<?xml version="1.0" encoding="UTF-8"?><rss version="2.0" xmlns:content="http://purl.org/rss/1.0/modules/content/">
  <channel>
    <title>Star &amp;mdash; Paul Sutton</title>
    <link>https://personaljournal.ca/paulsutton/tag:Star</link>
    <description>Personal Blog</description>
    <pubDate>Tue, 05 May 2026 13:05:48 +0000</pubDate>
    <item>
      <title>Exoplanets Transit simulator</title>
      <link>https://personaljournal.ca/paulsutton/exoplanets-transit-simulator</link>
      <description>&lt;![CDATA[Exoplanets Transit simulator&#xA;&#xA;This was posted to Mastodon by [Dr. Alexandre Santerne](&#xA;https://astrodon.social/@AlexSanterne).  Just had a go and it looks really nice and smooth, and has few options to change the simulation parameters.&#xA;&#xA;Do you know how #astronomers are hunting for #exoplanets ? Most of them are discovered with the transit and/or radial velocity techniques.&#xA;&#xA;We developed at #LAM (#laboratoire d&#39;#astrophysique de #Marseille) a web tool that simulate an #exoplanet and show you their photometric and radial velocity signals. Feel free to play with the parameters and see how they change the signals.&#xA;Links&#xA;&#xA;Exoplanet Simulator&#xA;Laboratoire d&#39;astrophysique de Marseille &#xA;&#xA;Tags&#xA;&#xA;#Exoplanet,#Astronomy,#Astrophysics,#Marselle,#Simulator,#Transit,&#xA;#Stars,#Star,#Exoplanet,#Spectra,#AbsorbtionSpectra,#EmissionSpectra&#xA;&#xA;hr&#xD;&#xA;&#xD;&#xA;table&#xD;&#xA;thead&#xD;&#xA;trtda rel=&#34;me&#34; href=&#34;https://qoto.org/@zleap&#34;Mastodon/a/td&#xD;&#xA;tda href=&#34;https://wiki.ircnow.org/?n=Shelllabs.Intro&#34;ShellLabs/td&#xD;&#xA;tda href=&#34;https://joinmastodon.org/&#34;Join Mastodon/a/td/tr/thead/table&#xD;&#xA;center&#xD;&#xA;AI statement : b Consent is NOT granted to use the content of this blog for the purposes of AI training or similar activity.  Consent CANNOT be assumed, it has to be granted. /b&#xD;&#xA;/center&#xD;&#xA;&#xD;&#xA;a href=&#34;https://liberapay.com/PaulSutton/donate&#34;img alt=&#34;Donate using Liberapay&#34; src=&#34;https://liberapay.com/assets/widgets/donate.svg&#34;/a&#xD;&#xA;]]&gt;</description>
      <content:encoded><![CDATA[<p>Exoplanets Transit simulator</p>

<p>This was posted to Mastodon by <a href="https://astrodon.social/@AlexSanterne" rel="nofollow">Dr. Alexandre Santerne</a>.  Just had a go and it looks really nice and smooth, and has few options to change the simulation parameters.</p>

<pre><code>Do you know how #astronomers are hunting for #exoplanets ? Most of them are discovered with the transit and/or radial velocity techniques.

We developed at #LAM (#laboratoire d&#39;#astrophysique de #Marseille) a web tool that simulate an #exoplanet and show you their photometric and radial velocity signals. Feel free to play with the parameters and see how they change the signals.
</code></pre>

<p><strong>Links</strong></p>
<ul><li><a href="https://exoplanet.lam.fr/exoPindir-en.html" rel="nofollow">Exoplanet Simulator</a></li>
<li><a href="https://www.lam.fr/" rel="nofollow">Laboratoire d&#39;astrophysique de Marseille </a></li></ul>

