Mission Control/ASTEROID DOSSIER: (2017 WG28)
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NOMINAL CISLUNAR PASSAGEGEMMA ENGINE: LOCAL SERVER BOX [ACTIVE] • meteors-gemma:latest

(2017 WG28)

Tracked by NASA JPL Near-Earth Object Web Service (NeoWs), (2017 WG28) is a X-type (Enstatite-Metallic) body measuring between 60.61m and 135.53m in diameter. On 2026-10-21, it completes a cislunar approach at 144.47 Lunar Distances (55,560,445 km) with a relative heliocentric velocity of 7.99 km/s.

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

(2017 WG28) (JPL ID 3789972) is a X-type (Enstatite-Metallic) Near-Earth Asteroid spanning 60.6m–135.5m (mean 98.1m). On 2026-10-21, it transits Earth's cislunar surveillance sector at 144.474 Lunar Distances (55,560,445 km) with a relative velocity of 7.99 km/s and a theoretical kinetic energy reserve of 10.76 megatons TNT. Its well-constrained heliocentric ephemeris passes safely outside Earth capture corridors while serving as an orbital calibration target.

Max Diameter (Ø)
135.53 m
Min: 60.61 m
Miss Distance
144.47 LD
55,560,445 km
Rel. Velocity
7.99 km/s
28,775 km/h
Kinetic Energy
29.855 MT
E = ½mv² TNT eq.

Exact Landmark Scale Comparison (135.53m)

1:1 Meter Scale
135.53m
(2017 WG28)
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)23.21 mag
Spectral ClassificationX-type (Enstatite-Metallic)
Estimated Bolide Mass3.910e+9 kg
Kinetic Energy (E = ½mv²)29.855 MT TNT (1.25e+17 J)
Transient Crater Diameter / Depth1,957 m Ø / 411 m deep
5-PSI Structural Overpressure Radius5.98 km
Thermal 3rd-Degree Burn Radius11.27 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 +22.57
Abs. Magnitude H = 23.21
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 WG28)

(2017 WG28) (H = 23.2, Vmag ≈ 22.6) 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 33.38° · Lon -106.50°136,800 km
Node T+1Lat 42.88° · Lon -96.92°122,617 km
Node T+2Lat 50.23° · Lon -87.33°109,667 km
Node T+3Lat 55.21° · Lon -77.75°97,950 km
Node T+4Lat 57.67° · Lon -68.17°87,467 km
Node T+5Lat 57.55° · Lon -58.58°78,217 km

Planetary Defense Frequently Asked Questions (Schema.org FAQ)

How big is (2017 WG28) compared to city landmarks?

(2017 WG28) has an estimated diameter between 60.61m and 135.53m. At its upper-bound size of 135.53m, it stands 31% as tall as the 443m Empire State Building in New York City and 41% of the 330m Eiffel Tower.

Will (2017 WG28) impact Earth during its 2026-10-21 approach?

No. NASA JPL Center for Near-Earth Object Studies (CNEOS) orbital solutions confirm (2017 WG28) will pass safely at a minimum distance of 144.47 Lunar Distances (55,560,445 km). You can still simulate a hypothetical street-level impact in our 3D CesiumJS simulator.

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(2017 WG28) — 3D Orbit, Size Comparison & Kinetic Impact Physics | Meteors.ai Space Network