comet
It stayed visible to the naked eye for 18 months in 1997, still a record.
Discovered independently by Alan Hale and Thomas Bopp in 1995, unusually far out, beyond Jupiter's orbit.
Its nucleus is exceptionally large, about 60 km across, a major reason for its remarkable brightness.
It is not due to return to the inner Solar System until around the year 2534.
Near the Sun it displayed three distinct tails at once: a dust tail, an ion tail, and a rare sodium tail.
At the time of its discovery it was beyond Jupiter's orbit, unusually far out for a comet spotted by amateur astronomers.
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