Some Simple SumsDave Mitchell |
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1. Wrestling with numbers Maths
is notorious for inducing mental panic – and yet it is supposed to SIMPLIFY
thinking. Suppose that there are n people in this room, to stop fights breaking
out, let’s all shake hands. Let t be
the time to shake hands, then if everyone shakes hands with everyone else, then
each of n people must shake hands with n-1 others, so the total time, big T,
taken by this orgy of peace-making equals n(n-1)t – or does it? Let’s run a test
for a small value of n. Suppose n=2, then the formula yields 2t, but we know
only one handshake is required. Aha, our formula has counted every handshake
from the point of view of every person- every shake has been double-counted, so
the correct formula is n(n-1)/2. Let’s
tabulate this for various n, Café Philosophiques do
attract a variable attendance -actually, rather more people than I have
included below, with our normal attendance of between 20 and 30, we would be a
long time shaking.
You
notice I have added some other columns. A new-age three-hug requires three
people, and work out the number of different three-hugs we have to divide by 3
times 2, the number of different orders in which the three people can be chosen
in order to eliminate double-counting and get the right answer. When counting just
the number of peoplem (collumn
2) I have put in a “divide by 1”, as there is no double counting. I have also
added a column of constant unity to the left and finally also a row for zero
people. These modifications are there to bring out the beautiful simplicity of
this table. You can now see that you don’t need to bother with multiplying
figures together. As you go to the right, the figure in each cell of the table
can be found by simply adding the figure in the cell above to the figure in the
cell above and to the left. This means that the figure in each cell is also the
sum of the series of ALL the numbers
in the column to the left up to and including the cell above and to the left.
If you know some algebra, you recognise that the first column tabulates value
of a constant, the second of a linear function, the second of a
function including a square of n ( a quadratic
function), the third a cubic
function, and that we could go on adding as many columns to the right as we
liked in order to tabulate values of the function n(n-1)(n-2)……..(n-r+1)/
1x2x3…xr, which is the number of r-hugs and is a polynomial involving n to the power r,
where r can be as large as we like. We call 1x2x3x4…..xr,
r factorial, or r! for short, as factorials crop up all over
the place in combinatorial mathematics (which is what we have been talking
about), probability theory and statistics. For me, this has been a classical
and beautiful mathematical exercise, embarking on a potentially endless journey
into more and more general results, with wider and wider implications, starting
from just one simple idea – that of shaking hands. Does
this sort of thing worry you? Well, you are in good company. We can trace back
mathematical thinking to, for instance, Babylonian problems still preserved on
4000-year-old inscribed and baked tablets. Already in those days, the master
was setting examples that can still terrify us today! I found a stone but did not
weigh it. I weighed out six times its weight and added 2 gin,
then added one third of one seventh of this weight multiplied by 24. The total
weight was finally 1 man-na. What was the original
weight of the stone? Answer,
4 1/3 man-na .This works out correctly if 1 man-na
equals 60 gin. Incidentally,
we see just how long ago and far away the basis of our conventional division of
hours into 60 minutes and minutes into 60 seconds, both of time and of angle,
was established. An
Egyptian problem, found on a Papyrus about 3600 years old, seems simpler: If 10 hekat
of fat is given out for a year, what is the amount used in a day? ( c.f.
if 104 black bin-bags are given out for a year, how many are used in a week?) The
answer however is not so simple, being expressed as: 1/64
hekat and 3 2/3 1/10 1/2190 ro.
