The Celestial Sphere
The Celestial Sphere describes a model of our view of the Universe. You'll learn about constellations, directions in the sky, and how the rotation of the Celestial Sphere looks from here on Earth.
Note: This article was written for observers in Fullerton, California.
What you should know: How to measure angles in degrees. Angles Review from Math is Fun.
Patterns in the Sky
For human observers, the stars appear in fixed patterns in the sky.
You might recognize the pattern of the stars in Vincent van Gogh's Starry Night Over the Rhône, which was painted in 1888:

Source
You might know it today as the Big Dipper, a part of the constellation Ursa Major.

Source: Acadia Photo Safari

Source: Torsten Bronger
This same pattern appears in texts written by human observers over a thousand years ago.
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The Dunhuang star map, from around 700 AD:

Source -
The Book of Fixed Stars from around 964 AD:
Source
All around the world, observers notice the same patterns,
but tell their own stories:

Sources: Stellarium, NASA/STScI
Constellations
In modern Astronomy, constellations are how we identify and name regions of the sky - NOT the patterns of the stars themselves.
The constellation Orion is everything in the highlighted region in this sky map:

Source: IAU, Sky and Telescope
The Dome of the Sky
Stars in constellations appear to be side-by-side, but they can be at very different distances from the Earth.

The red star Betelgeuse on Orion's "shoulder" is 650 light years away, but the purplish glowing Nebula M42 in the "sword" is 1,344 light years away. So Betelgeuse is closer to us than it is the nebula.

Sources: Dupree and Gililand, CfA/STScI/NASA/ESA and Filip Loic
How can you figure out how far away things are if you can’t reach them?
- Binocular vision (compare view from each eye.)
- Known size scaling (cows are really the same size.)
Source: RF Vila -
Atmospheric perspective (the effect of the air.)
Source: Joaquim Alves Gaspar -
Modern astronomers use versions of each of these methods to work out the distances to astronomical objects
- None of them work for unassisted human vision
- Stars are not small, but are very far away
- They have different sizes and distances, BUT appear as points in the sky
- except for the star closest to us... the Sun!
When we look at the night sky they seem to be sprinkled on a dome over our heads.
This is an optical illusion because we lack depth perception for such distant objects.
Directions in the Sky
The Horizon is the edge of the visible sky.
If you look to any side, you see the Horizon. This is where the sky appears to meet the most distant part of the ground you can see.
Horizon examples:

Ground to sky:
North, East, South, and West mark the directions you would travel out toward the horizon. They are the same directions you use to orient a map.

If you look directly overhead, you see the Zenith. This is the "top" of the dome.
Altitude, Azimuth, Meridian
We locate regions in the sky by azimuth (angle around the horizon) and altitude (angle above the horizon).

Azimuth on the horizon. Which direction do you face? For example: North, East, South, or West.
Up from the horizon to find altitude:
- On the Horizon (0°)
- Low in the sky (less than 45° up from the horizon)
- High in the sky (more than 45° up from the horizon)
- Zenith (directly overhead, 90° up from the horizon)
Sky Location example
The GPS satellite passes overhead:
from far away in the Northwest,
to the Zenith, to far away in the Southeast.

Polaris, the North Star
Polaris is seen directly above the North point of the horizon in the Northern Hemisphere.
In Fullerton, we see Polaris at an altitude of 34° above the horizon.

You can find Polaris from nearby star patterns - it's between the stars of the Big Dipper and the W-shaped Casseopeia.

The Sun and the Meridian
The sun rises in the East,
moves high in the Southern sky,
and sets in the West. Its path makes an arc across the sky.

We also divide the sky by the meridian, a line going from the North point of the hoizon to the South point.
This is where we get a.m. (ante meridian, before meridian) and p.m. (post meridian, after meridian).
The Celestial Sphere
Each night, the stars appear to move.
Polaris Time Lapse video: Looking North toward Polaris, the stars rotate around it.
This makes it seem like the stars are all on the surface of a spinning ball around us.
Animation of the Celestial Sphere: Source: Science Sims @ CCNY
Many early astronomers imagined that stars were really fixed on the surface of a Celestial Sphere that surrounded and revolved around the Earth.

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The celestial sphere is a scientific model.
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We now know it is not how things really are.
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It’s still a useful way to map the position and motion of the stars in our sky.
Features of the Celestial Sphere Model
The Celestial Sphere surrounds the Earth.
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The stars are in fixed positions on the sphere.
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The North Celestial Pole is directly above Earth's North Pole.

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The Celestial Equator is directly above Earth's equator. It's 90° down from Polaris.

The Celestial Sphere and your Local Sky
Your Local Sky is half of the celestial sphere; the half that is above your local horizon
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Your zenith is directly above your location on Earth. Your horizon is 90° down from your zenith in a full circle. The North Celestial Pole and Celestial Equator are tilted in your sky.

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The North point of your horizon is directly beneath the North Celestial Pole. Your meridian runs from North on your horizon, through the Zenith, to South on the opposite side of the horizon. East and West are to the left and the right if facing South.

Example Star Paths in the Local Sky
Below is a diagram of a the local sky facing East, with two example star paths. One path circles Polaris in the sky, and the other arcs from East to West.

Things to notice:
- The N/E/S/W directions are on the horizon.
- Polaris is high in the Northern sky.
- The Celestial Equator
- runs from East to West.
- is tilted compared to the Zenith.
- from the center of the dome, is 90° away Polaris.
- Star Path A follows the Celestial Equator. A star on this path rises across the horizon due East, travels high above the Southern horizon, and sets across the horizon due West.
- Star Path B circles Polaris. A star on this path never crosses the horizon. It moves from low in the Northern sky to the Zenith and back.
Check Your Understanding
You walk outside and turn so you are facing due North. Your zenith is:
You walk outside and turn so you are facing due North. South is:
Where in the diagram would you label North?

What direction is the observer looking in the diagram below?

You look to see the sun in the early evening. It's a few sun-heights above the horizon. You describe it as: (choose two)

Go Further
What stars can you see? Where Are the Stars? See How Light Pollution Affects Night Skies | Short Film Showcase by National Geographic (YouTube) explains how light pollution affects our view of the stars.
Ideas from this lecture are used in the The Rotating Sky Lab.
