2014 HQ124 is a sub-kilometer asteroid, classified as near-Earth object and potentially hazardous asteroid of the Aten group, approximately 400 meters (1,300 feet) in diameter. It passed 3.25lunar distances (LD) from Earth on 8 June 2014.[8] It was discovered on 23 April 2014 by NEOWISE.[2] It is estimated that an impact event would have had the energy equivalent of 2,000megatons of TNT and would have created a 5km (3mi) impact crater.[9] The news media misleadingly nicknamed it The Beast.[10]2014 HQ124 previously passed this close to Earth in 1952[8] and will not again until at least 2307.[11] Radar imaging suggests it may be a contact binary.[12]
2014 HQ124 orbits the Sun at a distance of 0.6–1.1AU once every 0 years and 9 months (287 days; semi-major axis of 0.85AU). Its orbit has an eccentricity of 0.26 and an inclination of 26° with respect to the ecliptic.[3]
2014 close approach
2014 HQ124 radar images in June 2014
On 6 June 2014, the asteroid brightened to about apparent magnitude 13.7 while in the southern constellation of Horologium.[13] Near its closest approach to Earth of 3.25 lunar distances on 8 June 2014, the asteroid crossed the celestial equator, making it a northern hemisphere object. It however had an elongation of about 20 degrees from the Sun,[13] and was lost in astronomical twilight during the closest approach to Earth. The Goldstone Deep Space Network observed the asteroid later on 8 June 2014,[14] when the asteroid was between 3.6 and 3.8 lunar distances.[12]
2014 HQ124 orbit showing high inclination and 2014 Earth flyby
The sky trajectory of 2014 HQ124, as seen from earth, with 12-hour motion markers
Physical characteristics
According to the survey carried out by the NEOWISE mission of NASA's Wide-field Infrared Survey Explorer, 2014 HQ124 measures (0.409±0.168) kilometers in diameter and its surface has an albedo of (0.291±0.216) based on an absolute magnitude of 18.9.[4][5]
Radar observations at Goldstone suggest that the object is elongated and irregular in shape, with its long axis measuring at least 370 meters (1,200 feet). Lance Benner suspects it the be a contact binary, composed of two merged objects forming a single asteroid with a lobed shape.[12]
Photometric observations by astronomers with the Mission Accessible Near-Earth Objects Survey (MANOS) and subsequent evaluation by Brian Warner's Collaborative Asteroid Lightcurve Link, determined that 2014 HQ124 has a rotation period of at least 16 hours.[6][7] While the object's spectral type is unknown, Warner assumes it to be an S-type asteroid, based on its high albedo, which is typical for stony asteroids.[6]
Related objects
On average, an object about the size of 2014 HQ124 will pass this close to Earth every few years.[15] Similar events, where other 100+ meter diameter asteroids have or will soon pass less than 4LD from Earth, include:
4179 Toutatis (~3000meters in diameter) passed 4.0LD from Earth on 29 September 2004
2004 XP14 (~500meters in diameter) passed 1.1LD from Earth on 3 July 2006
(308635) 2005 YU55 (~360meters in diameter) passed 0.8LD from Earth on 8 November 2011
2014 EG45 (~140meters in diameter) passed 3.2LD from Earth on 4 March 2014[16]
(357439) 2004 BL86 (~600meters in diameter) passed 3.1LD from Earth on 26 January 2015[17]
See also
List of asteroid close approaches to Earth in 2014
References
"2014 HQ124". Minor Planet Center. Retrieved 8 March 2020.
Mainzer, A. K.; Bauer, J. M.; Cutri, R. M.; Grav, T.; Kramer, E. A.; Masiero, J. R.; etal. (June 2016). "NEOWISE Diameters and Albedos V1.0". NASA Planetary Data System: EAR-A-COMPIL-5-NEOWISEDIAM-V1.0. Bibcode:2016PDSS..247.....M.
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