(2007 RV9)
Tracked by NASA JPL Near-Earth Object Web Service (NeoWs), (2007 RV9) is a Unreported by NASA NeoWs body measuring between 227.28m and 508.21m in diameter. On 2026-10-31, it completes a cislunar approach at 40.50 Lunar Distances (15,576,264 km) with a relative heliocentric velocity of 13.70 km/s.
(2007 RV9) (JPL ID 3384068) is a Unreported by NASA NeoWs Near-Earth Asteroid spanning 227.3m–508.2m (mean 367.7m). On 2026-10-31, it transits Earth's cislunar surveillance sector at 40.503 Lunar Distances (15,576,264 km) with a relative velocity of 13.70 km/s and a theoretical kinetic energy reserve of 1663.96 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 (508.21m)
Kinetic Impact Physics & Orbital Parameters
(2007 RV9) (H = 20.3, Vmag ≈ 16.8) 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 (2007 RV9) compared to city landmarks?
(2007 RV9) has an estimated diameter between 227.28m and 508.21m. At its upper-bound size of 508.21m, it stands 115% as tall as the 443m Empire State Building in New York City and 154% of the 330m Eiffel Tower.
What does the stored 2026-10-31 close-approach estimate show?
This catalog snapshot lists a nominal miss distance of 40.50 Lunar Distances (15,576,264 km) for (2007 RV9). 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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