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J AND H FILTER BRIGHTNESS OF VENUS: 2014-2020

Abstract

This paper summarizes J and H filter brightness measurememnts made of Venus between 2014 and 2020. Equations describing Venus' brightness at different solar phase angles are presented. There is also evidence, Venus is a bit dimmer (H filter) when its longitude is between 0 and 90 degrees than aother other longitudes. More measurements, however, are need to make firmer conclusions.

Acknowledgements

I would like to thank Gordon State College for a Faculty Development Grant in 2014 that made this work possible.

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