Difference between revisions of "January 15, 2004"

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=Gassendi Compared=
 
=Gassendi Compared=
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<td><div align="center" span class="main_sm">Image Credit:   
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<td><div align="center" span class="main_sm"><p>Image Credit:   
 
[mailto:john@jsussenbach.nl John Sussenbach] and
 
[mailto:john@jsussenbach.nl John Sussenbach] and
[http://www.lpi.usra.edu/research/lunar_orbiter/ NASA Lunar Orbiter IV]
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[http://www.lpi.usra.edu/research/lunar_orbiter/ NASA Lunar Orbiter IV]</p>
 
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astroimager John Sussenbach notes that his image has a resolution of about 0.3 seconds of arc, which is both better than  
 
astroimager John Sussenbach notes that his image has a resolution of about 0.3 seconds of arc, which is both better than  
 
theoretical for an 11" and comparable with the Lunar Orbiter image. Gassendi (diameter 110 km) is another floor-fractured  
 
theoretical for an 11" and comparable with the Lunar Orbiter image. Gassendi (diameter 110 km) is another floor-fractured  
crater, like [LPOD-2004-01-09.htm Posidonius] and [LPOD-2004-01-07.htm Petavius]. The crater  
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crater, like [[January_9,_2004|Posidonius]] and [[January_7,_2004|Petavius]]. The crater  
 
has been shallowed by floor uplift and lava flooding.  
 
has been shallowed by floor uplift and lava flooding.  
 
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[http://www.jsussenbach.nl/ Sussenbach's Digital Astroimaging Using Webcam]<br>
 
[http://www.jsussenbach.nl/ Sussenbach's Digital Astroimaging Using Webcam]<br>
 
[http://www.scienceandyou.org/articles/ess_11.shtml Gassendi the scientist]</p>
 
[http://www.scienceandyou.org/articles/ess_11.shtml Gassendi the scientist]</p>
<p class="story"> <b>Tomorrow's LPOD:</b> The End of Lunar Studies</p>
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<p><b>Yesterday's LPOD:</b> [[January 14, 2004|First and Last]] </p>
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<p><b>Tomorrow's LPOD:</b> [[January 16, 2004|The End of Lunar Studies]] </p>
 
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<td><p align="center" class="main_titles"><b>Author & Editor:</b><br>
 
<td><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>
<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>A service of:</b><br>
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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></td>
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===COMMENTS?===
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Latest revision as of 19:10, 7 February 2015

Gassendi Compared

LPOD-2004-01-15.jpeg

Gassendi Compared

The advent of webcams and image compositing and enhancing software has given amateur astronomers with modest size instruments the ability to acquire lunar images that equal or surpass the very best professional images. Now amateurs are pushing up against the resolution of space craft imaging. In this comparison of the lunar crater Gassendi, Dutch astroimager John Sussenbach notes that his image has a resolution of about 0.3 seconds of arc, which is both better than theoretical for an 11" and comparable with the Lunar Orbiter image. Gassendi (diameter 110 km) is another floor-fractured crater, like Posidonius and Petavius. The crater has been shallowed by floor uplift and lava flooding.

Technical Details:
Left image taken with a C11 and 2x Barlow plus Toucam Pro webcam on March 13, 2003. John stacked 150 of 1800 frames. Right image from multi-million dollar NASA spacecraft in lunar orbit.

Related Links:
Sussenbach's Digital Astroimaging Using Webcam
Gassendi the scientist

Yesterday's LPOD: First and Last

Tomorrow's LPOD: The End of Lunar Studies


Author & Editor:
Charles A. Wood

 


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