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VLWIR Sensors for Detecting and Tracking Near-Earth Asteroids

Award Information
Agency: National Aeronautics and Space Administration
Branch: N/A
Contract: 80NSSC18C0113
Agency Tracking Number: 175522
Amount: $749,426.00
Phase: Phase II
Program: SBIR
Solicitation Topic Code: S1
Solicitation Number: SBIR_17_P2
Timeline
Solicitation Year: 2017
Award Year: 2018
Award Start Date (Proposal Award Date): 2018-04-25
Award End Date (Contract End Date): 2020-04-24
Small Business Information
22 Cotton Road, Unit H, Suite 180, Nashua, NH, 03063-4219
DUNS: 168454770
HUBZone Owned: N
Woman Owned: N
Socially and Economically Disadvantaged: N
Principal Investigator
 Mani Sundaram
 (603) 821-3092
 msundaram@qmagiq.com
Business Contact
 Mani Sundaram
Phone: (603) 821-3092
Email: msundaram@qmagiq.com
Research Institution
N/A
Abstract

An important NASA mission is to detect, count and track near-earth asteroids for a variety of reasons including the hazards of collisions with our planet. Such asteroids are mostly dark, small and cold (~ 200K); so they are best detected in the very longwave infrared (VLWIR) wavelengths greater than ~ 12 microns where they glow brightest. To accomplish this, we developed in Phase I a record-performing focal plane array (FPA) of antimony-based strained layer superlattices (SLS) with cutoff wavelength = 13.5 microns, quantum efficiency = 30-50% in the 3.0-13.5 micron spectral band, dark current = 1/4th that of incumbent mercury cadmium telluride (MCT) per Rule07,  and operating with background-limited-performance (BLIP) at 75K with superb array uniformity, operability and image stability.  In Phase II, we propose to increase array format to 1024x1024, integrate the FPA with three spectral filters (one fire channel and two thermal channels), and package it into a compact camera.  The camera will be delivered to NASA for evaluation for missions like Landsat Data Continuity Mission - Thermal Infrared Sensor (LDCM-TIRS), where it will offer greater ground resolution in a small, lightweight, low-power package.

* Information listed above is at the time of submission. *

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