You might have heard that when you look up at the night sky, you see back in time. This is because stars are very far away from us and it takes starlight a very long time to reach the Earth.
The closest star to the Sun, Proxima Centauri, is 4.2 light years away. That means the light from this star has to travel 4.2 years before we get to see it.
Some other stars that you might know and recognize in the sky are even further away, their light is even older!
✨ Polaris, also known as The North Star, is 433 light years away. When we look at Polaris, we see the star as it was 433 years ago, the year Mary, Queen of Scots was executed.
What’s the farthest star you can see?
The debate on what is the farthest star you can see with an unaided eye is still ongoing. This question, believe it or not, is surprisingly difficult to answer, and here is why:
- It’s very tricky to measure stellar distances, especially for aging stars, like supergiants
- Many stars that appear to our eye as single points of light, are in fact, multiple star systems
- Some stars out there are variable stars, meaning their brightness changes over time
- ‘Seeing’ faint objects depends on the sky conditions and how good one’s eyesight is
What is the farthest star YOU have seen with your eyes?
The journey of the Sunlight
All these stars, even the nearest ones, are extremely distant. In comparison, our own Sun is [on average] only 93 million miles away from the Earth. The sunlight travels at…well…the speed of light [186 000 miles per second], and takes about 8 minutes and 20 seconds to cover that vast distance. But does that mean the sunlight we see is 8 minutes and 20 seconds old?
The sunlight is made up of tiny “packets of light” called photons, that originate in the Sun’s core. The photons are born in a nuclear fusion, when hydrogen cores smash together to make helium. As a byproduct of this reaction, a huge amount of energy is released in the form of photons. But those are not visible light photons, not the kind of light our eyes can see, but high energy gamma-ray photons. The gamma-ray photons will turn into visible light much later, when they lose a lot of energy on their 433 000 mile /700 000 kilometer long way out of the Sun.
The structure of the Sun
The Sun is composed of different layers, like an onion. The hottest and the densest part of the Sun is the core. There, a huge amount of matter, about ⅓ of the total mass of the Sun, is concentrated in a volume that extends from the centre to about ⅕ of the Sun’s radius. This is where all the nuclear fusion magic happens.
Surrounding the core is the radiative zone. It extends from 0.2 to 0.7 solar radii. As we move through the radiative zone, the temperature drops by about an order of magnitude, from 15 million degrees C in the core to to 2 million degrees C on the outer edge of the radiative zone. The density drops too.
Further out is the convective zone. It extends all the way to the visible surface. Radiative and convective zones got their names from the way the energy is being transferred through each zone, i.e. radiation and convection.
In between the two zones is tachocline, a thin [but very important] interface area. Astronomers think that this is where the Sun’s magnetic field originates
Finally, the outermost part of the Sun is the atmosphere. It’s made of different layers too.
So how does a photon travel through these layers?
☀️ When a gamma-ray photon is born in the Sun’s core, it begins its journey to the surface. But our photon doesn’t make it far because things are very crowded in the radiative zone. After moving a minuscule distance, the photon collides with a ‘solar stuff’ particle (hydrogen or helium), bounces off in a different direction, then collides with another particle and so on. Our photon loses a lot of energy to these collisions, becoming first X-ray and then UV photon. Through this continuous random bouncing back and forth (no wonder that mathematically this problem is known as random walk), up to a million years after it was born, our photon finally enters the convective zone.
☀️ In the convective zone things are way less hot and dense. The hot plasma here bubbles, the hot ‘stuff’ rises to the surface, cools down and sinks, just like water in a kettle. Our photon hitches a ride in one of these bubbles up to the visible surface. Now it’s free!
☀️ The final leg of the journey to the Earth our -now a visible light- photon travels in a straight line in just over 8 minutes.
But this is still only half of the story
The sunlight we see is 170 000 years and 8.5 minutes old. It is ancient!
But not to the photons themselves. You see, according to Einstein, the closer to the speed of light you travel , the more the time dilates ( i.e. the slower your clock ticks) and the more the lengths contract. Ultimately, for a photon that travels…well… at the light speed, the fastest speed there is, there is no time and no distance. In other words, photons have no age and they do not experience time. To them, entering your eye happens instantaneously after their birth – no thousands of years of bouncing, no huge distance from the Sun traveled! Isn’t that amazing?
Did you enjoy this post? Here are some other cool posts about the Sun