<p><strong>Tags</strong></p>

<p><a href="/paulsutton/tag:Exoplanet" class="hashtag" rel="nofollow"><span>#</span><span class="p-category">Exoplanet</span></a>,<a href="/paulsutton/tag:Astronomy" class="hashtag" rel="nofollow"><span>#</span><span class="p-category">Astronomy</span></a>,<a href="/paulsutton/tag:Astrophysics" class="hashtag" rel="nofollow"><span>#</span><span class="p-category">Astrophysics</span></a>,<a href="/paulsutton/tag:Marselle" class="hashtag" rel="nofollow"><span>#</span><span class="p-category">Marselle</span></a>,<a href="/paulsutton/tag:Simulator" class="hashtag" rel="nofollow"><span>#</span><span class="p-category">Simulator</span></a>,<a href="/paulsutton/tag:Transit" class="hashtag" rel="nofollow"><span>#</span><span class="p-category">Transit</span></a>,
<a href="/paulsutton/tag:Stars" class="hashtag" rel="nofollow"><span>#</span><span class="p-category">Stars</span></a>,<a href="/paulsutton/tag:Star" class="hashtag" rel="nofollow"><span>#</span><span class="p-category">Star</span></a>,<a href="/paulsutton/tag:Exoplanet" class="hashtag" rel="nofollow"><span>#</span><span class="p-category">Exoplanet</span></a>,<a href="/paulsutton/tag:Spectra" class="hashtag" rel="nofollow"><span>#</span><span class="p-category">Spectra</span></a>,<a href="/paulsutton/tag:AbsorbtionSpectra" class="hashtag" rel="nofollow"><span>#</span><span class="p-category">AbsorbtionSpectra</span></a>,<a href="/paulsutton/tag:EmissionSpectra" class="hashtag" rel="nofollow"><span>#</span><span class="p-category">EmissionSpectra</span></a></p>

<hr>

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]]></content:encoded>
      <guid>https://personaljournal.ca/paulsutton/exoplanets-transit-simulator</guid>
      <pubDate>Tue, 18 Jul 2023 06:00:00 +0000</pubDate>
    </item>
    <item>
      <title>Seeing universe&#39;s most massive known star</title>
      <link>https://personaljournal.ca/paulsutton/seeing-universes-most-massive-known-star</link>
      <description>&lt;![CDATA[Seeing universe&#39;s most massive known star&#xA;&#xA;Astronomy is making fantastic new discoveries all the time,  not just with space based telescopes but with ground based observatories too.&#xA;&#xA;By harnessing the capabilities of the Gemini South telescope in Chile, astronomers have obtained the sharpest image ever of the star R136a1, the most massive known star in the universe. Their research challenges our understanding of the most massive stars and suggests that they may not be as massive as previously thought. &#xA;This  article explains more.  &#xA;&#xA;We are improving our knowledge and understanding all the time, with new telescopes both earth and space based due to come online over the next decade alone.  This is probably a good time to start looking at studying astronomy and being part of something really exciting.&#xA;&#xA;Links&#xA;&#xA;Science Daily&#xA;Science Forums&#xA;&#xA;Tags&#xA;&#xA;#Science,#ScienceDaily,#Astronomy,#Star,#Massive,&#xA;&#xA;hr&#xD;&#xA;&#xD;&#xA;table&#xD;&#xA;thead&#xD;&#xA;trtda rel=&#34;me&#34; href=&#34;https://qoto.org/@zleap&#34;Mastodon/a/td&#xD;&#xA;tda href=&#34;https://wiki.ircnow.org/?n=Shelllabs.Intro&#34;ShellLabs/td&#xD;&#xA;tda href=&#34;https://joinmastodon.org/&#34;Join Mastodon/a/td/tr/thead/table&#xD;&#xA;center&#xD;&#xA;AI statement : b Consent is NOT granted to use the content of this blog for the purposes of AI training or similar activity.  Consent CANNOT be assumed, it has to be granted. /b&#xD;&#xA;/center&#xD;&#xA;&#xD;&#xA;a href=&#34;https://liberapay.com/PaulSutton/donate&#34;img alt=&#34;Donate using Liberapay&#34; src=&#34;https://liberapay.com/assets/widgets/donate.svg&#34;/a&#xD;&#xA;]]&gt;</description>
      <content:encoded><![CDATA[<p>Seeing universe&#39;s most massive known star</p>

