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- ...;s wall southward. When we finally get high resolution lunar topography we may find that Hainzel A tilts toward the south, helping explain the massive ter ...; Starmaster Newtonian Reflector + DMK-21F04 Firewire Camera. Left: Oct 3, 2006. JMI NGT12.5″ f/5 with OMI Torus Optics + 5 x Powermate + Philips SPC3 KB (464 words) - 23:41, 8 February 2015
- ...n Hainzel and Hainzel A’s appearance between about 3,800 million and 3,200 million years ago. The light was not favorable for a good look at C, co <p><b>Yesterday's LPOD:</b> [[October 6, 2006|A Very Tormented Floor]] </p>3 KB (486 words) - 16:54, 22 March 2015
- ...ine of overlapping craters on the floor are aligned with Imbrium, and thus may be distant secondaries from that basin-forming impact. The image also revea <p><em>This LPOD was originally posted April 3, 2004 - and its still the best image of Mersenius.</em></p>3 KB (486 words) - 23:42, 8 February 2015
- ...RESOLUTION=64&RESAMP_METHOD=NEAREST_NEIGHBOR&BANDS_SELECTED=%225,3,1%22&FORMAT=JPEG&LONBOX=16&LATBOX=16&GRIDLINE_FREQUENCY Oct 3, 2006. Details on image.</p>2 KB (372 words) - 23:43, 8 February 2015
- ...rupt. The front of mountain range is serrated; the uplift of the Apennines may have originally produced a smooth curve, but the collapses - like terraces ...125 Mak f/15 + 2X Barlow Apo + IR Cut On + Phillips Toucam Pro, mosaic of 3 images with 257 frames each; Registax 4. </p>2 KB (315 words) - 23:45, 8 February 2015
- ...areas between the various mountains and hills on the floor are smooth and may be impact melt. The rays of Anaxagoras appear to be symmetric – but it is Peach: 18 April 2006. C14 @ F41 + LU075M. Tarsoudis: 09 August 2006, LXD-75 Sc 8″ + Canon EoS 350d at afocal method + barlow 2.5X + 13mm3 KB (470 words) - 12:51, 22 March 2015
- ..., but none cross it. This provides a slight suggestion that the projectile may have come from the west, but not at a very low angle. It is peculiar that t Right: May 13, 2006. 32 cm f/5.75 Newtonian @ f/28 + Phillips ToUcam Pro webcam.</p>2 KB (391 words) - 12:51, 22 March 2015
- ...the mode of formation they are pieces of the rocks under Imbrium, uplifted 3-5 kilometers above their original position. Maybe this neighborhood hasn 20 April, 2006. C14 @ F41. Lumenera LU075M. </p>2 KB (244 words) - 17:27, 22 March 2015
- ...the rille, but it might be pre-existing lava from another source. Readers may want to download the image and treat it even more extremely to explore this Rükl chart 3<br />2 KB (382 words) - 17:36, 22 March 2015
- ...area were described on the low Sun view of the [[May_3,_2007|LPOD]] of May 3; compare that LPOD with this one to increase your understanding. </p> 2006/10/10, Utime: ~08:52. 200mm f/6 Newtonian reflector, Televue 3x Barlow, DMK2 KB (401 words) - 17:36, 22 March 2015
- ...mple craters. Nearby Carmichael is 20 km wide but is only slightly deeper (3.6 km) because it is a small complex crater. Lunar Orbiter IV images show it ...ce in levels. The colour image first gets a gaussian blur (pixel radius of 3 in this case, varies between images) then the colour saturation is increase4 KB (709 words) - 15:16, 15 March 2015
- ...could be coming. Of course, in the real future the teen going to the Moon may be named Lakshmi or Chang, rather than Mike, but that is OK. Let's encourag2 KB (413 words) - 08:31, 28 October 2018
- ...s wall southward. When we finally get high resolution lunar topography we may find that Hainzel A tilts toward the south, helping explain the massive ter (I am traveling Wed and Thursday, so this is a classic LPOD from Oct 6, 2006.)</em><br />3 KB (520 words) - 18:50, 13 October 2018
- ...rse) and no one understands why it exists. It appears that the entire area may be slightly ...eat of a classic LPOD from nearly 5 years ago - [[January_21,_2006|Jan 21, 2006]]. I hope some great <br />3 KB (494 words) - 18:48, 13 October 2018
- ...s of discovering a new crater are not high - about 3 in a 1000 - but there may be one!<br /> (3) A further thought: for a given sensor size, is there an optimal magnificat5 KB (897 words) - 19:02, 18 August 2018
- ...ove where accumulated over the time period between December 2005 and March 2006, a time when the Sun was near its southernmost latitude (south polar summer (3) That's a fascinating question, Bill, and I don't really know the answer.<b11 KB (1,934 words) - 18:51, 13 October 2018
- ...closely-spaced impact craters. In the 2005 LPOD I speculated that A and C may have formed simultaneously, and now we have a mechanism to explain how it c (3) Chuck -- Lots of sites show nice pictures of the Moon, the text for me is5 KB (875 words) - 22:14, 22 March 2015
- Dec 27, 2006, 16:50UT. TMB 13 cm telescope.<br /> ...see on the lunar surface but I would also think that at least some headway may've been made in this area to understand differences in impact energy / targ4 KB (733 words) - 15:44, 28 February 2015
- Originally published January 21, 2006 ...rse) and no one understands why it exists. It appears that the entire area may be slightly higher than the surroundings, like a miniature version of the A3 KB (433 words) - 01:04, 28 March 2016
- Originally published February 1, 2006 ...of a feature minutely studied. (This is a variant of the video-imager who may spend hours computer processing instantaneously acquired images.) This draw3 KB (451 words) - 01:04, 4 April 2016