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This is because their atmospheric opacities cause only minor deviations from blackbody colours when integrated over the broad-band sensitivity curves of the human visual system. White dwarfs can have much denser atmospheres, reaching $\\sim 1$\u2009g\u2009cm$^{-3}$ for the coolest known objects. If metals such as carbon, calcium, or sodium are present in these ultradense atmospheres, extreme broadening of atomic and molecular opacities can produce optical spectra that diverge significantly from blackbodies. We investigated how the combination of temperature and chemical composition can affect the perceived colours (chromaticity) of white dwarfs. While we found that most white dwarfs are similar in colour to blackbodies, we also demonstrate examples of known stars that would appear yellow, green, cyan, pink, or purple if viewed close enough for their stellar discs to be resolved. We examined the chromaticity distribution for the volume-limited 20\u2009pc local sample of white dwarfs finding a median correlated colour temperature of $\\approx 6800$\u2009K, establishing that, on average, white dwarfs are indeed white in colour. 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