operations and scientific investigations of the landing sites. The mapping and lander localization results also provided key information to provenance analysis of the samples. This paper presents a review of the landing site mapping and lander localization techniques and results in the two missions, including landing site topographic mapping using orbital images before landing, landing site topographic mapping using descent images after landing, lander localization, crater mapping and scientific applications, such as surface age determination, lunar chronology function update, and regolith thickness estimation.
- Open Access
- 10 February 2025
- Published by Institute of Electrical and Electronics Engineers (IEEE) in IEEE Journal of Selected Topics in Applied Earth Observations and Remote Sensing
- Vol. 18 (19391404) , 6393-6408
Visual Localization and Topographic Mapping for Zhurong Rover in Tianwen-1 Mars Mission
This paper presents the methods, results and applications of visual localization and topographic mapping for Zhurong rover in China's Tianwen-1 mars mission. New techniques, namely vignette correction and online camera mast calibration, were developed for the images captured by the rover's Navigation and Terrain Cameras (NaTeCam) to enhance the mapping qualities. During surface operations, photogrammetric techniques were routinely applied at the travelling waypoints. The NaTeCam images were obtained to generate 3D topographic mapping products with centimeter level to support obstacle analysis and rover path planning. Cross-site visual localization at adjacent waypoints was conducted to reduce the accumulated position errors in the onboard dead-reckoning result. Visual localization refinement was also employed by matching of the digital orthophoto map (DOM) from the rover images and the orbital basemap at waypoints where distinct terrain features were available to further eliminate the localization errors. Comparing with the reference rover traverse extracted from a HiRISE image in which the actual rover track is visible, the accuracies of the rover traverses generated from cross-site visual localization and DOM matching refinement are estimated to be 1.75% and 0.50% of the traverse length. The actual total traverse length is 2009 m, which is 88 m longer than 1921 m from odometer reading, revealing a forward wheel slipping caused by the downslope trend of the southward traverse. The visual localization and topographic mapping results of Zhurong rover have greatly supported the surface exploration planning, object approaching and scientific investigations in the mission.
- 10 February 2025
- Published by Institute of Electrical and Electronics Engineers (IEEE) in IEEE Journal of Selected Topics in Applied Earth Observations and Remote Sensing
- Vol. 18 (19391404) , 6393-6408
Open AccessVisual Localization and Topographic Mapping for Zhurong Rover in Tianwen-1 Mars Mission
This paper presents the methods, results and applications of visual localization and topographic mapping for Zhurong rover in China's Tianwen-1 mars mission. New techniques, namely vignette correction and online camera mast calibration, were developed for the images captured by the rover's Navigation and Terrain Cameras (NaTeCam) to enhance the mapping qualities. During surface operations, photogrammetric techniques were routinely applied at the travelling waypoints. The NaTeCam images were obtained to generate 3D topographic mapping products with centimeter level to support obstacle analysis and rover path planning. Cross-site visual localization at adjacent waypoints was conducted to reduce the accumulated position errors in the onboard dead-reckoning result. Visual localization refinement was also employed by matching of the digital orthophoto map (DOM) from the rover images and the orbital basemap at waypoints where distinct terrain features were available to further eliminate the localization errors. Comparing with the reference rover traverse extracted from a HiRISE image in which the actual rover track is visible, the accuracies of the rover traverses generated from cross-site visual localization and DOM matching refinement are estimated to be 1.75% and 0.50% of the traverse length. The actual total traverse length is 2009 m, which is 88 m longer than 1921 m from odometer reading, revealing a forward wheel slipping caused by the downslope trend of the southward traverse. The visual localization and topographic mapping results of Zhurong rover have greatly supported the surface exploration planning, object approaching and scientific investigations in the mission.
- Open Access
- 8 March 2024
- Published by Springer Nature in Nature Communications
- Vol. 15 (1) , 1-15
Lunar rock investigation and tri-aspect characterization of lunar farside regolith by a digital twin
Yutu-2 rover conducted an exciting expedition on the 41st lunar day to investigate a fin-shaped rock at Longji site (45.44°S, 177.56°E) by extending its locomotion margin on perilous peaks. The varied locomotion encountered, especially multi-form wheel slippage, during the journey to the target rock, established unique conditions for a fin-grained lunar regolith analysis regarding bearing, shear and lateral properties based on terramechanics. Here, we show a tri-aspect characterization of lunar regolith and infer the rock’s origin using a digital twin. We estimate internal friction angle within 21.5°−42.0° and associated cohesion of 520-3154 Pa in the Chang’E-4 operational site. These findings suggest shear characteristics similar to Apollo 12 mission samples but notably higher cohesion compared to regolith investigated on most nearside lunar missions. We estimate external friction angle in lateral properties to be within 8.3°−16.5°, which fills the gaps of the lateral property estimation of the lunar farside regolith and serves as a foundational parameter for subsequent engineering verifications. Our in-situ spectral investigations of the target rock unveil its composition of iron/magnesium-rich low-calcium pyroxene, linking it to the Zhinyu crater (45.34°S, 176.15°E) ejecta. Our results indicate that the combination of in-situ measurements with robotics technology in planetary exploration reveal the possibility of additional source regions contributing to the local materials at the Chang’E-4 site, implying a more complicated geological history in the vicinity.
