Movatterモバイル変換


[0]ホーム

URL:


Jump to content
WikipediaThe Free Encyclopedia
Search

3102 Krok

From Wikipedia, the free encyclopedia
Rare-type asteroid and slow rotator

3102 Krok
Discovery[1]
Discovered byL. Brožek
Discovery siteKleť Obs.
Discovery date21 August 1981
Designations
(3102) Krok
Named after
Duke Krok
(legendary Czech figure)[2]
1981 QA
NEO · Amor[1][3]
Orbital characteristics[1]
Epoch 16 February 2017 (JD 2457800.5)
Uncertainty parameter 0
Observation arc35.44 yr (12,944 days)
Aphelion3.1174AU
Perihelion1.1839 AU
2.1506 AU
Eccentricity0.4495
3.15yr (1,152 days)
86.843°
0° 18m 45s / day
Inclination8.4439°
172.09°
154.78°
Earth MOID0.1840 AU · 71.7LD
Physical characteristics
Dimensions1.48 km(derived)[4]
1.6 km[1]
147.8±0.3h[5]
149.4±1 h[6]
151.8[6]
0.20(assumed)[4]
QRS(Tholen)[1]
S(SMASS)[1]
Sqw[7] · QRS[4]
B–V = 0.834[1]
U–B = 0.521[1]
16.14±0.2(R)[6] · 16.2[1] · 16.40±0.15[5] · 16.47±0.35[8] · 16.524±0.15[4][9]

3102 Krok, provisional designation1981 QA, is a rare-typeasteroid andslow rotator, classified as anear-Earth object of theAmor group, that measures approximately 1.5 kilometers in diameter.

It was discovered on 21 August 1981, by Slovak astronomerLadislav Brožek atKleť Observatory in the Czech Republic.[3] The asteroid was named afterDuke Krok, a legendary Czech figure.[2]

Classification and orbit

[edit]

Krok orbits the Sun at a distance of 1.2–3.1 AU once every 3 years and 2 months (1,152 days). Its orbit has aneccentricity of 0.45 and aninclination of 8° with respect to theecliptic.[1] The body'sobservation arc begins with its official discovery observation at Klet, as noprecoveries were taken and no prior identifications were made.[3]

It has an Earthminimum orbital intersection distance of 0.1840 AU (27,500,000 km), which translates into 71.7lunar distances.[1]

Physical characteristics

[edit]

In theTholen classification,Krok is characterized as a rare QRS-type. In theSMASS taxonomy it is classified as a commonS-type asteroid, and the "ExploreNEOs" Warm Spitzer program assigns a transitional Sqw-type.[1][7] TheR- andQ-types also belong to the larger group of stony asteroids.

Rotation and shape

[edit]

In September 1991, a first rotationallightcurve ofKrok was obtained by American astronomer Alan Harris. Lightcurve analysis gave an exceptionally longrotation period of 147.8 hours with a brightness amplitude of 1.0magnitude, which indicates that the body has a non-spheroidal shape (U=3).[5]

Between 2000 and 2005, severalphotometric observations made by Czech astronomerPetr Pravec gave a similar period between 149.4 and 151.8 and an amplitude of 0.7 to 1.3 (U=3/3-).[6] This makesKrok asslow rotator.

Diameter and albedo

[edit]

According toTom Gehrels' 1994 publication "Hazards due to Comets and Asteroids",Krok measures 1.6 kilometers in diameter based on a generic surfacealbedo of 0.15,[1] while theCollaborative Asteroid Lightcurve Link assumes a standard albedo for stonyS-type asteroids of 0.20 and calculates a diameter of 1.48 kilometers with anabsolute magnitude of 16.5.[4]

Naming

[edit]

Thisminor planet was named afterDuke Krok, a legendary figure in Czech history, and the first judge ("duke") of the Slavonic tribes in ancient Bohemia. He was also the father ofPrincess Libuše, who, together with her husband Přemysl founded thePřemyslid dynasty of Czech royalty.[2] The official naming citation was published on 18 December 1994 (M.P.C.24410).[10]

References

[edit]
  1. ^abcdefghijklm"JPL Small-Body Database Browser: 3102 Krok (1981 QA)" (2017-01-28 last obs.).Jet Propulsion Laboratory. Retrieved25 April 2017.
  2. ^abcSchmadel, Lutz D. (2007). "(3102) Krok".Dictionary of Minor Planet Names – (3102) Krok.Springer Berlin Heidelberg. p. 256.doi:10.1007/978-3-540-29925-7_3103.ISBN 978-3-540-00238-3.
  3. ^abc"3102 Krok (1981 QA)".Minor Planet Center. Retrieved25 April 2017.
  4. ^abcde"LCDB Data for (3102) Krok". Asteroid Lightcurve Database (LCDB). Retrieved25 April 2017.
  5. ^abcHarris, A. W.; Young, J. W.; Dockweiler, Thor; Gibson, J.; Poutanen, M.; Bowell, E. (January 1992)."Asteroid lightcurve observations from 1981".Icarus.95 (1): 115–147.ResearchsupportedbyLowellObservatoryEndowmentandNASA.Bibcode:1992Icar...95..115H.doi:10.1016/0019-1035(92)90195-D.ISSN 0019-1035. Retrieved25 April 2017.
  6. ^abcdPravec, P.; Harris, A. W.; Scheirich, P.; Kusnirák, P.; Sarounová, L.; Hergenrother, C. W.; et al. (January 2005)."Tumbling asteroids".Icarus.173 (1):108–131.Bibcode:2005Icar..173..108P.doi:10.1016/j.icarus.2004.07.021. Retrieved25 April 2017.
  7. ^abThomas, Cristina A.; Emery, Joshua P.; Trilling, David E.; Delbó, Marco; Hora, Joseph L.; Mueller, Michael (January 2014)."Physical characterization of Warm Spitzer-observed near-Earth objects".Icarus.228:217–246.arXiv:1310.2000.Bibcode:2014Icar..228..217T.doi:10.1016/j.icarus.2013.10.004.hdl:2060/20140012047.S2CID 119278697. Retrieved25 April 2017.
  8. ^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.S2CID 53493339. Retrieved25 April 2017.
  9. ^Pravec, Petr; Harris, Alan W.; Kusnirák, Peter; Galád, Adrián; Hornoch, Kamil (September 2012)."Absolute magnitudes of asteroids and a revision of asteroid albedo estimates from WISE thermal observations".Icarus.221 (1):365–387.Bibcode:2012Icar..221..365P.doi:10.1016/j.icarus.2012.07.026. Retrieved25 April 2017.
  10. ^"MPC/MPO/MPS Archive".Minor Planet Center. Retrieved25 April 2017.

External links

[edit]
Minor planets
Asteroid
Distant minor planet
Comets
Other
Authority control databasesEdit this at Wikidata
Retrieved from "https://en.wikipedia.org/w/index.php?title=3102_Krok&oldid=1293149072"
Categories:
Hidden categories:

[8]ページ先頭

©2009-2025 Movatter.jp