Mission Control/ASTEROID DOSSIER: (2018 DA2)
GEMMA ENGINE: LOCAL SERVER BOX [ACTIVE]Launch in 3D City Impact Simulator
NOMINAL CISLUNAR PASSAGEGEMMA ENGINE: LOCAL SERVER BOX [ACTIVE] • meteors-gemma:latest

(2018 DA2)

Tracked by NASA JPL Near-Earth Object Web Service (NeoWs), (2018 DA2) is a X-type (Enstatite-Metallic) body measuring between 58.69m and 131.23m in diameter. On 2026-10-25, it completes a cislunar approach at 153.13 Lunar Distances (58,890,104.1 km) with a relative heliocentric velocity of 14.73 km/s.

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

(2018 DA2) (JPL ID 3799748) is a X-type (Enstatite-Metallic) Near-Earth Asteroid spanning 58.7m–131.2m (mean 95m). On 2026-10-25, it transits Earth's cislunar surveillance sector at 153.132 Lunar Distances (58,890,104 km) with a relative velocity of 14.73 km/s and a theoretical kinetic energy reserve of 33.16 megatons TNT. Its well-constrained heliocentric ephemeris passes safely outside Earth capture corridors while serving as an orbital calibration target.

Max Diameter (Ø)
131.23 m
Min: 58.69 m
Miss Distance
153.13 LD
58,890,104.1 km
Rel. Velocity
14.73 km/s
53,014 km/h
Kinetic Energy
91.996 MT
E = ½mv² TNT eq.

Exact Landmark Scale Comparison (131.23m)

1:1 Meter Scale
131.23m
(2018 DA2)
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)23.28 mag
Spectral ClassificationX-type (Enstatite-Metallic)
Estimated Bolide Mass3.550e+9 kg
Kinetic Energy (E = ½mv²)91.996 MT TNT (3.85e+17 J)
Transient Crater Diameter / Depth2,497 m Ø / 524 m deep
5-PSI Structural Overpressure Radius8.67 km
Thermal 3rd-Degree Burn Radius17.88 km
Equivalent Seismic MagnitudeMw 5.9
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 +22.78
Abs. Magnitude H = 23.28
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: (2018 DA2)

(2018 DA2) (H = 23.3, Vmag ≈ 22.8) 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 0.85° · Lon 171.90°136,800 km
Node T+1Lat 4.63° · Lon -178.52°122,617 km
Node T+2Lat 7.74° · Lon -168.93°109,667 km
Node T+3Lat 10.10° · Lon -159.35°97,950 km
Node T+4Lat 11.67° · Lon -149.77°87,467 km
Node T+5Lat 12.43° · Lon -140.18°78,217 km

Planetary Defense Frequently Asked Questions (Schema.org FAQ)

How big is (2018 DA2) compared to city landmarks?

(2018 DA2) has an estimated diameter between 58.69m and 131.23m. At its upper-bound size of 131.23m, it stands 30% as tall as the 443m Empire State Building in New York City and 40% of the 330m Eiffel Tower.

Will (2018 DA2) impact Earth during its 2026-10-25 approach?

No. NASA JPL Center for Near-Earth Object Studies (CNEOS) orbital solutions confirm (2018 DA2) will pass safely at a minimum distance of 153.13 Lunar Distances (58,890,104.1 km). You can still simulate a hypothetical street-level impact in our 3D CesiumJS simulator.

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(2018 DA2) — 3D Orbit, Size Comparison & Kinetic Impact Physics | Meteors.ai Space Network