Heliacal rising.
Sidereal time.
Take a picture of the stars before the dawn every day.
Just before dawn, while the sky is still dark, and the stars are still out.
Tomorrow, the same thing, just before dawn, while the Earth still blocks the Sun.
Heliacal rising.
Sidereal time.
Take a picture of the stars before the dawn every day.
Just before dawn, while the sky is still dark, and the stars are still out.
Tomorrow, the same thing, just before dawn, while the Earth still blocks the Sun.
Stars help us find our way. Stars are like a giant map in the sky that tells us where we are on the surface of the Earth. Sailors use them as a “map” to navigate the world. For thousands of years, the stars were stationary markers of latitude and longitude.
We are going to learn to map something new onto the sky: locations on the Earth! We can create an exciting new set of “constellations” out of the shapes of the continents on the Earth.
We live on a sphere so we can see half of the sky (a hemisphere) at any one moment. It’s easy to imagine half the Earth mapped onto half the sky. Keep reading to learn how.
Wherever you are on the Earth, when you look straight up (toward your zenith), you might see one star, but there are a bunch of other stars within view. All of the stars you see in the sky are directly overhead some other place on the Earth. Every place on Earth has their own set of stars directly overhead – their “zenith stars.”
Look up at any star in the night sky; that star is directly over some place on Earth. There are hundreds of “faraway zeniths” up there.
Every star maps to a location on Earth and every location on Earth maps to a star.
If you live in the western hemisphere, you can learn to look up and “see” the land borders of the North American and South American continents visible, projected into the sky like a giant painting on a curved ceiling. You can learn to see even more landforms in the sky – you can learn to see the entire western half of the Earth projected in the sky.
We can learn to see country outlines in the sky. The key is to imagine yourself at the center of the Earth looking out into space “through” a translucent Earth surface.
Here is a good way to visualize these countries-in-the-sky even when you are on the surface. Imagine that you can look up and see your location at the zenith.
When I do this, I see southern New York state, Long Island jutting out into the water like a long pier, and the wide Hudson River emptying past New York City. Eastward is the dark expanse of the Atlantic Ocean and low on the eastern horizon are the countries of Europe and West Africa.
Westward in the sky, I can see the outline of the west coast of the US. Then, there is a big blank space of the Pacific Ocean and a spot near the western horizon that is Hawaii.
There is one odd thing about the map as you see it in the sky… it’s reversed – as if seen in a mirror! This happens because we project the map lines outward into space toward the stars. When we look at the map this way it’s as if we are “inside” the Earth looking outward.
The map of the USA covers about 58˚ of sky from east-to-west. 58˚ is about 2x pinky-to-thumb (spread out all your fingers of both hands and touch thumbs). Your left pinky tip should be on your zenith. If you are in New York or somewhere on the east coast, the right pinky tip will indicate the approximate western edge of the USA.
Learn to see the zenith map in your sky using this Physical Astronomy technique.
Face south. Then, reach both hands straight up over your head and point above your head with both pointer fingers. You are pointing at your zenith. Now, bring both arms down until they are pointing one due east and one due west. You are pointing at two points in the sky that are zeniths for someone else.
When I do this exercise in New York, my left hand (the eastern) points at a spot in the starry sky that is the zenith star for someone in the country of Nigeria in West Africa. This is a location on the globe that is 6 time zones east. My right hand (the western) points at a spot in the sky that is the zenith for someone in the island state of Hawaii in the middle of the Pacific Ocean. This location is 6 time zones west of New York.
So, when I look at the eastern horizon sky I am looking at the starry sky that is already directly above a place 6 time zones ahead of me. I am looking at someone else’s zenith stars.
Face east, point up. Now, bring your arms down and point toward the north and the south directions. This time your right hand points south and your left hand points north. Your right hand points at a spot in the sky that is over the city of Cuzco, Peru (the closest city to Machu Pichu) and your left hand points to sky that is over Yekaterinburg, Russia – the 4th largest city in Russia.
If you do this physical astronomy exercise right after sunset, the eastern and southern zenith locations are in night, but the western and northern sky points are over Earth locations that still have daytime.
This means that you can see the star that is at their zenith, but they cannot see that star. For example, Seattle still has 3 hours of sunlight left in their day so stars are invisible behind blue sky. The city of Yekaterinburg is on the opposite side of the world and just after sunset in New York it faces the Sun and has a bright daytime sky!
We are on the night time side of the Earth and we can see the current zenith stars of Seattle and Yekaterinburg – but people who live in these cities cannot see them! They have to wait to rotate to the night time side of the Earth to see stars.
