(2016 UX80)
Tracked by NASA JPL Near-Earth Object Web Service (NeoWs), (2016 UX80) is a Unreported by NASA NeoWs body measuring between 34.4m and 76.92m in diameter. On 2026-10-31, it completes a cislunar approach at 101.64 Lunar Distances (39,089,492.1 km) with a relative heliocentric velocity of 19.60 km/s.
(2016 UX80) (JPL ID 3762437) is a Unreported by NASA NeoWs Near-Earth Asteroid spanning 34.4m–76.9m (mean 55.7m). On 2026-10-31, it transits Earth's cislunar surveillance sector at 101.645 Lunar Distances (39,089,492 km) with a relative velocity of 19.60 km/s and a theoretical kinetic energy reserve of 11.84 megatons TNT. Its well-constrained heliocentric ephemeris passes safely outside Earth capture corridors while serving as an orbital calibration target.
Exact Landmark Scale Comparison (76.92m)
Kinetic Impact Physics & Orbital Parameters
(2016 UX80) (H = 24.4, Vmag ≈ 23.0) is below consumer optical detection thresholds (requires ≥1000mm survey aperture); explore certified meteorite specimens[↗] or indoor optical projection instead.
Campo del Cielo Meteorite Specimen (Certified Iron-Nickel)
Authentic coarse octahedrite Group IAB iron-nickel meteorite fragment (92.9% Fe, 6.7% Ni) recovered from the Chaco crater field with certificate of authenticity.
Satin-black 5W warm-white LED optical glass lens planetarium projecting 60,000 stars and simulated meteor shower trajectories indoors.
3D Ephemeris Trajectory Waypoints
Planetary Defense Frequently Asked Questions (Schema.org FAQ)
How big is (2016 UX80) compared to city landmarks?
(2016 UX80) has an estimated diameter between 34.4m and 76.92m. At its upper-bound size of 76.92m, it stands 17% as tall as the 443m Empire State Building in New York City and 23% of the 330m Eiffel Tower.
What does the stored 2026-10-31 close-approach estimate show?
This catalog snapshot lists a nominal miss distance of 101.64 Lunar Distances (39,089,492.1 km) for (2016 UX80). This is not an impact prediction; check the latest NASA JPL record for updated orbital estimates. The 3D impact simulation is hypothetical.
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Authentic coarse octahedrite Group IAB iron-nickel meteorite fragment (92.9% Fe, 6.7% Ni) recovered from the Chaco crater field.
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