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Showing posts with label venus atmosphere. Show all posts
Showing posts with label venus atmosphere. Show all posts

Saturday, October 23, 2010

Leslie's Probability

Leslie’s intuitions about probability seem to be of a kind with the case of the double lottery winner. Suppose that you buy lottery tickets for Tuesday and Friday. There are on both occasions ten million possible numbers, so your chances of winning on Tuesday or Friday are each one in ten million. And now suppose that you win on Tuesday. What are your chances that you will win on Friday also? Most people will feel that the chances of winning on Friday after having won on Tuesday must be far less than your chances when you won on Tuesday: one in ten million times ten million (1/1014). But this is a mistake. It is one thing to ask, what are your chances that you will win in both Tuesday and Friday? The answer is: 1/1014. It is another thing to ask, what are the chances that you will win on Friday after winning on Tuesday? Well, you have one ticket and there are 10 million possible numbers. So your chances should be one in ten million (107). But people like Leslie find this hard to accept. They think that there is something valid about the intuition that tells us that after winning the lottery once, the chances of winning it again have to be far smaller than they were the first time. The difficulty comes from thinking, in this case, that if you won on Tuesday, to win again on Friday really means that you will have won on both Tuesday and Friday and that should have an extremely small probability (even compared to the small probability of winning one lottery to begin with).

To dispel this intuition, let us look at one example in which the closer we get to an unlikely combined result, the greater its probability. Suppose you flip a fair coin a hundred times. What are the chances that you will get a hundred heads? 1/2100. That is an extremely small number. Suppose now that on the first flip of the coin you get heads. What are the chances now that you will get 100 heads? There are 99 flips left. That means that you will have to get heads on all 99. Your chances then will be 1/299. That is a very small number, too, but it is twice as large as the number you had before (because the denominator, 299, is half of 2100: 2x299 is 2100). After getting 2 heads, your chances of getting 100 heads will be 1/298, which is a very small number, but twice as large as that of your second flip and 4 times as large as your first’s. The more heads you get, the closer you get to getting 100 heads, the more your chances improve of getting 100 heads. Suppose you have flipped 98 heads, so you have only two flips left. Your chances will be 1/22=1/4. You have gotten 99 heads? Your chances of getting 100 heads depend on your getting heads on your last try. That is 1/2.

Of course, the chances of getting 99 heads and one tail will at that point also be 1/2. At the start, there were 2100 possible combinations; getting 100 heads was just one of them (1/2100). But once you got heads on your first try, you eliminated half the possible combinations, that is 299 hitherto possible combinations. Check it: 299 + 299 = 2100. For an easier example: 22 + 22 = 23 (4 + 4 = 8) and 23 + 23 = 24 (8 + 8 = 16). If your base were 3, then you would have to add three numbers: 32 + 32 + 32 = 33 (9 + 9 + 9 = 27). If your base were 4 you would have to add four numbers, and so on. Now, when you get your second head in a row, you eliminate half of the existing possible combinations left up to that point, that is, you eliminate 298 additional possible combinations. And so on: every time you get heads, you eliminate half of the possible combinations still in existence up to that flipping of the coin. Until, finally, when you only have one flip to go, there are only two possible combinations left. The first will give you 99 heads and then tails. The second will give you100 heads as the result of getting heads on your last flip. Both combinations are equally probable. Therefore, your chances of getting 100 heads when you have already gotten 99 are far greater than when you first got a head, while the chances of getting a head on your last flip are exactly the same as the chances of getting a head on your first flip: 1/2.

Let us remember this reasoning when we begin to think about the probability that life could evolve from inorganic materials.

Thursday, October 14, 2010

Venus and the End of the World

Chapter 4M

Venus and the End of the World

Before concluding the discussion on these aspects of comparative planetology on too happy a note, I should mention that the hypothesis that Venus once had oceans, as appealing and reasonable as it may be, is by no means universally accepted. For it depends crucially on the plausible reading of the ratio of deuterium to common hydrogen as evidence that Venus has lost a substantial amount of water. But this is not the only possible reading.

Some scientists have argued that the same ratio of deuterium to hydrogen could be caused by a continuous re-supply of water to the atmosphere of Venus. They find this hypothesis more plausible because, at the present rate of escape, water would disappear from Venus altogether in a few hundred million years. This would mean that right now we are witnessing the very end of a long process. Most of us would not be bothered by this prospect, but some people feel that we should treat with suspicion all lucky coincidences in science. Imagine, Grinspoon tells us, that

You show up at a house where no one seems to have been home for a long time, but you hear water running. You go upstairs and find a vigorously draining bathtub which has only an inch of water in it. Now, it is possible that you showed up just as the last bit of water was running out -- but isn’t it more likely that the tap has been left running?[1]

The intuition behind this reasoning is a peculiar view of probability that sounds quite reasonable at first. Suppose that an urn contains two white balls and 98 black balls, while another contains two white balls and 9998 black balls. Without knowing which urn is which, you reach into one of them and come up with a white ball. You should conclude that in all probability you have reached into the smaller urn, for the chances of getting a white ball are two in a hundred, which are much higher than the two in ten thousand that you would find in the larger urn. It is not reasonable to believe that you have reached into the larger urn, since getting a white ball out of it is so much more unlikely.

