Linné (crater): Difference between revisions

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The estimated age of this [[Copernican period|copernican]] crater is only a few tens of millions of years. It was earlier believed to have a bowl shape, but data <ref>[http://www.lpi.usra.edu/meetings/lpsc2011/pdf/2063.pdf "Linne: Simple Lunar Mare crater geometry from LRO observations", ''42nd Lunar and Planetary Science Conference (2011)'']</ref> from the [[Lunar Reconnaissance Orbiter|LRO]] showed that it has a shape of a flattened, inverted cone. The crater is surrounded by a blanket of ejecta formed during the original impact. This ejecta has a relatively high [[albedo]], making the feature appear bright.
[[File:NASA's Planetary CSI - Crater Science Investigations.ogv|thumb|Learn what [[Lunar Reconnaissance Orbiter|LRO]] has learned about Linne Crater in this video.]][[Image:Linne crater 4098 h1.jpg|thumb|right|[[Lunar Orbiter 4]] image]]
In 1824 Wilhelm Lohrmann (1786-1840) of Dresden had drawn Linné as an 8&nbsp;km diameter crater in his acclaimed lunar atlas, and in 1837 [[Wilhelm Beer]] and [[Johann Heinrich Mädler]] had described Linne in ''Der Mond'' as a 10&nbsp;km crater.<ref>David Leverington, Babylon to Voyager and Beyond: A History of Planetary Astronomy, Cambridge University Press, 2003</ref> In 1866, the experienced lunar observer and mapmaker [[Johann Friedrich Julius Schmidt]] made the surprising claim that Linné had changed its appearance. Instead of a normal, somewhat deep crater it had become a mere white patch. A controversy arose that continued for many decades. However, this crater size tests the limit of visual perception of Earth-based telescopes. In conditions of poor seeingvisibility this feature can appear to vanish from sight <ref>[http://www.astrosurf.com/lunascan/Linncont.htm "The Linne' crater {{sic|nolink=y|controversey}}", ''The Lunascan Project'']</ref> (see also [[transient lunar phenomenon]]).
[[File:Linné crater color coded shaded relief map detail.png|thumb|right|Color coded shaded relief map of Linné crater]]