Current state of the multi-agent multi-view experimental and digital twin rendezvous (MMEDR-Autonomous) framework
Authors: Logan Banker, Michael Wozniak, Mohanad Alameer, Smriti Nandan Paul, David Meisinger, Grant Baer, Trevor Hunting, Ryan Dunham, Jay Kamdar
Organizations: Department of Mechanical and Aerospace Engineering, Missouri University of Science and Technology, Rolla, 65409, MO, United States · Purdue University, 610 Purdue Mall, West Lafayette, 47907, USA
As near-Earth resident space objects proliferate, there is an increasing demand for reliable technologies in applications of on-orbit servicing, debris removal, and orbit modification. Rendezvous and docking are critical mission phases for such applications and can benefit from greater autonomy to reduce operational complexity and human workload. Machine learning-based methods can be integrated within the guidance, navigation, and control (GNC) architecture to design a robust rendezvous and docking framework. In this work, the Multi-Agent Multi-View Experimental and Digital Twin Rendezvous (MMEDR-Autonomous) is introduced as a unified framework comprising a learning-based optical navigation network, a reinforcement learning-based guidance approach under ongoing development, and a hardware-in-the-loop testbed. Navigation employs a lightweight monocular pose estimation network with multi-scale feature fusion, trained on realistic image augmentations to mitigate domain shift. The guidance component is examined with emphasis on learning stability, reward design, and systematic hyperparameter tuning under mission-relevant constraints. Prior Control Barrier Function results for Clohessy-Wiltshire dynamics are reviewed as a basis for enforcing safety and operational constraints and for guiding future nonlinear controller design within the MMEDR-Autonomous framework. The MMEDR-Autonomous framework is currently progressing toward integrated experimental validation in multi-agent rendezvous scenarios.
Figures & tables
Figure 1: Chaser and Target Spacecraft in LVLH Frame, Figure Adapted from Khoury (2020)
Figure 2: Overall CNN Architecture for Optical Navigation, Based on Combination of MobileNetV3Large, FPN, and Deep-6DPose ( Howard et al., 2019 ; Lin et al., 2017 ; Do et al., 2018 )
Augment Type
Probability - Lightbox
Probability - Sunlamp
Brightness and Contrast
0.8
0.8
Gaussian Noise
0.7
0.8
Motion Blur
0.7
0.8
ISO Noise
0.7
0.8
Gamma
0.6
0.7
Sun Flare
-
0.7
Table 1: List of Augmentations and Probability of Application
Figure 3: Current State of the DCV-Space Testing Facility
Figure 4: CR20A Link Dimensions
Link
θ
d (mm)
a (mm)
α (deg)
1
θ1
230
0
90
2
θ2
0
825.2
0
3
θ3
0
746
0
4
θ4
175.6
0
-90
5
θ5
128.8
0
90
6
θ6
136.5
0
0
Table 2: D-H Parameters for Dobot CR20A Robot
Figure 5: Overview of All MMEDR Subsystems
Figure 6: Docking Results from Manual Shaping and a 50m Initial Distance
Figure 7: Successful Iterations of Bayesian optimization
Figure 8: Bayesian optimization Trajectory with Velocity Constraints
Training
Lightbox
Sunlamp
Augments
Et (m)
Eq ( ∘ )
Ep∗ (-)
Et (m)
Eq ( ∘ )
Ep∗ (-)
Without
1.95
76.25
1.65
1.93
89.59
1.85
With
0.36
45.65
0.86
0.52
66.74
1.28
Table 3: Testing Results for Lightbox and Sunlamp Domains, With and Without Data Augmentation (Described in Section 4.2.1 )
Model
Lightbox
Sunlamp
Et (m)
Eq ( ∘ )
Ep∗ (-)
Et (m)
Eq ( ∘ )
Ep∗ (-)
SPN
0.45
65.12
1.21
0.65
92.95
1.73
KRN
2.25
44.53
1.12
14.64
80.95
3.73
Ours
0.36
45.65
0.86
0.52
66.74
1.28
Table 4: Comparison of Synthetic-Only Training, Tested on Lightbox and Sunlamp Domains
Figure 9: Synthetic Images of the Aura Spacecraft Generated in Blender
Spacecraft rendezvous and proximity operations cover the navigation, guidance, and control needed to approach, inspect, dock with, or capture spacecraft safely.
Department of Aeronautics and Astronautics, Massachusetts Institute of Technology, Cambridge, MA 02139, USA · Los Alamos National Laboratory, Los Alamos, NM, USA