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A tidal tail is a thin, elongated region of stars and interstellar gas that extends into space from a galaxy. Tidal tails occur as a result of galactic tide forces between interacting galaxies. Examples of galaxies with tidal tails include the Tadpole Galaxy and the Mice Galaxies.
Comet Hale Bopp showing its two tails Courtesy of NASA. Comet Hale Bopp showing its two tails Courtesy of NASA. The ion tail T he ion tail is formed because the neutral gas, initially present in the cometary comae, is ionized by the solar radiation, giving birth to ions. These ions are susceptible to magnetic solar forces and are therefore swept out of the coma into a long, characteristic ion tail.