Difference between revisions of "McLaughlin"

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(Created page with "<div id="content_view" class="wiki" style="display: block"> =McLaughlin= {| class="wiki_table" | Lat: 47.1°N, Long: 92.9°W, Diam: 79 km, Depth: km, Rükl: ''(farside)''...")
 
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Lat: 47.1°N, Long: 92.9°W, Diam: 79 km, Depth: km, Rükl: ''(farside)'' [http://the-moon.wikispaces.com/Stratigraphy Nectarian]<br />
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Lat: 47.1°N, Long: 92.9°W, Diam: 79 km, Depth: km, Rükl: ''(farside)'' [http://the-moon.us/wiki/Stratigraphy Nectarian]<br />
 
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==Maps==
 
==Maps==
''([http://the-moon.wikispaces.com/LAC%20zone LAC zone] 36B1)'' [http://planetarynames.wr.usgs.gov/images/Lunar/lac_36.pdf USGS Digital Atlas PDF]<br /> <br />  
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''([http://the-moon.us/wiki/LAC%20zone LAC zone] 36B1)'' [http://planetarynames.wr.usgs.gov/images/Lunar/lac_36.pdf USGS Digital Atlas PDF]<br /> <br />  
 
==Description==
 
==Description==
 
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Revision as of 19:24, 11 April 2018

McLaughlin

Lat: 47.1°N, Long: 92.9°W, Diam: 79 km, Depth: km, Rükl: (farside) Nectarian

Table of Contents

[#McLaughlin McLaughlin]
[#McLaughlin-Images Images]
[#McLaughlin-Maps Maps]
[#McLaughlin-Description Description]
[#McLaughlin-Description: Wikipedia Description: Wikipedia]
[#McLaughlin-Additional Information Additional Information]
[#McLaughlin-Nomenclature Nomenclature]
[#McLaughlin-LPOD Articles LPOD Articles]
[#McLaughlin-Bibliography Bibliography]
external image normal_mclaughlin-clem1.jpgMcLaughlin.jpg
left: Clementine . right: LROC

Images

LPOD Photo Gallery Lunar Orbiter Images

  • McLaughlin was captured in Lunar Orbiter IV's frame LO-IV-190-med, north of the Lorentz-Nernst-Rontgen group, and south of the Poczobutt group (about "halfway" between these two groups).
  • Research Lunar Orbiter IV photography: Danny Caes



Maps

(LAC zone 36B1) USGS Digital Atlas PDF

Description


Description: Wikipedia

McLaughlin

Additional Information


Nomenclature

Dean Benjamin McLaughlin (October 25, 1901 - December 8, 1965) was an American astronomer. In 1954 he proposed the theory that there are volcanoes on Mars and that their eruptions change the albedo features called "mare" (The martian equivalent of Lunar mare). Today we know that there are indeed (most likely currently inactive) volcanoes on Mars, however they are not the cause for any changes on its surface.
- Erroneously printed as McLaughin (without the second "l") on page 78 (libration chart 7) in the 21st Century Atlas of the Moon (2012).- DannyCaes DannyCaes Jan 23, 2013

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 - afx3u2