Mission Control/ASTEROID DOSSIER: (2017 RJ15)
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NOMINAL CISLUNAR PASSAGEGEMMA ENGINE: LOCAL SERVER BOX [ACTIVE] • meteors-gemma:latest

(2017 RJ15)

Tracked by NASA JPL Near-Earth Object Web Service (NeoWs), (2017 RJ15) is a S-type (Silicate Stony) body measuring between 113.38m and 253.54m in diameter. On 2026-10-26, it completes a cislunar approach at 98.45 Lunar Distances (37,859,887.2 km) with a relative heliocentric velocity of 8.63 km/s.

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

(2017 RJ15) (JPL ID 3781448) is a S-type (Silicate Stony) Near-Earth Asteroid spanning 113.4m–253.5m (mean 183.5m). On 2026-10-26, it transits Earth's cislunar surveillance sector at 98.447 Lunar Distances (37,859,887 km) with a relative velocity of 8.63 km/s and a theoretical kinetic energy reserve of 81.97 megatons TNT. Its well-constrained heliocentric ephemeris passes safely outside Earth capture corridors while serving as an orbital calibration target.

Max Diameter (Ø)
253.54 m
Min: 113.38 m
Miss Distance
98.45 LD
37,859,887.2 km
Rel. Velocity
8.63 km/s
31,050 km/h
Kinetic Energy
227.591 MT
E = ½mv² TNT eq.

Exact Landmark Scale Comparison (253.54m)

1:1 Meter Scale
253.54m
(2017 RJ15)
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)21.85 mag
Spectral ClassificationS-type (Silicate Stony)
Estimated Bolide Mass2.560e+10 kg
Kinetic Energy (E = ½mv²)227.591 MT TNT (9.52e+17 J)
Transient Crater Diameter / Depth3,298 m Ø / 693 m deep
5-PSI Structural Overpressure Radius11.69 km
Thermal 3rd-Degree Burn Radius25.92 km
Equivalent Seismic MagnitudeMw 6.2
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 +20.30
Abs. Magnitude H = 21.85
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 RJ15)

(2017 RJ15) (H = 21.9, Vmag ≈ 20.3) 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 16.41° · Lon 163.40°136,800 km
Node T+1Lat 22.92° · Lon 172.98°122,617 km
Node T+2Lat 28.06° · Lon -177.43°109,667 km
Node T+3Lat 31.67° · Lon -167.85°97,950 km
Node T+4Lat 33.67° · Lon -158.27°87,467 km
Node T+5Lat 34.01° · Lon -148.68°78,217 km

Planetary Defense Frequently Asked Questions (Schema.org FAQ)

How big is (2017 RJ15) compared to city landmarks?

(2017 RJ15) has an estimated diameter between 113.38m and 253.54m. At its upper-bound size of 253.54m, it stands 57% as tall as the 443m Empire State Building in New York City and 77% of the 330m Eiffel Tower.

Will (2017 RJ15) impact Earth during its 2026-10-26 approach?

No. NASA JPL Center for Near-Earth Object Studies (CNEOS) orbital solutions confirm (2017 RJ15) will pass safely at a minimum distance of 98.45 Lunar Distances (37,859,887.2 km). You can still simulate a hypothetical street-level impact in our 3D CesiumJS simulator.

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(2017 RJ15) — 3D Orbit, Size Comparison & Kinetic Impact Physics | Meteors.ai Space Network