<p>Astronomy is making fantastic new discoveries all the time,  not just with space based telescopes but with ground based observatories too.</p>

<pre><code>By harnessing the capabilities of the Gemini South telescope in Chile, astronomers have obtained the sharpest image ever of the star R136a1, the most massive known star in the universe. Their research challenges our understanding of the most massive stars and suggests that they may not be as massive as previously thought. 
</code></pre>

<p>This  <a href="https://www.sciencedaily.com/releases/2022/08/220818163715.htm" rel="nofollow">article</a> explains more.</p>

<p>We are improving our knowledge and understanding all the time, with new telescopes both earth and space based due to come online over the next decade alone.  This is probably a good time to start looking at studying astronomy and being part of something really exciting.</p>

<p><strong>Links</strong></p>
<ul><li><a href="https://www.sciencedaily.com" rel="nofollow">Science Daily</a></li>
<li><a href="https://www.scienceforums.net" rel="nofollow">Science Forums</a></li></ul>

<p><strong>Tags</strong></p>

<p><a href="/paulsutton/tag:Science" class="hashtag" rel="nofollow"><span>#</span><span class="p-category">Science</span></a>,<a href="/paulsutton/tag:ScienceDaily" class="hashtag" rel="nofollow"><span>#</span><span class="p-category">ScienceDaily</span></a>,<a href="/paulsutton/tag:Astronomy" class="hashtag" rel="nofollow"><span>#</span><span class="p-category">Astronomy</span></a>,<a href="/paulsutton/tag:Star" class="hashtag" rel="nofollow"><span>#</span><span class="p-category">Star</span></a>,<a href="/paulsutton/tag:Massive" class="hashtag" rel="nofollow"><span>#</span><span class="p-category">Massive</span></a>,</p>

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]]></content:encoded>
      <guid>https://personaljournal.ca/paulsutton/seeing-universes-most-massive-known-star</guid>
      <pubDate>Fri, 26 Aug 2022 06:00:00 +0000</pubDate>
    </item>
    <item>
      <title>Abundances in Przybylski&#39;s star</title>
      <link>https://personaljournal.ca/paulsutton/abundances-in-przybylskis-star-x3lh</link>
      <description>&lt;![CDATA[Abundances in Przybylski&#39;s star&#xA;( per-zib-ill-skee)&#xA;&#xA;This looks like a really interesting paper, published on Oxford Academic [1],  examining,  what appears to be the unusual composition of Przybylski&#39;s star [2].  According to Wikipedia [3]* is in the &#34;Southern constellation of Centaurus&#34;&#xA;&#xA;See [4] for a better reference.  &#xA;&#xA;There seems to be quite a few heavier element detected.&#xA;&#xA;REFERENCES&#xA;&#xA;1 Oxford Academic&#xA;2 Paper&#xA;3 Przybylski&#39;sStar (Wikipedia)&#xA;https://www.daviddarling.info&#xA;&#xA;Related papers&#xA;&#xA;Isotope shift and search for metastable superheavy elements in astrophysical data &#xA;Isotope shift, non-linearity of King plots and the search for new particles &#xA;Magnetic and pulsational variability of Przybylski&#39;s star (HD10106&#xA;&#xA;This may also be useful / relevant&#xA;&#xA;Periodic Table of Isotopes&#xA;&#xA;TAGS&#xA;&#xA;#Astronomy,#Star,#Science,#Paper,#Chemistry,#Astrochemistry.&#xA;#arXiv,#Isotopes,#SuperHeavy&#xA;&#xA;DISCUSSION&#xA;&#xA;Discourse topic&#xA;&#xA;a rel=&#34;license&#34; href=&#34;http://creativecommons.org/licenses/by-sa/4.0/&#34;img alt=&#34;Creative Commons Licence&#34; style=&#34;border-width:0&#34; src=&#34;https://i.creativecommons.org/l/by-sa/4.0/88x31.png&#34; //abr /This work is licensed under a a rel=&#34;license&#34; href=&#34;http://creativecommons.org/licenses/by-sa/4.0/&#34;Creative Commons Attribution-ShareAlike 4.0 International License/a&#xA;&#xA;hr&#xD;&#xA;&#xD;&#xA;table&#xD;&#xA;thead&#xD;&#xA;trtda rel=&#34;me&#34; href=&#34;https://qoto.org/@zleap&#34;Mastodon/a/td&#xD;&#xA;tda href=&#34;https://wiki.ircnow.org/?n=Shelllabs.Intro&#34;ShellLabs/td&#xD;&#xA;tda href=&#34;https://joinmastodon.org/&#34;Join Mastodon/a/td/tr/thead/table&#xD;&#xA;center&#xD;&#xA;AI statement : b Consent is NOT granted to use the content of this blog for the purposes of AI training or similar activity.  Consent CANNOT be assumed, it has to be granted. /b&#xD;&#xA;/center&#xD;&#xA;&#xD;&#xA;a href=&#34;https://liberapay.com/PaulSutton/donate&#34;img alt=&#34;Donate using Liberapay&#34; src=&#34;https://liberapay.com/assets/widgets/donate.svg&#34;/a&#xD;&#xA;]]&gt;</description>
      <content:encoded><![CDATA[<p>Abundances in Przybylski&#39;s star
( per-zib-ill-skee)</p>

