As the sun travels through the galaxy, its extended magnetic bubble (known as the heliosphere), interacts with the gases and magnetism in the space between the stars a vast region known as the interstellar medium. <\/p>\n
However, astronomers have assumed that the heliosphere gets dragged out into a comet-like tail (not too dissimilar to a stretched-out raindrop), shaped by the interstellar medium, but scientists now think the suns magnetic field strength has been underestimated, overturning our understanding as to how our solar system looks from afar. <\/p>\n
VIDEO: Voyager 1 Not Even CLOSE to Leaving Solar System <\/p>\n
The heliosphere reaches far beyond the orbit of Pluto and it is filled with the energetic particles ejected by the sun contained within the solar wind. The suns magnetic field pushes outward with the solar wind, creating a magnetic bubble separating solar plasma from the interstellar medium. A balance of pressure between the outward pressure of the solar wind and the inward pressure of the interstellar medium is reached at the heliospheres boundary, called the heliopause. <\/p>\n
As the sun is moving, it was assumed that the heliopause is being shaped through its interaction with the interstellar magnetic field, but new models and observations suggest that the suns magnetic field is actually dominating its shape. Rather than producing a classical comet-like tail researchers now suggest two tails are formed from jets protruding from the suns north and south poles. <\/p>\n
GALLERY: Voyager 2s Epic Outer Solar System Odyssey <\/p>\n
Everyones assumption has been that the shape of the heliosphere was molded by the flow of interstellar material passing around it, said astronomer Merav Opher, of Boston University, lead author of a paper published in the Astrophysical Journal Letters in February. Scientists thought the solar wind flowing down the tail could easily pull the magnetic fields in the heliosphere along as it flowed by, creating this long tail. But it turns out the magnetic fields are strong enough to resist that pull so instead they squeeze the solar wind and create these two jets. <\/p>\n
Interestingly, other stars in our galaxy have been observed with this two-jet heliosphere morphology, but now the mechanisms behind the two tails are being revealed inside our own solar system. For example, the star BZ Cam, below, exhibits a shortened heliosphere shaped by 2 jets: <\/p>\n
ANALYSIS: Wheres the Edge of the Solar System? Its Complicated <\/p>\n
The revelation that our basic comet-like model of the suns heliosphere was incomplete came when NASAs Voyager 1 probe exited the heliosphere. On measuring the direction of the interstellar magnetic field the first mission ever to do so astronomers were surprised to find it matched the direction of our suns magnetic field, contrary to predictions. <\/p>\n
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Sun May Blast Two Jets of Plasma into Interstellar Space<\/a><\/p>\n","protected":false},"excerpt":{"rendered":" As the sun travels through the galaxy, its extended magnetic bubble (known as the heliosphere), interacts with the gases and magnetism in the space between the stars a vast region known as the interstellar medium. However, astronomers have assumed that the heliosphere gets dragged out into a comet-like tail (not too dissimilar to a stretched-out raindrop), shaped by the interstellar medium, but scientists now think the suns magnetic field strength has been underestimated, overturning our understanding as to how our solar system looks from afar. Continue reading