(I hekat = 320 ro) Here
we see that, with the exception of 2/3, and maybe also ¾, the Egyptian notation
and probably the Egyptian mind could not deal with fractions other than “One
share of however many”. A fraction like 56/73 (which the above addition of
shares equals) was beyond writing down and probably beyond thinking about. Problems
with notation have taken much of the following three and a half thousand years
to deal with. Modern fractions like 56 73rds only gradually
permeated Europe from Arabia and Note
that the above-mentioned three and a half
thousand years, say 3511 years, to be precise,
could have been expressed as: three
millennia plus five centuries plus one decade plus one year. It is
revealing to quote a Derbyshire sale catalogue dating from 1920 for lands
belonging to His Grace the Duke of Rutland: Here is a typical lot description
(shortened): Yeld Wood Farm, Woodlands & Cottage situate close to the As
you will know (?) there are forty perches to a rood and four roods to an acre. A
rood can be well visualised as the typical area of a mediaeval strip (or
perhaps half a strip), one furlong long by one pole wide, or 220 yards by 5 ½
yards. A perch is simply a square rod (or pole), 5 ½ yards by 5 ½ yards. So, you see how
the prospective buyer can actually visualise the land area involved, whereas
giving it as 82.87265, say 82.88, acres, or 82 and 71/80 acres, requires the
farmer to visualise 0.88 of an acre; probably he’d rather have it in roods and
perches. An ancient Egyptian might render the area for sale as 82 ½ ¼ 1/8 1/80 acres. All this takes
me back to primary school, I used to be able to add, subtract and even multiply
in acres, roods and perches, and in miles, furlongs, chains, rods, yards, feet
and inches. Measurement systems like this are meant to avoid the need to think
in terms of fractions or decimals. Almost any quantity can be expressed as
integral (whole number) multiples of units you have a habitual feel for. Same
with old money: one pounds, seven shillings and six pence ha’penny.
Nowadays, since decimalisation, we still have the various sized coins
reflecting our physical need to hand
over change in “roods and perches”, to speak metaphorically, namely the 50p,
the20p, the10p, 5p, 2p and 1p coins, but we no longer have common names for
them and may get quite confused trying to convert, say, 83p into a convenient palmful of change. Not so the
mathematician. He, or I maybe, have surrendered the
primitive need to visualise the sizes of the quantities we deal with in
exchange for the extreme simplicity of the decimal system. Everything is in
multiples or divisors by ten. 82.87265 acres may be hard to imagine, but it can
be multiplied by a hundred by a simple double shift of the decimal point. Other
multiplications, additions and subtractions take a bit longer than this but are
completely straightforward. In contrast, imagine trying to work out how many 4
ounce bags of sweets can be made up from a day’s production of 2 tons, 7
hundredweights, 3 stones, 5 pounds and 12 ounces, which latter is expressed
entirely in units I still have a real feel for. 2.372 tonnes = 2372 Kilograms = 23,720 100gramme
bags is so much easier! This handy
decimal system goes back at least to the 10, 100, 1000,
10000, 100000, 1000000,…. is getting hard to write, let alone
distinguish just how many 0’s there are. So generalising on 100 being 10
squared, written 10², we can write the sequence as: 10,10,²10³,
… and so on, these being
the sort of numbers that appear in successive columns of our handshake and hug
table. Similarly, the
sequence of numbers less than 1: 0.1, 0.01,
0.001, 0.0001, 0.00001,…. Can
be written 10‾1 (that is one over ten), 10ˉ² (one over tensquared), 10ˉ³, and so on. (For
mathematicians to deal with numbers less than 1 in these elegant decimal and
power expressions took a lot longer in the adoption than dealing with the
larger-than -one numbers. Finally, to join these sequences of powers together
we are forced to adopt the convention that the number 1, unity itself,= 10° , even though multiplying a number by itself zero
times seems meaningless) Now, at last we are in a position to start
measuring the Universe.
2.
Getting the Measure of the Universe In reaching out
to see the great and the little, we start with a measure of our own size, 1
metre – a stride, an arm’s length, a child’s height. – this
is our 10°. Let’s start
going up in scale in powers of ten, or, as practical scientists say
“orders of magnitude” Order 1 10metres; the width of the bookshop Order2 100 metres; a sprint, how far a shout
will carry, or a missile be thrown Order 3 1 kilometre; a walk to the station, a
waving friend visible Order 4 10 Km; the distance to the nearest town,
a long run Order
5 100Km; a journey to
the regional capital, to court, to prison, to the seaside. Now we are beginning to reach the edge
of the pre-industrial ordinary person’s experience Order 6 1000Km; travelling to the national capita
city, to another country, or on a pilgrimage An experience of
only a few courtiers, merchants, churchmen, armies Order 7 10,000Km; The voyage of Christopher
Columbus, Marco Polo’s travels Order
8 100,000Km; A girdle
around the Earth. We are now
getting to the edge of the ordinary person’s experience, but not beyond the
ingenious measurements of the Greek geometers, who obtained very good estimates
for the size of the Earth. Order 9 1 million Km; The distance to the Moon; beyond the
ordinary mortal, but again not beyond the ingenious Greeks, whose curiosity and
method is humbling. They visualised the distance in “stades”,
a foot-race distance of about 200 yards. Order
11 100 million Km; The
distance to the sun.
