Mission Control/ASTEROID DOSSIER: (2020 BW)
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NOMINAL CISLUNAR PASSAGEGEMMA ENGINE: LOCAL SERVER BOX [ACTIVE] • meteors-gemma:latest

(2020 BW)

Tracked by NASA JPL Near-Earth Object Web Service (NeoWs), (2020 BW) is a X-type (Enstatite-Metallic) body measuring between 36.69m and 82.04m in diameter. On 2026-10-21, it completes a cislunar approach at 100.19 Lunar Distances (38,529,546.2 km) with a relative heliocentric velocity of 18.14 km/s.

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

(2020 BW) (JPL ID 3986739) is a X-type (Enstatite-Metallic) Near-Earth Asteroid spanning 36.7m–82.0m (mean 59.4m). On 2026-10-21, it transits Earth's cislunar surveillance sector at 100.189 Lunar Distances (38,529,546 km) with a relative velocity of 18.14 km/s and a theoretical kinetic energy reserve of 12.29 megatons TNT. Its well-constrained heliocentric ephemeris passes safely outside Earth capture corridors while serving as an orbital calibration target.

Max Diameter (Ø)
82.04 m
Min: 36.69 m
Miss Distance
100.19 LD
38,529,546.2 km
Rel. Velocity
18.14 km/s
65,286 km/h
Kinetic Energy
34.089 MT
E = ½mv² TNT eq.

Exact Landmark Scale Comparison (82.04m)

1:1 Meter Scale
82.04m
(2020 BW)
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)24.3 mag
Spectral ClassificationX-type (Enstatite-Metallic)
Estimated Bolide Mass8.674e+8 kg
Kinetic Energy (E = ½mv²)34.089 MT TNT (1.43e+17 J)
Transient Crater Diameter / Depth1,897 m Ø / 398 m deep
5-PSI Structural Overpressure Radius6.25 km
Thermal 3rd-Degree Burn Radius11.9 km
Equivalent Seismic MagnitudeMw 5.6
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 +22.79
Abs. Magnitude H = 24.30
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: (2020 BW)

(2020 BW) (H = 24.3, Vmag ≈ 22.8) 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 -26.73° · Lon 31.20°136,800 km
Node T+1Lat -27.80° · Lon 40.78°122,617 km
Node T+2Lat -28.30° · Lon 50.37°109,667 km
Node T+3Lat -28.15° · Lon 59.95°97,950 km
Node T+4Lat -27.33° · Lon 69.53°87,467 km
Node T+5Lat -25.82° · Lon 79.12°78,217 km

Planetary Defense Frequently Asked Questions (Schema.org FAQ)

How big is (2020 BW) compared to city landmarks?

(2020 BW) has an estimated diameter between 36.69m and 82.04m. At its upper-bound size of 82.04m, it stands 19% as tall as the 443m Empire State Building in New York City and 25% of the 330m Eiffel Tower.

Will (2020 BW) impact Earth during its 2026-10-21 approach?

No. NASA JPL Center for Near-Earth Object Studies (CNEOS) orbital solutions confirm (2020 BW) will pass safely at a minimum distance of 100.19 Lunar Distances (38,529,546.2 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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(2020 BW) — 3D Orbit, Size Comparison & Kinetic Impact Physics | Meteors.ai Space Network