Mission Control/ASTEROID DOSSIER: (2019 UN4)
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NOMINAL CISLUNAR PASSAGEGEMMA ENGINE: LOCAL SERVER BOX [ACTIVE] • meteors-gemma:latest

(2019 UN4)

Tracked by NASA JPL Near-Earth Object Web Service (NeoWs), (2019 UN4) is a Q-type (Olivine-Pyroxene) body measuring between 73.21m and 163.7m in diameter. On 2026-10-20, it completes a cislunar approach at 81.80 Lunar Distances (31,456,932.5 km) with a relative heliocentric velocity of 11.28 km/s.

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

(2019 UN4) (JPL ID 3879533) is a Q-type (Olivine-Pyroxene) Near-Earth Asteroid spanning 73.2m–163.7m (mean 118.5m). On 2026-10-20, it transits Earth's cislunar surveillance sector at 81.798 Lunar Distances (31,456,933 km) with a relative velocity of 11.28 km/s and a theoretical kinetic energy reserve of 37.76 megatons TNT. Its well-constrained heliocentric ephemeris passes safely outside Earth capture corridors while serving as an orbital calibration target.

Max Diameter (Ø)
163.7 m
Min: 73.21 m
Miss Distance
81.80 LD
31,456,932.5 km
Rel. Velocity
11.28 km/s
40,612 km/h
Kinetic Energy
104.795 MT
E = ½mv² TNT eq.

Exact Landmark Scale Comparison (163.7m)

1:1 Meter Scale
163.7m
(2019 UN4)
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)22.8 mag
Spectral ClassificationQ-type (Olivine-Pyroxene)
Estimated Bolide Mass6.891e+9 kg
Kinetic Energy (E = ½mv²)104.795 MT TNT (4.39e+17 J)
Transient Crater Diameter / Depth2,638 m Ø / 554 m deep
5-PSI Structural Overpressure Radius9.05 km
Thermal 3rd-Degree Burn Radius18.86 km
Equivalent Seismic MagnitudeMw 6
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 +20.82
Abs. Magnitude H = 22.80
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: (2019 UN4)

(2019 UN4) (H = 22.8, Vmag ≈ 20.8) is below consumer optical detection thresholds (requires ≥1000mm survey aperture); explore certified meteorite specimens[↗] or indoor optical projection instead.

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3D Ephemeris Trajectory Waypoints

Node T+0Lat 16.41° · Lon -153.25°136,800 km
Node T+1Lat 22.92° · Lon -143.67°122,617 km
Node T+2Lat 28.06° · Lon -134.08°109,667 km
Node T+3Lat 31.67° · Lon -124.50°97,950 km
Node T+4Lat 33.67° · Lon -114.92°87,467 km
Node T+5Lat 34.01° · Lon -105.33°78,217 km

Planetary Defense Frequently Asked Questions (Schema.org FAQ)

How big is (2019 UN4) compared to city landmarks?

(2019 UN4) has an estimated diameter between 73.21m and 163.7m. At its upper-bound size of 163.7m, it stands 37% as tall as the 443m Empire State Building in New York City and 50% of the 330m Eiffel Tower.

Will (2019 UN4) impact Earth during its 2026-10-20 approach?

No. NASA JPL Center for Near-Earth Object Studies (CNEOS) orbital solutions confirm (2019 UN4) will pass safely at a minimum distance of 81.80 Lunar Distances (31,456,932.5 km). You can still simulate a hypothetical street-level impact in our 3D CesiumJS simulator.

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(2019 UN4) — 3D Orbit, Size Comparison & Kinetic Impact Physics | Meteors.ai Space Network