Project an imaginary map of the Earth into the sky. The map has to be the correct size so that when it is viewed from a distance it “covers” the same distances.
If a map is too close, it is just the same size as the territory. So, we have to choose the correct distance to project the zeniths. As the zenith map “projector screen” moves away from the Earth we see more of the borders of the Earth. But, at some point the distance of the map corresponds exactly to the faraway zeniths.
Our question is: “How far away from the Earth do you have to be so the landforms (like the continents) have an angular diameter that is equivalent to their “actual size” in the sky?” How far away does our imaginary zenith map USA (about 3000 miles wide) image have to be to cover 58 degrees of arc in the sky?
To answer this we need math.
The Earth is approximately 24,901 miles in circumference at the equator. If we can see half the sky from any point on the Earth, then we can “see” half the Earth projected onto the sky by the zenith map. That means that for 180˚ of sky we can “see” about 12,450 miles of the Earth’s surface projected into space. 12,450/180 = 69 miles. When 1 degree of arc spans 69 equatorial miles the image is “at” the correct distance.
So, at the equator every degree of sky covers about 69 miles in every direction. As you go towards the poles the longitude degrees (east and west) cover less and less zenith map distance, but the latitude degrees (north and south) always stretch 69 miles. Every 15˚ of sky equals about 1035 (69*15) miles.
The distance between your pointer finger and your pinky (when you hold your arm and hand stretched out in front of you) is 15˚ – so you are measuring about 1035 miles on Earth with that sky measurement. One pinky width is equal to 1˚, which is 69 miles of zenith map!
There is a simple calculation that helps us determine how far away something needs to be to fill just 1˚ of the sky. Here we use just a tiny drop of trigonometry to discover the “tangent of 1 degree.”
The tangent of 1˚ is 0.017455. The inverse of something is when you divide 1 by the number you want to invert. So, the inverse of 0.017455 (1/0.017455) is 57.29. The inverse of the tangent of 1˚ helps us figure out the distance something has to be to appear to be 1 degree angular diameter.
This page explains how to calculate distance from a known angular size. “When an object’s distance is 57.29 times its size, it has an angular size of 1 degree.”
So, 57.29 * 69 miles = 3,953 miles away! This is how far away the “map” has to be to show you your hemisphere of the Earth map. 3,953 miles is higher than low Earth orbit (LEO) satellites (lower than 1200 miles); it’s closer than geosynchronous satellites (at about 23,000 miles); and it’s about 1/60 the way to the Moon.
So, imagine that the Earth map is projected onto a screen – an imaginary celestial sphere, shell-shaped – that is quite close to the Earth and encircles us. It shows us our Earthen landforms and the oceans beside, superimposed in the sky.
We live on a sphere. When we look at out night sky we are able to see stars low on our horizon that are visible directly above someone else – one-quarter the way around the around the world in all directions.
If you live within 6 time zones of someone that means that you share some “simultaneous sky.” Anyone living further than 6 time zones away sees a completely different sky – unless you can see circumpolar stars that dip under the North Star. That means that you can see countries past the North Pole and down the other side of the globe.
Your zenith is yours – it is unique and changing all the time. Not even someone standing right beside you shares your zenith. You can use this idea of the zenith stars to comprehend the vast and mysterious experience of life on a sphere.
A list of extreme geographic points in the USA – Wikipedia – https://en.wikipedia.org/wiki/List_of_extreme_points_of_the_United_States
Many people ask “Why can’t I feel the Earth spinning?” Or “Why don’t we feel the rotation of the Earth?” The answer is that the Earth is so large and we are so small in comparison that we just get carried along for the ride.
We humans are tiny so we don’t notice that everything on Earth moves along with us. Until we look up and we see the Sun speeding through the sky – then the questions start to fly: “Why does the Sun move across the sky?”, “How big is the Earth?”, “How fast is the Earth spinning?”
It’s hard to imagine just how large the Earth is and just how fast it is carrying us around in its daily motion. How fast is the earth spinning?
You are about to learn the answer and learn how to experience this speed!
The Earth spins at about 1000 mph (1609 kph) at the equator. But we can’t feel it. This illusion of non-motion happens for several reasons:
Imagine riding in a fast car that has no windows. The car cruises on a smooth highway at 100 kph (62 mph). Inside the car we chat with our friends, the seats are comfortable, and maybe a hot drink sits placid in a cup holder. We don’t feel the motion at all unless the car turns or speeds up or slows down.
Everything seems to be staying still but this stillness is an illusion. All of this stuff in the car is moving along with us at the same speed. But, if you could open a window in the car you would see the motion of the other objects not in the car.
