<p>A supplement to the very good antlersoft answer:</p>
<p>There is a practical limitation on how much thick a lens can be. The glass (and the other optical materials) is transparent only to an extent.</p>
<p>While optical cables (made of glass) tens of kilometers long do exist, the glass used for lenses is made with different engineering compromises so it is much less transparent.</p>
<p>The net result from the limited glass transparency is that a lens that is few centimeters thick in the middle will lose a great deal of the light to the glass itself. One will get much of the light from the lens edges where the glass is thinest (and where the spherical aberration is worst). Pointless, isn't it?</p>
<p>The usual approach against the spherical aberration (to use only the central part of the lens) for a large, extinction-limited lens will get us almost no light.</p>
<p>There are also engineering limitations - e.g. how to make this much glass optically homogeneous? One will need to cool it down very very slowly just to avoid internal tensions and cracks and the glass may like to stratify in the meantime (creating a gradient in the optical properties).</p>
<p>You care much less about the materials in a reflector. Of course, you do care about them - the mirror has to be mechanically stiff and the shape has to be constant over an extended period of time, but the lens material has to have all of these mechanical properties in addition to the desired optical properties.</p>

CC BY-SA 4.0
2022-09-13T16:46:41.807Z
2022-09-13T16:46:41.807Z
fraxinus
<p>In addition to the answers above, and at the risk of sounding flippant, you can literally shoot holes in a reflector and it keeps working just fine. The Harlan J Smith telescope <a href="https://en.wikipedia.org/wiki/Harlan_J._Smith_Telescope" rel="nofollow noreferrer">suffered exactly that</a>. This is useful if your telescope, like JWST, might get hit by micrometeoroids.</p>
<p>Further, cleaning and recoating a mirror is easier. (Though not for JWST... )</p>

CC BY-SA 4.0
2022-09-14T16:00:22.380Z
2022-09-14T16:00:22.380Z
Andy Burns
<p>Several aspects of refractors limit their usefulness for large telescopes.</p>
<p>First is chromatic aberration.  Because refractors focus light with refraction, and refraction varies at different wavelengths of light, a single lens is unable to focus all colors at the same point.  Refracting telescopes try to correct this by combining a lens with a positive focal-ratio with a lens with a slightly longer negative focal-ratio and a higher index-of-refraction glass so the two dispersions (approximately) cancel out at the focus of the combined lens.  The focal-ratio of these <em>achromatic</em> lenses is necessarily much longer than either of the constituent lenses.  This has several disadvantages with respect to a mirror with the same diameter: first, the light has to traverse four surfaces rather than just one, at each surface some light is reflected back, and a flaw in any of the surfaces will distort the image; second, for a given focal length, the lens surfaces will be more strongly curved than the mirror, which is more difficult to get correct; third, the shortest practical focal length is necessarily longer, resulting in a longer and more unwieldy instrument.</p>
<p>Another consideration is actually supporting the optical elements.  Mirrors can be supported from the whole surface of their back sides, while lenses can only be supported from their edges (or else you give up the lack of diffraction in the optical path which is the primary advantage of the refractor).  Large lenses tend to bend slightly due to mechanical stress as the telescope is moved around the sky, reducing their image quality.</p>
<p>Very large recent telescopes have mirrors made in segments or meniscus shaped mirrors where the overall figure is maintained with supports that can dynamically adjust the mirror to account for mechanical stress.  This would be impossible with large lenses.</p>
<p>Refractors are best suited for small telescopes optimized for minimal diffraction.</p>

