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(242450) 2004 QY2 (prov. designation : 2004 QY2 ) is an asteroid on an eccentric orbit, classified as near-Earth object and potentially hazardous asteroid of the Apollo group , approximately 3 kilometers (2 miles) in diameter. It was discovered on 20 August 2004 by the Siding Spring Survey at an apparent magnitude of 16.5 using the 0.5-metre (20 in ) Uppsala Southern Schmidt Telescope .[2] It is one of the largest potentially hazardous asteroids known to exist.[6]
Orbit and classification [ edit ]
2004 QY2 orbits the Sun at a distance of 0.6–1.6 AU once every 14 months (412 days; semi-major axis of 1.08 AU ). Its orbit has an eccentricity of 0.48 and an inclination of 37° with respect to the ecliptic .[3] The body's observation arc begins with its official discovery observation at Siding Spring.[1]
The object is a member of the Apollo asteroids , the largest subgroup of near-Earth asteroids which cross the orbit of Earth . Unlike many other members of this dynamical group, 2004 QY2 is not a Mars-crosser , as its aphelion is too small to cross the orbit of the Red Planet at 1.66 AU.[3]
Close approaches [ edit ]
With an absolute magnitude of 14.7, 2004 QY2 is one of the brightest potentially hazardous asteroids ever discovered (see PHA-list ) .[6] [7] It has an Earth minimum orbital intersection distance of 0.0469 AU (7,020,000 km ), which translates into 18.3 lunar distances .[3] On 29 July 2012, it passed Earth at a distance of 0.4314 AU (64,540,000 km; 40,100,000 mi ).[3]
Sentry Risk Table [ edit ]
Due to its originally estimated size of 5.5 kilometers, 2004 QY2 was one of the largest objects to appear on the Sentry Risk Table .[8] It was removed from the Sentry Risk Table on 25 August 2004.[9]
Physical characteristics [ edit ]
According to the survey carried out by the NEOWISE mission of NASA's Wide-field Infrared Survey Explorer , 2004 QY2 has an albedo of 0.274, and it measures 2.914 and 3.320 kilometers in diameter, respectively.[4] [5]
As of 2018, no rotational lightcurve of 2004 QY2 has been obtained from photometric observations. The body's rotation period , shape and spin axis remain unknown.[10] In addition, the body's spectral type has never been assessed.[3] [10]
Numbering and naming [ edit ]
This minor planet was numbered by the Minor Planet Center on 26 June 2006.[11] As of 2018, it has not been named .[1]
References [ edit ]
^ a b "MPEC 2004-Q27 : 2004 QY2 (K04Q02Y)" . IAU Minor Planet Center. 22 August 2004. Retrieved 17 June 2012 .
^ a b c d e f g h "JPL Small-Body Database Browser: 242450 (2004 QY2)" (2016-04-01 last obs.). Jet Propulsion Laboratory . Retrieved 19 January 2018 .
^ a b c Nugent, C. R.; Mainzer, A.; Masiero, J.; Bauer, J.; Cutri, R. M.; Grav, T.; et al. (December 2015). "NEOWISE Reactivation Mission Year One: Preliminary Asteroid Diameters and Albedos". The Astrophysical Journal . 814 (2 ): 13. arXiv :1509.02522 . Bibcode :2015ApJ...814..117N . doi :10.1088/0004-637X/814/2/117 .
^ a b Mainzer, A.; Bauer, J.; Cutri, R. M.; Grav, T.; Masiero, J.; Beck, R.; et al. (September 2014). "Initial Performance of the NEOWISE Reactivation Mission". The Astrophysical Journal . 792 (1 ): 14. arXiv :1406.6025 . Bibcode :2014ApJ...792...30M . doi :10.1088/0004-637X/792/1/30 .
^ a b "List of the Potentially Hazardous Asteroids (PHAs)" . Minor Planet Center . Retrieved 19 January 2018 .
^ "JPL Small-Body Database Search Engine: PHAs and H < 15 (mag)" . JPL Solar System Dynamics. Retrieved 19 January 2018 .
^ "Major News about Minor Objects" . hohmanntransfer. 22 August 2004. Archived from the original on 5 November 2016. Retrieved 19 January 2018 .
^ "Sentry: Earth Impact Monitoring – Removed Objects" . NASA/JPL CNEOS – Center for Near-Earth Object Studies. Retrieved 19 January 2018 .
^ a b "LCDB Data for (242450)" . Asteroid Lightcurve Database (LCDB). Retrieved 19 January 2018 .
^ "MPC/MPO/MPS Archive" . Minor Planet Center . Retrieved 25 February 2018 .
External links [ edit ]
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