‘Celestial’ world is not too far away – and not in our lifetimes
“A small, circular world that is, at the very least, not very far away from Earth.”
– Professor John Ellis, University of New South Wales, Sydney, author of The World Within Us (Simon & Schuster, 2018) “I’m not sure if you’ve heard of it before, but the ‘Celtic’ world isn’t too far from Earth, and not just any world.
It’s not just a fantasy world.
The Earth is a celestial sphere.
We can’t see it.”
– David Deutsch, author The Sky is Not the Limit: How Humans Can Create a Universe That’s Beautiful (Crown Publishers, 2018).
The idea that we can create a world that looks a lot like Earth was first proposed by physicist David Deisch in 1957.
The idea came from the observation of the Earth’s curvature and its rotation as it orbits the sun.
Deutsch realised that our planet was tilted toward the Earth by about 0.05º or 0.06% – roughly about the diameter of a pencil.
We also know that the Earth is tilted at about 0° or 0°/sec by a period of about five million years.
But there’s a lot more to it than that.
Earth’s orbit is tilted by a lot, as it is on the sun’s axis.
This means that Earth’s spin is very much constant and that its rotation rate is also constant.
But it’s also true that we’re all orbiting at about the same rate, as we’re at about 1º or 2º/sec.
So it’s easy to imagine how the Earth would rotate, but not how it would look.
To create this world, Deutsch’s team, led by Professor David Deitsch at the University of Sydney, looked at the Earth at a certain distance, the Sun.
Their findings were published in Nature Geoscience in 2015.
The team measured how much the Earth was tilted in a circle by looking at how the rotation rate of the Sun changed as it moved across the sky.
As it passed over Earth, the rotation of the planet slowed down, meaning that the rotation was being accelerated by the Earth, not vice versa.
Deitsch and his team were able to measure how much Earth’s rotation rate changed at a particular distance by observing how the Sun’s spin changed as the Earth passed over it.
The spin of the planets Earth and the Sun are extremely complicated things.
Their spin is governed by the motion of the three planets around the sun and their orbits around the Milky Way.
But we’ve never known what the Earth spin actually looks like at that distance.
So, by measuring the rotation and the rotation velocity of the earth, the team was able to create a map of how Earth’s rotational rate changed as they moved across it.
They were also able to calculate the angular position of the world and the direction of the rotation.
So the team calculated that the rotational spin rate of Earth was about 0º/s.
This would make it slightly more than a quarter the radius of the solar system.
The result of this map was called The Earth, Its Rotation and Its Direction (TETD).
In the map above, you can see the position of Earth at various distances from the sun as it rotates around the Earth.
You can also see the direction the Earth rotates from its center.
The map is called the “TETS” map because the authors used the Earth as a reference point for the map.
“We looked at a map with two circles and two points,” says Deitsch.
“And what we did was, we looked at how much rotation there was and how fast it was.
And we found out that there was a lot of rotation at the center.
And that was good for our calculations.
But what we didn’t realise was that it was all very complicated.”
The map shows that the average rotational speed of the sun was about 1,200 kilometres per hour.
This is about half the speed of light.
So when the Earth orbits the Sun, the Earth spins at around 1,000 kilometres per second.
The rate of rotation is the same as that of a bullet going about 250 kilometres per minute.
That means that a bullet goes about 25,000,000 metres an hour.
It is this speed that is called “spin”.
In this diagram, the sun is on top of Earth.
We’re looking down.
The red lines show the path of the bullet, and the blue lines show its spin.
The arrow shows the Earth spinning away from the Sun at an angle of about 0 degrees.
The speed of sound, the speed at which objects move in relation to each other, is about 1012 kilometres per seconds.
“The Sun is really moving towards us at about 100 kilometres per sec,” says David Deitzer, a professor of physics at the Australian National University, who was not involved in the study.
Deitz says the speed is