Mission Control/ASTEROID DOSSIER: (2002 CN15)
GEMMA ENGINE: LOCAL SERVER BOX [ACTIVE]Launch in 3D City Impact Simulator
NOMINAL CISLUNAR PASSAGEGEMMA ENGINE: LOCAL SERVER BOX [ACTIVE] • meteors-gemma:latest

(2002 CN15)

Tracked by NASA JPL Near-Earth Object Web Service (NeoWs), (2002 CN15) is a X-type (Enstatite-Metallic) body measuring between 183.89m and 411.19m in diameter. On 2026-10-25, it completes a cislunar approach at 57.78 Lunar Distances (22,219,932.4 km) with a relative heliocentric velocity of 26.64 km/s.

LOCAL SERVER-BOX GEMMA SYNTHESIS (http://127.0.0.1:11434/v1):

(2002 CN15) (JPL ID 3114028) is a X-type (Enstatite-Metallic) Near-Earth Asteroid spanning 183.9m–411.2m (mean 297.5m). On 2026-10-25, it transits Earth's cislunar surveillance sector at 57.779 Lunar Distances (22,219,932 km) with a relative velocity of 26.64 km/s and a theoretical kinetic energy reserve of 3333.61 megatons TNT. Its well-constrained heliocentric ephemeris passes safely outside Earth capture corridors while serving as an orbital calibration target.

Max Diameter (Ø)
411.19 m
Min: 183.89 m
Miss Distance
57.78 LD
22,219,932.4 km
Rel. Velocity
26.64 km/s
95,922 km/h
Kinetic Energy
9,265.253 MT
E = ½mv² TNT eq.

Exact Landmark Scale Comparison (411.19m)

1:1 Meter Scale
411.19m
(2002 CN15)
443m
Manhattan
227m
Golden Gate
330m
Eiffel Tower
828m
Burj Khalifa
Inspect side-by-side in interactive Google Earth 3D Tiles:Open 3D Street-Level Simulator

Kinetic Impact Physics & Orbital Parameters

45° Incidence · 3,000 kg/m³
Absolute Magnitude (H)20.8 mag
Spectral ClassificationX-type (Enstatite-Metallic)
Estimated Bolide Mass1.092e+11 kg
Kinetic Energy (E = ½mv²)9,265.253 MT TNT (3.88e+19 J)
Transient Crater Diameter / Depth7,899 m Ø / 1,659 m deep
5-PSI Structural Overpressure Radius39.73 km
Thermal 3rd-Degree Burn Radius118.46 km
Equivalent Seismic MagnitudeMw 7.3
Primary Ephemeris Source:NASA JPL Small-Body Database Lookup
OPTICAL TRACKING REQUIREMENTS // PHOTOMETRIC LINK
TIER C: PLANETARY RADAR / SPECIMEN GRADE
Calculated Apparent Magnitude (Vmag)
Vmag +18.02
Abs. Magnitude H = 20.80
Required Aperture (mm)
≥ 1000 mm (Planetary Radar)
Professional ≥1000mm Survey CCD / Planetary Bistatic Radar Telemetry
Best Viewing Window
JPL Goldstone Radar / Vera C. Rubin LSST Ephemeris Window Only
Target: (2002 CN15)

(2002 CN15) (H = 20.8, Vmag ≈ 18.0) is below consumer optical detection thresholds (requires ≥1000mm survey aperture); explore certified meteorite specimens[↗] or indoor optical projection instead.

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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 with certificate of authenticity.

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3D Ephemeris Trajectory Waypoints

Node T+0Lat -11.88° · Lon -4.50°136,800 km
Node T+1Lat -10.34° · Lon 5.08°122,617 km
Node T+2Lat -8.89° · Lon 14.67°109,667 km
Node T+3Lat -7.56° · Lon 24.25°97,950 km
Node T+4Lat -6.33° · Lon 33.83°87,467 km
Node T+5Lat -5.22° · Lon 43.42°78,217 km

Planetary Defense Frequently Asked Questions (Schema.org FAQ)

How big is (2002 CN15) compared to city landmarks?

(2002 CN15) has an estimated diameter between 183.89m and 411.19m. At its upper-bound size of 411.19m, it stands 93% as tall as the 443m Empire State Building in New York City and 125% of the 330m Eiffel Tower.

Will (2002 CN15) impact Earth during its 2026-10-25 approach?

No. NASA JPL Center for Near-Earth Object Studies (CNEOS) orbital solutions confirm (2002 CN15) will pass safely at a minimum distance of 57.78 Lunar Distances (22,219,932.4 km). You can still simulate a hypothetical street-level impact in our 3D CesiumJS simulator.

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(2002 CN15) — 3D Orbit, Size Comparison & Kinetic Impact Physics | Meteors.ai Space Network