<p>This looks like a really interesting paper, published on Oxford Academic [1],  examining,  what appears to be the unusual composition of Przybylski&#39;s star [2].  According to Wikipedia [3]* is in the “Southern constellation of Centaurus”</p>
<ul><li>See [4] for a better reference.<br></li></ul>

<p>There seems to be quite a few heavier element detected.</p>

<p><strong>REFERENCES</strong></p>

<p>1 <a href="https://academic.oup.com" rel="nofollow">Oxford Academic</a>
2 <a href="https://academic.oup.com/mnras/article/317/2/299/1005394" rel="nofollow">Paper</a>
3 <a href="https://en.wikipedia.org/wiki/Przybylski%27s_Star" rel="nofollow">Przybylski&#39;s_Star (Wikipedia)</a>
4. <a href="https://www.daviddarling.info/encyclopedia/P/Przybylskis_Star.html" rel="nofollow">https://www.daviddarling.info</a></p>

<p>Related papers</p>
<ul><li><a href="https://arxiv.org/abs/1703.04250" rel="nofollow">Isotope shift and search for metastable superheavy elements in astrophysical data </a></li>
<li><a href="https://arxiv.org/abs/1709.00600" rel="nofollow">Isotope shift, non-linearity of King plots and the search for new particles </a></li>
<li><a href="https://arxiv.org/abs/1804.07260" rel="nofollow">Magnetic and pulsational variability of Przybylski&#39;s star (HD10106</a></li></ul>

<p>This may also be useful / relevant</p>

<p><img src="https://i0.wp.com/www.compoundchem.com/wp-content/uploads/2019/12/20-%E2%80%93-The-periodic-table-of-isotopes-v2.png?resize=1024%2C724&ssl=1" alt="Periodic Table of Isotopes"></p>

<p><strong>TAGS</strong></p>

<p><a href="/paulsutton/tag:Astronomy" class="hashtag" rel="nofollow"><span>#</span><span class="p-category">Astronomy</span></a>,<a href="/paulsutton/tag:Star" class="hashtag" rel="nofollow"><span>#</span><span class="p-category">Star</span></a>,<a href="/paulsutton/tag:Science" class="hashtag" rel="nofollow"><span>#</span><span class="p-category">Science</span></a>,<a href="/paulsutton/tag:Paper" class="hashtag" rel="nofollow"><span>#</span><span class="p-category">Paper</span></a>,<a href="/paulsutton/tag:Chemistry" class="hashtag" rel="nofollow"><span>#</span><span class="p-category">Chemistry</span></a>,<a href="/paulsutton/tag:Astrochemistry" class="hashtag" rel="nofollow"><span>#</span><span class="p-category">Astrochemistry</span></a>.
<a href="/paulsutton/tag:arXiv" class="hashtag" rel="nofollow"><span>#</span><span class="p-category">arXiv</span></a>,<a href="/paulsutton/tag:Isotopes" class="hashtag" rel="nofollow"><span>#</span><span class="p-category">Isotopes</span></a>,<a href="/paulsutton/tag:SuperHeavy" class="hashtag" rel="nofollow"><span>#</span><span class="p-category">SuperHeavy</span></a></p>

