Skip to main content

Lunar Surface as an Impact Counter, and its Stratigraphy

  • Chapter
An Introduction to the Study of the Moon

Part of the book series: Astrophysics and Space Science Library ((ASSL))

  • 113 Accesses

Abstract

In the preceding two chapters we gave a descriptive survey of the principal types of formations encountered on the lunar surface, as well as a brief account of the processes by which such individual formations could have originated. The aim of the present chapter will be to consider now the collective aspects of the observed surface features, their distribution and density over different types of lunar ground; and to draw some conclusions from this evidence which may throw light on the “partition function” of different processes considered in the preceding chapter, or on the conditions prevailing in interplanetary space.

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 39.99
Price excludes VAT (USA)
  • Available as PDF
  • Read on any device
  • Instant download
  • Own it forever
Softcover Book
USD 54.99
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

Preview

Unable to display preview. Download preview PDF.

Unable to display preview. Download preview PDF.

Bibliographical Notes

  • For recent investigations of the particular contents of space, and the mass-distribution of solid particles at a distance of one astronomical unit from the Sun, cf., Piotrowski (1953), Öpik (1956, 1958), Urey (1960), Brown (1960), Hawkins (1960, 1963, 1964) or Hartmann (1965).

    Google Scholar 

  • For statistical studies of crater distribution in different parts of the lunar surface cf., Arthur (1954), Öpik (1960), Kreiter (1960), McGillem and Miller (1962), Dodd, Salisbury and Smalley (1963), Palm and Strom (1963), Baldwin (1964, 1965), Marcus (1964, 1965), Ronca (1965) et al. The latest contribution to such studies by Fielder (1965) contains conclusions biased in favour of lunar volcanism which, as was shown by Marcus (1966), are unwarranted by the data on which they are based.

    Google Scholar 

  • Fundamental papers on absolute dating of lunar stratigraphy, based on a combination of the relevant lunar and interplanetary data, are those by Shoemaker, Hackman and Eggleton (1961), Shoemaker (1962, pp. 347–348), Shoemaker and Hackman (1962) or Eggleton and Marshall (1963).

    Google Scholar 

Download references

Author information

Authors and Affiliations

Authors

Rights and permissions

Reprints and permissions

Copyright information

© 1966 Springer Science+Business Media Dordrecht

About this chapter

Cite this chapter

Kopal, Z. (1966). Lunar Surface as an Impact Counter, and its Stratigraphy. In: An Introduction to the Study of the Moon. Astrophysics and Space Science Library. Springer, Dordrecht. https://doi.org/10.1007/978-94-017-6320-2_18

Download citation

  • DOI: https://doi.org/10.1007/978-94-017-6320-2_18

  • Publisher Name: Springer, Dordrecht

  • Print ISBN: 978-94-017-5850-5

  • Online ISBN: 978-94-017-6320-2

  • eBook Packages: Springer Book Archive

Publish with us

Policies and ethics