Distribution of shape elongations of main belt asteroids derived from Pan-STARRS1 photometry

H. Cibulková, H. Nortunen, J. Urech, M. Kaasalainen, P. Vereš, R. Jedicke, R. J. Wainscoat, M. Mommert, David E Trilling, E. Schunová-Lilly, E. A. Magnier, C. Waters, H. Flewelling

Research output: Contribution to journalArticle

4 Citations (Scopus)

Abstract

Context. A considerable amount of photometric data is produced by surveys such as Pan-STARRS, LONEOS, WISE, or Catalina. These data are a rich source of information about the physical properties of asteroids. There are several possible approaches for using these data. Light curve inversion is a typical method that works with individual asteroids. Our approach in focusing on large groups of asteroids, such as dynamical families and taxonomic classes, is statistical; the data are not sufficient for individual models.Aim. Our aim is to study the distributions of shape elongation ba and the spin axis latitude β for various subpopulations of asteroids and to compare our results, based on Pan-STARRS1 survey, with statistics previously carried out using various photometric databases, such as Lowell and WISE.Methods. We used the LEADER algorithm to compare the ba and β distributions for various subpopulations of asteroids. The algorithm creates a cumulative distributive function (CDF) of observed brightness variations, and computes the ba and β distributions with analytical basis functions that yield the observed CDF. A variant of LEADER is used to solve the joint distributions for synthetic populations to test the validity of the method.Results. When comparing distributions of shape elongation for groups of asteroids with different diameters D, we found that there are no differences for D < 25 km. We also constructed distributions for asteroids with different rotation periods and revealed that the fastest rotators with P = 0 - 4 h are more spheroidal than the population with P = 4-8 h.

Original languageEnglish (US)
Article numberA86
JournalAstronomy and Astrophysics
Volume611
DOIs
StatePublished - Mar 1 2018

Fingerprint

asteroid belts
asteroids
asteroid
elongation
photometry
Wide-field Infrared Survey Explorer
subpopulation
distribution
light curve
brightness
physical property
physical properties
statistics
inversions

Keywords

  • asteroids
  • general
  • Methods
  • Minor planets
  • photometric
  • statistical
  • Techniques

ASJC Scopus subject areas

  • Astronomy and Astrophysics
  • Space and Planetary Science

Cite this

Cibulková, H., Nortunen, H., Urech, J., Kaasalainen, M., Vereš, P., Jedicke, R., ... Flewelling, H. (2018). Distribution of shape elongations of main belt asteroids derived from Pan-STARRS1 photometry. Astronomy and Astrophysics, 611, [A86]. https://doi.org/10.1051/0004-6361/201731554

Distribution of shape elongations of main belt asteroids derived from Pan-STARRS1 photometry. / Cibulková, H.; Nortunen, H.; Urech, J.; Kaasalainen, M.; Vereš, P.; Jedicke, R.; Wainscoat, R. J.; Mommert, M.; Trilling, David E; Schunová-Lilly, E.; Magnier, E. A.; Waters, C.; Flewelling, H.

In: Astronomy and Astrophysics, Vol. 611, A86, 01.03.2018.

Research output: Contribution to journalArticle

Cibulková, H, Nortunen, H, Urech, J, Kaasalainen, M, Vereš, P, Jedicke, R, Wainscoat, RJ, Mommert, M, Trilling, DE, Schunová-Lilly, E, Magnier, EA, Waters, C & Flewelling, H 2018, 'Distribution of shape elongations of main belt asteroids derived from Pan-STARRS1 photometry', Astronomy and Astrophysics, vol. 611, A86. https://doi.org/10.1051/0004-6361/201731554
Cibulková, H. ; Nortunen, H. ; Urech, J. ; Kaasalainen, M. ; Vereš, P. ; Jedicke, R. ; Wainscoat, R. J. ; Mommert, M. ; Trilling, David E ; Schunová-Lilly, E. ; Magnier, E. A. ; Waters, C. ; Flewelling, H. / Distribution of shape elongations of main belt asteroids derived from Pan-STARRS1 photometry. In: Astronomy and Astrophysics. 2018 ; Vol. 611.
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AU - Vereš, P.

AU - Jedicke, R.

AU - Wainscoat, R. J.

AU - Mommert, M.

AU - Trilling, David E

AU - Schunová-Lilly, E.

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