Even this the Greeks tried to measure, and their estimate was “correct” to
within an order of magnitude; ity was more accurately
known by the 17th. Century. A digression, what is a triumph in science may remain useless
in practice! Order
12 1 billion Km; The
distance to Jupiter.
Only the invention of the “Gallilean” telescope made
this possible to conceive .Galileo first observed Jupiter’s 4 largest moons in
1610. They are easily seen with binoculars and, as early as 1676, small delays
in their eclipsing by the planet were used to obtain a good stab at the speed
of light, unimaginable at 186, 000 miles (Anglo-Saxon motorway units) per
second. Order
16 1 Light Year, or a
third of a parsec.
The nearest star is about 4 light-years away. Note the introduction of new
units to try to help us visualise the immensities. The distance to a star (not a planet) was
first measured in 1838, using parallax, the slight change in direction from
opposite sides of the Earth’s orbit. Order 21
Diameter of the Milky Way, our galaxy (100,000 light years) Advances in
the measurement and understanding of starlight spectrums and in so-called
Cepheid variable stars made measurements like this possible by about 1915. A digressional
quote from the internet, how to bring the Universe down to size: There are an estimated 150 globular clusters that swarm around our
galaxy. Each of them contains 100,000 to 1,000,000 stars in a spherical
region ONLY a few hundred light-years in diameter. Order 22 1 million light years, is the
approximate distance to the nearest other galaxy, The Great Nebula in
Andromeda, M 31. Controversy about whether “galaxies”, those fuzzy objects,
were gas clouds, perhaps forming stars, in the Milky Way, or other collections
of stars at a great distance, was finally settled only in 1923 (the approximate
birth date of Freeman Dyson) with the
aid of the 100 inch Mount Wilson telescope– individual stars could now be seen
in the M31 nebula. Order 25 In 1929, Edwin Hubble proposed his
celebrated “expanding universe” theory. The dimmer the supernovae, the further
away the galaxy and the bigger the red shift, explained by its
receding from us. A billion light years is about the limit for observations of
this type on galaxies. Order 26 Ten billion light years. The distance to the
edge of the observable universe is currently estimated as about 16 billion
light years, giving a visible diameter of twice this. So, the largest number we can come up with, relating the size of the
observable Universe to a stretchy human pace-length is some 3 X 10²6 Though the
Greeks imagination reached out to their estimate for the Sun’s distance, of order
10, it was not until the 17th. Century that planetary distances
became accepted, order 11 to 12, not until the 19th. Century
that the true remoteness of the fixed stars was revealed, order 16 and
not until the lifetime of the parents of many at this meeting that the true
scale of the observable Universe, orders 22 to 26, was understood and
accepted. Surely we must
question whether any existential philosophy more than 200 years old can have
more than inspirational or allegorical significance? 3.
Smaller and ever-smaller Time now to turn from telescopy
to microscopy and go down in scale to the smaller and smaller, starting
again from our “zeroth” order of I metre. Order Minus 1 10cms.
A “handy” size, the scale of a handspan,
a fist, a stone, a sheet of writing paper, a jug of milk. Order Minus 2 1 cm.
A finger’s-breadth, a flower, handwriting, an easily snapped
twig, a pebble Order Minus 3 1 mm. Getting hard to see. Grit, a seed,
a pin-head, your nails needing cutting Order Minus 4 0.1 mm. About as small as can be seen or
imagined to be see-able (!) by the naked eye. Small seeds, sand-grains, eye of
a needle. From mediaeval times, magnifiable to a more
comfortable scale by single-lens “reading glasses” ( as
in Name of the Rose) Order Minus 5 0.01mm. 10 micro-metres.
\Silt or “soil” particles; they don’t float but do smear. Pollen grains – may
blow about but can and need to settle. The cells of animal and plant tissues
are often in this range; first described by Robert Hooke, c. 1670 Order Minus 6 1 micrometre. Dust.
As we know, you can’t see it till it settles. In the 17th.
