Well, at least that’s what we know. What if these magnetic fields around stars are not visible? How do scientists study these?

Bride, Let’s answer.

Radio waves, a form of electromagnetic radiation, share properties with visible light.

But these waves have longer wavelengths and lower frequencies. These properties allow radio waves to navigate through the vast expanses of space to penetrate even the densest cosmic clouds makes it quite convenient.

Radio waves, unlike visible light, can be scattered or absorbed by interstellar dust and gas It can navigate through dust and cloud particles. Astronomers study these gases at radio wavelengths to understand the role of dust in various astrophysical events.

Furthermore, although magnetic fields cannot be observed directly, they have a major influence on how charged particles behave in space.

This interaction between magnetic fields and charged particles provides scientists with a useful way to study them. In addition, charged particles from the sun’s own wind Interacts with the Earth’s magnetic field and these particles follow the lines of the magnetic field and sometimes hit gases in our atmosphere.

When this event occurs, there are both visible lights and things you cannot see. radio lights that we can detect with special devices or instruments They produce. These lights show us how magnetic fields work.

In addition, magnetic fields around stars and other cosmic objects can trap charged particles.

Furthermore, these particles emit light as they move along these magnetic paths. also to this called synchrotron radiation and occurs when charged particles are highly accelerated under the influence of strong magnetic fields.

While following magnetic field lines, including radio waves They emit radiation with different wavelengths.

In summary; radio astronomy and spectroscopy Tools and methods like these help scientists study hidden magnetic fields around stars.

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