29075 (1950 DA)
Tracked by NASA JPL Near-Earth Object Web Service (NeoWs), 29075 (1950 DA) is a Not published by JPL SBDB body measuring between 1300m and 1300m in diameter. On 2032-03-02, it completes a cislunar approach at 29.48 Lunar Distances (11,332,364 km) with a relative heliocentric velocity of 15.58 km/s.
29075 (1950 DA) (JPL ID 29075) is a Not published by JPL SBDB Near-Earth Asteroid spanning 1300.0m–1300.0m (mean 1300m). On 2032-03-02, it transits Earth's cislunar surveillance sector at 29.481 Lunar Distances (11,332,364 km) with a relative velocity of 15.58 km/s and a theoretical kinetic energy reserve of 95101.37 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.
Exact Landmark Scale Comparison (1300m)
Kinetic Impact Physics & Orbital Parameters
29075 (1950 DA) (H = 17.3, Vmag ≈ 13.0) is below consumer optical detection thresholds (requires ≥1000mm survey aperture); explore certified meteorite specimens[↗] or indoor optical projection instead.
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.
Satin-black 5W warm-white LED optical glass lens planetarium projecting 60,000 stars and simulated meteor shower trajectories indoors.
3D Ephemeris Trajectory Waypoints
Planetary Defense Frequently Asked Questions (Schema.org FAQ)
How big is 29075 (1950 DA) compared to city landmarks?
29075 (1950 DA) has an estimated diameter between 1300m and 1300m. At its upper-bound size of 1300m, it stands 293% as tall as the 443m Empire State Building in New York City and 394% of the 330m Eiffel Tower.
What does the stored 2032-03-02 close-approach estimate show?
This catalog snapshot lists a nominal miss distance of 29.48 Lunar Distances (11,332,364 km) for 29075 (1950 DA). 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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Authentic coarse octahedrite Group IAB iron-nickel meteorite fragment (92.9% Fe, 6.7% Ni) recovered from the Chaco crater field.
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