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- Originally published February 4, 2005 [[File:LPOD-2005-02-04.jpeg|LPOD-2005-02-04.jpeg]]3 KB (455 words) - 02:04, 14 December 2015
- Originally published February 6, 2005 [[File:LPOD-2005-02-06.jpeg|LPOD-2005-02-06.jpeg]]3 KB (506 words) - 02:04, 16 December 2015
- Originally published February 14, 2005 {{HoverImage|LPOD-2005-02-14.jpeg|LPOD-2005-02-14b.jpeg}}3 KB (548 words) - 19:13, 23 December 2015
- Originally published February 15, 2005 [[File:LPOD-2005-02-15.jpeg|LPOD-2005-02-15.jpeg]]3 KB (408 words) - 02:04, 24 December 2015
- Originally published February 17, 2005 {{HoverImage|LPOD-2005-02-17.jpeg|LPOD-2005-02-17b.jpeg}}3 KB (478 words) - 02:04, 26 December 2015
- 15 August 2005. 32 cm f/5.75 Newtonian @ f/28 + Phillips ToUcam Pro webcam. Frames from av <p><b>Yesterday's LPOD:</b> [[December 9, 2016|Herigonius Pi & Eta]] </p>2 KB (333 words) - 02:04, 10 December 2016
- ...the US Geological Survey, and is called the Unified Lunar Control Network 2005. On average, there is a point about every 6.8 km along the surface, and the <p><b>Yesterday's LPOD:</b> [[December 13, 2016|The Edge of a Bull's Eye]] </p>3 KB (522 words) - 02:04, 14 December 2016
- Originally published March 15, 2008 ...posite image above where accumulated over the time period between December 2005 and March 2006, a time when the Sun was near its southernmost latitude (sou11 KB (1,937 words) - 18:57, 13 October 2018
- ...7|The System of Lunar Craters]]</em> catalog into quadrant maps. And since 2005 many of us have relied on the handy <em>[[April_16,_2006|Sky & Telescop <p><b>Yesterday's LPOD:</b> [[December 13, 2017|Learning a Lot About Little Hills]] </p>4 KB (694 words) - 02:04, 14 December 2017