<?xml version="1.0" encoding="utf-8"?>
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    <title>Belt of Venus</title>
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    <id>tag:www.perezmedia.net,2008-12-30:/beltofvenus/5</id>
    <updated>2010-03-08T06:22:44Z</updated>
    
    <generator uri="http://www.sixapart.com/movabletype/">Movable Type Pro 4.23-en</generator>

<entry>
    <title>Drawn to the UniverseAPR 2010 - Markarian&apos;s Chain</title>
    <link rel="alternate" type="text/html" href="http://www.perezmedia.net/beltofvenus/archives/001415.html" />
    <id>tag:www.perezmedia.net,2010:/beltofvenus//5.1415</id>

    <published>2010-03-08T05:14:21Z</published>
    <updated>2010-03-08T06:22:44Z</updated>

    <summary>Markarian&apos;s Chain is overflowing with galactic treasures and is the subject of the April 2010 column. Subject:Markarian&apos;s Chain Issue:April 2010 Astronomy Now Basic Media:Graphite on White Paper Featured Technique:Pre-plotting a stellar framework using an atlas or planetarium software, then sketching...</summary>
    <author>
        <name>Jeremy Perez</name>
        <uri>http://beltofvenus.perezmedia.net</uri>
    </author>
    
        <category term="Article" scheme="http://www.sixapart.com/ns/types#category" />
    
    
    <content type="html" xml:lang="en" xml:base="http://www.perezmedia.net/beltofvenus/">
        <![CDATA[<p>Markarian's Chain is overflowing with galactic treasures and is the subject of the April 2010 column.</p>

<table class="objectdata" style="margin-bottom: 15px;"> 
<tr><td><b>Subject:</b></td><td class="subject">Markarian's Chain</td></tr> 
<tr><td><b>Issue:</b></td><td><a href="http://www.astronomynowstore.com/ww/catalog/product_info.php?products_id=325" target="_blank">April 2010</a> <i>Astronomy Now</i></td></tr>
<tr><td><b>Basic Media:</b></td><td>Graphite on White Paper</td></tr> 
<tr><td><b>Featured Technique:</b></td><td>Pre-plotting a stellar framework using an atlas or planetarium software, then sketching galaxies and fainter stars across multiple telescopic fields.</td></tr>
<tr><td><b>Suggested Materials:</b></td><td>
<ul>
<li>Atlas or planetarium software</li>
<li>White artist grade paper</li>
<li>2H and HB Graphite Pencils</li>
<li>Clipboard and portable observing light</li>
</ul>
</td></tr>
</table>

<div class="imageblock"><A HREF="images/2010/img201004AN_mchainposlg.jpg" onMouseOver="rollover('img201004AN')" onMouseOut="rollout('img201004AN')"><IMG SRC="images/2010/img201004AN_mchainposA.jpg" NAME="img201004AN" ALT="Inverted, Positive Sketch of Markarian's Chain"></A>
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<p class="caption">Inverted, Positive Sketch of Markarian's Chain</p>
<p><i>Move mouse over image to view labels<br />Click for larger version.</i></p></div>

<div class="imageblock"><a href="images/2010/img201004AN_mchainneglg.jpg" target="_blank"><img src="images/2010/img201004AN_mchainneg.jpg" alt="Original Pencil Sketch of Markarian's Chain"></a><p class="caption">Original Pencil Sketch of Markarian's Chain</p><p><i>Click image to view larger version.</i></p></div>]]>
        
    </content>
</entry>

<entry>
    <title>90 Leonis (Struve 1552)</title>
    <link rel="alternate" type="text/html" href="http://www.perezmedia.net/beltofvenus/archives/001414.html" />
    <id>tag:www.perezmedia.net,2010:/beltofvenus//5.1414</id>

    <published>2010-02-28T23:08:54Z</published>
    <updated>2010-02-28T23:40:00Z</updated>

    <summary>90 Leonis</summary>
    <author>
        <name>Jeremy Perez</name>
        <uri>http://beltofvenus.perezmedia.net</uri>
    </author>
    
        <category term="Double Star" scheme="http://www.sixapart.com/ns/types#category" />
    
        <category term="SG-Double Star" scheme="http://www.sixapart.com/ns/types#category" />
    
        <category term="SGC-Leo" scheme="http://www.sixapart.com/ns/types#category" />
    
    
    <content type="html" xml:lang="en" xml:base="http://www.perezmedia.net/beltofvenus/">
        <![CDATA[<div class="imageblock"><a href="images/2009/img2009112601_90LEOlg.jpg" target="_blank"><img src="images/2009/img2009112601_90LEO.jpg" alt="Sketch of 90 Leonis (Struve 1552/STF 1552)"></a><p class="caption">Sketch of 90 Leonis (Struve 1552)</p><p><i>Click image to view larger version.</i></p></div> 

<p><b>Observation Notes:</b></p> 
<p>The trio of 90 Leonis appeared sky blue, cream, and dull orange. Sissy Haas sees yellow, yellow, gray and Smyth saw silvery-white, purplish, pale-red. </p>

<table class="objectdata">
<tr><td><b>Subject</b></td><td class="subject">90 Leonis (STF 1552 / ADS 8220)</td></tr>
<tr><td><b>Classification</b></td><td>Multiple Star</td></tr>
<tr><td><b>Position (J2000)*</b></td><td>Sextans [RA: 11 34 42.5 / Dec: +16 47 48.9]</td></tr>
<tr><td><b>Position Angle</b></td><td>AB: 214&deg; [My Measurement 2009.9]<br />AB: 208&deg; [WDS 2007]*<br />AC: 234&deg;<br />AC: 235&deg; [WDS 2007]*</td></tr>
<tr><td><b>Separation</b></td><td>AB: 4" [My Measurement 2009.9]<br />AB: 3.5" [WDS 2007]*<br />AC: 63" [My Measurement 2009.9]<br />AC: 63.2" [WDS 2007]*</td></tr>
<tr><td><b>Magnitudes*</b></td><td>A: 6.3; B: 7.3 C: 9.8</td></tr>
<tr><td><b>Spectral Types*</b></td><td>A: B4V; B: B9V; C: F5</td></tr>
<tr><td><b>Date/Time</b></td><td>NOV 26, 2009 - 4:50 AM (NOV 26, 2009 - 11:50 UT)</td></tr>
<tr><td><b>Observing Loc.</b></td><td>Flagstaff, AZ - Home</td></tr>
<tr><td><b>Instrument</b></td><td>Orion SkyQuest XT8 Dobsonian (203 mm dia./1200 mm F/L)</td></tr>
<tr><td><b>Eyepieces/Mag.</b></td><td>Pentax XW10 + 2X Barlow (240X)<br />Meade Astrometric EP + 2X Barlow (200X)</td></tr>
<tr><td><b>Conditions</b></td><td>Clear, cold</td></tr>
<tr><td><b>Seeing</b></td><td>3/10 Pickering</td></tr>
<tr><td><b>Transparency</b></td><td>Mag 6.0 NELM</td></tr>
<tr><td><b>*References</b></td><td>The Washington Visual Double Star Catalog (Mason+ 2001-2009); Catalogue of Stellar Spectral Classifications (Skiff, 2009); SIMBAD; <i>Double Stars for Small Telescopes</i> - Sissy Haas</td></tr>
</table>]]>
        
    </content>
</entry>

<entry>
    <title>35 Sextantis (Struve 1466)</title>
    <link rel="alternate" type="text/html" href="http://www.perezmedia.net/beltofvenus/archives/001413.html" />
    <id>tag:www.perezmedia.net,2010:/beltofvenus//5.1413</id>

    <published>2010-02-28T02:59:40Z</published>
    <updated>2010-02-28T23:40:28Z</updated>

    <summary>35 Sextantis</summary>
    <author>
        <name>Jeremy Perez</name>
        <uri>http://beltofvenus.perezmedia.net</uri>
    </author>
    
        <category term="Double Star" scheme="http://www.sixapart.com/ns/types#category" />
    
        <category term="SG-Double Star" scheme="http://www.sixapart.com/ns/types#category" />
    
        <category term="SGC-Sextans" scheme="http://www.sixapart.com/ns/types#category" />
    
    
    <content type="html" xml:lang="en" xml:base="http://www.perezmedia.net/beltofvenus/">
        <![CDATA[<div class="imageblock"><a href="images/2009/img2009112601_35SEXTANSlg.jpg" target="_blank"><img src="images/2009/img2009112601_35SEXTANS.jpg" alt="Sketch of 35 Sextantis (Struve 1466/STF 1466)"></a><p class="caption">Sketch of 35 Sextantis (Struve 1466)</p><p><i>Click image to view larger version.</i></p></div> 

<p><b>Observation Notes:</b></p> 
<p>This nice yellow-orange/pale blue binary was also seen as citrus-orange/blended-blue-green (Haas) and topaz-yellow/smalt-blue (Smyth). The faint C star showed to the southwest, but I didn't realize it was a component, so I didn't measure it.</p>

<table class="objectdata">
<tr><td><b>Subject</b></td><td class="subject">35 Sextantis (STF 1466 / ADS 7902)</td></tr>
<tr><td><b>Classification</b></td><td>Multiple Star</td></tr>
<tr><td><b>Position (J2000)*</b></td><td>Sextans [RA: 10 43 20.9 / Dec: +04 44 51.6]</td></tr>
<tr><td><b>Position Angle</b></td><td>AB: 239&deg; [My Measurement 2009.9]<br />AB: 239&deg; [WDS 2008]*<br />AC: 210&deg; [WDS 2003]*</td></tr>
<tr><td><b>Separation</b></td><td>AB: 8" [My Measurement 2009.9]<br />AB: 6.8" [WDS 2008]*<br />AC: 333.8" [WDS 2003]*</td></tr>
<tr><td><b>Magnitudes*</b></td><td>A: 6.2; B: 7.1 C: 8.1</td></tr>
<tr><td><b>Spectral Types*</b></td><td>A: K3III; B: K7D</td></tr>
<tr><td><b>Date/Time</b></td><td>NOV 26, 2009 - 4:10 AM (NOV 26, 2009 - 11:10 UT)</td></tr>
<tr><td><b>Observing Loc.</b></td><td>Flagstaff, AZ - Home</td></tr>
<tr><td><b>Instrument</b></td><td>Orion SkyQuest XT8 Dobsonian (203 mm dia./1200 mm F/L)</td></tr>
<tr><td><b>Eyepieces/Mag.</b></td><td>Pentax XW10 + 2X Barlow (240X)<br />Meade Astrometric EP + 2X Barlow (200X)</td></tr>
<tr><td><b>Conditions</b></td><td>Clear, cold</td></tr>
<tr><td><b>Seeing</b></td><td>3/10 Pickering</td></tr>
<tr><td><b>Transparency</b></td><td>Mag 6.0 NELM</td></tr>
<tr><td><b>*References</b></td><td>The Washington Visual Double Star Catalog (Mason+ 2001-2009); Catalogue of Stellar Spectral Classifications (Skiff, 2009); SIMBAD; <i>Double Stars for Small Telescopes</i> - Sissy Haas</td></tr>
</table>]]>
        