Century, the double-lens microscope allowing X20 to X200 magnification
brought this scale into view. Order Minus 7 0.1 micrometres or 100 nanometres. The wavelength of
visible light is in the range 400-700 Nm. and this limits
what could be distinguished using the best optical microscopes by late
Victorian times. Order Minus 9 1
nanometre, a billionth of a metre; about the diameter of a sugar molecule. The
actual existence of “molecules” became accepted during the 19th.
Century, but the direct investigation of their structure only began c. 1920
with X-ray crystallography, X-rays having a wavelength comparable to molecular
sizes. Order Minus
10 1 Angstrom, a tenth
of a nanometre, 100 picometres; typical effective
size and separation of atoms.
Order Minus 12 1 picometre , a billionth of a millimetre. The wavelength of the
electrons used in microscopy is about 5 picometres.
This limits the electron microscope, developed in the 1930’s. ORDER minus 13
This
is where “High Energy Physics” takes over; larger and larger linear and
circular accelerators:-, particularly since about 1960, CERN and the infant Large Hadron Collider Order Minus 15 1 femtometre roughly the radius
(whatever that means) of a proton or electron. The existence of the electron
was deduced about 1900, but protons and neutrons not until their tracks could
be followed in cloud or bubble chambers from about 1930 Order Minus 18 1 attometre
or nano-nanometre. About the feasible limit of High
Energy Physics and correspondingly the scale of elementary forces and particles
studied. Order Minus 45 The
Planck Length.
An entirely hypothetical and especially hard to understand
concept. May perhaps be thought of as the ultimate limit of the
precision with which a particle’s position could be ascertained in the quantum
theory. The energy of the probing particle/wave would be such that a black hole
would be formed, so no measurement would result (!?!) I have gone down to the very, to the 27th. Power, silly Planck Length just because I want
to give the Universe a chance to resist the power of the human mind! So, the extension of man’s ability to look at
very small things has gone from order 7 to order 18 in little
more than 100 years. As with the very large, surely our outlook should have
changed radically with such an expansion in our ability to observe the
sub-sub-microscopic entities of which everyday objects and ourselves are made
up. Certainly, we are filled with wonder by television programmes, articles and
books, but most of even us “educated classes” experience little outside the
everyday scale in our everyday lives. We are mostly scientifically ill-informed
and even more inexperienced; we probably do not own or rarely use a microscope
or a telescope, let alone an x-ray diffractometer or
a linear accelerator! It is very easy, still, for us to live in an
unquestioning mental world akain to that of the
“ancients” in which only a few visionaries posed fundamental questions. How
many of us have ever thought of estimating the moon’s distance by timing the
length of a lunar eclipse, as did the Greek natural philosophers. 4. But how BIG is the Universe, actually? "Space is big. Really big. You just
won't believe how vastly hugely mind-bogglingly big it is. I mean, you may
think it's a long way down the road to the chemist, but that's just peanuts to
space.” Douglas Adams: The Hitch-hiker’s Guide to the
Universe That is, how many
conceivable points does it contain? EASY! 4πR³, where
R is the radius in Planck Lengths, 1.6πX10 to power71x3, let’s
approximate a bit, after all my calculations may not be that precise, 10 to the power 324 is near enough. 5.
God’s Numbering System But the very hairs
of your head are all numbered. Matthew Ch. 10
Verse 30 God is supposed to have no problem numbering, that is
describing and knowing, every point in the World, now known to be so much
bigger than the Evangelist could have thought, and implied in the quotation. The readers of the Bible are supposed to be awe-struck by
this degree of omniscience. Not so Archimedes, who explains, in the 3rd.
century B.C, in a paper addressed to a King Gelon, that has numbering
system is perfectly capable of dealing with the number of grains of sand that might
be needed to fill the Universe. Our numbering system is also perfectly capable
of dealing with the scale of things, as we have already seen. Another way to look at this is to perform a card trick.
Imagine I am holding three perfectly
normal packs of 52 cards, excluding
troublesome jokers, 156 cards which to simplify things can be considered all to
be different, each pack having a different design on the back. I assure you
that this pack has not be prepared or tampered with in any unfair way, but the cards
are of course in one particular order. Now, watch carefully. Dave fans,
shuffles, fumbles and drops the whole pack on the floor. Oh *******!! How am I
ever to sort them out again? Well, if I work through all the possible orders to
find the right one – a 152-letter message, I will need not merely all the time
in the world, but much more than that! There are just two ways of ordering two cards, six of
ordering three, twenty-four of ordering four, in short 1x2x3x4x……x156 of
ordering them all – its that FACTORIAL again, 156! This number is rather large.
