ATLAS

Planetary Defense at Survey Scale - Enabled by DFM Optics

ATLAS in Action
ATLAS Model
ATLAS Optics
ATLAS Optics
ATLAS Optic Testing
ATLAS Optic Testing
ATLAS Mirror Cell
ATLAS Finished Mirror
ATLAS OTA being built
ATLAS Shutter Assembly
ATLAS with Dr. DFM: Dr. Frank Melsheimer
ATLAS with John Tonry
ATLAS Installed

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.

  • Learn More: Focus Stability. Why holding focus matters more than finding it.

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.

  • Learn More:  Space Domain Awareness - From survey cadence to custody cadence. Same engineering.

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:

  • Planetary defense discoveries
    More than 1,315 near-Earth asteroids, over 112 potentially hazardous asteroids, and about 111 comets identified to date, with discoveries flowing directly into the Minor Planet Center and JPL’s Scout system so impact probabilities can be evaluated quickly.
  • Third known interstellar object:
    3I/ATLAS (C/2025 N1) was discovered by the Chilean ATLAS telescope, only the third confirmed interstellar object, on a strongly hyperbolic orbit that constrains the properties of small bodies passing through the Solar System from interstellar space.
  • DART impact imaging for planetary defense
    Time-sequence imaging of NASA’s DART impact into Dimorphos, providing wide-field ground based context on plume evolution and ejecta dynamics that complements spacecraft and space telescope data and helps quantify the momentum transfer achieved.
  • ATLAS variable-star catalogs
    ATLAS-VAR produced about 4.7 million candidate variables from light curves of roughly 140 million stars with at least 100 observations each. The first main catalog lists hundreds of thousands of probable variables, including over 300,000 new objects across pulsators, eclipsing binaries, and irregular variables, supporting broad studies of stellar evolution and variability.
  • Young supernovae and fast transients
    ATLAS contributes at global scale to transient discovery. The ATLAS project lists over 5,000 supernovae in its discovery totals.  With wide sky coverage and a roughly two-day cadence, ATLAS ranks among the top global contributors to the IAU Transient Name Server, with hundreds of supernova candidates per year. It also discovers cataclysmic variables, stellar outbursts, gamma-ray burst afterglows, and other fast optical events, and participates in LIGO follow up to search for neutron-star merger counterparts.

Technical Snapshot

  • NASA-funded operational early warning system developed and operated by the University of Hawaiʻi.
  • f/2.0 wide-field survey telescope design with a 7.4° field of view listed in ATLAS technical specifications.
  • Focus stability engineered mechanically to preserve PSF uniformity, astrometry, and photometry at survey cadence.
  • Large full-aperture shutter proven over 10 million cycles and counting.
  • Discovery totals reported by the ATLAS project include 1,315 NEAs, 112 PHAs, 111 comets, and 5,005 supernovae.
  • 3I/ATLAS discovered July 1, 2025 by the NASA-funded ATLAS telescope in Chile.

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.

  • Learn More: Engineered to Endure - Built for duty cycle, not first light.

What ATLAS Demonstrates in Operations

  • ATLAS operates as an early-warning survey network. That validates wide-field optics as production infrastructure, not episodic science hardware.
  • Fast f/2 survey optics paired with a 7.4° field sustained high-étendue cadence at scale. That is how ATLAS covers enormous area without sacrificing measurement-grade quality.
  • Mechanically stabilized focus preserved PSF and centroid consistency across long nights. That protects astrometry and photometry when cadence is the metric.
  • A full-aperture shutter exceeding 10 million cycles demonstrates duty-cycle reliability. That matters when the system is expected to run nightly.
  • ATLAS outcomes at global scale demonstrate throughput in the field. That is the standard a survey node must meet before it can be trusted in SDA networks.

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.

  • Learn More:  Space Domain Awareness - From survey cadence to custody cadence. Same engineering.

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.