    </content>
</entry>

<entry>
    <title>Starscapes at Sunset Crater National Monument - FEB 13, 2010</title>
    <link rel="alternate" type="text/html" href="http://www.perezmedia.net/beltofvenus/archives/001411.html" />
    <id>tag:www.perezmedia.net,2010:/beltofvenus//5.1411</id>

    <published>2010-02-23T02:44:58Z</published>
    <updated>2010-02-23T04:03:06Z</updated>

    <summary><![CDATA[ Orion, Canis Major, and the Winter Milky Way soar over Sunset Crater Click for larger image FEB 13, 2010 - 01:00 AM MST Canon EOS 300D + Kit Lens @ 21 mm &bull; ISO 800 &bull; f/4.5 Composite: 11...]]></summary>
    <author>
        <name>Jeremy Perez</name>
        <uri>http://beltofvenus.perezmedia.net</uri>
    </author>
    
        <category term="Astro Photography" scheme="http://www.sixapart.com/ns/types#category" />
    
    
    <content type="html" xml:lang="en" xml:base="http://www.perezmedia.net/beltofvenus/">
        <![CDATA[<div class="imageblock">
<a href="images/2010/img2010021301_SunsetCraterlg.jpg"><img src="images/2010/img2010021301_SunsetCrater.jpg" alt="Photo of Orion, Canis Major, and the Winter Milky Way over Sunset Crater"></a>
<p class="caption">Orion, Canis Major, and the Winter Milky Way soar over Sunset Crater</p>
<p><i>Click for larger image</i><br />
FEB 13, 2010 - 01:00 AM MST<br />
Canon EOS 300D + Kit Lens @ 21 mm &bull; ISO 800 &bull; f/4.5<br />
Composite: 11 x 30 sec. aligned, stacked, and composited separately for sky and foreground</p>
</div>

<p>I said I was going to try this again. Things worked a little better this time (including remembering to check my ISO setting). I arrived early (12:30 AM :) at Cinder Hills Overlook to work on an observation and sketch of Messier 101. Orion and Sirius would be in good position over Sunset Crater between 12:30 and 1:30 AM. After getting the series of shots I wanted, I couldn't resist shooting another set to the northwest showing Orion, the Hyades, and the Pleiades all setting behind the hills and trees.</p>

<div class="imageblock">
<a href="images/2010/img2010021303_SunsetCraterlg.jpg"><img src="images/2010/img2010021303_SunsetCrater.jpg" alt="Photo of Mars, Procyon, and Sirius lining up over Sunset Crater"></a>
<p class="caption">Mars, Procyon, and Sirius line up over Sunset Crater</p>
<p><i>Click for larger image</i><br />
FEB 13, 2010 - 01:00 AM MST<br />
Canon EOS 300D + Kit Lens @ 21 mm &bull; ISO 800 &bull; f/4.5<br />
Composite: 6 x 30 sec. aligned, stacked, and composited separately for sky and foreground</p>
</div>

<p>I got three shots into that series before Rigel winked out behind the mountain. At that point, I noticed that Sirius, Procyon and Mars were making a brilliant alignment over the peak of the volcano. So I worked on a vertical series to capture them.</p>

<div class="imageblock">
<a href="images/2010/img2010021302_SunsetCraterlg.jpg"><img src="images/2010/img2010021302_SunsetCrater.jpg" alt="Photo of Mars, Procyon, and Sirius lining up over Sunset Crater"></a>
<p class="caption">Mars, Procyon, and Sirius line up over Sunset Crater</p>
<p><i>Click for larger image</i><br />
FEB 13, 2010 - 01:00 AM MST<br />
Canon EOS 300D + Kit Lens @ 21 mm &bull; ISO 800 &bull; f/4.5<br />
Composite: 6 x 30 sec. aligned, stacked, and composited separately for sky and foreground</p>
</div>
<p>Shooting 30 second tripod exposures makes random course-corrections pretty simple...perhaps too simple.</p>

<p>Processing one set of images is hard enough. Adding a second and third gave me a workout. It was a much needed workout too, since it forced me to refine my process. I made some improvements on the second image, and then again on the third image. By that time, I felt I had to go back and re-do the first and second again.</p>
<p>I've felt pretty confident handling stacking and compositing for sky and foreground. The processes I find challenging are:
<ol>
<li>Removing green/red blotchiness from the dark sky background</li>
<li>Removing just the right amount of noise without making the sky look plastic or crystalized</li>
<li>Reducing the appearance of vertical and horizontal bands in these short exposures.</li>
<li>Tamping down light pollution gradients with some level of finesse</li>
</ol>
</p>

<p>Briefly, some of the solutions I arrived at:
<ol>
<li>To color balance the background, I create a temporary layer, blur it extremely, and read RGB values in different parts of the sky that aren't hit hard by light pollution or air glow on the horizon. I then apply a curves adjustment layer to balance the background to an average of neutral. Unfortunately, that doesn't remove the color blotches. So I add a Hue/Saturation adjustment layer to substantially reduce saturation, and then use <i>Astronomy Tools</i> "Select Bright Stars" to create a mask for this layer that blocks out the stars, and leaves their color intact. Unfortunately, this removes the ability to feature any photographic color in the Milky Way, but for the type of color noise I have to deal with in these 30 second exposures, I think it's a good sacrifice. I also like the way it better conveys the more neutral visual experience of the sky.</li>
<li>I use Neat Image to tackle noise. Wide field images like this tend not to have decent sized empty areas that the software can sample for average noise. As a result I have to play with the settings over and over again to get what I like. I still don't have a good system here. Just experimentation. I've saved my latest setting in hopes that I can use it again, but I have a feeling I'll still have to fiddle with it quite a bit every time.</li>
<li>The <i>Astronomy Tools</i> "Horizontal/Vertical Banding Noise Removal" action really does a great job removing much of the banding. However I've got some pretty huge bands in these frames, and it doesn't remove those. Wherever these hit a soft hint of Milky Way, they become impossible to remove. A new camera may eventually help this situation :)</li>
<li>A couple of the shots contained a pretty ripe light pollution tongue that tore right into the Milky Way. It doesn't seem that obnoxious visually, so I did want to tame it a bit. I found that examining the individual color channels tended to give me some options. The green channel is the cleanest representation of the sky, but the blue channel hides the light pollution the best...the blue channel also seems to do a nice job of giving star groupings and the brightest blue stars a nice glow. I can do some channel blending operations to merge the best of these two channels to create a "Luminosity" layer. By setting this layer to Luminosity mode, I can trim the light pollution, bring out the Milky Way a little more, and in an added bonus, it blunts the horizontal/vertical banding a bit more if I'm careful how I blend blue and green (the blue usually has much worse banding than green). Adding a Hue/Saturation adjustment layer that subtly reduces the intensity of the yellow in shadow and midtones (to exclude stars) helps too.</li>
</ol>
</p>
<p>I've still got a lot of improvement to do, but with the system I've scripted out, I have high hopes it will go smoother on my next attempts.</p>]]>
        
    </content>
</entry>

<entry>
    <title>Markarian&apos;s Chain</title>
    <link rel="alternate" type="text/html" href="http://www.perezmedia.net/beltofvenus/archives/001410.html" />
    <id>tag:www.perezmedia.net,2010:/beltofvenus//5.1410</id>

    <published>2010-02-21T03:45:19Z</published>
    <updated>2010-02-21T05:49:33Z</updated>

    <summary>Markarian&apos;s Chain</summary>
    <author>
        <name>Jeremy Perez</name>
        <uri>http://beltofvenus.perezmedia.net</uri>
    </author>
    
        <category term="Deep Sky" scheme="http://www.sixapart.com/ns/types#category" />
    
        <category term="Galaxy" scheme="http://www.sixapart.com/ns/types#category" />
    
        <category term="SG-Deep Sky" scheme="http://www.sixapart.com/ns/types#category" />
    
        <category term="SG-Galaxy" scheme="http://www.sixapart.com/ns/types#category" />
    
        <category term="SGC-Coma Berenices" scheme="http://www.sixapart.com/ns/types#category" />
    
        <category term="SGC-Virgo" scheme="http://www.sixapart.com/ns/types#category" />
    
        <category term="Sketch Gallery" scheme="http://www.sixapart.com/ns/types#category" />
    
    
    <content type="html" xml:lang="en" xml:base="http://www.perezmedia.net/beltofvenus/">
        <![CDATA[<div class="imageblock"><A HREF="images/2010/img2010011502_MarkariansChain01lg.jpg" onMouseOver="rollover('img2010011502')" onMouseOut="rollout('img2010011502')"><IMG SRC="images/2010/img2010011502_MarkariansChain01A.jpg" NAME="img2010011502" ALT="Sketch of Markarian's Chain in the Virgo Cluster"></A>
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<p class="caption">Sketch of Markarian's Chain in the Virgo Cluster</p>
<p><i>Move mouse over image to view labels (magnitudes listed in parentheses)<br />Click for larger version.</i></p></div>

