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Journal articles on the topic 'Asteroid Landing'

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1

Yan, Weifeng, Ruoyu Feng, and Hexi Baoyin. "Stability of a Flexible Asteroid Lander with Landing Control." Aerospace 9, no. 11 (2022): 719. http://dx.doi.org/10.3390/aerospace9110719.

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Stable landing on asteroids is of considerable scientific and economic value but accompanied by huge difficulties. This paper proposes a novel flexible lander suitable for asteroids with microgravity and rugged surface. The gravity model with the artificial neural network and the surface model with the spherical harmonic method are introduced to establish the target asteroid’s dynamical environment. The flexible dynamics with the discrete shell model, the collision with the spring-damping model and viscous sliding friction, and the rigid coupling with the constraint violation stabilization met
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2

Chen, Danhe, Chuangyi Li, and Zhou Su. "Dynamics Research and Analysis of landing on the surface of Asteroid." Journal of Physics: Conference Series 2472, no. 1 (2023): 012033. http://dx.doi.org/10.1088/1742-6596/2472/1/012033.

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Abstract Asteroid detection has been the main research field of deep space exploration, and even in the future years. Countries have carried out missions to flyby and landing on the surface of asteroids, the sampling can help human explore the origins of small bodies, as well as origin of the solar system. While the particular environmental factors such as small size and low gravity of asteroids make the landing more difficult, this paper designs a four-legged inverted triangle soft lander, supplemented by thrust reversers and rope anchors for stable landing. A mathematical model of the lander
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Wang, R., K. Di, W. Wan, et al. "TOPOGRAPHIC MAPPING AND ANALYSIS BASED ON 3D RECONSTRUCTION MODEL OF SIMULATED ASTEROID." ISPRS - International Archives of the Photogrammetry, Remote Sensing and Spatial Information Sciences XLIII-B3-2020 (August 21, 2020): 1165–70. http://dx.doi.org/10.5194/isprs-archives-xliii-b3-2020-1165-2020.

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Abstract. Asteroid exploration is of great scientific significance in understanding the evolution of the solar system. Unlike lunar missions, asteroids are far away from the earth, the communication between the spacecraft and the ground station has a large delay. Moreover, the small size, irregular shape and uneven mass distribution of asteroids further increase the difficulty of landing missions. This paper presented a topographic mapping and analysis method based on three-dimensional (3D) reconstruction model of a simulated asteroid. First, 3D reconstruction of a simulated asteroid was achie
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4

Wang, Weimin, and K. L. Yung. "Analysis of a Mechanical Anchoring System for Landing on Asteroids." Journal of Physics: Conference Series 2542, no. 1 (2023): 012017. http://dx.doi.org/10.1088/1742-6596/2542/1/012017.

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Abstract The landing process to an asteroid is discussed with a Nimble Lander. The miniature harpoons are chosen as the anchoring device to landing to asteroid in the Nimble Lander. The analysis results provide detailed information of the anchoring with harpoon as anchoring device. Many different designs of harpoon have been tested by simulation, the best of three designs of harpoon are analyzed for anchoring to Apophis. Instead of the modelling of the anchor as a rigid cylindrical projectile in penetration models, the deformation of the harpoon is fully considered in the anchoring analysis. T
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Yongbin, Wang, Jiang Wansong, Long Long, Zhu Qian, Feng Rui, and Wang Liwu. "Design and Experimental Research of a New Type of Asteroid Anchoring System." International Journal of Aerospace Engineering 2021 (May 18, 2021): 1–7. http://dx.doi.org/10.1155/2021/6677877.

