1862 Apollo (1932 HA)
Tracked by NASA JPL Near-Earth Object Web Service (NeoWs), 1862 Apollo (1932 HA) is a Q-type (Silicate Apollo Prototype) body measuring between 1200m and 1500m in diameter. On 2026-10-31, it completes a cislunar approach at 11.40 Lunar Distances (4,382,160 km) with a relative heliocentric velocity of 21.40 km/s.
Exact Landmark Scale Comparison (1500m)
Kinetic Impact Physics & Orbital Parameters
1862 Apollo (1932 HA) (H = 16.3, Vmag ≈ 9.9) 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 1862 Apollo (1932 HA) compared to city landmarks?
1862 Apollo (1932 HA) has an estimated diameter between 1200m and 1500m. At its upper-bound size of 1500m, it stands 339% as tall as the 443m Empire State Building in New York City and 455% of the 330m Eiffel Tower.
Will 1862 Apollo (1932 HA) impact Earth during its 2026-10-31 approach?
No. NASA JPL Center for Near-Earth Object Studies (CNEOS) orbital solutions confirm 1862 Apollo (1932 HA) will pass safely at a minimum distance of 11.40 Lunar Distances (4,382,160 km). You can still simulate a hypothetical street-level impact in our 3D CesiumJS simulator.
High-transmission BaK-4 Porro prism 15x70 optics with tripod adapter for bright near-Earth flybys, comets, and bolide shower radiants.
Autonomous apochromatic triplet smart telescope with integrated plate-solving, live stacking, and dual-band filter for magnitude 10–16 NEOs.
Ultra-portable Sony IMX678 starlight tele-camera with AI equatorial tracking and automated asteroid field stacking.
Authentic coarse octahedrite Group IAB iron-nickel meteorite fragment (92.9% Fe, 6.7% Ni) recovered from the Chaco crater field.
Low-read-noise Sony STARVIS 2 CMOS planetary and all-sky meteor bolide detection camera with 2.0μm pixels.