https://www2.lpod.org/api.php?hideanons=1&hidebots=1&urlversion=1&days=7&limit=50&action=feedrecentchanges&feedformat=atomLPOD - Recent changes [en]2024-03-29T15:33:04ZTrack the most recent changes to the wiki in this feed.MediaWiki 1.31.1https://www2.lpod.org/index.php?title=Main_Page&diff=47927&oldid=47925Main Page2024-03-29T08:05:13Z<p>Changed redirect target from <a href="/wiki/March_28,_2024" title="March 28, 2024">March 28, 2024</a> to <a href="/wiki/March_29,_2024" title="March 29, 2024">March 29, 2024</a></p>
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</table>Apihttps://www2.lpod.org/index.php?title=March_29,_2024&diff=47926&oldid=0March 29, 20242024-03-29T08:05:12Z<p>Created page with "__NOTOC__ =Have You Knowingly Seen This Basin?= Originally published March 15, 2014 <!-- Start of content --> <!-- ws:start:WikiTextHeadingRule:0:<h1> --> <!-- ws:s..."</p>
<p><b>New page</b></p><div>__NOTOC__<br />
=Have You Knowingly Seen This Basin?=<br />
Originally published March 15, 2014<br />
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<em>image by [mailto:claude.navarro_toulouse@orange.fr Claude Navarro], Toulouse (France)</em><br /><br />
<br /><br />
With the very high resolution topographic digital terrain data from LRO it is possible to create or recreate any illumination for any piece of the lunar surface. Despite that capability it is personally wondrous to come across at the telescope such spectacular lighting as Claude captured here. Hartmann and Kuiper called this two-ring basin the Basin Near Schiller when they first described it in the early 1960s, but the quasi-official name is the Schiller-Zucchius Basin. Both names tell you that it is near Schiller, the almost cigar-snapped crater at center right. The main basin rim (335 km in diameter) is best displayed to the left of Schiller, where it curves around towards Zucchius, whose near rim only is illuminated at the terminator. At the snout end of Schiller a surprisingly strong shadow is cast by the very low basin rim to the north. Both sides of the 175 km wide inner basin ring are visible, and what this lighting shows very well is the rounded drop off of an inner, inner ring. Three small hills inside the inner, inner ring are usually inconspicuous, but this shadow-magnification reveals them clearly. The SZB is an old basin, and while there may be ancient basalts in it, the visible smooth material is largely fluidized ejecta from the formation of the Orientale Basin. <br /><br />
<br /><br />
<em>[mailto:tychocrater@yahoo.com Chuck Wood]</em><br /><br />
<em>I always need to thank Claude for being one of the translators of LPOD into the French [http://iluj.wikispaces.com l'image lunaire du jour]!</em><br /><br />
<br /><br />
<strong>Technical Details</strong><br /><br />
March/12/2014, 20:45 UT. C14 + Basler 1300 + IR pass 685. 250 images (on 2000) processed with AS2! and Registax 6.<br /><br />
<br /><br />
<strong>Related Links</strong><br /><br />
<em>[[21st Century Atlas of the Moon|21st Century Atlas]]</em> charts 24 &amp; B8.<br /><br />
<br /><br />
<p><b>Yesterday's LPOD:</b> [[March 28, 2024|First Time Observers Map]] </p><br />
<p><b>Tomorrow's LPOD:</b> [[March 30, 2024|The Hills Were Once Alive, but There Was No Music]] </p><br />
<hr /><br />
{{wiki/ArticleFooter}}</div>Apihttps://www2.lpod.org/index.php?title=Main_Page&diff=47925&oldid=47923Main Page2024-03-28T08:05:10Z<p>Changed redirect target from <a href="/wiki/March_27,_2024" title="March 27, 2024">March 27, 2024</a> to <a href="/wiki/March_28,_2024" title="March 28, 2024">March 28, 2024</a></p>
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</table>Apihttps://www2.lpod.org/index.php?title=March_28,_2024&diff=47924&oldid=0March 28, 20242024-03-28T08:05:08Z<p>Created page with "__NOTOC__ =First Time Observers Map= Originally published March 14, 2014 <!-- Start of content --> <!-- ws:start:WikiTextHeadingRule:0:<h1> --> <!-- ws:start:WikiTe..."</p>
<p><b>New page</b></p><div>__NOTOC__<br />
=First Time Observers Map=<br />
Originally published March 14, 2014<br />
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<em>image by Lee DeCovnick</em><br /><br />
<br /><br />