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Asteroid detection is of great significance to the study of the formation of the solar system and the origin of life. However, there are many types of asteroids, and they are far away from the earth, and the understanding of their various characteristics is not clear, which brings huge technical challenges to the landing and attachment of star catalogs. At present, the world is mainly based on surround, overflight, and short-term contact detection, and long-term attachment detection has not yet been realized. In order to solve the long-term attachment detection requirements of asteroids, focus
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6

Guo, Yundong, Jeng-Shyang Pan, Chengbo Qiu, et al. "SinGAN-Based Asteroid Surface Image Generation." Journal of Database Management 32, no. 4 (2021): 28–47. http://dx.doi.org/10.4018/jdm.2021100103.

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While it is risky considering spacecraft constraints and unknown environment on asteroid, surface sampling is an important technique for asteroid exploration. One of the sample return missions is to seek an optimal landing site, which may be in hazardous terrain. Since autonomous landing is particularly challenging, it is necessary to simulate the effectiveness of this process and prove the onboard optical hazard avoidance is robust to various uncertainties. This paper aims to generate realistic surface images of asteroids for simulations of asteroid exploration. A SinGAN-based method is propo
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7

Tang, Yijun, Yunxiao Jiang, Yuxiang Feng, Xiaoming Zhang, and Xiaojun Jiang. "Transformer-based Approach for Accurate Asteroid Spectra Taxonomy and Albedo Estimation." Astronomical Journal 169, no. 4 (2025): 201. https://doi.org/10.3847/1538-3881/adb710.

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Abstract China plans to launch a probe (Tianwen-2) around 2025, mainly to explore the near-Earth asteroid 2016 HO3 (469219, Kamo’oalewa). The mission involves close-range exploration, landing, and mining operations that require three-dimensional modeling of the asteroid, which requires prior knowledge of its material composition and uniformity. This information is crucial in progressive or ground exploration processes. Our research focuses on high-precision intelligent inversion of complex physical properties of asteroids based on spectral data, providing support for further analysis of astero
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8

Zhao, Zhijun, Shuang Wang, Delun Li, Hongtao Wang, Yongbing Wang, and Jingdong Zhao. "Development of an Anchoring System for the Soft Asteroid Landing Exploration." International Journal of Aerospace Engineering 2019 (February 7, 2019): 1–13. http://dx.doi.org/10.1155/2019/1257038.

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The landing mechanism is easy to flow away from the surface of the asteroid, as there is nearly no gravity on the asteroid. One of the most problems for the asteroid landing exploration is to anchor the landing mechanism on the asteroid surface. In the paper, an anchoring system employed on the soft asteroid anchoring is designed. It is mainly composed of penetrating unit, advancing unit, winding unit, damping unit, and so on. On the basis of the mechanical design, the resistance characteristic of the anchor body in penetrating process is analyzed, and the shape of the anchor tip is designed w
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9

Zhao, Yingjie, Hongwei Yang, and Jincheng Hu. "The Fast Generation of the Reachable Domain for Collision-Free Asteroid Landing." Mathematics 10, no. 20 (2022): 3763. http://dx.doi.org/10.3390/math10203763.

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For the mission requirement of collision-free asteroid landing with a given time of flight (TOF), a fast generation method of landing reachable domain based on section and expansion is proposed. First, to overcome the difficulties of trajectory optimization caused by anti-collision path constraints, a two-stage collision-free trajectory optimization model is used to improve the efficiency of trajectory optimization. Second, the velocity increment under a long TOF is analyzed to obtain the distribution law of the reachable domain affected by the TOF, and the generation problem of the reachable
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10

Su, Linli, Wenyu Feng, Lie Yang, Zichen Fan, Mingying Huo, and Naiming Qi. "Orbital Analysis of a Dual Asteroid System Explorer Based on the Finite Element Method." Aerospace 11, no. 12 (2024): 993. https://doi.org/10.3390/aerospace11120993.

