Hi, welcome to my tour of the Solar System. The first chapter of the tour was last month, which woefully described why the tour is taking place and where we would go. But hey, the tickets are free, even though the tour guide is not officially affiliated with any tour group.

For our first expanded stop on the tour, we’re starting with the main attraction: The Sun. It’s always there, very dependable, just like an ideal boyfriend/girlfriend; but what do we really know? Short of Facebook stalking, we actually know quite a bit about the Sun. Let’s start with covering some information about everybody’s favourite natural fusion reactor.

The Sun is crucial to developing and maintaining life on our little ball of happiness. The Earth receives light and heat from the Sun; but it also powers photosynthesis in plants, the climate, weather, and ocean currents. Without the Sun, life on Earth would be like Frankenstein’s monster, without Frankenstein; because Frankenstein and the Sun both bring life. Except I don’t think the Sun has ever had one of its creations, sneak into a bedroom and strangle a bride on her wedding night. Yet.

I’ve said this before, but the Sun is actually a star. It’s like the trick question you get asked, “What’s the closest star to Earth?” So your answer could be, “Proxima Centauri.” If it was, you would be wrong…because, say it with me, the Sun is a star!

If you’re on a first or second date, you might suggest a walk together in starlight. Your date will probably correct you, by replying it’s daylight outside and the stars are not visible. You can then calmly mention that the sunlight that we are experiencing is produced by the Sun; the Sun is a star; stars produce starlight; so therefore, we are walking in starlight. Your coolness and hotness factors will increase exponentially; like a geek.

The Sun is known as a yellow dwarf G-type main sequence star. Scientists are extremely clever and innovative people, but sometimes they can come up with some pretty bizarre names for things. If you saw that name on a Tinder profile, I’m sure you would be swiping left, but let’s look at the name and what it means.

Spoiler alert, but names tell you exactly what things actually are and what they do. Just like a green toaster, is a machine that’s green and toasts bread, or a book called, Pride and Prejudice, features two main characters that experience both pride and prejudice, or a man that dresses like a bat is called Batman, or a Horseshoe crab that…wait a minute.

There are many ways to describe main sequence stars in far better scientific terminology, than from a man that describes Azure, Royal Blue and Navy Blue, as Light Blue, Blue and Dark Blue, respectably.

A main sequence star is a star that crushes hydrogen atoms together, to form helium atoms in the star’s core. This is known as nuclear fusion, because it involves the fusion of atoms. It’s this process that releases the energy to make the star stable. This energy is pushing outwards, and it counteracts the force of gravity, which is trying to collapse the star. The Sun finds equilibrium through this, allowing it to continue to fuse atoms and release energy.

Let’s look at the G-type part now. Stars can be graded based on various factors using Stellar classification. These factors can include spectral characteristics, temperature, mass, luminosity and absolute magnitude. This puts our burning ball of hydrogen near the centre of the classification system; which is a G-type star. Not too hot, not too cool, it’s just right.

As for the another part of the name, yellow dwarf, the Sun is neither. It’s not a dwarf, because the Sun is about 1,392,700 km (865,000 miles) in diameter; which is 109 times the size of the Earth. That also means about 1 million Earths would fit inside the Sun. As for the mass, the Sun is estimated to be 1.989 x 10³⁰ kilograms. That’s a strange looking number, but what it means is that the Sun’s mass is 300,000 times that of Earth. There are other stars in the universe much larger than the Sun, but that is another story for another day.

Continuing with breaking your perception of our local star, the Sun is not yellow or orange. Yes, yes, I know yellow is in the name; but that doesn’t mean it’s accurate. Hey, Science, is a Horseshoe crab actually a crab? Hollywood and nearly every picture book have been lying to you, for your entire life. I’m very sorry, but the colour of the Sun is actually white.

So how do we know that the Sun is white? The Sun produces a lot of different light, which is a type of radiation; which in turn, is part of the electromagnetic spectrum. The Suns emits radio waves at different frequencies, as well as microwaves, infrared waves, visible light, ultraviolet waves, and X-rays; but not gamma rays. Gamma radiation is very different, just ask Bruce Banner.

One way to explain this, is that if you have ever played with a prism, witnessed a rainbow in the sky or seen The Dark Side of the Moon album cover by Pink Floyd, you’ll understand that visible light can be broken up into separate colours; violet, indigo, blue, green, yellow, orange and red. All of these colours have different wavelengths.

