The position of NASA's Voyager 1 and Voyager 2 probes, outside of the
heliosphere, a protective bubble created by the Sun that extends well past the orbit of Pluto, is shown in this NASA/JPL-Caltech illustration.
While the probes have left the
heliosphere, Voyager 1 and Voyager 2 are yet to leavethe solar system and won't be leaving anytime soon either.
In the ram direction the outer boundary of the
heliosphere is compressed, whereas in the opposite direction the
heliosphere is stretched out into an elongated tail.
"Instead of a prolonged, comet-like tail, this rough bubble-shape of the
heliosphere is due to the strong interstellar magnetic field-much stronger than what was anticipated in the past-combined with the fact that the ratio between particle pressure and magnetic pressure inside the heliosheath is high," said Kostas Dialynas, a space scientist at the Academy of Athens in Greece and lead author on the study.
Since then, scientists have eagerly anticipated the probes' departure from the
heliosphere, the bubble of particles that encircles the sun and planets, and their entry into the unexplored space between stars.
Some scientists have said that the spacecraft was still within the
heliosphere, the region of space dominated by the Sun and its wind of energetic particles and has not yet reached the space between the stars.
After much debate, data at last persuaded scientists that the car-size spacecraft had slipped outside the
heliosphere, a huge bubble of particles blown out by the sun.
space agency scientists now agree that Voyager is officially outside the protective bubble known as the
heliosphere that extends at least 13 billion kilometers beyond all the planets in our solar system, and has entered a cold, dark region known as interstellar space.
Scientists have been waiting for years for a signal from Voyager 1announcing that it had left the solar system and reached interstellar space as it explored the boundary region known as the
heliosphere.
His topics include radiative transfer in the sun's atmosphere, the dynamics of solar plasmas, observations of photospheric activity and magnetism, the solar wind and
heliosphere, and influences of solar variability on Earth.