26–30 Apr 2021
https://us02web.zoom.us/j/2709113918?pwd=ZnIyUml2VEN6YnkvSi90eTlwUzNLUT09
Europe/Kiev timezone

Investigations of two distant comets C / 2014 B1 (Schwartz) and C / 2012 K6 (Mgnaught) at heliocentric distances from 4-9 AU (12+3)

30 Apr 2021, 10:30
15m
https://us02web.zoom.us/j/2709113918?pwd=ZnIyUml2VEN6YnkvSi90eTlwUzNLUT09

https://us02web.zoom.us/j/2709113918?pwd=ZnIyUml2VEN6YnkvSi90eTlwUzNLUT09

https://us02web.zoom.us/j/2709113918?pwd=ZnIyUml2VEN6YnkvSi90eTlwUzNLUT09

Speaker

Mr Roman Ruzhytskyi (Taras Shevchenko National University of Kyiv, Kyiv, Ukraine)

Description

Using the software Astrometrica and Maxlm DL5 to the observed data for two distant comets C / 2014 B1 (Schwartz) and C / 2012 K6 (McNaught) obtained on the 2nd telescope at Terskol, their values ​​of apparent magnitude were obtained. Using the value of the visible stellar magnitude, the absolute stellar magnitude, dust productivity in the form of the parameter Afρ were calculated, and the color value was also found. The morphology of the comet coma for the studied comets was investigated using digital filters. The data obtained were comparable with data for other distant comets.

Author

Mr Roman Ruzhytskyi (Taras Shevchenko National University of Kyiv, Kyiv, Ukraine)

Co-author

Oleksandra Ivanova (Astronomical Observatory of the National Academy of Sciences of Ukraine)

Presentation materials

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