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In the study of dual asteroid systems, a model that can rapidly compute the motion and orientation of these bodies is essential. Traditional modeling techniques, such as the double ellipsoid or polyhedron methods, fail to deliver sufficient accuracy in estimating the interactions between dual asteroids. This inadequacy primarily stems from the non-tidally locked nature of asteroid systems, which necessitates continual adjustments to account for changes in gravitational fields. This study adopts the finite element method to precisely model the dynamic interaction forces within irregular, time-v
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11

Quan, Ronghui, Zhiying Song, and Zhigui Liu. "Dynamic 3D Simulation of Surface Charging on Rotating Asteroids." Astrophysical Journal 977, no. 1 (2024): 127. https://doi.org/10.3847/1538-4357/ad8e37.

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Abstract The surface-charging phenomenon of asteroids, mainly resulting from solar wind plasma and solar radiation, has been extensively studied. However, the influence of the asteroid’s rotation on surface charging is not yet fully understood. In this study, a neural network is established to replace numerical integration, improving the efficiency of dynamic 3D simulations. We simulate rotating asteroids and their surrounding plasma environments under various conditions, including the quiet solar wind and solar storms. Different minerals on the asteroid surface are also considered. Additional
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12

Dunham, David W., Robert W. Farquhar, James V. McAdams, et al. "Implementation of the First Asteroid Landing." Icarus 159, no. 2 (2002): 433–38. http://dx.doi.org/10.1006/icar.2002.6911.

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13

Cocaud, Cedric, and Takashi Kubota. "Development of an Intelligent Simulator with SLAM Functions for Visual Autonomous Landing on Small Celestial Bodies." Journal of Advanced Computational Intelligence and Intelligent Informatics 15, no. 8 (2011): 1167–74. http://dx.doi.org/10.20965/jaciii.2011.p1167.

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As space agencies are currently looking at Near Earth Asteroids as a next step on their exploration roadmap, high precision autonomous landing control schemes will be required for upcoming missions. In this paper, an intelligent simulator is proposed to reproduce all of the visual and dynamic aspects required to test an autonomous Simultaneous Localization and Mapping (SLAM) system. The proposed simulator provides position and attitude information to a spacecraft during its approach descent and Landing phase toward the surface of an asteroid or other small celestial bodies. Because the SLAM sy
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14

Geng, Shujuan, Binghong Zhou, and Mingtao Li. "On the capture of small stony asteroids into the Earth's orbit by atmospheric grazing." Monthly Notices of the Royal Astronomical Society 507, no. 3 (2021): 4661–68. http://dx.doi.org/10.1093/mnras/stab2439.

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ABSTRACT An Earth-grazing asteroid can be captured into a gravitational bound orbit around the Earth during its transitory atmospheric journey. Otherwise, it will either escape back to space or plunge to the Earth directly. With fragmentation taken into account, we subdivide the captured and direct impact modes, expanding the above three modes into five – escaping, captured impact with and without fragmentation, and direct impact with and without fragmentation. We then investigate the conditions of those various impact modes of shallow-angle impacts of small stony asteroids no larger than 100
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15

Song Zhi-Ying, Quan Rong-Hui, and Liu Zhi-Gui. "Surface Charging Characteristics of Rotating Asteroids in the Solar System." Acta Physica Sinica 73, no. 24 (2024): 0. http://dx.doi.org/10.7498/aps.73.20241182.

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The attachment and movement of charged particles in the space plasma environment can result in observable potentials on the asteroid surface, this surface charging phenomenon has been extensively studied. However, the influence of asteroid's rotation on surface charging and the surrounding plasma is not yet fully understood. Traditional methods using numerical integration and PIC have slow computation speeds, and mainly focus on the charging mechanisms of static asteroids. In this study, we established a multi-scale model based on neural networks and the finite element method, improving simula
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16

Guelman, M., and D. Harel. "Power limited soft landing on an asteroid." Journal of Guidance, Control, and Dynamics 17, no. 1 (1994): 15–20. http://dx.doi.org/10.2514/3.21153.

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17

Tachibana, S., H. Sawada, R. Okazaki, et al. "Pebbles and sand on asteroid (162173) Ryugu: In situ observation and particles returned to Earth." Science 375, no. 6584 (2022): 1011–16. http://dx.doi.org/10.1126/science.abj8624.

