Skip to main content Accessibility help
×
Hostname: page-component-848d4c4894-nr4z6 Total loading time: 0 Render date: 2024-06-05T01:50:26.849Z Has data issue: false hasContentIssue false

23 - Diatomite

Published online by Cambridge University Press:  16 January 2010

E. F. Stoermer
Affiliation:
University of Michigan, Ann Arbor
John P. Smol
Affiliation:
Queen's University, Ontario
Get access

Summary

Introduction

Diatomite is a porous, lightweight sedimentary rock resulting from accumulation and compaction of diatom remains (class Bacillariophyceae). The delicate shell or frustule of diatoms, which gives diatomite many of its useful properties, is composed of amorphous opaline silica (SiO2·nH2O). Most diatoms fall within the 10 µm to 100 µm size range, although some are as large as 1 mm (Tappan, 1980). It is estimated that 1 cubic inch of diatomite may contain 40 to 70 million diatoms (Crespin, 1946). While the specific gravity (density) of diatom frustules is nearly twice that of water, the perforations and open structure of the frustule renders diatomite a considerably lower effective density (between 0.12 g/cm3 and 0.25 g/cm3) and high porosity (from 75 to 85%), able to absorb and hold up to 3.5 times its own weight in liquid (Cleveland, 1966).

Diatomite of varying quality has been deposited in freshwater environments since at least the Eocene (~50 million years ago) and in marine environments since the Late Cretaceous (~80 million years ago). The purity of diatomites depends on the presence and amount of both clastic particles (silt and clay) and of organic materials, which limit the utility of diatomite in industrial applications. Some high commercial-grade diatomite contains up to 90% SiO2, with minor occurrence of calcium carbonate, volcanic glass, and terrigenous particles (Cressman, 1962; Cummins, 1960). Diatom-bearing rocks with a higher terrigenous component (e.g., diatomaceous shale or siliceous shale) are commonly interbedded with diatomite.

Type
Chapter
Information
The Diatoms
Applications for the Environmental and Earth Sciences
, pp. 436 - 444
Publisher: Cambridge University Press
Print publication year: 1999

Access options

Get access to the full version of this content by using one of the access options below. (Log in options will check for institutional or personal access. Content may require purchase if you do not have access.)

Save book to Kindle

To save this book to your Kindle, first ensure coreplatform@cambridge.org is added to your Approved Personal Document E-mail List under your Personal Document Settings on the Manage Your Content and Devices page of your Amazon account. Then enter the ‘name’ part of your Kindle email address below. Find out more about saving to your Kindle.

Note you can select to save to either the @free.kindle.com or @kindle.com variations. ‘@free.kindle.com’ emails are free but can only be saved to your device when it is connected to wi-fi. ‘@kindle.com’ emails can be delivered even when you are not connected to wi-fi, but note that service fees apply.

Find out more about the Kindle Personal Document Service.

Available formats
×

Save book to Dropbox

To save content items to your account, please confirm that you agree to abide by our usage policies. If this is the first time you use this feature, you will be asked to authorise Cambridge Core to connect with your account. Find out more about saving content to Dropbox.

Available formats
×

Save book to Google Drive

To save content items to your account, please confirm that you agree to abide by our usage policies. If this is the first time you use this feature, you will be asked to authorise Cambridge Core to connect with your account. Find out more about saving content to Google Drive.

Available formats
×