Mission Control/ASTEROID DOSSIER: 529819 (2010 PM58)
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529819 (2010 PM58)

Tracked by NASA JPL Near-Earth Object Web Service (NeoWs), 529819 (2010 PM58) is a Q-type (Olivine-Pyroxene) body measuring between 178.88m and 399.98m in diameter. On 2026-10-24, it completes a cislunar approach at 119.43 Lunar Distances (45,930,919.7 km) with a relative heliocentric velocity of 12.84 km/s.

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

529819 (2010 PM58) (JPL ID 2529819) is a Q-type (Olivine-Pyroxene) Near-Earth Asteroid spanning 178.9m–400.0m (mean 289.4m). On 2026-10-24, it transits Earth's cislunar surveillance sector at 119.434 Lunar Distances (45,930,920 km) with a relative velocity of 12.84 km/s and a theoretical kinetic energy reserve of 712.38 megatons TNT. Its well-constrained heliocentric ephemeris passes safely outside Earth capture corridors while serving as an orbital calibration target.

Max Diameter (Ø)
399.98 m
Min: 178.88 m
Miss Distance
119.43 LD
45,930,919.7 km
Rel. Velocity
12.84 km/s
46,217 km/h
Kinetic Energy
1,979.738 MT
E = ½mv² TNT eq.

Exact Landmark Scale Comparison (399.98m)

1:1 Meter Scale
399.98m
529819 (2010 PM58)
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)20.86 mag
Spectral ClassificationQ-type (Olivine-Pyroxene)
Estimated Bolide Mass1.005e+11 kg
Kinetic Energy (E = ½mv²)1,979.738 MT TNT (8.28e+18 J)
Transient Crater Diameter / Depth5,606 m Ø / 1,177 m deep
5-PSI Structural Overpressure Radius23.87 km
Thermal 3rd-Degree Burn Radius62.92 km
Equivalent Seismic MagnitudeMw 6.8
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 +19.77
Abs. Magnitude H = 20.86
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: 529819 (2010 PM58)

529819 (2010 PM58) (H = 20.9, Vmag ≈ 19.8) 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 19.23° · Lon 25.25°136,800 km
Node T+1Lat 26.25° · Lon 34.83°122,617 km
Node T+2Lat 31.76° · Lon 44.42°109,667 km
Node T+3Lat 35.60° · Lon 54.00°97,950 km
Node T+4Lat 37.67° · Lon 63.58°87,467 km
Node T+5Lat 37.93° · Lon 73.17°78,217 km

Planetary Defense Frequently Asked Questions (Schema.org FAQ)

How big is 529819 (2010 PM58) compared to city landmarks?

529819 (2010 PM58) has an estimated diameter between 178.88m and 399.98m. At its upper-bound size of 399.98m, it stands 90% as tall as the 443m Empire State Building in New York City and 121% of the 330m Eiffel Tower.

Will 529819 (2010 PM58) impact Earth during its 2026-10-24 approach?

No. NASA JPL Center for Near-Earth Object Studies (CNEOS) orbital solutions confirm 529819 (2010 PM58) will pass safely at a minimum distance of 119.43 Lunar Distances (45,930,919.7 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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529819 (2010 PM58) — 3D Orbit, Size Comparison & Kinetic Impact Physics | Meteors.ai Space Network