Mission Control/ASTEROID DOSSIER: 4179
NASA CATALOG + DOCUMENTED ANALYSISLaunch in 3D City Impact Simulator
POTENTIALLY HAZARDOUS ASTEROID (PHA)NASA CATALOG + DOCUMENTED ANALYSIS

4179 Toutatis (1989 AC)

Tracked by NASA JPL Near-Earth Object Web Service (NeoWs), 4179 Toutatis (1989 AC) is a Sk body measuring between 5400m and 5400m in diameter. On 2069-11-05, it completes a cislunar approach at 7.72 Lunar Distances (2,969,321 km) with a relative heliocentric velocity of 8.41 km/s.

AI-ASSISTED SUMMARY (may contain errors):

4179 Toutatis (1989 AC) (JPL ID 4179) is a Sk Near-Earth Asteroid spanning 5400.0m–5400.0m (mean 5400m). On 2069-11-05, it transits Earth's cislunar surveillance sector at 7.725 Lunar Distances (2,969,321 km) with a relative velocity of 8.41 km/s and a theoretical kinetic energy reserve of 1986072.43 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)
5400 m
Min: 5400 m
Miss Distance
7.72 LD
2,969,321 km
Rel. Velocity
8.41 km/s
30,276 km/h
Kinetic Energy
2,090,602.554 MT
E = ½mv² TNT eq.

Exact Landmark Scale Comparison (5400m)

1:1 Meter Scale
5400m
4179
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)15.29 mag
Spectral ClassificationSk
Estimated Bolide Mass2.473e+14 kg
Kinetic Energy (E = ½mv²)2,090,602.554 MT TNT (8.75e+21 J)
Transient Crater Diameter / Depth35,444 m Ø / 7,443 m deep
5-PSI Structural Overpressure Radius237.53 km
Thermal 3rd-Degree Burn Radius1092.62 km
Equivalent Seismic MagnitudeMw 8.8
Primary Ephemeris Source:NASA JPL Small-Body Database Lookup
OPTICAL TRACKING REQUIREMENTS // PHOTOMETRIC LINK
TIER B: SMART ASTROPHOTOGRAPHY SCOPE
Calculated Apparent Magnitude (Vmag)
Vmag +8.04
Abs. Magnitude H = 15.29
Required Aperture (mm)
50 mm Optical Aperture
Autonomous Plate-Solved Sidereal + Ephemeris Live Stacking (10s subs)
Best Viewing Window
Astronomical Midnight ± 3 Hours (Moon Illumination < 40%)
Target: 4179 Toutatis (1989 AC)

4179 Toutatis (1989 AC) (H = 15.3, Vmag ≈ 8.0) requires plate-solved smart telescope[↗] live-stacking integration beyond naked-eye threshold.

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3D Ephemeris Trajectory Waypoints

Node T+0Lat -4.10° · Lon 131.10°130,194 km
Node T+1Lat -1.19° · Lon 140.68°116,695 km
Node T+2Lat 1.27° · Lon 150.27°104,371 km
Node T+3Lat 3.23° · Lon 159.85°93,220 km
Node T+4Lat 4.67° · Lon 169.43°83,243 km
Node T+5Lat 5.56° · Lon 179.02°74,439 km

Planetary Defense Frequently Asked Questions (Schema.org FAQ)

How big is 4179 Toutatis (1989 AC) compared to city landmarks?

4179 Toutatis (1989 AC) has an estimated diameter between 5400m and 5400m. At its upper-bound size of 5400m, it stands 1219% as tall as the 443m Empire State Building in New York City and 1636% of the 330m Eiffel Tower.

What does the stored 2069-11-05 close-approach estimate show?

This catalog snapshot lists a nominal miss distance of 7.72 Lunar Distances (2,969,321 km) for 4179 Toutatis (1989 AC). 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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4179 Toutatis (1989 AC) — 3D Orbit, Size Comparison & Kinetic Impact Physics | Meteors.ai Space Network