When visible light passes through a medium and changes direction, this is called refraction. When visible light is split into the colour spectrum, this is called dispersion. In nature, visible light is being emitted from the Sun; so visible light contains all of the colours of the rainbow. And this works in reverse, because just like Captain Planet, when you combine all of the colours of the rainbow, you make white light. And this is a key point: visible light is white light. Visible light is sunlight, which is created by the Sun. So if visible light is white light, and white light is created by the Sun…the colour of the Sun is white.

I’m sure someone a lot smarter than me could do a better job at explaining this concept, but I don’t get paid for this, so I can’t hire any scientists to write this for me. Are you impressed with the Sun yet? No? Alright, let’s do some more!

The Sun is about 150 million km (93 million miles) from the spinning sphere of delight known as Earth. This distance is actually known as an astronomical unit (AU), which is the mean distance between the centre of the Sun and the centre of the Earth. This doesn’t mean that it’s always that distance, because both the star and the planet are moving through spacetime.

The Sun is pretty jacked too. It makes up 99.8% of all the mass in the solar system! Because of this, it never misses leg day. It’s also made of gas and plasma; which is the fourth state of matter, after gas, liquid and solid.

You may have heard that the Sun is old. Not as old as Mr. Burns from The Simpsons, but still pretty old. The Sun is about 4.6 billion years old. Let that sit with you for a moment. 4.6 billion years old. That is mind crushing; but just to dial it up to 11, the Sun is only half way through its life span.

For the interior of the Sun, a visit there would be…unpleasant, if you could stay there for any length of time. The Sun’s mass is made up of 70.6% hydrogen, 27.4% helium and 2% heavy elements like oxygen, nitrogen, carbon, neon, iron and others.

The Sun also has six different layers, which include the corona, which stretches 8 million km (5 million miles) above the Sun’s surface; the chromosphere, which is 400 km (250 miles) and 2100 km (1300 miles) above the solar surface; the photosphere, which is from the surface to about 400 km (250 miles) above that; the convective zone, this zone extends from a depth of about 200,000 km right up to the visible surface; the radiative zone, which has a depth of 515,000 km to 200,000 km; and the core, which is 170,000–140,000 km in depth (106,000-87,000 miles).

As you would expect the temperatures; just like the prices at the corner shop for ice cream, vary a lot. The temperatures are between 6,000 °C (11,000 °F) to 4,000 °C (7,200 °F) in the chromosphere; about 5,500 °C (10,000 °F) in the photosphere; about 2 million °C (4 million degrees °F) in the convective zone; between 7 million °C (12 million degrees °F) to around 2 million °C (4 million degrees °F) in the radiative zone; with 15 million degrees °C (27 million degrees °F) in the core.

With the corona, the temperatures range from 1 to 2 million °C (1.8 million to 3.6 million °F). This is interesting, because it means the upper atmosphere of the Sun, is actually 500 times hotter than the surface. Scientists are still trying to figure this out, along with why a Saiyan’s hair is always so perfect.

On a more serious note, I want to talk about the sheer power of the Sun and what it can actually do. We know that in the Sun’s core, the pressure and temperature is so high, it can fuse atoms together. When this happens, it releases a huge amount of energy.

To understand this, every second, of every single day, the Sun’s core fuses about 600 million tons of hydrogen into helium, which converts 4 million tons of matter into energy. This nuclear reaction is the energy equivalent of about 10 billion hydrogen bombs each second. Every second of every day.

That is 2 billion times more powerful, than the Tsar Bomba, the world’s largest nuclear bomb. Every second of every day.

The Sun produces enough energy every second, for almost 500,000 years of the world’s current energy needs. Every second of every day.

The energy that is released in the core, takes the form of a photon; and this is the source of the Sun’s light and heat. Photons are trapped in the core anywhere between 10,000 and 170,000 years, before they can escape. Once a photon makes to the surface of the Sun, it will only take eight minutes to travel from the Sun to reach Earth and you. Science is so cool.

And would you like to know what’s crazier? I haven’t even discussed the other things the Sun creates like sunspots, solar flares, the solar winds, coronal mass ejections, magnetic fields and neutrinos, or the gravitational influence it has on the rest of the Solar System, to name a few.

The Sun is glorious, beautiful, powerful, and yet it’s still terrifying. We have learnt so much already about our stellar neighbour, but with many new discoveries to come.

