Kurt Vonnegut said it all in Sirens of Titan.

Or maybe we are part of a galactic (or inter-galactic) double blind study.

arthur



-----Original Message-----
From: Keith Hudson [mailto:[EMAIL PROTECTED]
Sent: Monday, July 14, 2003 12:04 PM
To: [EMAIL PROTECTED]
Subject: [Futurework] Life from Mars?


Some FWers might be interested in an article fom this week's New Scientist:

<<<<
BORN LUCKY

Against all the odds, life establoished itself remarkably quickly on earth. 
Does this tgell us anything about where it began? Yes, says theoretical 
physicist Paul Davies, and the answer is out of this world.

Paul Davies

It's a shame that there are precious few hard facts when it comes to the 
origin of life. We have a rough idea when it began on Earth, and some 
interesting theories about where, but the how part has everybody stumped. 
Nobody knows how a mixture of lifeless chemicals spontaneously organised 
themselves into the first living cell. It may have been a straightforward 
sequence of unexceptional chemical processes, or a bizarre accident. The 
chief bugbear is that we have just the one sample of life to study -- Earth 
life. And the mere existence of life on Earth tells us nothing at all about 
how likely or unlikely it is, or whether it has happened elsewhere.

The great hope for astrobiologists is that another sample of life will be 
discovered somewhere beyond Earth, giving us a crucial comparison. But 
while we wait, there is one key fact about life on Earth that does provide 
us with an important data point, a fact that could tell us something about 
where it all began. This is the often-discussed fact that life started up 
with almost suspicious haste.

Following the birth of the solar system 4.55 billion years ago, the planets 
were pounded mercilessly by huge asteroids and comets. It is believed that 
around this time a horrendous cataclysm occurred when a rock the size of 
Mars slammed into Earth, creating the moon. This would have melted the 
planet and left the surface roasting hot for tens of millions of years. 
Even smaller impacts would have caused mayhem by swathing the globe in 
incandescent rock vapour, creating a searing heat blanket that would have 
boiled the oceans dry and sterilised the rock deep into the crust. The 
record of impact craters on the moon suggests that this hellish barrage 
began to abate only about 3.8 billion years ago.

 From the record of the rocks, most palaeobiologists are convinced that 
microbial life was flourishing on our planet as long as 3.5 billion years 
ago. Fossils from the Pilbara region of Western Australia imply that 
colonies of fairly sophisticated bacteria were already hard at work. The 
Pilbara fossils remain the oldest clear traces of life on Earth, but 
presumably there would have been an extended phase of evolution preceding 
this. Studies of carbon isotopes in Greenland rocks dating as far back as 
3.85 billion years have hinted at still earlier traces of life, though the 
evidence for this is hotly contested.

While the fossil hunters continue to follow the tenuous thread of life on 
Earth further and further back in time, it is already clear that life 
established itself almost as soon as the cosmic bombardment tailed off. Can 
this simple fact tell us anything about the origin of life?

Many scientists believe it can. The late Carl Sagan cited the rapidity of 
life's appearance as evidence that it must be easy to make, and might 
therefore be expected to arise on many other planets in the galaxy. The 
argument seems intuitively correct, but how much can be inferred from a 
single sample? Statistically speaking, the thorniest problem is that we 
haven't a clue what the probability is of life forming from scratch on a 
planet like ours. So we can't use this single example to infer whether life 
was inevitable or a sheer fluke.

We can, however, use it to turn hand-waving arguments into probabilities. 
Last year Charles Lineweaver and Tamara Davis of the University of New 
South Wales applied a statistical analysis to the problem (Astrobiology, 
vol 2, p293, 2002). Their argument is best explained by analogy with 
winning a lottery -- with life being the jackpot. In most lotteries punters 
have a good idea of what their chances of winning might be. But suppose a 
gambler enters some weekly lottery with no idea at all of the odds. If the 
gambler won the prize after, say, three weeks, what would he infer? He 
might have just got lucky and won a million-to-one prize on the third 
attempt. But most people would infer that the odds were very much lower -- 
closer to 1in 3 than 1 in1million.