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The Hayabusa2 spacecraft investigated the C-type (carbonaceous) asteroid (162173) Ryugu. The mission performed two landing operations to collect samples of surface and subsurface material, the latter exposed by an artificial impact. We present images of the second touchdown site, finding that ejecta from the impact crater was present at the sample location. Surface pebbles at both landing sites show morphological variations ranging from rugged to smooth, similar to Ryugu’s boulders, and shapes from quasi-spherical to flattened. The samples were returned to Earth on 6 December 2020. We describe
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18

Herrera-Sucarrat, E., P. L. Palmer, and R. M. Roberts. "Asteroid Observation and Landing Trajectories Using Invariant Manifolds." Journal of Guidance, Control, and Dynamics 37, no. 3 (2014): 907–20. http://dx.doi.org/10.2514/1.59594.

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19

Martin, Iain, Steve Parkes, Martin Dunstan, and Nick Rowell. "Asteroid Modeling for Testing Spacecraft Approach and Landing." IEEE Computer Graphics and Applications 34, no. 4 (2014): 52–62. http://dx.doi.org/10.1109/mcg.2014.22.

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20

Xiu, Wenbo, Jiateng Long, Shengying Zhu, and Pingyuan Cui. "Landmark robust selection for asteroid landing visual navigation." Acta Astronautica 214 (January 2024): 665–76. http://dx.doi.org/10.1016/j.actaastro.2023.11.029.

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21

Okada, Tatsuaki. "Thermography of Asteroid and Future Applications in Space Missions." Applied Sciences 10, no. 6 (2020): 2158. http://dx.doi.org/10.3390/app10062158.

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The Near-Earth Asteroid 162173 Ryugu is a C-type asteroid which preserves information about the ancient Solar System and is considered enriched in volatiles such as water and organics associated with the building blocks of life, and it is a potentially hazardous object that might impact Earth. Hayabusa2 is the asteroid explorer organized by the Japan Aerospace Exploration Agency to rendezvous with the asteroid and collect surface materials to return them to Earth. Thermography has been carried out from Hayabusa2 during the asteroid proximity phase, to unveil the thermophysical properties of th
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22

Cheng, Ma. "The significance and related technologies of asteroid detection." Highlights in Science, Engineering and Technology 48 (May 16, 2023): 295–317. http://dx.doi.org/10.54097/hset.v48i.8369.

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Asteroid detection mission plays an important role in the field of deep space exploration, and it has multiple theoretical and practical guidance advantages for asteroid detection missions, and also promotes all critical technologies of deep space exploration. At present, many asteroid exploration missions have been carried out around the world, and China also plans to launch the "Tianwen-2" probe around 2025 to carry out an integrated exploration mission of fly-by, orbit detection, attachment control and sample-return mission for asteroid 2016HO3. In this paper, we discuss the significance of
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23

Zhao, Zhijun, Jingdong Zhao, and Hong Liu. "Development of a Landing Mechanism for Asteroids with Soft Surface." International Journal of Aerospace Engineering 2013 (2013): 1–9. http://dx.doi.org/10.1155/2013/873135.

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A landing mechanism to an asteroid with soft surface is developed. It consists of three landing feet, landing legs, cardan element, damping element, equipment base, anchoring system, and so on. Static structural analysis and modal analysis are carried out to check the strength and natural frequency of the landing mechanism with FEA. Testing platform for the anchoring system is introduced, and then the penetrating and anchoring tests of the anchoring system are carried out in different media. It shows that cohesion of the media has large influence on the penetrating and anchoring performance of
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24

Mikawa, Masahiko. "Robust Wireless Communication for Small Exploration Rovers Equipped with Multiple Antennas by Estimating Attitudes of Rovers in Several Experimental Environments." Journal of Robotics and Mechatronics 29, no. 5 (2017): 864–76. http://dx.doi.org/10.20965/jrm.2017.p0864.