We often have friends, family and kids over to take their first look at the moon through a quality telescope. We use a 4" refractor for two reasons. First. almost everyone instinctively understands which end of the scope to look through, which is definitely not the case with a Newtonian or even an SCT like a Celestron 8. Second, many first time viewer are surprised by the brightness that hits their eye, and they become nervous about damaging their vision. The smaller aperture does a good job of reducing the moonlight to tolerable levels. And we use a high quality plossl (eyepiece) from 24mm to 32mm, since they are easy to look through and easy to focus for the novice observer.<br /><br />
So, when a first time observers looks at the moon through a quality scope, three things inevitably occur: everyone says, &quot;Wow!" a couple of times, they quietly realize they have no idea what they are looking at, and they always ask where did the moon landings occur. Here’s where this map, which is uploaded onto my iPad. comes in handy. Since the map is made from a prime focus photograph thorough this same scope, the scale is pretty close to what they are seeing through the eyepiece. I hold the iPad, and then ask them to start identifying what they see through the scope with what’s on the map. Their ability to name the features they are seeing is nice experience for them and us. After identifying the major maria, it is an easy segue into talking about how the maria were formed, and why the molten magma migrated to the nearside of the Moon facing Earth. I also like to briefly explain the age differences between Tycho (108 million years) and Copernicus (800 million years) in the contest of their rays. Astronomy outreach is an important part of being an amateur astronomer.. our fondest hope is that the twenty minutes we spend with a first time observer will lead them onto a new path of discovery.<br /><br />
<br /><br />
<em>Lee DeCovnick</em><br /><br />
<br /><br />
<strong>Technical Details</strong><br /><br />
March 12, 2014, Walnut Creek, Ca, Stellarvue SV102AE-25SV, f/11 at prime focus, Nikon D7100 DSLR, Baader Semi-APO filter, 1/640 second exposure, ISO 1250. iPhoto and Apple Preview editing tools.<br /><br />
<br /><br />
<p><b>Yesterday's LPOD:</b> [[March 27, 2024|Up, Up and Away]] </p><br />
<p><b>Tomorrow's LPOD:</b> [[March 29, 2024|Have You Knowingly Seen This Basin?]] </p><br />
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{{wiki/ArticleFooter}}</div>Apihttps://www2.lpod.org/index.php?title=Main_Page&diff=47923&oldid=47921Main Page2024-03-27T08:05:10Z<p>Changed redirect target from <a href="/wiki/March_26,_2024" title="March 26, 2024">March 26, 2024</a> to <a href="/wiki/March_27,_2024" title="March 27, 2024">March 27, 2024</a></p>
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</table>Apihttps://www2.lpod.org/index.php?title=March_27,_2024&diff=47922&oldid=0March 27, 20242024-03-27T08:05:08Z<p>Created page with "__NOTOC__ =Up, Up and Away= Originally published March 13, 2014 <!-- Start of content --> <!-- ws:start:WikiTextHeadingRule:0:<h1> --> <!-- ws:start:WikiTextLocalIm..."</p>
<p><b>New page</b></p><div>__NOTOC__<br />
=Up, Up and Away=<br />
Originally published March 13, 2014<br />
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<em>image by [mailto:mpraet@skynet.be Marnix Praet], Belgium</em><br /><br />
<br /><br />
I was busy taking pictures with my DMK 21-618 and a plane passed through my view, so I took 3 seperate images in registax and stichet them together, so now I see how sharp this DMK 21-618 camera take pictures ;-)<br /><br />
<br /><br />
<em>[mailto:mpraet@skynet.be Marnix Praet]</em><br /><br />
<br /><br />
<strong>Technical Details</strong><br /><br />
March 11, 2014. Newton 10" telescope.<br /><br />
<br /><br />
<strong>Related Links</strong><br /><br />
Marmix's [http://users.skynet.be/mpraet web site], [http://groups.yahoo.com/group/sterrenfreaks user group] and [https://www.facebook.com/marnix.praet.16 Facebook page]<br /><br />
<br /><br />
<p><b>Yesterday's LPOD:</b> [[March 26, 2024|Smoothed Plains]] </p><br />
<p><b>Tomorrow's LPOD:</b> [[March 28, 2024|First Time Observers Map]] </p><br />
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{{wiki/ArticleFooter}}</div>Apihttps://www2.lpod.org/index.php?title=Main_Page&diff=47921&oldid=47919Main Page2024-03-26T08:05:07Z<p>Changed redirect target from <a href="/wiki/March_25,_2024" title="March 25, 2024">March 25, 2024</a> to <a href="/wiki/March_26,_2024" title="March 26, 2024">March 26, 2024</a></p>
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</table>Apihttps://www2.lpod.org/index.php?title=March_26,_2024&diff=47920&oldid=0March 26, 20242024-03-26T08:05:06Z<p>Created page with "__NOTOC__ =Smoothed Plains= Originally published March 12, 2014 <!-- Start of content --> <!-- ws:start:WikiTextHeadingRule:0:<h1> --> <!-- ws:start:WikiTextLocalIm..."</p>
