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

(2019 HK)

Tracked by NASA JPL Near-Earth Object Web Service (NeoWs), (2019 HK) is a C-type (Carbonaceous Chondrite) body measuring between 38.42m and 85.91m in diameter. On 2026-10-23, it completes a cislunar approach at 151.61 Lunar Distances (58,303,042.5 km) with a relative heliocentric velocity of 22.28 km/s.

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

(2019 HK) (JPL ID 3841527) is a C-type (Carbonaceous Chondrite) Near-Earth Asteroid spanning 38.4m–85.9m (mean 62.2m). On 2026-10-23, it transits Earth's cislunar surveillance sector at 151.606 Lunar Distances (58,303,043 km) with a relative velocity of 22.28 km/s and a theoretical kinetic energy reserve of 21.31 megatons TNT. Its well-constrained heliocentric ephemeris passes safely outside Earth capture corridors while serving as an orbital calibration target.

Max Diameter (Ø)
85.91 m
Min: 38.42 m
Miss Distance
151.61 LD
58,303,042.5 km
Rel. Velocity
22.28 km/s
80,215 km/h
Kinetic Energy
59.093 MT
E = ½mv² TNT eq.

Exact Landmark Scale Comparison (85.91m)

1:1 Meter Scale
85.91m
(2019 HK)
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)24.2 mag
Spectral ClassificationC-type (Carbonaceous Chondrite)
Estimated Bolide Mass9.960e+8 kg
Kinetic Energy (E = ½mv²)59.093 MT TNT (2.47e+17 J)
Transient Crater Diameter / Depth2,153 m Ø / 452 m deep
5-PSI Structural Overpressure Radius7.49 km
Thermal 3rd-Degree Burn Radius14.91 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 +23.68
Abs. Magnitude H = 24.20
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 HK)

(2019 HK) (H = 24.2, Vmag ≈ 23.7) 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 -9.76° · Lon -7.05°136,800 km
Node T+1Lat -7.84° · Lon 2.53°122,617 km
Node T+2Lat -6.12° · Lon 12.12°109,667 km
Node T+3Lat -4.62° · Lon 21.70°97,950 km
Node T+4Lat -3.33° · Lon 31.28°87,467 km
Node T+5Lat -2.28° · Lon 40.87°78,217 km

Planetary Defense Frequently Asked Questions (Schema.org FAQ)

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

(2019 HK) has an estimated diameter between 38.42m and 85.91m. At its upper-bound size of 85.91m, it stands 19% as tall as the 443m Empire State Building in New York City and 26% of the 330m Eiffel Tower.

Will (2019 HK) impact Earth during its 2026-10-23 approach?

No. NASA JPL Center for Near-Earth Object Studies (CNEOS) orbital solutions confirm (2019 HK) will pass safely at a minimum distance of 151.61 Lunar Distances (58,303,042.5 km). You can still simulate a hypothetical street-level impact in our 3D CesiumJS simulator.

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