I haven’t had time to calculate it, but I do know that 70! Is approximately 10
to the 100th., so 100 factorial is going to be at least 10 to the
150th and somewhere around
the three-pack mark the number of ways of ordering the cards is going to exceed
10 to the power 324, the number of “Planck points” in the visible universe. So
there on the floor is all that God needs to number all the hairs on the head of
all of space. Now there is a very theoretical minimum conceivable time
interval ca;lled the Planck
Time, about 10 to the power of minus 43 seconds.( this is about We can also see that God would not need mnay
more playing cards to number not merely each point in the Universe, but each
point at each instant in the life of the Universe, each point in space time,
with plenty of room left over to describe what is going on at each point,
whether empty, or associated with a particle, or with the scale and direction
of each possible force field, and finish by giving this point in space-time a
fanciful name, perhaps inspired by Peak Rock-climb or Lead-mine nomenclature! Don’t Sneeze Now Arete or Second-Cousin’s
Fortune. There are even more names available that orderings of playing
cards. Which leads us to: 6.
Monkeys Typing Shakespeare Shall I compare thee to a summer’s
Day? Thou art more beautiful and
more temperate. Rough winds do shake the
darling buds of May And summer’s lease hath all too
short a date. At this point I had intended to
embark on some intricate calculations of the time it would take the proverbial
“monkeys” to type even this one supreme sonnet of Shakespeare, but I think you
have got my drift by now. Even were the monkeys able to employ, not
typewriters, but the still proverbial “Quantum Computer”, they would have no
chance of discovering even an early draft by the bard within the lifetime of
the Universe. This is, I suppose, a commonplace observation, but it is less
commonplace to ask; “How then DID the sonnets of Shakespeare ever GET
written – starting from the blankish, even if anthropophilic slate of the early Universe” Particularly as the Universe
got off to such a laggardly start in the race to
write Shakespeare’s works.. Nearly ten billion years
were given over just to forming giant stars, letting them manufacture heavy
elements and then blow themselves up, so that the scattered materials could
condense into a second generation of stars and dust containing elements useful
for forming iron and silicon planets. Another half-billion years at least were
required for things to solidify a bit on planet Earth and for Jupiter to vacuum
up most of the dangerous impacting meteors. Another mere hundred million years
or two sufficed for life to appear, but more than three billion years were used
up before it crept out of the sea. Another 300 million years were needed to
evolve mammals and 298 million years to evolve the first self-consciously intelligent
species. And during all this time, the monkeys can be imagined typing away, by
now well in the lead – they’ve written several very beautiful lines of a risqué
sonnet. Even the last two million years before the present, about a
ten-thousandth of the lifetime of the Universe, have largely been employed in
developing language from scratch, honing all our subtle passions, emotions and
abstract intelligence and in developing the art of story-telling and aural
tradition. Only in the last 50,000 or so years have written alphabets allowed
remembered culture to develop and be passed on. Urban living, with all its
special crafts, including those of playwright and poet, seems to extend back no further than
10,000 years before the present, and this period is essentially that which has
allowed literature, philosophy and science to be recorded so that the likes of
Shakespeare and Newton could rejoice in “standing upon the shoulders of giants”
to achieve there own dazzling in- and out-sights. So we allowed the typing
Monkeys a very long start indeed, but we still got there first! This shows the
true scale of the wonder of human thought Douglas Adams once again got here
first – his super-computer Deep Thought, faced with discovering
the QUESTION to which 42 is the ANSWER to the riddle of Life, the Universe and Everything
announces that it needs to design: “A computer which can calculate the Question to the Ultimate Answer,
a computer of such infinite and subtle complexity that organic life itself
shall form part of its operational matrix…. And it shall be called..the Earth” 7.
