(2016 WB10)
Tracked by NASA JPL Near-Earth Object Web Service (NeoWs), (2016 WB10) is a Unreported by NASA NeoWs body measuring between 178.88m and 399.98m in diameter. On 2026-11-07, it completes a cislunar approach at 129.05 Lunar Distances (49,630,513.3 km) with a relative heliocentric velocity of 16.22 km/s.
(2016 WB10) (JPL ID 3764887) is a Unreported by NASA NeoWs Near-Earth Asteroid spanning 178.9m–400.0m (mean 289.4m). On 2026-11-07, it transits Earth's cislunar surveillance sector at 129.054 Lunar Distances (49,630,513 km) with a relative velocity of 16.22 km/s and a theoretical kinetic energy reserve of 1136.73 megatons TNT. Its well-constrained heliocentric ephemeris passes safely outside Earth capture corridors while serving as an orbital calibration target.
Exact Landmark Scale Comparison (399.98m)
Kinetic Impact Physics & Orbital Parameters
(2016 WB10) (H = 20.9, Vmag ≈ 19.9) 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 WB10) compared to city landmarks?
(2016 WB10) has an estimated diameter between 178.88m and 399.98m. At its upper-bound size of 399.98m, it stands 90% as tall as the 443m Empire State Building in New York City and 121% of the 330m Eiffel Tower.
What does the stored 2026-11-07 close-approach estimate show?
This catalog snapshot lists a nominal miss distance of 129.05 Lunar Distances (49,630,513.3 km) for (2016 WB10). 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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