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Second Nexus © 2019
[DIGEST: New Scientist (1, 2), The Atlantic (1, 2), Royal Astronomical Society]
A recent simulation reveals that half of the matter in our galaxy came from the stellar winds of supernova explosions up to a million light years away. A team of astrophysicists from Northwestern University in Illinois discovered that cosmic rays, which are charged particles ejected from the centers of stars during supernovae at nearly the speed of light, are responsible for transporting this material between galaxies.
<p><span style="font-weight: 400;">Scientists previously believed this matter came from </span><a href="https://www.nbcnews.com/mach/mach/here-s-surprising-way-milky-way-galaxy-got-so-massive-ncna787316"><span style="font-weight: 400;">galactic collisions</span></a><span style="font-weight: 400;">.</span></p><p><span style="font-weight: 400;">The Milky Way contains </span><a href="https://asd.gsfc.nasa.gov/blueshift/index.php/2015/07/22/how-many-stars-in-the-milky-way/"><span style="font-weight: 400;">100-400 billion stars</span></a><span style="font-weight: 400;">, giant clouds of gas and dust, and countless smaller objects such as planets, asteroids, and comets. Hydrogen, the most abundant element in the universe, is converted into helium in the cores of stars through nuclear fusion. As stars age and deplete the hydrogen in their cores, their intense gravity continues to fuse helium into heavier elements such as carbon, oxygen and eventually iron. Once a star begins creating iron in its core, the core becomes too heavy, gravity pulls the star’s outer layers inward, and the star explodes as a supernova. This final process can take less than a second.</span></p><p><div data-conversation-spotlight=""></div></p><p><span style="font-weight: 400;">A </span><a href="https://phys.org/news/2016-03-kinds-supernovae.html"><span style="font-weight: 400;">supernova</span></a><span style="font-weight: 400;"> occurs when a star at least eight times as massive as our Sun spends its nuclear fuel and explodes, sending trillions upon trillions of tons of gas and dust and radiation into space. This is known as a Type 2 supernova. The heaviest and rarest elements in our universe, including gold, platinum, and uranium, are created in this process. This material is blasted out into space and over time begins to dissipate in all directions. </span></p><p><span style="font-weight: 400;">In 2014, astronomers Munier Salem and his colleagues at Columbia University in New York developed a simulation that showed these charged particles could drive </span><a href="https://www.newscientist.com/article/mg22429994-400-cosmic-rays-drive-the-galactic-pottery-wheel/"><span style="font-weight: 400;">winds strong enough to shape galaxies</span></a><span style="font-weight: 400;">. </span><span style="font-weight: 400;">These particle </span><a href="https://www.theatlantic.com/science/archive/2017/07/milky-way-intergalactic-winds/535023/"><span style="font-weight: 400;">winds</span></a><span style="font-weight: 400;"> are also believed to give galaxies like the Milky Way their </span><a href="http://www.astronomy.com/news/2015/07/new-hubble-image-shows-cosmic-wind-creating-pillars-of-destruction"><span style="font-weight: 400;">flat disc shape</span></a><span style="font-weight: 400;">, as galactic material is slowly blown away over time. Losing this matter, however, can prevent star formation. In order for stars to form, gas and dust must be dense enough to collapse into a stellar core and ignite nuclear fusion.</span></p><p><span style="font-weight: 400;">In June, Dr. Daniel Anglés-Alcázar, a postdoctoral fellow in astrophysics at Northwestern University and leader of the team of astrophysicists who conducted the research, decided to study the process of wind recycling. They </span><span style="font-weight: 400;">ran </span><a href="https://academic.oup.com/mnras/article-abstract/doi/10.1093/mnras/stx1517/3871367/The-Cosmic-Baryon-Cycle-and-Galaxy-Mass-Assembly?redirectedFrom=fulltext"><span style="font-weight: 400;">computer simulation</span><span style="font-weight: 400;">s</span></a><span style="font-weight: 400;"> which revealed that galaxies with 100 billion or more stars, like our own Milky Way, owe half of their mass to </span><a href="https://www.newscientist.com/article/2141950-half-the-atoms-inside-your-body-came-from-across-the-universe/#link_time=1501124403"><span style="font-weight: 400;">interstellar recycling</span></a><span style="font-weight: 400;">. </span><span style="font-weight: 400;">The simulations revealed that supernovae, the explosions that occur when massive stars die, produce </span><a href="https://www.theatlantic.com/science/archive/2017/07/milky-way-intergalactic-winds/535023/"><span style="font-weight: 400;">cosmic rays powerful enough</span></a><span style="font-weight: 400;"> to travel across space and get captured by distant galaxies.