Difference between revisions of "October 21, 2004"

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<p align="center" class="main_titles"><b>Author &amp; Editor:</b><br>  
 
<p align="center" class="main_titles"><b>Author &amp; Editor:</b><br>  
 
[mailto:tychocrater@yahoo.com Charles A. Wood]</p>
 
[mailto:tychocrater@yahoo.com Charles A. Wood]</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 Pablo Lonnie Pacheco Railey]  (Es)<br>
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[mailto:chlegrand@free.fr Christian Legrand] (Fr)</p>
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[http://www.observingthesky.org/ ObservingTheSky.Org]</p>
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<p align="center" class="main_titles"><b>Visit these other PODs:</b> <br>
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[http://antwrp.gsfc.nasa.gov/apod/astropix.html Astronomy] | [http://www.msss.com/ Mars] | [http://epod.usra.edu/ Earth]</p>
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Revision as of 15:01, 15 March 2015

60 of Tycho


LPOD-2004-10-21.jpeg

LPOD-2004-10-21b.jpeg

Image Credit: Chris Cook


60 of Tycho

Do you have aperture fever? Do you crave a big scope - a 14" or maybe an 18"? If so, I say, stop thinking small! You can use the Mt Wilson 60" reflector for your lunar studies. This image was taken afocally at the big scope's Cassegrain focus with a standard digital camera. As Chris Cook says anyone can reserve a night on the 60" through the Mt Wilson Institute. The fee is $900 for a full night. So get together 9 of your closest astro-buddies and take the images of a lifetime for half the cost of a specialty eyepiece. If you have mastered your imaging techniques and have good seeing you might capture images like this. The floor of Tycho is smooth with impact melt - the same material that makes a dark ring around Tycho at full Moon, but what shows up remarkably well is the chain of small secondary craters (arrowed on mouseover) to the northwest. These well-resolved craters are about 1.5 km wide. Also note that most of this field is peppered with a roughness that is partially due to Tycho ejecta raining down everywhere. But look at the floor of Tycho D and other nearby small craters. The smoothness of these floors suggests younger surfaces that are hard to explain. Also note the small domical hill on the floor of Heinsius Q - is that a lump of secondary ejecta, a wall slump, or a highland dome? Another peculiar rounded mound is arrowed SW of Heinsius. High resolution views always bring new questions!

Chuck Wood

Technical Details:
June 30, 2001, 8:18 pm PDT. Mt Wilson 60" reflector at the f/16 Cassegrain focus (24,384mm focal lenght) with a 100mm Masuyama Kellner eyepiece + Nikon Coolpix 800 digital camera, exposure: 1/30th second; minor enhancement in Adobe Photoshop 6.0.

Related Links:
["www.cookphoto.com" Chris Cook Photography]
Rukl Atlas of the Moon, Sheet 64

Yesterday's LPOD: Rough Domes

Tomorrow's LPOD: H-Alpha Moon



Author & Editor:
Charles A. Wood

 


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