101955 Bennu (1999 RQ36)
Tracked by NASA JPL Near-Earth Object Web Service (NeoWs), 101955 Bennu (1999 RQ36) is a B-type (Carbonaceous Rubble Pile) body measuring between 480m and 510m in diameter. On 2026-10-20, it completes a cislunar approach at 4.92 Lunar Distances (1,891,248 km) with a relative heliocentric velocity of 27.88 km/s.
Exact Landmark Scale Comparison (510m)
Kinetic Impact Physics & Orbital Parameters
101955 Bennu (1999 RQ36) (H = 20.2, Vmag ≈ 12.0) 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 101955 Bennu (1999 RQ36) compared to city landmarks?
101955 Bennu (1999 RQ36) has an estimated diameter between 480m and 510m. At its upper-bound size of 510m, it stands 115% as tall as the 443m Empire State Building in New York City and 155% of the 330m Eiffel Tower.
Will 101955 Bennu (1999 RQ36) impact Earth during its 2026-10-20 approach?
No. NASA JPL Center for Near-Earth Object Studies (CNEOS) orbital solutions confirm 101955 Bennu (1999 RQ36) will pass safely at a minimum distance of 4.92 Lunar Distances (1,891,248 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.