(357439) 2004 BL86

Near-Earth asteroid discovered in 2004 From Wikipedia, the free encyclopedia

(357439) 2004 BL86 is a bright sub-kilometer asteroid and binary system, classified as a near-Earth object and potentially hazardous asteroid of the Apollo group, approximately 300 meters (980 ft) in diameter. It was discovered on 30 January 2004 by astronomers of the Lincoln Near-Earth Asteroid Research at Lincoln Laboratory's Experimental Test Site near Socorro, New Mexico.[3] Its 70-meter (200 ft) moon was discovered during the asteroid's close approach to the Earth in January 2015.[4][5]

Discoverydate30 January 2004
(357439) 2004 BL86
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(357439) 2004 BL86
Goldstone radar image of 2004 BL86 and its minor-planet moon
Discovery[1][2]
Discovered byLINEAR
Discovery siteLincoln Lab's ETS
Discovery date30 January 2004
Designations
(357439) 2004 BL86
NEO Â· PHA Â· Apollo[1][3]
Orbital characteristics[1]
Epoch 4 September 2017 (JD 2458000.5)
Uncertainty parameter 0
Observation arc4,863 d (13.31 yr)
Aphelion2.1070 AU
Perihelion0.8974 AU
1.5022 AU
Eccentricity0.4026
673 d (1.84 yr)
169.27°
0° 32m 7.08s / day
Inclination23.775°
126.69°
311.45°
Known satellites1[4][5]
Earth MOID0.0092 AU (3.6 LD)
Physical characteristics
0.263±0.026 km[6]
0.290±0.030 km[7]
0.325±0.025 km[5][a]
2.620±0.001 h[6]
2.6205±0.0003 h[8]
2.637±0.024 h[7]
0.40[7]
0.40±0.08[6]
V[7][9][10]
19.05[9]
19.3[1][7]
19.51±0.02[6]
Close

2015 Earth approach

On 26 January 2015 at 16:20 UTC, 2004 BL86 passed 1,199,600 km (745,400 mi), or 3.1 lunar distances, from Earth.[11] The asteroid briefly peaked around apparent magnitude 9 and was near the celestial equator.[12] The asteroid was visible in telescopes with objectives of 100 mm (4 in) or larger; high-end binoculars under a dark sky may also have worked.[13] Near closest approach the asteroid was moving about 2.5 degrees per hour (2.5 arcseconds per second).[12][14] The asteroid came to opposition (furthest elongation in the sky from the Sun) on 27 January 2015 at 04:37 UTC.[12] Around 5:00 UTC, the asteroid was near M44 (the Beehive Cluster).[14]

The 26 January 2015 approach of 3.1 lunar distances was the closest approach of 2004 BL86 for at least the next 200 years.[11][15] For comparison, 2015 TB145, about twice the size of 2004 BL86, passed 486,800 km (302,500 mi), or 1.3 lunar distances, from Earth on 31 October 2015.[16]

Satellite

A minor-planet moon orbiting (357439) 2004 BL86 was first detected by ground-based telescopes by Joe Pollock and Petr Pravec.[8][17] Observations by the Goldstone Deep Space Communications Complex and Green Bank Telescope confirmed that it is a binary asteroid with a secondary roughly 70 meters (200 ft) across.[5] The secondary is estimated to orbit at least 500 meters (1,600 ft) from the primary.[4] About 16% of asteroids over 200 meters (660 ft) in diameter are thought to be binaries.[5]

Numbering and naming

This minor planet was numbered on 27 March 2013 (M.P.C. 83151).[18] As of 2020, it has not been named.[3]

Notes

  1. Radar Team 2015a: diameter primary 0.325±0.025 km. Diameter secondary 0.070 km. The satellites discovery is credited to Pollock et al.[8] Summary figures for (357439) 2004 BL86 at LCDB

References

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