Engineers attach the aluminum telescope for NASA’s NEO
Surveyor to the flight base frame at Space Dynamics Laboratory in Logan, Utah,
in September 2025. The telescope is connected via a system of struts that
prevents heat from passing from the spacecraft to the instrument.
Space Dynamics Laboratory/Allison Bills
The Near-Earth Object (NEO) Surveyor —
NASA’s first infrared space telescope purposely designed to discover
potentially hazardous asteroids and comets — is undergoing integration and
testing. With launch set for no earlier than September 2027, teams across the
United States are hard at work building the spacecraft’s components, planning
the kind of survey and science it will do, and developing the software to
process the huge quantity of data the mission will generate.
In 2005, Congress tasked NASA with
discovering potentially hazardous near-Earth objects, or NEOs, but many of
these objects are difficult to find with ground-based surveys. Some are as dark
as charcoal, others are tiny, and many lurk in the glare of the Sun, where
ground-based optical telescopes can’t see. To mitigate this, NEO Surveyor is being custom-built to scan the
solar system to detect objects that will glow in the infrared as they are
heated by the Sun — as opposed to the optical light they reflect, which is what
ground-based surveys measure — to provide enough advance warning for humanity
to do something about them, if necessary.
The spacecraft will travel about a
million miles (1.5 million kilometers) from our planet in the direction of the
Sun to a region of gravitational stability called the Sun-Earth Lagrange point (or L1 point), continuously scanning large swaths of the sky for
at least five years in search of NEOs that have yet to be found.
The bus structure of NASA’s NEO Surveyor, shown here,
underwent a round of testing at BAE Systems Space & Mission Systems in
Boulder, Colorado, in August 2025. The bus houses the power, propulsion,
avionics, and communication subsystems, all isolated from the telescope and
sensitive detectors.
BAE Systems Space & Mission Systems
“NEO Surveyor is a one-of-a-kind mission designed to solve a specific
challenge: finding asteroids and comets that pose the greatest risk to Earth,”
said Jim Fanson, the mission’s project manager at NASA’s Jet Propulsion
Laboratory in Southern California. “Our focus is on deploying a robust
observatory to the Sun-Earth L1 point, where it will conduct a continuous,
multi-year infrared survey. By identifying objects that ground telescopes can
miss, this mission will provide the critical data we need to safeguard our
planet for years to come.”
Modular approach
Having been assembled at JPL, both the spacecraft’s infrared telescope and its instrument enclosure are undergoing integration and testing at Utah
State University’s Space Dynamics Laboratory (SDL) in Logan. An angular
structure measuring 12 feet (3.7 meters) long, the instrument enclosure
protects the spacecraft’s telescope and removes heat that could otherwise
affect the heat-sensitive infrared observations. Project engineers plan
to carry out focus tests in a chamber at SDL that simulates the extreme
environment of deep space to ensure the instrument works as designed and the
camera remains in focus at very cold temperatures and in zero gravity.
The camera is composed of two detector arrays, tuned to generate detailed images of asteroids and
comets within two infrared bands. Each array creates a 16-megapixel mosaic of
the sky. Imaging the same part of the sky over the two infrared bands enables
the instrument to measure an asteroid or comet’s temperature, yielding an
estimate of the object’s size.
The spacecraft will also sport a 20-foot-long (6-meter-long) sunshade that allows it to look close to the Sun by
blocking glare from entering the telescope’s aperture. By far the largest
feature of NEO Surveyor, the structure also has solar panels on its Sun-facing
surface to generate the electricity to power the spacecraft’s systems.
At BAE Systems Space & Mission Systems in Boulder, Colorado, the
sunshade is currently undergoing tests with the spacecraft’s bus, which houses power, propulsion, avionics, and
communication subsystems. The integrated telescope and enclosure will from SDL
to travel to BAE Systems, where they will complete the spacecraft.
Science, data, survey strategy
Meanwhile, the mission’s science team is busy planning ways to harness the
full capabilities of this cutting-edge spacecraft.
“We have a multi-institutional team, from seasoned scientists to
undergraduate students, with a broad expertise in infrared mission design,”
said Amy Mainzer, the mission’s lead at University of California, Los Angeles
(UCLA). “We are currently working to develop the most efficient survey strategy
that the mission will use to detect some of the hardest-to-find asteroids in
our solar system, plus any comets that may be headed our way.”
When the mission’s data comes to Earth via NASA’s Deep Space Network, it will go to the NEO Surveyor Survey Data Center at
Caltech’s IPAC in Pasadena, California. Responsible for processing and
calibrating the huge number of observations that the spacecraft delivers, the
center will also produce images and source catalogs for archiving at the
NASA/IPAC Infrared Science Archive.
After identifying the moving objects in the data, IPAC will report them to the Minor Planet Center (MPC), the international clearinghouse for all position measurements of minor bodies in our solar system and responsible entity for designating new discoveries. This data can then be used by planetary defense groups, including JPL’s Center for Near Earth Object Studies (CNEOS), which calculates the orbits for all known asteroids and comets while also predicting the impact risk for hazardous objects many years into the future. The Department of Earth, Planetary, and Space Sciences at UCLA will plan the survey and deliver measurements of the asteroid and comet sizes and other physical properties to public archives every six months.
Source: NASA’s Next-Gen Near-Earth Asteroid Space Telescope Takes Shape - NASA Science


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