<p><strong>DISCUSSION</strong></p>
<ul><li><a href="https://discourse.qoto.org/t/abundances-in-przybylskis-star/595" rel="nofollow">Discourse topic</a></li></ul>

<p><a href="http://creativecommons.org/licenses/by-sa/4.0/" rel="nofollow"><img alt="Creative Commons Licence" style="border-width:0" src="https://i.creativecommons.org/l/by-sa/4.0/88x31.png"/></a><br/>This work is licensed under a <a href="http://creativecommons.org/licenses/by-sa/4.0/" rel="nofollow">Creative Commons Attribution-ShareAlike 4.0 International License</a></p>

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]]></content:encoded>
      <guid>https://personaljournal.ca/paulsutton/abundances-in-przybylskis-star-x3lh</guid>
      <pubDate>Tue, 30 Mar 2021 17:38:28 +0000</pubDate>
    </item>
    <item>
      <title>Abundances in Przybylski&#39;s star</title>
      <link>https://personaljournal.ca/paulsutton/abundances-in-przybylskis-star</link>
      <description>&lt;![CDATA[Abundances in Przybylski&#39;s star&#xA;( per-zib-ill-skee)&#xA;&#xA;This looks like a really interesting paper, published on Oxford Academic [1],  examining,  what appears to be the unusual composition of Przybylski&#39;s star [2].  According to Wikipedia* is in the &#34;Southern constellation of Centaurus&#34;&#xA;&#xA;I need a better academic references for this, which could be at [4].  &#xA;&#xA;There seems to be quite a few heavier element detected.&#xA;&#xA;REFERENCES&#xA;&#xA;1 Oxford Academic&#xA;2 Paper&#xA;3 Przybylski&#39;sStar (Wikipedia)&#xA;https://www.daviddarling.info&#xA;&#xA;Related papers&#xA;&#xA;Isotope shift and search for metastable superheavy elements in astrophysical data &#xA;Isotope shift, non-linearity of King plots and the search for new particles &#xA;Magnetic and pulsational variability of Przybylski&#39;s star (HD10106&#xA;&#xA;This may also be useful / relevant&#xA;&#xA;Periodic Table of Isotopes&#xA;&#xA;TAGS&#xA;&#xA;#Astronomy,#Star,#Science,#Paper,#Chemistry,#Astrochemistry.&#xA;#arXiv,#Isotopes,#SuperHeavy&#xA;&#xA;a href=&#34;https://liberapay.com/PaulSutton/donate&#34;img alt=&#34;Donate using Liberapay&#34; src=&#34;https://liberapay.com/assets/widgets/donate.svg&#34;/a&#xA;&#xA;img src=&#34;https://socialhub.activitypub.rocks/uploads/default/original/1X/6aac842b7ff5c58385a02f3a131c259281be88c8.png&#34; target=&#34;blank&#34; &#xA;&#xA;a rel=&#34;license&#34; href=&#34;http://creativecommons.org/licenses/by-sa/4.0/&#34;img alt=&#34;Creative Commons Licence&#34; style=&#34;border-width:0&#34; src=&#34;https://i.creativecommons.org/l/by-sa/4.0/88x31.png&#34; //abr /This work is licensed under a a rel=&#34;license&#34; href=&#34;http://creativecommons.org/licenses/by-sa/4.0/&#34;Creative Commons Attribution-ShareAlike 4.0 International License/a&#xA;&#xA;hr&#xD;&#xA;&#xD;&#xA;table&#xD;&#xA;thead&#xD;&#xA;trtda rel=&#34;me&#34; href=&#34;https://qoto.org/@zleap&#34;Mastodon/a/td&#xD;&#xA;tda href=&#34;https://wiki.ircnow.org/?n=Shelllabs.Intro&#34;ShellLabs/td&#xD;&#xA;tda href=&#34;https://joinmastodon.org/&#34;Join Mastodon/a/td/tr/thead/table&#xD;&#xA;center&#xD;&#xA;AI statement : b Consent is NOT granted to use the content of this blog for the purposes of AI training or similar activity.  Consent CANNOT be assumed, it has to be granted. /b&#xD;&#xA;/center&#xD;&#xA;&#xD;&#xA;a href=&#34;https://liberapay.com/PaulSutton/donate&#34;img alt=&#34;Donate using Liberapay&#34; src=&#34;https://liberapay.com/assets/widgets/donate.svg&#34;/a&#xD;&#xA;]]&gt;</description>
      <content:encoded><![CDATA[<p>Abundances in Przybylski&#39;s star
( per-zib-ill-skee)</p>

