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DK Eyewitness - Astronomy

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Where is the pole star? Pole Star<br />

To find a town on Earth, a map<br />

is used. To find a star in the night<br />

sky, astronomers need to use the<br />

celestial coordinates. The Pole Star<br />

is one useful marker in the northern<br />

hemisphere because it indicates the<br />

northern celestial pole. Since the<br />

north–south axes of both Earth and<br />

the sky run at right angles to the<br />

terrestrial and celestial equators,<br />

which are measured as 0°, the Pole<br />

Star is measured as 90° North. An<br />

observer looking at the Pole Star Arctic circle<br />

near the Arctic Circle sees it very<br />

high in the sky; near the equator,<br />

the Pole Star barely rises above Pole Star<br />

the horizon. In the South Pacific,<br />

it is never seen at all.<br />

Great Bear<br />

Pole Star<br />

80° Latitude (Greenland) 30° Latitude (Egypt) 0° Latitude (at the equator)<br />

Celestial sphere<br />

Pole<br />

Star<br />

Tropic of Cancer<br />

North/South axis<br />

North Pole<br />

A static Earth,<br />

surrounded by the<br />

crystalline sphere<br />

of the fixed stars<br />

Sun<br />

Saturn<br />

Tropic of<br />

Cancer<br />

Terrestrial<br />

equator<br />

Celestial<br />

equator<br />

Ecliptic<br />

Tropic of<br />

Capricorn<br />

South Pole<br />

To a distant star<br />

Sun<br />

Noon<br />

on first<br />

day<br />

Measuring time<br />

With solar time, one day equals the time it takes Earth to make one<br />

full rotation on its axis, from noon to noon. But because Earth is also<br />

orbiting the Sun as well as spinning, the solar day is<br />

Second noon<br />

for sidereal time<br />

Second noon for<br />

solar time<br />

not accurate in relation to distant stars, and it is the<br />

stars that concern astronomers. They measure time<br />

in relation to a distant star. This “day” is the time that<br />

passes between two successive “noons” of a star, noon<br />

being the moment when that star passes directly over<br />

the local meridian (p.27). This is called a sidereal day.<br />

Antarctic<br />

circle<br />

The celestial sphere<br />

This model of the celestial sphere<br />

records how the ancients viewed the<br />

universe. All the planets seemed to<br />

travel along the same band as the<br />

Sun. Since eclipses happened along<br />

this path, it was called the ecliptic.<br />

The ecliptic seemed to run at an angle<br />

of 23½° from the plane of Earth’s<br />

equator. When the Sun passed along<br />

the ecliptic, it turned back as it passed<br />

through the signs of Cancer in the<br />

north and Capricorn in the south.<br />

These points where the Sun turned in<br />

its path were called tropics.<br />

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