Observations of Halley's Comet, formally known as Comet
1P/Halley, have been traced back as far as 239 BC. There is no
historical record for any other periodic comet that can compare
with that of Halley's Comet.
Halley's Comet uniquely has been observed at 30 apparitions
over more than 2000 years because it is much larger and more
active than other periodic comets. It was named for Edmund
Halley who in 1705 realized the connection between several
previous cometary apparitions, and predicted its return in 1758-
59. In 1986, the Giotto spacecraft succeeded in imaging its nucleus
from a distance of only 10,000 km, and found it to be 15 km long
by 8 km wide. The coma and tail, which make the comet so
conspicuous, form when heating by the Sun causes gas and dust
to erupt as jets from the dark crust overlying the icy interior of
the comet nucleus.
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