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Astrophysics & Cosmology FAQ

The solar wind is composed of:

Charged particles (mostly protons and electrons) streaming from the Sun. The solar wind is a continuous outflow of charged particles (plasma) from the Sun's outer corona at ~400–800 km/s.

Short Answer

Charged particles (mostly protons and electrons) streaming from the Sun is the best answer.

Astrophysics questions often combine observation with first-principles physics. The winning move is to connect the measurement being made, such as luminosity, spectrum, redshift, or orbit, to the physical model behind it.

The solar wind is a continuous outflow of charged particles (plasma) from the Sun's outer corona at ~400–800 km/s.

Why This Answer Is Correct

This is a Medium-level question in Astrophysics & Cosmology. The prompt is really testing whether you can connect the concept to its defining physical relationship instead of picking a nearby-but-wrong term.

Good astrophysics reasoning always asks what the telescope actually measured and what physical quantity that measurement traces.

Choices At A Glance

  • A. Neutrons and protons
  • B. Photons only
  • C. Charged particles (mostly protons and electrons) streaming from the Sun
  • D. Solar neutrinos

When similar options appear on an exam, eliminate the ones that break the core law, use the wrong units, or confuse a definition with a consequence.

Topic Snapshot

Topic: Astrophysics & Cosmology

Difficulty: Medium

Best next move: Re-state the governing law in your own words, then solve one more example from the same topic before moving on.