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<blockquote style="position: relative; padding-left: 55px;"><section><a href="https://mastodon.social/users/ArpBot/statuses/114061706612656148">Arp Bot 🤖 (arpbot@mastodon.social)'s status on Tuesday, 25-Feb-2025 09:39:12 JST</a><a href="https://mastodon.social/@ArpBot" title="arpbot@mastodon.social"><img src="https://gnusocial.jp/avatar/310204-48-20241228000143.webp" width="48" height="48" alt="Arp Bot 🤖" style="position: absolute; left: 0; top: 0;">Arp Bot 🤖</a></section><article><p>Composite image of Arp 26, also known as M101 or the Pinwheel Galaxy.</p><p>X-rays from Chandra (purple) show the hottest areas of the spiral galaxy. Infrared light from Spitzer (red) traces dust and visible light from Hubble (yellow) highlights starlight . Ultraviolet light from GALEX (blue) shows the emission from young stars.</p><p>Credit: NASA, CXC, SAO;NASA, JPL-Caltech;NASA, STScI<br>Source: <a href="https://chandra.harvard.edu/photo/2012/m101/" rel="nofollow">https://chandra.harvard.edu/photo/2012/m101/</a></p><p><a href="https://mastodon.social/tags/ArpGalaxy" rel="tag">#ArpGalaxy</a> <a href="https://mastodon.social/tags/Galaxy" rel="tag">#Galaxy</a> <a href="https://mastodon.social/tags/Space" rel="tag">#Space</a> <a href="https://mastodon.social/tags/Astronony" rel="tag">#Astronony</a></p></article><footer><a rel="bookmark" href="https://gnusocial.jp/conversation/4625601#notice-9054834">In conversation</a><time datetime="2025-02-25T09:39:12+09:00" title="Tuesday, 25-Feb-2025 09:39:12 JST">about 8 months ago</time> <span>from <span><a href="https://mastodon.social/@ArpBot/114061706612656148" rel="external" title="Sent from mastodon.social via ActivityPub">mastodon.social</a></span></span><a href="https://mastodon.social/@ArpBot/114061706612656148">permalink</a><h4>Attachments</h4><ol><li><label><a rel="external" href="https://gnusocial.jp/attachment/4195508">A multiwavelength image of a spiral galaxy. The galaxy has a small pink core. Several arms spiral clockwise around the core. They are crossed by pink, filamentary dust lanes and made of a haze of yellow stars. Along the arms are purple splotches. In the outer parts of the galaxy, the arms appear blue, dotted with blue star clusters. The arms are somewhat well-defined but asymmetric. One arm curls from about 6 o'clock to 9 o'clock and is mostly separated from the body of the galaxy. Other arms cover the area from 12 o'clock to 6 o'clock.</a></label><br><a href="https://files.mastodon.social/media_attachments/files/114/061/706/561/883/051/original/684a5c9f03f465ee.jpg" rel="external">https://files.mastodon.social/media_attachments/files/114/061/706/561/883/051/original/684a5c9f03f465ee.jpg</a></li><li><article><header><div>Domain not in remote thumbnail source whitelist: chandra.harvard.edu</div><h5><a href="https://chandra.harvard.edu/photo/2012/m101/#ArpGalaxy">Chandra :: Photo Album :: M101 :: May 24, 2012</a></h5><div></div></header><div>Information about the Chandra X-ray Observatory, which was launched on July 23, 1999, its mission and goals, and the people who built it.</div><footer></footer></article></li></ol></footer></blockquote>

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Arp Bot 🤖 (arpbot@mastodon.social)'s status on Tuesday, 25-Feb-2025 09:39:12 JST Arp Bot 🤖
Composite image of Arp 26, also known as M101 or the Pinwheel Galaxy.
X-rays from Chandra (purple) show the hottest areas of the spiral galaxy. Infrared light from Spitzer (red) traces dust and visible light from Hubble (yellow) highlights starlight . Ultraviolet light from GALEX (blue) shows the emission from young stars.
Credit: NASA, CXC, SAO;NASA, JPL-Caltech;NASA, STScI
Source: https://chandra.harvard.edu/photo/2012/m101/
#ArpGalaxy #Galaxy #Space #Astronony
In conversationabout 8 months ago from mastodon.socialpermalink
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1. A multiwavelength image of a spiral galaxy. The galaxy has a small pink core. Several arms spiral clockwise around the core. They are crossed by pink, filamentary dust lanes and made of a haze of yellow stars. Along the arms are purple splotches. In the outer parts of the galaxy, the arms appear blue, dotted with blue star clusters. The arms are somewhat well-defined but asymmetric. One arm curls from about 6 o'clock to 9 o'clock and is mostly separated from the body of the galaxy. Other arms cover the area from 12 o'clock to 6 o'clock.
  https://files.mastodon.social/media_attachments/files/114/061/706/561/883/051/original/684a5c9f03f465ee.jpg
2. Domain not in remote thumbnail source whitelist: chandra.harvard.edu
  Chandra :: Photo Album :: M101 :: May 24, 2012
  Information about the Chandra X-ray Observatory, which was launched on July 23, 1999, its mission and goals, and the people who built it.

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