Mission Control/ASTEROID DOSSIER: (2017 TK6)
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NOMINAL CISLUNAR PASSAGEGEMMA ENGINE: LOCAL SERVER BOX [ACTIVE] • meteors-gemma:latest

(2017 TK6)

Tracked by NASA JPL Near-Earth Object Web Service (NeoWs), (2017 TK6) is a S-type (Silicate Stony) body measuring between 31.52m and 70.48m in diameter. On 2026-10-25, it completes a cislunar approach at 47.92 Lunar Distances (18,428,131.2 km) with a relative heliocentric velocity of 15.06 km/s.

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

(2017 TK6) (JPL ID 3786454) is a S-type (Silicate Stony) Near-Earth Asteroid spanning 31.5m–70.5m (mean 51m). On 2026-10-25, it transits Earth's cislunar surveillance sector at 47.919 Lunar Distances (18,428,131 km) with a relative velocity of 15.06 km/s and a theoretical kinetic energy reserve of 5.37 megatons TNT. Its well-constrained heliocentric ephemeris passes safely outside Earth capture corridors while serving as an orbital calibration target.

Max Diameter (Ø)
70.48 m
Min: 31.52 m
Miss Distance
47.92 LD
18,428,131.2 km
Rel. Velocity
15.06 km/s
54,216 km/h
Kinetic Energy
14.905 MT
E = ½mv² TNT eq.

Exact Landmark Scale Comparison (70.48m)

1:1 Meter Scale
70.48m
(2017 TK6)
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)24.63 mag
Spectral ClassificationS-type (Silicate Stony)
Estimated Bolide Mass5.499e+8 kg
Kinetic Energy (E = ½mv²)14.905 MT TNT (6.24e+16 J)
Transient Crater Diameter / Depth1,553 m Ø / 326 m deep
5-PSI Structural Overpressure Radius4.76 km
Thermal 3rd-Degree Burn Radius8.48 km
Equivalent Seismic MagnitudeMw 5.4
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 +21.42
Abs. Magnitude H = 24.63
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: (2017 TK6)

(2017 TK6) (H = 24.6, Vmag ≈ 21.4) is below consumer optical detection thresholds (requires ≥1000mm survey aperture); explore certified meteorite specimens[↗] or indoor optical projection instead.

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Authentic coarse octahedrite Group IAB iron-nickel meteorite fragment (92.9% Fe, 6.7% Ni) recovered from the Chaco crater field with certificate of authenticity.

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3D Ephemeris Trajectory Waypoints

Node T+0Lat 39.74° · Lon -79.30°136,800 km
Node T+1Lat 50.36° · Lon -69.72°122,617 km
Node T+2Lat 58.55° · Lon -60.13°109,667 km
Node T+3Lat 64.04° · Lon -50.55°97,950 km
Node T+4Lat 66.67° · Lon -40.97°87,467 km
Node T+5Lat 66.37° · Lon -31.38°78,217 km

Planetary Defense Frequently Asked Questions (Schema.org FAQ)

How big is (2017 TK6) compared to city landmarks?

(2017 TK6) has an estimated diameter between 31.52m and 70.48m. At its upper-bound size of 70.48m, it stands 16% as tall as the 443m Empire State Building in New York City and 21% of the 330m Eiffel Tower.

Will (2017 TK6) impact Earth during its 2026-10-25 approach?

No. NASA JPL Center for Near-Earth Object Studies (CNEOS) orbital solutions confirm (2017 TK6) will pass safely at a minimum distance of 47.92 Lunar Distances (18,428,131.2 km). You can still simulate a hypothetical street-level impact in our 3D CesiumJS simulator.

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(2017 TK6) — 3D Orbit, Size Comparison & Kinetic Impact Physics | Meteors.ai Space Network