Hostname: page-component-78c5997874-m6dg7 Total loading time: 0 Render date: 2024-11-19T22:07:28.863Z Has data issue: false hasContentIssue false
  • English
  • Français

The latest spectral analysis on asteroids at NAO Rozhen

Published online by Cambridge University Press:  12 October 2020

Elena Vchkova Bebekovska Open the ORCID record for Elena Vchkova Bebekovska [Opens in a new window] ,
Galin Borisov ,
Zahary Donchev  and
Gordana Apostolovska Open the ORCID record for Gordana Apostolovska [Opens in a new window]
Elena Vchkova Bebekovska
Affiliation:
Institute of Physics, Faculty of Science, Ss. Cyril and Methodius University, Skopje, Republic of Macedonia, Arhimedova 3, 1000 Skopje, Republic of Macedonia email: [email protected]
Galin Borisov
Affiliation:
Armagh Observatory and Planetarium, College Hill, BT61 9DG Armagh, UK Institute of Astronomy with National Astronomical Observatory, Bulgarian Academy of Sciences, 72, Tsarigradsko Chaussée Blvd., BG-1784 Sofia, Bulgaria
Zahary Donchev
Affiliation:
Institute of Astronomy with National Astronomical Observatory, Bulgarian Academy of Sciences, 72, Tsarigradsko Chaussée Blvd., BG-1784 Sofia, Bulgaria
Gordana Apostolovska
Affiliation:
Institute of Physics, Faculty of Science, Ss. Cyril and Methodius University, Skopje, Republic of Macedonia, Arhimedova 3, 1000 Skopje, Republic of Macedonia email: [email protected]
Rights & Permissions [Opens in a new window]

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

By virtue of the physical, chemical and dynamical characteristics of asteroids, researchers gain insight into the formation and evolution of our Solar system. Since these objects do not undergo any changes, or the changes during the Solar system evolution are insignificant, we are certain they carry important information regarding the formation of our planetary system and its evolution. Knowing the spectral class of an asteroid is crucial for determining its chemical properties. In our work the spectral classification was done on several asteroids by comparing their spectra with laboratory spectra. We determined spectral types of the asteroids by the overall shapes of the spectra between 450 nm and 700 nm. Increasing the number of asteroids with known rotation period, shapes and spectra enriches the asteroid database of physical and dynamical characteristics of asteroid population.

Keywords

minor planetsasteroidstechniques: spectroscopicmethods: laboratory
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 15 , Symposium S350: Laboratory Astrophysics: From Observations to Interpretation , April 2019 , pp. 448 - 450
Copyright
© International Astronomical Union 2020

References

Bebekovska, E., Borisov, G., Donchev, Z., Apostolovska, G. 2017, Astrometry and Astrophysics in the Gaia sky, Proceedings IAU Symposium No. 330 Google Scholar
Bus, S. J., Vila, F. & Barucci, M. A. 2012, Asteroids III, Univ. of Arizona Press, 169Google Scholar
Jockers, K. et al. 2000, Kinematika I Fizika Neb. Tel, Suppl, No 3, 13Google Scholar
Popescu, M. et al. 2012, A&A, 544, A130 Google Scholar