(2013 NG10)
Tracked by NASA JPL Near-Earth Object Web Service (NeoWs), (2013 NG10) is a Unreported by NASA NeoWs body measuring between 76.66m and 171.41m in diameter. On 2026-11-06, it completes a cislunar approach at 169.55 Lunar Distances (65,204,888.3 km) with a relative heliocentric velocity of 14.24 km/s.
(2013 NG10) (JPL ID 3644814) is a Unreported by NASA NeoWs Near-Earth Asteroid spanning 76.7m–171.4m (mean 124m). On 2026-11-06, it transits Earth's cislunar surveillance sector at 169.553 Lunar Distances (65,204,888 km) with a relative velocity of 14.24 km/s and a theoretical kinetic energy reserve of 68.99 megatons TNT. Its well-constrained heliocentric ephemeris passes safely outside Earth capture corridors while serving as an orbital calibration target.
Exact Landmark Scale Comparison (171.41m)
Kinetic Impact Physics & Orbital Parameters
(2013 NG10) (H = 22.7, Vmag ≈ 22.4) 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 (2013 NG10) compared to city landmarks?
(2013 NG10) has an estimated diameter between 76.66m and 171.41m. At its upper-bound size of 171.41m, it stands 39% as tall as the 443m Empire State Building in New York City and 52% of the 330m Eiffel Tower.
What does the stored 2026-11-06 close-approach estimate show?
This catalog snapshot lists a nominal miss distance of 169.55 Lunar Distances (65,204,888.3 km) for (2013 NG10). 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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