Space Topics: Voyager
The Interstellar Mission
When Voyager 2 passed by Neptune in 1989, the mission had run out of planets
to visit. But both spacecraft were on courses that would eventually
escape the solar system entirely. In 1990, the Voyager mission was extended
again, and the planetary explorers turned into interstellar explorers, and
the Voyager Interstellar Mission began.
While the Voyagers were beyond the orbits of all the planets, they were still
and are still well within the realm of the Sun’s magnetic field or heliosphere.
Often described as a “bubble” blown up by a supersonic, solar
wind of electrically-charged particles coming from the Sun’s atmosphere,
the heliosphere extends far beyond the orbit of the outermost planet, which
sometimes is Pluto and sometimes Neptune, and out to the farthest reaches
of the Sun’s magnetic field.
Scientists believe that the heliosphere’s boundary or heliopause – the
region between the heliosphere and interstellar space, where the spacecraft
are headed now -- fluctuates with the varying strengths of the solar wind
during the 11-year cycle of the Sun’s maximum and minimum atmospheric
flux. Beyond the heliosphere is interstellar space, where particles from exploded
stars and other materials float and soar.
Voyagers at the edge of the solar system
Our solar system exists inside a heliosphere, a bubble created by the outward flow of the solar wind. The region that separates our system from interstellar space is the heliopause. In between these is the termination shock, where the solar wind slows from supersonic to subsonic speeds.
Credit: JPL / NASA
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The Voyager spacecraft have four instruments that can measure the solar wind:
the plasma subsystem; the magnetometer, which measures the magnetic fields
carried out into interplanetary space by the solar wind; the planetary radio
astronomy subsystem; and the ultraviolet spectrometer subsystem. Where the
mission once commanded personnel numbering around 600, only 10 scientists
and engineers now man the mission. Continuing funding cuts may further reduce
staff, leaving those who remain to figure new and perhaps riskier ways to
carry on.
On December 17, 2004, Voyager 1 reached the “termination shock,” the
beginning of the heliopause. (As the solar wind approaches the heliopause it
must slow down from millions to 400,000 kilometers per hour (250,000 miles per
hour); this abrupt change is the termination shock.) Five to 20 years after
reaching the termination shock, Voyager 1 should reach the heliopause. But
it’s a race against time. If they make it -- and we still have contact
before their power is spent -- they could return data not only from the
heliopause, but perhaps taste the interstellar space environment to reveal
some of the particles from other stars. It would be the crowning achievement
of a remarkable voyage.
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