<p><b>Observation Notes:</b></p> 
<p>The heart of the Virgo Cluster is a wonderful place to visit from a dark site. Every nudge of the telescope brings another galaxy...or three or five into the eyepiece...and it's hard to beat the density around Markarian's Chain.</p>
<p>In preparation for a tour of the area, I printed a chart and pre-traced 31 of the brightest stars to serve as a multi-field framework on a 9" x 12" sketch sheet. This saved a lot of sketching frustration as I panned across the 2.5&deg; x 4&deg; field. Over the course of the three hour observation, I ended up with 27 galaxies from 8.8 magnitude Messier 87 to 13.1 magnitude IC 3258. Most were quick catches, but a few required some star chart scrutiny to locate.</p>
<p>The list of galaxies observed:
<ul>
<li>Messier 84 (vMag 9.4)</li>
<li>Messier 86 (vMag 9.0)</li>
<li>Messier 87 (vMag 8.8)</li>
<li>Messier 88 (vMag 9.7)</li>
<li>NGC 4351 (vMag 12.3)</li>
<li>NGC 4377 (vMag 11.9)</li>
<li>NGC 4387 (vMag 12.1)</li>
<li>NGC 4388 (vMag 11.3)</li>
<li>NGC 4402 (vMag 12.2)</li>
<li>NGC 4413 (vMag 12.3)</li>
<li>NGC 4425 (vMag 11.8)</li>
<li>NGC 4431 (vMag 12.9)</li>
<li>NGC 4435 (vMag 10.8)</li>
<li>NGC 4438 (vMag 10.0)</li>
<li>NGC 4440 (vMag 12.1)</li>
<li>NGC 4458 (vMag 12.1)</li>
<li>NGC 4459 (vMag 10.4)</li>
<li>NGC 4461 (vMag 11.1)</li>
<li>NGC 4468 (vMag 13.0)</li>
<li>NGC 4473 (vMag 10.1)</li>
<li>NGC 4474 (vMag 11.8)</li>
<li>NGC 4476 (vMag 12.1)</li>
<li>NGC 4477 (vMag 10.4)</li>
<li>NGC 4478 (vMag 11.3)</li>
<li>NGC 4479 (vMag 12.6)</li>
<li>NGC 4506 (vMag 12.9)</li>
<li>IC 3258 (vMag 13.1)</li>
</ul>
<p>Each of these galaxies is worth its own dedicated observation and sketch, but I wanted this to be more about the swarm than the individuals. Fortunately, the full page size of the sketch allowed some leeway for conveying a little detail in most of the galaxies--particularly Messier 88 and NGC 4438. As David Moody often advises, don't let your eyepiece field stop dictate the extent of your sketch. It's good advice.</p>
<p>
<table class="objectdata">
<tr><td><b>Subject</b></td><td class="subject">Markarian's Chain:</td></tr>
<tr><td><b>Classification</b></td><td>Galaxy Chain</td></tr>
<tr><td><b>Position (J2000)*</b></td><td>Virgo and Coma Berenices</td></tr>
<tr><td><b>Date/Time</b></td><td>JAN 15, 2010:  02:00 - 05:00 AM (JAN 15, 2010: 09:00 - 12:00 UT)</td></tr>
<tr><td><b>Observing Loc.</b></td><td>Cinder Hills Overlook, Sunset Crater National Monument, AZ</td></tr>
<tr><td><b>Instrument</b></td><td>Orion SkyQuest XT8 Dobsonian (203 mm dia./1200 mm F/L)</td></tr>
<tr><td><b>Eyepieces/Mag.</td><td>32 mm Sirius Pl&ouml;ssl (37.5X); Pentax XW10 (120X); + 2X Barlow (240X)</td></tr>
<tr><td><b>Conditions</b></td><td>Clear, cold, slight breeze</td></tr>
<tr><td><b>Seeing</b></td><td>5/10 Pickering</td></tr>
<tr><td><b>Transparency</b></td><td>Mag 7.0+ NELM</td></tr>
<tr><td><b>*References</b></td><td>Starry Night Pro Plus 5.x; <a href="http://www.ngcicproject.com" target="_blank">NGCIC Project</a></td></tr>
</table>]]>
        
    </content>
</entry>

<entry>
    <title>Drawn to the UniverseMAR 2010 - Tau and 83 Leonis</title>
    <link rel="alternate" type="text/html" href="http://www.perezmedia.net/beltofvenus/archives/001409.html" />
    <id>tag:www.perezmedia.net,2010:/beltofvenus//5.1409</id>

    <published>2010-02-20T03:51:13Z</published>
    <updated>2010-02-20T04:30:02Z</updated>

    <summary>Tau and 83 Leonis make a stunning and colorful low power double-double and are the subject of March 2010 Drawn to the Universe Column in Astronomy Now. Subject:Tau and 83 Leonis Issue:March 2010 Astronomy Now Basic Media:Graphite on Paper and...</summary>
    <author>
        <name>Jeremy Perez</name>
        <uri>http://beltofvenus.perezmedia.net</uri>
    </author>
    
        <category term="Article" scheme="http://www.sixapart.com/ns/types#category" />
    
    
    <content type="html" xml:lang="en" xml:base="http://www.perezmedia.net/beltofvenus/">
        <![CDATA[<p>Tau and 83 Leonis make a stunning and colorful low power double-double and are the subject of March 2010 Drawn to the Universe Column in <i>Astronomy Now</i>.</p>

<table class="objectdata" style="margin-bottom: 15px;"> 
<tr><td><b>Subject:</b></td><td class="subject">Tau and 83 Leonis</td></tr> 
<tr><td><b>Issue:</b></td><td><a href="http://www.astronomynowstore.com/ww/catalog/product_info.php?products_id=324" target="_blank">March 2010</a> <i>Astronomy Now</i></td></tr>
<tr><td><b>Basic Media:</b></td><td>Graphite on Paper and Digital Editing</td></tr> 
<tr><td><b>Featured Technique:</b></td><td>Using image editing software to create digital double star sketches.</td></tr>
<tr><td><b>Suggested Materials:</b></td><td>
<ul>
<li>Observing forms or white paper with pre-drawn circles</li>
<li>Pencil</li>
<li>Clipboard and portable observing light</li>
<li>Scanner and image editing software such as Adobe Photoshop, Photoshop Elements, Paintshop Pro or <a href="http://www.gimp.org" target="_blank">GIMP</a></li>
</ul>
</td></tr>
</table>

<div class="imageblock"><a href="images/2010/img201003AN_TauLEOlg.jpg" target="_blank"><img src="images/2010/img201003AN_TauLEO.jpg" alt="Digital Sketch of Tau and 83 Leonis"></a><p class="caption">Digital Sketch of Tau and 83 Leonis</p><p><i>Click image to view larger version.</i></p></div>

<div class="imageblock"><a href="images/2010/img201003AN_TauLEOoriglg.jpg" target="_blank"><img src="images/2010/img201003AN_TauLEOorig.jpg" alt="Original Pencil Sketch of Tau and 83 Leonis"></a><p class="caption">Original Pencil Sketch of Tau and 83 Leonis</p><p><i>Click image to view larger version.</i></p></div>]]>
        
    </content>
</entry>

<entry>
    <title>Cinder Hills Overlook</title>
    <link rel="alternate" type="text/html" href="http://www.perezmedia.net/beltofvenus/archives/001408.html" />
    <id>tag:www.perezmedia.net,2010:/beltofvenus//5.1408</id>

    <published>2010-02-12T04:00:39Z</published>
    <updated>2010-02-23T05:43:16Z</updated>

    <summary> Orion, Canis Major and the Winter Milky Way soar over Sunset Crater as seen from Cinder Hills Overlook Cinder Hills Overlook is a cul-de-sac at the top of a small hill on the eastern edge of Sunset Crater National...</summary>
    <author>
        <name>Jeremy Perez</name>
        <uri>http://beltofvenus.perezmedia.net</uri>
    </author>
    
        <category term="Article" scheme="http://www.sixapart.com/ns/types#category" />
    
    
    <content type="html" xml:lang="en" xml:base="http://www.perezmedia.net/beltofvenus/">
        <![CDATA[<div class="imageblock">
<p><a href="images/2010/img2010021301_SunsetCraterlg.jpg"><img src="images/2010/img2010021301_SunsetCrater.jpg"></a></p>
<p class="caption">Orion, Canis Major and the Winter Milky Way soar over Sunset Crater as seen from Cinder Hills Overlook</p>
</div>

<p>Cinder Hills Overlook is a cul-de-sac at the top of a small hill on the eastern edge of Sunset Crater National Monument. The site is situated amid a stunning volcanic landscape with gorgeous, dark skies after evening twilight. The entrance to the park is a mere 12 miles north of Flagstaff on Highway 89.</p>

<p>Because this is within the boundary of a national monument, be sure to obey any posted signs. One standing rule is that there is no camping allowed inside the monument. So, if you need some sleep after packing things up for the night, you will need to move down the road a bit. There is a forest service road just across the main road from the Cinder Hills Overlook entrance. This forest service road heads outside the monument, and there are a number of places to pull off to get some rest.</p>

<p>This is common sense, but it bears stating--please treat this site with respect so that others will be able to enjoy it in the future:</p>
<ul><li>Park and set up equipment in a way that does not block vehicle traffic that may need to pass</li>
<li>Pack out all trash</li>
<li>Do not hike off road or off trail inside the monument</li>
<li>Obey posted signs</li>
<li>Cooperate with park personnel</li></ul>

<p>The site can accommodate several vehicles. However, if you wish to plan an observing event, please contact a ranger at the visitor center beforehand to discuss your plans.</p>

<div class="imageblock">
<p><a href="images/2010/img2010021101_SunsetCraterAeriallg.jpg"><img src="images/2010/img2010021101_SunsetCraterAerial.jpg"></a></p>
<p class="caption">Google Earth aerial view of Cinder Hills Overlook - Facing Southwest</p>
</div>

