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ASTEROID LIGHTCURVE ANALYSIS AT CS3-PALMER DIVIDE STATION: 2014 DECEMBER - 2015 MARCH.

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POTENTIAL BINARY AND TUMBLING ASTEROIDS FROM THE CENTER FOR SOLAR SYSTEM STUDIES.

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  • 1Center for Solar System Studies / MoreData!, 446 Sycamore Ave., Eaton, CO 80615 USA.

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Astronomers confirmed two binary asteroids and identified a rare wide binary asteroid candidate. Further analysis is needed for another asteroid suspected to be binary or tumbling.

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Area of Science:

  • Asteroid science
  • Photometric observations
  • Binary asteroid systems

Background:

  • Asteroids are remnants from the early solar system.
  • Understanding asteroid composition and dynamics is crucial for planetary science.
  • Binary asteroids offer unique insights into small body formation and evolution.

Purpose of the Study:

  • To conduct CCD photometric observations of selected asteroids.
  • To identify and characterize binary asteroid systems.
  • To investigate the rotational periods and potential multiplicity of asteroids.

Main Methods:

  • Utilized CCD photometric observations in 2019.
  • Analyzed light curves to determine rotational periods.
  • Re-evaluated archival data for period analysis.

Main Results:

  • Confirmed 2602 Moore (Vestoid) and 27568 (2000 PT6) (Hungaria) as binary asteroids.
  • Identified 3880 Kaiserman (Hungaria) as a suspected binary.
  • Near-Earth asteroid 142040 (2002 QE15) exhibits a long period (46.4 h) and is a candidate for a very wide binary system.
  • Asteroid 2937 Gibbs (Phocaea) showed ambiguous periods, leaving its binary or tumbling state undetermined.

Conclusions:

  • The study contributes to the census of binary asteroids.
  • The discovery of a potential very wide binary system is significant.
  • Further observations are required for ambiguous cases like 2937 Gibbs.