Difference between revisions of "April 8, 2010"
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| − | <em>image by [mailto:jocelyn.serot@wanadoo.fr | + | <em>image by [mailto:jocelyn.serot@wanadoo.fr Jocelyn Sérot], France</em><br /> |
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| − | What a land of contrasts. Smooth mare lavas from circular-edged Sinus Aestuum at upper left embay and truncate the highly textured hilly terrain left of the image center. The hilly stuff is Imbrium ejecta laid down hundreds of millions of years before these lavas erupted onto the low spots. At bottom right are Pallas and Murchison, which formed before Imbrium as evidenced by the erosion of their rims and [http://www.lpod.org/?m=20061102 | + | What a land of contrasts. Smooth mare lavas from circular-edged Sinus Aestuum at upper left embay and truncate the highly textured hilly terrain left of the image center. The hilly stuff is Imbrium ejecta laid down hundreds of millions of years before these lavas erupted onto the low spots. At bottom right are Pallas and Murchison, which formed before Imbrium as evidenced by the erosion of their rims and [http://www.lpod.org/?m=20061102 flow] of rough pasty ejecta onto Pallas' floor. The Bode III rille meanders northward just above its namesake crater (the biggest one, nearly full of shadows), and Bode I (both numbers from the <em>System of Lunar Craters</em> chart D4) is near top center of the image; I wonder if they were once connected as a single rille? This is a wondrously smooth-toned image that invites further exploration.<br /> |
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| − | <em>[mailto:tychocrater@yahoo.com | + | <em>[mailto:tychocrater@yahoo.com Chuck Wood]</em><br /> |
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<strong>Technical Details</strong><br /> | <strong>Technical Details</strong><br /> | ||
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| − | <div>You can support LPOD when you buy any book from Amazon thru [http://www.lpod.org/?page_id=591 | + | <div>You can support LPOD when you buy any book from Amazon thru [http://www.lpod.org/?page_id=591 LPOD!]<br /> |
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===COMMENTS?=== | ===COMMENTS?=== | ||
| − | + | Register, and click on the <b>Discussion</b> tab at the top of the page. | |
Revision as of 17:18, 11 January 2015
Textured Ejecta
image by Jocelyn Sérot, France
What a land of contrasts. Smooth mare lavas from circular-edged Sinus Aestuum at upper left embay and truncate the highly textured hilly terrain left of the image center. The hilly stuff is Imbrium ejecta laid down hundreds of millions of years before these lavas erupted onto the low spots. At bottom right are Pallas and Murchison, which formed before Imbrium as evidenced by the erosion of their rims and flow of rough pasty ejecta onto Pallas' floor. The Bode III rille meanders northward just above its namesake crater (the biggest one, nearly full of shadows), and Bode I (both numbers from the System of Lunar Craters chart D4) is near top center of the image; I wonder if they were once connected as a single rille? This is a wondrously smooth-toned image that invites further exploration.
Chuck Wood
Technical Details
2010-03-22, 18h32 UT. Mewlon 210 @ F/D=24, DMK 31, Avistack+Registax (300/2500 im. stacked)
Related Links
Rükl plate 33
COMMENTS?
Register, and click on the Discussion tab at the top of the page.
