Overview
- Goldstone Solar System Radar captured 41 high-resolution images of asteroid 2025 OW during its July 28 flyby at 1.6 lunar distances.
- Radar measurements reveal the 60-meter object has an irregular monolithic structure and spins once every 1.5–3 minutes.
- Detailed observations reduced trajectory uncertainties and confirmed that 2025 OW’s July 28 approach is its closest for the foreseeable future.
- JPL’s Center for Near-Earth Object Studies refined the asteroid’s orbit to rule out any imminent impact risk.
- This successful tracking and characterization demonstrate the effectiveness of NASA’s planetary defense monitoring systems.