- 8 March 2024
- Published by Springer Nature in Nature Communications
- Vol. 15 (1) , 1-15
Open AccessLunar rock investigation and tri-aspect characterization of lunar farside regolith by a digital twin
Yutu-2 rover conducted an exciting expedition on the 41st lunar day to investigate a fin-shaped rock at Longji site (45.44°S, 177.56°E) by extending its locomotion margin on perilous peaks. The varied locomotion encountered, especially multi-form wheel slippage, during the journey to the target rock, established unique conditions for a fin-grained lunar regolith analysis regarding bearing, shear and lateral properties based on terramechanics. Here, we show a tri-aspect characterization of lunar regolith and infer the rock’s origin using a digital twin. We estimate internal friction angle within 21.5°−42.0° and associated cohesion of 520-3154 Pa in the Chang’E-4 operational site. These findings suggest shear characteristics similar to Apollo 12 mission samples but notably higher cohesion compared to regolith investigated on most nearside lunar missions. We estimate external friction angle in lateral properties to be within 8.3°−16.5°, which fills the gaps of the lateral property estimation of the lunar farside regolith and serves as a foundational parameter for subsequent engineering verifications. Our in-situ spectral investigations of the target rock unveil its composition of iron/magnesium-rich low-calcium pyroxene, linking it to the Zhinyu crater (45.34°S, 176.15°E) ejecta. Our results indicate that the combination of in-situ measurements with robotics technology in planetary exploration reveal the possibility of additional source regions contributing to the local materials at the Chang’E-4 site, implying a more complicated geological history in the vicinity.
- Open Access
- 11 December 2023
- Published by MDPI AG in Remote Sensing
- Vol. 15 (24) , 5691
Analysis of Illumination Conditions in the Lunar South Polar Region Using Multi-Temporal High-Resolution Orbital Images
The illumination conditions of the lunar south pole region are complex due to the rugged terrain and very low solar elevation angles, posing significant challenges to the safety of lunar landing and rover explorations. High-spatial and temporal-resolution analyses of the illumination conditions in the south pole region are essential to support mission planning and surface operations. This paper proposes a method for illumination condition analysis in the lunar pole region using multi-temporal high-resolution orbital images with a pre-selected landing area of Chang’E-7 as the study area. Firstly, a database of historical multi-temporal high-resolution (0.69–1.97 m/pixel) orbital images, with associated image acquisition time, solar elevation angle, and azimuth angle, is established after preprocessing and registration. Secondly, images with the nearest solar elevation and azimuth at the planned time for mission operations are retrieved from the database for subsequent illumination condition analysis and exploration support. The differences in the actual solar positions at the mission moments from that of the nearest sun position image are calculated and their impact on illumination conditions is evaluated. Experimental results of the study area demonstrate that the constructed image database and the proposed illumination analysis method using multi-temporal images, with the assistance of DEM in a small number of cases, can effectively support the mission planning and operations for the Chang’E-7 mission in the near future.
- 11 December 2023
- Published by MDPI AG in Remote Sensing
- Vol. 15 (24) , 5691
Open AccessAnalysis of Illumination Conditions in the Lunar South Polar Region Using Multi-Temporal High-Resolution Orbital Images
The illumination conditions of the lunar south pole region are complex due to the rugged terrain and very low solar elevation angles, posing significant challenges to the safety of lunar landing and rover explorations. High-spatial and temporal-resolution analyses of the illumination conditions in the south pole region are essential to support mission planning and surface operations. This paper proposes a method for illumination condition analysis in the lunar pole region using multi-temporal high-resolution orbital images with a pre-selected landing area of Chang’E-7 as the study area. Firstly, a database of historical multi-temporal high-resolution (0.69–1.97 m/pixel) orbital images, with associated image acquisition time, solar elevation angle, and azimuth angle, is established after preprocessing and registration. Secondly, images with the nearest solar elevation and azimuth at the planned time for mission operations are retrieved from the database for subsequent illumination condition analysis and exploration support. The differences in the actual solar positions at the mission moments from that of the nearest sun position image are calculated and their impact on illumination conditions is evaluated. Experimental results of the study area demonstrate that the constructed image database and the proposed illumination analysis method using multi-temporal images, with the assistance of DEM in a small number of cases, can effectively support the mission planning and operations for the Chang’E-7 mission in the near future.
