Difference between revisions of "Cryptomaria"

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<div style="margin-left: 1em">[#toc0 ]</div><div style="margin-left: 2em">[#x-Description Description]</div><div style="margin-left: 2em">[#x-Additional Information Additional Information]</div><div style="margin-left: 2em">[#x-LPOD Articles LPOD Articles]</div><div style="margin-left: 2em">[#x-Bibliography Bibliography]</div></div><br />  
 
<div style="margin-left: 1em">[#toc0 ]</div><div style="margin-left: 2em">[#x-Description Description]</div><div style="margin-left: 2em">[#x-Additional Information Additional Information]</div><div style="margin-left: 2em">[#x-LPOD Articles LPOD Articles]</div><div style="margin-left: 2em">[#x-Bibliography Bibliography]</div></div><br />  
 
==Description==
 
==Description==
  Cryptomaria are buried mare basalt lavas. They are indicated by impact craters that excavate below surface bright materials (typically dustings by basin and crater ejecta) to bring up dark material. These dark halo craters often look similar to volcanic dark halo craters (as in [/Alphonsus Alphonsus]) but they are not associated with rilles or other volcanic features. Cryptomaria that are not buried deeper than a few tens of meters can also be detected with 70 cm radar which penetrates the surface debris and bounces off the underlying basalt surfaces. [/Hartmann%20and%20Wood%2C%201971 Hartmann and Wood, 1971] provided an early description of crytomaria, and Jim Head and his student Irene Antonenko studied them in detail. <br /> <br />  
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  Cryptomaria are buried mare basalt lavas. They are indicated by impact craters that excavate below surface bright materials (typically dustings by basin and crater ejecta) to bring up dark material. These dark halo craters often look similar to volcanic dark halo craters (as in [[Alphonsus|Alphonsus]]) but they are not associated with rilles or other volcanic features. Cryptomaria that are not buried deeper than a few tens of meters can also be detected with 70 cm radar which penetrates the surface debris and bounces off the underlying basalt surfaces. [[Hartmann%20and%20Wood%2C%201971|Hartmann and Wood, 1971]] provided an early description of crytomaria, and Jim Head and his student Irene Antonenko studied them in detail. <br /> <br />  
 
==Additional Information==
 
==Additional Information==
[/Cryptomaria%20List Cryptomaria List]<br /> <br />  
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[[Cryptomaria%20List|Cryptomaria List]]<br /> <br />  
 
==LPOD Articles==
 
==LPOD Articles==
 
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Revision as of 15:44, 15 April 2018

18

(glossary entry)

Table of Contents

[#toc0 ]
[#x-Description Description]
[#x-Additional Information Additional Information]
[#x-LPOD Articles LPOD Articles]
[#x-Bibliography Bibliography]

Description

Cryptomaria are buried mare basalt lavas. They are indicated by impact craters that excavate below surface bright materials (typically dustings by basin and crater ejecta) to bring up dark material. These dark halo craters often look similar to volcanic dark halo craters (as in Alphonsus) but they are not associated with rilles or other volcanic features. Cryptomaria that are not buried deeper than a few tens of meters can also be detected with 70 cm radar which penetrates the surface debris and bounces off the underlying basalt surfaces. Hartmann and Wood, 1971 provided an early description of crytomaria, and Jim Head and his student Irene Antonenko studied them in detail. 

Additional Information

Cryptomaria List

LPOD Articles


Bibliography




This page has been edited 1 times. The last modification was made by - tychocrater tychocrater on Jun 13, 2009 3:24 pm - mgx2