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1822 Waterman

From Wikipedia, the free encyclopedia
Main-belt asteroid

1822 Waterman
Discovery[1]
Discovered byIndiana University
(Indiana Asteroid Program)
Discovery siteGoethe Link Obs.
Discovery date25 July 1950
Designations
(1822) Waterman
Named after
Alan T. Waterman
(American physicist)[2]
1950 OO · 1943 EB
1953 MA · 1963 TT
main-belt · (inner)[3]
Orbital characteristics[1]
Epoch 4 September 2017 (JD 2458000.5)
Uncertainty parameter 0
Observation arc66.64 yr (24,342 days)
Aphelion2.5023AU
Perihelion1.8378 AU
2.1700 AU
Eccentricity0.1531
3.20yr (1,168 days)
45.052°
Inclination0.9567°
221.25°
30.351°
Physical characteristics
Dimensions6.054±0.098[4]
6.515±0.060 km[5]
7.46 km(calculated)[3]
7.581±0.002h[6]
0.20(assumed)[3]
0.2639±0.0659[5]
0.325±0.046[4]
S[3]
13.0[5] · 13.1[1][3] · 14.04±0.51[7]

1822 Waterman, provisional designation1950 OO, is a stonyasteroid from the inner regions of theasteroid belt, approximately 6.5 kilometers in diameter.

It was discovered on 25 July 1950, by Indiana University'sIndiana Asteroid Program at itsGoethe Link Observatory near Brooklyn, Indiana, United States.[8] The asteroid was named after American physicistAlan T. Waterman.[2]

Orbit and classification

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Waterman is aS-type asteroid. It orbits the Sun in theinner main-belt at a distance of 1.8–2.5 AU once every 3 years and 2 months (1,168 days). Its orbit has aneccentricity of 0.15 and aninclination of 1° with respect to theecliptic.[1] The body'sobservation arc begins with its official discovery observation, as its first identification,1943 EB, made at the GermanSonneberg Observatory in 1943, remained unused.[8]

Physical characteristics

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Rotation period

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In January 2013, a rotationallightcurve ofWaterman was obtained from photometric observation taken at the U.S Etscorn Observatory in New Mexico. It gave a well-definedrotation period of 7.581 hours with a brightness variation of 0.51magnitude (U=3).[6]

Diameter and albedo

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According to the survey carried out by NASA'sWide-field Infrared Survey Explorer with its subsequentNEOWISE mission,Waterman measures between 6.06 and 6.52 kilometers in diameter, and its surface has analbedo between 0.264 and 0.325.[4][5] TheCollaborative Asteroid Lightcurve Link assumes a standard albedo for stony asteroids of 0.20 and calculates a diameter of 7.46 kilometers with anabsolute magnitude of 13.1.[3]

Naming

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Thisminor planet was named in honor of American physicistAlan Tower Waterman (1892–1967), who was the first director of the U.S.National Science Foundation. He went to Washington to serve with OSRD (1941–45), ONR (1946–51), and NSF (1951–63), after being an academic physicist for 25 years.[2]

Waterman was awarded the Karl Taylor Compton Gold Medal for distinguished statesmanship in science, thePublic Welfare Medal and thePresidential Medal of Freedom.[2][9] The officialnaming citation was published by theMinor Planet Center on 1 June 1975 (M.P.C. 3825).[10]

References

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  1. ^abcd"JPL Small-Body Database Browser: 1822 Waterman (1950 OO)" (2017-03-17 last obs.).Jet Propulsion Laboratory. Archived fromthe original on 20 December 2016. Retrieved8 June 2017.
  2. ^abcdSchmadel, Lutz D. (2007). "(1822) Waterman".Dictionary of Minor Planet Names – (1822) Waterman.Springer Berlin Heidelberg. p. 146.doi:10.1007/978-3-540-29925-7_1823.ISBN 978-3-540-00238-3.
  3. ^abcdef"LCDB Data for (1822) Waterman". Asteroid Lightcurve Database (LCDB). Retrieved15 December 2016.
  4. ^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. Retrieved15 December 2016.
  5. ^abcdMainzer, A.; Grav, T.; Masiero, J.; Hand, E.; Bauer, J.; Tholen, D.; et al. (November 2011). "NEOWISE Studies of Spectrophotometrically Classified Asteroids: Preliminary Results".The Astrophysical Journal.741 (2): 25.arXiv:1109.6407.Bibcode:2011ApJ...741...90M.doi:10.1088/0004-637X/741/2/90.
  6. ^abKlinglesmith, Daniel A. III; Hanowell, Jesse; Risley, Ethan; Janek, Turk; Vargas, Angelica; Warren, Curtis Alan (July 2013)."Etscorn Observed Asteroids: Results for Size Asteroids December 2012 - March 2013".The Minor Planet Bulletin.40 (3):154–156.Bibcode:2013MPBu...40..154K.ISSN 1052-8091. Retrieved15 December 2016.
  7. ^Veres, Peter; Jedicke, Robert; Fitzsimmons, Alan; Denneau, Larry; Granvik, Mikael; Bolin, Bryce; et al. (November 2015)."Absolute magnitudes and slope parameters for 250,000 asteroids observed by Pan-STARRS PS1 - Preliminary results".Icarus.261:34–47.arXiv:1506.00762.Bibcode:2015Icar..261...34V.doi:10.1016/j.icarus.2015.08.007. Retrieved15 December 2016.
  8. ^ab"1822 Waterman (1950 OO)".Minor Planet Center. Retrieved15 December 2016.
  9. ^"Public Welfare Medal".National Academy of Sciences. Retrieved22 August 2016.
  10. ^Schmadel, Lutz D. "Appendix – Publication Dates of the MPCs".Dictionary of Minor Planet Names – Addendum to Fifth Edition (2006–2008). Springer Berlin Heidelberg. p. 221.doi:10.1007/978-3-642-01965-4.ISBN 978-3-642-01964-7.

External links

[edit]
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Asteroid
Distant minor planet
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Authority control databasesEdit this at Wikidata
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