(2012 PZ19)
Tracked by NASA JPL Near-Earth Object Web Service (NeoWs), (2012 PZ19) is a Unreported by NASA NeoWs body measuring between 32.7m and 73.12m in diameter. On 2026-11-05, it completes a cislunar approach at 98.83 Lunar Distances (38,008,117.4 km) with a relative heliocentric velocity of 12.75 km/s.
(2012 PZ19) (JPL ID 3607528) is a Unreported by NASA NeoWs Near-Earth Asteroid spanning 32.7m–73.1m (mean 52.9m). On 2026-11-05, it transits Earth's cislunar surveillance sector at 98.833 Lunar Distances (38,008,117 km) with a relative velocity of 12.75 km/s and a theoretical kinetic energy reserve of 4.29 megatons TNT. Its well-constrained heliocentric ephemeris passes safely outside Earth capture corridors while serving as an orbital calibration target.
Exact Landmark Scale Comparison (73.12m)
Kinetic Impact Physics & Orbital Parameters
(2012 PZ19) (H = 24.6, 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 (2012 PZ19) compared to city landmarks?
(2012 PZ19) has an estimated diameter between 32.7m and 73.12m. At its upper-bound size of 73.12m, it stands 17% as tall as the 443m Empire State Building in New York City and 22% of the 330m Eiffel Tower.
What does the stored 2026-11-05 close-approach estimate show?
This catalog snapshot lists a nominal miss distance of 98.83 Lunar Distances (38,008,117.4 km) for (2012 PZ19). 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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