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	<title>Comets &#8211; PekDar – Astrophotography Engineering</title>
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	<link>https://astrophotography.pekdar.net</link>
	<description>Autorskie rozwiązania Hardware, Projekty 3D i Zaawansowane Poradniki</description>
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	<title>Comets &#8211; PekDar – Astrophotography Engineering</title>
	<link>https://astrophotography.pekdar.net</link>
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		<title>SynScan: Manually Adding Comets and Custom Objects (User Object)</title>
		<link>https://astrophotography.pekdar.net/en/synscan-goto-manual-comet-input-user-object/</link>
		
		<dc:creator><![CDATA[PekDar]]></dc:creator>
		<pubDate>Tue, 28 Apr 2020 11:00:08 +0000</pubDate>
				<category><![CDATA[Equipment]]></category>
		<category><![CDATA[Software]]></category>
		<category><![CDATA[Comets]]></category>
		<category><![CDATA[Ephemerides]]></category>
		<category><![CDATA[J2000]]></category>
		<category><![CDATA[NEQ6]]></category>
		<category><![CDATA[SynScan]]></category>
		<category><![CDATA[User Object]]></category>
		<guid isPermaLink="false">https://astrophotography.pekdar.net/?p=3952</guid>

					<description><![CDATA[SynScan User Object &#8211; The Database is Not Enough The object database in SynScan hand controllers (used in Sky-Watcher NEQ6, HEQ5, EQ6-R mounts) contains thousands of entries from the Messier, NGC, and IC catalogs. However, it is helpless against dynamic objects: new comets, fast-moving asteroids, or supernovae. To point the telescope at such an object without using a computer (EQMOD), we must use the User Object function and manually input equatorial coordinates. Step 1: Obtaining Ephemerides (J2000) Before touching the controller, you must know the object&#8217;s current position. Comets move relative to the background stars. Yesterday&#8217;s coordinates might be useless today. Source: Use TheSkyLive or Minor Planet Center. Format: You need Right Ascension (RA) and Declination (Dec). Important: Ensure the coordinates are for the J2000.0 epoch (standard for SynScan), not &#8220;JNow&#8221; (Topocentric), although for wide fields the difference might be negligible, in astrophotography it matters. Step 2: Shortened SynScan Procedure Power up the mount and perform the standard alignment (1, 2, or 3-Star Alignment). In the main menu, select: Object List -&#62; User Object. Select New Object (or edit an existing one). Enter the coordinates: RA (Right Ascension): In HH:MM:SS format. Dec (Declination): In DD:MM:SS format. Remember to toggle the + / - sign depending on the celestial hemisphere. Confirm and select View Object -&#62; Slew. The mount will point to the defined position. Technical Limitation: Tracking By entering an object this way, the mount treats it like a fixed star. It will track it at the sidereal rate. However, comets have their own proper motion. During long exposures (over 60-120 seconds) or with comets very close to Earth, the comet&#8217;s nucleus might appear trailed on the image, even if the stars are pinpoint sharp. Solution: This is a &#8220;point-in-time&#8221; method. If the comet is fast, you must update the coordinates in the controller every 30-60 minutes using fresh ephemeris data.   NEQ6Pro GOTO – user object configuration step by step Now we need to add, a new user object on the GOTO system controller. Go to the Object List → User Objects → New Object menu and press Enter on the controller keyboard. The controller will display information asking for the type of coordinates. Enter Coordi .: 1) RA-Dec 2) AzAlt. We are interested in the first position 1) RA-Dec, press the 1 key on the controller. Using the available controller keyboard, enter the comet&#8217;s coordinates: 8h28.4m +68°28 After entering the coordinates, press the Enter key to confirm. The controller will ask whether to save the entered data, press Enter again Select the number under the object will to be saved, in this example it is the first item # 01 on the list of user objects. Press Enter to confirm your selection. After saving the data in the GOTO system, you can now set up the telescope mount on our comet C/2019 Y4 (ATLAS). Go to the controller menu and select Object List → User Objects → User vol. # 01 → Recall Object and confirm with Enter. The mount has positioned itself on the comet. Ready! A description of how to add a new object, to the Stellarium database can be found here.  ]]></description>
