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19848 Yeungchuchiu

From Wikipedia, the free encyclopedia
Main-belt asteroid

19848 Yeungchuchiu
Yeungchuchiu modeled from itslightcurve
Discovery[1]
Discovered byW. K. Yeung
Discovery siteDesert Beaver Obs.
Discovery date2 October 2000
Designations
(19848) Yeungchuchiu
Named after
Chu Chiu Yeung
(discoverer's father)[2]
2000 TR · 1998 KR38
1999 SY6
main-belt · Eos[3]
Orbital characteristics[1]
Epoch 4 September 2017 (JD 2458000.5)
Uncertainty parameter 0
Observation arc34.82 yr (12,718 days)
Aphelion3.2372AU
Perihelion2.7768 AU
3.0070 AU
Eccentricity0.0766
5.21yr (1,905 days)
94.290°
0° 11m 20.4s / day
Inclination11.061°
54.759°
350.16°
Physical characteristics
11.69±0.55 km[4]
12.700±0.134[5]
12.90 km(calculated)[3]
13.242±0.282 km[6]
3.450±0.002 h[7]
3.4508±0.0003 h[8]
0.14(assumed)[3]
0.170±0.020[4][5]
0.2107±0.0250[6]
S[3]
12.2[1][3][4] · 11.7[6] · 12.227±0.002(R)[8] · 12.49±0.28[9]

19848 Yeungchuchiu (provisional designation2000 TR) is a stonyEos asteroid from the outer region of theasteroid belt, approximately 12 kilometers (7.5 miles) in diameter. It was discovered on 2 October 2000 by Canadian amateur astronomerWilliam Yeung at theDesert Beaver Observatory in Arizona, United States. It is the largest object found by the discoverer, just 1°.2 west of Jupiter, who named it after his father, Chu Chiu Yeung.[2][10]

Orbit and classification

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Yeungchuchiu is a member of theEos family, an orbital group of more than 4,000 asteroids, which are known for mostly being of stony composition. It orbits the Sun in theouter main-belt at a distance of 2.8–3.2 AU once every 5 years and 3 months (1,905 days). Its orbit has aneccentricity of 0.08 and aninclination of 11° with respect to theecliptic.[1] The firstprecovery was taken at the AustralianSiding Spring Observatory in 1982, extending the asteroid'sobservation arc by 18 years prior to its discovery.[10]

Naming

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Thisminor planet was named by the discoverer after his father, Chu Chiu Yeung (born 1925), in gratitude for his unconditional support.[2] The approved naming citation was published by theMinor Planet Center on 9 March 2001 (M.P.C. 42368).[11]

Physical characteristics

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Rotation period

[edit]
Lightcurve based 3D-model of Yeungchuchiu

In November 2005, a rotationallightcurve of Yeungchuchiu was obtained fromphotometric observations by the discoverer at theDesert Eagle Observatory in Arizona. Lightcurve analysis gave a well-definedrotation period of3.450 hours with a brightness variation of 0.70magnitude (U=3).[7] The large amplitude suggests that the body is of non-spherical shape and that the long axis is almost twice as long as the short axis. It is likely that the rotational axis was almost perpendicular to the observation's line-of-sight.[7] A second lightcurve was obtained at thePalomar Transient Factory in September 2010, and gave a concurring period of3.4508±0.0003 hours with an amplitude of 0.63 in magnitude (U=2).[8]

Diameter and albedo

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According to the survey carried out by NASA'sWide-field Infrared Survey Explorer and its subsequentNEOWISE mission, the asteroid measures 11.7 and 13.2 kilometers in diameter with analbedo for its surface of 0.17 and 0.21, respectively.[6][4] TheCollaborative Asteroid Lightcurve Link assumes an albedo forstony asteroids of 0.21 and calculates a diameter of 12.9 kilometers with anabsolute magnitude of 12.2.[3]

References

[edit]
  1. ^abcd"JPL Small-Body Database Browser: 19848 Yeungchuchiu (2000 TR)" (2017-05-04 last obs.).Jet Propulsion Laboratory. Retrieved27 June 2017.
  2. ^abcSchmadel, Lutz D. (2007). "(19848) Yeungchuchiu".Dictionary of Minor Planet Names.Springer Berlin Heidelberg. p. 859.doi:10.1007/978-3-540-29925-7_9589.ISBN 978-3-540-00238-3.
  3. ^abcdef"LCDB Data for (19848) Yeungchuchiu". Asteroid Lightcurve Database (LCDB). Retrieved17 May 2016.
  4. ^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. Retrieved17 May 2016.
  5. ^abMasiero, Joseph R.; Mainzer, A. K.; Grav, T.; Bauer, J. M.; Cutri, R. M.; Dailey, J.; et al. (November 2011)."Main Belt Asteroids with WISE/NEOWISE. I. Preliminary Albedos and Diameters".The Astrophysical Journal.741 (2): 20.arXiv:1109.4096.Bibcode:2011ApJ...741...68M.doi:10.1088/0004-637X/741/2/68. Retrieved3 December 2016.
  6. ^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. Retrieved17 May 2016.
  7. ^abcYeung, Kwong W. (September 2006)."Lightcurve analysis for 19848 Yeungchuchiu".The Minor Planet Bulletin.33 (3): 49.Bibcode:2006MPBu...33...49Y.ISSN 1052-8091. Retrieved17 May 2016.
  8. ^abcWaszczak, Adam; Chang, Chan-Kao; Ofek, Eran O.; Laher, Russ; Masci, Frank; Levitan, David; et al. (September 2015)."Asteroid Light Curves from the Palomar Transient Factory Survey: Rotation Periods and Phase Functions from Sparse Photometry".The Astronomical Journal.150 (3): 35.arXiv:1504.04041.Bibcode:2015AJ....150...75W.doi:10.1088/0004-6256/150/3/75. Retrieved17 May 2016.
  9. ^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. Retrieved17 May 2016.
  10. ^ab"19848 Yeungchuchiu (2000 TR)".Minor Planet Center. Retrieved1 January 2016.
  11. ^"MPC/MPO/MPS Archive".Minor Planet Center. Retrieved17 May 2016.

External links

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