<p>We can't see the core, but we can see deeper into the photosphere of the sun. The deeper layers of the photosphere are hotter and brighter, and this is the cause of limb darkening.</p>

CC BY-SA 4.0
2018-07-03T13:36:42.430Z
To add up on that, this figure might help the readers understand more: https://www.google.com/url?sa=i&rct=j&q=&esrc=s&source=images&cd=&cad=rja&uact=8&ved=2ahUKEwjVqNmVhoPcAhUn6oMKHT_jBYsQjRx6BAgBEAU&url=https%3A%2F%2Fen.wikipedia.org%2Fwiki%2FLimb_darkening&psig=AOvVaw2IuNuBqaRHhxZC_B5PCDJz&ust=1530711308674832
Kornpob Bhirombhakdi
CC BY-SA 4.0
2018-07-03T13:39:10.770Z
According to the figure, you can only see deep from the real surface of the sun up to the distance L. So, looking directly to the center of the sun gives you looking deeper (drawing a circle with different radii from the center of the sun) inside the surface, therefore hotter and brighter.
Kornpob Bhirombhakdi
CC BY-SA 4.0
2018-06-28T20:24:45.430Z
2018-06-28T20:24:45.430Z
James K
<p>The visible surface of the Sun is defined by that location within the Sun's atmosphere from which photons produced in the gas can escape towards the Earth. That location is determined by the amount of gas <em>between</em> it and the Earth, since that gas would reabsorb photons if there were enough of it.</p>

<p>Now you need to think about the geometry of a roughly, spherically symmetric Sun.  When we look at the solar centre, photons can escape from a certain layer in its interior. That layer is nowhere near the core of the Sun, it is the solar photosphere at a temperature of approximately 6000K and at a radius of $6.96\times 10^8$ m from the centre.</p>

<p>Now imagine looking towards the limb. The same quantity of intervening gas is reached by the time you get to a layer in the Sun that is at a larger radius than at the solar centre. Because the temperature decreases as you move outwards in the solar photosphere, this layer is cooler and has a lower surface brightness (surface brightness is proportional to $T^4$). As a result, the solar centre looks hotter and brighter than the limb of the Sun.</p>

CC BY-SA 4.0
2018-06-29T07:30:52.327Z
2018-06-29T07:30:52.327Z
ProfRob
<p>Is <a href="https://en.wikipedia.org/wiki/Limb_darkening" rel="nofollow noreferrer">limb darkening</a> of the Sun because at centre we are directly looking the core and different zones, whereas at limbs we are seeing only the photospheric part (and less beneath photospheric part)? Or there is some other physics behind this phenomenon?</p>

CC BY-SA 4.0
2018-06-29T15:50:06.440Z
I don't understand. What is 'Limb Darkening?'
Andrew Johnson
CC BY-SA 4.0
2018-06-30T02:25:50.653Z
When you look at sun, the limb (edges) of sun appears darker than then other part. That is limb darkening.
Kartik Chhajed
<the-sun>
Is Limb Darkening because at centre we are directly looking core, whereas at limbs we are seeing only photospheric part?
Kartik Chhajed
# Is Limb Darkening because at centre we are directly looking core, whereas at limbs we are seeing only photospheric part?

(Asked by: username_0 on 2018-06-28)

Is [limb darkening](https://en.wikipedia.org/wiki/Limb_darkening) of the Sun because at centre we are directly looking the core and different zones, whereas at limbs we are seeing only the photospheric part (and less beneath photospheric part)? Or there is some other physics behind this phenomenon?

**Tags:** the-sun
> **Comments:**
> **username_1**: I don't understand. What is 'Limb Darkening?'  
> **username_0**: When you look at sun, the limb (edges) of sun appears darker than then other part. That is limb darkening.  

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## 2 answers

### Answer by username_2 on 2018-06-28. Score: 2

We can't see the core, but we can see deeper into the photosphere of the sun. The deeper layers of the photosphere are hotter and brighter, and this is the cause of limb darkening.

> **Comments:**
> **username_3**: To add up on that, this figure might help the readers understand more: https://www.google.com/url?sa=i&rct=j&q=&esrc=s&source=images&cd=&cad=rja&uact=8&ved=2ahUKEwjVqNmVhoPcAhUn6oMKHT_jBYsQjRx6BAgBEAU&url=https%3A%2F%2Fen.wikipedia.org%2Fwiki%2FLimb_darkening&psig=AOvVaw2IuNuBqaRHhxZC_B5PCDJz&ust=1530711308674832  
> **username_3**: According to the figure, you can only see deep from the real surface of the sun up to the distance L. So, looking directly to the center of the sun gives you looking deeper (drawing a circle with different radii from the center of the sun) inside the surface, therefore hotter and brighter.  

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### Answer by username_4 on 2018-06-29. Score: 1

The visible surface of the Sun is defined by that location within the Sun's atmosphere from which photons produced in the gas can escape towards the Earth. That location is determined by the amount of gas *between* it and the Earth, since that gas would reabsorb photons if there were enough of it.

Now you need to think about the geometry of a roughly, spherically symmetric Sun. When we look at the solar centre, photons can escape from a certain layer in its interior. That layer is nowhere near the core of the Sun, it is the solar photosphere at a temperature of approximately 6000K and at a radius of $6.96\times 10^8$ m from the centre.

Now imagine looking towards the limb. The same quantity of intervening gas is reached by the time you get to a layer in the Sun that is at a larger radius than at the solar centre. Because the temperature decreases as you move outwards in the solar photosphere, this layer is cooler and has a lower surface brightness (surface brightness is proportional to $T^4$). As a result, the solar centre looks hotter and brighter than the limb of the Sun.


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