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We are developing a robotic system for an asteroid surface exploration. The system consists ofmultiplesmall size rovers, that communicate with each other over a wireless network. Since the rovers configure over a wireless mesh sensor network on an asteroid, it is possible to explore a large area on the asteroid effectively. The rovers will be equipped with a hopping mechanism for transportation, which is suitable for exploration in a micro-gravity environment like a small asteroid’s surface. However, it is difficult to control the rover’s attitude during the landing. Therefore, a cube-shaped r
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25

Furfaro, Roberto, Dario Cersosimo, and Daniel R. Wibben. "Asteroid Precision Landing via Multiple Sliding Surfaces Guidance Techniques." Journal of Guidance, Control, and Dynamics 36, no. 4 (2013): 1075–92. http://dx.doi.org/10.2514/1.58246.

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26

Showstack, R. "NEAR spacecraft makes first-ever landing on an asteroid." Eos, Transactions American Geophysical Union 82, no. 8 (2001): 98. http://dx.doi.org/10.1029/01eo00051.

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27

Sanchez, Julio C., Francisco Gavilan, and Rafael Vazquez. "A Predictive Guidance Algorithm for Autonomous Asteroid Soft Landing." IFAC-PapersOnLine 51, no. 12 (2018): 6–11. http://dx.doi.org/10.1016/j.ifacol.2018.07.080.

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28

Yu, Meng, Shuang Li, Shuquan Wang, and Xiangyu Huang. "Single crater-aided inertial navigation for autonomous asteroid landing." Advances in Space Research 63, no. 2 (2019): 1085–99. http://dx.doi.org/10.1016/j.asr.2018.09.035.

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29

Kang, Shen, Jianan Wang, Chaoyong Li, and Jiayuan Shan. "Nonlinear optimal control with disturbance rejection for asteroid landing." Journal of the Franklin Institute 355, no. 16 (2018): 8027–48. http://dx.doi.org/10.1016/j.jfranklin.2018.06.028.

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30

Lin, Boyu, and Hutao Cui. "Research on A Low Computational Cost Vision-aided Inertial Navigation Method for Precision Landing on Asteroid." Journal of Physics: Conference Series 2203, no. 1 (2022): 012020. http://dx.doi.org/10.1088/1742-6596/2203/1/012020.

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Abstract Asteroid exploration missions demand more autonomous navigation system that are precise and in real-time. Visual-aided inertial navigation systems combine the advantages of autonomy of inertial navigation systems and accuracy of visual navigation systems. However, both increase the computational burden for the information processing. With the goal of decreasing the computational load, this paper proposes a low cost vision-aided inertial navigation method which can calculate increment position, velocity and attitude directly in inertial frame by pre-integrating IMU measurements. For vi
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31

Zhao, Zhijun, JingDong Zhao, and Hong Liu. "Landing Dynamic and Key Parameter Estimations of a Landing Mechanism to Asteroid with Soft Surface." International Journal of Aeronautical and Space Sciences 14, no. 3 (2013): 237–46. http://dx.doi.org/10.5139/ijass.2013.14.3.237.

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32

Schulz, Rita. "The Rosetta Mission: Comet and Asteroid Exploration." Proceedings of the International Astronomical Union 5, S263 (2009): 312–16. http://dx.doi.org/10.1017/s1743921310001997.

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AbstractIn March 2004 the European Space Agency launched its Planetary Cornerstone Mission Rosetta to rendezvous with Jupiter-family comet 67P/Churyumov-Gerasimenko. The Rosetta mission represents the next step into the improvement of our understanding of comet nuclei naturally following the four successful comet nucleus fly-by missions carried out in the past. It will however not perform a simple fly-by at its target comet, but combines an Orbiter and a Lander Mission. The Rosetta spacecraft will go in orbit around the comet nucleus when it is still far away from the Sun, and escort the comet
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33

Preusker, F., F. Scholten, S. Elgner, et al. "The MASCOT landing area on asteroid (162173) Ryugu: Stereo-photogrammetric analysis using images of the ONC onboard the Hayabusa2 spacecraft." Astronomy & Astrophysics 632 (December 2019): L4. http://dx.doi.org/10.1051/0004-6361/201936759.

