(2005 EW169)
Tracked by NASA JPL Near-Earth Object Web Service (NeoWs), (2005 EW169) is a Unreported by NASA NeoWs body measuring between 310.85m and 695.09m in diameter. On 2026-11-05, it completes a cislunar approach at 109.25 Lunar Distances (42,014,074.6 km) with a relative heliocentric velocity of 14.91 km/s.
(2005 EW169) (JPL ID 3274302) is a Unreported by NASA NeoWs Near-Earth Asteroid spanning 310.9m–695.1m (mean 503m). On 2026-11-05, it transits Earth's cislunar surveillance sector at 109.249 Lunar Distances (42,014,075 km) with a relative velocity of 14.91 km/s and a theoretical kinetic energy reserve of 5046.58 megatons TNT. Classified as a Potentially Hazardous Asteroid (PHA) due to its Minimum Orbit Intersection Distance (MOID <= 0.05 AU) and absolute magnitude (H <= 22.0), it remains under high-priority radar and optical astrometric tracking.
Exact Landmark Scale Comparison (695.09m)
Kinetic Impact Physics & Orbital Parameters
(2005 EW169) (H = 19.7, Vmag ≈ 18.4) 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 (2005 EW169) compared to city landmarks?
(2005 EW169) has an estimated diameter between 310.85m and 695.09m. At its upper-bound size of 695.09m, it stands 157% as tall as the 443m Empire State Building in New York City and 211% 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 109.25 Lunar Distances (42,014,074.6 km) for (2005 EW169). 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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