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The interplanetary medium (IPM) or interplanetary space consists of the mass and energy which fills the Solar System, and through which all the larger Solar System bodies, such as planets, dwarf planets, asteroids, and comets, move. The IPM stops at the heliopause, outside of which the interstellar medium begins. Before 1950, interplanetary space was…
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interplanetary medium solar wind vacuum space magnetic particles sun earth dust field planets heliopause plasma magnetosphere 100 also distance temperatures
| Subject | Predicate | Object | Confidence | Src |
|---|---|---|---|---|
| Interplanetary medium | is a | plasma | 0.90 | text |
| coronal mass ejections | instance of | and may be affected by magnetic fields and solar activity events | 0.80 | text |
| the Moon have no magnetic field | instance of | Bodies | 0.80 | text |
| the solar wind can impact directly on their surface | instance of | Bodies | 0.80 | text |
| Interplanetary medium | related to Composition and physical characteristics | The | 0.60 | section |
| Interplanetary medium | related to Composition and physical characteristics | Sun | 0.60 | section |
| Interplanetary medium | related to Composition and physical characteristics | Typical | 0.60 | section |
| Interplanetary medium | related to Composition and physical characteristics | In | 0.60 | section |
| Interplanetary medium | related to Composition and physical characteristics | Earth | 0.60 | section |
| Interplanetary medium | related to Composition and physical characteristics | For | 0.60 | section |
| Interplanetary medium | related to Composition and physical characteristics | Joseph Fourier | 0.60 | section |
| Interplanetary medium | related to Composition and physical characteristics | Earth's | 0.60 | section |
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