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1230 Riceia

From Wikipedia, the free encyclopedia
Main-belt asteroid

1230 Riceia
Shape model ofRiceia from itslightcurve
Discovery[1]
Discovered byK. Reinmuth
Discovery siteHeidelberg Obs.
Discovery date9 October 1931
Designations
(1230) Riceia
Pronunciation/ˈrsiə/
Named after
Hugh Rice[2]
(U.S. amateur astronomer)
1931 TX1 · 1964 TS
1964 UE · 1975 HH
main-belt · (inner)[3]
background[4]
Orbital characteristics[1]
Epoch 4 September 2017 (JD 2458000.5)
Uncertainty parameter 0
Observation arc86.13 yr (31,459 days)
Aphelion3.0335AU
Perihelion2.1104 AU
2.5719 AU
Eccentricity0.1795
4.12yr (1,507 days)
288.81°
0° 14m 20.4s / day
Inclination10.515°
200.55°
185.25°
Physical characteristics
Dimensions6.194±0.344 km[5]
7.46 km(calculated)[3]
6.67317±0.00001h[6]
0.20(assumed)[3]
0.318±0.037[5]
S[3][7]
12.90[5] · 13.0[1][3] · 13.11±0.22[7]

1230 Riceia, provisional designation1931 TX1, is a stony backgroundasteroid from the central regions of theasteroid belt, approximately 6 kilometers in diameter. It was discovered on 9 October 1931, by German astronomerKarl Reinmuth at theHeidelberg-Königstuhl State Observatory.[8] The asteroid was named afterHugh Rice, amateur astronomer of New York and director of the Museum of Natural Sciences.[2]

Orbit and classification

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Riceia is a non-family asteroid from the main belt'sbackground population.[4] It orbits the Sun in thecentral asteroid belt at a distance of 2.1–3.0 AU once every 4 years and 1 month (1,507 days;semi-major axis of 2.57 AU). Its orbit has aneccentricity of 0.18 and aninclination of 11° with respect to theecliptic.[1]

The body'sobservation arc begins at Heidelberg on 17 October 1931, or eight days after its official discovery observation.[8]

Physical characteristics

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Riceia has been characterized as a stonyS-type asteroid byPan-STARRS photometric survey.[7]

Rotation period and pole

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In 2016, a rotationallightcurve ofRiceia was modeled from photometric data from the Lowell Photometric Database. Lightcurve analysis gave a siderealrotation period of 6.67317 hours as well as aspin axis of (37.0°, −63.0°) inecliptic coordinates (λ, β).[6]

Diameter and albedo

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According to the survey carried out by theNEOWISE mission of NASA'sWide-field Infrared Survey Explorer,Riceia measures 6.19 kilometers in diameter and its surface has a highalbedo of 0.318.[5] TheCollaborative Asteroid Lightcurve Link assumes a standard albedo for stony asteroids of 0.20 and calculates a diameter of 7.46 kilometers based on anabsolute magnitude of 13.0.[3]

Naming

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Thisminor planet was named after American amateur astronomer Hugh Rice, director of the Museum of Natural Sciences (possiblyAMNH).[2] The naming was proposed by Irving Meyer and endorsed by German astronomerGustav Stracke who mentioned on a postcard in February 1937, that his American college, Meyer, who himself did not discover any asteroids, requested the naming after the city of Rutherford, where a private observatory was located at the time.[9]

The official naming citation was mentioned inThe Names of the Minor Planets byPaul Herget in 1955 (H 113).[2]

References

[edit]
  1. ^abcd"JPL Small-Body Database Browser: 1230 Riceia (1931 TX1)" (2017-11-25 last obs.).Jet Propulsion Laboratory. Archived fromthe original on 18 September 2020. Retrieved10 January 2018.
  2. ^abcdSchmadel, Lutz D. (2007). "(1230) Riceia".Dictionary of Minor Planet Names – (1230) Riceia.Springer Berlin Heidelberg. p. 102.doi:10.1007/978-3-540-29925-7_1231.ISBN 978-3-540-00238-3.
  3. ^abcdef"LCDB Data for (1230) Riceia". Asteroid Lightcurve Database (LCDB). Retrieved10 January 2018.
  4. ^ab"Asteroid 1230 Riceia – Proper Elements". AstDyS-2, Asteroids – Dynamic Site. Retrieved29 October 2019.
  5. ^abcdMasiero, Joseph R.; Mainzer, A. K.; Grav, T.; Bauer, J. M.; Cutri, R. M.; Nugent, C.; et al. (November 2012)."Preliminary Analysis of WISE/NEOWISE 3-Band Cryogenic and Post-cryogenic Observations of Main Belt Asteroids".The Astrophysical Journal Letters.759 (1): 5.arXiv:1209.5794.Bibcode:2012ApJ...759L...8M.doi:10.1088/2041-8205/759/1/L8. Retrieved10 January 2018.
  6. ^abDurech, J.; Hanus, J.; Oszkiewicz, D.; Vanco, R. (March 2016)."Asteroid models from the Lowell photometric database".Astronomy and Astrophysics.587: 6.arXiv:1601.02909.Bibcode:2016A&A...587A..48D.doi:10.1051/0004-6361/201527573. Retrieved10 January 2018.
  7. ^abcVeres, 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. Retrieved10 January 2018.
  8. ^ab"1230 Riceia (1931 TX1)".Minor Planet Center. Retrieved10 January 2018.
  9. ^Schmadel, Lutz D. (2007). "(1249) Rutherfordia".Dictionary of Minor Planet Names – (1249) Rutherfordia. Springer Berlin Heidelberg. p. 104.doi:10.1007/978-3-540-29925-7_1250.ISBN 978-3-540-00238-3.

External links

[edit]
Minor planets
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