<?xml version="1.0" encoding="utf-8"?>
<rss version="2.0" xmlns:dc="http://purl.org/dc/elements/1.1/" xmlns:content="http://purl.org/rss/1.0/modules/content/">
    <channel>
        <title>Flipper</title>
        <link>https://paragraph.com/@neverstoptowin</link>
        <description>undefined</description>
        <lastBuildDate>Fri, 01 May 2026 22:27:37 GMT</lastBuildDate>
        <docs>https://validator.w3.org/feed/docs/rss2.html</docs>
        <generator>https://github.com/jpmonette/feed</generator>
        <language>en</language>
        <image>
            <title>Flipper</title>
            <url>https://storage.googleapis.com/papyrus_images/7350015b1f27cb0b6d21dca49361d72e47e493370687b200a9a701f03db61985.jpg</url>
            <link>https://paragraph.com/@neverstoptowin</link>
        </image>
        <copyright>All rights reserved</copyright>
        <item>
            <title><![CDATA[On Melancholy Hill]]></title>
            <link>https://paragraph.com/@neverstoptowin/on-melancholy-hill</link>
            <guid>IXG7MrrIActiPpYkyzT2</guid>
            <pubDate>Wed, 01 Feb 2023 07:53:41 GMT</pubDate>
            <description><![CDATA[Up on Melancholy Hill There&apos;s a plastic tree Are you here with me? Just looking out on the day Of another dream Well you can&apos;t get what you want But you can get me So let&apos;s set out to sea, love &apos;Cause you are my medicine When you&apos;re close to me When you&apos;re close to me So call in the submarines &apos;Round the world we&apos;ll go Does anybody know, love If we&apos;re looking out on the day Of another dream? If you can&apos;t get what you want Then come with me Up ...]]></description>
            <content:encoded><![CDATA[<p>Up on Melancholy Hill There&apos;s a plastic tree Are you here with me? Just looking out on the day Of another dream</p><p>Well you can&apos;t get what you want But you can get me So let&apos;s set out to sea, love &apos;Cause you are my medicine When you&apos;re close to me When you&apos;re close to me</p><p>So call in the submarines &apos;Round the world we&apos;ll go Does anybody know, love If we&apos;re looking out on the day Of another dream?</p><p>If you can&apos;t get what you want Then come with me</p><p>Up on Melancholy Hill Sits a manatee Just looking out for the day When you&apos;re close to me When you&apos;re close to me</p><p>When you&apos;re close to me</p><p>Перевести на русский</p>]]></content:encoded>
            <author>neverstoptowin@newsletter.paragraph.com (Flipper)</author>
        </item>
        <item>
            <title><![CDATA[Milky Way]]></title>
            <link>https://paragraph.com/@neverstoptowin/milky-way</link>
            <guid>DI7VwCmF1oeCt0DJHLQH</guid>
            <pubDate>Sat, 21 Jan 2023 11:53:56 GMT</pubDate>
            <description><![CDATA[The Milky Way[b] is the galaxy that includes our Solar System, with the name describing the galaxy&apos;s appearance from Earth: a hazy band of light seen in the night sky formed from stars that cannot be individually distinguished by the naked eye. The term Milky Way is a translation of the Latin via lactea, from the Greek γαλακτικός κύκλος (galaktikos kýklos), meaning "milky circle".[24][25] From Earth, the Milky Way appears as a band because its disk-shaped structure is viewed from within....]]></description>