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									<h3>SynScan User Object &#8211; The Database is Not Enough</h3>
<div class="wp-block-image" style="text-align: left;">
<figure class="aligncenter size-large">The object database in SynScan hand controllers (used in Sky-Watcher NEQ6, HEQ5, EQ6-R mounts) contains thousands of entries from the Messier, NGC, and IC catalogs. However, it is helpless against dynamic objects: new comets, fast-moving asteroids, or supernovae. To point the telescope at such an object without using a computer (EQMOD), we must use the <b>User Object</b> function and manually input equatorial coordinates.</figure>
<h3>Step 1: Obtaining Ephemerides (J2000)</h3>
<p data-path-to-node="27">Before touching the controller, you must know the object&#8217;s current position. Comets move relative to the background stars. Yesterday&#8217;s coordinates might be useless today.</p>
<ul data-path-to-node="28">
<li>
<p data-path-to-node="28,0,0"><b>Source:</b> Use <i>TheSkyLive</i> or <i>Minor Planet Center</i>.</p>
</li>
<li>
<p data-path-to-node="28,1,0"><b>Format:</b> You need <b>Right Ascension (RA)</b> and <b>Declination (Dec)</b>.</p>
</li>
<li>
<p data-path-to-node="28,2,0"><b>Important:</b> Ensure the coordinates are for the <b>J2000.0</b> epoch (standard for SynScan), not &#8220;JNow&#8221; (Topocentric), although for wide fields the difference might be negligible, in astrophotography it matters.</p>
</li>
</ul>
<h3>Step 2: Shortened SynScan Procedure</h3>
<ul>
<li>
<p data-path-to-node="30,0,0">Power up the mount and perform the standard alignment (1, 2, or 3-Star Alignment).</p>
</li>
<li>
<p data-path-to-node="30,1,0">In the main menu, select: <code>Object List</code> -&gt; <code>User Object</code>.</p>
</li>
<li>
<p data-path-to-node="30,2,0">Select <code>New Object</code> (or edit an existing one).</p>
</li>
<li>
<p data-path-to-node="30,3,0">Enter the coordinates:</p>
<ul data-path-to-node="30,3,1">
<li>
<p data-path-to-node="30,3,1,0,0"><b>RA (Right Ascension):</b> In <code>HH:MM:SS</code> format.</p>
</li>
<li>
<p data-path-to-node="30,3,1,1,0"><b>Dec (Declination):</b> In <code>DD:MM:SS</code> format. Remember to toggle the <code>+</code> / <code>-</code> sign depending on the celestial hemisphere.</p>
</li>
</ul>
</li>
<li>
<p data-path-to-node="30,4,0">Confirm and select <code>View Object</code> -&gt; <code>Slew</code>. The mount will point to the defined position.</p>
</li>
</ul>
<h3>Technical Limitation: Tracking</h3>
<p data-path-to-node="31">By entering an object this way, the mount treats it like a fixed star. It will track it at the <b>sidereal</b> rate. However, comets have their own proper motion. During long exposures (over 60-120 seconds) or with comets very close to Earth, the comet&#8217;s nucleus might appear trailed on the image, even if the stars are pinpoint sharp.</p>
<ul data-path-to-node="32">
<li>
<p data-path-to-node="32,0,0"><b>Solution:</b> This is a &#8220;point-in-time&#8221; method. If the comet is fast, you must update the coordinates in the controller every 30-60 minutes using fresh ephemeris data.</p>
</li>
</ul>
</div>
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<p></p></div></div></div></div></div></section></div> <a href="https://astrophotography.pekdar.net/en/synscan-goto-manual-comet-input-user-object/#more-3952" class="more-link elementor-more-link"><span aria-label="Continue reading SynScan: Manually Adding Comets and Custom Objects (User Object)">read more</span></a>]]></content:encoded>
					
