Mission Control/ASTEROID DOSSIER: (2017 KU4)
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NOMINAL CISLUNAR PASSAGEGEMMA ENGINE: LOCAL SERVER BOX [ACTIVE] • meteors-gemma:latest

(2017 KU4)

Tracked by NASA JPL Near-Earth Object Web Service (NeoWs), (2017 KU4) is a S-type (Silicate Stony) body measuring between 46.19m and 103.29m in diameter. On 2026-10-21, it completes a cislunar approach at 149.20 Lunar Distances (57,376,893.3 km) with a relative heliocentric velocity of 18.69 km/s.

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

(2017 KU4) (JPL ID 3774725) is a S-type (Silicate Stony) Near-Earth Asteroid spanning 46.2m–103.3m (mean 74.7m). On 2026-10-21, it transits Earth's cislunar surveillance sector at 149.197 Lunar Distances (57,376,893 km) with a relative velocity of 18.69 km/s and a theoretical kinetic energy reserve of 25.97 megatons TNT. Its well-constrained heliocentric ephemeris passes safely outside Earth capture corridors while serving as an orbital calibration target.

Max Diameter (Ø)
103.29 m
Min: 46.19 m
Miss Distance
149.20 LD
57,376,893.3 km
Rel. Velocity
18.69 km/s
67,295 km/h
Kinetic Energy
72.282 MT
E = ½mv² TNT eq.

Exact Landmark Scale Comparison (103.29m)

1:1 Meter Scale
103.29m
(2017 KU4)
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)23.8 mag
Spectral ClassificationS-type (Silicate Stony)
Estimated Bolide Mass1.731e+9 kg
Kinetic Energy (E = ½mv²)72.282 MT TNT (3.02e+17 J)
Transient Crater Diameter / Depth2,301 m Ø / 483 m deep
5-PSI Structural Overpressure Radius8.01 km
Thermal 3rd-Degree Burn Radius16.19 km
Equivalent Seismic MagnitudeMw 5.8
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 +23.24
Abs. Magnitude H = 23.80
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: (2017 KU4)

(2017 KU4) (H = 23.8, Vmag ≈ 23.2) 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 33.38° · Lon -135.40°136,800 km
Node T+1Lat 42.88° · Lon -125.82°122,617 km
Node T+2Lat 50.23° · Lon -116.23°109,667 km
Node T+3Lat 55.21° · Lon -106.65°97,950 km
Node T+4Lat 57.67° · Lon -97.07°87,467 km
Node T+5Lat 57.55° · Lon -87.48°78,217 km

Planetary Defense Frequently Asked Questions (Schema.org FAQ)

How big is (2017 KU4) compared to city landmarks?

(2017 KU4) has an estimated diameter between 46.19m and 103.29m. At its upper-bound size of 103.29m, it stands 23% as tall as the 443m Empire State Building in New York City and 31% of the 330m Eiffel Tower.

Will (2017 KU4) impact Earth during its 2026-10-21 approach?

No. NASA JPL Center for Near-Earth Object Studies (CNEOS) orbital solutions confirm (2017 KU4) will pass safely at a minimum distance of 149.20 Lunar Distances (57,376,893.3 km). You can still simulate a hypothetical street-level impact in our 3D CesiumJS simulator.

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(2017 KU4) — 3D Orbit, Size Comparison & Kinetic Impact Physics | Meteors.ai Space Network