Hey, it’s you! I’m so glad you could make it! This is the third chapter of our little tour of the Solar System and I was beginning to think you weren’t going to make it. For the obligatory recap of the tour, the first chapter was the introduction, while the second was all about the Sun.
Since the last stop was the Sun, we should be moving onto the next celestial object, which is Mercury; the first planet from the Sun. The problem is, I feel it could be important to discuss just what a planet is, and how they are different from a dwarf planet.
I briefly mentioned dwarf planets in the introduction, because let’s face it, they sound made up. It’s ok to admit it, you’re among friends. Dwarf planets are real, but they’re not as famous as their larger siblings; however they are no less important. Seriously.
Ok Scott, stop talking and actually say something! What is a dwarf planet? That is an insightful question, so here is a ridiculous answer. Let’s hop in our DeLorean time machine of the mind and travel back in time to visit three important dates: 1930, 2005 and 2006.
In 1930, a planet was discovered by Clyde Tombaugh, which was later named as Pluto.1 Pluto become known as the ninth planet of the Solar System, and history and science textbooks would never be the same. Um….that’s not truly accurate is it? I remember learning about Pluto at primary school: we had nine planets in the Solar System and even though Pluto was the smallest, it was still identified as a planet.
For over 60 years, Pluto got to hang out with its older siblings, because it was still identified as a planet. Well, until 2005 it was. Over the years, technology has advanced with new developments, that has allowed humanity to view the universe in amazing new ways. Because of this, new objects were being discovered in our Solar System and beyond; but especially in and around the Kuiper belt, which is a disc like region of space, beyond Neptune.
And just so we are on the same page, Pluto resides in the Kuiper belt.
So back to 2005. Among the media released discoveries of Makemake and Haumea, another object was discovered: Eris. When the first measurements of Eris were released, it appears that it was actually larger than Pluto, even though it was further away. This development led a lot of scientists to call for the reclassification of Pluto. They also thought another object named Ceres, which was discovered in 1801, finally needed a permanent classification as well.
We can now move to 2006, which was Pluto’s least favourite year ever. Enter the International Astronomical Union (IAU). The IAU has been described as:
…a nongovernmental organisation with the objective of advancing astronomy in all aspects, including promoting astronomical research, outreach, education, and development through global co-operation.
Basically the IAU get to decide things about astronomy.
In 2006, the IAU held a general assembly, with one of the issues concerning Pluto and what to do about it; along with some other objects. This led to the definition of a planet, which consists of three criteria.
1.) Is in orbit around the Sun.
2.) Has sufficient mass to assume hydrostatic equilibrium.
3.) Has “cleared the neighbourhood” around its orbit.
The first criteria is obvious, the planet must orbit around the Sun.
The second criteria talks about the planet achieving hydrostatic equilibrium, which is just a shape that is nearly round.
The third criteria is about when a planet orbits the Sun, it must be the most dominant gravitational object, in that orbit. It means the planet needs to be able to sling or clear the neighbourhood of any other smaller objects in its path.
When Pluto was measured against these three criteria, it passed the first and second, but failed the third. And a long story short, Pluto was declassified as a planet and reclassified as a dwarf planet, along with others.
Textbooks were rewritten and suddenly Pluto no longer could sit with the cool kids, but needed to sit at a different table.
This being the case, a definition for a dwarf planet was established.
1.) It must orbit the Sun, and not be a moon.
2.) Has enough mass to be round.
3.) Has not cleared its orbit of debris.
To date, our Solar System has eight planets that meet all three planetary criteria. Starting with the closest to the Sun, we have Mercury, Venus, Earth, Mars, Jupiter, Saturn, Uranus and Neptune.
As for dwarf planets, they are planetoids that fail on one, two or even all three of the IAU planetary criteria; but pass all of the IAU dwarf planetary criteria. To the best of my understanding2, there are five official dwarf planets in our Solar System. Starting with the closest to the Sun, we have some amazing names like Ceres, Pluto, Makemake, Haumea and Eris.
There are five other dwarf planets in the Solar System, which are known as Trans-Neptunian objects or TNOs, that are waiting to be officially recognised as dwarf planets.3 In order from the Sun, they are Orcus, Salacia, Quaoar, Gonggong and Sedna.
Basically that’s it. A planet is identified as a planet, because it passes all three IAU planetary criteria, whereas the dwarf planets, fail at least with one of the planetary criteria. Whether this is fair, is another story for another day. Clear as mud?
That’s it for another week, I’m sorry. I’ve got to go and bore my wife with rugby and football scores now. Thanks once again for reading, following and subscribing to Some Geek Told Me; it means a lot. Remember to walk your dog; watch a banned movie; stay away from Sour Cream and Chives; and I’ll see you next week.
1 The story behind Pluto’s name, deserves its own tv movie.
2 Let’s face it, that isn’t very much.
3 Again, to the best of my understanding.
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