Mission Control/ASTEROID DOSSIER: 1685
NASA CATALOG + DOCUMENTED ANALYSISLaunch in 3D City Impact Simulator
NOMINAL CISLUNAR PASSAGENASA CATALOG + DOCUMENTED ANALYSIS

1685 Toro (1948 OA)

Tracked by NASA JPL Near-Earth Object Web Service (NeoWs), 1685 Toro (1948 OA) is a S / S body measuring between 3400m and 3400m in diameter. On 2032-01-20, it completes a cislunar approach at 50.13 Lunar Distances (19,269,048 km) with a relative heliocentric velocity of 16.03 km/s.

AI-ASSISTED SUMMARY (may contain errors):

1685 Toro (1948 OA) (JPL ID 1685) is a S / S Near-Earth Asteroid spanning 3400.0m–3400.0m (mean 3400m). On 2032-01-20, it transits Earth's cislunar surveillance sector at 50.128 Lunar Distances (19,269,048 km) with a relative velocity of 16.03 km/s and a theoretical kinetic energy reserve of 1801049.32 megatons TNT. Its well-constrained heliocentric ephemeris passes safely outside Earth capture corridors while serving as an orbital calibration target.

Max Diameter (Ø)
3400 m
Min: 3400 m
Miss Distance
50.13 LD
19,269,048 km
Rel. Velocity
16.03 km/s
57,708 km/h
Kinetic Energy
1,895,841.393 MT
E = ½mv² TNT eq.

Exact Landmark Scale Comparison (3400m)

1:1 Meter Scale
3400m
1685
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)14.26 mag
Spectral ClassificationS / S
Estimated Bolide Mass6.174e+13 kg
Kinetic Energy (E = ½mv²)1,895,841.393 MT TNT (7.93e+21 J)
Transient Crater Diameter / Depth32,816 m Ø / 6,891 m deep
5-PSI Structural Overpressure Radius229.99 km
Thermal 3rd-Degree Burn Radius1049.68 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 +11.16
Abs. Magnitude H = 14.26
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: 1685 Toro (1948 OA)

1685 Toro (1948 OA) (H = 14.3, Vmag ≈ 11.2) requires plate-solved smart telescope[↗] live-stacking integration beyond naked-eye threshold.

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3D Ephemeris Trajectory Waypoints

Node T+0Lat 41.86° · Lon 171.05°136,800 km
Node T+1Lat 52.85° · Lon -179.37°122,617 km
Node T+2Lat 61.32° · Lon -169.78°109,667 km
Node T+3Lat 66.98° · Lon -160.20°97,950 km
Node T+4Lat 69.67° · Lon -150.62°87,467 km
Node T+5Lat 69.31° · Lon -141.03°78,217 km

Planetary Defense Frequently Asked Questions (Schema.org FAQ)

How big is 1685 Toro (1948 OA) compared to city landmarks?

1685 Toro (1948 OA) has an estimated diameter between 3400m and 3400m. At its upper-bound size of 3400m, it stands 767% as tall as the 443m Empire State Building in New York City and 1030% of the 330m Eiffel Tower.

What does the stored 2032-01-20 close-approach estimate show?

This catalog snapshot lists a nominal miss distance of 50.13 Lunar Distances (19,269,048 km) for 1685 Toro (1948 OA). 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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1685 Toro (1948 OA) — 3D Orbit, Size Comparison & Kinetic Impact Physics | Meteors.ai Space Network