<hr />

<div class="imageblock">
<p><img src="images/2010/img2010021101_Map.jpg"></p>
<p class="caption">Google Maps view of Cinder Hills Overlook<br />
<a href="http://maps.google.com/?ie=UTF8&amp;t=h&amp;ll=35.37166,-111.490567&amp;spn=0.006124,0.00912&amp;z=16&amp;source=embed" style="color:#0000FF;text-align:left">View Browsable Map</a>
</p>
</div>

<hr />


<div style="margin-top: 15px">
<h3>Site Information</h3>
<p><table class="objectdata">
<tr><td><b>Site Name</b></td><td><b style="color: white">Cinder Hills Overlook &mdash; Sunset Crater National Monument</b></td></tr>
<tr><td><b>Coordinates</b></td><td>35 22 17.2 N / 111 29 25.1 W</td></tr>
<tr><td><b>Elevation</b></td><td>7065 ft (2153 m)</td></tr>
<tr><td><b>Directions</b></td><td>Drive 12 miles north of Flagstaff on US Hwy 89. Turn right at the Sunset Crater/Wupatki Loop entrance. Drive 2 miles to the visitor center. If you arrive before 5 PM, you can pay the entrance fee at the booth or visitor center. After 5 PM, the booth and visitor center are closed, but the road remains open all night. Cinder Hills Overlook, is 3.5 miles beyond the visitor center, on the right side of the road. Drive another .2 mile to the cul-de-sac </td></tr>
<tr><td><b>Accessibility</b></td><td>Easy access. Paved road all the way to the parking area. Parking area is asphalt.</td></tr>
<tr><td><b>Capacity</b></td><td>Parking area can accommodate several vehicles and equipment. </td></tr>
<tr><td><b>Horizon</b></td><td>There are a few trees and snags around the parking area--primarily on the north side. The horizon to the south and east are excellent. The bulk of Sunset Crater volcano lies to the west and southwest.</td></tr>
<tr><td><b>Light Domes</b></td><td>Senset Crater does an excellent job blocking the modest Flagstaff light dome to the southwest. The light dome can be seen along the southern slope of the volcano, but it does not otherwise adversely effect sky quality.</td></tr>
<tr><td><b>Weather</b></td><td>
<b>Temperature Ranges</b><br />
<b>Jan:</b> Avg. Max: 43&deg;F / Avg. Min: 17&deg;F<br />
<b>Apr:</b> Avg. Max: 58&deg;F / Avg. Min: 27&deg;F<br />
<b>Jul:</b> Avg. Max: 82&deg;F / Avg. Min: 50&deg;F<br />
<b>Oct:</b> Avg. Max: 63&deg;F / Avg. Min: 31&deg;F<br />
Nocturnal cold air drainage can be a problem here, and this area is prone to stronger winds than the surrounding plateau. If the wind becomes a problem, heading north to Wupatki National Monument can sometimes bring relief. All Northern Arizona sites are susceptible to cloudy weather during the monsoon season which runs on average from early July through mid-September. The months of May and June are on average the most reliably dry months of the year.</td></tr>
<tr><td><b>Incidental Traffic</b></td><td>The site rarely sees nighttime traffic. However, if someone heads up the road to the cul-de-sac, you will have advance warning to protect your vision as approaching headlights are filtered through numerous downhill trees. Parts of the main park road below are visible from the observing site. Headlights are a minor nuisance, but traffic is very infrequent, especially during the winter months. During summer, the cinder hills 1.5 miles south of the site may play host to the flickering headlights of off-road vehicles enjoying nighttime recreation. If this happens, observing objects away from the southern horizon can help remove the distraction until things settle down later in the evening.</td></tr>

<tr><td><b>Seeing</b></td><td>Seeing is hit and miss here.</td></tr>
<tr><td><b>Transparency</b></td><td>High elevation and typically dry air make for excellent transparency.</td></tr>
</table>



<h3>Photo Gallery</h3>
<ul class="gallery">

<li><a href="001411.html"><h5>Mars, Procyon and<br />Sirius Line Up<br />&nbsp;</h5></a>
<a href="images/2010/img2010021302_SunsetCraterlg.jpg" target="_blank"><img src="images/2010/img2010021302_SunsetCratert.jpg"></a><h4>&nbsp;</h4></li>

<li><a href="001411.html"><h5>Orion and Taurus<br />Setting<br />&nbsp;</h5></a>
<a href="images/2010/img2010021303_SunsetCraterlg.jpg" target="_blank"><img src="images/2010/img2010021303_SunsetCratert.jpg"></a><h4>&nbsp;</h4></li>

<li><a href="001411.html"><h5>Orion, Canis Major<br />Setting<br />&nbsp;</h5></a>
<a href="images/2010/img2010021301_SunsetCraterlg.jpg" target="_blank"><img src="images/2010/img2010021301_SunsetCratert.jpg"></a><h4>&nbsp;</h4></li>

<li><a href="000494.html"><h5>Orion and the<br />Winter Milky Way<br />&nbsp;</h5></a>
<a href="images/2005/img20051001_3918rev1lg.jpg" target="_blank"><img src="images/2005/img20051001_3918rev1t.jpg"></a><h4>&nbsp;</h4></li>

<li><a href="000494.html"><h5>Cygnus<br />Milky Way<br />&nbsp;</h5></a>
<a href="images/2005/img20051001_3926.jpg" target="_blank"><img src="images/2005/img20051001_3926t.jpg"></a><h4>&nbsp;</h4></li>

<li><a href="000494.html"><h5>Observing beside<br />Sunset Crater<br />&nbsp;</h5></a>
<a href="images/2005/img20051001_3915.jpg" target="_blank"><img src="images/2005/img20051001_3915t.jpg"></a><h4>&nbsp;</h4></li>

<li><a href="000494.html"><h5>Twilight Moonrise<br />&nbsp;<br />&nbsp;</h5></a>
<a href="images/2005/img20051001_3950LG.jpg" target="_blank"><img src="images/2005/img20051001_3950t.jpg"></a><h4>&nbsp;</h4></li>

<li><a href="000494.html"><h5>Cinder Hills<br />Sunrise<br />&nbsp;</h5></a>
<a href="images/2005/img20051001_3973LG.jpg" target="_blank"><img src="images/2005/img20051001_3973t.jpg"></a><h4>&nbsp;</h4></li>

<li><a href="000494.html"><h5>Sunrise Lights<br />Sunset Crater<br />&nbsp;</h5></a>
<a href="images/2005/img20051001_3986LG.jpg" target="_blank"><img src="images/2005/img20051001_3986t.jpg"></a><h4>&nbsp;</h4></li>

</ul>
</div>
<p>Updated February 11, 2010.</p>]]>
        
    </content>
</entry>

<entry>
    <title>Starset at Sunset Crater National Monument - JAN 15, 2010</title>
    <link rel="alternate" type="text/html" href="http://www.perezmedia.net/beltofvenus/archives/001404.html" />
    <id>tag:www.perezmedia.net,2010:/beltofvenus//5.1404</id>

    <published>2010-01-29T19:28:11Z</published>
    <updated>2010-01-29T19:40:17Z</updated>

    <summary><![CDATA[ Orion and Canis Major setting over Sunset Crater Click for larger image JAN 15, 2010 - 03:00 AM MST Canon EOS 300D + Kit Lens @ 21 mm &bull; ISO 200 &bull; f/4.5 Composite: 5 x 30 sec. aligned...]]></summary>
    <author>
        <name>Jeremy Perez</name>
        <uri>http://beltofvenus.perezmedia.net</uri>
    </author>
    
        <category term="Astro Photography" scheme="http://www.sixapart.com/ns/types#category" />
    
    
    <content type="html" xml:lang="en" xml:base="http://www.perezmedia.net/beltofvenus/">
        <![CDATA[<div class="imageblock">
<a href="images/2010/img2010011500_OrionSiriuslg.jpg"><img src="images/2010/img2010011500_OrionSirius.jpg" alt="Photo of Orion and Canis Major over Sunset Crater"></a>
<p class="caption">Orion and Canis Major setting over Sunset Crater</p>
<p><i>Click for larger image</i><br />
JAN 15, 2010 - 03:00 AM MST<br />
Canon EOS 300D + Kit Lens @ 21 mm &bull; ISO 200 &bull; f/4.5<br />
Composite: 5 x 30 sec. aligned and stacked for sky + 5 min. foreground</p>
</div>

<p>While observing at Sunset Crater a couple weeks ago, I was struck by the beauty of Orion and Canis Major setting over the snow-covered volcano. So I took a break at about 3 AM to take some photos. It was a spur of the moment decision, so I didn't get everything right. The photo above is a combination of 5 30-second shots aligned and stacked for the sky, and a 5 minute exposure of the foreground. I adjusted exposure on both sky and foreground to try and convey the relative brightness of both as naturally as possible. The moon wasn't out, so the snow is lit by starlight.</p>

<p>A couple of the things that went wrong--<br />
I was in a hurry to get the shot before the bright stars in Canis Major's legs dipped behind the peak, so I rushed through focus, and think I could have done better there. I also goofed up and didn't check my ISO setting...which was set to 200. D'oh! If I had set to ISO 800, I think I could have pulled the Milky Way out nicely. As it is, the Milky Way barely breaks through some severe horizontal banding noise, so I had to leave it alone. It's all about signal to noise, and I didn't grab enough signal. I did have the foresight to shoot in RAW, so I had otherwise decent data to play with. I could probably do better with the processing, but astro photos are really hard to process--especially when sensor noise wants to demolish the sky with every tiny curve move. So I called it good where it's at.</p>

<p>I do have plans to shoot this again when I head back out there in a couple weeks to work on a sketch for the May column. There should still be plenty of snow up there to catch the starlight. Also: ISO 800...ISO 800...ISO 800...</p>]]>
        
    </content>
</entry>

<entry>
    <title>Drawn to the UniverseFEB 2010 - Mars</title>
    <link rel="alternate" type="text/html" href="http://www.perezmedia.net/beltofvenus/archives/001403.html" />
    <id>tag:www.perezmedia.net,2010:/beltofvenus//5.1403</id>

    <published>2010-01-26T05:03:53Z</published>
    <updated>2010-01-26T05:26:32Z</updated>