- Open Access
- 22 March 2023
- Published by Springer Nature in Research Square
Technology enabled science: investigation of a fin-shaped rock by the Yutu-2 rover on the lunar farside
Technology advancement in modern planetary exploration has extended extraterrestrial geological science by sending rovers on challenging, possibly risky but highly scientific-valuable ventures, such as ascending towards the crater walls, traversing steep slopes of sand dunes and travelling through the lava tube. On the 41st lunar day, the first lunar farside prospector, the Yutu-2 rover, carried out an exciting expedition towards a scientifically interesting fin-shaped rock for spectral investigation, taking a high risk of wheel skidding and lateral slippage along a narrow and uneven passage. The rover successfully achieved new findings by extending its locomotion margin on perilous peaks, while its safety was maintained on the basis of ingenious exploration strategies and digital twin-based performance analysis. Surface morphology analysis of the fin-shaped rock indicates that it has suffered certain degrees of impacts. The further in situ spectral investigations suggest that the target rock is composed of Fe/Mg-rich low-Ca pyroxene, thus inferred to belongs to the Zhinyu crater ejecta, rather than those of the Finsen crater. Engineering locomotive data of the rover was used for comprehensive lunar regolith property identification, presenting the first shear parameter range of the farside regolith and an initial estimation on its lateral property in the extraterrestrial environment. The estimated internal friction angle is within 21.5°-42.0° and the associated cohesion is 520-3154 Pa, which suggests that the lunar regolith at Chang’E-4 site had similar shear characteristics to samples measured by direct shear approach on the Apollo 12 mission, but relatively larger cohesion than the counterpart investigated on most of nearside lunar missions. This study demonstrates a paradigm of the in-depth integration of science and technology in space exploration, where planetary science is enabled by engineering support, and new demands of scientific exploration in turn generate motivation for the improvement of technology.
- 22 March 2023
- Published by Springer Nature in Research Square
Open AccessTechnology enabled science: investigation of a fin-shaped rock by the Yutu-2 rover on the lunar farside
Technology advancement in modern planetary exploration has extended extraterrestrial geological science by sending rovers on challenging, possibly risky but highly scientific-valuable ventures, such as ascending towards the crater walls, traversing steep slopes of sand dunes and travelling through the lava tube. On the 41st lunar day, the first lunar farside prospector, the Yutu-2 rover, carried out an exciting expedition towards a scientifically interesting fin-shaped rock for spectral investigation, taking a high risk of wheel skidding and lateral slippage along a narrow and uneven passage. The rover successfully achieved new findings by extending its locomotion margin on perilous peaks, while its safety was maintained on the basis of ingenious exploration strategies and digital twin-based performance analysis. Surface morphology analysis of the fin-shaped rock indicates that it has suffered certain degrees of impacts. The further in situ spectral investigations suggest that the target rock is composed of Fe/Mg-rich low-Ca pyroxene, thus inferred to belongs to the Zhinyu crater ejecta, rather than those of the Finsen crater. Engineering locomotive data of the rover was used for comprehensive lunar regolith property identification, presenting the first shear parameter range of the farside regolith and an initial estimation on its lateral property in the extraterrestrial environment. The estimated internal friction angle is within 21.5°-42.0° and the associated cohesion is 520-3154 Pa, which suggests that the lunar regolith at Chang’E-4 site had similar shear characteristics to samples measured by direct shear approach on the Apollo 12 mission, but relatively larger cohesion than the counterpart investigated on most of nearside lunar missions. This study demonstrates a paradigm of the in-depth integration of science and technology in space exploration, where planetary science is enabled by engineering support, and new demands of scientific exploration in turn generate motivation for the improvement of technology.
