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There is no close-up image of the heliosphere. The 3D model shows an artist’s impression.

Region at the edge of the Solar System

Heliosphere

The Sun is always puffing tiny particles out into space – the solar wind. It blows a giant, invisible bubble around the whole Solar System. This bubble is called the heliosphere. Only the two Voyager probes have flown out of it so far.

▶ View the heliosphere in the 3D model

Fact file

Type
Region at the edge of the Solar System

Interesting facts about the heliosphere

Formation

The solar wind races outwards at 400 to 800 km/s until it meets the thin gas between the stars. There it is slowed down and piles up.

Structure

At about 90 AU the solar wind slows abruptly (termination shock); at about 120 AU it comes to an end (heliopause). Because the Sun is moving through the Milky Way, the bubble is probably not round but has a kind of tail.

Exploration

The Voyager probes measured the boundary directly: particles from the solar wind suddenly became rarer, those from the Milky Way more common. NASA's IBEX probe maps the boundary from Earth orbit.

Importance for Earth

The heliosphere protects us like a shield from a large part of the cosmic radiation coming from the Milky Way.

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