Difference between revisions of "February 23, 2005"
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=The Big and Little of It= | =The Big and Little of It= | ||
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| − | <tr><td><div align="center" class="main_sm">Image Credit: [mailto:anthony@perseus.gr Anthony Ayiomamitis]</p> | + | <tr><td><div align="center" class="main_sm"><p>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="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 [[February_21,_2005|lunar phase poster]] as an excellent resource for schools and the public.</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 [[February_21,_2005|lunar phase poster]] as an excellent resource for schools and the public.</p> | ||
| − | <blockquote><p align="right">— [mailto:tychocrater@yahoo.com Chuck Wood]</blockquote> | + | <blockquote> |
| − | <p align="left" | + | <p align="right">— [mailto:tychocrater@yahoo.com Chuck Wood]</p></blockquote> |
| + | <p align="left"><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> | ||
<p><b>Related Links:</b><br> | <p><b>Related Links:</b><br> | ||
[http://www.perseus.gr/ Anthony’s Astro Gallery] | [http://www.perseus.gr/ Anthony’s Astro Gallery] | ||
<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 | + | </p> |
| + | <p><b>Yesterday's LPOD:</b> [[February 22, 2005|New Light On A Familiar Domefield]] </p> | ||
| + | <p><b>Tomorrow's LPOD:</b> [[February 24, 2005|Double Your Pleasure]] </p> | ||
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<p align="center" class="main_titles"><b>Author & Editor:</b><br> | <p align="center" class="main_titles"><b>Author & Editor:</b><br> | ||
[mailto:tychocrater@yahoo.com Charles A. Wood]</p> | [mailto:tychocrater@yahoo.com Charles A. Wood]</p> | ||
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Latest revision as of 14:11, 15 March 2015
The Big and Little of It
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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: Yesterday's LPOD: New Light On A Familiar Domefield Tomorrow's LPOD: Double Your Pleasure |
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Author & Editor: |
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