If we assume that planet Earth could have spawned life at any time between, 
say, 3.9 billion years ago and today, then it gives us pause for thought 
that the great lottery called Life was won in just a few hundred million 
years -- maybe less. Using a refined version of the gambler's argument, 
Lineweaver and Davis conclude that there is at least a 13 per cent 
probability that life will form at some stage on a planet where the 
requisite conditions for life to arise have existed for at least one 
billion years. Of course, the authors are quick to point out this does not 
guarantee the galaxy will be teeming with life, because we still don't know 
how "Earth-like" another planet might need to be for it to lie in the same 
reference class as Earth for such statistical reasoning. But their work at 
least quantifies what many scientists have long claimed in a somewhat vague 
way.

Something else needs to be taken into account. The factors that determine 
how long life takes to get going on an Earth-like planet will depend on 
unknown details of physics and chemistry, for example how long it will be 
before certain rare but crucial molecules form by chance in a primordial 
soup. On the other hand, the factors that determine how long a planet 
remains congenial for life will be determined by completely different 
aspects of science, such as the life expectancy of stars, which depends in 
turn on gravitation and nuclear physics. Because there is no physical 
connection between these two timescales, it would be an unlikely 
coincidence if they happened to be about the same. Therefore, it seems 
reasonable to believe that life will either form much faster or much slower 
than typical stars take to burn up most of their fuel (between 5 and 10 
billion years).

Most biologists are conservative on the matter and opt for the latter: the 
molecules of life are hard to form by chance, and on average would take 
very much longer to arise than the window of opportunity of several billion 
years during which an Earth-like planet would be able to sustain life. It 
happened on Earth by a fluke, they say. But why did it happen so quickly? 
After all, life could have taken another billion years to get going, and 
there would still be time for scientists to evolve and squabble over the 
subject before the sun turns into a red giant. One response is to shrug 
this detail aside. If the chances of life starting on Earth at some stage 
are, say, a mere trillion to one, then the chances of it starting as soon 
as it did might be ten trillion to one. So what? It is practically a 
miracle anyway, and one might as well be hanged for a sheep as for a lamb.

But this would be too hasty. It is still possible to draw an interesting 
conclusion from Lineweaver and Davis's analysis, even if life is a fluke 
and unlikely to emerge more than once in the observable universe. In common 
with most researchers, Lineweaver and Davis assume that life arose on Earth 
from scratch. But there is a contending explanation for why life got going 
so fast: perhaps it did not originate here at all. Maybe it came from 
somewhere else in the universe. If the early asteroid-battered Earth were 
subjected to a continual influx of extraterrestrial organisms, it would be 
no surprise if life colonised our planet pretty much as soon as conditions 
became favourable.

The theory that life came to Earth from space is far from new. It was much 
discussed in the i9th century, and became the subject of a book published 
in 1906 by the Swedish chemist Svante Arrhenius, who called the idea 
"panspermia" meaning "seeds everywhere". Arrhenius had in mind swarms of 
bacteria wafting naked across the galaxy, propelled by the pressure of 
starlight. Nowadays panspermia is not much favoured by astrobiologists, 
with the notable exception of Chandra Wickramasinghe at the University of 
Wales. The main problem with the theory is the high levels of radiation in 
space, which would prove lethal to all known microorganisms in fairly short 
order.

But another scenario circumvents the radiation hazard. It was first mooted 
in rather vague terms in 1871 by the physicist Lord Kelvin, and is now 
receiving increasing support among scientists. It goes like this. The same 
bombardment that threatened early life also blasted vast quantities of rock 
into space from the surfaces of numerous planets. Some of this debris would 
have eventually hit the Earth. If another planet in the solar system had 
already spawned life, then microbes cocooned inside these ejected rocks, 
shielded from the radiation, could have made the journey unscathed.

If life did arrive here inside a meteorite, where did it come from? The 
prime candidate is Mars. A couple of dozen Martian rocks have been 
identified on Earth and many more must be lying around undetected. It has 
been estimated that an average of one Martian rock a month falls to Earth. 
And Mars fits the bill when it comes to the cradle of life, too. Although a 
freeze-dried desert today, the Red Planet was once warm and wet, possessing 
a thick atmosphere, liquid water and active volcanism. Being a smaller 
planet, it cooled quicker than Earth and could have been ready for life at 
least half a billion years earlier. The first life forms may have cowered 
deep in the crust, which would have afforded a measure of protection 
against the bombardment. This subsurface zone on Mars may have cooled 
enough to host life as long ago as 4.5 billion years, while Earth's crust 
still sizzled.

