Mission Control/ASTEROID DOSSIER: (2013 VO5)
NASA CATALOG + DOCUMENTED ANALYSISLaunch in 3D City Impact Simulator
POTENTIALLY HAZARDOUS ASTEROID (PHA)NASA CATALOG + DOCUMENTED ANALYSIS

(2013 VO5)

Tracked by NASA JPL Near-Earth Object Web Service (NeoWs), (2013 VO5) is a Unreported by NASA NeoWs body measuring between 142.09m and 317.72m in diameter. On 2026-11-11, it completes a cislunar approach at 53.56 Lunar Distances (20,596,821 km) with a relative heliocentric velocity of 27.47 km/s.

AI-ASSISTED SUMMARY (may contain errors):

(2013 VO5) (JPL ID 3653537) is a Unreported by NASA NeoWs Near-Earth Asteroid spanning 142.1m–317.7m (mean 229.9m). On 2026-11-11, it transits Earth's cislunar surveillance sector at 53.558 Lunar Distances (20,596,821 km) with a relative velocity of 27.47 km/s and a theoretical kinetic energy reserve of 1635.62 megatons TNT. Classified as a Potentially Hazardous Asteroid (PHA) due to its Minimum Orbit Intersection Distance (MOID <= 0.05 AU) and absolute magnitude (H <= 22.0), it remains under high-priority radar and optical astrometric tracking.

Max Diameter (Ø)
317.72 m
Min: 142.09 m
Miss Distance
53.56 LD
20,596,821 km
Rel. Velocity
27.47 km/s
98,906 km/h
Kinetic Energy
4,544.391 MT
E = ½mv² TNT eq.

Exact Landmark Scale Comparison (317.72m)

1:1 Meter Scale
317.72m
(2013 VO5)
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)21.36 mag
Spectral ClassificationUnreported by NASA NeoWs
Estimated Bolide Mass5.038e+10 kg
Kinetic Energy (E = ½mv²)4,544.391 MT TNT (1.90e+19 J)
Transient Crater Diameter / Depth6,548 m Ø / 1,375 m deep
5-PSI Structural Overpressure Radius31.41 km
Thermal 3rd-Degree Burn Radius88.46 km
Equivalent Seismic MagnitudeMw 7
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 +18.41
Abs. Magnitude H = 21.36
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: (2013 VO5)

(2013 VO5) (H = 21.4, Vmag ≈ 18.4) 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 19.94° · Lon -1.95°136,800 km
Node T+1Lat 27.08° · Lon 7.63°122,617 km
Node T+2Lat 32.68° · Lon 17.22°109,667 km
Node T+3Lat 36.58° · Lon 26.80°97,950 km
Node T+4Lat 38.67° · Lon 36.38°87,467 km
Node T+5Lat 38.91° · Lon 45.97°78,217 km

Planetary Defense Frequently Asked Questions (Schema.org FAQ)

How big is (2013 VO5) compared to city landmarks?

(2013 VO5) has an estimated diameter between 142.09m and 317.72m. At its upper-bound size of 317.72m, it stands 72% as tall as the 443m Empire State Building in New York City and 96% of the 330m Eiffel Tower.

What does the stored 2026-11-11 close-approach estimate show?

This catalog snapshot lists a nominal miss distance of 53.56 Lunar Distances (20,596,821 km) for (2013 VO5). This is not an impact prediction; check the latest NASA JPL record for updated orbital estimates. The 3D impact simulation is hypothetical.

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(2013 VO5) — 3D Orbit, Size Comparison & Kinetic Impact Physics | Meteors.ai Space Network