- Open Access
- 16 March 2022
- Published by MDPI AG in Remote Sensing
- Vol. 14 (6) , 1442
High-Precision Registration of Lunar Global Mapping Products Based on Spherical Triangular Mesh
Lunar global mapping products provide a solid data foundation for lunar scientific research and exploration. As the widespread geometric inconsistencies among multi-source mapping products seriously affect the synergistic use of the products, high-precision registration of multiple lunar global products is critical, and it is highly challenging due to large coverage and complex local geometric inconsistencies. In this research, we propose a spherical triangular-mesh-based method for high-precision registration of lunar global mapping products, which involves four steps: data preprocessing, feature point extraction and matching, spherical Delaunay triangulation, and geometric correction with spherical barycentric coordinates. This global registration method avoids map projection distortions by using spherical coordinates directly, and achieves high precision by confining the geometric models to spherical triangular facets. Experiments are conducted using two groups of different types of mapping products to verify the proposed method quantitatively and qualitatively. The results show that the geometric inconsistencies are reduced from hundreds of pixels to sub-pixel level globally after the registration, demonstrating the effectiveness of the proposed method.
- 16 March 2022
- Published by MDPI AG in Remote Sensing
- Vol. 14 (6) , 1442
Open AccessHigh-Precision Registration of Lunar Global Mapping Products Based on Spherical Triangular Mesh
Lunar global mapping products provide a solid data foundation for lunar scientific research and exploration. As the widespread geometric inconsistencies among multi-source mapping products seriously affect the synergistic use of the products, high-precision registration of multiple lunar global products is critical, and it is highly challenging due to large coverage and complex local geometric inconsistencies. In this research, we propose a spherical triangular-mesh-based method for high-precision registration of lunar global mapping products, which involves four steps: data preprocessing, feature point extraction and matching, spherical Delaunay triangulation, and geometric correction with spherical barycentric coordinates. This global registration method avoids map projection distortions by using spherical coordinates directly, and achieves high precision by confining the geometric models to spherical triangular facets. Experiments are conducted using two groups of different types of mapping products to verify the proposed method quantitatively and qualitatively. The results show that the geometric inconsistencies are reduced from hundreds of pixels to sub-pixel level globally after the registration, demonstrating the effectiveness of the proposed method.
- 7 March 2022
- Published by Springer Nature in Nature Geoscience
- Vol. 15 (3) , 171-176
Surface characteristics of the Zhurong Mars rover traverse at Utopia Planitia
- 7 March 2022
- Published by Springer Nature in Nature Geoscience
- Vol. 15 (3) , 171-176
Surface characteristics of the Zhurong Mars rover traverse at Utopia Planitia
- Open Access
- 30 August 2021
- Published by MDPI AG in Remote Sensing
- Vol. 13 (17) , 3439
Visual Localization of the Tianwen-1 Lander Using Orbital, Descent and Rover Images
Tianwen-1, China’s first Mars exploration mission, was successfully landed in the southern part of Utopia Planitia on 15 May 2021 (UTC+8). Timely and accurately determining the landing location is critical for the subsequent mission operations. For timely localization, the remote landmarks, selected from the panorama generated by the earliest received Navigation and Terrain Cameras (NaTeCam) images, were matched with the Digital Orthophoto Map (DOM) generated by high resolution imaging camera (HiRIC) images to obtain the initial result based on the triangulation method. Then, the initial localization result was refined by the descent images received later and the NaTeCam DOM. Finally, the lander location was determined to be (25.066°N, 109.925°E). Verified by the new orbital image with the lander and Zhurong rover visible, the localization accuracy was within a pixel of the HiRIC DOM.
- 30 August 2021
- Published by MDPI AG in Remote Sensing
- Vol. 13 (17) , 3439
Open AccessVisual Localization of the Tianwen-1 Lander Using Orbital, Descent and Rover Images
Tianwen-1, China’s first Mars exploration mission, was successfully landed in the southern part of Utopia Planitia on 15 May 2021 (UTC+8). Timely and accurately determining the landing location is critical for the subsequent mission operations. For timely localization, the remote landmarks, selected from the panorama generated by the earliest received Navigation and Terrain Cameras (NaTeCam) images, were matched with the Digital Orthophoto Map (DOM) generated by high resolution imaging camera (HiRIC) images to obtain the initial result based on the triangulation method. Then, the initial localization result was refined by the descent images received later and the NaTeCam DOM. Finally, the lander location was determined to be (25.066°N, 109.925°E). Verified by the new orbital image with the lander and Zhurong rover visible, the localization accuracy was within a pixel of the HiRIC DOM.
