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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 SPC
    3 KB (464 words) - 23:41, 8 February 2015
  • ...n Hainzel and Hainzel A&#8217;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&#038;RESAMP_METHOD=NEAREST_NEIGHBOR&#038;BANDS_SELECTED=%225,3,1%22&#038;FORMAT=JPEG&#038;LONBOX=16&#038;LATBOX=16&#038;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&#8243; + Canon EoS 350d at afocal method + barlow 2.5X + 13mm
    3 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&#8 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, DMK
    2 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 increase
    4 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 encourag
    2 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 magnificat
    5 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.<b
    11 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 is
    5 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 / targ
    4 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 A
    3 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 draw
    3 KB (451 words) - 01:04, 4 April 2016

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