These intuitions about probability come with their own problems, however. The first problem is that it turns scientific reasoning on its head. In the case of Venus, it leads us to expect that the amount of water we find is normal (that it has been like that for a long time). It leads us to assume that things are pretty much as we find them (a steady-state) because otherwise the situation would be very unusual and thus unlikely.

Notice how differently we reason in science. When we first observe any phenomenon, we take pains to determine whether our sample is representative. The history of science is littered with ideas that seemed promising but went nowhere because they were based on the assumption that we were looking at the normal state of things (this is the fallacy of induction). That is, normally we have to demonstrate that our sample of observations indeed represents the usual state of affairs. We are not allowed to take that for granted. Otherwise we may conclude, say, that we have discovered a new branch of the homo family based on one fossil with a peculiar skeleton, only to find out much later that it was the skeleton of an individual with a bone disease (a true case). We worry about whether the Viking and Venera landers ended up in representative locations in Mars and Venus, whether the Galileo probe went into a section of Jupiter that is like the rest of the atmosphere (it didn’t). Nature is rich and what we come to observe may actually be as unusual as flowers, birds, and bees are in the solar system: they exist in only one world – Earth – out of the many that orbit the sun.

The kind of reasoning that leads to a steady-state view of water in Venus also leads to some very strange views when applied elsewhere. John Leslie, for example, has concluded in The End of the World that the human species is likely to become extinct very soon.[2] He reasons that if the human species were to live for a long time, let’s say millions of years, then the amount of people alive today would be an insignificant percentage of the total amount of human beings that will ever be alive. Thus, he thinks, belonging to such an unusual group of humans (those of today) would be extremely unlikely. On the other hand, if the world were to end within fifty years or so, we would be part of the largest group of humans who will ever be alive (the six billion or so alive today are far more than all the rest of the humans who have ever lived put together). And it is more likely, then, that if you were to pick a human at random he would belong to the overwhelming majority than to a very small minority. Therefore the human species is far more likely than not to become extinct very soon.

Many sensible people would consider Leslie’s argument a reductio ad absurdum of the kind of probabilistic reasoning under examination here. Nevertheless, he, like others, sticks to his probabilistic intuitions, despite counterarguments like the following. Suppose the devil places ten people in a room and tells them that he will kill them all if he gets double sixes in a roll of the dice. If they survive, he will then place 100 people in the room, and then 1,000, and so on, always multiplying by ten. And every time the devil will roll the dice in hopes of getting a double six. Now, most of us will think that the chances of any one group getting killed will be 1 in 36, but according to Leslie, the ill-fated chances of the group of ten thousand have to be far greater than those of the group of ten. Leslie concludes not that there is something very wrong with his reasoning, but that he has encountered a paradox of probability. And he remains worried about the end of humanity, just in case the paradox should resolve itself in the direction of his reasoning.

There is no paradox, however. The probability estimate that takes into account a causal mechanism has priority (in this case, that the devil will kill all the people in the room if he rolls double sixes), as do all probability estimates that clearly have more relevance. For example, suppose that an ordinary man goes to the hospital to have an appendectomy. He is informed by his doctors that the chances that the operation will go well are 98%, for their survey shows that that 98 out of every 100 patients who undergo the operation do well. But suppose now that the patient is 89 years old and suffering from cancer and its debilitating effects. Surely the previous estimate would not apply to him. Let’s say, for the sake of argument, that statistical records have been kept for people in his condition and that people in his condition survive less than 5% of the time. This latter estimate is the one that should guide his decision to undergo the operation, for it is based on the factors most relevant to him. It would be preposterous of him to say, “But my chances might still be 98%.”

It may turn out that the amount of water of Venus in a steady state, but to have confidence in that idea we need independent scientific reasons in its favor, not peculiar intuitions about probability. A candidate to keep the Venusian atmosphere re-supplied with water is volcanism. A good possible outside source of water is the combination of comets and their fragments, for they are basically a mixture of ice water and other compounds. As Grinspoon points out, however, comets collide with planets often but not continuously and, thus, we would not know whether that hypothesis is consistent with our present readings of Venusian water (comets would supply water in spurts). Furthermore, this approach needs to assume that the exceptionally large ratio of deuterium to hydrogen would exist in Venus for any given short period of time. Otherwise we would have to conclude again that Venus has been losing water for a long time. Now, some scientists say that in first coming up with the “oceans in Venus” hypothesis we assume the original Venusian deuterium-to-hydrogen ratio should be close to Earth’s, but that this assumption may be incorrect: after all, they are different planets. This point is fine as far as it goes. But the ratio is 120 times greater on Venus than on Earth! It is difficult to imagine what could account for such a phenomenal difference in natural ratios between the two planets. The original ocean hypothesis must continue to be considered most reasonable until further notice.

