Difference between revisions of "Tompkins & Pieters, 1999"
(Created page with "<div id="content_view" class="wiki" style="display: block"> =Tompkins & Pieters, 1999= (glossary entry)<br /> <div id="toc"> =Table of Contents= <div style="margin-left:...") |
|||
| (One intermediate revision by the same user not shown) | |||
| Line 2: | Line 2: | ||
=Tompkins & Pieters, 1999= | =Tompkins & Pieters, 1999= | ||
(glossary entry)<br /> <div id="toc"> | (glossary entry)<br /> <div id="toc"> | ||
| − | + | <br /> | |
| − | |||
==Description== | ==Description== | ||
| − | The authors use [ | + | The authors use [[Clementine|Clementine]] UVIS multispectral data to characterize the [[Central%20peak%20composition|mineralogical composition]] of the central peaks of 109 impact craters ranging in diameter from 40 to 180 km. These craters can be found by typing the word Tompkins in the search box to the left.<br /> <br /> |
==Additional Information== | ==Additional Information== | ||
<br /> | <br /> | ||
| Line 13: | Line 12: | ||
Stefanie Tompkins and Carle M. Pieters (1999) [http://adsabs.harvard.edu/abs/1999M&PS...34...25T Mineralogy of the lunar crust: Results from Clementine] ''Meteoritics & Planetary Science, vol. 34'', pp. 25-41 .<br /> <br /> | Stefanie Tompkins and Carle M. Pieters (1999) [http://adsabs.harvard.edu/abs/1999M&PS...34...25T Mineralogy of the lunar crust: Results from Clementine] ''Meteoritics & Planetary Science, vol. 34'', pp. 25-41 .<br /> <br /> | ||
---- | ---- | ||
| − | + | </div> | |
Latest revision as of 16:55, 15 April 2018
Contents
Tompkins & Pieters, 1999
(glossary entry)
Description
The authors use Clementine UVIS multispectral data to characterize the mineralogical composition of the central peaks of 109 impact craters ranging in diameter from 40 to 180 km. These craters can be found by typing the word Tompkins in the search box to the left.
Additional Information
LPOD Articles
Bibliography
Stefanie Tompkins and Carle M. Pieters (1999) Mineralogy of the lunar crust: Results from Clementine Meteoritics & Planetary Science, vol. 34, pp. 25-41 .