    <summary>Mars is making its closest approach of 2010 on January 27. The red planet can be challenging to observe, but sketching your observations will help you get the most from the view at the eyepiece. In the February issue of...</summary>
    <author>
        <name>Jeremy Perez</name>
        <uri>http://beltofvenus.perezmedia.net</uri>
    </author>
    
        <category term="Article" scheme="http://www.sixapart.com/ns/types#category" />
    
    
    <content type="html" xml:lang="en" xml:base="http://www.perezmedia.net/beltofvenus/">
        <![CDATA[<p>Mars is making its closest approach of 2010 on January 27. The red planet can be challenging to observe, but sketching your observations will help you get the most from the view at the eyepiece. In the February issue of <i>Astronomy Now</i>, we cover methods you can use to sketch Mars.</p>

<table class="objectdata" style="margin-bottom: 15px;"> 
<tr><td><b>Subject:</b></td><td class="subject">Mars</td></tr> 
<tr><td><b>Issue:</b></td><td><a href="http://www.astronomynowstore.com/ww/catalog/product_info.php?products_id=323" target="_blank">February 2010</a> <i>Astronomy Now</i></td></tr>
<tr><td><b>Basic Media:</b></td><td>Graphite on artist grade paper.</td></tr> 
<tr><td><b>Featured Technique:</b></td><td>Creating contour field sketches with a value diagram to quickly render features, then using these to create a refined sketch later under controlled conditions. Sidebar suggests experimenting with color techniques as well.</td></tr>
<tr><td><b>Suggested Materials:</b></td><td>
<ul>
<li>Observing forms or white paper with pre-drawn circles 50 mm in diameter</li>
<li>Acid free drawing paper for the final drawing</li>
<li>HB, 2B, and optional 9B graphite pencils</li>
<li>Blending stump and artist's chamois</li>
<li>White vinyl eraser and putty rubber</li>
<li>Clipboard and portable observing light</li>
</ul>
</td></tr>
</table>

<div class="imageblock"><a href="images/2010/img201002AN_Marslg.jpg" target="_blank"><img src="images/2010/img201002AN_Mars.jpg" alt="Sketch of the Mars"></a><p class="caption">Sketch of Mars - CM 265&deg;</p><p><i>Click image to view larger version.</i></p></div>]]>
        
    </content>
</entry>

<entry>
    <title>Messier 42 and Messier 43 (The Orion Nebula)</title>
    <link rel="alternate" type="text/html" href="http://www.perezmedia.net/beltofvenus/archives/000325.html" />
    <id>tag:www.perezmedia.net,2004:/beltofvenus//5.325</id>

    <published>2010-01-23T04:32:00Z</published>
    <updated>2010-01-23T05:28:09Z</updated>

    <summary>M042</summary>
    <author>
        <name>Jeremy Perez</name>
        <uri>http://beltofvenus.perezmedia.net</uri>
    </author>
    
        <category term="Deep Sky" scheme="http://www.sixapart.com/ns/types#category" />
    
        <category term="Diffuse Nebula" scheme="http://www.sixapart.com/ns/types#category" />
    
        <category term="Messier" scheme="http://www.sixapart.com/ns/types#category" />
    
        <category term="SG-Deep Sky" scheme="http://www.sixapart.com/ns/types#category" />
    
        <category term="SG-Emission Nebula" scheme="http://www.sixapart.com/ns/types#category" />
    
        <category term="SG-Messier" scheme="http://www.sixapart.com/ns/types#category" />
    
        <category term="SG-Nebula" scheme="http://www.sixapart.com/ns/types#category" />
    
        <category term="SGC-Orion" scheme="http://www.sixapart.com/ns/types#category" />
    
        <category term="Sketch Gallery" scheme="http://www.sixapart.com/ns/types#category" />
    
    
    <content type="html" xml:lang="en" xml:base="http://www.perezmedia.net/beltofvenus/">
        <![CDATA[<div class="imageblock"><a href="images/2010/img2010011401_M42lg.jpg" target=_blank"><img src="images/2010/img2010011401_M42.jpg" alt="Sketch of Messier 42 and Messier 43 (M42/M43 Orion Nebula)"></a><p class="caption">Sketch of Messier 42 and Messier 43 (Orion Nebula)</p><p><i>Click image for larger version.</i></p></div>

<p><b>Observation Notes:</b></p>

<p>In my ongoing effort to refine my observation and sketches of M42/43, I made a new sketch on January 14. I used most of the previously sketched star field as a starting point so I could spend more time on the nebula. Working within a larger 6 inch circle really helped. The minty green color was striking throughout the nebula, particularly around the trapezium. As for structure, the sketch pretty much tells the story, except for the fact that there was a lot more detail to be squeezed out. I can tell that I'll be coming back again and again for more.</p>

<p><b>Object Information:</b></p>
<p>The Orion Nebula lies 1500 to 1600 light years away and is the brightest diffuse nebula in the sky. It is the brightest portion of a much larger cloud of gas and dust which extends over an area of 10 degrees. This cloud also contains Barnard's Loop, the Horsehead Nebula and the reflection nebula around M78. The brilliant M42 extends to a diameter of 30 light years. </p>

<p>The incredible complexity of the nebula is so great that various aspects of it have been given some creative names. Some of the more prominent are:
Fish's Mouth = the dark lane extending from the north into the brightest portion of the nebula<br />
Wings = the bright regions to both sides<br />
Trapezium cluster = the bright cluster of stars pointed to by the Fish's Mouth<br />
The Sword = the wing extension to the south on the east<br />
The Thrust = the bright nebulosity below the Trapezium<br />
The Sail = the fainter western extension</p>

<p>The Hubble Space Telescope discovered dark, protoplanetary discs called Proplyds around the region of the Trapezium. These investigations have shown that the blazing radiation of the Trapezium stars is eroding the Proplyds so that the lower-mass stars forming there may not maintain enough material to form planetary systems.</p>

<p>M42 was discovered by Nicholas-Claude Fabri de Peiresc in 1610, but it seems strange that its nebulosity was not discovered sooner, since it is easily visible to the naked eye. Charles Messier cataloged it in 1769.</p>

<p class="imageblock"><img src="images/2010/img2010011401_M42dss.jpg"></p>

<table class="objectdata">
<tr><td><b>Subject</b></td><td class="subject">M42 (NGC 1976) / M43 (1982)</td></tr>
<tr><td><b>Classification</b></td><td>Diffuse Nebulae</td></tr>
<tr><td><b>Position</b></td><td>Orion: M42: [RA: 05 35 17.2 / Dec: -05 23 27]*<br />M43: [05 35 31.3 / Dec.: -05 16 03]</td></tr>
<tr><td><b>Size*</b></td><td>M42: 90' x 60' / M43: 20' x 15'</td></tr>
<tr><td><b>Brightness*</b></td><td>M42: 4.0 bMag / M43: 9.0 bMag</td></tr>
<tr><td><b>Date/Time</b></td><td>January 14, 2010 - 10:00 AM <br />(January 15, 2010 05:00 UT)</td></tr>
<tr><td><b>Observing Loc.</b></td><td>Cinder Hills Overlook, Sunset Crater National Monument, AZ</td></tr>
<tr><td><b>Instrument</b></td><td>Orion SkyQuest XT8 Dobsonian (203 mm dia./1200 mm F/L)</td></tr>
<tr><td><b>Eyepieces/Mag.</b></td><td>32 mm (37.5X)</td></tr>
<tr><td><b>Seeing</b></td><td>5/10 Pickering</td></tr>
<tr><td><b>Transparency</b></td><td>Mag 7+ NELM</td></tr>
<tr><td><b>*Sources</b></td><td><a href="http://archive.stsci.edu/dss/acknowledging.html" target="_blank">DSS</a>; <a href="http://www.ngcicproject.org">NGCIC Project</a>; <a href="http://www.seds.org/messier/M/m042.html" target="_blank">SEDS</a></td></tr>
</table>
<p>*Based on published data.</p>

<hr />

<b>October 22, 2006 Observation:</b>

<p class="imageblock"><a href="images/2006/img2006102201_M42rev1lg.jpg" target=_blank"><img src="images/2006/img2006102201_M42rev1.jpg" border="1" color="ffffff"></a><br /><i>Click image for larger version.</i></p>

<p><b>Observation Notes:</b></p>
<p>I've been looking forward to making another low-power sketch of this beauty. It continues to amaze me that the patch around the trapezium is so boxy. There is a break on the west edge of this patch, which brightens again on the other side. The northwest side of the larger extent of the nebula is the brightest. The southern wing has a nice sharp edge with a hook that points inward. After fading out to the southwest, there is some patchy brightening that subtly picks up again. I noted a minty green color that was strongest in the trapezium box, but extended subtly through the other bright portions of the nebula.</p>

<p>After having some trouble with the regular sketch paper I used on 2006/M4 (SWAN) earlier in the evening, I used a nice, sturdy sheet of smooth bristol for this sketch. It worked very nicely and took multiple layers of graphite without resistance. I did feel that my standard 3" sketch circle is not big enough for the amount of fine detail available in this object. I may need to consider a 5" circle for some objects in the future. The sketch took an hour and a half to complete and contains 103 stars.</p>

<table class="objectdata">
<tr><td><b>Date/Time</b></td><td>October 22, 2006 - 12:30 AM <br />(October 22, 07:30 UT)</td></tr>
<tr><td><b>Observing Loc.</b></td><td>Cinder Hills Overlook, Sunset Crater National Monument, AZ</td></tr>
<tr><td><b>Instrument</b></td><td>Orion SVP 6LT Reflector (150 mm dia./1200 mm F/L)</td></tr>
<tr><td><b>Eyepieces/Mag.</b></td><td>32 mm (37.5X)</td></tr>
<tr><td><b>Seeing</b></td><td>5/10 Pickering</td></tr>
<tr><td><b>Transparency</b></td><td>Mag 6.8 NELM</td></tr>
</table>

<hr>

<b>December 12, 2004 Observation</b>

<p class="imageblock"><img src="images/2004/img20041212_01_M42_37xc.jpg"><br /><br />