This proliferation of ideas is by no means restricted to planetary geologies. But perhaps we can see this point better by discussing several illustrations in connection with another point, namely that the variety we find in the solar system permits us to test our ideas of the Earth.



[1]. D.H. Grinspoon, op. cit., p. 109.

[2]. J. Leslie, The End of the World, Routledge, 1996. Leslie believes that this statistical reasoning should make us more fearful of possible cosmic cataclysms, such as giant asteroid impacts and space-time-gobbling new universes growing inside our universe, as well as man-made catastrophes such as nuclear war.

Monday, June 28, 2010

Comparative Planetology and Serendipity

Chapter 4A

Comparative Planetology and Serendipity


Science fiction gave us forests on the back side of the Moon, Martian canals constructed by advanced civilizations, and, in Venus, a throwback to happy early times: paradise. Unfortunately the Moon is lifeless, Mars is a desert, and Venus is hell. As our knowledge of the solar system has advanced, we have moved our imagination beyond its confines. The worlds of strange intelligent creatures and monstrous beasts, of great wisdom or unparalleled horror might well exist – but around some distant star, safe from the rocket probes that might render empty what fiction has filled with the riches of dreams.

A social critic may wish to know why we should then want to explore the inhospitable worlds within our rockets’ reach. Can there be, for example, any link between the exploration of Venus' poisonous atmosphere and the well being of those who breathe our own atmosphere?

There is. There are many in fact. Let me begin with one striking and important example of the serendipity of comparative planetology: the discovery of the threat to the ozone layer.


Ozone forms when oxygen molecules (O2) capture oxygen atoms (O) to combine into larger molecules, ozone (O3). Ozone acts as a nasty pollutant on the surface, particularly in the air of our large cities, but at high altitudes it absorbs ultraviolet radiation and reduces considerably the amount that penetrates the atmosphere. Thus the ozone layer protects plants and animals on the surface from excessive ultraviolet radiation that would damage their DNA and cause widespread cancer. Indeed, life was confined to the oceans for much of the history of our planet, until the level of atmospheric oxygen grew enough to form a substantial ozone layer.

Now to Venus. When NASA scientists found fluorine and chlorine compounds in the atmosphere of Venus, they investigated the chemistry of those molecules and determined the rate constants of their chemical reactions. Those rate constants were later used by Sherwood Roland and Mario Molina to discover that chlorofluorocarbons (CFCs) destroy ozone in the presence of high ultraviolet radiation. That is, they discovered that the Earth’s ozone layer might be in trouble. This discovery came as a shock to many researchers and industrialists, for CFCs had been developed precisely because they were supposed to be inert and thus, since they could not react with anything, they could not harm anything. They seemed just perfect for use in air conditioners, refrigerators, and aerosol deodorant cans.

Unfortunately, high in the atmosphere, ultraviolet radiation breaks up the CFC molecules, and the freed chlorine atoms interact with the ozone, destroying it. This discovery was confirmed by Michael McElroy, whose group had the required tools because, as Carl Sagan pointed out, they were working on the chlorine and fluorine chemistry of the atmosphere of Venus.[1]


The presence of a large hole in the ozone layer over Antarctica was further confirmed by satellite data and later tracked and made vivid and dramatic by satellite pictures. This prompted scientists, industrialists, and governments, acting in concert, to ban CFCs, so as to significantly reduce the threat by the year 2010 (although it will take some forty or fifty years longer for the CFCs already in the atmosphere to dissipate and the ozone layer over Antarctica to recover).

This example is a beautiful illustration of the serendipity of comparative planetology. By investigating the atmosphere of Venus we transform our knowledge of planetary atmospheres; this knowledge makes us aware of a serious problem; and space technology helps us monitor the problem and provides the information needed to achieve a solution. And eventually we put the solution to the problem into effect.

Such is the link we seek between planetary science and the well being of humankind: we need to explore the solar system in order to improve our views about the Earth. And we need to improve those views so that we may deal more wisely with certain social and environmental problems that could become acute in a few decades or outright disasters in the long run.

My aim is to show that the serendipity of exploring the solar system will pay off here on Earth. In support of that conclusion I will advance the following argument. To have a good grasp of global problems and their possibly serious consequences, we need to understand our global environment. But to understand the global environment of the Earth it is important to understand the Earth as a planet. To understand the Earth as a planet, however, it is necessary to study the other members of the solar system. And, of course, to study the solar system well we need to go into space.



[1]. Sagan, C., Pale Blue Dot, Random House, 1994, p. 222. I have adapted this section so far from Sagans book.