The sky is our open window to find those other objects that are not “on the Earth.” We will use them to explore the Earth’s speed and movement.
Another reason that we can’t feel the Earth spinning is because our sense of balance. We get this sense from organs of the inner ear. We know what it feels like to move. We can feel a car accelerate and turn – but these sense organs don’t help us feel the Earth’s changes in speed and constant turning.
It’s easy to feel and then believe that the Earth stays still and everything else moves around us; the Earth doesn’t seem to be moving. The idea of a moving Earth seems preposterous. It’s no wonder it took humans so long to figure out that the Earth is spinning and moving!
However, you can learn a surprising way to feel the rotation of the Earth – and it has to do with the speed of sound. You can “feel the Earth spin under your feet” and all it takes is a little bit of imagination.
The speed of sound in air is 1235 kph (767 mph). This is really fast, but it is still a visible and imaginable speed.
The speed of the Earth’s rotation at the equator is faster than the speed of sound! But, because of the Earth’s shape, the Earth’s rotation speed is exactly equal to the speed of sound at two latitudes on the Earth: 42.97 North and 42.97 South.
What does this mean for you and your approach to physical astronomy? You have to train your brain to see the speed of sound, then you will be able to feel the Earth spinning. You will understand that the speed of sound is the speed of day.
We can train our brains to “see” the speed of the Earth’s rotation (I’ve named this speed the “Speed of Day“). This is possible because “the speed of sound = the speed of Earth spinning.”
How fast is the Earth spinning? Once you have a clear idea of how fast sound goes, you can get a clear idea of how fast the Earth is spinning – and by experiencing this speed you can easily imagine just how incredibly large the Earth is.
One way of visualizing the speed of the Earth’s rotation is to imagine that a gigantic bell rings each time the Sun enters a new time zone. Imagine that there is no sound loss over distance and the sound of that bell can be heard across the whole time zone (up to 1000 miles).
When this bell rings, the sound takes time to travel. It will travel at the speed of sound: 767 miles per hour.
Bangor, ME and Detroit, MI – two American cities on opposite ends of the eastern US timezone – are 1183 km (735 miles) apart. The sound of our imaginary bell takes about 1 hour to travel between these cities.
Since these cities are near 42.97 N latitude, the Earth takes about 1 hour to spin underneath the Sun.
Sound, which seems quite fast, is actually slow enough to “see” it moving. Once you can see the speed of sound you have seen the speed of the surface of the Earth.
The Earth rotates once per day. People at the equator are moving at faster than the speed of sound, people near the poles are moving slower than the speed of sound. People living at latitude 42.97 N and 42.97 S are moving at exactly the speed of sound.
Editor’s Note: Credit goes to Bob Berman (aka SkyManBob) for first pointing out the latitude/speed of sound correspondence to me. I first learned about this idea in his fantastically engaging book Zoom – How Everything Moves. It has a footnote in Chapter 5 that says people at Coney Island are moving at 795 mph – just over the speed of sound. It got me wondering… how can people experience this speed? The result is this article. Thanks, Bob!
Editor’s Note: Another Bob (aka AstroBob) gets credit for helping me refine this article with insights about our common perception of motion.
List of cities at 43˚N latitude.
Calculations showing speed of rotation at different latitudes on the surface of the Earth.
Video showing how to use your video camera to measure the speed of sound – good science fair project!
Video by the Exploratorium visualizing the speed of sound in a very creative way – Clapping Speed of Sound.
A visualization of the Earth’s surface rotation speed at each latitude.
A general audience article discussing how we experience the motion of the Earth.
In this exercise called “The Sky Below Us” you will learn to see the Earth as a giant ball and understand that the Earth is floating in space. This will allow you to see the sky below us.
The “speed of day” is the speed of Earth’s rotation: 1600 kilometers per hour (kph) which is about 1000 mph.
1600 kph is fast. Most people have never experienced anything moving at this speed. Commercial jet airplanes fly at 1000 kph (600 mph). Click here to continue reading…
Most people, when they look up at the night sky can easily see stars and identify some familiar groups of stars (asterisms and constellations). Some people can even find and name some planets – Venus, Jupiter, and Mars are all bright and easy to see.
But, there are many invisible wonders in the sky – and some of them can be seen without a telescope. In fact they are so big that a telescope is not the right tool to use; we have to use something even more powerful… imagination!
Using visualization and imagination, I am going to show you how to find and “see” a very large structure in our sky: the solar system disk itself.
Practice the fundamental skills of observation. Learn to see the giant geometries of space.Click here to continue reading…