The search for Pluto (the Roman
God of the Underworld), which began shortly after the discovery of Neptune, was most
associated with the astronomer Percival Lowell, a man more famous for his ideas about Mars
than discovery of distant planets. Still, the idea of a 'Planet X' fascinated him and soon
he began searching the heavens for this planet with a team of researchers, using his
private observatory in Flagstaff, Arizona. After many years of trawling through
photographs nothing was found until, 13 years after Lowell's death, a young amateur
astronomer named Clyde Tombaugh finally discovered Pluto in February 1930.
Since then this icy planet has fascinated many people the world over, yet not that much
is actually known about it, as its sheer distance from us has so far prohibited any space missions
to send probes near it, and makes viewing it from the ground harder too. However, this situation is changing - ever bigger
and more powerful telescopes are helping us to understand this planet, and as we keep learning
more details about this amazing world, it becomes ever more intriguing.
One of the reasons that Pluto is so fascinating for me, is that it seems a bit like a seagull in the desert -
totally out of place amongst its cosmic neighbours. All of the other 4 outer planets leading to Pluto are massive gas-giants
yet Pluto is small and solid. Due to this, and the fact that Pluto is considered to be a very large KBO - Kuiper Belt Object,
there has been some discussion as to whether Pluto should be officially classified as a planet.
Some Facts
Regardless, it has an average Density of between 1.8 and 2.1 g/cm3, and
is estimated to be composed of 50-75% rock mixed with ice. Proof of Pluto's icy surface temperature
comes with the knowledge that it's surface is composed 98% of Nitrogen, with traces of Carbon Monoxide and Methane, which can only be present
as a solid under 70K.
Also noteworthy is Pluto's highly elliptical orbit, because although it's usually
the farthest planet from the Sun, there is an occasion during its orbit that it's actually
inside Neptune's orbit! This last happened in 1979 and serves to demonstrate just how much the planet's
distance from the Sun varies. At the moment it has recently passed its closest point and is
slowly increasing its distance from the Sun. Pluto also has
a thin atmosphere of Carbon Dioxide and Methane. This atmosphere is not permanent though
and when Pluto gets too far from the Sun, it collapses. This is next expected to happen in
2020 or so, although we can't be sure as it has never actually been observed.
Charon
As I already mentioned, Pluto is a planet of superlatives - the smallest, farthest and coldest
'planet' orbiting the Sun. Its diameter is a mere 2,320 kilometers (about two thirds that of
our moon), and yet, rather surprisingly, Pluto has a
moon of its own; Charon. Charon is 1,210 kilometers wide, more than half the diameter of
Pluto itself, and becuse of this, Pluto is often referred to as a 'Double Planet'. Charon thereofore holds the record of being the largest Moon
relative to its planet in the Solar System.
It is considered very likely that Pluto and Charon were formed independantly of each other,
unlike the Earth and our moon, due to the fact that its surface composition is thought to be very different (mainly water ice) and
also because it has a much lighter density (approx 1.2g/cm3 to Pluto's 1.8-2.1).
Strangely, Charon circles Pluto in a slightly eccentric orbit (0.0076),
probably due to the recent collision of a sizeable object. Another peculiar feature had by Pluto
and Charon though is that Charon orbits Pluto in the same 6.387 days that Pluto takes to
rotate, keeping the two locked in synchronous rotation. Charon therefore behaves like our
moon in this respect - it always keeps the same face towards Pluto; the difference in this case
however is that Pluto also always keeps the same face towards Charon!