This is an introductory astronomy survey class that covers our understanding of the physical universe and its major constituents, including planetary systems, stars, galaxies, black holes, quasars, larger structures, and the universe as a whole.
Optical Telescopes (UV, Visible, IR)
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Del curso dictado por Caltech
The Evolving Universe
369 calificaciones
De la lección
Introduction and Some Basics
Conoce a los instructores
S. George DjorgovskiProfessor
Astronomy
So today we'll start talking about how do we actually measure stuff in astronomy.
The data of course basis of every science in astronomy that we get
data by observing, and that means we have to use a variety of telescopes.
So first, let's talk about telescopes and visible light.
Often people call them optical.
But the same thing applies for ultraviolet or most of the infrared.
Now Galileo did not invent the telescope.
There was some Dutch person, and
this is actually the first known drawing of a telescope from a book in 1609.
That pretty much what Galileo will figure out how to do.
So Galileo made first usable telescope,
and that was a refracting telescope using lenses,
what you usually think of as telescopes today.
And Newton came up with a reflecting telescope that uses curved mirrors
instead of curved glass to bend light rays, and
those are the telescopes that are most used today.
So if you look at the history of telescopes, they get bigger and
bigger, and the reason for that is that collecting area.
The bigger collecting area of your telescope, the more light you gather per
unit time, and therefore the fainter things you can see.
A human eye has pupil diameter, a few millimeters.
That doesn't give you much of a collecting area.
It's also not a great detector either.
But this is a log linear plot, so
you can see that the collecting area of telescopes kept increasing exponentially.
At first, they were all refractors, telescopes based on lenses.
But then reflectors start coming in, and for the past couple centuries at least,
that's pretty much the only astronomical telescopes that are really being used.
Some of the famous ones are noted here.
Hale is the 200 inch telescope of Mount Telomere from 1948,
it was superseded by the Soviet six meter, which has never
produced much science to begin with, which shows that size is not everything.
Hubble, which is one of the most productive if not the most productive
telescope in history, is not very big.
It's 2.4 meter diameter mirror.
But, as they say in real estate, it's location, location, location.
And state of the art today are the twin Keck 10 meter telescopes in Hawaii.
There is a very similar one in Canary Islands called Grantecan.
And the future telescopes are following same design.
The 30 meter telescope or TMT, which was built by Caltech, UC Canada,
China, India, and probably other partners.
So what are the issues that we worry about making telescopes?
First of all, those mirrors tend to be pretty massive.
And that has several different problems associated with it.
First, mechanical issues of moving the damn thing.
But then, they also bend under their own weight, and then finally,
things expand when the get warmer, shrink when their cooler, that changes the shape.
So, a lot of the skill or improvement in technology of making
telescopes was in making the mirrors lighter and easier to manipulate.
So first they started removing pieces of glass they didn't need.
And polymer mirror is like that.
I'll show you this in a moment.
Today there are like thin meniscus mirrors, and
then there are multiple segmented designs.
And there are also crazy ideas like spinning a dish full of liquid mercury.
And so, because of the spin it will assume parabolic shape surface and
you can use a telescope because it looks straight-up.
Mercury being toxic this is not always a good idea.
The important thing is that in order for a telescope to actually produce good quality
images, the deviations from the perfect figure, which is usually a parabola,
can't be any larger than about one tenth of the wavelength.
Now, think what that means.
For a, say, ten meter telescope in Hawaii.
That means the wavelengths are typically of the order of, well,
say visible light is 500 nanometers.
So the biggest bumps you can have are 50 nanometers.
50 nanometers, that's 5 times 10 to the minus 8th,
so divide that by 10, so it's 5 parts in a billion.
Now if the Keck telescope mirror was the size of the planet Earth,
what would be those biggest bumps that we can tolerate?
So diameter of planet Earth is, let's say, to first order, 12,000 kilometers.
Well, it's 12,000 kilometers, 12 million meters, and 12 billion millimeters.
So, 5 times 12, it's 60 millimeters.
So the biggest imperfections it can
tolerate would be of the order of three inches.
Where the whole primary size of the planet Earth.
This is how precise they have to be done.
Here is the mirror from polymer 200 inch, when it's still being made.
You're looking from the top is a perfectly smooth surface through which you look.
The weird stuff underneath are holes.
Cavities that were put there to remove the excess volume of the glass,
and then the top surface was polished with great precision.
That pretty much is the end of how big you can make them.
Eight meter mirrors are the biggest mirrors people make today.
And then they can support them with active optics.
A lot of little pistons pushing keeping the figure just right as the telescope
turns around.
And a completely different approach is segmented mirror design.
Instead of having single monolithic mirror to be your primary,
you chop it up in a whole lot of hexagonal pieces.
Well, you don't cut the mirror, you would build the pieces and
put them together, each of which is the appropriate segment of the parabola.
And then you have to control their position with similar accuracy to what I
told you earlier.
So this how the two Keck telescopes were built, and
this is a design that's now being copied elsewhere, including
the next generation of space telescopes, because it's a very clever idea.
The person who developed this idea was Jerry Nelson.
