14. Astronomy , Cosmology
Planet Formation
Nobody knows for sure how planets are formed, because we
haven’t been around to watch one. But we have a pretty good idea. The driving
factor here, as is often the case, is gravity. If you take a large cloud of gas
and debris in space, all the bits of the cloud attract all the other bits
together; that is what gravity does. The bits will gradually move towards the
‘centre of gravity’ of the cloud, and eventually form a glob of ‘proto planet’
– if it happens to be near a star, that is. And if it is near a star, it will
also be orbiting it, or else it will fall into the star, or disappear into
inter stellar space. Technically of course, a planet has to be in orbit around
a star, but the process I am describing could apply elsewhere – as indeed it
does for star formation, only on a larger scale.
Gravitational
attraction depends on two things – the amount of matter, and the distance
between them. The closer things are, the stronger the gravitational attraction.
So as the cloud ‘condenses’, the movement gets faster as the
bits get closer, the attraction increases, gets faster, and so on until they
all come together in a clump. This is our old friend positive feedback. Even
when the bits have stuck together, gravity hasn’t quite finished its work. If
the planet is big enough, the gravitational forces will cause the inner planet
to heat up. This is partly why the centre of the earth is hot. It is not the
only reason, though; atomic decay adds a large part to the heating. This caused
a lot of confusion in the early days of evolutionary theory. It was thought
that the earth was not old enough to provide enough time for evolution to have
done its work, until it was realised that the nuclear decay was the key factor
that kept the earth’s core hot.
Novas, Supernovas
When a star grows
old, and loses its youthful vitality, it gets weak and tired. It just can’t
throw off the energy like it used to (you know, like sunlight). Now a large
object like a star has a lot of gravitational attraction between all the bits
of stuff inside it. When it can’t throw off enough energy, it starts to lose
the battle with gravity (a bit like we do when we get old). It starts to
collapse under its own gravitational strain.
Now the thing
about gravity is that the closer things get, the stronger the gravitational
attraction gets. So as the star starts to shrink, the attraction of its own
stuff gets stronger. And as it gets stronger, it collapses more quickly. And as
it collapses more, the stuff gets closer, and the gravity gets stronger. Sounds
familiar? Its that old positive feedback again. The collapsing strengthens the
gravitational attraction, and that quickens the collapse, so much so that the
final collapse of a huge star can be a matter of seconds. Perhaps its not quite
classic feedback, but its close enough. In a way it is similar to thermal
runaway, on rather a large scale.
So what happens?
Well, when a big star collapses far enough, it starts to heat up under the
strain (sounds a bit like me). The heat energy starts to counter balance the
gravitation energy, and when it gets hot enough it just explodes. Depending on
how big the star is, it is either a huge explosion (a nova) or a ginormous one
(a supernova).
If the star isn’t
big enough, it just can’t hack being a nova, so it settles down into a sort of
quiet old age as a white dwarf, or a neutron star. Though apparently all is not
quite so quiet as you might expect. While doing my research, I came across a
reference to thermal runaway on the surface of white dwarfs. You may be glad to
know that I am not going into that in depth, but it just goes to show how
widespread these fundamental processes are.
Goldilocks
I will leave you
with one final (possible) example of feedback in the cosmos. Paul Davies has
written a book on The Goldilocks Enigma.
The title refers to the difficult puzzle of why it is that many things about
the Cosmos and the earth are ‘just right’ for life to form. Many physical
constants and processes are remarkably ‘fine tuned’ so that stars can form and
produce all the other elements, and the earth is also in the right kind of
orbit round the right kind of star so that life can form. There is some debate
about just how fine the tuning actually is, but all agree that it remains something
of a difficult question. There are several attempts to provide answers, and I
am not going to go into all of them here. Many are built around something
called the ‘Anthropic Principle’, which comes in various flavours, but
basically says that things have got to be the way they are for us to be here
asking the question. So don’t worry about it.
Davies doesn’t
like this answer, and has come up with another one which is a bit tricky to
explain, as it depends on quantum physics. It has been said, and oft repeated,
that if you think you understand quantum physics, then you haven’t really
understood it. Rather fittingly, there seems to be some uncertainty as to who
said this; some say Richard Feynman, some Neils Bohr, or even John Wheeler, who
seems to get everywhere, like a quantum particle. Maybe they all said it.
Quantum physics was developed in the early part of the twentieth century, and a
hundred years later, scientists are still unsure of what it really ‘means’.
Like the old joke about economists, if you ask five scientists to explain what
quantum physics really tells us, you will get six different answers. There are
many popular science books that try and explain these problems, such as John
Gribbin’s Schrodinger’s Kittens, so I
am not going to go into detail.
The hard part of
the quantum world is that it seems that on the very small scale, things just do
not behave in any sensible way. Particles are not in any exact place (or maybe
even time), but are rather fuzzy, or at least that is one way of looking at it.
Quantum
physicists explain the difference between this and the ‘real world’ that we are
used to by saying that the fuzziness ‘collapses’ at some rather hard to
determine point. Others though say that this is the wrong way of looking at it,
and that the universe is actually a ‘multiverse’ consisting of a very large
(possibly infinite) number of universes in a sort of tangled super universe all
running in parallel. People working on quantum cosmology tend to this view,
because that is the way the mathematics leads them when you try and do the
maths on the whole universe. This viewpoint was originally proposed by Everett , expanded by De Witt, and championed
recently by David Deutsch, among others. One of the strange consequences of
this view of things is that there is (according to Davies and others) no such
thing as a ‘unique past’. This is pretty hard to get hold of, because I can
generally remember things in the past, or at least, I used to be able to before
I started having senior moments. The point is, that in the multiverse,
different universe strands become entangled and unentangled in a way that makes
it impossible to completely separate them.
Now what Davies
is proposing is that there is some kind of feedback loop that operates on the
whole multiverse so that in some sense the future influences the past, as well
as the past influencing the future. There is a nice kind of symmetry in this
that I quite like, and in fact I had some ideas along these lines, for totally
different reasons, a long time ago. Just because an idea looks nice doesn’t
make it right though. Anyway, what Davies is saying is that life, and
intelligence, form a fundamental part of the whole scheme of things, and so in
a way is responsible for tweaking the multiverse in the right direction for
life to form. So it all depends on feedback, life the universe and everything.
You can’t top that, so I will stop right here.