Live NASA Data
NASA asteroid
tracker
Live close approach data from NASA's NeoWs API, refreshed every 30 minutes. The table below shows every upcoming asteroid flyby currently in the NASA catalogue - miss distances, estimated sizes, velocities, and hazard classifications.
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Next five approaches
The nearest upcoming flybys, sorted by date. Data from NASA NeoWs. Updated every 30 minutes.
All upcoming approaches
Full sortable table from the NASA NeoWs feed. Filter by hazard status, sort by date, distance, or size, and switch between lunar distances, kilometres, and AU.
| Name | Date | Est. Diameter | Miss Distance(LD) | Velocity | Hazard | |
|---|---|---|---|---|---|---|
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Reading the data
Miss distance in this tracker is given in lunar distances (LD). One LD equals 384,400 km - the average Earth-Moon distance. An asteroid at 1 LD passes at the same distance as the Moon. At 10 LD, it is ten times farther. Raw kilometres are shown alongside for reference.
Estimated diameter is given as a range because size calculations depend on the assumed surface reflectivity (albedo). Dark asteroids must be larger to appear equally bright as paler ones. Until an asteroid is observed by radar or imaged by a spacecraft, the size estimate carries inherent uncertainty.
Velocity is the asteroid's speed relative to Earth at closest approach. Most near-Earth asteroids pass at between 20,000 and 100,000 km/h. The encounter typically lasts a few hours at most.
The amber "Hazardous" badge marks potentially hazardous asteroids (PHAs) - objects 140 metres or larger with orbits passing within 0.05 AU of Earth's orbital path. This is a monitoring classification. None of the objects shown carry a meaningful impact probability.
How NASA tracks asteroids
Ground-based survey telescopes photograph the same region of sky several times in one night. Software compares frames and flags objects that have moved between exposures. That movement is the signature of a nearby solar system body.
Confirmed detections are reported to the International Astronomical Union's Minor Planet Center, which assigns a provisional designation and coordinates follow-up observations. Multiple nights of tracking let CNEOS compute an orbital solution - a mathematical model of the object's path around the Sun.
The orbital solution feeds into close-approach predictions, which appear in the NeoWs feed used by this tracker. For newly discovered objects, the uncertainty on miss distance can be large - sometimes spanning millions of kilometres. It shrinks rapidly as more observations come in.
Related pages
Next close approach
Live countdown to the next recorded flyby with full approach card.
What is CNEOS?
The NASA centre that produces all asteroid tracking data.
What is a near-Earth object?
How NEOs are defined and how the catalogue is built.
How NASA discovers asteroids
The survey telescopes and methods behind new detections.