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2010 KZ39

From Wikipedia, the free encyclopedia
Trans-Neptunian object

2010 KZ39
Discovery[1][2][3]
Discovered by
Discovery siteLas Campañas Obs.
(first observed)
Discovery date21 May 2010
(first observed)
Designations
2010 KZ39
Orbital characteristics[4][5]
Epoch 2024 October 17 (JD 2460600.5)
Uncertainty parameter 4
Observation arc11.94 yr (4,361 days)
Aphelion47.55 AU
Perihelion42.48 AU
45.01 AU
Eccentricity0.0563
302.0 yr (110,300 days)
256.5°
0° 0m 11.736s / day
Inclination26.156°
53.277°
≈ 6 May 2110[6]
±5 months
322.6°
Knownsatellites0
Physical characteristics
743 km?[11] 660 km (estimated albedo)[12]
0.10(assumed)[7]
20.7[13]

2010 KZ39 is atrans-Neptunian object orbiting the Sun as adetached object in the outer reaches of theSolar System. The object was first observed on 21 May 2010 by astronomersAndrzej Udalski,Scott Sheppard, M. Szymanski andChad Trujillo at theLas Campañas Observatory in Chile.[1][3]

Description

[edit]
Follow-up images of2010 KZ39 taken atLas Campañas Obs.

2010 KZ39 orbits the Sun at a distance of 42.5–47.6 AU once every 302 years, similar toMakemake,19521 Chaos and other bodies that circle the Sun in 6:11resonance toNeptune. Its orbit has aneccentricity of 0.056 and aninclination of 26° with respect to theecliptic.

Using the best-fit values for its orbit, it is expected to come toperihelion in 2109.[4] It has been observed 50 times over 12 years and has anuncertainty parameter of 4.[1] As of 2016, it is 46.1 AU from the Sun.[13] The body's spectral type as well as its rotation period remain unknown.

References

[edit]
  1. ^abc"(2010 KZ39)".Minor Planet Center. Retrieved21 September 2016.
  2. ^"MPEC 2010-L38 : 2010 KZ39".IAU Minor Planet Center. 8 June 2010. Retrieved3 December 2010.
  3. ^abAll four named discoverers are uncredited in sources.
  4. ^abcd"JPL Small-Body Database Browser: (2010 KZ39)" (2012-03-20 last obs.).Jet Propulsion Laboratory. Retrieved3 April 2017.
  5. ^abMarc W. Buie."Orbit Fit and Astrometric record for 10KZ39" (last observation: 2012-03-20 using 28 of 28 observations over 1.83 years). SwRI (Space Science Department). Retrieved18 August 2011.
  6. ^JPL Horizons Observer Location: @sun (Perihelion occurs when deldot changes from negative to positive. Uncertainty in time of perihelion is3-sigma.)
  7. ^ab"LCDB Data for 2010 KZ39". Asteroid Lightcurve Database (LCDB). Retrieved3 April 2017.
  8. ^Dan Bruton."Conversion of Absolute Magnitude to Diameter for Minor Planets". Department of Physics & Astronomy (Stephen F. Austin State University). Archived fromthe original on 23 July 2011. Retrieved18 August 2011.
  9. ^Benecchi, Susan D.; Sheppard, Scott S. (May 2013)."Light Curves of 32 Large Transneptunian Objects".The Astronomical Journal.145 (5): 19.arXiv:1301.5791.Bibcode:2013AJ....145..124B.doi:10.1088/0004-6256/145/5/124.S2CID 54183985. Retrieved3 April 2017.
  10. ^Michael E. Brown."How many dwarf planets are there in the outer solar system? (updates daily)".California Institute of Technology. Retrieved14 August 2019.
  11. ^"List of known trans-Neptunian objects".www.johnstonsarchive.net. Archived fromthe original on 14 August 2025. Retrieved24 November 2025.
  12. ^"Asteroid Size Estimator".cneos.jpl.nasa.gov. Archived fromthe original on 30 August 2025. Retrieved24 November 2025.
  13. ^ab"AstDyS: 2010 KZ39 Ephemerides". AstDyS. Retrieved7 April 2014.

External links

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or H ≤ 4.0)
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