CC BY-SA 4.0
2022-09-11T22:57:46.503Z
different but related: [What are the benefits of a large refracting telescope?](https://astronomy.stackexchange.com/q/34235/7982)
uhoh
CC BY-SA 4.0
2022-09-12T05:48:25.517Z
Additionally, a reflector needs one perfect surface.  The simple refractor needs two perfect surfaces *and* a perfectly homogeneous medium (glass, Pyrex, quartz, etc) between the two surfaces...
DJohnM
CC BY-SA 4.0
2022-09-12T14:59:43.607Z
Why can't you build a large lens made of segments like you do with mirrors? It's useful on a small scale already: https://en.wikipedia.org/wiki/Light_field_camera
Mad Physicist
CC BY-SA 4.0
2022-09-12T16:30:33.477Z
Why can't reflectors have its secondary mirror off to the side and not cause diffraction?
Passer By
CC BY-SA 4.0
2022-09-12T16:44:42.460Z
You always have diffraction, at least on the edge of the optical surface. That holds also for Schiefspiegler. https://en.m.wikipedia.org/wiki/Schiefspiegler - and you trade for increased coma and aberration errors
planetmaker
CC BY-SA 4.0
2022-09-12T21:48:44.920Z
The @MadPhysicist never heard about Fresnel lenses, please read https://en.wikipedia.org/wiki/Fresnel_lens carefully
Uwe
CC BY-SA 4.0
2022-09-12T22:11:04.380Z
@Uwe. I have, but the largest planned reflectors are on the ~30-40m scale, while the biggest fresnel lens is 10x smaller and used for a lighthouse. It's still monolithic, which does not really explain why piecewise refractors aren't a thing
Mad Physicist
CC BY-SA 4.0
2022-09-12T23:44:20.627Z
@MadPhysicist the lighthouse lenses designed by fresnel himself were not monolythic
Uwe
CC BY-SA 4.0
2022-09-13T12:25:00.217Z
@phaser you can do that to avoid the additional diffraction from a central obstruction; but the tradeoff is either needing a much more heavily curved and asymmetric mirror (essentially you're making primary that's a segment outside of where the central obstruction of a much larger mirror) or tilting the primary to aim for an off axis secondary and via the tilt adding additional aberrations to compensate for.  The net tradeoffs are such that those designs are almost exclusively amateur telescope maker projects by people bored with making more conventional models.
Dan Is Fiddling By Firelight
CC BY-SA 4.0
2022-09-14T12:09:06.443Z
Why does chromatic aberration affect refractors though? Camera lenses have multiple lenses components in them to compensate for chromatic aberration, and they are in practice small refracting telescopes.
Tomáš Zato
CC BY-SA 4.0
2022-09-14T21:20:52.567Z
@TomášZato-ReinstateMonica they attempt to minimize it, but can never get rid of it entirely, and the cost is a more complex multi-lens system with expensive and exotic lens materials: https://en.wikipedia.org/wiki/Superachromat
Christopher James Huff
CC BY-SA 4.0
2022-09-11T15:37:44.333Z
2022-09-12T11:24:57.790Z
2022-09-12T11:24:57.790Z
antlersoft
<p>I've noticed lately that reflector telescopes are used much more than refractors. The majority of telescopes I see in telescope shops or featured by people online are reflectors. Even the Hubble and JWST are reflector telescopes. Is the reflector just preferred by a lot of people or are there real advantages of having a reflector over a refractor?</p>

CC BY-SA 4.0
2022-09-11T13:56:26.167Z
Tubes get too big and lenses too heavy with large refractors.
AtmosphericPrisonEscape
CC BY-SA 4.0
2022-09-11T22:32:10.407Z
https://xkcd.com/1791/
Eliza Wilson
CC BY-SA 4.0
2022-09-13T12:13:52.017Z
For the new telescopes like JWST, it's even possible to divide the mirror into segments and focus them separately. On a refraction telescope it's much harder to build a variable-geometry aspherical lens.
user3528438
CC BY-SA 4.0
2022-09-14T20:51:06.447Z
@ElizaWilson That's why we can't see dark matter it's made of vampires!
Schwern
<telescope>
Why are almost all modern telescopes reflectors?
chowder
# Why are almost all modern telescopes reflectors?

(Asked by: username_0 on 2022-09-11)

I've noticed lately that reflector telescopes are used much more than refractors. The majority of telescopes I see in telescope shops or featured by people online are reflectors. Even the Hubble and JWST are reflector telescopes. Is the reflector just preferred by a lot of people or are there real advantages of having a reflector over a refractor?

**Tags:** telescope
> **Comments:**
> **username_1**: Tubes get too big and lenses too heavy with large refractors.  
> **username_2**: https://xkcd.com/1791/  
> **username_3**: For the new telescopes like JWST, it's even possible to divide the mirror into segments and focus them separately. On a refraction telescope it's much harder to build a variable-geometry aspherical lens.  
> **username_4**: @ElizaWilson That's why we can't see dark matter it's made of vampires!  

---

## 3 answers

### Answer by username_7 on 2022-09-11. Score: 39 | Accepted answer

Several aspects of refractors limit their usefulness for large telescopes.

First is chromatic aberration. Because refractors focus light with refraction, and refraction varies at different wavelengths of light, a single lens is unable to focus all colors at the same point. Refracting telescopes try to correct this by combining a lens with a positive focal-ratio with a lens with a slightly longer negative focal-ratio and a higher index-of-refraction glass so the two dispersions (approximately) cancel out at the focus of the combined lens. The focal-ratio of these *achromatic* lenses is necessarily much longer than either of the constituent lenses. This has several disadvantages with respect to a mirror with the same diameter: first, the light has to traverse four surfaces rather than just one, at each surface some light is reflected back, and a flaw in any of the surfaces will distort the image; second, for a given focal length, the lens surfaces will be more strongly curved than the mirror, which is more difficult to get correct; third, the shortest practical focal length is necessarily longer, resulting in a longer and more unwieldy instrument.

