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13154 Petermrva

From Wikipedia, the free encyclopedia

Stony Flora asteroid
13154 Petermrva
Discovery[1]
Discovered byA. Galád
A. Pravda
Discovery siteModra Obs.
Discovery date7 September 1995
Designations
(13154) Petermrva
Named after
Peter Mrva
(Slovakamateur astronomer)[2]
1995 RC · 1972 TL6
main-belt · Flora[3]
Orbital characteristics[1]
Epoch 4 September 2017 (JD 2458000.5)
Uncertainty parameter 0
Observation arc44.58 yr (16,282 days)
Aphelion2.5790AU
Perihelion1.8401 AU
2.2095 AU
Eccentricity0.1672
3.28yr (1,200 days)
230.03°
0° 18m 0.36s / day
Inclination5.5206°
331.59°
59.149°
Physical characteristics
Dimensions4.170±0.239 km[4][5]
4.176 km[6]
4.18 km(taken)[3]
2.9848±0.0002h[a]
2.98502±0.00004 h[7]
0.1464[6]
0.152±0.020[4][5]
S[3]
14.1[1] · 14.11±0.03(R)[a] · 14.46±0.32[8] · 14.56[4] · 14.6±0.058[6]

13154 Petermrva, provisional designation1995 RC, is a stony Floraasteroid from the inner regions of theasteroid belt, approximately 4.2 kilometers in diameter. It was discovered on 7 September 1995, by Slovak astronomersAdrián Galád and Alexander Pravda at theModra Observatory in the Bratislava Region of Slovakia.[9] The asteroid was named after Slovak amateur astronomerPeter Mrva.[2]

Orbit and classification

[edit]

Petermrva is a member of theFlora family, one of the largest families ofstony asteroids. It orbits the Sun in theinner main-belt at a distance of 1.8–2.6 AU once every 3 years and 3 months (1,200 days). Its orbit has aneccentricity of 0.17 and aninclination of 6° with respect to theecliptic.[1] The firstprecovery was taken atCrimea-Nauchnij in 1972, extending the asteroid'sobservation arc by 23 years prior to its discovery.[9]

Physical characteristics

[edit]

Two well-defined rotationallightcurves ofPetermrva were obtained from photometric observations at the Modra andOndřejov Observatory rendered arotation period of2.98502±0.00004 and2.9848±0.0002 hours, with a brightness amplitude of 0.18 and 0.14 inmagnitude, respectively (U=3/3).[7][a]

According to the thermal observation carried out by theNEOWISE mission of NASA'sWide-field Infrared Survey Explorer,Petermrva measures 4.2 kilometer and has an untypically lowalbedo of 0.15.[4]

Naming

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Thisminor planet is named after Slovak amateur astronomer Peter Mrva (born 1962) who participated in the construction the discovering Modra Observatory, after which the minor planet11118 Modra is named. He was also one of the first observers at the newly installed observatory. The second discoverer, Alexander Pravda, is thankful for his explanation and inspiration in some fields of astronomy and computer graphics.[2] The approved naming citation was published by theMinor Planet Center on 27 April 2002 (M.P.C. 45338).[10]

Notes

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  1. ^abcPravec (2008) web:lightcurve plot-A andlightcurve plot-B of (13154) Petermrva rotation period2.9848±0.0002 hours with a brightness amplitude of0.14 mag. The Collaborative Asteroid Lightcurve Link rates the observations with a quality code of 3 (U=3), which denotes a secure result within the precision given and no ambiguity. Summary figures atCollaborative Asteroid Lightcurve Link (CALL) andOndrejov Asteroid Photometry Project, Pravec, P.; Wolf, M.; Sarounova, L.

References

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  1. ^abcd"JPL Small-Body Database Browser: 13154 Petermrva (1995 RC)" (2017-05-05 last obs.).Jet Propulsion Laboratory. Archived fromthe original on 4 November 2020. Retrieved5 July 2017.
  2. ^abcSchmadel, Lutz D. (2007). "(13154) Petermrva".Dictionary of Minor Planet Names – (13154) Petermrva.Springer Berlin Heidelberg. p. 793.doi:10.1007/978-3-540-29925-7_8748.ISBN 978-3-540-00238-3.
  3. ^abc"LCDB Data for (13154) Petermrva". Asteroid Lightcurve Database (LCDB). Retrieved17 May 2016.
  4. ^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.S2CID 118700974. 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.S2CID 118745497. Retrieved3 December 2016.
  6. ^abcPravec, 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. Retrieved17 May 2016.
  7. ^abGalád, A. (April 2007)."Lightcurves and Synodic Periods for Asteroids 1998 ST49, (13154) and (27529)".Earth.100 (1–2):77–82.Bibcode:2007EM&P..100...77G.doi:10.1007/s11038-006-9099-1.S2CID 121454395. Retrieved17 May 2016.
  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. Retrieved17 May 2016.
  9. ^ab"13154 Petermrva (1995 RC)".Minor Planet Center. Retrieved24 January 2016.
  10. ^"MPC/MPO/MPS Archive".Minor Planet Center. Retrieved17 May 2016.

External links

[edit]
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