Mission Control/ASTEROID DOSSIER: (2017 TJ2)
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NOMINAL CISLUNAR PASSAGEGEMMA ENGINE: LOCAL SERVER BOX [ACTIVE] • meteors-gemma:latest

(2017 TJ2)

Tracked by NASA JPL Near-Earth Object Web Service (NeoWs), (2017 TJ2) is a V-type (Basaltic Achondrite) body measuring between 27.2m and 60.82m in diameter. On 2026-10-25, it completes a cislunar approach at 101.94 Lunar Distances (39,203,868.5 km) with a relative heliocentric velocity of 13.78 km/s.

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

(2017 TJ2) (JPL ID 3785687) is a V-type (Basaltic Achondrite) Near-Earth Asteroid spanning 27.2m–60.8m (mean 44m). On 2026-10-25, it transits Earth's cislunar surveillance sector at 101.942 Lunar Distances (39,203,869 km) with a relative velocity of 13.78 km/s and a theoretical kinetic energy reserve of 2.88 megatons TNT. Its well-constrained heliocentric ephemeris passes safely outside Earth capture corridors while serving as an orbital calibration target.

Max Diameter (Ø)
60.82 m
Min: 27.2 m
Miss Distance
101.94 LD
39,203,868.5 km
Rel. Velocity
13.78 km/s
49,612 km/h
Kinetic Energy
8.02 MT
E = ½mv² TNT eq.

Exact Landmark Scale Comparison (60.82m)

1:1 Meter Scale
60.82m
(2017 TJ2)
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)24.95 mag
Spectral ClassificationV-type (Basaltic Achondrite)
Estimated Bolide Mass3.534e+8 kg
Kinetic Energy (E = ½mv²)8.02 MT TNT (3.36e+16 J)
Transient Crater Diameter / Depth1,331 m Ø / 280 m deep
5-PSI Structural Overpressure Radius3.88 km
Thermal 3rd-Degree Burn Radius6.57 km
Equivalent Seismic MagnitudeMw 5.2
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 +23.48
Abs. Magnitude H = 24.95
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 TJ2)

(2017 TJ2) (H = 24.9, Vmag ≈ 23.5) 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 5.80° · Lon 6.55°136,800 km
Node T+1Lat 10.45° · Lon 16.13°122,617 km
Node T+2Lat 14.20° · Lon 25.72°109,667 km
Node T+3Lat 16.96° · Lon 35.30°97,950 km
Node T+4Lat 18.67° · Lon 44.88°87,467 km
Node T+5Lat 19.30° · Lon 54.47°78,217 km

Planetary Defense Frequently Asked Questions (Schema.org FAQ)

How big is (2017 TJ2) compared to city landmarks?

(2017 TJ2) has an estimated diameter between 27.2m and 60.82m. At its upper-bound size of 60.82m, it stands 14% as tall as the 443m Empire State Building in New York City and 18% of the 330m Eiffel Tower.

Will (2017 TJ2) impact Earth during its 2026-10-25 approach?

No. NASA JPL Center for Near-Earth Object Studies (CNEOS) orbital solutions confirm (2017 TJ2) will pass safely at a minimum distance of 101.94 Lunar Distances (39,203,868.5 km). You can still simulate a hypothetical street-level impact in our 3D CesiumJS simulator.

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(2017 TJ2) — 3D Orbit, Size Comparison & Kinetic Impact Physics | Meteors.ai Space Network