Mission Control/ASTEROID DOSSIER: 516803 (2010 JG88)
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516803 (2010 JG88)

Tracked by NASA JPL Near-Earth Object Web Service (NeoWs), 516803 (2010 JG88) is a X-type (Enstatite-Metallic) body measuring between 331.55m and 741.38m in diameter. On 2026-10-26, it completes a cislunar approach at 33.75 Lunar Distances (12,978,696.8 km) with a relative heliocentric velocity of 20.40 km/s.

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

516803 (2010 JG88) (JPL ID 2516803) is a X-type (Enstatite-Metallic) Near-Earth Asteroid spanning 331.6m–741.4m (mean 536.5m). On 2026-10-26, it transits Earth's cislunar surveillance sector at 33.749 Lunar Distances (12,978,697 km) with a relative velocity of 20.40 km/s and a theoretical kinetic energy reserve of 11462.42 megatons TNT. Its well-constrained heliocentric ephemeris passes safely outside Earth capture corridors while serving as an orbital calibration target.

Max Diameter (Ø)
741.38 m
Min: 331.55 m
Miss Distance
33.75 LD
12,978,696.8 km
Rel. Velocity
20.40 km/s
73,447 km/h
Kinetic Energy
31,839.504 MT
E = ½mv² TNT eq.

Exact Landmark Scale Comparison (741.38m)

1:1 Meter Scale
741.38m
516803 (2010 JG88)
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)19.52 mag
Spectral ClassificationX-type (Enstatite-Metallic)
Estimated Bolide Mass6.401e+11 kg
Kinetic Energy (E = ½mv²)31,839.504 MT TNT (1.33e+20 J)
Transient Crater Diameter / Depth11,124 m Ø / 2,336 m deep
5-PSI Structural Overpressure Radius59.71 km
Thermal 3rd-Degree Burn Radius196.51 km
Equivalent Seismic MagnitudeMw 7.6
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 +15.53
Abs. Magnitude H = 19.52
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: 516803 (2010 JG88)

516803 (2010 JG88) (H = 19.5, Vmag ≈ 15.5) 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 10.75° · Lon 0.60°136,800 km
Node T+1Lat 16.27° · Lon 10.18°122,617 km
Node T+2Lat 20.67° · Lon 19.77°109,667 km
Node T+3Lat 23.83° · Lon 29.35°97,950 km
Node T+4Lat 25.67° · Lon 38.93°87,467 km
Node T+5Lat 26.16° · Lon 48.52°78,217 km

Planetary Defense Frequently Asked Questions (Schema.org FAQ)

How big is 516803 (2010 JG88) compared to city landmarks?

516803 (2010 JG88) has an estimated diameter between 331.55m and 741.38m. At its upper-bound size of 741.38m, it stands 167% as tall as the 443m Empire State Building in New York City and 225% of the 330m Eiffel Tower.

Will 516803 (2010 JG88) impact Earth during its 2026-10-26 approach?

No. NASA JPL Center for Near-Earth Object Studies (CNEOS) orbital solutions confirm 516803 (2010 JG88) will pass safely at a minimum distance of 33.75 Lunar Distances (12,978,696.8 km). You can still simulate a hypothetical street-level impact in our 3D CesiumJS simulator.

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516803 (2010 JG88) — 3D Orbit, Size Comparison & Kinetic Impact Physics | Meteors.ai Space Network