Heads and tails
When far from the Sun, a comet resembles a dirty snowball a few kilometres wide.
Only when it reaches somewhere around the orbit of Mars do the Sun’s light and heat awaken the snowball from its hibernation so that it displays
itself for the admiration of astronomers.
A comet’s regalia has four components: a nucleus; a coma, which together with the nucleus makes up the head; a tail (although not in all cases); and, around the whole comet, a bubble of hydrogen,
millions of kilometres across, invisible to the eye but detectable by
instruments in space.
The fount of all cometary activity is the nucleus, the dirty snowball, composed
mostly of frozen water caked with dark dust. Under the warming influence of the
Sun, fountains of evaporating ice burst through the crust to form an enveloping
halo of gas and dust, the coma. An ordinary comet’s coma is about 10,000 kilometres wide, big enough to engulf the Earth, but in
the greatest comets, Halley’s among them, the coma spans more than 100,000 kilometres, half the distance
from the Earth to the Moon. For all its size, the coma is still transparent – stars can be seen shining through it, as they can through the tail. The gases
of a comet are far thinner than your breath.
In the popular mind a comet would not be a comet without its tail, but in truth the majority of comets are as tailless as
a Manx cat. Amputee comets are almost invariably faint, though, so just about
every comet that you are likely to see with the naked eye will have a tail, or
possibly two: one composed of gas and one of dust. You can tell the two apart
because the tail of gas is straighter, whereas the tail of dust is more curved
and smudgy. Note that the direction in which a comet spreads its tail is no
clue to the course the comet is steering, for a tail is not the wake of a
comet. Rather, the tail blows away from the Sun, so a departing comet actually
chases its own tail.
The black heart of Halley
The nucleus of Halley’s Comet, a dust-encrusted block of ice with a surface as dark as soot, as
photographed by the European space probe Giotto in 1986 March. It was 15 km
long by 7 km wide, larger than many astronomers had expected. Gas and dust was
spraying out from the nucleus through cracks in the surface. The ‘dirty snowball’ model of comet nuclei was put forward by the American astronomer Fred Whipple in 1950, but Halley’s nucleus was the first to be seen. Max Planck Institute for Solar System
Gas tails of comets are evidence that there is a ‘wind’ of sorts in space, known as the solar wind. This is a stream of atomic particles from the Sun which blows gas away from
the comet’s head like a flag in a breeze. Bombarded by the Sun’s ultraviolet light, the gas in the tail fluoresces like an advertising sign, as
does the gas in the coma, producing an ethereal self-luminance. Gas tails can
stretch for 100 million kilometres or more, as did that of Halley’s Comet in 1910.
Dust tails are shorter, and shine simply by reflecting sunlight. Impacts by
photons of sunlight push dust specks away from the comet’s head, an effect known as radiation pressure. As the dust recedes from the head it spreads out into a fan shape.
Clearly, a comet pays dearly for its moment of glory when near the Sun by
irretrievably shedding mass – over a hundred million tons each trip, in the case of a bright comet like
Halley’s. Yet the nucleus is big enough to survive thousands of returns. ☄
The magnificent Comet Hale–Bopp of 1997 displayed the two types of cometary tail to perfection: a straight,
blue gas tail and a broader, curving dust tail. European Southern Observatory.