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At a glance

Why do we need NEOSM?

Space may be vast, but it’s not empty. Earth is bombarded by tiny space rocks called meteors every day, most of which burn up in our atmosphere. Larger meteors, like the one that exploded over Chelyabinsk, Russia in 2013, can damage buildings and cause minor injuries. And on rare occasions, asteroids and comets strike Earth and cause global devastation—the dinosaurs perished when this happened 66 million years ago.

Know your foes

Fortunately, NASA and other space agencies are working on tests to deflect near-Earth objects (NEOs) on course to hit our planet. But before we can stop them, we have to find them. In 2005, the U.S. Congress ordered NASA to find 90% of the estimated 25,000 NEOs larger than 140 meters—the size threshold at which an object can level an entire city. The deadline was 2020. So far, we’ve found just 37%. At our current detection rate, it will take more than 30 years to meet this mandate.

Right now, ground-based telescopes are the primary means of detecting NEOs, but they have limitations. They can’t search during bad weather, and there aren’t enough in the southern hemisphere. Furthermore, since they can’t scan the sky during daytime, many objects coming from directions near the Sun often go undetected. The solution? Park a space telescope between Earth and the Sun and scan regions of space we can’t see well from Earth.  

This is the impetus behind NEOSM, NASA’s Near-Earth Object Surveillance Mission. NEOSM would launch as soon as 2025 and within 10 years meet Congress’s goal of finding 90% of near-Earth objects 140 meters and wider. Finding and studying these objects will not only help us figure out if any are on course to hit Earth, but will also help lay the groundwork for survey and deflection missions if one is found. 

Asteroid Apophis radar images

NASA/JPL-Caltech

Asteroid Apophis radar images
These images of asteroid Apophis were captured by radar in 2012. In 2029, the 370-meter-wide space rock will come as close as 31,300 kilometers (19,400 miles) from Earth—closer than most communications satellites.

A truly awesome mission

Mission team members have been overheard pronouncing NEOSM as “nee-awesome.” Whether or not that pronunciation becomes official as the mission moves toward launch remains to be seen!

How NEOSM will look for potentially hazardous asteroids

NEOSM will park itself at the Sun-Earth L1 point—a spot 1.5 million kilometers (930,000 miles) away from Earth where the gravitational pull from the Sun and Earth balance each other out, allowing spacecraft to hang around indefinitely without using much fuel. From this location, NEOSM will look ahead of and behind Earth’s orbital path, spotting asteroids that we otherwise wouldn’t be able to see because of the Sun’s glare.

Sun-Earth Lagrange Points

Wikimedia Commons / User Xander89

Sun-Earth Lagrange Points
Lagrange points, named after mathematician Joseph-Louis Lagrange, are locations around two bodies where the gravitational pull from each body balances out, allowing a spacecraft to hang around indefinitely without using much fuel.

NEOSM is a 50-centimeter-wide telescope. Its camera sees things in infrared wavelengths—a type of light not visible to human eyes. Infrared light reveals heat signatures, which is perfect for asteroids because they are very dark and hard to see against the blackness of space. In infrared light, they glow because they heat up in the Sun and re-radiate that heat back into space. 

NEOSM is both a replacement and an improvement upon NASA’s current asteroid-hunting space telescope, NEOWISE. NEOWISE launched in 2009 and was originally an astrophysics telescope before being repurposed as an asteroid hunter in 2013. Though NEOWISE has discovered hundreds of asteroids, it is not optimized for the job in ways NEOSM will be. NEOWISE has a smaller telescope mirror and sits in Earth orbit, which limits its search capabilities. Its orbit is currently drifting to the point where it will soon be unable to observe asteroids without stray light entering the telescope. 

What you can do to support NEOSM

After years of neglecting NASA’s planetary defense budget, Congress finally began increasing it, and in 2019 NASA announced it would formally pursue the NEOSM mission. But the agency’s latest budget request, which is developed under the direction of the White House, only included enough funding for NEOSM to develop the telescope’s camera—not enough for the entire mission. You can help by writing your members of Congress and asking them to fund the mission.

Help us get NEOSM funded

Planetary defense is one of The Planetary Society's top priorities. An asteroid or comet impact is the only preventable, large-scale natural disaster, and we are committed to working with Congress and NASA to make the NEOSM mission a reality. Sign up for our Space Advocate newsletter to stay informed of when we need you to take action and help. 

You can also learn more about our broader Planetary Defense efforts, including our Shoemaker NEO Grant program. We fund amateur and professional astronomers around the world working to find, track, and study NEOs.

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