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2019 BZ3
Very small near-Earth asteroid From Wikipedia, the free encyclopedia
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2019 BZ3 is a very small near-Earth asteroid of the Apollo group, approximately 6 meters (20 feet) in diameter. It was first observed by the Mount Lemmon Survey on 28 January 2019, just hours after the asteroid's sub-lunar flyby of Earth at less than 0.12 lunar distance.[1][4]
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Orbit and classification
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2019 BZ3 is an Apollo asteroid, the largest subgroup of near-Earth objects. It orbits the Sun at a distance of 0.96–3.6 AU once every 3 years and 6 months (1,268 days; semi-major axis of 2.29 AU). Its orbit has a high eccentricity of 0.58 and an inclination of 11° with respect to the ecliptic.[2] The body still has a high orbital uncertainty of 5 and 7, respectively.[1][2] Its observation arc of only 8 days begins with its official first observation at Mount Lemmon Observatory on 28 January 2019.[1]
Close approaches
2019 BZ3 has an Earth minimum orbital intersection distance of 0.000457 AU (68,000 km), which corresponds to 0.18 lunar distances (LD).[2] Due to its very small size, however, 2019 BZ3 is not a potentially hazardous asteroid, which are required to be approximately 140 meters (460 ft) in diameter, that is, to be brighter than an absolute magnitude of 22.
- Flybys
On 27 January 2019 at UTC 23:29, 2019 BZ3 passed Earth at a nominal distance of 48,130 km (0.125 LD) with a relative velocity of 11.37 km. Six hours later, it flew by the Moon at 350400 km.[2][4] The object's next close approaches will occur on 17 December 2025 at a much greater distance of 56 LD (0.143 AU), and on 29 January 2085 at 5.5 LD (0.0142 AU).[5]
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Numbering and naming
This minor planet has not yet been numbered by the Minor Planet Center and remains unnamed.[1]
Physical characteristics
2019 BZ3 has an undetermined spectral type. Based on a generic magnitude-to-diameter conversion, the asteroid measures approximately 6 meter in diameter for an assumed albedo of 0.15 and absolute magnitude 28.8.[3] The estimated diameter may vary between 5 and 10 meters depending on whether an albedo for a dark carbonaceous (0.05) or a bright stony (0.25) asteroid is assumed.[3]
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References
External links
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