This is Parker Solar Probe

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Information about Parker Solar Probe

Why do we study the solar wind and the Sun?

Scientists want to understand how the sun works

The Sun is the source of the solar wind; a flow of gases from the Sun that streams past Earth at speeds of more than 500 km per second (a million miles per hour).

Solar winds

Disturbances in the solar wind shake Earth's magnetic field and pump energy into the radiation belts.

Space weather and sattelite lifetime

This "Space Weather" can change the orbits of satellites and shorten their lifetimes. Shaking Earth's magnetic field can also cause surges in power lines that destroy equipment and knock out power over large areas.

Three important discoveries that Parker Solar Probe has made

  • Alfvén critical surface – the boundary where solar material anchored to the Sun first escapes and becomes the solar wind.

  • Corona layer has spikes and valleys that wrinkle the surface.

  • formation of solar winds from giant plums and solar materials.

  • The sound of the sun was recorded for the first time.

  • Trajectory of magnetic fields was discovered first time ever

    • Challenges that Parker Solar Probe faced.

  • Dust zone around the sun was much denser, which can caused more damage than was planned.

  • Extreme temperature over 1500 degrees Fahrenheit.

  • The Parker Solar Probe is millions km away from the earth and it would be impossible to fix the malfunctions immediately.

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