Integrated Optical Payloads and High-Bandwidth RF Data Acquisition for Deep Space Missions

Integrated Optical Payloads and High-Bandwidth RF Data Acquisition for Deep Space Missions Date: May 9, 2026 Abstract This proposal outlines a high-performance system architecture for deep-space reconnaissance. It addresses the critical synchronization between diffraction-limited photo-optics and Ka-band radio-frequency (RF) data acquisition. By integrating a silicon-carbide optical bench with FPGA-based signal processing, the system overcomes the data bottleneck, allowing for the transmission of high-density imagery over interplanetary distances with minimal signal degradation. 1. Optical Subsystem Specifications The imaging payload is designed for high-resolution reconnaissance under extreme thermal and vacuum conditions. * Optical Configuration: A Ritchey-Chrétien (RC) reflective system utilizing a 300mm primary mirror. * Substrate Material: Reaction-Bonded Silicon Carbide (SiC) to ensure a high stiffness-to-weight ratio and thermal stability. * Detector: A radiation-hardened Back-Illuminated (BSI) CMOS Sensor optimized for high Quantum Efficiency (QE) in low-photon environments. * Focal Length: 2400mm, providing sub-meter ground sample distance (GSD) from orbital altitudes. 2. Data Acquisition and On-Board Processing To manage the high-volume output of the optical subsystem, a dedicated data-handling pipeline is utilized: * Storage: 2TB Space-Qualified Solid State Recorder (SSR) utilizing a high-speed NVMe interface. * Preprocessing: Real-time lossless wavelet compression (standard CCSDS 122.0) executed via Field Programmable Gate Array (FPGA) to reduce the telemetry footprint. * Packetization: Data is encapsulated into AOS (Advanced Orbiting Systems) frames for seamless integration with Earth-based ground stations. 3. Radio Frequency (RF) Signal Chain The communication architecture is optimized for long-range, high-bandwidth data return. * Frequency Band: Ka-Band (32 GHz) for high-throughput science data downlink. * Antenna System: 1.5-meter High-Gain Antenna (HGA) with dual-axis gimbaling for precise Earth-pointing. * Modulation and Coding: Implementation of 16-APSK modulation and Low-Density Parity-Check (LDPC) codes to maximize data rates at low Signal-to-Noise Ratios (SNR). * Link Budget: Designed for a minimum 100 Mbps downlink at 1 AU (Astronomical Unit). 4. System Integration and Mission Profile The proposal follows a Store-and-Forward operational cycle: 5. Phase I (Acquisition): Targeted high-speed optical capture during planetary flybys. 6. Phase II (Processing): Autonomous on-board data prioritization and compression. 7. Phase III (Transmission): Programmed downlink windows via the Deep Space Network (DSN) using optimized RF signal bursts. 8. Conclusion The integration of high-aperture optics with high-frequency radio signals represents a significant advancement in deep-space data return. This unified architecture ensures that high-fidelity scientific imagery can be acquired and successfully transmitted across the solar system, providing a scalable blueprint for future interstellar missions. Keywords: Space Optics, Data Acquisition, Ka-Band, Satellite Imaging, RF Signal Processing, Aerospace Engineering.