Mission Control/ASTEROID DOSSIER: (2019 TD8)
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NOMINAL CISLUNAR PASSAGEGEMMA ENGINE: LOCAL SERVER BOX [ACTIVE] • meteors-gemma:latest

(2019 TD8)

Tracked by NASA JPL Near-Earth Object Web Service (NeoWs), (2019 TD8) is a S-type (Silicate Stony) body measuring between 33.46m and 74.82m in diameter. On 2026-10-20, it completes a cislunar approach at 145.61 Lunar Distances (55,996,035.4 km) with a relative heliocentric velocity of 17.22 km/s.

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

(2019 TD8) (JPL ID 3879288) is a S-type (Silicate Stony) Near-Earth Asteroid spanning 33.5m–74.8m (mean 54.1m). On 2026-10-20, it transits Earth's cislunar surveillance sector at 145.607 Lunar Distances (55,996,035 km) with a relative velocity of 17.22 km/s and a theoretical kinetic energy reserve of 8.37 megatons TNT. Its well-constrained heliocentric ephemeris passes safely outside Earth capture corridors while serving as an orbital calibration target.

Max Diameter (Ø)
74.82 m
Min: 33.46 m
Miss Distance
145.61 LD
55,996,035.4 km
Rel. Velocity
17.22 km/s
61,999 km/h
Kinetic Energy
23.319 MT
E = ½mv² TNT eq.

Exact Landmark Scale Comparison (74.82m)

1:1 Meter Scale
74.82m
(2019 TD8)
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)24.5 mag
Spectral ClassificationS-type (Silicate Stony)
Estimated Bolide Mass6.579e+8 kg
Kinetic Energy (E = ½mv²)23.319 MT TNT (9.76e+16 J)
Transient Crater Diameter / Depth1,726 m Ø / 362 m deep
5-PSI Structural Overpressure Radius5.51 km
Thermal 3rd-Degree Burn Radius10.18 km
Equivalent Seismic MagnitudeMw 5.5
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 +23.88
Abs. Magnitude H = 24.50
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: (2019 TD8)

(2019 TD8) (H = 24.5, Vmag ≈ 23.9) 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 35.50° · Lon 27.80°136,800 km
Node T+1Lat 45.37° · Lon 37.38°122,617 km
Node T+2Lat 53.01° · Lon 46.97°109,667 km
Node T+3Lat 58.16° · Lon 56.55°97,950 km
Node T+4Lat 60.67° · Lon 66.13°87,467 km
Node T+5Lat 60.49° · Lon 75.72°78,217 km

Planetary Defense Frequently Asked Questions (Schema.org FAQ)

How big is (2019 TD8) compared to city landmarks?

(2019 TD8) has an estimated diameter between 33.46m and 74.82m. At its upper-bound size of 74.82m, it stands 17% as tall as the 443m Empire State Building in New York City and 23% of the 330m Eiffel Tower.

Will (2019 TD8) impact Earth during its 2026-10-20 approach?

No. NASA JPL Center for Near-Earth Object Studies (CNEOS) orbital solutions confirm (2019 TD8) will pass safely at a minimum distance of 145.61 Lunar Distances (55,996,035.4 km). You can still simulate a hypothetical street-level impact in our 3D CesiumJS simulator.

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(2019 TD8) — 3D Orbit, Size Comparison & Kinetic Impact Physics | Meteors.ai Space Network