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From the Magnification Wikipedia page, I have the following equality:

M = di/do = f/(do – f) = (di – f)/f

with M the magnification, f the focal length, do the distance from the subject to the lens, and di the distance from the lens to the sensor.

So, when the magnification is 1 we should have di = do = 2f.

With my macro lens (EF 100mm f/2.8 L IS USM Macro), the minimum working distance (from subject to sensor) is 30cm, at this distance the magnification is 1. From what I unsderstand from the formula, this distance should be di + do = 4f = 40cm.

So I think I missing something, can someone explain where I'm wrong?

  • 1
    There's a remarkable amount of thought put into the answers here. I imagine that if we sat all posters down there would be a large argument followed by a very enlightening answer. As it stands, IMHO, it would be best to read several of the responses and understand that none of them (including mine) concretely solve the problem but rather together, they present a treatise on how complicated this issue is. – PhotoScientist May 30 '18 at 16:44
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    Perhaps the underlying issue is that OP has [unwittingly] asked two questions here: What is the equation governing the conjugate distances in a compound lens? as well as How can a photographer measure the conjugate distances of a lens in the field? I think the level of debate in comments is because the two questions do not have a practical single answer. – PhotoScientist May 30 '18 at 17:56
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The equation assumes a simple single element lens that is bilaterally symmetrical. The camera lens, to mitigate the 7 major aberrations (shortcomings that degrade) is constructed using several individual glass lens elements. Some are positive in power, some with negative power. Some are air-spaced apart and some are cemented together. Because this array becomes quite complex, the point from which we measure focal length will likely be shifted away from the physical center of the lens barrel.

In a true telephoto design, the rear nodal (measuring point) is shifted forward. This action shortens the length of the lens barrel making the camera plus lens less awkward to hold, use, and store. In some designs, the rear nodal can actually fall in the air ahead of the lens barrel.

As the equation states: at unity (magnification 1), the subject distance is 2 focal length lengths forward and the back focus is 2 focal lengths behind the rear nodal. The problem is --- you can’t easily locate the rear nodal. However, once magnification 1 has been achieved, you can now measure the distance subject–to-image. Many cameras provide a symbol (circle bisected with a line) on the camera frame; to locate the position of the image plane.

In any event, measure distance subject-to-image and divide by 4. This division reveals the focal length. Divide by 2 and this division locates the rear nodal point. Now you are better equipped to utilize the “lens maker’s formula”.

  • You wrote: “measure distance subject-to-image and divide by 4 [to get the focal length]”. This is incorrect. At unity magnification, the subject is at 2f distance from the front nodal point, whereas the image is at 2f from the rear nodal point. The subject-to-image distance is 4f plus (or minus, depending on their relative position) the distance between the nodal points. – Edgar Bonet May 29 '18 at 20:14
  • @EdgarBonet A theoretical thin lens has zero thickness. Obviously, no such lens actually exists. – Michael C May 29 '18 at 20:28
  • @MichaelClark: Your comment is both correct and irrelevant. We are not talking about thin lenses here. – Edgar Bonet May 29 '18 at 21:13
  • @EdgarBonet The formulae in the OP certainly are based upon a thin lens. – Michael C May 29 '18 at 21:15
  • @AlanMarcus The equations in the OP assume a theoretical thin lens - a subtle but significant difference from a "simple single element lens that is bilaterally symmetrical." Since a thin lens has zero thickness, there's no need to account for the positions of "front" or "rear" nodal points in such formulae. – Michael C May 29 '18 at 21:21
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first of all, kudos on your effort to break a photography problem down to first principles.

The discrepancy you've observed stems from a common oversimplification. Your 100mm Lens is actually what optical engineers refer to as a "lens assembly" As you likely know, it is comprised of multiple lens elements in groups working in tandem to form, refine, and transmit the image seen by your imaging sensor.

If your 100mm lens assembly consisted of a single 100mm lens element you would have massive distortions and only red, green, or blue could be in focus at a time but the thin lens magnification equation you'd linked would hold true. Magnification of 1 would be achieved when the subject is 200mm from the nodal point and the lens assembly would need to be physically greater than 200mm in length. Even then, this would only be strictly accurate to the extent which the thin lens equation is appropriate (and it is not particularly appropriate here.) A proper answer would come from a derivation of the lensmaker's equation

A corollary of the difference between an assembly and a thin lens is bilocated nodal points. A thin lens has a single location for both the front and rear nodal points; Both are collocated with the entrance pupil. If this were true of your lens assembly you would be able to free-lens by rotation around your lens' aperture without any parallax to the subject or sensor. I'm sure if you tried this with the 100mm macro you would find that its not true. A thick lens has two nodal points which are only collocated if its net index is 0, I.E. it has no focal length. A lens assembly can be approximated by a virtual thick lens with two idealized indices such that the virtual lens has the same vertices, relative focal lengths, entrance pupil, and (saliently) nodal points as the lens assembly.

