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2024 McLaughlin

From Wikipedia, the free encyclopedia
Asteroid on the inner regions of the Asteroid belt

2024 McLaughlin
Discovery[1]
Discovered byIndiana University
(Indiana Asteroid Program)
Discovery siteGoethe Link Obs.
Discovery date23 October 1952
Designations
(2024) McLaughlin
Named after
Dean B. McLaughlin
(American astronomer)[2]
1952 UR · 1938 WP
1982 BX4
main-belt · Vesta[citation needed]
Orbital characteristics[1]
Epoch 4 September 2017 (JD 2458000.5)
Uncertainty parameter 0
Observation arc78.35 yr (28,619 days)
Aphelion2.6479AU
Perihelion2.0019 AU
2.3249 AU
Eccentricity0.1389
3.54yr (1,295 days)
126.79°
0° 16m 40.8s / day
Inclination7.3117°
69.231°
291.34°
Physical characteristics
Dimensions7.915±0.079[3]
0.173±0.020[3]
12.9[1]

2024 McLaughlin, provisional designation1952 UR, is anasteroid from the inner regions of theasteroid belt, approximately 8 kilometer in diameter. It was discovered 23 October 1952, by theIndiana Asteroid Program atGoethe Link Observatory near Brooklyn, Indiana, and named after American astronomerDean Benjamin McLaughlin.[2][4]

Orbit and classification

[edit]

McLaughlin orbits the Sun in theinner main-belt at a distance of 2.0–2.6 AU once every 3 years and 6 months (1,295 days). Its orbit has aneccentricity of 0.14 and aninclination of 7° with respect to theecliptic.[1]

The asteroid was first identified as1938 WP at the FinnishTurku Observatory in 1938, extending the body'sobservation arc by 14 years prior to its official discovery observation.[4]

Physical characteristics

[edit]

According to the survey carried out by NASA'sWide-field Infrared Survey Explorer with its subsequentNEOWISE mission, the asteroid measures 7.9 kilometers in diameter and its surface has analbedo of 0.173.[3]

As of 2017,McLaughlin's composition,rotation period and shape remain unknown.[1][5]

Naming

[edit]

Thisminor planet was named in memory of American astronomer and geologistDean Benjamin McLaughlin (1901–1965).[2]

McLaughlin was an astronomical spectroscopist at Swarthmore College and theUniversity of Michigan, and was the first to thoroughly measurestellar rotation, most notably the rotation ofAlgol. As a geologist he was one of the first to interpret the telescopically observable markings on Mars, which were later confirmed by direct observations from spacecraft(also seeAlbedo features). Thelunar andMartian craterMcLaughlin are also named in his honour.[2] The official naming citation was published by theMinor Planet Center on 6 June 1982 (M.P.C. 6955).[6]

References

[edit]
  1. ^abcde"JPL Small-Body Database Browser: 2024 McLaughlin (1952 UR)" (2017-03-27 last obs.).Jet Propulsion Laboratory. Retrieved10 June 2017.
  2. ^abcdSchmadel, Lutz D. (2007). "(2024) McLaughlin".Dictionary of Minor Planet Names – (2024) McLaughlin.Springer Berlin Heidelberg. p. 164.doi:10.1007/978-3-540-29925-7_2025.ISBN 978-3-540-00238-3.
  3. ^abcMasiero, Joseph R.; Grav, T.; Mainzer, A. K.; Nugent, C. R.; Bauer, J. M.; Stevenson, R.; et al. (August 2014)."Main-belt Asteroids with WISE/NEOWISE: Near-infrared Albedos".The Astrophysical Journal.791 (2): 11.arXiv:1406.6645.Bibcode:2014ApJ...791..121M.doi:10.1088/0004-637X/791/2/121. Retrieved8 December 2016.
  4. ^ab"2024 McLaughlin (1952 UR)".Minor Planet Center. Retrieved8 December 2016.
  5. ^"LCDB Data for (2024) McLaughlin". Asteroid Lightcurve Database (LCDB). Retrieved10 June 2017.
  6. ^"MPC/MPO/MPS Archive".Minor Planet Center. Retrieved8 December 2016.


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