<p><b>New page</b></p><div>__NOTOC__<br />
=Smoothed Plains=<br />
Originally published March 12, 2014<br />
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<em>image by [mailto:lujafer@gmail.com Luis J. Fernández], Barcelona, Spain</em><br /><br />
<br /><br />
This is a fascinating image because of the way it has been processed. The mountains are full of angular roughness but the maria look like they have been filtered to smooth out details, as if the lava flows were very fluid and froze with a nice smooth surface. This treatment emphasizes the broad surfaces of the maria rather than their details, and makes the mountains stand out as sharply different terrains. One thing that pops out is a broad swell east of Aristillus and pushing up against the south part of the Caucasus Mountains. LRO QuickMap [http://bit.ly/1fSLcNE shows] that this swell rises about 400 m above the mare to the west, and is partly made of the older lavas cut by the Theaetetus Rilles, but includes Imbrium lavas too. Many swells face up against individual mountains or mountain walls, but I don't know why.<br /><br />
<br /><br />
<em>[mailto:tychocrater@yahoo.com Chuck Wood]</em><br /><br />
<br /><br />
<strong>Technical Details</strong><br /><br />
2014-03-08 20:38: UT. Celestron C8 SC, mount CGEM, Camera ZWO ASI 120MC with IR PRO 740 filter.<br /><br />
<br /><br />
<strong>Related Links</strong><br /><br />
<em>[[21st Century Atlas of the Moon|21st Century Atlas]]</em> chart 11.<br /><br />
Luis' astronomy [http://www.youtube.com/watch?v=xw9GwlJIcHQ video] and [http://astrorionis.blogspot.com.es blog]<br /><br />
<br /><br />
<p><b>Yesterday's LPOD:</b> [[March 25, 2024|A Mega-Ridge]] </p><br />
<p><b>Tomorrow's LPOD:</b> [[March 27, 2024|Up, Up and Away]] </p><br />
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{{wiki/ArticleFooter}}</div>Apihttps://www2.lpod.org/index.php?title=Main_Page&diff=47919&oldid=47917Main Page2024-03-25T08:05:08Z<p>Changed redirect target from <a href="/wiki/March_24,_2024" title="March 24, 2024">March 24, 2024</a> to <a href="/wiki/March_25,_2024" title="March 25, 2024">March 25, 2024</a></p>
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</table>Apihttps://www2.lpod.org/index.php?title=March_25,_2024&diff=47918&oldid=0March 25, 20242024-03-25T08:05:07Z<p>Created page with "__NOTOC__ =A Mega-Ridge= Originally published March 11, 2014 <!-- Start of content --> <!-- ws:start:WikiTextHeadingRule:0:<h1> --> <!-- ws:start:WikiTextLocalImage..."</p>
<p><b>New page</b></p><div>__NOTOC__<br />
=A Mega-Ridge=<br />
Originally published March 11, 2014<br />
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<em>image by [mailto:mwirths@starband.net Michael Wirths], Baja California, Mexico</em><br /><br />
<br /><br />
Mike's wonderful new image of Tranquillitatis makes the Lamont region look like the gnarled hand of a hard worker. Narrow and wide ridges cause the mare surface to undulate at different wavelengths, a complexity that will evaporate with a slightly higher illumination into a flat dark lava plain. For me, the most interesting part of the image - meaning there is something seldom seen to enjoy and ponder - is the bottom half. In particular, the segmented broad ridge that crosses the south end of the mare between [http://bit.ly/1i1HTlQ Censorinus B and the Apollo 11 landing area]. At some places this is seen (courtesy of LRO QuickMap) to be a fault, whose north side rises 100-150 m. The linear tectonic feature is roughly continuous with the Guttenberg Rilles family, although the individual rilles are at a different angle. This family and the mare tectonic feature are radial to the center of Imbrium, as are the straight ridge from Maskelyne to Lamont, the ridge that crosses northern Lamont, and the Cauchy Fault. The basin's formation must have had some structural influence on the orientation of the ridges and fractures.<br /><br />
<br /><br />
<em>[mailto:tychocrater@yahoo.com Chuck Wood]</em><br /><br />
<br /><br />
<strong>Technical Details</strong><br /><br />
March 6, 2014<br /><br />
<br /><br />
<strong>Related Links</strong><br /><br />
<em>[[21st Century Atlas of the Moon|21st Century Atlas]]</em> chart 7.<br /><br />
Mike's bed and breakfast astronomy [http://www.bajadarkskies.com website]<br /><br />
<br /><br />
<p><b>Yesterday's LPOD:</b> [[March 24, 2024|Cosmos &amp; the Moon]] </p><br />
<p><b>Tomorrow's LPOD:</b> [[March 26, 2024|Smoothed Plains]] </p><br />