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A high-resolution 3D surface model, map-projected to a digital terrain model (DTM), and precisely ortho-rectified context images (orthoimages) of MASCOT landing site area are important data sets for the scientific analysis of relevant data that have been acquired with MASCOT’s image camera system MASCam and other instruments (e.g., the radiometer MARA and the magnetometer MASMag). We performed a stereo-photogrammetric (SPG) analysis of 1050 images acquired from the Hayabusa2 Optical Navigation Camera system (ONC) during the asteroid characterization phase and the MASCOT release phase in early
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34

Liu, Z., X. Chen, X. Li, and F. Jia. "A Framework of High-precision State Estimation for Approaching, Orbiting, and Touching an Asteroid." Journal of Physics: Conference Series 2239, no. 1 (2022): 012007. http://dx.doi.org/10.1088/1742-6596/2239/1/012007.

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Abstract High-precision state estimation lies at the core of asteroid exploration. This paper investigates the high-precision state estimation methods in asteroid approaching, orbiting, and touching phases. The system and measurement models are established, and state estimation strategies are designed respectively for each phase. In the approaching phase, the star image is used to directly determine the relative orbit of the spacecraft to the target asteroid. To improve the optical state estimation precision, a deceleration-orientation-deceleration strategy is developed. In the orbiting phase,
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35

Liu, Keping, Fengxia Liu, Shenquan Wang, and Yuanchun Li. "Finite-Time Spacecraft’s Soft Landing on Asteroids Using PD and Nonsingular Terminal Sliding Mode Control." Mathematical Problems in Engineering 2015 (2015): 1–10. http://dx.doi.org/10.1155/2015/510618.

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This paper presents a continuous control law of probe, which consists of PD (proportional-derivative) controller and nonsingular terminal sliding mode controller for probe descending and landing phases, respectively, in the case of the asteroid irregular shape and low gravity. The probe dynamic model is deduced in the landing site coordinate system firstly. Then the reference trajectory based on optimal polynomial in open-loop state is designed, with the suboptimal fuel consumption. Taking into account different characteristics of phases, PD controller and nonsingular terminal sliding mode con
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36

Chengyu Zhang, 张成渝, 梁潇 Xiao Liang, 吴奋陟 Fenzhi Wu, and 张琳 Lin Zhang. "Overview of optical navigation for asteroid exploration descent and landing." Infrared and Laser Engineering 49, no. 5 (2020): 20201009. http://dx.doi.org/10.3788/irla.15_invited-zhangchengyu.

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Quan, Qiquan, Tingzhang Wang, Hao Guan, Dewei Tang, and Zongquan Deng. "Electromagnetic damping asteroid landing cushioning mechanism and dynamic simulation analysis." Advances in Space Research 69, no. 7 (2022): 2756–69. http://dx.doi.org/10.1016/j.asr.2022.01.015.

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38

Ogawa, Naoko, Fuyuto Terui, and Jun'ichiro Kawaguchi. "Precise Landing of Space Probe on Asteroid Using Multiple Markers." IFAC Proceedings Volumes 43, no. 15 (2010): 172–77. http://dx.doi.org/10.3182/20100906-5-jp-2022.00030.

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39

Yang, Hongwei, Xiaoli Bai, and Hexi Baoyin. "Rapid Trajectory Planning for Asteroid Landing with Thrust Magnitude Constraint." Journal of Guidance, Control, and Dynamics 40, no. 10 (2017): 2713–20. http://dx.doi.org/10.2514/1.g002346.

