Carbon Nano-Tube Polymer Composite Mirrors for CubeSat Telescopes
Find Innovative SolutionsGenerate Solutions
Solution Overview
Problem
Current optical telescopes for CubeSat spacecraft are constrained by size, mass, and spectral range limitations, making them unsuitable for compact, cost-efficient, and mass-producible solutions for deep space planetary science investigations and communication systems, particularly in the UV-VIS-IR range.
Innovation Solution
A compact, lightweight, cost-efficient UV-VIS-IR 1U-2U CubeSat telescope with a fast focal-ratio, reflective optics design using carbon nano-tube polymer matrix composite primary and secondary mirrors, capable of mass manufacture, and an optical coupling interface for commercial-off-the-shelf spectrometers, allowing for efficient integration with CubeSat configurations.
Engineering Contradictions & Design Principles
Engineering Contradiction Analysis
1Measurement precision
If traditional optical telescopes are used for CubeSat, then spectral range and imaging quality are improved, but size, mass, and manufacturing cost increase
Solution Approach 1:
The patent employs carbon nano-tube polymer matrix composite materials to fabricate telescope mirrors, combining the lightweight properties of carbon nanotubes with polymer matrices to achieve high strength-to-weight ratio while maintaining structural integrity for optical applications
Solution Approach 2:
The patent utilizes 3D printing technology to create mandrels with precise geometric parameters that define the final mirror shape, enabling complex optical surfaces to be manufactured with controlled dimensional accuracy without traditional polishing processes
2Measurement precision
If traditional optical telescopes are used for CubeSat, then optical performance is improved, but manufacturing cost and production time increase
Solution Approach 1:
The patent creates reusable 3D printed mandrels that can be replicated to produce multiple identical telescope mirrors, enabling mass production and reducing per-unit manufacturing costs through standardized tooling and processes
Solution Approach 2:
The patent replaces traditional mechanical polishing and figure-setting processes with 3D printing technology, allowing direct fabrication of optical surfaces from digital models without requiring skilled labor-intensive manual polishing operations
3Volume of moving object
If telescope size is reduced for CubeSat constraints, then volume and mass are reduced, but optical performance and spectral range deteriorate
Solution Approach 1:
The patent divides the telescope system into modular components including separate primary and secondary mirrors, allowing each element to be independently optimized and manufactured, then assembled to achieve the required overall optical performance within volume constraints
Solution Approach 2:
The patent employs curved reflective surfaces with optimized radii of curvature to achieve effective focal lengths and spectral coverage that would require larger aperture diameters in traditional flat-mirror designs, maximizing optical performance within compact volumes
4Weight of moving object
If fast focal-ratio reflective optics are used, then mass and complexity are reduced, but manufacturing precision requirements increase
Solution Approach 1:
The patent replaces traditional mechanical polishing processes with 3D printing technology, where the mandrel geometry directly defines the mirror surface figure, eliminating the need for high-precision manual polishing while maintaining surface accuracy through digital modeling control
Applied Scientific Principles
This section explains which scientific principles are used to turn an abstract innovation direction into a practical engineering solution.
Function Achieved in This Case
Enables low-cost, low-mass instrumentation for array or swarm CubeSat configurations, supporting lunar, planetary, and Earth science investigations, as well as spacecraft communication systems, by providing wide wavelength coverage and rapid instrument integration within stringent volume and mass constraints.
Implementation Method 1
reflective optics design using carbon nano-tube polymer matrix composite primary and secondary mirrors
Data Source
AI summary
The present invention relates to a compact, lightweight, cost-efficient ultraviolet-visible-far infrared (UV-VIS-IR) telescope system, covering the 300 nm to 2500 nm (0.3 μm to 2.5 μm) spectral range, based on a fast focal-ratio, reflective optics design, and an optical coupling interface appropriate for COTS spectrometers, commensurate with about 1U-2U CubeSat payload volume.