For extra credit, you could check the description of a compound lens and try to guess which combinations of lens focal lengths would create the situation you've described. NB the "telescope magnification." This is essentially what a lens designer does.

For additional reading you can check out the different types of photographic lens designs

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Most fixed focal length lens focus by changing their focal length in addition to moving the lens's nodal point(s). To focus on an object close to the camera, the lens reduces its focal length. A lens specified as "100 mm" is usually "100 mm when focused at infinity", but not necessarily so when focused on a close object.

  • @ Matthieu Moy --- Focal length is a measurement taken when the camera is focused on an object at an infinite distance. At all other closer distances the image forming rays are elongated. When focusing on closer than infinity distances, we shed the name “focal length” and substitute “back focus distance”. – Alan Marcus May 29 '18 at 15:55
  • @AlanMarcus We also sometimes use effective focal length to describe the angle of view given by a lens that "breathes" as it is focused closer. – Michael C May 29 '18 at 21:12
  • @AlanMarcus: I never saw this definition for "focal length". From the physics point of view, the focal length is a property of the lens, regardless of where the object and image are, hence independent of any notion of focus. Your definition of "back focus distance" doesn't match the one found on wikipedia and on most results searching "back focus distance" on google. – Matthieu Moy May 30 '18 at 7:47
  • @MichaelClark I understand the definition of effective focal length to be the reciprocal of pixel pitch times inverse tangent of IFOV which is rederived from the definition [ifov=tan(px/efl)] I think this fits how you've described EFL as an angular measurement? – PhotoScientist May 30 '18 at 17:49
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There are two reasons why the subject-to-image distance is not 40 cm at unit magnification:

  1. the focal length of the lens may not be 100 mm
  2. the distance between the principal planes may not be zero.

Which of these reasons is the most important is impossible to tell without detailed information on the optical design of the lens.

Focal length

The value “100 mm” written on the lens itself is a nominal focal distance, which is normally a rounded value of the real focal distance when the lens is focused at infinity.

Some lenses, usually called “unit focusing” lenses, achieve focus by moving the optical assembly as a whole. These lenses have a focal distance which does not vary with focusing. However, many complex lenses, including virtually any modern macro lens, have some sort of “close range correction” (in Nikon parlance): their optical formula changes as you focus, which enables better correction of aberrations. These lenses have a focal distance which varies as you focus.

These two facts: the rounding of the nominal focal length and the fact that it varies when you focus, mean you do not know what the actual focal length of the lens is at unit magnification.

Principal planes

The Wikipedia page you cite defines do and di as the distance from the lens to the object (resp. image), but note that these definitions appear in a section that is specifically about thin lenses. Your lens being a thick compound lens, this begs the question of the applicability of the formula.

It turns out that the thin lens approximation is not applicable in this situation. However, the formula is still valid if interpreted in the context of the thick lens model. In this model, the plane of the thin lens is replaced by two planes, which are called “principal planes”:

  • the “front” (or “primary”, or “object side”) principal plane is used for measuring distances in object space
  • the “back” (or “secondary”, or “image side”) principal plane is used for measuring distances in image space

These are conjugate planes with unit magnification. In the figure below (source), they are the vertical planes that go through H1, N1 and H2, N2:

thick lens diagram

Note that this way of describing an optical system in terms of its cardinal points (the Fi, Hi and Ni above) is also applicable to compound lenses. See for example this old drawing of a telephoto lens (source) where both principal planes (the vertical planes through Ni and No) are on the left side of the leftmost element:

tele lens diagram

Thus, your formula is still valid provided you define:

  • do as the distance from the subject to the primary principal plane
  • di as the distance from the secondary principal plane to the image

This gives the subject-to-image distance as

do + e + di = 4f + e

at unit magnification, where e is the (possibly negative) distance between the principal planes. Note that the thin lens approximation essentially says that the principal planes are coincident (e = 0), but it is not applicable to your case.

For more info about this topic, you can take a look at:

The thin lens misconception

I wrote this answer mostly to help clear a popular misconception, which appears in some of the answers here, including the one you accepted: that a photographic lens is equivalent to a thin lens.

It turns out that in most photographic situations (basically all non-macro situations), the subject-to-lens distance is much larger than any characteristic distance of the lens itself. In such situations it doesn't really matter which reference point you use for measuring the distance to the subject. It is then convenient to forget about the distance that separates the principal planes and consider that the rear principal plane is the only one that matters. This is equivalent to setting e = 0, which is basically the thin lens approximation.

Sticking to this approximation makes learning optics a lot simpler, as you don't need to understand notions such as principal planes, principal or nodal points, object space, image space, and so on. Considering that:

  • the approximation is good enough for most (non macro) purposes
  • knowledge in optics is only useful to a photographer at a qualitative level, as you are not going to design lenses, and you don't need optics expertise to become a great photographer

it is understandable that the thin lens is the model most commonly taught to photographers. And yet the approximation breaks when dealing with a complex thick lens at macro distances. The answers that tell you that the focal distance is one quarter of the subject-to-image distance illustrate how this misconception leads to people posting wrong answers.