The Pen is mightier than the Interstellar Sword So much for the scale of the
Universe, we can hack it! Actually, we
can have a good stab at bringing the mind-boggling idea (one of our own, it
must be allowed ) of INFINITY down to size. Actually, it turns out that there is not one
“infinity”, but an infinity of infinities, of which the endless string of
numbers, 1,2,3,4,5,6,7,8,9,…….is the littlest sister. These distinctions were
clarified by Georg Ferdinand Ludwig Philipp Cantor
in the late nineteenth century. Incidentally, it is obvious that his parents
knew he was destined for great things! Well, Masters of the
Universe are we? Well, no. We
can certainly think, but we cannot do much. The Earth in its
present age is our Ivory Tower; we are pub-philosophers, mere impractical
theoreticians when faced with the real world. We are trapped in a doomed pub, I
mean planet, in an otherwise inhospitable solar system. And Doomsday, for
technological civilisation at least, may be nearer than we would like. Don’t
for a minute imagine we can terraform and colonise
Mars or a Jovian moon – we can’t even stop the spread of the Project Daedalus
looked at a “fly-by” (i.e. non-decelerating) trip to Barnard’s Star, taking 50
years at an average speed of 15% of the speed of light. The starship
would weigh only 46,000 tons – launchable by only
1000 Saturn Rockets using only a few million tons of fuel. BUT, its propulsion
would be by fusion (after decades of experimentation STILL far from achievable
in a controlled way) of 26,000 tons of Helium, mined from the atmosphere of
Jupiter. And that is the LEAST starry-eyed of the several alternatives they
pursued! I have not checked the
calculations (maybe I could), but if the energy needed for such a voyage were
not to be excised from Jupiter, who would certainly hardly notice, it would
require the siphoning off from domestic use of energy equivalent to more than
50 years-worth of the entire national consumption of the USA. The trouble is
that Barnard’s Star and other possibly “hopeful” star systems are about 200
million times as far away as the Moon. If we were content, as we have been so
far with Voyager 1 and 2, to let an interplanetary rocket just keep on going,
it would take several million years to reach the target star. Personally, I think this is
well worth doing. The von Daniken assertion that
Aliens have visited the Earth is just faintly possible if by “aliens” you mean
an interstellar probe sent out some time in the last hundred or two million
years by another advanced civilisation. Maybe the craft burnt up on entering
our atmosphere – maybe you have seen it burn up on a clear night in August, but
maybe some blistered remnant got through and is lying buried in the
Carboniferous rocks of the Peak District! Or maybe we should send out a rocket
containing thousands of lead and insulation-encased spores or viruses, or just
some amino acids or RNA. The mother capsule would travel beyond the solar
system and then be programmed to shatter explosively, sending its millions of
separate seeds to scatter throughout the galaxy. There is all the time in the
Universe for them to find a home. Maybe, as Fred Hoyle maintained with his So we can’t get there. It takes
too long, or it takes too much energy to get up to speeds comparable with the
speed of light. But what about light itself, and the invisible spectrum of
electromagnetic radiation of which it is part? That’s travelling at the speed
of light already! If we shout loud enough, we can be heard at Barnard’s star in
only ten year’s time. An answering “COOEEE” might come back within the lifetime
of those of us gathered here tonight. The sending out of messages and the
listening for messages that might be aimed at us is, of course known by the
acronym SETI, the Search for Extra-terrestrial Intelligence”. At a conference in 1961, Frank
Drake set out his eponymous Drake
Equation for the number of interstellar-communicating civilisations at
present in our Galaxy.(The fact that the “present” is
modified by the long times taken for messages to travel even at the speed of
light need not bother us TOO much –though there is a danger that everyone will
have gone to sleep before a reply comes through from the other side of the
Milky Way). Let N be the number of such civilisations, then: N
= ( Rate of Star Formation )X (fraction with planets)
X( number of habitable planets) X( probability of life emerging) X (probability
of intelligence evolving) X (probability of electromagnetic technology
developing)X(lifetime of electromagnetically-active civilisation) The value, even the range of
values, that all of these factors might take has remained controversial for the
last 47 years. There is even major disagreement about the rate of star
formation, a “simple” matter of statistics and physics. If there are 200
billion stars in the Milky Way, and the galaxy is 10 billion years old, hey
presto, the average rate of formation is 20 per year. Most great minds, using
much more sophisticated arguments, have still come out with estimates in the
range 4 to 50 per year, but there is a school of thought that thinks the great
pioneering days of the Milky Way are over, we are past the galactic menopause!
