Outer edge of solar system
The outer structure of the heliosphere is determined by the interactions between the solar wind and the winds of interstellar space. The solar wind streams away from the Sun in all directions at speeds of several hundred km/s in the Earth's vicinity. At some distance from the Sun, well beyond the orbit of Neptune, this.
The heliosphere is the , , and outermostlayer of the . It takes the shape of a vast, tailed bubble-like . In plasma physics terms, it is the cavity formed by the Sun.
The heliopause is the final known boundary between the heliosphere and the interstellar space that is filled with material, especially plasma.
The heliosphere is the area under the influence of the Sun; the two major components to determining its edge are theand thefrom.
The heliosphere is thought to change significantly over the course of millions of years due to extrasolar effects such as closeror the traversingof.
Despite its name, the heliosphere's shape is not a perfect sphere.Its shape is determined by three factors: the interstellar medium (ISM), the.
Detection by spacecraftThe precise distance to and shape of the heliopause are still uncertain. Interplanetary/interstellar .
• 1904: Astronomers using thewith afind evidence of thewhile observing the binary starin .
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