Difference between revisions of "October 23, 2009"
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<em>Lunar Orbiter V-M213 and H213 (right) images from [http://www.lpi.usra.edu/resources/lunarorbiter/mission/?5 LPI Lunar Orbiter Photo Gallery]</em><br /> | <em>Lunar Orbiter V-M213 and H213 (right) images from [http://www.lpi.usra.edu/resources/lunarorbiter/mission/?5 LPI Lunar Orbiter Photo Gallery]</em><br /> | ||
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| − | The Planetary Society's indefatigable Emily Lakdawalla [http://planetary.org/blog/article/00002173/ reports] that a team of Kaguya scientists is publishing an article about a skylight | + | The Planetary Society's indefatigable Emily Lakdawalla [http://planetary.org/blog/article/00002173/ reports] that a team of Kaguya scientists is publishing an article about a skylight |
| − | discovered in a rille in the Marius Hills. <em>Skylight</em> is the word that cavers use to describe collapses of a cave roof thus connecting the surface | + | discovered in a rille in the Marius Hills. <em>Skylight</em> is the word that cavers use to describe collapses of a cave roof thus connecting the surface |
| − | to the underground tunnel. The Marius Hills rilles, like all of the Moon's sinuous rilles, are most likely volcanic channels and tubes, so | + | to the underground tunnel. The Marius Hills rilles, like all of the Moon's sinuous rilles, are most likely volcanic channels and tubes, so |
| − | skylights are not unexpected; certainly they are common in terrestrial [http://outdoors.webshots.com/photo/1085338227044816609LLSZAI lava tubes]. But the Marius Hills lavas are probably about 3-3.5 b.y. | + | skylights are not unexpected; certainly they are common in terrestrial [http://outdoors.webshots.com/photo/1085338227044816609LLSZAI lava tubes]. But the Marius Hills lavas are probably about 3-3.5 b.y. |
| − | old so most lava tubes have long since been de-roofed by small scale meteorite cratering. The Kaguya discovery of a 65 m skylight is | + | old so most lava tubes have long since been de-roofed by small scale meteorite cratering. The Kaguya discovery of a 65 m skylight is |
| − | interesting because it is sharp-edged and may have formed much more recently than the rilles. There are a number of other skylight | + | interesting because it is sharp-edged and may have formed much more recently than the rilles. There are a number of other skylight |
| − | type depressions nearby and associated with other rilles that probably also mark lava tubes. In 1972 Dale Cruikshank and I published | + | type depressions nearby and associated with other rilles that probably also mark lava tubes. In 1972 Dale Cruikshank and I published |
| − | [http://articles.adsabs.harvard.edu/cgi-bin/nph-iarticle_query?1972Moon....3..412C&amp;data_type=PDF_HIGH&amp;whole_paper=YES&amp;type=PRINTER&amp;filetype=.pdf descriptions] of Hawaiian lava tubes and skylights and likely lunar examples. The image above is from our paper depicting two rilles in the | + | [http://articles.adsabs.harvard.edu/cgi-bin/nph-iarticle_query?1972Moon....3..412C&amp;data_type=PDF_HIGH&amp;whole_paper=YES&amp;type=PRINTER&amp;filetype=.pdf descriptions] of Hawaiian lava tubes and skylights and likely lunar examples. The image above is from our paper depicting two rilles in the |
| − | Marius Hills near the crater which may be the ~3 km wide Galilaei M. Both rilles appear to start on the edge of a volcanic hill, with the largest | + | Marius Hills near the crater which may be the ~3 km wide Galilaei M. Both rilles appear to start on the edge of a volcanic hill, with the largest |
| − | rille having a characteristic tadpole-like vent area. Beyond the crater M the large rille becomes a series of elongated pits extending about 10 | + | rille having a characteristic tadpole-like vent area. Beyond the crater M the large rille becomes a series of elongated pits extending about 10 |
| − | km and then a lack of collapses suggests a preserved tunnel whose direction is indicated by a cluster of pits about 8 km further to the southwest. | + | km and then a lack of collapses suggests a preserved tunnel whose direction is indicated by a cluster of pits about 8 km further to the southwest. |
| − | The narrower rille starts with a series of aligned pits and then has completely collapsed until near its southern end. There - seen better in the | + | The narrower rille starts with a series of aligned pits and then has completely collapsed until near its southern end. There - seen better in the |
