astro.wikisort.org - Asteroid(52760) 1998 ML14, provisional designation 1998 ML14, is a stony asteroid, classified as near-Earth object of the Apollo group and potentially hazardous asteroid, approximately 1 kilometer in diameter. It was discovered on 24 June 1998, by the LINEAR survey at the Lincoln Laboratory's Experimental Test Site in Socorro, New Mexico.[2]
(52760) 1998 ML14|
Discovered by | LINEAR |
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Discovery site | Lincoln Lab's ETS |
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Discovery date | 24 June 1998 |
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MPC designation | (52760) 1998 ML14 |
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Alternative designations | 1998 ML14 |
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Minor planet category | NEO · Apollo[1][2] · PHA[1][2] |
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Epoch 4 September 2017 (JD 2458000.5) |
Uncertainty parameter 0 |
Observation arc | 15.54 yr (5,676 days) |
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Aphelion | 3.9104 AU |
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Perihelion | 0.9071 AU |
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Semi-major axis | 2.4088 AU |
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Eccentricity | 0.6234 |
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Orbital period (sidereal) | 3.74 yr (1,366 days) |
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Mean anomaly | 21.557° |
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Mean motion | 0° 15m 48.96s / day |
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Inclination | 2.4274° |
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Longitude of ascending node | 338.72° |
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Argument of perihelion | 20.324° |
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Earth MOID | 0.0167 AU · 6.5 LD |
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Dimensions | 1.0±0.05 km[3] 0.81±0.16 km[4] 1.17 km (derived)[5] |
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Synodic rotation period | 14.98±0.06 h[6] 14.98±0.06 h[7] 14.28±0.01 h[8] |
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Geometric albedo | 0.27±0.24[4] 0.20 (assumed)[5] |
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Spectral type | S (Tholen)[5] |
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Absolute magnitude (H) | 16.93±0.01[7] · 17.02[5][6] · 17.5[1] |
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Description
1998 ML14 orbits the Sun at a distance of 0.9–3.9 AU once every 3 years and 9 months (1,366 days). Its orbit has an eccentricity of 0.62 and an inclination of 2° with respect to the ecliptic.[1] It is also a Mars-crossing asteroid.
Shortly after its discovery, 1998 ML14 was imaged by radar at Goldstone and Arecibo.[9]
The study showed that the asteroid has a rotation period of 15 hours, and a shape that is roughly spherical, with some steep protrusions and large craters.[6][7][8]
On 24 August 2013 it passed at a distance of 21.9 Lunar distances.[1] It was hoped to be observed by Goldstone radar.[10]
Numbering and naming
This minor planet was numbered by the Minor Planet Center on 16 February 2003.[11] As of 2018, it has not been named.[2]
References
- "JPL Small-Body Database Browser: 52760 (1998 ML14)" (2014-01-07 last obs.). Jet Propulsion Laboratory. Retrieved 23 October 2017.
- "52760 (1998 ML14)". Minor Planet Center. Retrieved 23 October 2017.
- Ostro, Steven J.; Hudson, R. Scott; Benner, Lance A. M.; Nolan, Michael C.; Giorgini, Jon D.; Scheeres, Daniel J.; et al. (September 2001). "Radar observations of asteroid 1998 ML14". Meteoritics and Planetary Science. 36 (9): 1225–1236. Bibcode:2001M&PS...36.1225O. doi:10.1111/j.1945-5100.2001.tb01956.x.
- Mueller, Michael; Delbo', M.; Hora, J. L.; Trilling, D. E.; Bhattacharya, B.; Bottke, W. F.; et al. (April 2011). "ExploreNEOs. III. Physical Characterization of 65 Potential Spacecraft Target Asteroids" (PDF). The Astronomical Journal. 141 (4): 9. Bibcode:2011AJ....141..109M. doi:10.1088/0004-6256/141/4/109.
- "LCDB Data for (52760)". Asteroid Lightcurve Database (LCDB). Retrieved 23 October 2017.
- Hicks, M. D.; Weissman, P. R.; Rabinowitz, D. L.; Chamberlin, A. B.; Buratti, B. J.; Lee, C. O. (September 1998). "Close Encounters: Observations of the Earth-crossing Asteroids 1998 KY26 and 1998 ML14". American Astronomical Society. 30: 1029. Bibcode:1998DPS....30.1006H.
- Hicks, M.; Weissman, P. (August 1998). "1998 ML_14". IAU Circ. 6987 (6987): 1. Bibcode:1998IAUC.6987....1H.
- Warner, Brian D. (April 2014). "Near-Earth Asteroid Lightcurve Analysis at CS3-Palmer Divide Station: 2013 September–December". The Minor Planet Bulletin. 41 (2): 113–124. Bibcode:2014MPBu...41..113W. ISSN 1052-8091. PMC 7268210. PMID 32494788.
- "NEA CIRCULAR POLARIZATION RATIO RANKING". Asteroid Radar Research. 11 April 2006. Archived from the original on 25 April 2001. Retrieved 15 December 2009.
- Goldstone radar
- "MPC/MPO/MPS Archive". Minor Planet Center. Retrieved 24 February 2018.
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