- Open Access
- 28 July 2021
- Published by MDPI AG in Remote Sensing
- Vol. 13 (15) , 2975
A Photogrammetric-Photometric Stereo Method for High-Resolution Lunar Topographic Mapping Using Yutu-2 Rover Images
Topographic products are important for mission operations and scientific research in lunar exploration. In a lunar rover mission, high-resolution digital elevation models are typically generated at waypoints by photogrammetry methods based on rover stereo images acquired by stereo cameras. In case stereo images are not available, the stereo-photogrammetric method will not be applicable. Alternatively, photometric stereo method can recover topographic information with pixel-level resolution from three or more images, which are acquired by one camera under the same viewing geometry with different illumination conditions. In this research, we extend the concept of photometric stereo to photogrammetric-photometric stereo by incorporating collinearity equations into imaging irradiance model. The proposed photogrammetric-photometric stereo algorithm for surface construction involves three steps. First, the terrain normal vector in object space is derived from collinearity equations, and image irradiance equation for close-range topographic mapping is determined. Second, based on image irradiance equations of multiple images, the height gradients in image space can be solved. Finally, the height map is reconstructed through global least-squares surface reconstruction with spectral regularization. Experiments were carried out using simulated lunar rover images and actual lunar rover images acquired by Yutu-2 rover of Chang’e-4 mission. The results indicate that the proposed method achieves high-resolution and high-precision surface reconstruction, and outperforms the traditional photometric stereo methods. The proposed method is valuable for ground-based lunar surface reconstruction and can be applicable to surface reconstruction of Earth and other planets.
- 28 July 2021
- Published by MDPI AG in Remote Sensing
- Vol. 13 (15) , 2975
Open AccessA Photogrammetric-Photometric Stereo Method for High-Resolution Lunar Topographic Mapping Using Yutu-2 Rover Images
Topographic products are important for mission operations and scientific research in lunar exploration. In a lunar rover mission, high-resolution digital elevation models are typically generated at waypoints by photogrammetry methods based on rover stereo images acquired by stereo cameras. In case stereo images are not available, the stereo-photogrammetric method will not be applicable. Alternatively, photometric stereo method can recover topographic information with pixel-level resolution from three or more images, which are acquired by one camera under the same viewing geometry with different illumination conditions. In this research, we extend the concept of photometric stereo to photogrammetric-photometric stereo by incorporating collinearity equations into imaging irradiance model. The proposed photogrammetric-photometric stereo algorithm for surface construction involves three steps. First, the terrain normal vector in object space is derived from collinearity equations, and image irradiance equation for close-range topographic mapping is determined. Second, based on image irradiance equations of multiple images, the height gradients in image space can be solved. Finally, the height map is reconstructed through global least-squares surface reconstruction with spectral regularization. Experiments were carried out using simulated lunar rover images and actual lunar rover images acquired by Yutu-2 rover of Chang’e-4 mission. The results indicate that the proposed method achieves high-resolution and high-precision surface reconstruction, and outperforms the traditional photometric stereo methods. The proposed method is valuable for ground-based lunar surface reconstruction and can be applicable to surface reconstruction of Earth and other planets.
- Open Access
- 7 February 2021
- Published by MDPI AG in Remote Sensing
- Vol. 13 (4) , 590
Localization of the Chang’e-5 Lander Using Radio-Tracking and Image-Based Methods
Chang’e-5, China’s first unmanned lunar sample-return mission, was successfully landed in Northern Oceanus Procellarum on 1 December 2020. Determining the lander location precisely and timely is critical for both engineering operations and subsequent scientific research. Localization of the lander was performed using radio-tracking and image-based methods. The lander location was determined to be (51.92°W, 43.06°N) by both methods. Other localization results were compared for cross-validation. The localization results greatly contributed to the planning of the ascender lifting off from the lander and subsequent maneuvers, and they will contribute to scientific analysis of the returned samples and in situ acquired data.
- 7 February 2021
- Published by MDPI AG in Remote Sensing
- Vol. 13 (4) , 590
Open AccessLocalization of the Chang’e-5 Lander Using Radio-Tracking and Image-Based Methods
Chang’e-5, China’s first unmanned lunar sample-return mission, was successfully landed in Northern Oceanus Procellarum on 1 December 2020. Determining the lander location precisely and timely is critical for both engineering operations and subsequent scientific research. Localization of the lander was performed using radio-tracking and image-based methods. The lander location was determined to be (51.92°W, 43.06°N) by both methods. Other localization results were compared for cross-validation. The localization results greatly contributed to the planning of the ascender lifting off from the lander and subsequent maneuvers, and they will contribute to scientific analysis of the returned samples and in situ acquired data.