Another consideration is actually supporting the optical elements. Mirrors can be supported from the whole surface of their back sides, while lenses can only be supported from their edges (or else you give up the lack of diffraction in the optical path which is the primary advantage of the refractor). Large lenses tend to bend slightly due to mechanical stress as the telescope is moved around the sky, reducing their image quality.

Very large recent telescopes have mirrors made in segments or meniscus shaped mirrors where the overall figure is maintained with supports that can dynamically adjust the mirror to account for mechanical stress. This would be impossible with large lenses.

Refractors are best suited for small telescopes optimized for minimal diffraction.

> **Comments:**
> **username_8**: different but related: [What are the benefits of a large refracting telescope?](https://astronomy.stackexchange.com/q/34235/7982)  
> **username_9**: Additionally, a reflector needs one perfect surface.  The simple refractor needs two perfect surfaces *and* a perfectly homogeneous medium (glass, Pyrex, quartz, etc) between the two surfaces...  
> **username_10**: Why can't you build a large lens made of segments like you do with mirrors? It's useful on a small scale already: https://en.wikipedia.org/wiki/Light_field_camera  
> **username_11**: Why can't reflectors have its secondary mirror off to the side and not cause diffraction?  
> **username_12**: You always have diffraction, at least on the edge of the optical surface. That holds also for Schiefspiegler. https://en.m.wikipedia.org/wiki/Schiefspiegler - and you trade for increased coma and aberration errors  
> **username_13**: The @MadPhysicist never heard about Fresnel lenses, please read https://en.wikipedia.org/wiki/Fresnel_lens carefully  
> **username_10**: @Uwe. I have, but the largest planned reflectors are on the ~30-40m scale, while the biggest fresnel lens is 10x smaller and used for a lighthouse. It's still monolithic, which does not really explain why piecewise refractors aren't a thing  
> **username_13**: @MadPhysicist the lighthouse lenses designed by fresnel himself were not monolythic  
> **username_14**: @phaser you can do that to avoid the additional diffraction from a central obstruction; but the tradeoff is either needing a much more heavily curved and asymmetric mirror (essentially you're making primary that's a segment outside of where the central obstruction of a much larger mirror) or tilting the primary to aim for an off axis secondary and via the tilt adding additional aberrations to compensate for.  The net tradeoffs are such that those designs are almost exclusively amateur telescope maker projects by people bored with making more conventional models.  
> **username_15**: Why does chromatic aberration affect refractors though? Camera lenses have multiple lenses components in them to compensate for chromatic aberration, and they are in practice small refracting telescopes.  
> **username_16**: @TomášZato-ReinstateMonica they attempt to minimize it, but can never get rid of it entirely, and the cost is a more complex multi-lens system with expensive and exotic lens materials: https://en.wikipedia.org/wiki/Superachromat  

---

### Answer by username_5 on 2022-09-13. Score: 4

A supplement to the very good antlersoft answer:

There is a practical limitation on how much thick a lens can be. The glass (and the other optical materials) is transparent only to an extent.

While optical cables (made of glass) tens of kilometers long do exist, the glass used for lenses is made with different engineering compromises so it is much less transparent.

The net result from the limited glass transparency is that a lens that is few centimeters thick in the middle will lose a great deal of the light to the glass itself. One will get much of the light from the lens edges where the glass is thinest (and where the spherical aberration is worst). Pointless, isn't it?

The usual approach against the spherical aberration (to use only the central part of the lens) for a large, extinction-limited lens will get us almost no light.

There are also engineering limitations - e.g. how to make this much glass optically homogeneous? One will need to cool it down very very slowly just to avoid internal tensions and cracks and the glass may like to stratify in the meantime (creating a gradient in the optical properties).

You care much less about the materials in a reflector. Of course, you do care about them - the mirror has to be mechanically stiff and the shape has to be constant over an extended period of time, but the lens material has to have all of these mechanical properties in addition to the desired optical properties.


---

### Answer by username_6 on 2022-09-14. Score: 1

In addition to the answers above, and at the risk of sounding flippant, you can literally shoot holes in a reflector and it keeps working just fine. The Harlan J Smith telescope [suffered exactly that](https://en.wikipedia.org/wiki/Harlan_J._Smith_Telescope). This is useful if your telescope, like JWST, might get hit by micrometeoroids.

Further, cleaning and recoating a mirror is easier. (Though not for JWST... )


---

