Difference between revisions of "June 3, 2012"
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| − | <em>LRO WAC mosaic processed by [mailto:mauricejscollins@hotmail.com | + | <em>LRO WAC mosaic processed by [mailto:mauricejscollins@hotmail.com Maurice Collins], New Zealand</em><br /> |
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The Lunar Reconnaissance Orbiter images demand a re-cataloging of many types of lunar features, especially rilles.<br /> | The Lunar Reconnaissance Orbiter images demand a re-cataloging of many types of lunar features, especially rilles.<br /> | ||
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mosaic that Maurice has constructed using individual low Sun WAC images. The bottom half is the steely surface of<br /> | mosaic that Maurice has constructed using individual low Sun WAC images. The bottom half is the steely surface of<br /> | ||
Mare Frigoris, and immediately above it is an older material - it has a lot higher density of small craters - which is<br /> | Mare Frigoris, and immediately above it is an older material - it has a lot higher density of small craters - which is<br /> | ||
| − | [http://www.lpi.usra.edu/meetings/lpsc2000/pdf/1822.pdf | + | [http://www.lpi.usra.edu/meetings/lpsc2000/pdf/1822.pdf probably] ejecta from the formation of Imbrium and smaller cratering events. Two named rilles cross the older terrain,<br /> |
the Sheepshanks Rille on the left, and the more conspicuous (probably because it is about perpendicular to the<br /> | the Sheepshanks Rille on the left, and the more conspicuous (probably because it is about perpendicular to the<br /> | ||
illumination) Gärtner Rille inside the crater with that name. As pointed out [http://lpod.wikispaces.com/May+14%2C+2010 previously], these two rilles seem to connect<br /> | illumination) Gärtner Rille inside the crater with that name. As pointed out [http://lpod.wikispaces.com/May+14%2C+2010 previously], these two rilles seem to connect<br /> | ||
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QuickMap Path tool shows no consistent downslope direction that might be relevant if these rilles formed by lava flowing<br /> | QuickMap Path tool shows no consistent downslope direction that might be relevant if these rilles formed by lava flowing<br /> | ||
through a channel or tube, so the rilles probably formed instead as a result of a dike carrying magma underground.<br /> | through a channel or tube, so the rilles probably formed instead as a result of a dike carrying magma underground.<br /> | ||
| − | A shadow-filled elongated crater at bottom right is seen in the higher Sun QuickMap [http://target.lroc.asu.edu/da/qmap.html?mv=eqc&mcx=1124125.19461&mcy=1687130.12724&mz=8 | + | A shadow-filled elongated crater at bottom right is seen in the higher Sun QuickMap [http://target.lroc.asu.edu/da/qmap.html?mv=eqc&mcx=1124125.19461&mcy=1687130.12724&mz=8 mosaic] to be a slightly eroded<br /> |
vee-shaped volcanic vent similar to [http://lpod.wikispaces.com/April+22%2C+2009 The Kiss]. Finally, at the top center of the image on the floor of Kane the shading <br /> | vee-shaped volcanic vent similar to [http://lpod.wikispaces.com/April+22%2C+2009 The Kiss]. Finally, at the top center of the image on the floor of Kane the shading <br /> | ||
suggests a dimple with a low dome to its east. Like all areas of the Moon, the more you look, the more you find of interest.<br /> | suggests a dimple with a low dome to its east. Like all areas of the Moon, the more you look, the more you find of interest.<br /> | ||
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| − | <em>[mailto:tychocrater@yahoo.com | + | <em>[mailto:tychocrater@yahoo.com Chuck Wood]</em><br /> |
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<strong>Related Links</strong><br /> | <strong>Related Links</strong><br /> | ||
Revision as of 17:50, 11 January 2015
A Kiss, a Dimple And Self-Same Rille
LRO WAC mosaic processed by Maurice Collins, New Zealand
The Lunar Reconnaissance Orbiter images demand a re-cataloging of many types of lunar features, especially rilles.
The NAC images are not very useful for multi-kilometer scale features, but the 100 m resolution of the Wide Angle
Camera (WAC) images and mosaics are about ten times better than the best terrestrial views, leading to detection of
previously unnoticed rilles and a much better depiction of known ones. An example of the latter case is shown in this
mosaic that Maurice has constructed using individual low Sun WAC images. The bottom half is the steely surface of
Mare Frigoris, and immediately above it is an older material - it has a lot higher density of small craters - which is
probably ejecta from the formation of Imbrium and smaller cratering events. Two named rilles cross the older terrain,
the Sheepshanks Rille on the left, and the more conspicuous (probably because it is about perpendicular to the
illumination) Gärtner Rille inside the crater with that name. As pointed out previously, these two rilles seem to connect
and be a single complex structure. This new wider view and lower Sun mosaic provides more details. The west end of
the rille may have originally continued further, and may now be covered by Frigoris lavas. A rille crosses the main one
near the middle of the Sheepshanks component and a nexus of shorter rilles occurs to the south. A near-circular rille
pattern exists at the northern end of the Gärtner Rille, and the rille continues fiurther east than previously seen. The
QuickMap Path tool shows no consistent downslope direction that might be relevant if these rilles formed by lava flowing
through a channel or tube, so the rilles probably formed instead as a result of a dike carrying magma underground.
A shadow-filled elongated crater at bottom right is seen in the higher Sun QuickMap mosaic to be a slightly eroded
vee-shaped volcanic vent similar to The Kiss. Finally, at the top center of the image on the floor of Kane the shading
suggests a dimple with a low dome to its east. Like all areas of the Moon, the more you look, the more you find of interest.
Chuck Wood
Related Links
Rükl plates 5 & 6
