Mission Control/ASTEROID DOSSIER: 423100 (2004 BX1)
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NOMINAL CISLUNAR PASSAGEGEMMA ENGINE: LOCAL SERVER BOX [ACTIVE] • meteors-gemma:latest

423100 (2004 BX1)

Tracked by NASA JPL Near-Earth Object Web Service (NeoWs), 423100 (2004 BX1) is a Q-type (Olivine-Pyroxene) body measuring between 542.69m and 1213.5m in diameter. On 2026-10-20, it completes a cislunar approach at 171.47 Lunar Distances (65,943,991.3 km) with a relative heliocentric velocity of 37.87 km/s.

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

423100 (2004 BX1) (JPL ID 2423100) is a Q-type (Olivine-Pyroxene) Near-Earth Asteroid spanning 542.7m–1213.5m (mean 878.1m). On 2026-10-20, it transits Earth's cislunar surveillance sector at 171.474 Lunar Distances (65,943,991 km) with a relative velocity of 37.87 km/s and a theoretical kinetic energy reserve of 173131.28 megatons TNT. Its well-constrained heliocentric ephemeris passes safely outside Earth capture corridors while serving as an orbital calibration target.

Max Diameter (Ø)
1213.5 m
Min: 542.69 m
Miss Distance
171.47 LD
65,943,991.3 km
Rel. Velocity
37.87 km/s
136,321 km/h
Kinetic Energy
480,993.654 MT
E = ½mv² TNT eq.

Exact Landmark Scale Comparison (1213.5m)

1:1 Meter Scale
1213.5m
423100 (2004 BX1)
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)18.45 mag
Spectral ClassificationQ-type (Olivine-Pyroxene)
Estimated Bolide Mass2.807e+12 kg
Kinetic Energy (E = ½mv²)480,993.654 MT TNT (2.01e+21 J)
Transient Crater Diameter / Depth21,446 m Ø / 4,504 m deep
5-PSI Structural Overpressure Radius146.27 km
Thermal 3rd-Degree Burn Radius598.18 km
Equivalent Seismic MagnitudeMw 8.4
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 +18.23
Abs. Magnitude H = 18.45
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: 423100 (2004 BX1)

423100 (2004 BX1) (H = 18.4, Vmag ≈ 18.2) 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 2.97° · Lon -0.25°136,800 km
Node T+1Lat 7.12° · Lon 9.33°122,617 km
Node T+2Lat 10.51° · Lon 18.92°109,667 km
Node T+3Lat 13.04° · Lon 28.50°97,950 km
Node T+4Lat 14.67° · Lon 38.08°87,467 km
Node T+5Lat 15.37° · Lon 47.67°78,217 km

Planetary Defense Frequently Asked Questions (Schema.org FAQ)

How big is 423100 (2004 BX1) compared to city landmarks?

423100 (2004 BX1) has an estimated diameter between 542.69m and 1213.5m. At its upper-bound size of 1213.5m, it stands 274% as tall as the 443m Empire State Building in New York City and 368% of the 330m Eiffel Tower.

Will 423100 (2004 BX1) impact Earth during its 2026-10-20 approach?

No. NASA JPL Center for Near-Earth Object Studies (CNEOS) orbital solutions confirm 423100 (2004 BX1) will pass safely at a minimum distance of 171.47 Lunar Distances (65,943,991.3 km). You can still simulate a hypothetical street-level impact in our 3D CesiumJS simulator.

Hall-of-Fame Near-Earth Asteroids & Historic CNEOS Bolides
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423100 (2004 BX1) — 3D Orbit, Size Comparison & Kinetic Impact Physics | Meteors.ai Space Network