(2009 WA)
Tracked by NASA JPL Near-Earth Object Web Service (NeoWs), (2009 WA) is a Unreported by NASA NeoWs body measuring between 153.66m and 343.59m in diameter. On 2026-11-07, it completes a cislunar approach at 87.37 Lunar Distances (33,598,737.1 km) with a relative heliocentric velocity of 18.13 km/s.
(2009 WA) (JPL ID 3476774) is a Unreported by NASA NeoWs Near-Earth Asteroid spanning 153.7m–343.6m (mean 248.6m). On 2026-11-07, it transits Earth's cislunar surveillance sector at 87.367 Lunar Distances (33,598,737 km) with a relative velocity of 18.13 km/s and a theoretical kinetic energy reserve of 900.28 megatons TNT. Its well-constrained heliocentric ephemeris passes safely outside Earth capture corridors while serving as an orbital calibration target.
Exact Landmark Scale Comparison (343.59m)
Kinetic Impact Physics & Orbital Parameters
(2009 WA) (H = 21.2, Vmag ≈ 19.4) 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 (2009 WA) compared to city landmarks?
(2009 WA) has an estimated diameter between 153.66m and 343.59m. At its upper-bound size of 343.59m, it stands 78% as tall as the 443m Empire State Building in New York City and 104% 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 87.37 Lunar Distances (33,598,737.1 km) for (2009 WA). 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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