(2016 LC11)
Tracked by NASA JPL Near-Earth Object Web Service (NeoWs), (2016 LC11) is a Unreported by NASA NeoWs body measuring between 330.03m and 737.97m in diameter. On 2026-11-08, it completes a cislunar approach at 179.80 Lunar Distances (69,147,004.5 km) with a relative heliocentric velocity of 28.78 km/s.
(2016 LC11) (JPL ID 3753874) is a Unreported by NASA NeoWs Near-Earth Asteroid spanning 330.0m–738.0m (mean 534m). On 2026-11-08, it transits Earth's cislunar surveillance sector at 179.803 Lunar Distances (69,147,005 km) with a relative velocity of 28.78 km/s and a theoretical kinetic energy reserve of 22488.83 megatons TNT. Its well-constrained heliocentric ephemeris passes safely outside Earth capture corridors while serving as an orbital calibration target.
Exact Landmark Scale Comparison (737.97m)
Kinetic Impact Physics & Orbital Parameters
(2016 LC11) (H = 19.5, 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 (2016 LC11) compared to city landmarks?
(2016 LC11) has an estimated diameter between 330.03m and 737.97m. At its upper-bound size of 737.97m, it stands 167% as tall as the 443m Empire State Building in New York City and 224% of the 330m Eiffel Tower.
What does the stored 2026-11-08 close-approach estimate show?
This catalog snapshot lists a nominal miss distance of 179.80 Lunar Distances (69,147,004.5 km) for (2016 LC11). This is not an impact prediction; check the latest NASA JPL record for updated orbital estimates. The 3D impact simulation is hypothetical.
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.