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The James Webb Space Telescope is a reflecting telescope,
which means it images of the universe
with the help of mirrors.
We are here at L3-IOS-Tinsley in Richmond,
California to find out just how the observatory will work.
So I'd like to first show you one of our primary mirror
segments.
And before we get too close, we'll
want to put our mask on to protect the optical surface.
OK.
This is one of our 18 primary mirror segments.
Once they're all complete, they'll
combine to make one large, primary mirror.
You can see the front side surfaces highly polished.
And as we rotate to the backside surface,
you'll see that there is a honeycomb light
weighting so it reduces the payload when it goes up
into space.
And yet, it's very stiff.
It looks like you can attach things to it too.
Yes, they bond more hardware on the backside surface,
which makes it an even stronger structure.
And that's the way it'll go up in the space.
There are several other mirrors that we're doing here
for James Webb Space Telescope.
We have a secondary mirror element.
We have a tertiary mirror element.
And we're also doing the fine-steering mirror.
For those of us who don't understand
how a telescope works, why do you have so many mirrors?
The light that comes from space is collected
into the primary mirrors.
Primary mirrors then take that light and image
and bring it to the secondary mirror, which projects it
to the tertiary mirror.
And then that goes to the fine steering mirror.
And then with fine-steering mirror,
they're able to adjust it, and move it around, and get
the images that they're looking for.
Why all the bouncing around?
Well, the mirrors work together to reduce the aperture size
to a format that can fit on a camera, that we can image.
Now that we've seen the primary mirror,
I'd love to show you the secondary mirror.
So, Andrea, what's going on here?
We are performing a microscope inspection of the surface.
What he's doing here is he's getting
very close to the optical surface
so that he can capture surface data.
And then we can look at that later on.
And you can see this one is unique
compared to the other mirrors.
This one is a convex hyperbola, whereas the primary mirror
and the tertiary mirror are all concave.
And there's only one of these?
There's only one of these.
So on the telescope the light captured
from the primary bounces onto this next, right?
Yep.
That's why they call it the secondary element.
Two switches that could pick two.
We also have the tertiary mirror,
which is a concave ellipse.
This is a onesie mirror, just like the secondary
and the fine-steering mirror.
It's a one-of-a-kind in the telescope.
And with this mirror, we run through the same sort
of rigorous testing that we do for the primary
and the secondary mirror.
And we get down to those tight specifications
that are required to maximize the image resolution.
Thanks a lot for your time, Andrea,
and showing us your mirrors.
You're welcome.
Andrea showed us a segment of the primary mirror,
the secondary mirror, and the tertiary mirror.
She wasn't able to show us the fine-steering mirror.
And that's the mirror that keeps the beam of light
collected by the telescope centered and stabilized.
That's because that fine-steering mirror
is inside this thermal chamber going
through some extreme temperature changes
to simulate the conditions of space.
Thanks for joining us for another edition
of Behind the Webb.
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