I hope the first stop on our tour has made sense. Please let me know if it does. And with that, I’m done. There are so many bags under my eyes, I could use them for shopping; so I need to go to bed. Thanks for reading, following and subscribing to Some Geek Told Me. This project keeps me off the streets, and prevents me from dealing comic books in dark alleys at midnight. I’ll see you next week.

One of my simple goals for 2023; not in terms of teaching the public about the dangers of Sour Cream and Chives, is to write more science based content. So to kick the new year off, I’m going to be writing about astronomy; namely the Solar System. Each month I’ll use a badly scratched and well used magnifying glass, to look at some of the stellar¹ features within our Solar System.

I chose to write about astronomy, because it’s the first field of science I fell in love with. I didn’t even have to ask its phone number either; though to be fair, if it did give me a phone number, it would be fake. Nice.

I plan on starting off in the centre of the Solar System and slowly work my way out, so with each new month, I’ll be adding a new entry into my expansion pack. They will be full of facts and information, so they may look, sound, and read a bit differently than my other blogs. Hell, it could even be an improvement.

So for the first tour, we’ll be making very brief stops across the Solar System. A quick introduction will be made to each family member, then we’ll move onto the next one. Clear as mud? Great, so you need to strap yourself in, because we’re going to meet the family!

Our first stop of the Solar System is meeting the single parent that looks after the family. The funny thing about this parent, is that it’s actually a fusion reactor. We call it the Sun and just to make sure everybody understands how important the Sun is to us and rest of the family, we need to remember a few small things:

1.) The Sun is actually a star.

2.) The Sun is around 4.5 billion years old.

3.) The Sun’s mass is so large, that everything within the Solar System orbits it. This includes comets, asteroids, planets and us.

Moving on from the Sun; which many of its ex-partners simply can’t do, we need to discuss the siblings; also known as planets. And just like nearly everything, you can place siblings in groups. A person could have a brother or sister, half-brother/half-sister, step-brother/step-sister or an adopted brother or adopted sister.

The same can be said for the planets of the Solar System. They can be grouped into three simple types: terrestrial planets, dwarf planets and gas planets.

The four planets closest to the Sun, in order are Mercury, Venus, Earth (Yay!) and Mars. These are the terrestrial planets, also known as the rock planets or Inner Planets. They are rocky planets that are dense and small, they contain various metals and have a solid physical surface; as well as a few or no natural satellites (moons).

Beyond Mars, the fourth planet from the Sun, and Jupiter, the fifth planet from the Sun, lies a region called the Asteroid Belt. This area of space has millions of asteroids of various sizes, that orbit the Sun as well. It’s here in the Asteroid Belt, that we meet Ceres, the first member of the second group; the dwarf planets.

Just to clear things up, dwarf planets do not have beards, swing axes, enjoy singing, living with princesses, like mining or wear mithril. They are known as dwarf planets because there is a small difference between them and planets. This difference was established by the International Astronomical Union (IAU) in 2006 upon three criteria.

Remember when everyone’s favourite ninth planet from the Sun, Pluto, was demoted from planet to dwarf planet? Pluto remembers, because it failed to achieve one of the three criteria; which I will cover in another blog, very soon. People are still emotional about Pluto getting kicked out of the club, but I will explain it, I promise.

Ok, are you still with me? Great, let’s push on. Now we visit the four gas planets, also known as the gas giants or Outer Planets. These are Jupiter, Saturn, Uranus and Neptune. These planets are different from the Inner Planets, because they filled with different gases, they have no physical surface and they are extremely cold. They also have rings, multiple moons and they’re huge; each one is larger than the Earth.

Past Neptune’s orbit, we have the Kuiper Belt. This region of space could possibly be the source and origin of short-period comets. The Kuiper Belt also has a collection of dwarf planets, which fall under the label of trans-Neptunian objects or TNOs. These include Pluto, Haumea, Makemake and Eris.

There are some other TNOs named Gonggong, Quaoar, Sedna, Orcus and Salacia; and from what I understand, these TNOs have not been given the prestigious title of dwarf planet. Yet.

There are many other parts to our Solar System, but I’ll just be sticking to the Sun, Inner Planets, the Asteroid Belt and Ceres, Outer Planets, along with the Kuiper Belt and dwarf planets for the time being. So the first blog will be about the Sun in February, and I’ll try to put the Solar System post up on the fourth Monday of the month. Maybe, though it depends on how enthusiastic I feel.

This side mission is different for me, so I hope it makes sense. Alright that’s it, go watch some football, read a banned book, walk your dog and I’ll see you next week.

¹ Pun very much intended.