            <content:encoded><![CDATA[<p>The <strong>Milky Way</strong><a target="_blank" rel="noopener noreferrer nofollow ugc" class="dont-break-out" href="https://en.wikipedia.org/wiki/Milky_Way#cite_note-context-25">[b]</a> is the <a target="_blank" rel="noopener noreferrer nofollow ugc" class="dont-break-out" href="https://en.wikipedia.org/wiki/Galaxy">galaxy</a> that includes our <a target="_blank" rel="noopener noreferrer nofollow ugc" class="dont-break-out" href="https://en.wikipedia.org/wiki/Solar_System">Solar System</a>, with the name describing the galaxy&apos;s appearance from <a target="_blank" rel="noopener noreferrer nofollow ugc" class="dont-break-out" href="https://en.wikipedia.org/wiki/Earth">Earth</a>: a hazy band of light seen in the <a target="_blank" rel="noopener noreferrer nofollow ugc" class="dont-break-out" href="https://en.wikipedia.org/wiki/Night_sky">night sky</a> formed from stars that cannot be individually distinguished by the <a target="_blank" rel="noopener noreferrer nofollow ugc" class="dont-break-out" href="https://en.wikipedia.org/wiki/Naked_eye">naked eye</a>. The term <em>Milky Way</em> is a translation of the Latin <em>via lactea</em>, from the <a target="_blank" rel="noopener noreferrer nofollow ugc" class="dont-break-out" href="https://en.wikipedia.org/wiki/Ancient_Greek">Greek</a> γαλακτικός κύκλος (<em>galaktikos kýklos</em>), meaning &quot;milky circle&quot;.<a target="_blank" rel="noopener noreferrer nofollow ugc" class="dont-break-out" href="https://en.wikipedia.org/wiki/Milky_Way#cite_note-eo_galaxy-26">[24]</a><a target="_blank" rel="noopener noreferrer nofollow ugc" class="dont-break-out" href="https://en.wikipedia.org/wiki/Milky_Way#cite_note-Jankowski-27">[25]</a> From Earth, the Milky Way appears as a band because its disk-shaped structure is viewed from within. <a target="_blank" rel="noopener noreferrer nofollow ugc" class="dont-break-out" href="https://en.wikipedia.org/wiki/Galileo_Galilei">Galileo Galilei</a> first resolved the band of light into individual stars with his telescope in 1610. Until the early 1920s, most astronomers thought that the Milky Way contained all the stars in the <a target="_blank" rel="noopener noreferrer nofollow ugc" class="dont-break-out" href="https://en.wikipedia.org/wiki/Universe">Universe</a>.<a target="_blank" rel="noopener noreferrer nofollow ugc" class="dont-break-out" href="https://en.wikipedia.org/wiki/Milky_Way#cite_note-28">[26]</a> Following the 1920 <a target="_blank" rel="noopener noreferrer nofollow ugc" class="dont-break-out" href="https://en.wikipedia.org/wiki/Great_Debate_(astronomy)">Great Debate</a> between the astronomers <a target="_blank" rel="noopener noreferrer nofollow ugc" class="dont-break-out" href="https://en.wikipedia.org/wiki/Harlow_Shapley">Harlow Shapley</a> and <a target="_blank" rel="noopener noreferrer nofollow ugc" class="dont-break-out" href="https://en.wikipedia.org/wiki/Heber_Doust_Curtis">Heber Doust Curtis</a>,<a target="_blank" rel="noopener noreferrer nofollow ugc" class="dont-break-out" href="https://en.wikipedia.org/wiki/Milky_Way#cite_note-shapley_curtis-29">[27]</a> observations by <a target="_blank" rel="noopener noreferrer nofollow ugc" class="dont-break-out" href="https://en.wikipedia.org/wiki/Edwin_Hubble">Edwin Hubble</a> showed that the Milky Way is just one of many galaxies.</p><p>The Milky Way is a <a target="_blank" rel="noopener noreferrer nofollow ugc" class="dont-break-out" href="https://en.wikipedia.org/wiki/Barred_spiral_galaxy">barred spiral galaxy</a> with an estimated <a target="_blank" rel="noopener noreferrer nofollow ugc" class="dont-break-out" href="https://en.wikipedia.org/wiki/Galaxy#Isophotal_diameter">D25 isophotal diameter</a> of 26.8 ± 1.1 <a target="_blank" rel="noopener noreferrer nofollow ugc" class="dont-break-out" href="https://en.wikipedia.org/wiki/Parsec#Parsecs_and_kiloparsecs">kiloparsecs</a> (87,400 ± 3,590 <a target="_blank" rel="noopener noreferrer nofollow ugc" class="dont-break-out" href="https://en.wikipedia.org/wiki/Light-year">light-years</a>),<a target="_blank" rel="noopener noreferrer nofollow ugc" class="dont-break-out" href="https://en.wikipedia.org/wiki/Milky_Way#cite_note-Goodwin-9">[8]</a> but only about 1,000 light years thick at the spiral arms (more at the bulge). Recent simulations suggest that a <a target="_blank" rel="noopener noreferrer nofollow ugc" class="dont-break-out" href="https://en.wikipedia.org/wiki/Dark_matter">dark matter</a> area, also containing some visible stars, may extend up to a diameter of almost 2 million light-years (613 kpc).