2014 HQ124 orbits the Sun at a distance of 0.6–1.1 AU once every 0 years and 9 months (287 days; semi-major axis of 0.85 AU). Its orbit has an eccentricity of 0.26 and an inclination of 26° with respect to the ecliptic.[3]
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 to 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 4 LD from Earth, include:
4179 Toutatis (~3000 meters in diameter) passed 4.0 LD from Earth on 29 September 2004
2004 XP14 (~500 meters in diameter) passed 1.1 LD from Earth on 3 July 2006
(308635) 2005 YU55 (~360 meters in diameter) passed 0.8 LD from Earth on 8 November 2011
2014 EG45 (~140 meters in diameter) passed 3.2 LD from Earth on 4 March 2014[16]
(357439) 2004 BL86 (~600 meters in diameter) passed 3.1 LD from Earth on 26 January 2015[17]
^ abcMainzer, A. K.; Bauer, J. M.; Cutri, R. M.; Grav, T.; Kramer, E. A.; Masiero, J. R.; et al. (June 2016). "NEOWISE Diameters and Albedos V1.0". NASA Planetary Data System: EAR-A-COMPIL-5-NEOWISEDIAM-V1.0. Bibcode:2016PDSS..247.....M.