Difference between revisions of "October 10, 2004"

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    <tr><td><div align="center" class="main_sm">Image Credit: [mailto:mariosantiago@sapo.pt Mario Santiago ]</p>
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<tr><td><div align="center" class="main_sm">Image Credit: [mailto:mariosantiago@sapo.pt Mario Santiago ]</p>
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<p align="center"><b>Professor and Student</b></p>
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<p align="center"><b>Professor and Student</b></p>
<p align="left">Giovanni Baptista Riccioli was a 17th century Jesuit scientist who devised the system of names still used on the Moon. His nomenclature was displayed on a map constructed by his former student Francesco Maria Grimaldi. To commemorate their hard work, Riccioli named a crater after each of them, and modestly gave the larger to his student. The crater Riccioli (diameter 145 km) is striated with ejecta from the formation of the Orientale impact basin to the southwest. The lack of ejecta on the mare patch on the floor of Grimaldi (230 km) demonstrates that the lava flows there and the small patch in Riccioli erupted more recently than 3.84 billion years ago, Orientale's birthday. Crater counts suggest that the Riccioli mare leak is about 3.48 b.y. old and Grimaldi has ages of 3.25 and 2.50 b.y. This latter age is remarkably, perhaps even suspiciously young. More interesting to telescopic observers are details seen on the floor of Grimaldi. The large dome on the northern portion of the mare (circled on mouseover) is well known, and Mario's image also shows some smaller and steeper hills north of the big dome. Because these appear in the higher sun Lunar Orbiter IV view, these hills are most likely to be remnant pieces of Orientale ejecta that were not covered by the later lavas. But the largest of these hills (top one circled on the mouseover) is more complex - on the Orbiter image it looks like a steep-sided dome with small hills on its north and south edges. At the southwest edge of the mare there is a shadow (arrowed) which implies a relatively steep slope where the mare lava flows over the crater floor. Lunar mare lavas had a very fluid consistency, so it is always peculiar to find a steep slope - something was unusual there!</p>
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<p align="left">Giovanni Baptista Riccioli was a 17th century Jesuit scientist who devised the system of names still used on the Moon. His nomenclature was displayed on a map constructed by his former student Francesco Maria Grimaldi. To commemorate their hard work, Riccioli named a crater after each of them, and modestly gave the larger to his student. The crater Riccioli (diameter 145 km) is striated with ejecta from the formation of the Orientale impact basin to the southwest. The lack of ejecta on the mare patch on the floor of Grimaldi (230 km) demonstrates that the lava flows there and the small patch in Riccioli erupted more recently than 3.84 billion years ago, Orientale's birthday. Crater counts suggest that the Riccioli mare leak is about 3.48 b.y. old and Grimaldi has ages of 3.25 and 2.50 b.y. This latter age is remarkably, perhaps even suspiciously young. More interesting to telescopic observers are details seen on the floor of Grimaldi. The large dome on the northern portion of the mare (circled on mouseover) is well known, and Mario's image also shows some smaller and steeper hills north of the big dome. Because these appear in the higher sun Lunar Orbiter IV view, these hills are most likely to be remnant pieces of Orientale ejecta that were not covered by the later lavas. But the largest of these hills (top one circled on the mouseover) is more complex - on the Orbiter image it looks like a steep-sided dome with small hills on its north and south edges. At the southwest edge of the mare there is a shadow (arrowed) which implies a relatively steep slope where the mare lava flows over the crater floor. Lunar mare lavas had a very fluid consistency, so it is always peculiar to find a steep slope - something was unusual there!</p>
<blockquote><p align="right">&#8212; [mailto:chuck@observingthesky.org Chuck Wood]</blockquote>
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<blockquote><p align="right">&#8212; [mailto:tychocrater@yahoo.com Chuck Wood]</blockquote>
 
<p align="left"><p><b>Technical Details:</b><br>
 
<p align="left"><p><b>Technical Details:</b><br>
 
03/04/2004 23 47 UT, STF Mirage 7 Deluxe Maksutov-Cassegrain + Toucam 840K + infra-red filter</p>
 
03/04/2004 23 47 UT, STF Mirage 7 Deluxe Maksutov-Cassegrain + Toucam 840K + infra-red filter</p>
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<br>Rukl <i>Atlas of the Moon</i> Sheet 39
 
