Mission Control/ASTEROID DOSSIER: (2015 FV284)
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POTENTIALLY HAZARDOUS ASTEROID (PHA)NASA CATALOG + DOCUMENTED ANALYSIS

(2015 FV284)

Tracked by NASA JPL Near-Earth Object Web Service (NeoWs), (2015 FV284) is a Unreported by NASA NeoWs body measuring between 175.61m and 392.68m in diameter. On 2026-11-09, it completes a cislunar approach at 100.12 Lunar Distances (38,504,605.9 km) with a relative heliocentric velocity of 15.57 km/s.

AI-ASSISTED SUMMARY (may contain errors):

(2015 FV284) (JPL ID 3715094) is a Unreported by NASA NeoWs Near-Earth Asteroid spanning 175.6m–392.7m (mean 284.1m). On 2026-11-09, it transits Earth's cislunar surveillance sector at 100.124 Lunar Distances (38,504,606 km) with a relative velocity of 15.57 km/s and a theoretical kinetic energy reserve of 991.95 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)
392.68 m
Min: 175.61 m
Miss Distance
100.12 LD
38,504,605.9 km
Rel. Velocity
15.57 km/s
56,070 km/h
Kinetic Energy
2,757.215 MT
E = ½mv² TNT eq.

Exact Landmark Scale Comparison (392.68m)

1:1 Meter Scale
392.68m
(2015 FV284)
443m
Manhattan
227m
Golden Gate
330m
Eiffel Tower
828m
Burj Khalifa
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Kinetic Impact Physics & Orbital Parameters

45° Incidence · 3,000 kg/m³
Absolute Magnitude (H)20.9 mag
Spectral ClassificationUnreported by NASA NeoWs
Estimated Bolide Mass9.511e+10 kg
Kinetic Energy (E = ½mv²)2,757.215 MT TNT (1.15e+19 J)
Transient Crater Diameter / Depth6,017 m Ø / 1,264 m deep
5-PSI Structural Overpressure Radius26.63 km
Thermal 3rd-Degree Burn Radius72.07 km
Equivalent Seismic MagnitudeMw 6.9
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 +19.39
Abs. Magnitude H = 20.90
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: (2015 FV284)

(2015 FV284) (H = 20.9, Vmag ≈ 19.4) 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 43.98° · Lon -89.50°136,800 km
Node T+1Lat 55.35° · Lon -79.92°122,617 km
Node T+2Lat 64.09° · Lon -70.33°109,667 km
Node T+3Lat 69.92° · Lon -60.75°97,950 km
Node T+4Lat 72.67° · Lon -51.17°87,467 km
Node T+5Lat 72.26° · Lon -41.58°78,217 km

Planetary Defense Frequently Asked Questions (Schema.org FAQ)

How big is (2015 FV284) compared to city landmarks?

(2015 FV284) has an estimated diameter between 175.61m and 392.68m. At its upper-bound size of 392.68m, it stands 89% as tall as the 443m Empire State Building in New York City and 119% of the 330m Eiffel Tower.

What does the stored 2026-11-09 close-approach estimate show?

This catalog snapshot lists a nominal miss distance of 100.12 Lunar Distances (38,504,605.9 km) for (2015 FV284). This is not an impact prediction; check the latest NASA JPL record for updated orbital estimates. The 3D impact simulation is hypothetical.

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(2015 FV284) — 3D Orbit, Size Comparison & Kinetic Impact Physics | Meteors.ai Space Network