Mission Control/ASTEROID DOSSIER: (2004 HX53)
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(2004 HX53)

Tracked by NASA JPL Near-Earth Object Web Service (NeoWs), (2004 HX53) is a X-type (Enstatite-Metallic) body measuring between 50.65m and 113.25m in diameter. On 2026-10-24, it completes a cislunar approach at 35.80 Lunar Distances (13,765,534.9 km) with a relative heliocentric velocity of 12.61 km/s.

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

(2004 HX53) (JPL ID 3180184) is a X-type (Enstatite-Metallic) Near-Earth Asteroid spanning 50.6m–113.3m (mean 82m). On 2026-10-24, it transits Earth's cislunar surveillance sector at 35.795 Lunar Distances (13,765,535 km) with a relative velocity of 12.61 km/s and a theoretical kinetic energy reserve of 15.64 megatons TNT. Its well-constrained heliocentric ephemeris passes safely outside Earth capture corridors while serving as an orbital calibration target.

Max Diameter (Ø)
113.25 m
Min: 50.65 m
Miss Distance
35.80 LD
13,765,534.9 km
Rel. Velocity
12.61 km/s
45,400 km/h
Kinetic Energy
43.362 MT
E = ½mv² TNT eq.

Exact Landmark Scale Comparison (113.25m)

1:1 Meter Scale
113.25m
(2004 HX53)
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)23.6 mag
Spectral ClassificationX-type (Enstatite-Metallic)
Estimated Bolide Mass2.282e+9 kg
Kinetic Energy (E = ½mv²)43.362 MT TNT (1.81e+17 J)
Transient Crater Diameter / Depth2,079 m Ø / 437 m deep
5-PSI Structural Overpressure Radius6.77 km
Thermal 3rd-Degree Burn Radius13.13 km
Equivalent Seismic MagnitudeMw 5.7
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 +19.74
Abs. Magnitude H = 23.60
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: (2004 HX53)

(2004 HX53) (H = 23.6, Vmag ≈ 19.7) 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 -18.95° · Lon 177.00°136,800 km
Node T+1Lat -18.65° · Lon -173.42°122,617 km
Node T+2Lat -18.13° · Lon -163.83°109,667 km
Node T+3Lat -17.36° · Lon -154.25°97,950 km
Node T+4Lat -16.33° · Lon -144.67°87,467 km
Node T+5Lat -15.03° · Lon -135.08°78,217 km

Planetary Defense Frequently Asked Questions (Schema.org FAQ)

How big is (2004 HX53) compared to city landmarks?

(2004 HX53) has an estimated diameter between 50.65m and 113.25m. At its upper-bound size of 113.25m, it stands 26% as tall as the 443m Empire State Building in New York City and 34% of the 330m Eiffel Tower.

Will (2004 HX53) impact Earth during its 2026-10-24 approach?

No. NASA JPL Center for Near-Earth Object Studies (CNEOS) orbital solutions confirm (2004 HX53) will pass safely at a minimum distance of 35.80 Lunar Distances (13,765,534.9 km). You can still simulate a hypothetical street-level impact in our 3D CesiumJS simulator.

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(2004 HX53) — 3D Orbit, Size Comparison & Kinetic Impact Physics | Meteors.ai Space Network