<img src="images/2004/img20041212_02_M42_120xc.jpg" border="1" color="ffffff"><br /></p>

<p><b>Observation Notes:</b></p>
<p style="text-align: center"><img src="images/2004/img20041212_03_M42_Finder.jpg" border="1" color="ffffff" align="right" HSPACE=8>Boy, I was fighting fogged eyepieces on this one. For this first sketch of M42, I decided to go without the Ultrablock filter. It still looked great. One common comparison is that it looks like a bird, but the way the 'wings' of the nebula are swept back reminded me more of: A) a Shadow Vessel from Babylon-5, B) a face hugger from Alien, C) a brine shrimp. Heh. Man that's not flattering for such a beautiful nebula. It was bright, and minty green in the lightest area.</p>

<p>When I viewed it yesterday in Bill's 18" dobsonian, it was a great aqua green with a sliver of salmon pink along the linear south edge of the trapezium pocket. It was so detailed, it looked like a dark storm cloud lit from within by a great bolt of lightning--setting its innards on fire in brilliant, ominous 3-D.</p>

<p>Back to my scope...the notch that flowed toward the trapezium from the east looked like a mitten reaching into a bright pocket to snatch the brilliant stars within. The larger, more diffuse interior of the nebula seemed brightest along the northern region. The outer boundary of the 'wings' on the eastern edge was gilded brighter than the rest of the inside...except for the trapezium pocket which is the brightest. I could just make out the E and F stars at 120X. The F star was very tightly bound to its bright companion. M43 punctuated the northeast section of the view with its comma outline.</p>

<p>M42 is also catalogued as LBN 974, Sh2-281, h 360, and GC 1179. M43 is also catalogued as H III-1, GC 1185, CED 55G.</p>

<table class="objectdata">
<tr><td><b>Date/Time</b></td><td>December 12, 2004 - 1:00 AM<br />December 12, 2004 - 08:00 UT</td></tr>
<tr><td><b>Observing Loc.</b></td><td>Flagstaff, AZ - Home</td></tr>
<tr><td><b>Instrument</b></td><td>Orion SVP 6LT Reflector (150 mm dia./1200 mm F/L)</td></tr>
<tr><td><b>Eyepieces/Mag.</b></td><td>32 mm (37.5X); 10 mm (120X)</td></tr>
<tr><td><b>Seeing</b></td><td>5/10 Pickering</td></tr>
<tr><td><b>Transparency</b></td><td>Mag 5.8 NELM</td></tr>
</table>
<p>*Based on published data.</p>]]>
        
    </content>
</entry>

<entry>
    <title>NGC 2244 and Sh 2-275 - The Rosette Nebula</title>
    <link rel="alternate" type="text/html" href="http://www.perezmedia.net/beltofvenus/archives/000541.html" />
    <id>tag:www.perezmedia.net,2006:/beltofvenus//5.541</id>

    <published>2010-01-17T05:28:00Z</published>
    <updated>2010-01-17T08:01:12Z</updated>

    <summary>NGC 2244 and Sh 2-275</summary>
    <author>
        <name>Jeremy Perez</name>
        <uri>http://beltofvenus.perezmedia.net</uri>
    </author>
    
        <category term="Deep Sky" scheme="http://www.sixapart.com/ns/types#category" />
    
        <category term="Diffuse Nebula" scheme="http://www.sixapart.com/ns/types#category" />
    
        <category term="Open Cluster" scheme="http://www.sixapart.com/ns/types#category" />
    
        <category term="SG-Deep Sky" scheme="http://www.sixapart.com/ns/types#category" />
    
        <category term="SG-Emission Nebula" scheme="http://www.sixapart.com/ns/types#category" />
    
        <category term="SG-Nebula" scheme="http://www.sixapart.com/ns/types#category" />
    
        <category term="SG-Open Cluster" scheme="http://www.sixapart.com/ns/types#category" />
    
        <category term="SG-Star Cluster" scheme="http://www.sixapart.com/ns/types#category" />
    
        <category term="SGC-Monoceros" scheme="http://www.sixapart.com/ns/types#category" />
    
        <category term="Sketch Gallery" scheme="http://www.sixapart.com/ns/types#category" />
    
    
    <content type="html" xml:lang="en" xml:base="http://www.perezmedia.net/beltofvenus/">
        <![CDATA[<div class="imageblock"><a href="images/2010/img2010011501_RosetteNeblg.jpg" target="_blank"><img src="images/2010/img2010011501_RosetteNeb.jpg" alt="Sketch of NGC 2244 (NGC 2239) and Sh 2-275 (The Rosette Nebula)"></a><p class="caption">Sketch of NGC 2244 (NGC 2239) and Sh 2-275 (Rosette Nebula)</p><p><i>Click image to view larger version.</i></p></div> 

<p><b>Observation Notes:</b></p>
<p>If you find yourself at a dark site with Orion and Monoceros sprawled across the meridian, don't pass up this gorgeous showpiece of the winter sky. While at Sunset Crater National Monument, working on a set of observing/sketching projects, I spent an hour re-observing the nebulosity surrounding the cluster. I used a tracing of my previously sketched star field as a starting point to save time.</p>

<p>As before, the nebulosity was visible unfiltered, but adding the Ultrablock filter helped immensely. The central hollow was bordered by a rather straight run of nebulosity to the north. The western edge of the hollow peeled away along the northwest edge, forming a beak-like appendage. The nebula seemed to curl away on the southwestern side, allowing an opening to form on the south edge of the central void. Two nested arcs of nebulosity wrapped the east side to complete the shroud. Further out on the north east edge of the field, some more smoky structure emerged. That striking yellow-orange star still popped out along the southeast edge of the central rim.</p>

<p>To allow better control over the shading, I prepared this sketch in a large, 6 inch (15 cm) circle. I used an artist's chamois loaded with graphite to softly rough in the broad swaths of nebulosity. I then followed up with a graphite-loaded blending stump to build up the details and variations in luminosity.</p>

<p><b>Object Information:</b></p>
<p>The common designation NGC 2244 refers to the cluster of stars at the center of this stellar nursery. The nebulous region is described by the designations NGC 2237, 2238 and 2246. This nebula and star cluster is more than 1 degree across. Star formation is still in progress. This object lies about 5,500 light years away, and is about 130 light years in diameter. The open cluster (NGC 2244) was discovered in 1690 by Flamsteed. The nebulous regions were later discovered by John Herschel, Marth, and Swift.</p> 

<div class="imageblock"><img src="images/2010/img2010011501_RosetteNebdss.jpg" alt="Sketch/DSS photo comparison of NGC 2244 (NGC 2239) and Sh 2-275 (The Rosette Nebula)"></a><p class="caption">Sketch/DSS Photo Comparison of NGC 2244 (NGC 2239)<br />and Sh 2-275 (The Rosette Nebula)</p></div> 

<p><table class="objectdata">
<tr><td><b>Subject</b></td><td class="subject">Nebula: Sh 2-275 (The Rosette Nebula) <br />-- Includes NGC 2237, 2238, 2246<br />Open Cluster: NGC 2244 (NGC 2239)</td></tr>
<tr><td><b>Other Desig.</b></td><td><b>NGC 2244:</b> NGC 2239, Lund 222, h 392, GC 1420, OCL 515, Cr 99, Mel 47, CED 76B<br /><b>Sh 2-275:</b> NGC 2246, NGC 2237, NGC 2238, LBN 948, LBN 949, Sh2-274, GC 5361, CED 76A, </td></tr>
<tr><td><b>Classification*</b></td><td>Open Cluster (III 2 m n) and Emission Nebula</td></tr>
<tr><td><b>Position*</b></td><td>Monoceros [RA: 06:31:55.6 / Dec: +04:56:35]</td></tr>
<tr><td><b>Size*</b></td><td>NGC 2244: 24'<br />Sh 2-275: 80' x 60'</td></tr>
<tr><td><b>Brightness*</b></td><td>NGC 2244: 4.8 bMag<br />Sh 2-275: 6.0 bMag</td></tr>
<tr><td><b>Date/Time</b></td><td>January 15, 2010 - 12:00 AM MST<br>(January 15, 2010 - 07:00 UT)</td></tr>
<tr><td><b>Observing Loc.</b></td><td>Cinder Hills Overlook, Sunset Crater National Monument, Arizona</td></tr>
<tr><td><b>Instrument</b></td><td>Orion SkyQuest XT8 Dobsonian (203 mm dia./1200 mm F/L)</td></tr>
<tr><td><b>Eyepieces/Mag.</b></td><td>32 mm Sirius Plossl (37.5X / 88' TFOV)</td></tr>
<tr><td><b>Conditions</b></td><td>Clear, cold, breezy</td></tr>
<tr><td><b>Seeing</b></td><td>5/10</td></tr>
<tr><td><b>Transparency</b></td><td>Mag 7+</td></tr>
<tr><td><b>*Sources</b></td><td><a href="http://www.ngcicproject.org" target="_blank">NGC/IC Project</a><br /><a href="http://www.seds.org/messier/xtra/ngc/n2244.html" target="_blank">SEDS<td></tr>
</table></p>

<hr />
<p><b>February 24, 2006 Observation:</b></p>

<div class="imageblock"><A HREF="javascript:myVoid()" onMouseOver="rollover('img2006022402A')" onMouseOut="rollout('img2006022402A')"><IMG SRC="http://www.perezmedia.net/beltofvenus/archives/images/2006/img2006022402_NGC2244A.jpg" NAME="img2006022402A" ALT="Step 1" BORDER=1 COLOR=FFFFFF></A>
<SCRIPT TYPE="text/javascript">
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<br />
<i>Move mouse over image for labels.</i></div>

<p><b>Observation Notes:</b></p>
<p><img src="http://www.perezmedia.net/beltofvenus/archives/images/2006/img2006022402_NGC2244finder.jpg" border="1" color="ffffff" align="right">This is really an incredible nebula from a dark site. While the nebulosity is only hinted at without a a filter, once the Ultrablock filter is inserted, its beautiful form really takes shape. The central region is home to a bright, but sparse open cluster and is mainly clear of nebulosity, with softly glowing petals of light encircling it. The brightest portion of the nebula appeared to be north of the core, and the western quadrant appeared to be lacking in stars. A bright yellow star sparkled just east-southeast of center as shown in the sketch.</p> 