Regarding the fraction with planets, there have been enormous strides since the
detection of the first extra-solar planet was announced only in 1995, but
discoveries since then have tended to confirm what had long been assumed, that
most single (rather than double or multiple) stars will have planets in stable
orbits. Habitable planets are, however, rather special beasts, and just how
special the Earth is has become more and more evident. It seems we need to be
not only the right distance from the sun, but big enough to hold an atmosphere,
but not so big that the greenhouse effect spirals. Maybe the right constitution
to produce vulcanism and plate-tectonics has been
crucial. Maybe we need the large moon to
produce an intertidal zone. Almost certainly we have
needed father Jupiter to clean up the solar system of large boulders the impact
of which would otherwise produce too frequent and too comprehensive extinctions
of multi-cellular lifeforms. Even given this perfect
planet, is it inevitable that life will spontaneously appear, or was it an
ultimately improbable one-off event? The principle
of mediocrity supports the common appearance of life, but can in the
absence of further evidence be trumped by the anthropic principle- that the Earth, the Universe and Laws of Nature might
be tailor-made to suit our navel-contemplating development ,
so that our being here says nothing about the likelihood of comparable beings
elsewhere – we’re here because we’re here
because we’re here, you might say. As for the development of intelligence,
speculation goes wild – suppose the dinosaurs had not bee extinguished; suppose
mammals had not survived. The most depressing
factor in the Drake Equation however is
the lifetime of a technologically advanced civilisation. Our look at how the
Universe wrote the works of Shakespeare without employing monkeys makes it seem
that we are living in a period of exponentially increasing “progress”,
comparable changes occurring in a billion, then a million, then a thousand,
then a hundred, then twenty years. Are we approaching an asymptote a very few years hence, when all will revert catastrophically
to a much earlier phase – or will the pace of change slow as we arrive on a
high plateau of wellbeing? History and current anxieties do not encourage
optimism. Imagine that there is a “High Plateau” civilisation somewhere in our
galaxy. A million years ago their telescopes identified a promising planet in
orbit around Sol; there was even the spectroscopic signature of oxygen in its
atmosphere, an almost certain sign of organic life. Straightaway, they trained
their radio telescopes on the Earth and initiated both a listening watch and
transmission of a beacon signal. For thousands of years, that is for thousands
of generations (c.f. Douglas Adams’ priests watching over the computer Deep
Thought – he got there first AGAIN), this stable civilisation persevered in
watching and calling Earth. If we examine our own culture, you can see how
unlikely even this possible scenario is. Finally, they gave up hope and
switched their gaze elsewhere – in our year 1933, perhaps, just before we
discovered cosmic radio interference. Maybe they will look again in another few
thousand year’s time – but will our technological civilisation still be here? So, even if there can be
life out there among the stars, we may have only a thousand billionths of a
chance of “catching it in when we knock, especially if it operates a timeshare.
8.
Some
Conclusions – Douglas Adams wuz here. We have conducted a lightning tour through the historic
development of mathematics and how its notations have helped us to tame the
immense scale of the Universe, a scale that has only become apparent in the
last four centuries or so. In my humble opinion, mankind will never reach a
limit to our ability to think about the laws by which this Universe operates,
the flexibility of even our so-called “Hunter-gatherer” minds far, far exceeds
the demands that physics and cosmology place upon us. There is a beautiful and dangerous snag, though. I have left
out of all this the study of life itself – of ourselves. Here, our very
flexibility and complexity means that our studies of ourselves lag ever further
and further behind our individual and cultural creations. Our abstract
abilities can remain abstract in the ever expanding frontiers of pure
mathematics, or abstraction can become realised as Music, as Art, as
Literature, as Financial Instruments, as Warfare – as Philosophy. The scope of
our ability to outrun our own understanding is another indication of how the
physical universe is orders of magnitude simpler than the creations of our own
individual and social selves. Is it surprising that, during my lifetime we seem
to have turned in on ourselves, becoming obsessed not with exploring the world
“out there” but with understanding and trying to control the social and
environmental implications of our own species. Nevertheless, in our big Ivory Tower the earth, and this little
ivory tower, The Café Philosophique, we can have so
much mental fun. There is no limit to what we might think, and every one of us,
and every thought we have is unique and almost infinitely improbable! Douglas
Adams always gets there first, we have indeed invented The
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Note:Dave Mitchell Scarthin Books, Cromford, www.scarthinbooks.com February 2008, revised November 2008
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