<a target="_blank" rel="noopener noreferrer nofollow ugc" class="dont-break-out" href="https://en.wikipedia.org/wiki/Milky_Way#cite_note-croswell2020-30">[28]</a><a target="_blank" rel="noopener noreferrer nofollow ugc" class="dont-break-out" href="https://en.wikipedia.org/wiki/Milky_Way#cite_note-dearson2020-31">[29]</a> The Milky Way has several <a target="_blank" rel="noopener noreferrer nofollow ugc" class="dont-break-out" href="https://en.wikipedia.org/wiki/List_of_Milky_Way%27s_satellite_galaxies">satellite galaxies</a> and is part of the <a target="_blank" rel="noopener noreferrer nofollow ugc" class="dont-break-out" href="https://en.wikipedia.org/wiki/Local_Group">Local Group</a> of galaxies, which form part of the <a target="_blank" rel="noopener noreferrer nofollow ugc" class="dont-break-out" href="https://en.wikipedia.org/wiki/Virgo_Supercluster">Virgo Supercluster</a>, which is itself a component of the <a target="_blank" rel="noopener noreferrer nofollow ugc" class="dont-break-out" href="https://en.wikipedia.org/wiki/Laniakea_Supercluster">Laniakea Supercluster</a>.<a target="_blank" rel="noopener noreferrer nofollow ugc" class="dont-break-out" href="https://en.wikipedia.org/wiki/Milky_Way#cite_note-32">[30]</a><a target="_blank" rel="noopener noreferrer nofollow ugc" class="dont-break-out" href="https://en.wikipedia.org/wiki/Milky_Way#cite_note-33">[31]</a></p><p>It is estimated to contain 100–400 billion stars<a target="_blank" rel="noopener noreferrer nofollow ugc" class="dont-break-out" href="https://en.wikipedia.org/wiki/Milky_Way#cite_note-34">[32]</a><a target="_blank" rel="noopener noreferrer nofollow ugc" class="dont-break-out" href="https://en.wikipedia.org/wiki/Milky_Way#cite_note-35">[33]</a> and at least that number of <a target="_blank" rel="noopener noreferrer nofollow ugc" class="dont-break-out" href="https://en.wikipedia.org/wiki/Planets">planets</a>.<a target="_blank" rel="noopener noreferrer nofollow ugc" class="dont-break-out" href="https://en.wikipedia.org/wiki/Milky_Way#cite_note-Nature-20120111-36">[34]</a><a target="_blank" rel="noopener noreferrer nofollow ugc" class="dont-break-out" href="https://en.wikipedia.org/wiki/Milky_Way#cite_note-Space-20130102-37">[35]</a> The Solar System is located at a radius of about 27,000 light-years (8.3 kpc) from the <a target="_blank" rel="noopener noreferrer nofollow ugc" class="dont-break-out" href="https://en.wikipedia.org/wiki/Galactic_Center">Galactic Center</a>,<a target="_blank" rel="noopener noreferrer nofollow ugc" class="dont-break-out" href="https://en.wikipedia.org/wiki/Milky_Way#cite_note-Gillessen2016-38">[36]</a> on the inner edge of the <a target="_blank" rel="noopener noreferrer nofollow ugc" class="dont-break-out" href="https://en.wikipedia.org/wiki/Orion_Arm">Orion Arm</a>, one of the spiral-shaped concentrations of gas and dust. The stars in the innermost 10,000 light-years form a <a target="_blank" rel="noopener noreferrer nofollow ugc" class="dont-break-out" href="https://en.wikipedia.org/wiki/Bulge_(astronomy)">bulge</a> and one or more bars that radiate from the bulge. The Galactic Center is an intense radio source known as <a target="_blank" rel="noopener noreferrer nofollow ugc" class="dont-break-out" href="https://en.wikipedia.org/wiki/Sagittarius_A*">Sagittarius A*</a>, a <a target="_blank" rel="noopener noreferrer nofollow ugc" class="dont-break-out" href="https://en.wikipedia.org/wiki/Supermassive_black_hole">supermassive black hole</a> of 4.100 (± 0.034) million <a target="_blank" rel="noopener noreferrer nofollow ugc" class="dont-break-out" href="https://en.wikipedia.org/wiki/Solar_mass">solar masses</a>.