Mission Control/ASTEROID DOSSIER: 488509 (2000 UW13)
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488509 (2000 UW13)

Tracked by NASA JPL Near-Earth Object Web Service (NeoWs), 488509 (2000 UW13) is a Q-type (Olivine-Pyroxene) body measuring between 200.7m and 448.79m in diameter. On 2026-10-26, it completes a cislunar approach at 172.73 Lunar Distances (66,425,278.8 km) with a relative heliocentric velocity of 18.63 km/s.

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

488509 (2000 UW13) (JPL ID 2488509) is a Q-type (Olivine-Pyroxene) Near-Earth Asteroid spanning 200.7m–448.8m (mean 324.7m). On 2026-10-26, it transits Earth's cislunar surveillance sector at 172.726 Lunar Distances (66,425,279 km) with a relative velocity of 18.63 km/s and a theoretical kinetic energy reserve of 2119.05 megatons TNT. Its well-constrained heliocentric ephemeris passes safely outside Earth capture corridors while serving as an orbital calibration target.

Max Diameter (Ø)
448.79 m
Min: 200.7 m
Miss Distance
172.73 LD
66,425,278.8 km
Rel. Velocity
18.63 km/s
67,072 km/h
Kinetic Energy
5,889.793 MT
E = ½mv² TNT eq.

Exact Landmark Scale Comparison (448.79m)

1:1 Meter Scale
448.79m
488509 (2000 UW13)
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)20.61 mag
Spectral ClassificationQ-type (Olivine-Pyroxene)
Estimated Bolide Mass1.420e+11 kg
Kinetic Energy (E = ½mv²)5,889.793 MT TNT (2.46e+19 J)
Transient Crater Diameter / Depth7,225 m Ø / 1,517 m deep
5-PSI Structural Overpressure Radius34.21 km
Thermal 3rd-Degree Burn Radius98.38 km
Equivalent Seismic MagnitudeMw 7.1
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 +20.41
Abs. Magnitude H = 20.61
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: 488509 (2000 UW13)

488509 (2000 UW13) (H = 20.6, Vmag ≈ 20.4) 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 33.38° · Lon 171.05°136,800 km
Node T+1Lat 42.88° · Lon -179.37°122,617 km
Node T+2Lat 50.23° · Lon -169.78°109,667 km
Node T+3Lat 55.21° · Lon -160.20°97,950 km
Node T+4Lat 57.67° · Lon -150.62°87,467 km
Node T+5Lat 57.55° · Lon -141.03°78,217 km

Planetary Defense Frequently Asked Questions (Schema.org FAQ)

How big is 488509 (2000 UW13) compared to city landmarks?

488509 (2000 UW13) has an estimated diameter between 200.7m and 448.79m. At its upper-bound size of 448.79m, it stands 101% as tall as the 443m Empire State Building in New York City and 136% of the 330m Eiffel Tower.

Will 488509 (2000 UW13) impact Earth during its 2026-10-26 approach?

No. NASA JPL Center for Near-Earth Object Studies (CNEOS) orbital solutions confirm 488509 (2000 UW13) will pass safely at a minimum distance of 172.73 Lunar Distances (66,425,278.8 km). You can still simulate a hypothetical street-level impact in our 3D CesiumJS simulator.

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488509 (2000 UW13) — 3D Orbit, Size Comparison & Kinetic Impact Physics | Meteors.ai Space Network