Mission Control/ASTEROID DOSSIER: (2009 UY17)
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POTENTIALLY HAZARDOUS ASTEROID (PHA)GEMMA ENGINE: LOCAL SERVER BOX [ACTIVE] • meteors-gemma:latest

(2009 UY17)

Tracked by NASA JPL Near-Earth Object Web Service (NeoWs), (2009 UY17) is a V-type (Basaltic Achondrite) body measuring between 174m and 389.08m in diameter. On 2026-10-19, it completes a cislunar approach at 68.13 Lunar Distances (26,198,830.9 km) with a relative heliocentric velocity of 23.62 km/s.

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

(2009 UY17) (JPL ID 3472299) is a V-type (Basaltic Achondrite) Near-Earth Asteroid spanning 174.0m–389.1m (mean 281.5m). On 2026-10-19, it transits Earth's cislunar surveillance sector at 68.125 Lunar Distances (26,198,831 km) with a relative velocity of 23.62 km/s and a theoretical kinetic energy reserve of 2218.93 megatons TNT. Classified as a Potentially Hazardous Asteroid (PHA) due to its Minimum Orbit Intersection Distance (MOID <= 0.05 AU) and absolute magnitude (H <= 22.0), it remains under high-priority radar and optical astrometric tracking.

Max Diameter (Ø)
389.08 m
Min: 174 m
Miss Distance
68.13 LD
26,198,830.9 km
Rel. Velocity
23.62 km/s
85,025 km/h
Kinetic Energy
6,167.386 MT
E = ½mv² TNT eq.

Exact Landmark Scale Comparison (389.08m)

1:1 Meter Scale
389.08m
(2009 UY17)
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)20.92 mag
Spectral ClassificationV-type (Basaltic Achondrite)
Estimated Bolide Mass9.252e+10 kg
Kinetic Energy (E = ½mv²)6,167.386 MT TNT (2.58e+19 J)
Transient Crater Diameter / Depth7,175 m Ø / 1,507 m deep
5-PSI Structural Overpressure Radius34.74 km
Thermal 3rd-Degree Burn Radius100.25 km
Equivalent Seismic MagnitudeMw 7.1
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 +18.51
Abs. Magnitude H = 20.92
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: (2009 UY17)

(2009 UY17) (H = 20.9, Vmag ≈ 18.5) 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 22.06° · Lon 167.65°136,800 km
Node T+1Lat 29.57° · Lon 177.23°122,617 km
Node T+2Lat 35.45° · Lon -173.18°109,667 km
Node T+3Lat 39.52° · Lon -163.60°97,950 km
Node T+4Lat 41.67° · Lon -154.02°87,467 km
Node T+5Lat 41.85° · Lon -144.43°78,217 km

Planetary Defense Frequently Asked Questions (Schema.org FAQ)

How big is (2009 UY17) compared to city landmarks?

(2009 UY17) has an estimated diameter between 174m and 389.08m. At its upper-bound size of 389.08m, it stands 88% as tall as the 443m Empire State Building in New York City and 118% of the 330m Eiffel Tower.

Will (2009 UY17) impact Earth during its 2026-10-19 approach?

No. NASA JPL Center for Near-Earth Object Studies (CNEOS) orbital solutions confirm (2009 UY17) will pass safely at a minimum distance of 68.13 Lunar Distances (26,198,830.9 km). You can still simulate a hypothetical street-level impact in our 3D CesiumJS simulator.

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(2009 UY17) — 3D Orbit, Size Comparison & Kinetic Impact Physics | Meteors.ai Space Network