		
		
			</item>
		<item>
		<title>Stellarium: Adding New Comets and Asteroids</title>
		<link>https://astrophotography.pekdar.net/en/stellarium-adding-comets-asteroids/</link>
		
		<dc:creator><![CDATA[PekDar]]></dc:creator>
		<pubDate>Mon, 20 Apr 2020 11:51:51 +0000</pubDate>
				<category><![CDATA[Software]]></category>
		<category><![CDATA[Asteroids]]></category>
		<category><![CDATA[Astronomy]]></category>
		<category><![CDATA[Comets]]></category>
		<category><![CDATA[Minor Planet Center]]></category>
		<category><![CDATA[MPC]]></category>
		<category><![CDATA[Orbital elements]]></category>
		<category><![CDATA[Session Planning]]></category>
		<category><![CDATA[Solar System Editor]]></category>
		<category><![CDATA[Stellarium]]></category>
		<guid isPermaLink="false">http://www.astrofoto.pekdar.net/?p=1263</guid>

					<description><![CDATA[Stellarium &#8211; Beyond the Standard Catalog The Solar System database in Stellarium is updated regularly, but new comets appear faster than official data packages. To plan a photography session for an object that has &#8220;just arrived,&#8221; you must use the Solar System Editor plugin. The Mechanism: Orbital Elements (MPC) Stellarium does not store images of comets but rather their orbital elements (including perihelion, eccentricity, inclination). Based on these, the software engine calculates the object&#8217;s current position in the sky for your specific location. The most reliable source for this data is the Minor Planet Center (MPC). Shortened Step-by-Step Instructions Activate the Plugin: Go to &#8220;Configuration Window&#8221; [F2] -&#62; &#8220;Plugins&#8221; -&#62; &#8220;Solar System Editor&#8221;. Ensure &#8220;Load at startup&#8221; is checked and restart the program. Import Data: In the plugin settings, select the &#8220;Solar System&#8221; tab and click &#8220;Import orbital elements in MPC format&#8221;. Select Object Type: Choose &#8220;Comets&#8221; or &#8220;Asteroids.&#8221; Online Source: Select an MPC server from the list (e.g., MPC&#8217;s list of observable comets). The program will connect to the web and download the list. Search: Type the comet&#8217;s name (e.g., &#8220;C/2023 A3&#8221;). Once it appears, check it and click &#8220;Add objects&#8221;. Why is this better than manual entry? Manual entry of orbital elements is prone to formatting errors, leading to incorrect position calculations. Automatic import from the MPC ensures that parameters are up-to-date, which is crucial as comet orbits undergo subtle changes due to planetary gravity. Detailed guide You will need Stellarium version 0.18 minimum and internet access. Run Stellarium and go to Configuration Window (F2 key).   Click the Plugins tab. On the left from the list at the bottom, click on Solar System Editor and enable the Load at startup option. Close the window and restart Stellarium. Go to Configuration Window (F2) → Plugins → Solar System Editor and click the configure plugin button. Go to the Solar System tab and click Import orbital elements in MPC format … Click on the Lists tab, enable Comets. In the Select the source section, enable Download a list of objects from the Internet. Click on the drop-down list and select MPCORB: comets. Click on Get orbital elements. In the Import Data window, enter the searched comet in the text field, C/2019 Y4 (ATLAS). Select the object and click Add objects. Close all configuration windows. Go to object search and click the magnifying glass &#8211; Search window (F3)   In the search field, enter C/2019 Y4. The search engine will complete the rest of the entry itself. Click the magnifying glass.   The program will set the sky on comet its own. Done]]></description>
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<h3>Stellarium &#8211; Beyond the Standard Catalog</h3>
<p>The Solar System database in <a href="https://stellarium.org/" target="_blank" rel="noopener">Stellarium</a> is updated regularly, but new comets appear faster than official data packages. To plan a photography session for an object that has &#8220;just arrived,&#8221; you must use the <b>Solar System Editor</b> plugin.</p>
<h3>The Mechanism: Orbital Elements (MPC)</h3>
<p>Stellarium does not store images of comets but rather their orbital elements (including perihelion, eccentricity, inclination). Based on these, the software engine calculates the object&#8217;s current position in the sky for your specific location. The most reliable source for this data is the <b>Minor Planet Center (MPC)</b>.</p>
<h3>Shortened Step-by-Step Instructions</h3>
<ul>
<li>
<p data-path-to-node="25,0,0"><b>Activate the Plugin:</b> Go to &#8220;Configuration Window&#8221; [F2] -&gt; &#8220;Plugins&#8221; -&gt; <b>&#8220;Solar System Editor&#8221;</b>. Ensure &#8220;Load at startup&#8221; is checked and restart the program.</p>
</li>
<li>
<p data-path-to-node="25,1,0"><b>Import Data:</b> In the plugin settings, select the &#8220;Solar System&#8221; tab and click <b>&#8220;Import orbital elements in MPC format&#8221;</b>.</p>
</li>
<li>
<p data-path-to-node="25,2,0"><b>Select Object Type:</b> Choose &#8220;Comets&#8221; or &#8220;Asteroids.&#8221;</p>
</li>
<li>
<p data-path-to-node="25,3,0"><b>Online Source:</b> Select an MPC server from the list (e.g., <i>MPC&#8217;s list of observable comets</i>). The program will connect to the web and download the list.</p>
</li>
<li>
<p data-path-to-node="25,4,0"><b>Search:</b> Type the comet&#8217;s name (e.g., &#8220;C/2023 A3&#8221;). Once it appears, check it and click <b>&#8220;Add objects&#8221;</b>.</p>
</li>
</ul>
<h3>Why is this better than manual entry?</h3>
<p>Manual entry of orbital elements is prone to formatting errors, leading to incorrect position calculations. Automatic import from the MPC ensures that parameters are up-to-date, which is crucial as comet orbits undergo subtle changes due to planetary gravity.</p>

<p></p></div></div></div></div></div></section></div> <a href="https://astrophotography.pekdar.net/en/stellarium-adding-comets-asteroids/#more-2903" class="more-link elementor-more-link"><span aria-label="Continue reading Stellarium: Adding New Comets and Asteroids">read more</span></a>]]></content:encoded>
					
		
		
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