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{{wiki/ArticleFooter}}</div>Apihttps://www2.lpod.org/index.php?title=Main_Page&diff=47917&oldid=47915Main Page2024-03-24T08:05:08Z<p>Changed redirect target from <a href="/wiki/March_23,_2024" title="March 23, 2024">March 23, 2024</a> to <a href="/wiki/March_24,_2024" title="March 24, 2024">March 24, 2024</a></p>
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</table>Apihttps://www2.lpod.org/index.php?title=March_24,_2024&diff=47916&oldid=0March 24, 20242024-03-24T08:05:07Z<p>Created page with "__NOTOC__ =Cosmos & the Moon= Originally published March 10, 2014 <!-- Start of content --> <!-- ws:start:WikiTextHeadingRule:0:<h1> --> <!-- ws:start:WikiTextL..."</p>
<p><b>New page</b></p><div>__NOTOC__<br />
=Cosmos &amp; the Moon=<br />
Originally published March 10, 2014<br />
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<em>image by [mailto:dpeach_78@yahoo.co.uk Damian Peach], UK</em><br /><br />
<br /><br />
I am watching the first minutes of COSMOS and remembering that the nearest cosmic neighbor is our Moon. <br />
There is an infinity of galaxies to explore, not to mention multiverse bubbles, but nowhere in the cosmos can <br />
our personal exploration see more details than at the Moon. Damian's excellent image shows a detail that<br />
often is not visible, and rarely captured as clearly. Humboldt is a glorious large crater that everyone would <br />
know if it were easily visible from Earth. We see it obliquely, looking across a rille-cracked floor, to the dark <br />
lavas of Mare Australe to the southeast. But now Neil Tyson has just finished with his story of being hosted <br />
by Carl Sagan, and its time for me to finish too.<br />
<br /><br />
<em>[mailto:tychocrater@yahoo.com Chuck Wood]</em><br /><br />
<br /><br />
<strong>Technical Details</strong><br /><br />
March 5, 2014.<br /><br />
<br /><br />
<br /><br />
<strong>Related Links</strong><br /><br />
<em>[[21st Century Atlas of the Moon|21st Century Atlas]]</em> charts 4 &amp; L3.<br /><br />
<br /><br />
<p><b>Yesterday's LPOD:</b> [[March 23, 2024|Xquisite]] </p><br />
<p><b>Tomorrow's LPOD:</b> [[March 25, 2024|A Mega-Ridge]] </p><br />
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{{wiki/ArticleFooter}}</div>Apihttps://www2.lpod.org/index.php?title=Main_Page&diff=47915&oldid=47913Main Page2024-03-23T08:05:08Z<p>Changed redirect target from <a href="/wiki/March_22,_2024" title="March 22, 2024">March 22, 2024</a> to <a href="/wiki/March_23,_2024" title="March 23, 2024">March 23, 2024</a></p>
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</table>Apihttps://www2.lpod.org/index.php?title=March_23,_2024&diff=47914&oldid=0March 23, 20242024-03-23T08:05:07Z<p>Created page with "__NOTOC__ =Xquisite= Originally published March 9, 2014 <!-- Start of content --> <!-- ws:start:WikiTextHeadingRule:0:<h1> --> <!-- ws:start:WikiTextLocalImageRule:..."</p>
<p><b>New page</b></p><div>__NOTOC__<br />
=Xquisite=<br />
Originally published March 9, 2014<br />
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<em>image by [mailto:sally.e.russell@gmail.com Sally Russell], England</em><br /><br />
<br /><br />
Mars has a [http://science1.nasa.gov/science-news/science-at-nasa/2001/ast24may_1/ face], but the best the Moon can offer is an [https://the-moon.us/wiki/Lunar_X X]. The face is nothing other than an accident of topography and lighting, and that is the same for the X. There is no geologic import to the X, it is just the close approach of [http://bit.ly/1hZa2uo three craters' rims], and yet it is a pleasure to unexpectedly see it, as Sally did. I never plan my looking at the Moon; with the restrictions I have due to houses, trees, clouds and coldness, I take whatever I can get, so am surprised and delighted every time.<br /><br />
<br /><br />
<em>[mailto:tychocrater@yahoo.com Chuck Wood]</em><br /><br />
<br /><br />
<strong>Technical Details</strong><br /><br />
2014 March 08, 21:42-22:20UT. 105mm F5.8 refractor, 3.5mm eyepiece (x173). Seeing: Antoniadi III. Slight haze, calm, 5°C. White pastel on black paper, sketch size 13cm x 18cm.<br /><br />
<br /><br />
<strong>Related Links</strong><br /><br />
<em>[[21st Century Atlas of the Moon|21st Century Atlas]]</em> chart 13.<br /><br />
<br /><br />
<p><b>Yesterday's LPOD:</b> [[March 22, 2024|Four with One Shot]] </p><br />
<p><b>Tomorrow's LPOD:</b> [[March 24, 2024|Cosmos &amp; the Moon]] </p><br />
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