| − | high res version of the same image on the right - the pits are elongated and taper but mostly do not touch. Although volcanological nomenclature | + | high res version of the same image on the right - the pits are elongated and taper but mostly do not touch. Although volcanological nomenclature |
| − | is often not well defined I would say that these pits, like those along the larger rille, are skylights. Because the mare between the pits is continuous | + | is often not well defined I would say that these pits, like those along the larger rille, are skylights. Because the mare between the pits is continuous |
| − | the underlying lava tube has not collapsed. The Marius Hills remain a fascinating area for high resolution imaging, but intact lava tubes are | + | the underlying lava tube has not collapsed. The Marius Hills remain a fascinating area for high resolution imaging, but intact lava tubes are |
| − | probably widespread across the lunar maria and may be enterable along skylights and abrupt rille terminations. | + | probably widespread across the lunar maria and may be enterable along skylights and abrupt rille terminations. |
<br /> | <br /> | ||
<em>[mailto:tychocrater@yahoo.com Chuck Wood]</em><br /> | <em>[mailto:tychocrater@yahoo.com Chuck Wood]</em><br /> | ||
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Rükl plate [http://the-moon.wikispaces.com/R%C3%BCkl+29 29]<br /> | Rükl plate [http://the-moon.wikispaces.com/R%C3%BCkl+29 29]<br /> | ||
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| + | <hr /> | ||
<p><b>Yesterday's LPOD:</b> [[October 22, 2009|The Other Apollo]] </p> | <p><b>Yesterday's LPOD:</b> [[October 22, 2009|The Other Apollo]] </p> | ||
<p><b>Tomorrow's LPOD:</b> [[October 24, 2009|Das Mystery]] </p> | <p><b>Tomorrow's LPOD:</b> [[October 24, 2009|Das Mystery]] </p> | ||
| − | < | + | <!-- End of content --> |
{{wiki/ArticleFooter}} | {{wiki/ArticleFooter}} | ||
Revision as of 18:58, 28 February 2015
Trail of Skylights
Lunar Orbiter V-M213 and H213 (right) images from LPI Lunar Orbiter Photo Gallery
The Planetary Society's indefatigable Emily Lakdawalla reports that a team of Kaguya scientists is publishing an article about a skylight
discovered in a rille in the Marius Hills. Skylight is the word that cavers use to describe collapses of a cave roof thus connecting the surface
to the underground tunnel. The Marius Hills rilles, like all of the Moon's sinuous rilles, are most likely volcanic channels and tubes, so
skylights are not unexpected; certainly they are common in terrestrial lava tubes. But the Marius Hills lavas are probably about 3-3.5 b.y.
old so most lava tubes have long since been de-roofed by small scale meteorite cratering. The Kaguya discovery of a 65 m skylight is
interesting because it is sharp-edged and may have formed much more recently than the rilles. There are a number of other skylight
type depressions nearby and associated with other rilles that probably also mark lava tubes. In 1972 Dale Cruikshank and I published
descriptions of Hawaiian lava tubes and skylights and likely lunar examples. The image above is from our paper depicting two rilles in the
Marius Hills near the crater which may be the ~3 km wide Galilaei M. Both rilles appear to start on the edge of a volcanic hill, with the largest
rille having a characteristic tadpole-like vent area. Beyond the crater M the large rille becomes a series of elongated pits extending about 10
km and then a lack of collapses suggests a preserved tunnel whose direction is indicated by a cluster of pits about 8 km further to the southwest.
The narrower rille starts with a series of aligned pits and then has completely collapsed until near its southern end. There - seen better in the
high res version of the same image on the right - the pits are elongated and taper but mostly do not touch. Although volcanological nomenclature
is often not well defined I would say that these pits, like those along the larger rille, are skylights. Because the mare between the pits is continuous
the underlying lava tube has not collapsed. The Marius Hills remain a fascinating area for high resolution imaging, but intact lava tubes are
probably widespread across the lunar maria and may be enterable along skylights and abrupt rille terminations.
Chuck Wood
Related Links
Rükl plate 29
Yesterday's LPOD: The Other Apollo
Tomorrow's LPOD: Das Mystery
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