<p><table class="objectdata">
<tr><td><b>Date/Time</b></td><td>February 24, 2006 - 11:30 PM MST<br>(February 25, 2006 - 06:30 UT)</td></tr>
<tr><td><b>Observing Loc.</b></td><td>Anderson Mesa, AZ</td></tr>
<tr><td><b>Instrument</b></td><td>Orion SVP 6LT Reflector (150 mm dia./1200 mm F/L)</td></tr>
<tr><td><b>Eyepieces/Mag.</b></td><td>32 mm (37.5X)</td></tr>
<tr><td><b>Conditions</b></td><td>Clear, calm, 21Â°F</td></tr>
<tr><td><b>Seeing</b></td><td>3-4/10</td></tr>
<tr><td><b>Transparency</b></td><td>Mag 6.8</td></tr>
</table></p>]]>
        
    </content>
</entry>

<entry>
    <title>NGC 2169 and Struve 848</title>
    <link rel="alternate" type="text/html" href="http://www.perezmedia.net/beltofvenus/archives/001402.html" />
    <id>tag:www.perezmedia.net,2010:/beltofvenus//5.1402</id>

    <published>2010-01-10T23:15:12Z</published>
    <updated>2010-01-11T01:29:21Z</updated>

    <summary>NGC 2169</summary>
    <author>
        <name>Jeremy Perez</name>
        <uri>http://beltofvenus.perezmedia.net</uri>
    </author>
    
        <category term="Deep Sky" scheme="http://www.sixapart.com/ns/types#category" />
    
        <category term="Double Star" scheme="http://www.sixapart.com/ns/types#category" />
    
        <category term="Open Cluster" scheme="http://www.sixapart.com/ns/types#category" />
    
        <category term="SG-Deep Sky" scheme="http://www.sixapart.com/ns/types#category" />
    
        <category term="SG-Double Star" scheme="http://www.sixapart.com/ns/types#category" />
    
        <category term="SG-Open Cluster" scheme="http://www.sixapart.com/ns/types#category" />
    
        <category term="SG-Star Cluster" scheme="http://www.sixapart.com/ns/types#category" />
    
        <category term="SGC-Orion" scheme="http://www.sixapart.com/ns/types#category" />
    
    
    <content type="html" xml:lang="en" xml:base="http://www.perezmedia.net/beltofvenus/">
        <![CDATA[<div class="imageblock"><A HREF="images/2009/img2009010201_NGC2169lg.jpg" onMouseOver="rollover('img2009010201')" onMouseOut="rollout('img2009010201')"><IMG SRC="images/2009/img2009010201_NGC2169A.jpg" NAME="img2009010201" ALT="Sketch of NGC 2169 (37 Cluster) and Struve 848 (STF 848)"></A>
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<p class="caption">Sketch of NGC 2169 (The 37 Cluster) and Struve 848</p>
<p><i>Move mouse over image to view label.<br />Click for larger version.</i></p></div>

<p><b>Observation Notes</b></p>
<p>So many old sketches, so little time--this one is over a year old.</p>
<p>NGC 2169 really did look like an upside-down, angular #37. I plotted 19 stars in the immediate vicinity of the cluster, which appeared to be about 4 x 5 arc minutes in size. One golden-yellow star glimmered in the number 7 on the northwest side of the cluster.</p>
<p>Several doubles marked the field, but one in particular drew me in. The brightest star in the cluster, on the northern corner of the number 3 appeared elongated at 120X. I inserted the 2X barlow and found that it was indeed a close double. The primary appeared white with a dull blue secondary. I broke out the astrometric eyepiece and measured a PA of 112 degrees and estimated a separation of 1.5 arc seconds based on the diffraction pattern.</p>
<p>After coming inside, I headed over to <a href="http://vizier.u-strasbg.fr/viz-bin/VizieR" target="_blank">Vizier</a> and found the identity of the double as Struve 848. The star positions I sketched in the cluster could use some help, as seen in the DSS comparison below. Perhaps another time!</p>

<div class="imageblock"><img src="images/2009/img2009010201_NGC2169dss.jpg" alt="Sketch/DSS Photo Comparison of NGC 2169 (37 Cluster)"><p class="caption">Sketch/DSS Photo Comparison of NGC 2169 (The 37 Cluster)</p></div>

<table class="objectdata">
<tr><td><b>Subject</b></td><td class="subject">NGC 2169 (37 Cluster)</td></tr>
<tr><td><b>Classification</b></td><td>Open Cluster (III 3 m)</td></tr>
<tr><td><b>AKA*</b></td><td>Cr 83, OCL 481, Lund 206, H VIII-24, h 379, GC 1361</td></tr>
<tr><td><b>Position*</b></td><td>Orion: [RA: 06 08 24.3 / Dec. +13 57 53]</td></tr>
<tr><td><b>Size*</b></td><td>6'</td></tr>
<tr><td><b>Magnitude*</b></td><td>vMag 5.9</td></tr>
</table>

<table class="objectdata">
<tr><td><b>Subject</b></td><td class="subject">Struve 848 (STF 848 / ADS 4728)</td></tr>
<tr><td><b>Classification</b></td><td>Multiple Star</td></tr>
<tr><td><b>Position (J2000)*</b></td><td>Orion [RA: 06 08 30.3 / Dec: +13 58 16]</td></tr>
<tr><td><b>Position Angle</b></td><td>AB: 112&deg; [My Measurement 2009.0]<br />AB: 108&deg; [CCDM 1951]*<br />AC: 291&deg; [CCDM 1985]*<br />AD: 125&deg; [CCDM 1985]*</td></tr>
<tr><td><b>Separation</b></td><td>AB: 1.5" [My Measurement 2009.0]<br />AB: 2.5" [CCDM 1951]*<br />AC: 17.3" [CCDM 1985]*<br />AD: 27.5" [CCDM 1985]*</td></tr>
<tr><td><b>Magnitudes*</b></td><td>A: 7.3; B: 8.2</td></tr>
<tr><td><b>Spectral Types*</b></td><td>A: B1V; B: B2V</td></tr>
</table>

<table class="objectdata">
<tr><td><b>Date/Time</b></td><td>JAN 2, 2009 - 12:15 AM (JAN 2, 2009 - 07:15 UT)</td></tr>
<tr><td><b>Observing Loc.</b></td><td>Flagstaff, Arizona - Home</td></tr>
<tr><td><b>Instrument</b></td><td>Orion SkyQuest XT8 Dobsonian (203 mm dia./1200 mm F/L)</td></tr>
<tr><td><b>Eyepieces/Mag.</b></td><td>Pentax XW10 (120X)<br />Pentax XW10 + 2X Barlow (240X)<br />Meade Astrometric EP + 2X Barlow (200X)</td></tr>
<tr><td><b>Conditions</b></td><td>Clear, cold, calm</td></tr>
<tr><td><b>Seeing</b></td><td>6/10 Pickering</td></tr>
<tr><td><b>Transparency</b></td><td>Mag 5.8 NELM</td></tr>
<tr><td><b>*Sources</b></td><td><a href="http://www.ngcicproject.org" target="_blank">NGCIC Project</a>; <a href="http://archive.stsci.edu/dss/acknowledging.html" target="_blank">DSS</a>; The Washington Visual Double Star Catalog (Mason+ 2001-2010); Catalogue of Stellar Spectral Classifications (Skiff, 2009); SIMBAD<td></tr>
</table>]]>
        
    </content>
</entry>

<entry>
    <title>Mars - CM 265 Deg.DEC 14, 2009 - 11:30 UT</title>
    <link rel="alternate" type="text/html" href="http://www.perezmedia.net/beltofvenus/archives/001401.html" />
    <id>tag:www.perezmedia.net,2009:/beltofvenus//5.1401</id>

    <published>2009-12-28T05:35:17Z</published>
    <updated>2009-12-28T06:14:45Z</updated>

    <summary>Mars 2009121401</summary>
    <author>
        <name>Jeremy Perez</name>
        <uri>http://beltofvenus.perezmedia.net</uri>
    </author>
    
        <category term="Planetary" scheme="http://www.sixapart.com/ns/types#category" />
    
        <category term="SG-Mars" scheme="http://www.sixapart.com/ns/types#category" />
    
        <category term="SG-Planetary" scheme="http://www.sixapart.com/ns/types#category" />
    
        <category term="Sketch Gallery" scheme="http://www.sixapart.com/ns/types#category" />
    
    
    <content type="html" xml:lang="en" xml:base="http://www.perezmedia.net/beltofvenus/">
        <![CDATA[<div class="imageblock"><A HREF="images/2009/img2009121401_MarsUFlg.jpg" onMouseOver="rollover('img2009121401')" onMouseOut="rollout('img2009121401')"><IMG SRC="images/2009/img2009121401_MarsUFA.jpg" NAME="img2009121401" ALT="Sketch of Mars - CM 265 Degrees - DEC 14, 2009 - 11:30 UT"></A>
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<p class="caption">Sketch of Mars - CM 265&deg; - Unfiltered<br />DEC 14, 2009 - 11:30 UT</p><p><i>Move mouse over image to view labels. Click to view larger version.</i></p><br /></div>

<div class="imageblock"><p><img src="images/2009/img2009121401_MarsW80A.jpg"></p>
<p class="caption">Sketch of Mars - CM 265&deg; - Filter: Wratten #80A<br />DEC 14, 2009 - 11:30 UT</p></div>

<p><b>Observation Notes:</b></p>
<p>It has been a long time since my last Mars observation (<a href="http://www.perezmedia.net/beltofvenus/archives/000583.html">DEC 21, 2005</a>). At 11 arc seconds under soft seeing, details took some time to discern. The north polar cap was large and prominent and Syrtis Major was well placed on the following hemisphere. Hellas was bright, as was Arabia. I didn't detect any limb haze in the unfiltered view. The Wratten #80A did show some brighter spots as noted in the sketch above. I'm looking forward to some more good views of Mars as it approaches a maximum size of 14 arc seconds later in January.</p>

