Heliosphere - Bow Shock

Bow Shock

By 2012, it was determined the Sun has no bow shock. Before then, it was hypothesized that the Sun had a bow shock produced in its travels within the interstellar medium (see image). The shock is named from its resemblance to the wake left by a ship's bow and is formed for similar reasons, though of plasma instead of water. Bow shocks will occur if the interstellar medium is moving supersonically "toward" the sun, since its solar wind moves "away" from the sun supersonically. When the interstellar wind hits the heliosphere it slows and creates a region of turbulence. NASA's Robert Nemiroff and Jerry Bonnell believed the solar bow shock may have lain at around 230 AU

This phenomenon has been observed outside our solar system by NASA's orbital GALEX telescope. The red giant star Mira in the constellation Cetus has been shown to have both a cometlike debris tail of ejecta from the star and a distinct bow shock preceding it in the direction of its movement through space (at over 130 kilometers per second).

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