He was a Caltech undergrad, so we expect
every one of you to come up with equal revolutionary idea, [INAUDIBLE] astronomy.
Where are we going in the future?
There are telescopes that look individual targets or small fields really deep,
but also there are telescopes that sweep large areas and do sky surveys.
The pre-eminent of those now under design is the large synoptic survey telescope or
LSST, and it has the strange design.
Usually if you want wide field, just some tricks in optics you have to play.
So even though it's 8.4 meter diameter, it's really equivalent
of 6.5 meter because of all these holes in it and so on.
And the idea is that that telescope will survey the sky.
It will be based in Chile, and it will produce 30 TB every night.
It will essentially produce one long sky survey every week, more or less.
And people select targets from their bigger telescopes.
An example of the next generation big telescopes is the 30 meter telescope
that's being developed here at the University of California,
and with all these other partners.
And it's essentially a gigantic Keck.
But Kecks have 36 segments, each of which is about size of a person.
This one has 738 segments, a little smaller.
And they all still have to be adjusted in a very precise fashion.
The competition for a 30-meter telescope is so-called the Giant Magellan Telescope.
Which is built by our friends over at Carnegie Observatories across the freeway,
in Arizona, and they think they can do this with a small number of large mirrors,
8 meter class mirrors.
They'll probably work just fine, and we'll see who gets to build one first.
These toys get to be very expensive.
The price tag of one of these is over a billion dollars now.
And they'll probably take upward of $50 million per year to operate.
Put this in a context, Keck telescopes are roughly $100 million a piece and
they cost about $23 million per year to operate, two of them.
So, astronomy is really a big science today.
And Europeans are planning European Southern Observatory, ESO, or
European Extremely Large Telescope.
They're just very unimaginative coming up with these names.
They're called VLT, Very Large Telescope.
[INAUDIBLE] They have now.
So Extremely Large Telescope.
And it has to be bigger than the American one, so this is why it's 40.
I predict it's going to be a 31 meter by the time they're done.
Now there are problems in doing astronomy from the ground.
Obviously the weather is an issue.
This is why people go to things like really dry deserts in Chile and so on.
But also this, this is actual composite when there are no clouds of United States.
Taken from the orbit and you can see exactly where the people live and
where the roads are.
So you want to go to places that are really dark.
The big bright splotch on the lower left is of course Southern California,
Los Angeles.
Clearly not a good place to do astronomy.
But somewhere in the kind of dark part next to it is Mt Palomar.
And you can barely see Baja peninsula below.
And there is a really excellent Mexican observatory there, San Pedro Marten.
So this planet is good for many things, but it's actually not all of a great
place to do astronomy because of the presence of atmosphere.
Things like oxygen, and water vapor,
and so on, which is why we send telescopes in space.
So this is Hubble Space Telescope, which is up there since 1990.
It's still going strong, and
it's truly revolutionized astronomy even though the size is not large.
The absence of atmosphere, which removes all the turbulence essentially and
also ability to go to ultraviolet that doesn't go through its atmosphere.
That's what makes Hubble so successful.
Currently under construction is the next generation of space telescope called
the James Webb Space Telescope, or JWST, which is six and
half meter diameter, which you can see is just like KECK.
It's one of the segmented designs.
The strange contraption, in which it sits, is a thermal shield, and
there are solar panels on the back and
the idea is that this telescope would not be in Earth's orbit.
It would actually be in a Lagrange point behind the Earth.
So that Earth will be shielding it in part from sunlight, and
we'll be observing from there.
Now, problem with this is,
that once you send it to Lagrange orbit, there is no fixing it.
All right.
Hubble's been serviced many times, very well.
It'll be a problem to service something like this.
So, it's gonna work perfectly the first time.
And it will be optimized for near infrared.
We also go to space to observe wavelengths that don't go through Earth's atmosphere,
like much of the thermal infrared, and the Pasadena, Caltech, and
JPL are leaders in this game.
This is picture of a Spitzer space telescope,
one of NASA's great observatories, which is run out of that building,
and it's been producing fantastic sciences still going on.
The one on the right is GALEX for
Galaxy Evolution Explorer, which was the ultraviolet observatory.
Also run out of here from this building by Chris Martin and his team.
And that really We have surveyed sky in ultraviolet better than has ever done.
Now that telescope has run out, run the course of its life.
There have been many, many good missions that observed
sky in variety of wavelengths that don't go through Earth's atmosphere.
We'll talk a little bit about some of the high energy ones in a bit.
So, questions about this?
Yes, please.
>> [INAUDIBLE]
>> I'm sorry, the question is, why do you spend so
much money on ground based telescopes when it's better to go to space?
>> [INAUDIBLE] >> Well,
space telescope cost lot more than ground-based telescopes.
To launch one of these things is probably a cool billion dollars right there.
Just for rocket, for space shuttle.
To develop it is probably a few times that much.
I don't know what price tag on Hubble is by now, but
it's certainly upward of ten billion dollars.
I think the construction tab for James Web would be of the same order, maybe more.
So things are always much more expensive in space.
You go to space only if you really cannot do it any other way.
Such as Earth's atmosphere absorbing stuff.
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