Learn β AsteroidWatch
A near-Earth object (NEO) is an asteroid or comet whose orbit brings it into Earthβs neighborhood as it loops around the Sun. The vast majority are near-Earth asteroids (NEAs) β rocky leftovers from the formation of the solar system. When one passes relatively near our planet, astronomers call it a βclose approach,β a flyby on the objectβs own orbit. Despite the name, βcloseβ here is astronomical: most close approaches happen millions of kilometres away.
- Near-Earth objects and close approachesWhat makes an object βnear-Earth,β what a close approach really is, and why βcloseβ usually means millions of kilometres away.
- How asteroid size and orbits are measuredBrightness and albedo give a size estimate; tracking an object across the sky pins down its orbit, MOID and velocity.
- Impact-hazard scales and monitoringWhat βpotentially hazardousβ actually means, how the Torino and Palermo scales communicate risk, and how Sentry watches automatically.
- Putting impact risk in contextHow often objects of each size actually arrive, and how planetary defense β surveys and missions like DART β turns a passive watch into an active one.