The implications for the statistical argument are striking. If Mars had a 
"window of opportunity" several times longer than Earth's in the period 
prior to life's first known appearance, the chances of life starting there 
rather than here are correspondingly higher. But it goes much deeper that 
that. The size of the "Mars advantage" hinges not just on the longer window 
of opportunity that the Red Planet enjoyed. It also depends on the number 
of difficult steps involved in generating life.

If a single very improbable event -- such as the spontaneous assembly of a 
lucky combination of key molecules -- sparked life, then it is about five 
times as likely that life started on Mars and came here in a meteorite as 
the orthodox terrestrial alternative. But if more than one very unlikely 
step is involved in getting life started, things get seriously interesting. 
If life required three unlikely molecular combinations -- say, one to make 
long strands of nucleic acid, another to make certain proteins, and another 
to make the right sort of cellular structure -- that would make a Martian 
origin 125 times as likely; a 99 per cent probability that it happened on 
Mars and not on Earth. More steps than that and the odds favouring Mars 
become overwhelming.

There is of course another possibility: that life came from outside the 
solar system altogether. After all, the Earth is only about a third as old 
as the universe -- there may have been Earth-like planets in the galaxy 
billions of years before the solar system formed. In the run-up to the 
period when life is known definitely to have existed here on Earth, life 
would have had much longer to arise on these planets than it would on Mars.

But against this advantage of a longer window of opportunity must be set 
the much slimmer chance that such extra-solar life could traverse the many 
light years of interstellar space needed to bring it to the solar system. 
Jay Melosh of the University of Arizona and his colleagues have studied the 
fate of rocky ejecta both within and between star systems, and they doubt 
that a single interstellar rock has ever hit Earth throughout its entire 
history. Unless the origin of life required several exceedingly unlikely 
steps -- thus amplifying the relative advantage of a longer window of 
opportunity -- Mars remains the best bet for being the cradle of life.

What supporting evidence can we find? Perhaps we can invoke the emergence 
of human beings -- the product of a long sequence of events, starting with 
biogenesis and extending through many evolutionary steps tc intelligence. 
The economist and philosopher Richard Hanson from George Mason University 
in Virginia, elaborating on an argument first used 20 years ago by the 
physicist Brandon Carter of the Meudon Observatory in Paris, has shown 
that, if a sequence of steps -- some relatively easy, some hard -- are 
needed to attain a certain goal in a fixed length of time, then the 
expected time left over when the last step has been successfully completed 
is roughly the same as the time taken by the hardest step in the total 
sequence.

If it is true that the first step towards our emergence -- the origin of 
life -- is the hardest, taking on average much longer than the age of the 
Earth, then Hanson's argument suggests its flukey occurrence took roughly 
as long as the remaining time left. Astronomers reckon the sun will become 
too hot for life on Earth in about another billion years, so that suggests 
life took about a billion years to form -- a figure implausibly long for 
the Earth, but much closer to the few hundred million years during which 
Mars would have been a suitable incubator before life appeared here.

None of this tells us anything about how life began, only that if the 
process was hard -- as many biologists say it was -- it probably came from 
Mars, and if it was easy it should have formed spontaneously on both Earth 
and Mars at some stage. And of course statistical reasoning is no 
substitute for hard facts. The clincher will come if a future mission to 
Mars provides unambiguous evidence for terrestrial-type life there before 
it existed here. Other hard facts closer to home would also help: a Martian 
provenance of life would be greatly strengthened if Earth's known window of 
opportunity were to become sharply narrowed, for example as a result of a 
clear sign of life at work here 3.9 billion years ago coupled with 
confirmation of the hostility of the early bombardment. But in the absence 
of any more reliable data about life on Earth, Mars or beyond, statistical 
reasoning is about all we have to go on. And, for the moment, the odds make 
it a racing certainty that we are all descended from Martians.

New Scientist 12 July 2003

Paul Davies is a theoretical physicist in the Australian Centre 
forAstrobiology at Macquarie University, Sydney. His 1999 book, The Fifth 
Miracle, has been reissued by Penguin as The Origin of Life.
 >>>>


Keith Hudson, 6 Upper Camden Place, Bath, England

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