Learn about the origin and evolution of life and the search for life beyond the Earth.

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來自 The University of Edinburgh 的課程

天体生物学和寻找外星生命

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Learn about the origin and evolution of life and the search for life beyond the Earth.

從本節課中

Extraterrestrial Intelligence

What are the possibilities for intelligent life elsewhere? How would we deal with contact with an extraterrestrial intelligence and what would be the impact on society? Who would represent Earth?

- Charles CockellProfessor

Astrobiology

One of the most enduring questions in astrobiology is there anyone

out there by anyone, that means extraterrestrial intelligence.

Could we find another intelligence civilization in the galaxy or

in the universe at large?

Well, one of the first people to really think about this and

apply these ideas was Frank Drake.

The American astronomer and astrophysicist,

a pioneer in the search for extra-terrestrial intelligence.

In 1961 he wrote down an equation that's become rather famous and

has now become known as the Drake Equation, to try and estimate the number

of communicative civilizations there might be in the universe.

Of course, one of the first things we have to do is define what a civilisation is and

there are number of ways that we might do that.

We might define a civilisation as a group of organisms that

have built certain technology.

Maybe they have built cities or something else, but of course, if we're going to

detect an intelligent civilisation, they need to be transmitting signals to us.

So from an operative point of view we might simply define an intelligent

civilization as a civilization that is able to communicate with us, for example,

using radio waves.

The Drake Equation is about trying to estimate the number of communicative

civilizations.

What are the terms of this equation?

This is the Drake Equation and it's made up of a number of factors.

We have to estimate values for those factors to be able to put them together to

estimate the total number of communicative civilizations in our galaxy,

or perhaps in the universe.

The first term, R,

is the rate of formation of suitable stars, suitable stars for life.

We know the G star is suitable for life, because our own star is a G type star.

There might be other stars that are also suitable for planets with intelligent

life, for example N stars, but at the moment we don't really know enough

about the types of stars that can give rise to intelligences on a planet.

But we need to work out the rate of formation suitable stars to be able

to put that term into the equation, so that's clearly one forthcoming challenge.

Astropologist.

The next time is the fraction of these stars with planets.

A few decades ago this was pure speculation,

we just to know of planets around other stars.

Now with an increasing quantity of data about planets orbiting distant stars we

can begin to get more accurate estimate of the number of stars that actually host

planets.

So we can begin to put some estimate on this term in the equation FP.

Once we know that,

we then have to know the number of Earth-like worlds per planetary system.

And again the moment we don't know exactly what this number is, but

as we increase the search for Earth-like planets and by that I mean.

Rocky terrestrial type planets that could host liquid water and even biology.

Then we can start to put that number into the equation.

The search for extra sort of planets around other stars and

particularly the recent search for

Earth-like planets around other stars is bringing us closer to a time well,

we can actually estimate a number that could go into the Drake equation.

Once we have that number,

we then need to work out the fraction of these planets where life develops.

We just don't know enough about the origin of life, what conditions are required for

the origin of life to be able to workout the fraction of

planets that are habitable, that do actually give rise to life.

And this again is a challenge for astrobiologists to work out

what really were the conditions for the origin of life.

How likely or inevitable is it that these conditions will be met

on other planets that are habitable.

And so what fraction of planets will inevitably give rise to life.

That's another term we don't have an accurate number for but

we would need in order to be able to work out the solution to this Drake equation.

Once we know the number or

fraction of planets where there's life, we don't need to be able to work out

a fraction of those planet where intelligent life evolves and develops.

And again at the moment, that's entirely speculation.

We don't even know whether there are other planets in our galaxy or

in the universe that have life.

Left alone whether they have intelligent life.

But if we were to be able to work that out,

if we were to be able to look at enough earth like planets around other stars,

assess them for their potential for life and assess whether they could support

intelligent life we could then move onto the next term in the Drake equation

which is the fraction of those planets that are communicating.

And the only way that we can really work that out is to try and

pick up signals from other planets where there are intelligent civilizations

that are communicating.

And then finally,

the last term in this equation is the lifetime of communicating civilizations.

This is a term that constrains the total number of civilizations

that are attempting to communicate by taking into account the fact

that these civilizations might have finite lifetimes.

Civilizations might destroy themselves.

For other biological or technological reasons,

they may come to an end after a certain length of time.

We would need to take that into account to work out the total number of communicative

civilizations.

So this Drake equation contains sometimes that we can be more accurate about, for

example the fraction of stars that have planets.

Sometimes we really don't know anything about the current time

such as the number of habitual worlds that give rise to intelligent life.

But the Drake Equation is a very interesting way of thinking about

astropology.

It's a very interesting way of ordering our thoughts.

And ultimately it's the equation that we will need to be able to estimate

a value for in order to be able to know whether the search for

extra-terrestrial intelligence is an initiative that's worth undertaking.

When Frank Drake first came up with this equation,

he estimated that there are 10,000 communicative civilizations in our galaxy,

based on the numbers that were known then.

Of course,

trying to come up with more accurate numbers is a very difficult thing to do.

But astrobiologists need to use the Drake Equation to try and formulate a more

accurate assessment of the number of communicative civilizations in the galaxy.

Given the number of planets that have been observed around other stars.

And the numbers of Earth-like planets that are beginning to be detected around other

stars, we might expect that this number will change possibly even upwards

over the coming decades.

Although, again, we still don't know even if there are many Earth-like planets in

the galaxy, how many of those might support intelligence.

So what have we learned?

Well, we've learned of course we don't know whether there is anyone out there.

But by coming up with this equation,

the Drake equation, we have some sort of method of trying to quantify or

estimate the numbers of communicative civilizations in the galaxy.

The equation depends upon many factors,

many factors that depend upon the formation of planets around the stars,

the formation of habitable conditions on those planets and

the emergence of life eventually intelligent life.

Frank Drake first attempted to come up with the value that results in

this equation here estimated 10,000 communicative civilizations in the galaxy.

This equation is a very good way of underpinning our search for

extraterrestrial intelligence and try to find out where the search for

extraterrestrial intelligence fits in with astrobiology.