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	<title>000 light-years &#8211; Science</title>
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	<title>000 light-years &#8211; Science</title>
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		<title>Black hole &#8220;blast&#8221; reaches 300,000 light years</title>
		<link>https://scienmag.com/black-hole-blast-reaches-300000-light-years/</link>
		
		<dc:creator><![CDATA[Grant Pearson]]></dc:creator>
		<pubDate>Wed, 29 Jul 2026 17:12:05 +0000</pubDate>
				<category><![CDATA[Space]]></category>
		<category><![CDATA[000 light-years]]></category>
		<category><![CDATA[astrophysics black hole research]]></category>
		<category><![CDATA[black hole feedback mechanisms]]></category>
		<category><![CDATA[black hole impact on galaxy clusters]]></category>
		<category><![CDATA[black hole outflows and galaxy formation]]></category>
		<category><![CDATA[black hole wind reach 300]]></category>
		<category><![CDATA[black hole-driven galaxy regulation]]></category>
		<category><![CDATA[cosmic scale black hole emissions]]></category>
		<category><![CDATA[galaxy evolution and black hole influence]]></category>
		<category><![CDATA[galaxy-black hole relationship]]></category>
		<category><![CDATA[hierarchical universe structure]]></category>
		<category><![CDATA[Supermassive black hole energy jets]]></category>
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					<description><![CDATA[image: Schematic illustration of the hierarchical structure of the Universe, from a galaxy group (a collection of galaxies) to an individual galaxy and the supermassive black hole at its center. Although a black hole is more than 100 million times smaller than the radius of its host galaxy, it plays a crucial role in the galaxy&#8217;s [&#8230;]]]></description>
										<content:encoded><![CDATA[<div class="entry">
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                    <img decoding="async" src="https://scienmag.com/wp-content/uploads/2026/07/1785345125_529_Return-exactly-one-rewritten-English-science-news-headline-for-the.jpeg" alt="Figure 1">
                  </div><figcaption class="caption">
                  <strong>image: Schematic illustration of the hierarchical structure of the Universe, from a galaxy group (a collection of galaxies) to an individual galaxy and the supermassive black hole at its center. Although a black hole is more than 100 million times smaller than the radius of its host galaxy, it plays a crucial role in the galaxy&#8217;s central region.<br />
</strong><br />
                  view <span class="no-break-text">more <i class="fa fa-angle-right"></i></span></p>
<p class="credit">Credit: Tohoku University</p>
</figcaption></figure>
<p>                            A team of researchers has discovered that the winds generated by supermassive black holes are 100 times more powerful than previously thought, carrying energy across distances of approximately 300,000 light-years. The discovery demonstrates that these explosive winds impact the vast expanse of space beyond the galaxies they inhabit.</p>
<p>&#8220;Black holes are largely known for sucking matter in, but they also eject gas in the form of powerful winds,&#8221; says Satoshi Yamada, Assistant Professor at Tohoku University&#8217;s Frontier Institute for Interdisciplinary Sciences (FRIS). &#8220;These winds were thought to be contained within the galaxy, but our study revealed that the force is immensely more powerful than previously understood.&#8221;</p>
<p>Yamada and his team, comprising colleagues from Kanazawa University and Tokyo Metropolitan University among others, harnessed the X-ray astronomy satellite XRISM to observe the activity of the quasar H1821+643, which is located in the constellation of Draco, approximately 3.4 billion light-years from Earth. Quasars are extremely luminous objects powered by supermassive black holes that actively consume gas.</p>
<p>The rapidly growing black hole is located at the center of the galaxy cluster, where it drives turbulence in the surrounding hot gas that emits X-rays. The researchers precisely determined the motion of the gas by analyzing the emission lines of iron ions.</p>
<p>High-precision observations by XRISM revealed that the high-temperature gas surrounding the black hole does not remain static, but violently disperses over a wide area due to turbulence. The researchers also confirmed that the flow of gas extends beyond the host galaxy, reaching distances of about 300,000 light-years away. The amount of energy involved in the turbulence was approximately 100 times greater than previous estimates and equivalent to several billion supernova explosions &#8211; the explosions that occur when stars reach the end of their lives.</p>
<p>&#8220;For the first time, we have shown that black holes influence the broader cosmic environment through a shock wave of astonishing power,&#8221; adds Yamada. &#8220;Black holes are key drivers of gas flows and motion in space, transporting vast amounts of energy to different regions of the cosmos.&#8221;</p>
<p>Details of the research were published in the journal <em>Nature Astronomy</em> on July 28, 2026.</p>
<p>Future observations are expected to further clarify the effects of black holes on their surrounding environment and how matter and elements circulate throughout the cosmos.</p>
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<div class="details">
<div class="well">
<h4>Journal</h4>
<p>                            Nature Astronomy
                        </p></div>
<div class="well">
<h4>DOI</h4>
<p>                            <a href="http://dx.doi.org/10.1038/s41550-026-02939-x" target="_blank">10.1038/s41550-026-02939-x <i class="fa fa-sign-out"></i></a>
                        </div>
<div class="well">
<h4>Article Title</h4>
<p>                            Vigorous turbulence driven by quasar-mode feedback in a cluster core
                        </p></div>
<div class="well">
<h4>Article Publication Date</h4>
<p>                            28-Jul-2026
                        </p></div></div></div></div>
<p></p>
<div class="contact-info">
                <strong>Media Contact</strong></p>
<p>                                    Public Relations Office</p>
<p>                    Tohoku University</p>
<p>                public_relations@grp.tohoku.ac.jp<br />
            </p></div>
<p></p>
<dl class="dl-horizontal meta stacked">
<dt class="yellow">Journal</dt>
<dd class="yellow"><em>Nature Astronomy</em></dd>
<dt class="red">DOI</dt>
<dd class="red"><em>10.1038/s41550-026-02939-x</em></dd>
</dl>
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