Skip to main content

Types of Telescopes

  • Chapter
  • First Online:
Telescopes and Techniques

Part of the book series: Undergraduate Lecture Notes in Physics ((ULNP))

  • 3817 Accesses

Abstract

Until recently, the invention of the telescope was generally attributed to a Dutch spectacle maker called Hans Lippershey (or Johann or Lipperhey or Lippersheim, 1570–1619). He worked at Middelburg on the island of Walcheren, some 130 km southwest of Amsterdam. The probably apocryphal story has it that in 1608 his children discovered, while playing with some of his spare lenses, that one combination made a distant church spire appear much closer. The exact combination of lenses they and he used is no longer known. It could have been a pair of converging lenses, though these would produce an upside-down image, so a converging lens and a diverging lens such as Galileo’s invention is also possible.

This is a preview of subscription content, log in via an institution to check access.

Access this chapter

Chapter
USD 29.95
Price excludes VAT (USA)
  • Available as PDF
  • Read on any device
  • Instant download
  • Own it forever
eBook
USD 44.99
Price excludes VAT (USA)
  • Available as EPUB and PDF
  • Read on any device
  • Instant download
  • Own it forever
Softcover Book
USD 59.99
Price excludes VAT (USA)
  • Compact, lightweight edition
  • Dispatched in 3 to 5 business days
  • Free shipping worldwide - see info

Tax calculation will be finalised at checkout

Purchases are for personal use only

Institutional subscriptions

Notes

  1. 1.

    Little is known for certain about Cassegrain. Research by Andre Baranne and Francois Launay in 1997 suggests that he might have been the priest and teacher Laurent Cassegrain (c. 1629–1693, probably born near Chartres). Other suggestions include Guillaume Cassegrain (a sculptor), Jacques Cassegrain (a doctor) and Nicolas Cassegrain (nothing further known). Quite possibly some of these names may belong to the same individual.

  2. 2.

    Angular measure is normally in degrees (°), minutes of arc (′) and seconds of arc (″), with

    360° = a full circle

    60′ = 1°

    60″ = 1′

    For some purposes, though, radians need to be used, and

     2π radians = 360° = a full circle

    so that

     1 radian = 57.2958° = 57° 17′ 45″ = 206,264″ and 1° = 0.01745 radians.

    The use of hours, minutes and seconds as an angular measure is discussed in Chap. 4.

  3. 3.

    Named for Karl Jansky (1905–50) who, in 1932, started off radio astronomy by detecting radio emission from the galactic center.

  4. 4.

    The RATAN−600 radio telescope in the Caucasus has a diameter twice that of the Arecibo dish, but consists of just a thin annulus made up from 895 7.4 m × 2 m mirrors. Its maximum practical collecting area is thus around 10,000 m2 compared with Arecibo’s 73,000 m2.

  5. 5.

    Originally MERLIN stood for ‘Multi-Element Radio Linked Interferometer Network.’ It now uses dedicated fiber optic cables to link the telescopes, but the original acronym has been retained.

Author information

Authors and Affiliations

Authors

Corresponding author

Correspondence to C. R. Kitchin .

Rights and permissions

Reprints and permissions

Copyright information

© 2013 Springer Science+Business Media New York

About this chapter

Cite this chapter

Kitchin, C.R. (2013). Types of Telescopes. In: Telescopes and Techniques. Undergraduate Lecture Notes in Physics. Springer, New York, NY. https://doi.org/10.1007/978-1-4614-4891-4_1

Download citation

  • DOI: https://doi.org/10.1007/978-1-4614-4891-4_1

  • Published:

  • Publisher Name: Springer, New York, NY

  • Print ISBN: 978-1-4614-4890-7

  • Online ISBN: 978-1-4614-4891-4

  • eBook Packages: Physics and AstronomyPhysics and Astronomy (R0)

Publish with us

Policies and ethics