VOYAGES THROUGH THE HELIOSPHERE
What was Voyager 2's recent discovery?
The supersonic wind from the Sun blows at 400 kilometres per second, and creates a bubble called the heliosphere. We already knew that this wind slows abruptly as it approaches the heliosphere's boundary and comes up against interstellar wind, resulting in a sonic shock. In 2004, Voyager 1 crossed that shock in the northern part of the Solar System at about 94 astronomical units (AU). [1 AU is the distance from Earth to the Sun.] Then, in 2007, Voyager 2 crossed the shock at 84 AU in the southern Solar System. So the heliosphere must be asymmetrical. This is probably due to an interstellar magnetic field pushing inwards more in the south than the north.
Did the shock crossing hold surprises?
Yes. We expected the solar wind ions to be heated, possibly to 1,000,000 °C, by the kinetic energy generated when the wind suddenly slows. Instead, the bulk of the kinetic energy heated interstellar ions in the heliosheath -- the outer layer of the heliosphere. These data also suggest that the shock is dynamic and constantly reforms itself, rather than being a stable, permanent structure as most models assume.
Why is it important to map the heliosphere?
The complex interaction between the solar wind -- which changes during the solar cycle -- and material outside the Solar System determines how large the bubble is and how well we are protected from galactic cosmic rays in interstellar space.
Has Voyager surpassed expectation?
Yes. We hoped to reach interstellar space, but didn't know how long it would take or how long the spacecraft would last. They have enough power to last until 2025. Models suggest that Voyager 1 will reach interstellar space first, in about 5–10 years. But we don't know how thick the heliosheath is, nor how strongly the interaction with the interstellar wind affects the solar wind.
INTERNATIONAL WEEKLY JOURNAL OF SCIENCE
ISSUE 454, xi (July 3, 2008)