Astronomy:2014 HQ124
Radar image of 2014 HQ124 taken by the Arecibo Observatory on 8 June 2014 | |
Discovery[1][2] | |
---|---|
Discovered by | NEOWISE (C51) |
Discovery date | 23 April 2014 |
Designations | |
2014 HQ124 | |
Minor planet category | NEO · Aten · PHA[1][3] |
Orbital characteristics[3] | |
Epoch 31 May 2020 (JD 2459000.5) | |
Uncertainty parameter 1 | |
Observation arc | 4.09 yr (1,495 d) |
|{{{apsis}}}|helion}} | 1.0712 AU |
|{{{apsis}}}|helion}} | 0.6303 AU |
0.8508 AU | |
Eccentricity | 0.2591 |
Orbital period | 287 days |
Mean anomaly | 97.870° |
Mean motion | 1° 15m 21.6s / day |
Inclination | 26.371° |
Longitude of ascending node | 257.56° |
144.51° | |
Earth MOID | 0.0084 astronomical unit|AU (3.27 LD) |
Physical characteristics | |
Mean diameter | 0.409±0.168 km[4][5] |
Rotation period | >16 h[6][7] |
Geometric albedo | 0.291±0.216[4][5] |
S (assumed)[6] | |
Absolute magnitude (H) | 18.9[1][3] |
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 3.25 lunar 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 2,000 megatons of TNT and would have created a 5 km (3 mi) 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]
Orbit
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]
2014 close approach
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]
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 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]
See also
- List of asteroid close approaches to Earth in 2014
References
- ↑ 1.0 1.1 1.2 "2014 HQ124". Minor Planet Center. https://www.minorplanetcenter.net/db_search/show_object?object_id=2014+HQ124.
- ↑ 2.0 2.1 "MPEC 2014-H67: 2014 HQ124". IAU Minor Planet Center. 2014-04-28. http://www.minorplanetcenter.net/mpec/K14/K14H67.html. (K14HC4Q)
- ↑ 3.0 3.1 3.2 3.3 "JPL Small-Body Database Browser: (2014 HQ124)". Jet Propulsion Laboratory. https://ssd.jpl.nasa.gov/sbdb.cgi?sstr=3669253.
- ↑ 4.0 4.1 4.2 Mainzer, 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.
- ↑ 5.0 5.1 5.2 "Asteroid 2014 HQ124". Small Bodies Data Ferret. https://sbntools.psi.edu/ferret/SimpleSearch/results.action?targetName=2014+HQ124.
- ↑ 6.0 6.1 6.2 6.3 "LCDB Data for (2014+HQ124)". Asteroid Lightcurve Database (LCDB). http://www.minorplanet.info/PHP/generateOneAsteroidInfo.php?AstInfo=2014+HQ124.
- ↑ 7.0 7.1 Thirouin, A.; Moskovitz, N.; Binzel, R. P.; Christensen, E.; DeMeo, F. E.; Person, M. J. et al. (December 2016). "The Mission Accessible Near-Earth Objects Survey (MANOS): First Photometric Results". The Astronomical Journal 152 (6): 163. doi:10.3847/0004-6256/152/6/163. ISSN 0004-6256. Bibcode: 2016AJ....152..163T.
- ↑ 8.0 8.1 "JPL Close-Approach Data: (2014 HQ124)". http://ssd.jpl.nasa.gov/sbdb.cgi?sstr=2014HQ124;cad=1#cad.
- ↑ Mike Wall (2014-06-06). ""Beast" Asteroid to Fly by Earth on Sunday". Scientific American. http://www.scientificamerican.com/article/beast-asteroid-to-fly-by-earth-on-sunday/.
- ↑ @AreciboRadar (8 June 2014). "For the record, we do not use nicknames to refer to asteroids. Anthropomorphizing nature is confusing and misleading.". https://twitter.com/AreciboRadar/status/475709720842366977.
- ↑ "This was the closest Earth encounter by the object until at least 2307.". Twitter: Michael Busch. 2014-06-10. https://twitter.com/michael_w_busch/status/476449735335632896.
- ↑ 12.0 12.1 12.2 Dyches, Preston (2014-06-12). "Giant Telescopes Pair Up to Image Near-Earth Asteroid". JPL news. Jet Propulsion Laboratory. http://www.jpl.nasa.gov/news/news.php?release=2014-186.
- ↑ 13.0 13.1 "2014HQ124 Ephemerides for 4 June 2014 through 10 June 2014". NEODyS (Near Earth Objects – Dynamic Site). http://newton.spacedys.com/neodys/index.php?pc=1.1.3.1&n=2014HQ124&oc=500&y0=2014&m0=6&d0=4&h0=0&mi0=0&y1=2014&m1=6&d1=10&h1=0&mi1=0&ti=2.0&tiu=hours.
- ↑ Lance A. M. Benner (2014-05-30). "Goldstone Radar Observations Planning: 2014 HQ124". NASA/JPL Asteroid Radar Research. http://echo.jpl.nasa.gov/asteroids/2014HQ124/2014HQ124_planning.html.
- ↑ "Asteroid Discovered by NASA to Pass Earth Safely". Jet Propulsion Laboratory. 2014-06-06. http://www.jpl.nasa.gov/news/news.php?release=2014-178.
- ↑ "JPL Close-Approach Data: (2014 EG45)". http://ssd.jpl.nasa.gov/sbdb.cgi?sstr=2014EG45;cad=1#cad.
- ↑ "JPL Close-Approach Data: 357439 (2004 BL86)". http://ssd.jpl.nasa.gov/sbdb.cgi?sstr=2004BL86;cad=1#cad.
External links
- Near-Earth Asteroid 2014 HQ124 (Slooh broadcast 5 June 2014)
- High Resolution Radar at Arecibo Observatory Reveals Asteroid As a Beauty, Not a Beast (USRA June 12, 2014)
- 2014 HQ124 at NeoDyS-2, Near Earth Objects—Dynamic Site
- Ephemeris · Obs prediction · Orbital info · MOID · Proper elements · Obs info · Close · Physical info · NEOCC
- 2014 HQ124 at ESA–space situational awareness
- 2014 HQ124 at the JPL Small-Body Database
Original source: https://en.wikipedia.org/wiki/2014 HQ124.
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