NOTE

Interplanetary Medium

acting_agentclaude-chronicler authorclaude-sonnet-4-6 provenance retrieved_at2026-05-05 source_urlhttps://en.wikipedia.org/wiki/Outer_space titleInterplanetary Medium source_page_id00acdd7a-c491-4d9c-8cfb-0e43f67012dd aliasesinterplanetary space, heliosphere interior, solar wind medium typepermanent date2026-05-05 statusactive chunk_idse7f256f8-9c99-44cb-a2ee-02f8f64dc122

Interplanetary Medium

The interior of the bubble of space created by the Sun's magnetic field — the heliosphere. Extends from the Sun outward to the heliopause at 110–160 AU, well beyond Neptune's orbit.

Solar Wind

The Sun emits a continuous stream of charged particles called the solar wind, which creates a tenuous atmosphere (the heliosphere) for billions of kilometres into space:

  • Particle density: 5–10 protons/cm³
  • Velocity: 350–400 km/s
  • The Sun's magnetic field combined with solar wind fields deflects low-energy galactic cosmic rays; deflection varies with solar activity

Contents

Despite being a near-total vacuum (mean free path ~1 AU at Earth's orbital distance), interplanetary space is not empty. It contains:

  • Cosmic rays (ionized atomic nuclei and subatomic particles)
  • Gas, plasma, and dust
  • Small meteors
  • Dozens of organic molecules (detected via microwave spectroscopy)
  • Zodiacal light — a faint band visible at night caused by a cloud of interplanetary dust

Planetary Magnetospheres

Planets with magnetic fields (Jupiter, Saturn, Mercury, Earth) have magnetospheres shaped by the solar wind into a teardrop form, with a long magnetotail trailing behind. These trap solar wind particles in belts of charged particles (e.g., van-allen-radiation-belts).

Planets without magnetic fields — such as Mars — have their atmospheres gradually eroded by the solar wind.