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=A Long Graben= | =A Long Graben= | ||
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| − | + | <td><div align="center" span class="main_sm">Image Credit: [mailto:tbash@ptd.net" class="one Tom Bash ]</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>A Long Graben</b></p> | |
| − | + | <p class="story" align="left"> | |
| − | + | Graben is a German word meaning ditch or trough. Geologically, graben form by the dropping downward of a linear block between two parallel faults. Terrestrial graben typically occur in regions of extension - where forces pull the surface apart in directions perpendicular to the resulting graben. This image shows the long linear Sirsalis Rrille, which appears to be lunar graben. High resolution Lunar Orbiter images show that the rille widens where it cuts topographically high land, implying that its side faults steeply dip at an angle of about 60 degrees from the horizontal. Jim Head and Lionel Wilson propose that the extension that allows lunar graben to form is due to the displacement of the crust due to the rise of a dike (or dyke for UK readers) that carries magma toward the surface. At the Parry Rille, near Fra Mauro, the dike reached the surface, constructing small cones and spreading pyroclastic material. There is no evidence of associated volcanism along the Sirsalis Rille so that dike solidified before its magma reached the lunar surface. From the width (about 4 km maximum) and depth (230 m) Head and Wilson calculate that the dike that formed the Sirsalis Rille is about 600 - 700 m wide and rose to about 2.4 km below the surface. This dikes is amazing for it rose nearly 100 km from its source of magma! And remember that the Sirsalis Rille is about 350-400 km long, so its dike must be a thin sheet of magma that slices thru the lunar crust and upper mantle. Amazing! specially if true! And it is probably true, for one of the strongest magnetic fields on the Moon traces the Sirsalis Rille - its solidified dike must be the source of the magnetic field. | |
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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> | |
| − | + | March 4, 2004, using a C11 with a ToUcam web cam. | |
| − | + | <p class="story" align="left"><b>Related Links: </b><br> | |
| − | + | Head & Wilson (1993) Lunar graben formation due to near-surface deformation accompanying dike emplacement. <i>Planet. Space Sci.</i> 41, 719-727.<br> | |
| − | + | [http://www.lpi.usra.edu/research/lunar_orbiter/bin/info.shtml?459 Lunar Orbiter IV View] | |
| − | + | <p class="story"><b>Tomorrow's LPOD:</b> Transient TLP</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
A Long Graben
[javascript:;" onMouseOver="MM_swapImage('Image1',,'images/LPOD-2004-07-06b.jpeg',1)" onMouseOut="MM_swapImgRestore() |
Image Credit: " class="one Tom Bash |
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A Long Graben Graben is a German word meaning ditch or trough. Geologically, graben form by the dropping downward of a linear block between two parallel faults. Terrestrial graben typically occur in regions of extension - where forces pull the surface apart in directions perpendicular to the resulting graben. This image shows the long linear Sirsalis Rrille, which appears to be lunar graben. High resolution Lunar Orbiter images show that the rille widens where it cuts topographically high land, implying that its side faults steeply dip at an angle of about 60 degrees from the horizontal. Jim Head and Lionel Wilson propose that the extension that allows lunar graben to form is due to the displacement of the crust due to the rise of a dike (or dyke for UK readers) that carries magma toward the surface. At the Parry Rille, near Fra Mauro, the dike reached the surface, constructing small cones and spreading pyroclastic material. There is no evidence of associated volcanism along the Sirsalis Rille so that dike solidified before its magma reached the lunar surface. From the width (about 4 km maximum) and depth (230 m) Head and Wilson calculate that the dike that formed the Sirsalis Rille is about 600 - 700 m wide and rose to about 2.4 km below the surface. This dikes is amazing for it rose nearly 100 km from its source of magma! And remember that the Sirsalis Rille is about 350-400 km long, so its dike must be a thin sheet of magma that slices thru the lunar crust and upper mantle. Amazing! specially if true! And it is probably true, for one of the strongest magnetic fields on the Moon traces the Sirsalis Rille - its solidified dike must be the source of the magnetic field. Technical Details: Related Links: Tomorrow's LPOD: Transient TLP |
Author & Editor: Technical Consultant: A service of: |
COMMENTS?
Click on this icon File:PostIcon.jpg at the upper right to post a comment.
