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Curious Kids: why is the Sun’s atmosphere hotter than its surface?

31 Aug 2021

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Why is the Sun’s atmosphere hotter than its surface? — Olivia, age 9, Canberra

Hi Olivia, that’s a great question! In fact, it’s such a great question many scientists around the world are trying to answer it.

The truth of the matter is — we don’t know! But we do have some ideas about where the energy that heats the Sun’s atmosphere might be coming from, and it has a lot to do with the Sun’s magnetic field. Let me explain what this means.

The temperature of the Sun

Heat is created in the very centre of the Sun, at its core, where the temperature is a blistering 27 million degrees Celsius. And just like walking away from a campfire, the temperature gets cooler further away from the core.

The temperature of the Sun’s surface is about 6,000?, which means it’s much cooler than the core. Also, it continues to cool down for a short distance above the surface.

But higher above the surface, in the atmosphere, the temperature suddenly shoots up to more than a million degrees! So there must be something that’s heating the Sun’s atmosphere. But we can’t easily find out what it is.

The key is the Sun’s magnetic field

The leading idea among experts is the Sun’s magnetic field is actually bringing energy from inside the Sun up through its surface and into its atmosphere.

Like Earth, the Sun has a magnetic field. We can imagine a magnetic field as invisible lines connecting the North and South poles of a star or planet.

We can’t see magnetic fields, but we know they are there because we have objects that react to them. For example, a compass needle on Earth will always point to the North pole because it lines up with Earth’s magnetic field.

Here you can see how Earth’s magnetic field extends out into space and loops back. The red end is the North magnetic pole and the white end is the South pole. Shutterstock

While the Sun also has a North and South pole, its magnetic field behaves differently to Earth’s and looks a lot messier. At the surface of the Sun, the magnetic field lines look like many loops rising up out of the surface into the atmosphere — and these loops are changing all the time.

If the loops touch each other they can cause sudden explosions of enormous amounts of energy that heat up the atmosphere. We also know there are waves travelling along the magnetic field lines bringing energy up. Could they be responsible for heating the atmosphere?

Is it a combination of the waves and the explosions, or something else altogether? Being able to measure the Sun’s magnetic field would really help us understand what’s going on.

This is what we think the Sun’s magnetic field lines might look like if we could see them coming up from its surface. NASA

Measuring the magnetic field

Magnetic fields may be invisible, but we can still measure them because they make small changes to the light that comes from the Sun. The surface of the Sun is very bright, so it’s easy to see changes in the light coming from the surface, and measure the magnetic field there.

But the Sun’s atmosphere is so hot the light there is not visible anymore. Rather it makes X-rays, which are a type of light we can’t see! Even if we use special X-ray telescopes, the X-rays from the Sun’s atmosphere are too dim for us to figure out what the magnetic field in the atmosphere looks like.

The good news is there is a brand new satellite, NASA’s Parker Solar Probe, which is now orbiting close to the Sun (but not too close) and actually flying through the magnetic field to measure it. We should be receiving a lot of exciting new information from it over the next five years.

These magnetic field measurements will bring us closer to understanding what is making the atmosphere of the Sun, and other stars, much hotter than their surface.

NASA’s Solar Parker Probe is about the size of a car. NASA

Read more: Curious Kids: how does the Sun make such pretty colours at sunsets and sunrises?


The authors do not work for, consult, own shares in or receive funding from any company or organisation that would benefit from this article, and have disclosed no relevant affiliations beyond their academic appointment.


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This content was originally published by The Conversation. Original publishers retain all rights. It appears here for a limited time before automated archiving. By The Conversation

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