Planetary Defense at Survey Scale - Enabled by DFM Optics
ATLAS is NASA’s operational early warning network for hazardous near-Earth objects, developed and operated by the University of Hawaiʻi. It scans enormous sky area at high cadence to find small impactors with days to weeks of warning. DFM designed and built the f/2.0, 7.4° wide-field optical systems at the core of each telescope, delivering the étendue, uniform image quality, and focus stability that make survey data reliable at scale.
Mission: Last Alert Before Impact
ATLAS is not a general-purpose observatory. It is a dedicated planetary defense system designed to detect small impactors with days to weeks of warning, support civil defense decision-making, and refine our understanding of near-Earth small-body populations.
Operational reality is simple. Survey success depends on repeatable image quality across thousands of pointings, and on astrometry and photometry that remain stable as the night cools. DFM’s role is to protect the optical behavior that makes the data trustworthy.
The Enabling Hardware: Fast Optics Plus a Wide, Corrected Field
ATLAS relies on optics that combine very fast focal ratios with a large, corrected field. At f/2.0, small focus shifts broaden the PSF and bias centroids. ATLAS protects measurement consistency by stabilizing the optical prescription mechanically rather than relying on constant refocusing, keeping the survey pipeline fed with uniform data.
DFM’s optical assemblies are built to deliver wide-field image quality suitable for large-format detectors and pipeline-grade measurements. The aim is not a peak lab result. The aim is repeatable performance across the full observing program.
From Planetary Defense to Space Domain Awareness
Although ATLAS was built for planetary defense, its survey behavior aligns directly with modern Space Domain Awareness (SDA) needs. Wide-area discovery, time-domain characterization, and statistical sampling of faint populations are the same design problems SDA faces when optical speed, field of view, and cadence must work as one system.
ATLAS demonstrates that wide-field survey nodes can run reliably night after night as production infrastructure, and that optics are not merely a component - they are the capability.
Science and Mission Highlights
ATLAS has become one of the most productive time-domain survey systems in operation, translating high étendue and cadence into actionable awareness in a dynamic sky.
Highlights Include:
DFM's Role in ATLAS
DFM provided the optical assemblies that define ATLAS’s collecting power and field of view. This includes optical design, fabrication, verification, and mechanical design for stable behavior in real observatory conditions.
DFM also designed and manufactured the large full-aperture shutter, proven over 10 million cycles. ATLAS demonstrates what DFM is built to deliver. Wide-field systems that run reliably as production infrastructure. Optics are not merely a component. They are the capability.
What ATLAS Demonstrates in Operations
Bring ATLAS-Class Survey Capability into Your Next Program
Join the programs that set the benchmark for wide-field sky surveys. DFM’s work on ATLAS reflects a broader heritage spanning beam director trackers, debris monitoring, and SDA-class survey systems that deliver proven performance behind discoveries, custody, and characterization. The same design principles that make ATLAS effective for planetary defense now underpin DFM’s LEO ScopeTM and HS-series products for modern SDA architectures.
If your program depends on reliable detection, precision pointing, and proven throughput, connect with us to evaluate how ATLAS-grade capability can be tailored to your mission and deployed as a system or network.