<a target="_blank" rel="noopener noreferrer nofollow ugc" class="dont-break-out" href="https://en.wikipedia.org/wiki/Milky_Way#cite_note-NYT-20220131-39">[37]</a><a target="_blank" rel="noopener noreferrer nofollow ugc" class="dont-break-out" href="https://en.wikipedia.org/wiki/Milky_Way#cite_note-ARX-20220128-40">[38]</a> Stars and gases at a wide range of distances from the Galactic Center orbit at approximately 220 kilometers per second. The constant rotational speed appears to contradict the laws of <a target="_blank" rel="noopener noreferrer nofollow ugc" class="dont-break-out" href="https://en.wikipedia.org/wiki/Kepler%27s_laws_of_planetary_motion">Keplerian dynamics</a> and suggests that much (about 90%)<a target="_blank" rel="noopener noreferrer nofollow ugc" class="dont-break-out" href="https://en.wikipedia.org/wiki/Milky_Way#cite_note-SA-20190308-41">[39]</a><a target="_blank" rel="noopener noreferrer nofollow ugc" class="dont-break-out" href="https://en.wikipedia.org/wiki/Milky_Way#cite_note-ARX-20190208-42">[40]</a> of the <a target="_blank" rel="noopener noreferrer nofollow ugc" class="dont-break-out" href="https://en.wikipedia.org/wiki/Mass">mass</a> of the Milky Way is invisible to telescopes, neither emitting nor absorbing <a target="_blank" rel="noopener noreferrer nofollow ugc" class="dont-break-out" href="https://en.wikipedia.org/wiki/Electromagnetic_radiation">electromagnetic radiation</a>. This conjectural mass has been termed &quot;<a target="_blank" rel="noopener noreferrer nofollow ugc" class="dont-break-out" href="https://en.wikipedia.org/wiki/Dark_matter">dark matter</a>&quot;.<a target="_blank" rel="noopener noreferrer nofollow ugc" class="dont-break-out" href="https://en.wikipedia.org/wiki/Milky_Way#cite_note-Koupelis_Kuhn2007-43">[41]</a> The rotational period is about 212 million years at the radius of the Sun.<a target="_blank" rel="noopener noreferrer nofollow ugc" class="dont-break-out" href="https://en.wikipedia.org/wiki/Milky_Way#cite_note-newview-15">[14]</a></p><p>The Milky Way as a whole is moving at a velocity of approximately 600 km per second with respect to extragalactic frames of reference. The oldest stars in the Milky Way are nearly as old as the Universe itself and thus probably formed shortly after the <a target="_blank" rel="noopener noreferrer nofollow ugc" class="dont-break-out" href="https://en.wikipedia.org/wiki/Chronology_of_the_universe#Dark_Ages">Dark Ages</a> of the <a target="_blank" rel="noopener noreferrer nofollow ugc" class="dont-break-out" href="https://en.wikipedia.org/wiki/Big_Bang">Big Bang</a>.</p>]]></content:encoded>
            <author>neverstoptowin@newsletter.paragraph.com (Flipper)</author>
            <enclosure url="https://storage.googleapis.com/papyrus_images/fcb8551b0c4fc3490adeab0ff98ee0efd7a838f92918eb08a4a7a2162159c153.jpg" length="0" type="image/jpg"/>
        </item>
        <item>
            <title><![CDATA[Ocean drive]]></title>
            <link>https://paragraph.com/@neverstoptowin/ocean-drive</link>
            <guid>YHVQHBG208HoSE0nh08S</guid>
            <pubDate>Thu, 13 Oct 2022 07:04:55 GMT</pubDate>
            <description><![CDATA[need a vication]]></description>
            <content:encoded><![CDATA[<p>need a vication</p>]]></content:encoded>
            <author>neverstoptowin@newsletter.paragraph.com (Flipper)</author>
        </item>
    </channel>
</rss>