<br>Rukl <i>Atlas of the Moon</i> Sheet 39
 
<p align="left"><b>Tomorrow's LPOD: </b> Fertility Central</p>
 
<p align="left"><b>Tomorrow's LPOD: </b> Fertility Central</p>
<p><img src="MainPage/spacer.gif" width="640" height="1"></p></td>
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<p align="center" class="main_titles"><b>Author &amp; Editor:</b><br>  
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<p align="center" class="main_titles"><b>Author &amp; Editor:</b><br>  
[mailto:chuck@observingthesky.org Charles A. Wood]</p>
+
[mailto:tychocrater@yahoo.com Charles A. Wood]</p>
<p align="center" class="main_titles"><b>Technical Consultant:</b><br>
+
<p align="center" class="main_titles"><b>Technical Consultant:</b><br>
[mailto:anthony@perseus.gr Anthony Ayiomamitis]</p>
+
[mailto:anthony@perseus.gr Anthony Ayiomamitis]</p>
<p align="center" class="main_titles"><b>Contact Translator:</b><br>
+
<p align="center" class="main_titles"><b>Contact Translator:</b><br>
[mailto:pablolonnie@yahoo.com.mx" class="one Pablo Lonnie Pacheco Railey]  (Es)<br>
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[mailto:pablolonnie@yahoo.com.mx" class="one Pablo Lonnie Pacheco Railey]  (Es)<br>
[mailto:chlegrand@free.fr" class="one Christian Legrand] (Fr)</p>
+
[mailto:chlegrand@free.fr" class="one Christian Legrand] (Fr)</p>
<p align="center" class="main_titles"><b>[mailto:webuser@observingthesky.org Contact Webmaster]</b></p>
+
<p align="center" class="main_titles"><b>[mailto:webuser@observingthesky.org Contact Webmaster]</b></p>
<p align="center" class="main_titles"><b>A service of:</b><br>
+
<p align="center" class="main_titles"><b>A service of:</b><br>
[http://www.observingthesky.org/" class="one ObservingTheSky.Org]</p>
+
[http://www.observingthesky.org/" class="one ObservingTheSky.Org]</p>
<p align="center" class="main_titles"><b>Visit these other PODs:</b> <br>
+
<p align="center" class="main_titles"><b>Visit these other PODs:</b> <br>
[http://antwrp.gsfc.nasa.gov/apod/astropix.html" class="one Astronomy] | [http://www.msss.com/" class="one Mars] | [http://epod.usra.edu/" class="one Earth]</p>
+
[http://antwrp.gsfc.nasa.gov/apod/astropix.html" class="one Astronomy] | [http://www.msss.com/" class="one Mars] | [http://epod.usra.edu/" class="one Earth]</p>
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<p>&nbsp;</p>
 
<p>&nbsp;</p>
 
 
 
 
 
----
 
----
 
===COMMENTS?===  
 
===COMMENTS?===  
 
Click on this icon [[image:PostIcon.jpg]] at the upper right to post a comment.
 
Click on this icon [[image:PostIcon.jpg]] at the upper right to post a comment.

Revision as of 18:26, 4 January 2015

Professor and Student

<nobr>Professor and Student</nobr>

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Image Credit: Mario Santiago


Professor and Student

Giovanni Baptista Riccioli was a 17th century Jesuit scientist who devised the system of names still used on the Moon. His nomenclature was displayed on a map constructed by his former student Francesco Maria Grimaldi. To commemorate their hard work, Riccioli named a crater after each of them, and modestly gave the larger to his student. The crater Riccioli (diameter 145 km) is striated with ejecta from the formation of the Orientale impact basin to the southwest. The lack of ejecta on the mare patch on the floor of Grimaldi (230 km) demonstrates that the lava flows there and the small patch in Riccioli erupted more recently than 3.84 billion years ago, Orientale's birthday. Crater counts suggest that the Riccioli mare leak is about 3.48 b.y. old and Grimaldi has ages of 3.25 and 2.50 b.y. This latter age is remarkably, perhaps even suspiciously young. More interesting to telescopic observers are details seen on the floor of Grimaldi. The large dome on the northern portion of the mare (circled on mouseover) is well known, and Mario's image also shows some smaller and steeper hills north of the big dome. Because these appear in the higher sun Lunar Orbiter IV view, these hills are most likely to be remnant pieces of Orientale ejecta that were not covered by the later lavas. But the largest of these hills (top one circled on the mouseover) is more complex - on the Orbiter image it looks like a steep-sided dome with small hills on its north and south edges. At the southwest edge of the mare there is a shadow (arrowed) which implies a relatively steep slope where the mare lava flows over the crater floor. Lunar mare lavas had a very fluid consistency, so it is always peculiar to find a steep slope - something was unusual there!

Chuck Wood

Technical Details:
03/04/2004 23 47 UT, STF Mirage 7 Deluxe Maksutov-Cassegrain + Toucam 840K + infra-red filter

Related Links:
Lunar Orbiter IV View
Rukl Atlas of the Moon Sheet 39

Tomorrow's LPOD: Fertility Central



Author & Editor:
Charles A. Wood

Technical Consultant:
Anthony Ayiomamitis

Contact Translator:
" class="one Pablo Lonnie Pacheco Railey (Es)
" class="one Christian Legrand (Fr)

Contact Webmaster

A service of:
" class="one ObservingTheSky.Org

Visit these other PODs:
" class="one Astronomy | " class="one Mars | " class="one Earth

 


COMMENTS?

Click on this icon File:PostIcon.jpg at the upper right to post a comment.