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40

Yang, Hongwei, and Hexi Baoyin. "Fuel-optimal control for soft landing on an irregular asteroid." IEEE Transactions on Aerospace and Electronic Systems 51, no. 3 (2015): 1688–97. http://dx.doi.org/10.1109/taes.2015.140295.

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41

Zhu, Lingchao, and Shuquan Wang. "Orbit-Attitude Coupled Tracking and Landing Control for an Asteroid." IOP Conference Series: Materials Science and Engineering 685 (November 22, 2019): 012003. http://dx.doi.org/10.1088/1757-899x/685/1/012003.

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42

Zhang, Bo, and Yuanli Cai. "Twistor-based pose control for asteroid landing with path constraints." Nonlinear Dynamics 100, no. 3 (2020): 2427–48. http://dx.doi.org/10.1007/s11071-020-05610-w.

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43

Chen, Gang, Peilin Cai, Yifan Wang, Long Zhang, and Ji Liang. "Trajectory Optimization for Asteroid Landing Considering Gravitational Orbit-Attitude Coupling." IEEE Access 7 (2019): 126464–78. http://dx.doi.org/10.1109/access.2019.2938821.

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44

Tsuda, Yuichi, Takanao Saiki, Fuyuto Terui, Satoru Nakazawa, Makoto Yoshikawa, and Sei-ichiro Watanabe. "Hayabusa2 mission status: Landing, roving and cratering on asteroid Ryugu." Acta Astronautica 171 (June 2020): 42–54. http://dx.doi.org/10.1016/j.actaastro.2020.02.035.

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45

Dias, Nicole G., Paulo Gordo, Hugo Onderwater, Rui Melicio, and António Amorim. "Analysis on the Isostatic Bipod Mounts for the HERA Mission LIDAR." Applied Sciences 12, no. 7 (2022): 3497. http://dx.doi.org/10.3390/app12073497.

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The Light Detection and Ranging (LIDAR) is a time-of-flight altimeter instrument being developed for the HERA mission, designated as Planetary ALTimeter (PALT). PALT is positioned in the center of the top face of the HERA probe, and therefore, it cannot use radiators to stabilize its internal temperature. The contribution of this paper is the design of isostatic bipod mounts for the LIDAR primary mirror. The performance of PALT must be maintained over a wide operational range, from −60 °C to 80 °C. These temperature requirements imply that a careful isostatic mount structure design is critical
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46

Mathavaraj, S., and Radhakant Padhi. "Quasi-Spectral Unscented MPSP Guidance for Robust Soft-Landing on Asteroid." Journal of Optimization Theory and Applications 191, no. 2-3 (2021): 823–45. http://dx.doi.org/10.1007/s10957-021-01953-5.

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47

Cheng, Lin, Zhenbo Wang, Fanghua Jiang, and Junfeng Li. "Fast Generation of Optimal Asteroid Landing Trajectories Using Deep Neural Networks." IEEE Transactions on Aerospace and Electronic Systems 56, no. 4 (2020): 2642–55. http://dx.doi.org/10.1109/taes.2019.2952700.

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48

Veverka, J., B. Farquhar, M. Robinson, et al. "The landing of the NEAR-Shoemaker spacecraft on asteroid 433 Eros." Nature 413, no. 6854 (2001): 390–93. http://dx.doi.org/10.1038/35096507.

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49

Sun, Zibin, Lin Cheng, and Shengping Gong. "Semi-analytic approximate time-optimal asteroid landing with dimensionality reduction shooting." Acta Astronautica 225 (December 2024): 729–40. http://dx.doi.org/10.1016/j.actaastro.2024.09.032.

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Kubota, Takashi, Tatsuaki Hashimoto, Shujiro Sawai, et al. "An autonomous navigation and guidance system for MUSES-C asteroid landing." Acta Astronautica 52, no. 2-6 (2003): 125–31. http://dx.doi.org/10.1016/s0094-5765(02)00147-9.

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