Difference between revisions of "February 23, 2005"
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| − | + | <td width="50%"><h2><nobr>The Big and Little of It</nobr></h2></td> | |
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| − | + | <img src="archive/2005/02/images/LPOD-2005-02-23.jpeg" border="0"> | |
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| − | + | <tr><td><div align="center" class="main_sm">Image Credit: [mailto:anthony@perseus.gr Anthony Ayiomamitis]</p> | |
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| − | + | <p align="center"><b>The Big and Little of It</b></p> | |
| − | + | <p align="left">The Moon is far from constant. It varies visibly in size and shape more than any other celestial object. But it is harder to tell – almost impossible visibly? – that the Moon also varies in actual size as seen from Earth. The reason for this variation is simple. The Moon’s orbit is elliptical – sometimes it is near Earth and 14 days later it is nearly 50,000 km further away. In other words the lunar distance and size vary by 14% monthly. I wonder when this was observationally discovered? Anthony has captured nearly the maximum variation in the lunar size difference in these two images of full Moons during 2004. Also note that while there is little difference in longitudinal libration, the libration in latitude has tipped the North Pole into a favorable view in the summer image, and the opposite pole is best in December. This image joins the [http://www.lpod.org/LPOD-2005-02-21.htm lunar phase poster] as an excellent resource for schools and the public.</p> | |
| − | + | <blockquote><p align="right">— [mailto:tychocrater@yahoo.com Chuck Wood]</blockquote> | |
<p align="left"><p><b>Technical Details:</b><br> | <p align="left"><p><b>Technical Details:</b><br> | ||
TeleVue Pronto + TeleVue Zero-Length Adapter + Canon EOS 300d. [http://www.perseus.gr/Astro-Lunar-Scenes-Apo-Perigee.htm Full details.] </p> | TeleVue Pronto + TeleVue Zero-Length Adapter + Canon EOS 300d. [http://www.perseus.gr/Astro-Lunar-Scenes-Apo-Perigee.htm Full details.] </p> | ||
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<br>[http://antwrp.gsfc.nasa.gov/apod/ap041021.html Apogee-Perigee Quarters] | <br>[http://antwrp.gsfc.nasa.gov/apod/ap041021.html Apogee-Perigee Quarters] | ||
<p align="left"><b>Tomorrow's LPOD: </b> Double Your Pleasure – The Moon By Day</p> | <p align="left"><b>Tomorrow's LPOD: </b> Double Your Pleasure – The Moon By Day</p> | ||
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| − | + | <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> | |
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</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 17:29, 4 January 2015
The Big and Little of It
<nobr>The Big and Little of It</nobr> |
<img src="archive/2005/02/images/LPOD-2005-02-23.jpeg" border="0"> |
Image Credit: Anthony Ayiomamitis
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The Big and Little of It The Moon is far from constant. It varies visibly in size and shape more than any other celestial object. But it is harder to tell – almost impossible visibly? – that the Moon also varies in actual size as seen from Earth. The reason for this variation is simple. The Moon’s orbit is elliptical – sometimes it is near Earth and 14 days later it is nearly 50,000 km further away. In other words the lunar distance and size vary by 14% monthly. I wonder when this was observationally discovered? Anthony has captured nearly the maximum variation in the lunar size difference in these two images of full Moons during 2004. Also note that while there is little difference in longitudinal libration, the libration in latitude has tipped the North Pole into a favorable view in the summer image, and the opposite pole is best in December. This image joins the lunar phase poster as an excellent resource for schools and the public. Technical Details: Related Links: Tomorrow's LPOD: Double Your Pleasure – The Moon By Day |
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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.
