{"id":6437,"date":"2010-01-25T09:18:00","date_gmt":"2010-01-25T09:18:00","guid":{"rendered":"http:\/\/euvolution.com\/futurist-transhuman-news-blog\/voyager-makes-an-interstellar-discovery\/"},"modified":"2010-01-25T09:18:00","modified_gmt":"2010-01-25T09:18:00","slug":"voyager-makes-an-interstellar-discovery","status":"publish","type":"post","link":"https:\/\/www.euvolution.com\/futurist-transhuman-news-blog\/space-station\/voyager-makes-an-interstellar-discovery.php","title":{"rendered":"Voyager Makes an Interstellar Discovery"},"content":{"rendered":"
The solar system<\/span> is passing through an interstellar cloud that physics says should not exist. In the Dec. 24th issue of Nature<\/em>, a team of scientists reveal how NASA<\/a>'s Voyager spacecraft<\/span> have solved the mystery. <\/span> <\/div>

\"see\"Using data from Voyager<\/span>, we have discovered a strong magnetic field just outside the solar system,\" explains lead author Merav Opher<\/span>, a NASA Heliophysics <\/span>Guest Investigator from George Mason University. \"This magnetic field holds the interstellar cloud together and solves the long-standing puzzle of how it can exist at all.\"<\/span><\/p>

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Right:<\/strong> Voyager flies through the outer bounds of the heliosphere en route to interstellar space<\/span>. A strong magnetic field reported by Opher <\/span>et al in the Dec. 24, 2009, issue of Nature is delineated in yellow. Image copyright 2009, The American Museum of Natural History. [larger image<\/a>]<\/span><\/p>

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The discovery <\/span>has implications for the future when the solar system<\/span> will eventually bump into other, similar clouds in our arm of the Milky Way galaxy<\/span>.<\/span><\/p>

Astronomers <\/span>call the cloud we're running into now the Local Interstellar Cloud or \"Local Fluff<\/span>\" for short. It's about 30 light years wide and contains a wispy mixture of hydrogen and helium atoms at a temperature of 6000 C. The existential mystery of the Fluff has to do with its surroundings. About 10 million years ago, a cluster of supernovas exploded nearby, creating a giant bubble of million-degree gas. The Fluff is completely surrounded by this high-pressure supernova exhaust and should be crushed or dispersed by it.<\/span> <\/p>

\"The observed temperature and density of the local cloud do not provide enough pressure to resist the 'crushing action' of the hot gas around it,\" says Opher.<\/span><\/p>

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So how does the Fluff survive? The Voyagers have found an answer. <\/span><\/p>

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\"Voyager <\/span>data show that the Fluff is much more strongly magnetized than anyone had previously suspected—between 4 and 5 microgauss*<\/sup>,\" says Opher. \"This magnetic field can provide the extra pressure required to resist destruction.\"<\/span><\/p>

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\"see<\/a><\/span><\/p>

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Above:<\/strong> An artist's concept of the Local Interstellar Cloud, also known as the \"Local Fluff.\" Credit: Linda Huff (American Scientist) and Priscilla Frisch (University of Chicago) [more<\/a>]<\/span><\/p>

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NASA<\/span>'s two Voyager probes<\/span> have been racing out of the solar system for more than 30 years. They are now beyond the orbit of Pluto <\/span>and on the verge of entering interstellar space—but they are not there yet. <\/span><\/p>

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\"The Voyagers <\/span>are not actually inside the Local Fluff,\" says Opher<\/span>. \"But they are getting close and can sense what the cloud is like as they approach it.\"<\/span><\/p>

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The Fluff is held at bay just beyond the edge of the solar system<\/span> by the sun's magnetic field, which is inflated by solar wind into a magnetic bubble more than 10 billion km wide. Called the \"heliosphere<\/span>,\" this bubble acts as a shield that helps protect the inner solar system from galactic cosmic rays and interstellar clouds. The two Voyagers are located in the outermost layer of the heliosphere, or \"heliosheath<\/span>,\" where the solar wind is slowed by the pressure of interstellar gas<\/span>.<\/span><\/p>

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Voyager <\/span>1 entered the heliosheath <\/span>in Dec. 2004; Voyager 2 followed almost 3 years later in Aug. 2007. These crossings were key to Opher et al<\/em>'s discovery.<\/span><\/p>

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\"see<\/a>Right:<\/strong> The anatomy of the heliosphere. Since this illustration was made, Voyager 2 has joined Voyager 1 inside the heliosheath, a thick outer layer where the solar wind is slowed by the pressure of interstellar gas. [larger image<\/a>] <\/span><\/p>

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The size of the heliosphere is determined by a balance of forces: Solar wind <\/span>inflates the bubble from the inside while the Local Fluff compresses it from the outside. Voyager's crossings into the heliosheath revealed the approximate size of the heliosphere and, thus, how much pressure the Local Fluff exerts. A portion of that pressure is magnetic and corresponds to the ~5 microgauss Opher's team has reported in Nature<\/em>.<\/span><\/p>

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The fact that the Fluff is strongly magnetized means that other clouds in the galactic neighborhood could be, too. Eventually, the solar system will run into some of them, and their strong magnetic fields could compress the heliosphere even more than it is compressed now. Additional compression could allow more cosmic rays to reach the inner solar system<\/span>, possibly affecting terrestrial climate and the ability of astronauts to travel safely through space<\/span>. On the other hand, astronauts wouldn't have to travel so far because interstellar space would be closer than ever. These events would play out on time scales of tens to hundreds of thousands of years, which is how long it takes for the solar system to move from one cloud to the next.<\/span><\/p>

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\"There could be interesting times ahead!\" says Opher<\/span>.<\/span><\/p>

View my blog's last three great articles....<\/span><\/p>