</span></p><p class="shortcode-media shortcode-media-rebelmouse-image"><img type="lazy-image" data-runner-src="https://assets.rebelmouse.io/eyJhbGciOiJIUzI1NiIsInR5cCI6IkpXVCJ9.eyJpbWFnZSI6Imh0dHBzOi8vYXNzZXRzLnJibC5tcy8yMjAzODU2NC9vcmlnaW4uanBnIiwiZXhwaXJlc19hdCI6MTYzMjM0NzU1MH0.Bpxr4w876lKRk4JVBHLSJwxrEZMTg81oCCHbxATd4kQ/img.jpg?width=980" id="88317" class="rm-shortcode" data-rm-shortcode-id="eab4bdf12fd7855ad5cedd4685650b1f" data-rm-shortcode-name="rebelmouse-image"><small class="image-media media-caption" placeholder="add caption...">Credit: <a href="https://cdn.theatlantic.com/assets/media/img/mt/2017/07/1._Pair_of_nearby_galaxies_with_possible_intergalactic_transfer-1/lead_960.jpg?1501176494">Source</a>.</small></p><p><span style="font-weight: 400;">Until now, </span><span style="font-weight: 400;">“we did not realize how much of the mass in today’s Milky Way-like galaxies was actually ‘stolen’ from the winds of other galaxies,” said </span><span style="font-weight: 400;">co-author </span><a href="http://www.physics.northwestern.edu/people/faculty/core-faculty/claude-andre-faucher-giguere.html"><span style="font-weight: 400;">Claude-André Faucher-Giguère</span></a><span style="font-weight: 400;">. Cosmic rays lose energy and density over time as they travel through space, </span><span style="font-weight: 400;">and g</span><span style="font-weight: 400;">alactic winds were previously </span><a href="https://www.newscientist.com/article/2141950-half-the-atoms-inside-your-body-came-from-across-the-universe/#link_time=1501124403"><span style="font-weight: 400;">thought too weak</span></a><span style="font-weight: 400;"> to account for such a large transfer of material. “We assumed that the winds were confined to the galaxies they came from – that they could recycle by falling back onto the galaxy that ejected them, but not transfer much mass from one galaxy to another.”</span></p><p><span style="font-weight: 400;">The researchers demonstrated a process that they named “</span><a href="https://www.theatlantic.com/science/archive/2017/07/milky-way-intergalactic-winds/535023/"><span style="font-weight: 400;">intergalactic transfer</span></a><span style="font-weight: 400;">,” where gases flow from smaller galaxies to larger galaxies, like the Milky Way. </span></p><p><span style="font-weight: 400;">Based on the simulations, the researchers concluded that intergalactic winds may be responsible for up to 50 percent of all matter. “Half of our very own galaxy,” they </span><a href="https://www.theatlantic.com/science/archive/2017/07/milky-way-intergalactic-winds/535023/#Correction"><span style="font-weight: 400;">suggest</span></a><span style="font-weight: 400;">, “could have originated from another corner of the universe. The atoms that built the solar system, the planets, and even our own bodies may have come from another galaxy perhaps as far as 1 million light-years away.”</span></p><p><span style="font-weight: 400;">“It was actually surprising for us to find out that there is that much exchange of mass between galaxies,” Anglés-Alcázar said. “It’s very interesting to think of our galaxy not as some isolated entity, but to think of the galaxy as being surrounded by gas which may come from many different sources.”</span></p><p><span style="font-weight: 400;">Earlier this year, astronomers at the Harvard-Smithsonian Center for Astrophysics </span><a href="https://www.theatlantic.com/science/archive/2017/01/galaxy-theft/512801/"><span style="font-weight: 400;">discovered</span></a><span style="font-weight: 400;"> that some of the most distant stars in the galaxy were pulled from the Sagittarius dwarf galaxy, a much smaller galaxy that surrounds the Milky Way. Gravitational tides were believed to be responsible for that transfer.</span></p><p><span style="font-weight: 400;">More computer simulations will be needed to better understand intergalactic transfers. Anglés-Alcázar suggests that the phenomenon could eventually be directly observed using the Hubble Telescope.</span></p>
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