Mission Control/ASTEROID DOSSIER: (2013 GA80)
NASA CATALOG + DOCUMENTED ANALYSISLaunch in 3D City Impact Simulator
POTENTIALLY HAZARDOUS ASTEROID (PHA)NASA CATALOG + DOCUMENTED ANALYSIS

(2013 GA80)

Tracked by NASA JPL Near-Earth Object Web Service (NeoWs), (2013 GA80) is a Unreported by NASA NeoWs body measuring between 133.22m and 297.88m in diameter. On 2026-11-04, it completes a cislunar approach at 147.75 Lunar Distances (56,821,340.2 km) with a relative heliocentric velocity of 17.84 km/s.

AI-ASSISTED SUMMARY (may contain errors):

(2013 GA80) (JPL ID 3634847) is a Unreported by NASA NeoWs Near-Earth Asteroid spanning 133.2m–297.9m (mean 215.6m). On 2026-11-04, it transits Earth's cislunar surveillance sector at 147.753 Lunar Distances (56,821,340 km) with a relative velocity of 17.84 km/s and a theoretical kinetic energy reserve of 568.99 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)
297.88 m
Min: 133.22 m
Miss Distance
147.75 LD
56,821,340.2 km
Rel. Velocity
17.84 km/s
64,235 km/h
Kinetic Energy
1,579.64 MT
E = ½mv² TNT eq.

Exact Landmark Scale Comparison (297.88m)

1:1 Meter Scale
297.88m
(2013 GA80)
443m
Manhattan
227m
Golden Gate
330m
Eiffel Tower
828m
Burj Khalifa
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Kinetic Impact Physics & Orbital Parameters

45° Incidence · 3,000 kg/m³
Absolute Magnitude (H)21.5 mag
Spectral ClassificationUnreported by NASA NeoWs
Estimated Bolide Mass4.152e+10 kg
Kinetic Energy (E = ½mv²)1,579.64 MT TNT (6.61e+18 J)
Transient Crater Diameter / Depth5,149 m Ø / 1,081 m deep
5-PSI Structural Overpressure Radius22.16 km
Thermal 3rd-Degree Burn Radius57.35 km
Equivalent Seismic MagnitudeMw 6.7
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 +20.92
Abs. Magnitude H = 21.50
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 GA80)

(2013 GA80) (H = 21.5, Vmag ≈ 20.9) 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 17.11° · Lon -145.60°136,800 km
Node T+1Lat 23.75° · Lon -136.02°122,617 km
Node T+2Lat 28.98° · Lon -126.43°109,667 km
Node T+3Lat 32.66° · Lon -116.85°97,950 km
Node T+4Lat 34.67° · Lon -107.27°87,467 km
Node T+5Lat 34.99° · Lon -97.68°78,217 km

Planetary Defense Frequently Asked Questions (Schema.org FAQ)

How big is (2013 GA80) compared to city landmarks?

(2013 GA80) has an estimated diameter between 133.22m and 297.88m. At its upper-bound size of 297.88m, it stands 67% as tall as the 443m Empire State Building in New York City and 90% of the 330m Eiffel Tower.

What does the stored 2026-11-04 close-approach estimate show?

This catalog snapshot lists a nominal miss distance of 147.75 Lunar Distances (56,821,340.2 km) for (2013 GA80). 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 GA80) — 3D Orbit, Size Comparison & Kinetic Impact Physics | Meteors.ai Space Network