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29P/Schwassmann-Wachmann comet, Mirosław Stygar

29P/Schwassmann-Wachmann comet

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29P/Schwassmann-Wachmann comet, Mirosław Stygar

29P/Schwassmann-Wachmann comet

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Description

29P/Schwassmann–Wachmann (29P) is a periodic comet that orbits the Sun once every 5.3 years. Discovered in 1930 by Arnold Schwassmann and Arno Arthur Wachmann, this comet is notable for its bright and extended coma, or cloud of gas and dust, produced by the sublimation of frozen material on its surface (technically speaking it's more asteroid than comet).

The nucleus of 29P is estimated to be about 3.2 kilometers in diameter, and its coma can reach a diameter of up to 6 million kilometers. The comet's orbital inclination is approximately 6.3 degrees, meaning it follows a relatively circular path around the Sun. As it approaches perihelion – the point in its orbit where it is closest to the Sun – its coma can become particularly bright, making the comet visible to the naked eye.

The composition of 29P is fairly typical for comets, with a mix of volatile compounds such as carbon dioxide, water, and methane, as well as dust particles and organic molecules. During its close approach to the Sun, these materials sublimate and form the coma, which can be observed in visible light as well as infrared and ultraviolet wavelengths.

29P has been studied in detail by various astronomical instruments, including the Hubble Space Telescope, which has allowed researchers to map the rotation of its nucleus. The comet has also been observed in great detail using ground-based instruments, such as the Very Large Telescope in Chile.

The project included eight photographic sessions (two of them with my telescope and six with iTelescope observatory), spectroscopic measurements (unfortunately unsuccessful), photometric measurements and analysis of the nucleus by the Larson-Sekanina algorithm.

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29P/Schwassmann-Wachmann comet, Mirosław Stygar

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