NEO Surveyor update: 20-foot tall sunshade for NASA's asteroid hunter now ready

NEO Surveyor's sunshade stands at 20 feet tall and is 8 feet wide at its base. It will serve a dual purpose on the mission—keeping the infrared space telescope cool and providing the spacecraft with power.
The large sunshade of NASA’s Near-Earth Object Surveyor mission is inspected by a technician at BAE Systems Space & Mission Systems in Boulder, Colorado, in late July (Cover Image Source: BAE Systems Space & Mission Systems)
The large sunshade of NASA’s Near-Earth Object Surveyor mission is inspected by a technician at BAE Systems Space & Mission Systems in Boulder, Colorado, in late July (Cover Image Source: BAE Systems Space & Mission Systems)

NASA’s Near-Earth Object (NEO) Surveyor is another step closer to its mission. Teams have finished integrating solar arrays onto the telescope’s sunshade, according to an update by the agency on Monday. The overall process was performed at BAE Systems Space & Mission Systems in Boulder, Colorado. The structure will play a crucial dual role: shielding the telescope from the Sun’s glare and generating power for the spacecraft as it searches for potentially hazardous asteroids and comets.

The first space-based telescope aimed at detecting a large number of asteroids and comets that could pose a threat to Earth, NEO Surveyor is scheduled for launch in September 2027. Standing at a height of approximately 20 feet and having a width of 8 feet at its base, the sunshade is the biggest component of the spacecraft. Its two flat panels are joined at an angle of 23.5 degrees and carry 864 interconnected solar cells.

The sunshade started its journey at Applied Aerospace in Stockton, California, where it was built. It was later moved to SolAero Technologies in Albuquerque, New Mexico, where technicians installed the solar cells onto it in January, giving the array a peak output of 2 kilowatts, which will be enough to charge the batteries onboard the spacecraft. In March, the sunshade passed environmental testing at a facility in El Segundo, California, after which it traveled to BAE Systems Space & Mission Systems in Boulder, Colorado, in May. There, engineers integrated Sun sensors, which will help determine the spacecraft’s orientation, and temperature sensors onto the sunshade, while also putting the solar array through functional and performance testing.

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 (Image Source: Space Dynamics Laboratory/Allison Bills)

After launch, the spacecraft will travel to the Sun-Earth Lagrange point 1, or L1, located at around 1 million miles (1.5 million kilometers) from Earth. From there, it will survey vast portions of the sky continuously for a minimum of five years, looking for near-Earth objects (NEOs) not yet discovered. NEO Surveyor will view the same region of sky in two infrared wavelength bands, with each of the telescope's pair of detector arrays generating a 16-megapixel mosaic of the sky. A comparison of the data obtained from these two bands will allow scientists to determine an object's temperature, and, from that, its size. Furthermore, these findings can be paired with the target's location and motion readings, and researchers can then assess which near-Earth objects could pose a threat to Earth.

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 (Image Source: BAE Systems Space & Mission Systems)

The concept of NEO Surveyor originated when Congress directed NASA in 2005 to find potentially hazardous NEOs. It has been seen that observations conducted from the Earth are incapable of spotting these objects, as they can may not be bright enough, may be small-sized, or maybe shielded by sunlight. NEO Surveyor is specifically designed to overcome this by detecting the infrared glow of objects warmed by the Sun, rather than the reflected visible light that ground-based observations depend on. The goal is to give humanity enough advance warning to respond if needed.

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