Mission Control/ASTEROID DOSSIER: (2014 QS295)
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(2014 QS295)

Tracked by NASA JPL Near-Earth Object Web Service (NeoWs), (2014 QS295) is a M-type (Metallic Nickel-Iron) body measuring between 103.41m and 231.23m in diameter. On 2026-10-22, it completes a cislunar approach at 121.87 Lunar Distances (46,868,764.8 km) with a relative heliocentric velocity of 9.55 km/s.

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

(2014 QS295) (JPL ID 3683469) is a M-type (Metallic Nickel-Iron) Near-Earth Asteroid spanning 103.4m–231.2m (mean 167.3m). On 2026-10-22, it transits Earth's cislunar surveillance sector at 121.873 Lunar Distances (46,868,765 km) with a relative velocity of 9.55 km/s and a theoretical kinetic energy reserve of 141.57 megatons TNT. Its well-constrained heliocentric ephemeris passes safely outside Earth capture corridors while serving as an orbital calibration target.

Max Diameter (Ø)
231.23 m
Min: 103.41 m
Miss Distance
121.87 LD
46,868,764.8 km
Rel. Velocity
9.55 km/s
34,373 km/h
Kinetic Energy
211.571 MT
E = ½mv² TNT eq.

Exact Landmark Scale Comparison (231.23m)

1:1 Meter Scale
231.23m
(2014 QS295)
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)22.05 mag
Spectral ClassificationM-type (Metallic Nickel-Iron)
Estimated Bolide Mass1.942e+10 kg
Kinetic Energy (E = ½mv²)211.571 MT TNT (8.85e+17 J)
Transient Crater Diameter / Depth3,210 m Ø / 674 m deep
5-PSI Structural Overpressure Radius11.41 km
Thermal 3rd-Degree Burn Radius25.15 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 +21.00
Abs. Magnitude H = 22.05
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: (2014 QS295)

(2014 QS295) (H = 22.1, Vmag ≈ 21.0) is below consumer optical detection thresholds (requires ≥1000mm survey aperture); explore certified meteorite specimens[↗] or indoor optical projection instead.

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Campo del Cielo Meteorite Specimen (Certified Iron-Nickel)

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 26.30° · Lon -103.10°136,800 km
Node T+1Lat 34.56° · Lon -93.52°122,617 km
Node T+2Lat 40.99° · Lon -83.93°109,667 km
Node T+3Lat 45.41° · Lon -74.35°97,950 km
Node T+4Lat 47.67° · Lon -64.77°87,467 km
Node T+5Lat 47.74° · Lon -55.18°78,217 km

Planetary Defense Frequently Asked Questions (Schema.org FAQ)

How big is (2014 QS295) compared to city landmarks?

(2014 QS295) has an estimated diameter between 103.41m and 231.23m. At its upper-bound size of 231.23m, it stands 52% as tall as the 443m Empire State Building in New York City and 70% of the 330m Eiffel Tower.

Will (2014 QS295) impact Earth during its 2026-10-22 approach?

No. NASA JPL Center for Near-Earth Object Studies (CNEOS) orbital solutions confirm (2014 QS295) will pass safely at a minimum distance of 121.87 Lunar Distances (46,868,764.8 km). You can still simulate a hypothetical street-level impact in our 3D CesiumJS simulator.

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(2014 QS295) — 3D Orbit, Size Comparison & Kinetic Impact Physics | Meteors.ai Space Network