<p>This looks like a really interesting paper, published on Oxford Academic [1],  examining,  what appears to be the unusual composition of Przybylski&#39;s star [2].  According to Wikipedia* is in the “Southern constellation of Centaurus”</p>
<ul><li>I need a better academic references for this, which could be at [4].<br></li></ul>

<p>There seems to be quite a few heavier element detected.</p>

<p><strong>REFERENCES</strong></p>

<p>1 <a href="https://academic.oup.com" rel="nofollow">Oxford Academic</a>
2 <a href="https://academic.oup.com/mnras/article/317/2/299/1005394" rel="nofollow">Paper</a>
3 <a href="https://en.wikipedia.org/wiki/Przybylski%27s_Star" rel="nofollow">Przybylski&#39;s_Star (Wikipedia)</a>
4. <a href="https://www.daviddarling.info/encyclopedia/P/Przybylskis_Star.html" rel="nofollow">https://www.daviddarling.info</a></p>

<p>Related papers</p>
<ul><li><a href="https://arxiv.org/abs/1703.04250" rel="nofollow">Isotope shift and search for metastable superheavy elements in astrophysical data </a></li>
<li><a href="https://arxiv.org/abs/1709.00600" rel="nofollow">Isotope shift, non-linearity of King plots and the search for new particles </a></li>
<li><a href="https://arxiv.org/abs/1804.07260" rel="nofollow">Magnetic and pulsational variability of Przybylski&#39;s star (HD10106</a></li></ul>

<p>This may also be useful / relevant</p>

<p><img src="https://i0.wp.com/www.compoundchem.com/wp-content/uploads/2019/12/20-%E2%80%93-The-periodic-table-of-isotopes-v2.png?resize=1024%2C724&ssl=1" alt="Periodic Table of Isotopes"></p>

<p><strong>TAGS</strong></p>

<p><a href="/paulsutton/tag:Astronomy" class="hashtag" rel="nofollow"><span>#</span><span class="p-category">Astronomy</span></a>,<a href="/paulsutton/tag:Star" class="hashtag" rel="nofollow"><span>#</span><span class="p-category">Star</span></a>,<a href="/paulsutton/tag:Science" class="hashtag" rel="nofollow"><span>#</span><span class="p-category">Science</span></a>,<a href="/paulsutton/tag:Paper" class="hashtag" rel="nofollow"><span>#</span><span class="p-category">Paper</span></a>,<a href="/paulsutton/tag:Chemistry" class="hashtag" rel="nofollow"><span>#</span><span class="p-category">Chemistry</span></a>,<a href="/paulsutton/tag:Astrochemistry" class="hashtag" rel="nofollow"><span>#</span><span class="p-category">Astrochemistry</span></a>.
<a href="/paulsutton/tag:arXiv" class="hashtag" rel="nofollow"><span>#</span><span class="p-category">arXiv</span></a>,<a href="/paulsutton/tag:Isotopes" class="hashtag" rel="nofollow"><span>#</span><span class="p-category">Isotopes</span></a>,<a href="/paulsutton/tag:SuperHeavy" class="hashtag" rel="nofollow"><span>#</span><span class="p-category">SuperHeavy</span></a></p>

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      <guid>https://personaljournal.ca/paulsutton/abundances-in-przybylskis-star</guid>
      <pubDate>Fri, 26 Mar 2021 16:25:06 +0000</pubDate>
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