SATPC0038199 Tab 07 SOW_Redacted.pdf
PDF 343 KB Posted
- Attached to
- Cubert Hyperspectral Light Field Camera Federal contract opportunity
- Solicitation number
- 80NSSC25901438Q
About this file
This Statement of Work (SOW) details the requirements for the Autonomous Science and Technology for Responsive Adaptability (ASTRA) project, which aims to develop an artificial intelligence agent for complex decision-making on spaceflight-relevant robotic vehicles. The project specifically requires a hyperspectral imager with specific technical specifications: wavelength range of 350-1000 nm, less than 500g weight, greater than 30-degree field of view, mosaic bandpass filter, and at least 5 nm spectral sampling resolution. The proposed solution is the ULTRIS X20 Light Field Camera, which meets these requirements with 164 spectral bands, 20MP sensor size, and a typical 35-degree field of view. The performance will take place at NASA Goddard Space Flight Center's Planetary Environments Laboratory in Greenbelt, MD, with testing scheduled from June 2025 through August 2026, and an estimated delivery lead time of 8-12 weeks after receipt of order.
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STATEMENT OF WORK
1. Objective/Requirements
The Autonomous Science and Technology for Responsive Adaptability (ASTRA) project goals are to develop and test an artificial intelligence (AI) agent designed specifically for onboard complex decision-making that can adapt to updated mission priorities. To achieve these goals within the fiscal year timeline, ASTRA requires a hyperspectral imager that has a low enough Size, Weight, and Power (SWAP) to be integrated onto and used on a variety of spaceflight-relevant robotic vehicles (e.g., uncrewed aerial systems, ballons, small rovers). Specifically, ASTRA requires a payload that is less than 500 g. ASTRA also requires a hyperspectral imager that has greater than 30-degree field of view, a mosaic bandpass filter, and at least 5 nm spectral sampling resolution in order to perform the required tests.
2. Characteristics, Scope, and Specs
The imager/spectrometer shall perform the following duties and specifications:
Perform hyperspectral imaging and spectral graphing over the wavelength range of
350 1000 nm.
Perform imaging and spectral sampling in laboratory and outdoor environments.
Perform spectral sampling at a resolution of 5 nm.
Perform bandpass filtering using a mosaic.
Capture images and spectra over a 30 degree field of view.
Maintain a standalone mass of < 500 g.
LINE PART NO. DESCRIPTION QTY.
1 X20 ULTRIS X20 Light Field Camera Wavelength range: 350 - 1000 nm Sensor size: 20MP Spectral Bands: 164 Spectral Sampling: 4nm FWHM: Constant 10 nm Spatial Resolution: 410 x 410px (168,100 spectra/cube) Data Depth: 12bit Max. Frame Rate: 8 Hz Data Link: GigE Field 0f View (FOV): typ. 35° Weight: 350g Size: 57x60x60mm
2 Flight Lite U Flight Lite Package Cubert CUVIS HSI Software Cubert Touch (GUI) & Core for Windows Cubert CubeExport Cubert SDK (Python, C++, C#) Radiometric Calibration Flight Recorder Pokini F2 (Mini PC) for customized / mobile solutions USG SiRFIV USB GPS Receiver Camera Accessory Package (cables, protection case, power supply, reference target)
3. Place of Performance
Code 699, Planetary Environments Laboratory NASA Goddard Space Flight Center Greenbelt, MD
4. Period of Performance
ASTRA testing will begin during June 2025 and is projected to continue through August 2026 with opportunities for follow-on activities.
Estimated delivery lead-time is 8/12 weeks ARO.
File details come from the government source that posted it. Updated .