<p>The JWST has three mirrors(*), the main mirror (6.5m in diameter) A secondary mirror, held on three struts in front of the main mirror and a tertiary mirror that reflects the light into the various instruments.</p>
<p>The length of the light path from Main mirror to focal point is about 20m, but this is not the focal length, since the secondary mirror is convex, the tertiary mirror is also curved to remove the astigmatism caused by the secondary being slightly off-centre.  The convex curvature on the secondary has a &quot;telephoto&quot; effect, lengthening the effective focal length.</p>
<p>The convex secondary mirror gives an <em>effective</em> focal length of 131.4m. The three mirrors together function <em>as if</em> the telescope had a single mirror with focal length 131.4m. This layout is called a &quot;Cassegrain&quot; telescope, and is popular both for billion-dollar telescopes and amateur instruments.  It allows for a much longer focal length to fit in a short stable package.  Both Hubble and the VST are also Cassegrain telescopes.</p>
<p>Here is an animation to show <a href="https://youtu.be/y9Z2GbFJWmo" rel="noreferrer">how light is collected by the mirrors.</a></p>
<hr />
<p>(*) It actually has lots more, but to understand the focal length there are effectively three.</p>

CC BY-SA 4.0
2022-11-06T06:10:05.470Z
yes, okay, but the 20 hexagonal ones act as one mirror
James K
CC BY-SA 4.0
2022-11-06T07:03:16.250Z
it's three mirrors to some primary focus for which the focal length is quoted, but I think any light reaching an actual detector or image sensor sees more like eight or ten reflections in total [NIRISS](https://jwst-docs.stsci.edu/jwst-near-infrared-imager-and-slitless-spectrograph/niriss-instrumentation/niriss-optics-and-focal-plane) and [MIRI](https://jwst-docs.stsci.edu/jwst-mid-infrared-instrument/miri-instrumentation/miri-optics-and-focal-plane) and [NIRCAM](https://jwst-docs.stsci.edu/jwst-near-infrared-camera/nircam-instrumentation/nircam-optics)
uhoh
CC BY-SA 4.0
2022-11-06T07:13:34.493Z
Yes, but that is, in the context of the question, an engineering detail.  It is the cassegrain construction with a convex secondary that gives an effective focal length longer than the light path length.
James K
CC BY-SA 4.0
2022-11-06T07:49:41.503Z
Hexagonal.segments of the primary mirror are flat and just tilted to each other oř curved?
Leos Ondra
CC BY-SA 4.0
2022-11-06T08:17:40.697Z
@LeosOndra very carefully curved. See the figure here https://webb.nasa.gov/content/observatory/ote/mirrors/index.html three curvatures labeled "A", "B" and "C" are used to make a very specific shape. It's a 3-mirror anistigmat or [Korsch design](https://en.wikipedia.org/wiki/Three-mirror_anastigmat#Korsch_telescope)
uhoh
CC BY-SA 4.0
2022-11-06T08:26:11.267Z
@JamesK it turns out it's not Cassegrain; it's a [three Mirror Anastigmat](https://astronomy.stackexchange.com/a/49247/7982) or[Korsch](https://astronomy.stackexchange.com/a/49904/7982) design.
uhoh
CC BY-SA 4.0
2022-11-05T21:53:48.683Z
2022-11-06T07:15:01.290Z
2022-11-06T07:15:01.290Z
James K
<p>How does the James Webb Space Telescope achieve a focal length of 131.4m ?</p>

CC BY-SA 4.0
2022-11-05T21:41:44.877Z
https://www.reddit.com/r/telescopes/comments/rmra88/how_does_the_webb_space_telescope_achieves_1314m/
James K
<observational-astronomy><telescope><space-telescope><james-webb-space-telescope><observatory>
How does the James Webb Space Telescope achieve a focal length of 131.4m?
Sebastyen Laroche
# How does the James Webb Space Telescope achieve a focal length of 131.4m?

(Asked by: username_0 on 2022-11-05)

How does the James Webb Space Telescope achieve a focal length of 131.4m ?

**Tags:** observational-astronomy, telescope, space-telescope, james-webb-space-telescope, observatory
> **Comments:**
> **username_1**: https://www.reddit.com/r/telescopes/comments/rmra88/how_does_the_webb_space_telescope_achieves_1314m/  

---

## 1 answers

### Answer by username_1 on 2022-11-05. Score: 13 | Accepted answer

The JWST has three mirrors(\*), the main mirror (6.5m in diameter) A secondary mirror, held on three struts in front of the main mirror and a tertiary mirror that reflects the light into the various instruments.

The length of the light path from Main mirror to focal point is about 20m, but this is not the focal length, since the secondary mirror is convex, the tertiary mirror is also curved to remove the astigmatism caused by the secondary being slightly off-centre. The convex curvature on the secondary has a "telephoto" effect, lengthening the effective focal length.

The convex secondary mirror gives an *effective* focal length of 131.4m. The three mirrors together function *as if* the telescope had a single mirror with focal length 131.4m. This layout is called a "Cassegrain" telescope, and is popular both for billion-dollar telescopes and amateur instruments. It allows for a much longer focal length to fit in a short stable package. Both Hubble and the VST are also Cassegrain telescopes.

Here is an animation to show [how light is collected by the mirrors.](https://youtu.be/y9Z2GbFJWmo)

---

(\*) It actually has lots more, but to understand the focal length there are effectively three.

> **Comments:**
> **username_1**: yes, okay, but the 20 hexagonal ones act as one mirror  
> **username_2**: it's three mirrors to some primary focus for which the focal length is quoted, but I think any light reaching an actual detector or image sensor sees more like eight or ten reflections in total [NIRISS](https://jwst-docs.stsci.edu/jwst-near-infrared-imager-and-slitless-spectrograph/niriss-instrumentation/niriss-optics-and-focal-plane) and [MIRI](https://jwst-docs.stsci.edu/jwst-mid-infrared-instrument/miri-instrumentation/miri-optics-and-focal-plane) and [NIRCAM](https://jwst-docs.stsci.edu/jwst-near-infrared-camera/nircam-instrumentation/nircam-optics)  
> **username_1**: Yes, but that is, in the context of the question, an engineering detail.  It is the cassegrain construction with a convex secondary that gives an effective focal length longer than the light path length.  
> **username_3**: Hexagonal.segments of the primary mirror are flat and just tilted to each other oř curved?  
> **username_2**: @LeosOndra very carefully curved. See the figure here https://webb.nasa.gov/content/observatory/ote/mirrors/index.html three curvatures labeled "A", "B" and "C" are used to make a very specific shape. It's a 3-mirror anistigmat or [Korsch design](https://en.wikipedia.org/wiki/Three-mirror_anastigmat#Korsch_telescope)  
> **username_2**: @JamesK it turns out it's not Cassegrain; it's a [three Mirror Anastigmat](https://astronomy.stackexchange.com/a/49247/7982) or[Korsch](https://astronomy.stackexchange.com/a/49904/7982) design.  

---

