Difference between revisions of "LPOD June 13, 2008"
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| − | [[Image:LPOD-June13-08.jpg|LPOD-June13-08.jpg]]<br /> ''image by [mailto:mwirths@starband.net Mike Wirths]''<br /> <br /> Mike's back. After disappearing for six months, Mike has resurfaced in the Mexican state of Baja California, where the skies seem to be clear and his 18" Starmaster telescope is singing again. This image, with east up, is of a triple junction of rilles surrounding [ | + | [[Image:LPOD-June13-08.jpg|LPOD-June13-08.jpg]]<br /> ''image by [mailto:mwirths@starband.net Mike Wirths]''<br /> <br /> Mike's back. After disappearing for six months, Mike has resurfaced in the Mexican state of Baja California, where the skies seem to be clear and his 18" Starmaster telescope is singing again. This image, with east up, is of a triple junction of rilles surrounding [[Promontorium%20Archerusia|Promontorium Archerusia]], with Plinius above all. On the left are the [[Rimae%20Menelaus|Menelaus Rilles]], presumably formed when the load of younger mare (with the ridges) in the middle of Serenitatis, caused crustal subsidence and fractures at the mare's edges. The [[Rimae%20Plinius|Plinius Rilles]] had the same origin. It is surprising though, that both rille sets don't curve to follow the basin rim, but rather ram right into the promontorium. Similarly, the [[Rimae%20Maclear|Maclear Rilles]], coming from the south, and nominally concentric to sagging mare lavas in Tranquillitatis, don't curve but also run into Prom. Archerusia. In fact, nearly all of the ''concentric'' rilles along the edges of Serenitatis and Tranquilitatis are straight - its only when looked at as a family that their concentricity is seen. I suppose the flexing of the maria at their edges creates the regional stress conditions that permit fracturing, but local, near surface conditions somehow limit the rilles to straight segments. Interestingly, the [[Rimae%20Hippalus|Hippalus Rilles]] are curved, running parallel to the presumed rim of the Humorum Basin. Perhaps their greater width indicates that they reach down to a greater depth, and are less controlled by near-surface weakenesses.<br /> <br /> ''Chuck Wood''<br /> <br /> '''Technical Details'''<br /> June 9, 2008. 18" Starmaster + 2.5 Televue barlow + Infinity 2-2 camera + red filter; processed with Registax 5 beta.<br /> <br /> '''Related Links'''<br /> Rükl plates 24 & 35<br /> <br /> <br /> |
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| − | '''COMMENTS'''<br /> <span style="FONT-SIZE: 80%">To [ | + | '''COMMENTS'''<br /> <span style="FONT-SIZE: 80%">To [[LPOD%20Comments|post comments]] regarding this LPOD you need to first register for the wiki by clicking the "Join this space" link under the Full Moon icon in the upper left corner of the screen, and wait for your membership to be approved. Once registered, you may still need to "Sign In" (link at top right of screen) to remove the "Protected" icon from the top of the LPOD page. Once you don't see a "Protected" icon, please click [http://the-moon.us/wiki/page/edit/LPOD+June+13,+2008 here] and enter your comment in the space below. ''Please do not edit the LPOD itself!''</span><br /> <br /> 1. Another thing I notice about this image is how the highland material has been raked in a direction that seems to be radial to Mare Imbrium. I would suppose then that Mare Tranquilitatis and Serenitatis are older than Imbrium?<br /> <br /> <span style="FONT-FAMILY: Arial">(2) Taking in the bigger picture, isn't the area behind Menelaus a trough of Serenetatis, where one also gets to see this rake-like appearance extending all the way up past Julius Caesar and Boscovich, and terminating just on Tranquillitatis's north-westerm shore? Interesting here too, I query, are parts of Auwers's crater (just right of Menelaus in the picture) rim predominantly trailing radially away (to the right in the picture) from the direction of Imbrium, which might give a sense as to its impact energy; assuming that Auwers is an old crater. </span><span style="FONT-FAMILY: Arial"> </span><span style="FONT-FAMILY: Arial">John - [http://www.moonposter.ie/ www.moonposter.ie] </span><br /> |
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Latest revision as of 15:57, 15 April 2018
STRAIGHT OR CONCENTRIC?
image by Mike Wirths
Mike's back. After disappearing for six months, Mike has resurfaced in the Mexican state of Baja California, where the skies seem to be clear and his 18" Starmaster telescope is singing again. This image, with east up, is of a triple junction of rilles surrounding Promontorium Archerusia, with Plinius above all. On the left are the Menelaus Rilles, presumably formed when the load of younger mare (with the ridges) in the middle of Serenitatis, caused crustal subsidence and fractures at the mare's edges. The Plinius Rilles had the same origin. It is surprising though, that both rille sets don't curve to follow the basin rim, but rather ram right into the promontorium. Similarly, the Maclear Rilles, coming from the south, and nominally concentric to sagging mare lavas in Tranquillitatis, don't curve but also run into Prom. Archerusia. In fact, nearly all of the concentric rilles along the edges of Serenitatis and Tranquilitatis are straight - its only when looked at as a family that their concentricity is seen. I suppose the flexing of the maria at their edges creates the regional stress conditions that permit fracturing, but local, near surface conditions somehow limit the rilles to straight segments. Interestingly, the Hippalus Rilles are curved, running parallel to the presumed rim of the Humorum Basin. Perhaps their greater width indicates that they reach down to a greater depth, and are less controlled by near-surface weakenesses.
Chuck Wood
Technical Details
June 9, 2008. 18" Starmaster + 2.5 Televue barlow + Infinity 2-2 camera + red filter; processed with Registax 5 beta.
Related Links
Rükl plates 24 & 35
COMMENTS
To post comments regarding this LPOD you need to first register for the wiki by clicking the "Join this space" link under the Full Moon icon in the upper left corner of the screen, and wait for your membership to be approved. Once registered, you may still need to "Sign In" (link at top right of screen) to remove the "Protected" icon from the top of the LPOD page. Once you don't see a "Protected" icon, please click here and enter your comment in the space below. Please do not edit the LPOD itself!
1. Another thing I notice about this image is how the highland material has been raked in a direction that seems to be radial to Mare Imbrium. I would suppose then that Mare Tranquilitatis and Serenitatis are older than Imbrium?
(2) Taking in the bigger picture, isn't the area behind Menelaus a trough of Serenetatis, where one also gets to see this rake-like appearance extending all the way up past Julius Caesar and Boscovich, and terminating just on Tranquillitatis's north-westerm shore? Interesting here too, I query, are parts of Auwers's crater (just right of Menelaus in the picture) rim predominantly trailing radially away (to the right in the picture) from the direction of Imbrium, which might give a sense as to its impact energy; assuming that Auwers is an old crater. John - www.moonposter.ie
