Difference between revisions of "February 17, 2005"
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− | + | <td width="50%"><h2><nobr>Keeping Up With The Smythiis</nobr></h2></td> | |
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<table width="80%" border="0" align="center" cellpadding="8"> | <table width="80%" border="0" align="center" cellpadding="8"> | ||
− | + | <tr><td><div align="center" class="main_sm">Image Credit: [mailto:mariosantiago@sapo.pt Mario Santiago]</p> | |
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<table class="story" border="0" bgcolor="#FFFFFF" width="90%" cellpadding="10" align="center"><tr><td> | <table class="story" border="0" bgcolor="#FFFFFF" width="90%" cellpadding="10" align="center"><tr><td> | ||
− | + | <p align="center"><b>Keeping Up With The Smythiis</b></p> | |
− | + | <p align="left">The equatorial eastern limb of the Moon is more interesting than much of the terrain immediately nearer the Earthside. The reason is twofold: (1) the area between Crisium and Fecunditatis and the limb is boring because it lacks any distinctive large fresh craters, and instead is a mishmash of older, look-alike craters flooded with and surrounded by mare material; and (2) the limb is home to two maria – [http://www.lpod.org/LPOD-2004-10-09.htm Marginis ] and Smythii – that occupy two impact basins. Of the two, Smythii offers more vestiges of its basin structure – principally its well-defined, curved rim. When the sunset terminator is just east of Smythii you can observe the shadow cast by the rim and appreciate that the mare is substantially lower than the rim. In fact, Clementine altimeter readings show that the rim rises an amazing 6-8 km above the mare. The circular outline of the rim is clearly demonstrated in Mario’s rectified view (mouseover) of Smythii made using PlanetWarp. Also clear is the two different shades of mare lavas. Crater counts imply that the darker Smythii lavas may be among the youngest on the Moon, perhaps 1.5 b.y. old.</p> | |
− | + | <blockquote><p align="right">— [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> | ||
13/02/2005 at 18:09/18:15 UT (in daylight!). 2 images mosaic made with Orion SkyView Pro Newtonian (8 inches f/5) + Ccd Atik 2HS + Barlow 2x + Qcfocus + Registax. Planet Warp v.1 used for warped image.</p> | 13/02/2005 at 18:09/18:15 UT (in daylight!). 2 images mosaic made with Orion SkyView Pro Newtonian (8 inches f/5) + Ccd Atik 2HS + Barlow 2x + Qcfocus + Registax. Planet Warp v.1 used for warped image.</p> | ||
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Rukl Plates 38 & 49 | Rukl Plates 38 & 49 | ||
<p align="left"><b>Tomorrow's LPOD: </b> Memory of a Crater</p> | <p align="left"><b>Tomorrow's LPOD: </b> Memory of a Crater</p> | ||
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</table> | </table> | ||
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− | + | <td><hr></td> | |
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− | + | <p align="center" class="main_titles"><b>Author & Editor:</b><br> | |
− | + | [mailto:tychocrater@yahoo.com Charles A. Wood]</p> | |
− | + | <p align="center" class="main_titles"><b>Technical Consultant:</b><br> | |
− | + | [mailto:anthony@perseus.gr Anthony Ayiomamitis]</p> | |
− | + | <p align="center" class="main_titles"><b>Contact Translator:</b><br> | |
− | + | [mailto:pablolonnie@yahoo.com.mx" class="one Pablo Lonnie Pacheco Railey] (Es)<br> | |
− | + | [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>A service of:</b><br> | |
− | + | [http://www.observingthesky.org/" class="one ObservingTheSky.Org]</p> | |
− | + | <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> | |
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</table> | </table> | ||
<p> </p> | <p> </p> | ||
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===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 18:29, 4 January 2015
Keeping Up With The Smythiis
<nobr>Keeping Up With The Smythiis</nobr> |
[#" onMouseOver = "document.images['main_image'].src='archive/2005/02/images/LPOD-2005-02-17b.jpeg'; return true" onMouseOut = "document.images['main_image'].src='archive/2005/02/images/LPOD-2005-02-17.jpeg'; return false <img src="archive/2005/02/images/LPOD-2005-02-17.jpeg" name="main_image" border="0" id="main_image">] |
Image Credit: Mario Santiago
|
Keeping Up With The Smythiis The equatorial eastern limb of the Moon is more interesting than much of the terrain immediately nearer the Earthside. The reason is twofold: (1) the area between Crisium and Fecunditatis and the limb is boring because it lacks any distinctive large fresh craters, and instead is a mishmash of older, look-alike craters flooded with and surrounded by mare material; and (2) the limb is home to two maria – Marginis and Smythii – that occupy two impact basins. Of the two, Smythii offers more vestiges of its basin structure – principally its well-defined, curved rim. When the sunset terminator is just east of Smythii you can observe the shadow cast by the rim and appreciate that the mare is substantially lower than the rim. In fact, Clementine altimeter readings show that the rim rises an amazing 6-8 km above the mare. The circular outline of the rim is clearly demonstrated in Mario’s rectified view (mouseover) of Smythii made using PlanetWarp. Also clear is the two different shades of mare lavas. Crater counts imply that the darker Smythii lavas may be among the youngest on the Moon, perhaps 1.5 b.y. old. Technical Details: Related Links: Tomorrow's LPOD: Memory of a Crater |
Author & Editor: Technical Consultant: Contact Translator: A service of: Visit these other PODs: |
COMMENTS?
Click on this icon File:PostIcon.jpg at the upper right to post a comment.