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  • <p><em> This is a repeat of the Sept 6, 2004 LPOD. Are there newer images of Taruntius?</em></p> ...crater that was the source of the southern ash deposit. The northern vent may be the elongated crater south of Taruntius C (Cameron). The full Moon view
    3 KB (440 words) - 23:40, 8 February 2015
  • ...ight knob on top. The crater-cutting valley points back to Serenitatis and may be one of the few known secondary crater chains from that basin-forming eve 11 September, 2006, 2:35 UT. 10&#8243; f4.8 Newtonian + DMK21-AF0 + Astronomik Red filter + 5x
    2 KB (353 words) - 16:54, 22 March 2015
  • ..., Hainzel, Hainzel A and C. A quick look at this grouping in this lighting may leave one with the mistaken impression that these three are the result of a <p><b>Yesterday's LPOD:</b> [[October 6, 2006|A Very Tormented Floor]] </p>
    3 KB (486 words) - 16:54, 22 March 2015
  • ...sed floor the shadow would extend towards the east. Hevelius&#8217;s floor may be domed - at least the southern part which casts a shadow to the west. The 4 Nov, 2006, 02:02-02:16 UT. 200mm f/6 Newtonian reflector, Televue 3x Barlow , DMK 21BF04 B/W camera, &#8216;Blu
    2 KB (323 words) - 20:40, 7 February 2015
  • <p><em>Chuck Wood Note: This interpretation may be correct, but since the Apollo 16 mission failed to sample volcanic lavas 10 Dec, 2006, ~08:43 UT. 200mm f/6 Newtonian reflector, Televue 3x Barlow , DMK 21BF04 B/W camera, &#8216;Blu
    3 KB (518 words) - 21:32, 14 February 2015
  • ...Nectaris and that it may be related to the formation of that basin. And it may be, but the smooth surface that the southern part of the fault cuts seems l 2006/10/10, Utime: ~07:24. 200mm f/6 Newtonian reflector + Televue 3x Barlow + DMK 21BF04 B/W camera + &#8216;B
    3 KB (430 words) - 21:42, 22 March 2015
  • ...a lunar globe with me, but it seems like these sets of striated materials may be radial to the Imbrium Basin. Is that true? Are the tiny pits southeast o Aug 16, 2006, 9:30 UT. 10&#8243; mak/cass at f30 with a DMK21BF04 mosaic of 6 images, 150-200 frames each.</p>
    2 KB (267 words) - 21:45, 22 March 2015
  • ...even saw two of these craters on [[October_11,_2006|LPOD]]! But you still may not recognize la Pérouse, whose scarped rim rises above the terminator, an October 8, 2006; 04:54UT. Newtonian 10&#8243; f/6 at f/16 + Philips ToUcam Pro II camera.</p>
    2 KB (361 words) - 17:27, 22 March 2015
  • ...Damian Peach&#8217;s [http://www.damianpeach.com/lunar.htm website], which may be the largest collection of high quality lunar images by any single observ 14 April, 2006. C14 @ F41. Lumenera LU075M. </p>
    2 KB (320 words) - 20:03, 8 February 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 <p><b>Tomorrow's LPOD:</b> [[October 16, 2007|6 Degrees of Separation]] </p>
    2 KB (382 words) - 17:36, 22 March 2015
  • ...mple Tycho&#8217;s impact melts, seen here on the crater&#8217;s floor, we may be able to find trace amounts of the projectile&#8217;s material and confir 2006/04/20. C14 @ F41. LU075M</p>
    2 KB (396 words) - 00:04, 9 February 2015
  • ...his 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 21BF04 B/W camera, Blue IR-bloc
    2 KB (401 words) - 17:36, 22 March 2015
  • ...filling part of the gap. This lead me to speculate that the two big rilles may once have connected, but that seems unlikely because the head of the Mairan 2nd November 2006. 10in f4.8 Newtonian, DMK 21AF04, 4x PowerMate, red filter, 1/30s, gain 600
    2 KB (414 words) - 06:04, 8 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
  • ...File:LPOD-Jan8-11.jpg|LPOD-Jan8-11.jpg]]<!-- ws:end:WikiTextLocalImageRule:6 --><br /> ...rse) and no one understands why it exists. It appears that the entire area may be slightly
    3 KB (494 words) - 18:48, 13 October 2018
  • ...File:LPOD-May9-11.jpg|LPOD-May9-11.jpg]]<!-- ws:end:WikiTextLocalImageRule:6 --><br /> August 11, 2006. 31 cm Newtonian. f/21. SkyNyx 2.1M. Wratten 25A filter. Frames stacked usi
    3 KB (446 words) - 18:53, 13 October 2018
  • ...le:LPOD-Aug11-11.jpg|LPOD-Aug11-11.jpg]]<!-- ws:end:WikiTextLocalImageRule:6 --><br /> ...seems consistent with the idea of uplift for as the mountain was raised it may have expanded laterally, allowing downdropping of a piece of its summit. <b
    3 KB (491 words) - 18:43, 13 October 2018
  • ...yot_2006_11_05.jpg|lyot_2006_11_05.jpg]]<!-- ws:end:WikiTextLocalImageRule:6 --><br /> This is a classic LPOD originally published Nov 5, 2006.<br />
    2 KB (363 words) - 18:53, 13 October 2018
  • Dec 27, 2006, 16:50UT. TMB 13 cm telescope.<br /> ...looking at Aristoteles and Eudoxus with my telescope this Sunday evening (6-8-08). With temperatures in the mid-70s F.and clear skies, I was able to sp
    4 KB (733 words) - 15:44, 28 February 2015
  • Originally published March 12, 2006 ...currence of mare material deep in the southern highlands. The non-descript 6-km wide crater Buch B lies north of Buch and NE of Maurolycus. In 1962, Gen
    3 KB (480 words) - 01:04, 3 May 2016

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