Difference between revisions of "May 9, 2005"

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    <tr><td><div align="center" class="main_sm">Image Credit: Hevelius and [mailto:chuck@observingthesky.org Charles A. Wood]</p>
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<tr><td><div align="center" class="main_sm"><p>Image Credit: Hevelius and [http://www.usno.navy.mil/library/rare/rare.html The U.S. Naval Observatory Library]</p>
<p align="center" class="main_titles"><b>Technical Consultant:</b><br>
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[mailto:anthony@perseus.gr Anthony Ayiomamitis]</p>
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<p align="center" class="main_titles"><b>Contact Translator:</b><br>
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[mailto:pablolonnie@yahoo.com.mx" class="one Pablo Lonnie Pacheco Railey]  (Es)<br>
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[mailto:chlegrand@free.fr" class="one Christian Legrand] (Fr)</p>
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<p align="center" class="main_titles"><b>[mailto:webuser@observingthesky.org Contact Webmaster]</b></p>
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<p align="center"><b>NOT the Source of Lunar Nomenclature</b></p>
<p align="center" class="main_titles"><b>A service of:</b><br>
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<p align="left">In 1647, Johannes Hevelius made the second major chart of the Moon that showed and named identifiable features - Langrenus was first in 1645. Using a 12 ft long, 50 power telescope Hevelius made three maps - including a full Moon view - the eastern half of which is seen here. The double rim demonstrates that Hevelius recognized and mapped the effects of libration. Hevelius named 286 craters, mountains and maria, but only 10 of his names, including the Alpes and Apennines, are still used. Hevelius’ names were long and cumbersome; more significantly, four years later Grimaldi’s map appeared with the simplifed nomnclature of Riccioli. These are the hundreds of names we know today: Copernicus, Plato, Ptolemaeus, and most of the others.</p>
[http://www.observingthesky.org/" class="one ObservingTheSky.Org]</p>
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<p align="center" class="main_titles"><b>Visit these other PODs:</b> <br>
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<p align="right">&#8212; [mailto:tychocrater@yahoo.com Chuck Wood]</p></blockquote>
[http://antwrp.gsfc.nasa.gov/apod/astropix.html" class="one Astronomy] | [http://www.msss.com/" class="one Mars] | [http://epod.usra.edu/" class="one Earth]</p>
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<p align="left"><b>Related Links:</b><br>
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[http://www.adlerplanetarium.org/learn/history/astronomers/hevelius01.ssi Hevelius]
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<p><b>Yesterday's LPOD:</b> [[May 8, 2005|Splayed Rays]] </p>
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<p><b>Tomorrow's LPOD:</b> [[May 10, 2005|Theo as You've Never See It]] </p>
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<p align="center" class="main_titles"><b>Author &amp; Editor:</b><br>
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[mailto:tychocrater@yahoo.com Charles A. Wood]</p>
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===COMMENTS?===
 
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Latest revision as of 15:15, 15 March 2015

NOT the Source of Lunar Nomenclature

LPOD-2005-05-09.jpeg

Image Credit: Hevelius and The U.S. Naval Observatory Library


NOT the Source of Lunar Nomenclature

In 1647, Johannes Hevelius made the second major chart of the Moon that showed and named identifiable features - Langrenus was first in 1645. Using a 12 ft long, 50 power telescope Hevelius made three maps - including a full Moon view - the eastern half of which is seen here. The double rim demonstrates that Hevelius recognized and mapped the effects of libration. Hevelius named 286 craters, mountains and maria, but only 10 of his names, including the Alpes and Apennines, are still used. Hevelius’ names were long and cumbersome; more significantly, four years later Grimaldi’s map appeared with the simplifed nomnclature of Riccioli. These are the hundreds of names we know today: Copernicus, Plato, Ptolemaeus, and most of the others.

Chuck Wood

Related Links:
Hevelius

Yesterday's LPOD: Splayed Rays

Tomorrow's LPOD: Theo as You've Never See It



Author & Editor:
Charles A. Wood

 


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