Telephoto lens

From Wikipedia, the free encyclopedia

This is an old revision of this page, as edited by Fountains of Bryn Mawr (talk | contribs) at 13:04, 20 April 2012 (Undid revision 488282032 by 96.238.214.97 (talk)). The present address (URL) is a permanent link to this revision, which may differ significantly from the current revision.

A collection of telephoto lenses

In photography and cinematography, a telephoto lens is a specific type of a long-focus lens in which the physical length of the lens is shorter than the focal length.[1] This is achieved by incorporating a special lens group known as a telephoto group that extends the light path to create a long-focus lens in a much shorter overall design. The angle of view and other effects of long-focus lenses are the same for telephoto lenses of the same specified focal length. Long-focal-length lenses are often informally referred to as telephoto lenses although this is technically incorrect: a telephoto lens specifically incorporates the telephoto group.[2]

Telephoto lenses are sometimes broken into the further sub-types of medium telephoto: lenses covering between a 30° and 10° field of view (85mm to 135mm in 35mm film format), and super telephoto: lenses covering between 8° through less than 1° field of view (over 300mm in 35mm film format).[3]

Construction

A 500 mm lens of a non-telephoto design
A 150–500mm telephoto zoom lens

If a camera lens were to be constructed from a single lens of 500 mm focal length, then when the lens is focused on an object at infinity, the lens will be 500 mm away from the focal plane where the film or sensor is. The centre of the lens is referred to as the optical centre of the lens. Even constructing the lens out of several elements to minimize aberrations, will still have the optical centre within the construction.

As the focal length of such lenses increases, the physical length of lens becomes inconveniently long. But such lenses are not telephoto lenses, no matter how extreme the focal length. They are simply known as long-focus lenses.[1] A telephoto lens works by having the outermost (i.e. light gathering) element of a much shorter focal length than the equivalent long-focus lens and then incorporating a second set of elements close to the film or sensor plane that extend the cone of light so that it appears to have come from a lens of much greater focal length.

Diagram of a typical telephoto lens with a large positive lens and a smaller negative telephoto group combined to create a much longer focal length - f.

The basic construction of a telephoto lens consists of front lens elements that, as a group, have a positive focus. The focal length of this group is shorter than the effective focal length of the lens. The converging rays from this group are intercepted by the rear lens group, sometimes called the "telephoto group," which has a negative focus. The simplest telephoto designs could consist of one element in each group, but in practice, more than one element is used in each group to correct for various aberrations. The combination of these two groups produces a lens assembly that is physically shorter than a long-focus lens producing the same image size.

Diagram of a catadioptric mirrors lens.

This same property is achieved in camera lenses that combined mirrors with lenses. These designs called catadioptric, 'reflex', or 'mirror' lenses have a curved mirror as the primary objective with some form of negative lens in front of the mirror to correct optical aberrations. They also use a curved secondary mirror to relay the image that extends the light cone the same way the negative lens telephoto group does. The mirrors also fold the light path. This makes them much shorter, lighter, and cheaper than an all refractive lens, but at the cost of some optical compromises due to aberrations caused by the central obstruction from the secondary mirror.

The heaviest telephoto lens was made by Carl Zeiss and has a focal length of 1700 mm with a maximum aperture of f/4, implying a 425 mm (16.7 inch) entrance pupil. It is designed for use with a medium format Hasselblad 203 FE camera and weighs 256 kg (564 lb).[citation needed]

Retrofocus lenses

Inverting the telephoto configuration, employing one or more negative lens groups in front of a positive lens group, creates a wide-angle lens with an increased back focal distance. These are called retrofocus lenses or inverted telephotos, which have greater clearance from the rear element to the film plane than their focal length would permit with a conventional wide-angle lens optical design. This allows for greater clearance for other optical or mechanical parts such as the mirror parts in a single-lens reflex camera. Zoom lenses that are telephotos at one extreme of the zoom range and retrofocus at the other are now common.[citation needed]

History

The concept of the telephoto lens, in reflecting form, was first described by Johannes Kepler in his Dioptrice of 1611,[4] and re-invented by Peter Barlow in 1834.[5]

Histories of photography usually credit Thomas Rudolphus Dallmeyer with the invention of the photographic telephoto lens in 1891, though it was independently invented by others about the same time; some credit his father John Henry Dallmeyer in 1860.[6]

In 1883 or 1884 New Zealand photographer Alexander McKay discovered he could create a much more manageable long-focus lens by combining a shorter focal length telescope objective lens with negative lenses and other optical parts from opera glasses to modify the light cone. Some of his photographs are preserved in the holdings of the Turnbull Library in Wellington, and two of these can be unequivocally dated as having been taken during May 1886. One of McKay’s photographs shows the Russian warship Vjestnik anchored in Wellington harbour about two and a half kilometres away, with its rigging lines and gun ports clearly visible. The other, taken from the same point, is of a local hotel, the Shepherds Arms, about 100 metres distant from the camera. The masts of the Vjestnik are visible in the background. McKay's other photographic achievements include photo-micrographs, and a ‘shadow-less technique’ for photographing fossils.[7]

McKay presented his work to the Wellington Philosophical Society (the precursor of the Royal Society of New Zealand) in 1890.[8]

See also

References

  1. ^ a b R. E. Jacobson, The manual of photography: photographic and digital imaging, page 93
  2. ^ Gregory Hallock Smith, Camera lenses: from box camera to digital, page 207
  3. ^ photographywebsite.co.uk - Lens Types Explained
  4. ^ Edward John Wall and Thomas Bolas (1902). The Dictionary of Photography for the Amateur and Professional Photographer. London: Hazell, Watson, and Viney Ld.
  5. ^ Ray N. Wilson (2004). Reflecting Telescope Optics. Springer. ISBN 978-3-540-40106-3.
  6. ^ New York Times Staff (2004). The New York Times Guide to Essential Knowledge. Macmillan. ISBN 978-0-312-31367-8.
  7. ^ Graham Bishop (2008). The Real McKay: The remarkable life of Alexander McKay, geologist. (1841-1917). Dunedin: Otago University Press. ISBN 978-1-877372-22-3.
  8. ^ Alexander McKay (1891). "On Some Means for increasing the Scale of Photographic Lenses, and the Use of Telescopic Powers in Connection with an Ordinary Camera". Transactions of the New Zealand Institute. XIII: 461–465.

External links