The First Results of the Photometric Observation of Selected Asteroids on KT-50 Telescope of Mobitel Complex of RI «MAO»

Authors

  • A.V. Pomazan Research Institute «Mykolaiv Astronomical Observatory»
  • N.V. Maigurova Research Institute «Mykolaiv Astronomical Observatory»

DOI:

https://doi.org/10.15407/scine13.01.024

Keywords:

asteroids, light curves, phase-magnitude dependencies, photometric observations

Abstract

The first results of the photometric observations of asteroids performed on the telescope KT-50 of Mobitel complex (SRI MAO) during 2016 are presented in the paper. Asteroids were selected based on the infrared survey NEOWISE, moving objects catalog SDSS MOC-3 and MPC database. Selected asteroids have a relatively high albedo (pV>0.2) and are located in the Outer Main Belt (semi-major axis a>0.28 a.u.). The observations were made using filter close to the Rc standard band of Cousins system. Standard deviations of the instrumental differential magnitude measurements were in the range of 0.01m-0.03m for a 10m-15.5m reference stars. The light curve based on the results of the differential aperture photometry was obtained from long series of observations of the asteroid (2144) Marietta.

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Published

2024-08-27

How to Cite

Pomazan, A., & Maigurova, N. (2024). The First Results of the Photometric Observation of Selected Asteroids on KT-50 Telescope of Mobitel Complex of RI «MAO». Science and Innovation, 13(1), 24–29. https://doi.org/10.15407/scine13.01.024

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Section

Scientific Framework of Innovation Activity