Sky science
Heliopause
Direct answer
Heliopause: The Heliopause is the boundary region where outward solar-wind pressure balances the surrounding interstellar medium.
It is the outer plasma boundary of the heliosphere.
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At a glance
- Found in
- Astronomy & Skywatching
- Related
- Solar Wind, Heliosphere, Planetary Magnetosphere, Van Allen Radiation Belts
It is the outer plasma boundary of the heliosphere.
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The story behind Heliopause
Voyager 1 and Voyager 2 supplied the first in-situ crossings of the heliopause.
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The Wandering Stars
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Why Heliopause matters
Heliopause marks a transition from solar-wind plasma to interstellar conditions.
Heliopause in practice: an example
A rise in galactic cosmic rays helped identify Voyager’s transition into interstellar space.
Where readings of Heliopause go wrong
Crossing the heliopause does not mean escaping the Sun’s gravity or Oort Cloud.
Sources and editorial method
Research references used for this entry include:
- NASA Science: The Sun - NASA reference for solar structure, activity, the solar wind, and heliophysics.
- NASA Science: Solar System Exploration - NASA overview of planets, moons, small bodies, rings, and the structure of the Solar System.
- Source
- The Great Almanac Dictionary
- Category
- Astronomy & Skywatching
- Last updated
- 2026-09-26
Understand the heliopause crossing
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More in Astronomy & Skywatching
- Magnification
- Periapsis
- Rayleigh Criterion
- Solar Elongation
- Tidal Locking
- Apoapsis
- Barycenter
- Ecliptic
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Common questions
What is the Heliopause?
The Heliopause is the boundary region where outward solar-wind pressure balances the surrounding interstellar medium.
What do people get wrong about the Heliopause?
Crossing the heliopause does not mean escaping the Sun’s gravity or Oort Cloud.
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