Mission Control/ASTEROID DOSSIER: (2019 UM6)
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NOMINAL CISLUNAR PASSAGEGEMMA ENGINE: LOCAL SERVER BOX [ACTIVE] • meteors-gemma:latest

(2019 UM6)

Tracked by NASA JPL Near-Earth Object Web Service (NeoWs), (2019 UM6) is a M-type (Metallic Nickel-Iron) body measuring between 78.08m and 174.6m in diameter. On 2026-10-26, it completes a cislunar approach at 120.54 Lunar Distances (46,355,017.5 km) with a relative heliocentric velocity of 8.96 km/s.

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

(2019 UM6) (JPL ID 3879718) is a M-type (Metallic Nickel-Iron) Near-Earth Asteroid spanning 78.1m–174.6m (mean 126.3m). On 2026-10-26, it transits Earth's cislunar surveillance sector at 120.537 Lunar Distances (46,355,018 km) with a relative velocity of 8.96 km/s and a theoretical kinetic energy reserve of 53.69 megatons TNT. Its well-constrained heliocentric ephemeris passes safely outside Earth capture corridors while serving as an orbital calibration target.

Max Diameter (Ø)
174.6 m
Min: 78.08 m
Miss Distance
120.54 LD
46,355,017.5 km
Rel. Velocity
8.96 km/s
32,270 km/h
Kinetic Energy
80.285 MT
E = ½mv² TNT eq.

Exact Landmark Scale Comparison (174.6m)

1:1 Meter Scale
174.6m
(2019 UM6)
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)22.66 mag
Spectral ClassificationM-type (Metallic Nickel-Iron)
Estimated Bolide Mass8.361e+9 kg
Kinetic Energy (E = ½mv²)80.285 MT TNT (3.36e+17 J)
Transient Crater Diameter / Depth2,508 m Ø / 527 m deep
5-PSI Structural Overpressure Radius8.29 km
Thermal 3rd-Degree Burn Radius16.91 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 +21.59
Abs. Magnitude H = 22.66
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 UM6)

(2019 UM6) (H = 22.7, Vmag ≈ 21.6) is below consumer optical detection thresholds (requires ≥1000mm survey aperture); explore certified meteorite specimens[↗] or indoor optical projection instead.

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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.

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3D Ephemeris Trajectory Waypoints

Node T+0Lat -4.81° · Lon -41.90°136,800 km
Node T+1Lat -2.02° · Lon -32.32°122,617 km
Node T+2Lat 0.34° · Lon -22.73°109,667 km
Node T+3Lat 2.25° · Lon -13.15°97,950 km
Node T+4Lat 3.67° · Lon -3.57°87,467 km
Node T+5Lat 4.58° · Lon 6.02°78,217 km

Planetary Defense Frequently Asked Questions (Schema.org FAQ)

How big is (2019 UM6) compared to city landmarks?

(2019 UM6) has an estimated diameter between 78.08m and 174.6m. At its upper-bound size of 174.6m, it stands 39% as tall as the 443m Empire State Building in New York City and 53% of the 330m Eiffel Tower.

Will (2019 UM6) impact Earth during its 2026-10-26 approach?

No. NASA JPL Center for Near-Earth Object Studies (CNEOS) orbital solutions confirm (2019 UM6) will pass safely at a minimum distance of 120.54 Lunar Distances (46,355,017.5 km). You can still simulate a hypothetical street-level impact in our 3D CesiumJS simulator.

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(2019 UM6) — 3D Orbit, Size Comparison & Kinetic Impact Physics | Meteors.ai Space Network