  • @ Edgar Bonet --- Nodal Points: The camera lens has several principal points. The two in this discussion are the forward and rear nodal points. While named front and rear nodal. It may be the case that they are reversed as to their actual locations. The essence of their significance – a ray coming in to this system aimed at the forward nodal, exits the system aimed away from the rear nodal. The object distance is subject to front nodal. The image distance (back focus) is focused image to rear nodal. – Alan Marcus May 30 '18 at 15:41
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    The thick lens equation is slightly better than the thin but neither would materially predict the performance of the lens OP is inquiring about. The thick lens equation can only be used for an optical system with no net negative elements. Given that the aperture (presumably the entrance pupil) of this lens is less than 200mm from the sensor, we know that negative elements are in the lens. Rather than attempting to provide OP with an equation (perhaps lensmakers?), it may be better to help him to discover the characteristics of the assembly empirically. I may revise my answer. – PhotoScientist May 30 '18 at 16:17
  • @PhotoScientist: The thick lens model is applicable to any non-afocal, axially-symmetric optical system within the paraxial approximation. Wether the system is made of positive elements, negative elements, or a mixture of both makes no difference. The model can obviously not predict the performance of a lens, as the paraxial approximation essentially ignores all aberrations. It can, however, exactly predict the position of the paraxial image. – Edgar Bonet May 30 '18 at 16:47
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    @EdgarBonet Granted that is correct; but for a complex optical system like the 100mm macro in question your model would require that appropriate front an rear surfaces be virtualized whose indices correspond to the idealized thick lens but have no bearing on the actual optical system. Only then can the location of the nodal points be predicted. What I was implying is that the actual elements of the lens can be used to make this determination only if there is no negative element. I worry that your approach, while computationally correct, is difficult to implement in the field. – PhotoScientist May 30 '18 at 17:06
  • I assume that, unlike Alan Marcus, we agree that the location of the front and rear nodal points is the key to accurately assessing the conjugate distances OP is inquiring about. – PhotoScientist May 30 '18 at 17:06
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Working distance is measured from the front of the lens to the subject. For your EF 100mm f/2.8 L IS USM Macro lens the working distance at minimum focus distance (MFD)/full magnification is approximately 133mm.

Focus distance is measured from the subject to the imaging plane (film or sensor). For your EF 100mm f/2.8 L IS USM Macro lens the focus distance at full magnification/MFD is 300mm.

Most lenses' focal lengths are measured when the lens is focused at infinity (and then rounded to the nearest "standard" focal length). As focus distance is reduced, the angle of view provided by the lens often changes. This is what is know as focus breathing. The 300mm MFD of your EF 100mm f/2.8 L IS USM Macro reveals to us that the effective focal length at 1:1 magnification is about 75mm. This is fairly common for a Macro lens with focal length in the 90-105mm range. The Tamron 90mm f/2.8 Di VC USD Macro (F017), for instance, also has an MFD of 300mm at 1:1 magnification.

Additionally, focal length for a compound lens is approximated from the focal length a single lens would need to be to provide the same amount of magnification. A compound lens is a system of several lenses, usually arranged in groups, that together act as a single lens. Pretty much every commercially available lens for interchangeable lens camera systems are compound lenses. Your EF 100mm f/2.8 L IS Macro has 15 lens elements arranged in 12 groups.

For most wide angle lenses which have a retrofocus design, this theoretical simple single lens point is well behind the front of the lens. For telephoto lenses this point is, by definition, in front of the front of the lens.

When focused at the 300mm minimum focus distance (MFD), the front of your EF 100mm f/2.8 L IS USM Macro is about 168mm in front of the sensor. But the field of view and magnification provided by the lens at MFD makes it effectively a 75mm lens at that focus distance. This means a simple 75mm lens would need to be at 150mm in front of the sensor (which also places it at 150mm away from the subject) for 1:1 magnification. This places the effective center point of your EF 100mm f/2.8 Macro about 18mm behind the front of the lens when focused at the MFD.

So I think I missing something, can someone explain where I'm wrong?

When applying formulae such as those in your question, you need to use 75mm for the lens' focal length when it is focused at MFD.

  • “focal length for a compound lens is measured from the point where a single theoretical thin lens would be placed to provide the same amount of magnification”. That's wrong. The focal length is the distance between the focal points and the corresponding principal points. There is no thin lens approximation involved. In your answer you are neglecting the distance between the principal (or nodal) points, which in general is not a reasonable approximation for a macro lens at close distances. – Edgar Bonet May 29 '18 at 21:26
  • Please explain to me how the nodal points of different single lenses with varying refractive indexes/thicknesses (equivalent to the performance of a compound lens) would be the same distance from the center of each lens? – Michael C May 29 '18 at 21:38
  • @EdgarBonet I've removed all references to thin lenses from the answer. But the formulae in the OP are thin lens equations, as pointed out in this answer to which you don't seem to have the same objection. – Michael C May 29 '18 at 21:51

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