Difference between revisions of "July 4, 2004"
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=Threading the Pillars= | =Threading the Pillars= | ||
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| − | + | <td><div align="center" span class="main_sm">Image Credit: [mailto:kcpaulhk@yahoo.com.hk" class="one KC Pau]</div></td> | |
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| − | + | <table class="story" border="0" bgcolor="#FFFFFF" width="90%" cellpadding="10" align="center"><tr><td> | |
| − | + | <p class="story" align="center"><b>Threading the Pillars</b></p> | |
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| − | + | [http://www.lpod.org/LPOD-2004-01-15.htm Gassendi] steals the limelight when the Moon is 11 days old, but there are other less prominent features nearby that tell interesting stories. To the northeast of Gassendi at the southern end of Oceanus Procellarum is a very delicate rille with an important connection to Mare Humorum. West of the 15 km wide crater Herigonius - mouseover for names - is the Herigonius sinuous rille. It begins in a small pit on the Ewing mare ridge and meanders first to the west and then southward toward Humorum. On KC's image the rising sun reflects like a bright sinuous snake from the western wall of the narrow rille (white arrows). The rille curves around low mare ridges - which thus must have been there first - and west of the crater Herigonius K merges invisibly with a second fainter rille (black arrows). The combined rilles flow between two elongated ridges that I call the Pillars and dies out to the south. Spectral mapping shows that the basalts that emptied from the sinuous rilles - which are lava channels - are dark, medium -titanium lavas. These lavas apparently flowed south (long white arrow) and filled the central-eastern portion of Mare Humorum. Thus, the thin rille that you can just barely detect in a telescope is the channel that delivered most of the visible lava in Mare [http://www.lpod.org/LPOD-2004-02-18.htm Humorum]! | |
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| − | + | <p align="right" class="story">— [mailto:tychocrater@yahoo.com Chuck Wood]</blockquote> | |
| − | + | <p class="story" align="left"><b>Technical Details:</b><br> | |
| − | + | 28 Jun 2004, 13h21m (UT), 10" Newtonian with 2.5X barlow and Philips Toucam Pro. | |
| − | + | <p class="story" align="left"><b>Related Links: </b><br> | |
| − | + | [http://www.lpi.usra.edu/research/lunar_orbiter/images/img/iv_137_h2.jpg Lunar Orbiter IV View] <br> | |
| − | + | [http://www.lpi.usra.edu/research/apollo/images/AS16/119/19162.jpg Apollo 16 View] | |
| − | + | <p class="story"><b>Tomorrow's LPOD:</b> Insularum Interlude</p> | |
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| − | + | <td><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>A service of:</b><br> | |
| − | + | [http://www.observingthesky.org/ ObservingTheSky.Org]</p> | |
| − | + | <p align="center" class="main_titles"><b>Visit these other PODs:</b> <br> | |
| − | + | [http://antwrp.gsfc.nasa.gov/apod/astropix.html Astronomy] | [http://www.msss.com/ Mars] | [http://epod.usra.edu/ Earth]</p></td> | |
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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 18:22, 4 January 2015
Threading the Pillars
[javascript:;" onMouseOver="MM_swapImage('Image1',,'images/LPOD-2004-07-04b.jpeg',1)" onMouseOut="MM_swapImgRestore() |
Image Credit: " class="one KC Pau |
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Threading the Pillars Gassendi steals the limelight when the Moon is 11 days old, but there are other less prominent features nearby that tell interesting stories. To the northeast of Gassendi at the southern end of Oceanus Procellarum is a very delicate rille with an important connection to Mare Humorum. West of the 15 km wide crater Herigonius - mouseover for names - is the Herigonius sinuous rille. It begins in a small pit on the Ewing mare ridge and meanders first to the west and then southward toward Humorum. On KC's image the rising sun reflects like a bright sinuous snake from the western wall of the narrow rille (white arrows). The rille curves around low mare ridges - which thus must have been there first - and west of the crater Herigonius K merges invisibly with a second fainter rille (black arrows). The combined rilles flow between two elongated ridges that I call the Pillars and dies out to the south. Spectral mapping shows that the basalts that emptied from the sinuous rilles - which are lava channels - are dark, medium -titanium lavas. These lavas apparently flowed south (long white arrow) and filled the central-eastern portion of Mare Humorum. Thus, the thin rille that you can just barely detect in a telescope is the channel that delivered most of the visible lava in Mare Humorum! Technical Details: Related Links: Tomorrow's LPOD: Insularum Interlude |
Author & Editor: Technical Consultant: A service of: |
COMMENTS?
Click on this icon File:PostIcon.jpg at the upper right to post a comment.
