Difference between revisions of "Cantor"
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([http://the-moon.us/wiki/LAC%20zone LAC zone] 30C1) ''[http://planetarynames.wr.usgs.gov/images/Lunar/lac_30.pdf USGS Digital Atlas PDF]''<br /> <br /> | ([http://the-moon.us/wiki/LAC%20zone LAC zone] 30C1) ''[http://planetarynames.wr.usgs.gov/images/Lunar/lac_30.pdf USGS Digital Atlas PDF]''<br /> <br /> | ||
==Description== | ==Description== | ||
| − | '''Cantor''' is a crater of the [http://the-moon.us/wiki/stratigraphy Late Imbrium] period (3.85 to 3.74 bn years), and lies some 800 kilometres away from [http://the-moon.us/wiki/Humboldtianum%2C%20Mare Mare Humboltianum] to the north-west and, roughly, the same distance from [http://the-moon.us/wiki/Mare%20Moscoviense Mare Moscoviense] to the east -- both [http://the-moon.us/wiki/stratigraphy Nectarian] (3.92 to 3.85 bn years) in age The crater's appearance looks relatively young with its sharp-ish rims, but overall its shape is more oval, or hexagonal, than your average round-looking crater -- due, no doubt, to the result of extended terracing effects in the north-south (less in the east-west) direction. The floor of '''Cantor''' has been altered into a series of hills and rises due to these events; with the central regions predominantly showing a broken set of peaks dis-conjoined.<span class="membersnap">- | + | '''Cantor''' is a crater of the [http://the-moon.us/wiki/stratigraphy Late Imbrium] period (3.85 to 3.74 bn years), and lies some 800 kilometres away from [http://the-moon.us/wiki/Humboldtianum%2C%20Mare Mare Humboltianum] to the north-west and, roughly, the same distance from [http://the-moon.us/wiki/Mare%20Moscoviense Mare Moscoviense] to the east -- both [http://the-moon.us/wiki/stratigraphy Nectarian] (3.92 to 3.85 bn years) in age The crater's appearance looks relatively young with its sharp-ish rims, but overall its shape is more oval, or hexagonal, than your average round-looking crater -- due, no doubt, to the result of extended terracing effects in the north-south (less in the east-west) direction. The floor of '''Cantor''' has been altered into a series of hills and rises due to these events; with the central regions predominantly showing a broken set of peaks dis-conjoined.<span class="membersnap">- JohnMoore2</span><br /> <br /> |
===Wikipedia=== | ===Wikipedia=== | ||
[http://en.wikipedia.org/wiki/Cantor_(crater) Cantor]<br /> <br /> | [http://en.wikipedia.org/wiki/Cantor_(crater) Cantor]<br /> <br /> | ||
Latest revision as of 21:05, 16 April 2018
Contents
Cantor
| Lat: 37.98°N, Long: 118.5°E, Diam: 75.72 km, Depth: km, Rükl: (farside) | |
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Right: Colo-coded Lac 30 from USGS Digital Atlas//
Images
LPOD Photo Gallery Lunar Orbiter Images Apollo Images Clementine
Cantor was also captured near the lower right corner of Apollo 16's Fairchild-camera photograph AS16-M-3002, which was made during Trans Earth Coast (TEC).
Research: Danny Caes
Maps
(LAC zone 30C1) USGS Digital Atlas PDF
Description
Cantor is a crater of the Late Imbrium period (3.85 to 3.74 bn years), and lies some 800 kilometres away from Mare Humboltianum to the north-west and, roughly, the same distance from Mare Moscoviense to the east -- both Nectarian (3.92 to 3.85 bn years) in age The crater's appearance looks relatively young with its sharp-ish rims, but overall its shape is more oval, or hexagonal, than your average round-looking crater -- due, no doubt, to the result of extended terracing effects in the north-south (less in the east-west) direction. The floor of Cantor has been altered into a series of hills and rises due to these events; with the central regions predominantly showing a broken set of peaks dis-conjoined.- JohnMoore2
Wikipedia
Additional Information
- IAU page: Cantor
- Central peak composition: Anorthosite & GNTA1 (Tompkins & Pieters, 1999)
Nomenclature
- Georg; German mathematician (1845-1918)
- Moritz; German mathematician (1829-1920).
LROC Articles
LPOD Articles
Bibliography
Named Features -- Prev: Cannon -- Next: Capella
