Difference between revisions of "May 5, 2005"

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<p align="center" class="main_titles"><b>Author &amp; Editor:</b><br>  
 
<p align="center" class="main_titles"><b>Author &amp; Editor:</b><br>  
 
[mailto:tychocrater@yahoo.com Charles A. Wood]</p>
 
[mailto:tychocrater@yahoo.com Charles A. Wood]</p>
<p align="center" class="main_titles"><b>Technical Consultant:</b><br>
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[mailto:anthony@perseus.gr Anthony Ayiomamitis]</p>
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<p align="center" class="main_titles"><b>Contact Translator:</b><br>
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[mailto:pablolonnie@yahoo.com.mx Pablo Lonnie Pacheco Railey]  (Es)<br>
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[mailto:chlegrand@free.fr Christian Legrand] (Fr)</p>
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<p align="center" class="main_titles"><b>[mailto:webuser@observingthesky.org Contact Webmaster]</b></p>
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<p align="center" class="main_titles"><b>A service of:</b><br>
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[http://www.observingthesky.org/ ObservingTheSky.Org]</p>
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<p align="center" class="main_titles"><b>Visit these other PODs:</b> <br>
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[http://antwrp.gsfc.nasa.gov/apod/astropix.html Astronomy] | [http://www.msss.com/ Mars] | [http://epod.usra.edu/ Earth]</p>
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Latest revision as of 15:15, 15 March 2015

Grimaldi Dome


LPOD-2005-05-05.jpeg

LPOD-2005-05-05b.jpeg

Image Credit: K.C. Pau


Grimaldi Dome

Grimaldi is a small impact basin always seen as a chubby ellipse because of its location near the western limb. It is more easily recognized when the sun is high and it’s mare patch makes a distinctive dark spot. With a lower sun, Grimaldi’s mare patch is seen to be relatively smooth with a cluster of small hills to the north. But with even lower sun and larger image scale as in KC’s wonderful image above, more subtle features become visible. There are two or three ghost craters whose partial rims appear as arcuate mare ridges. But most interesting is the complexity of the well known dome on the left (north) side of the image. This dome is about 22 km wide and it’s west (bottom) side seems steeper than it’s east edge. A few bright peaks protrude slightly above the dome and a small flat-floored depression occurs just off-center. This Grimaldi dome looks multi-lobed like a heart, but none of it except the bright hills are visible on the higher sun Lunar Orbiter IV view. On the strongly stretched view (mouseover) there are some other very small dome-like bumps, one near the heart dome and two or three nearer the ghost crater in the southern half of the floor. And have you noticed that this patch of maria has no name? Since Grimaldi is an impact basin it is obvious that the name must be Mare Grimaldi! Or maybe, since it is a small basin, Lacus Grimaldi.

Chuck Wood

Technical Details:
April 22, 2005 with 10" newtonian + 5X barlow + Philips Toucam Pro.

Related Links:
Lunar Orbiter IV View

Yesterday's LPOD: Musical Nomenclature

Tomorrow's LPOD: A Handy New Map



Author & Editor:
Charles A. Wood

 


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