Difference between revisions of "May 9, 2005"
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=NOT the Source of Lunar Nomenclature= | =NOT the Source of Lunar Nomenclature= | ||
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<table width="85%" border="0" align="center" cellpadding="6" cellspacing="2"> | <table width="85%" border="0" align="center" cellpadding="6" cellspacing="2"> | ||
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| − | + | <td width="50%"><h2><nobr>NOT the Source of Lunar Nomenclature</nobr></h2></td> | |
| − | + | </tr> | |
</table> | </table> | ||
<table width="85%" border="0" align="center" cellpadding="6" cellspacing="2"> | <table width="85%" border="0" align="center" cellpadding="6" cellspacing="2"> | ||
| − | + | <tr><td colspan="2" valign="top"><div align="center"> | |
| − | + | <img src="archive/2005/05/images/LPOD-2005-05-09.jpeg" border="0"> | |
| − | + | </div></td> | |
| − | + | </tr> | |
</table> | </table> | ||
<table width="80%" border="0" align="center" cellpadding="8"> | <table width="80%" border="0" align="center" cellpadding="8"> | ||
| − | + | <tr><td><div align="center" class="main_sm">Image Credit: Hevelius and [http://www.usno.navy.mil/library/rare/rare.html The U.S. Naval Observatory Library]</p> | |
| − | + | </div></td> | |
| − | + | </tr> | |
| − | + | </table> | |
<br> | <br> | ||
<table class="story" border="0" bgcolor="#FFFFFF" width="90%" cellpadding="10" align="center"><tr><td> | <table class="story" border="0" bgcolor="#FFFFFF" width="90%" cellpadding="10" align="center"><tr><td> | ||
| − | + | <p align="center"><b>NOT the Source of Lunar Nomenclature</b></p> | |
| − | + | <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 Grimaldis 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> | |
| − | + | <blockquote><p align="right">— [mailto:tychocrater@yahoo.com Chuck Wood]</blockquote> | |
<p align="left"><p><b>Related Links:</b><br> | <p align="left"><p><b>Related Links:</b><br> | ||
[http://www.adlerplanetarium.org/learn/history/astronomers/hevelius01.ssi Hevelius] | [http://www.adlerplanetarium.org/learn/history/astronomers/hevelius01.ssi Hevelius] | ||
<p align="left"><b>Tomorrow's LPOD: </b> Theo as Youve Never See It</p> | <p align="left"><b>Tomorrow's LPOD: </b> Theo as Youve Never See It</p> | ||
| − | + | </tr> | |
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</table> | </table> | ||
<br> | <br> | ||
<table width="100%" border="0" cellspacing="2" cellpadding="4"> | <table width="100%" border="0" cellspacing="2" cellpadding="4"> | ||
| − | + | <tr> | |
| − | + | <td><hr></td> | |
| − | + | </tr> | |
| − | + | <tr><td> | |
| − | + | <p align="center" class="main_titles"><b>Author & Editor:</b><br> | |
| − | + | [mailto:tychocrater@yahoo.com Charles A. Wood]</p> | |
| − | + | <p align="center" class="main_titles"><b>Technical Consultant:</b><br> | |
| − | + | [mailto:anthony@perseus.gr Anthony Ayiomamitis]</p> | |
| − | + | <p align="center" class="main_titles"><b>Contact Translator:</b><br> | |
| − | + | [mailto:pablolonnie@yahoo.com.mx" class="one Pablo Lonnie Pacheco Railey] (Es)<br> | |
| − | + | [mailto:chlegrand@free.fr" class="one Christian Legrand] (Fr)</p> | |
| − | + | <p align="center" class="main_titles"><b>[mailto:webuser@observingthesky.org Contact Webmaster]</b></p> | |
| − | + | <p align="center" class="main_titles"><b>A service of:</b><br> | |
| − | + | [http://www.observingthesky.org/" class="one ObservingTheSky.Org]</p> | |
| − | + | <p align="center" class="main_titles"><b>Visit these other PODs:</b> <br> | |
| − | + | [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> | |
| − | + | </td></tr> | |
</table> | </table> | ||
<p> </p> | <p> </p> | ||
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===COMMENTS?=== | ===COMMENTS?=== | ||
Click on this icon [[image:PostIcon.jpg]] at the upper right to post a comment. | Click on this icon [[image:PostIcon.jpg]] at the upper right to post a comment. | ||
Revision as of 18:32, 4 January 2015
NOT the Source of Lunar Nomenclature
<nobr>NOT the Source of Lunar Nomenclature</nobr> |
<img src="archive/2005/05/images/LPOD-2005-05-09.jpeg" border="0"> |
Image Credit: Hevelius and The U.S. Naval Observatory Library
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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 Grimaldis 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. Related Links: Tomorrow's LPOD: Theo as Youve Never See It |
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Author & Editor: Technical Consultant: Contact Translator: A service of: Visit these other PODs: |
COMMENTS?
Click on this icon File:PostIcon.jpg at the upper right to post a comment.
