<?xml version="1.0" encoding="UTF-8"?><rss version="2.0"
	xmlns:content="http://purl.org/rss/1.0/modules/content/"
	xmlns:dc="http://purl.org/dc/elements/1.1/"
	xmlns:atom="http://www.w3.org/2005/Atom"
	xmlns:sy="http://purl.org/rss/1.0/modules/syndication/"
	
	>
<channel>
	<title>
	Comments on: Exoplanet detected inside gap in accretion disk surrounding a Sunlike star	</title>
	<atom:link href="https://behindtheblack.com/behind-the-black/points-of-information/exoplanet-detected-inside-gap-in-accretion-disk-surrounding-a-sunlike-star/feed/" rel="self" type="application/rss+xml" />
	<link>https://behindtheblack.com/behind-the-black/points-of-information/exoplanet-detected-inside-gap-in-accretion-disk-surrounding-a-sunlike-star/</link>
	<description></description>
	<lastBuildDate>Thu, 04 Sep 2025 05:52:12 +0000</lastBuildDate>
	<sy:updatePeriod>
	hourly	</sy:updatePeriod>
	<sy:updateFrequency>
	1	</sy:updateFrequency>
	<generator>https://wordpress.org/?v=6.9.4</generator>
	<item>
		<title>
		By: Blair Ivey		</title>
		<link>https://behindtheblack.com/behind-the-black/points-of-information/exoplanet-detected-inside-gap-in-accretion-disk-surrounding-a-sunlike-star/#comment-1622440</link>

		<dc:creator><![CDATA[Blair Ivey]]></dc:creator>
		<pubDate>Thu, 04 Sep 2025 05:52:12 +0000</pubDate>
		<guid isPermaLink="false">https://behindtheblack.com/?p=116677#comment-1622440</guid>

					<description><![CDATA[&quot; . . . leaving room for lesser planets to form out of denser material  . . .&quot;

&quot;And where are you from?&quot;

&quot;The Lesser Planets.&quot;

&quot;Oh.&quot;]]></description>
			<content:encoded><![CDATA[<p>&#8221; . . . leaving room for lesser planets to form out of denser material  . . .&#8221;</p>
<p>&#8220;And where are you from?&#8221;</p>
<p>&#8220;The Lesser Planets.&#8221;</p>
<p>&#8220;Oh.&#8221;</p>
]]></content:encoded>
		
			</item>
		<item>
		<title>
		By: Max		</title>
		<link>https://behindtheblack.com/behind-the-black/points-of-information/exoplanet-detected-inside-gap-in-accretion-disk-surrounding-a-sunlike-star/#comment-1622436</link>

		<dc:creator><![CDATA[Max]]></dc:creator>
		<pubDate>Wed, 03 Sep 2025 23:44:09 +0000</pubDate>
		<guid isPermaLink="false">https://behindtheblack.com/?p=116677#comment-1622436</guid>

					<description><![CDATA[I’ve never been sure about the correct direction for migration. 
   As a planet gets more massive while holding it’s directional inertia, does increased mass push it outward? Or does the increase in mass, increase it’s gravitational pull to the star causing a migration inward? 
   Or are the two forces in balance?

   I assumed because the larger concentrations of gas and dust is near the star that that is where planet creation is most likely, and the more massive they get the further out they migrate? (Using our own system as a model, gas giants far out into the system) leaving room for lesser planets to form out of denser material left over closer to the sun. 
    But then stellar nurseries create a new suns from clouds of material that is irregular in shape, that is “not” in the shape of a disk... this leads me to believe that the accretion disk may have been massive out gassing from the sun to begin with. 

   I see the other planet close to the center as a white spot similar to the white spot in the gap of the ring. But I also see a dark spot near the center and another opposite of the planet in the same ring gap. 
   Three anomalies at the bottom of the picture, one looks like a brown dwarf with a circular outline but it could be a object in our own system that got captured in the picture. 
   Follow up pictures in the near future will show significant movement to verify theory. Bigger space telescopes and technology improvement will solve many mysteries in our lifetime!]]></description>
			<content:encoded><![CDATA[<p>I’ve never been sure about the correct direction for migration.<br />
   As a planet gets more massive while holding it’s directional inertia, does increased mass push it outward? Or does the increase in mass, increase it’s gravitational pull to the star causing a migration inward?<br />
   Or are the two forces in balance?</p>
<p>   I assumed because the larger concentrations of gas and dust is near the star that that is where planet creation is most likely, and the more massive they get the further out they migrate? (Using our own system as a model, gas giants far out into the system) leaving room for lesser planets to form out of denser material left over closer to the sun.<br />
    But then stellar nurseries create a new suns from clouds of material that is irregular in shape, that is “not” in the shape of a disk&#8230; this leads me to believe that the accretion disk may have been massive out gassing from the sun to begin with. </p>
<p>   I see the other planet close to the center as a white spot similar to the white spot in the gap of the ring. But I also see a dark spot near the center and another opposite of the planet in the same ring gap.<br />
   Three anomalies at the bottom of the picture, one looks like a brown dwarf with a circular outline but it could be a object in our own system that got captured in the picture.<br />
   Follow up pictures in the near future will show significant movement to verify theory. Bigger space telescopes and technology improvement will solve many mysteries in our lifetime!</p>
]]></content:encoded>
		
			</item>
		<item>
		<title>
		By: F		</title>
		<link>https://behindtheblack.com/behind-the-black/points-of-information/exoplanet-detected-inside-gap-in-accretion-disk-surrounding-a-sunlike-star/#comment-1622189</link>

		<dc:creator><![CDATA[F]]></dc:creator>
		<pubDate>Mon, 01 Sep 2025 01:36:54 +0000</pubDate>
		<guid isPermaLink="false">https://behindtheblack.com/?p=116677#comment-1622189</guid>

					<description><![CDATA[Guess what!!

The climate on the new planet is already changing.]]></description>
			<content:encoded><![CDATA[<p>Guess what!!</p>
<p>The climate on the new planet is already changing.</p>
]]></content:encoded>
		
			</item>
	</channel>
</rss>