<table class="objectdata">
<tr><td><b>Subject</b></td><td class="subject">Mars - CM 265&deg;</td></tr>
<tr><td><b>Classification</b></td><td>Planet</td></tr>
<tr><td><b>Position*</b></td><td>Leo [RA: 09 30 53.3 / Dec: +17 53 39]</td></tr>
<tr><td><b>Angular Size*</b></td><td>11 arcseconds</td></tr>
<tr><td><b>Brightness*</b></td><td>-0.4</td></tr>
<tr><td><b>Date/Time</b></td><td>DEC 14, 2009, 04:30 AM MST<br>(DEC 14, 2009, 11:30 UT)</td></tr>
<tr><td><b>Observing Loc.</b></td><td>Flagstaff, Arizona, USA - Home</td></tr>
<tr><td><b>Instrument</b></td><td>Orion SkyQuest XT8 Dobsonian (203 mm dia./1200 mm F/L)</td></tr>
<tr><td><b>Eyepieces/Mag.</b></td><td>4 mm UO Orthoscopic (300X)</td></tr>
<tr><td><b>Conditions</b></td><td>P. Cloudy, cold</td></tr>
<tr><td><b>Seeing</b></td><td>Ant. III</td></tr>
<tr><td><b>Transparency</b></td><td>Mag 5.2 NELM</td></tr>
<tr><td><b>*Sources</b></td><td>Starry Night Pro Plus 5.8.2<br /><a href="http://www.britastro.org/mars/maps.htm" target="_blank">British Astronomical Society Mars Maps</a></td></tr>
</table>]]>
        
    </content>
</entry>

<entry>
    <title>Jupiter - Neptune Conjunction - DEC 24, 2009</title>
    <link rel="alternate" type="text/html" href="http://www.perezmedia.net/beltofvenus/archives/001400.html" />
    <id>tag:www.perezmedia.net,2009:/beltofvenus//5.1400</id>

    <published>2009-12-25T07:29:31Z</published>
    <updated>2009-12-25T08:16:47Z</updated>

    <summary>Jupiter-Neptune Conjunction</summary>
    <author>
        <name>Jeremy Perez</name>
        <uri>http://beltofvenus.perezmedia.net</uri>
    </author>
    
        <category term="Planetary" scheme="http://www.sixapart.com/ns/types#category" />
    
        <category term="SG-Jupiter" scheme="http://www.sixapart.com/ns/types#category" />
    
        <category term="SG-Neptune" scheme="http://www.sixapart.com/ns/types#category" />
    
        <category term="SG-Planetary" scheme="http://www.sixapart.com/ns/types#category" />
    
    
    <content type="html" xml:lang="en" xml:base="http://www.perezmedia.net/beltofvenus/">
        <![CDATA[<div class="imageblock">
<A HREF="images/2009/img2009122401_JupiterNeptunelg.jpg" onMouseOver="rollover('img2009122401')" onMouseOut="rollout('img2009122401')"><IMG SRC="images/2009/img2009122401_JupiterNeptuneA.jpg" NAME="img2009122401" ALT="Digital Illustration: Jupiter-Neptune Conjunction" BORDER=1 COLOR=FFFFFF></A>
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<p class="caption">Digital Illustration: Jupiter-Neptune Conjunction</p>
<p class="subcaption">Move mouse over sketch above to view labels.<br />Click for larger version.</p>
</div>

<p><b>Observation Notes:</b></p>

<p>Jupiter and Neptune have spent the last several days passing within a degree of each other. I finally got out to observe the pair tonight when they were separated by about 48 arc minutes. Through the 32 mm eyepiece, Jupiter and its moons were dazzling of course. In comparison, Neptune was seriously outclassed. I hadn't brought a chart with me, and I was worried at first that I might confuse it with one of several nearby 8th magnitude stars. But giving my eye a few seconds to just let things register allowed me to see the blue green color and know that was it. Examining it at 120X with the Pentax XW10 made the color appear richer and brought out the slightly soft, non-stellar appearance of its 2 arc second disc.</p>
<p>Although Neptune's faint presentation kept it from being a spectacular conjunction, the view <b>was</b> colorful. Neptune's blue-green met the bright cream color of Jupiter, the yellow of Ganymede, and the yellow-orange of Io. Realizing that Neptune is nearly five times further away than Jupiter, but both were sharing the same space in the sky made for an enjoyable observation.</p>
<p>I made a graphite sketch at the eyepiece, detailing color, equatorial cloud belts, flaring and diffraction spikes around Jupiter. I scanned the drawing and used Photoshop to clean up the stars, Neptune, and Jupiter's moons. Jupiter is redrawn completely and flare/diffraction spikes added using digital tools. I had a little trouble deciding the best way to present the view, so I've included two images. The second one below zooms in a little closer, and clicking for the large version may show details a little better.</p>
<p>The pair is widening now, and in a couple days they will be more than a degree apart. So be sure to get a look right away if you want to see them in the same telescopic field of view.</p>
<div class="imageblock">
<a href="images/2009/img2009122401A_JupiterNeptunelg.jpg"><img src="images/2009/img2009122401A_JupiterNeptune.jpg" ALT="Digital Illustration: Jupiter-Neptune Conjunction"></a>
<p class="caption">Digital Illustration: Jupiter-Neptune Conjunction</p>
<p class="subcaption">Click for larger version.</p>
</div>

<p><table class="objectdata">
<tr><td><b>Subject</b></td><td class="subject">Jupiter-Neptune Conjuction</td></tr>
<tr><td><b>Classification</b></td><td>Planet</td></tr>
<tr><td><b>Position*</b></td><td>Jupiter: Capricornus [RA: 21 49 50.6 / Dec: -14 07 30]<br />Neptune: Capricornus [RA: 21 46 47.2 / Dec: -13 49 58]</td></tr>
<tr><td><b>Angular Size*</b></td><td>Jupiter: 35"<br />Neptune: 2.2"</td></tr>
<tr><td><b>Brightness*</b></td><td>Jupiter: -2.1<br / >Neptune: 7.9</td></tr>
<tr><td><b>Date/Time</b></td><td>DEC 24, 2009 - 6:25 PM <br>(DEC 25, 2009 - 01:25 UT)</td></tr>
<tr><td><b>Observing Loc.</b></td><td>Flagstaff, Arizona, USA - Home</td></tr>
<tr><td><b>Instrument</b></td><td>Orion SkyQuest XT8 Dobsonian (203 mm dia./1200 mm F/L)</td></tr>
<tr><td><b>Eyepieces/Mag.</b></td><td>32 mm Sirius Pl&ouml;ssl (37.5 X)</td></tr>
<tr><td><b>Conditions</b></td><td>Clear, cold</td></tr>
<tr><td><b>Seeing</b></td><td>4/10</td></tr>
<tr><td><b>Transparency</b></td><td>Twilight - Mag 4 NELM</td></tr>
<tr><td><b>*Sources</b></td><td>Starry Night Pro Plus 5.8</td></tr>
</table></p>]]>
        
    </content>
</entry>

<entry>
    <title>Drawn to the UniverseJAN 2010 - The Winter Milky Way</title>
    <link rel="alternate" type="text/html" href="http://www.perezmedia.net/beltofvenus/archives/001398.html" />
    <id>tag:www.perezmedia.net,2009:/beltofvenus//5.1398</id>

    <published>2009-12-19T01:12:57Z</published>
    <updated>2009-12-19T01:23:54Z</updated>

    <summary>The winter Milky Way is moving into view. Although it&apos;s not as bold as its summer counterpart, it still has much to offer the naked eye from a dark site. In the January issue of Astronomy Now, we&apos;ll look at...</summary>
    <author>
        <name>Jeremy Perez</name>
        <uri>http://beltofvenus.perezmedia.net</uri>
    </author>
    
        <category term="Article" scheme="http://www.sixapart.com/ns/types#category" />
    
    
    <content type="html" xml:lang="en" xml:base="http://www.perezmedia.net/beltofvenus/">
        <![CDATA[<p>The winter Milky Way is moving into view. Although it's not as bold as its summer counterpart, it still has much to offer the naked eye from a dark site. In the January issue of <i>Astronomy Now</i>,  we'll look at some methods you can use to capture the Milky Way on paper.</p>

<table class="objectdata" style="margin-bottom: 15px;"> 
<tr><td><b>Subject:</b></td><td class="subject">Winter Milky Way</td></tr> 
<tr><td><b>Issue:</b></td><td><a href="http://www.astronomynowstore.com/ww/catalog/product_info.php?products_id=322" target="_blank">January 2010</a> <i>Astronomy Now</i></td></tr>
<tr><td><b>Basic Media:</b></td><td>Graphite on artist grade paper.</td></tr> 
<tr><td><b>Featured Technique:</b></td><td>Naked eye sketching beginning with plotting the stars across a broad stretch of sky, then observing and shading structure in the Milky Way.</td></tr>
<tr><td><b>Suggested Materials:</b></td><td>
<ul>
<li>White artist grade stock</li>
<li>HB and 2H graphite pencils</li>
<li>Blending stump and artist's chamois</li>
<li>Kneaded eraser (putty rubber)</li>
<li>Clipboard and adjustable red light</li>
</ul>
</td></tr>
</table>

<div class="imageblock"><a href="images/2010/img201001AN_WinterMWposlg.jpg" target="_blank"><img src="images/2010/img201001AN_WinterMWpos.jpg" alt="Positive sketch of the Winter Milky Way"></a><p class="caption">Inverted, Positive Sketch of the Winter Milky Way</p><p><i>Click image to view larger version.</i></p></div>

<div class="imageblock"><a href="images/2010/img201001AN_WinterMWneglg.jpg" target="_blank"><img src="images/2010/img201001AN_WinterMWneg.jpg" alt="Negative sketch of the Winter Milky Way"></a><p class="caption">Original, Negative Sketch of the Winter Milky Way</p><p><i>Click image to view larger version.</i></p></div>]]>
        
    </content>
</entry>

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