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How to Find the Constellations

[Key Words] [General] [Right Ascension] [Declination]
[So Where Am I Looking]

Key Words

 

General
The sky has been mapped out just like our planet. Earth is mapped out by latitude and longitude. Latitude measures the distance away from the equator. It is a series of lines parallel to the equator. The equator is 0°. Above that, the numbers continue to rise until you reach the north pole, which is 90° North (90°). If you start on the equator and work your way down, you will reach the south pole at 90° South (-90°). Longitude measures the distance away from the prime meridian. Lines that radiate from the north and south pole are used for measurement. They work east and west until meeting up at the 180° mark, halfway around the world.

The sky has a similar system that is used for position. It all lies on the celestial sphere. This sphere is not a physical object, just like the latitude and longitude lines on earth. Stars appear to be flattened onto this celestial sphere. The celestial equator is a line that runs all around the celestial sphere inline with earth's equator. The celestial poles are formed where the north and south poles intersect the celestial sphere. Keep in mind that these are all imaginary and do not really appear in the sky.

Right Ascension
What astronomers use in place of longitude is called right ascension (RA). Right ascension is measured in hours, minutes, and seconds. The 0° mark is located at the vernal equinox. The vernal equinox is the point in which the ecliptic crosses the celestial equator on the suns way north. We can make a line of right ascension by connecting an imaginary line from the north celestial pole, through the north star, right over our head (called the zenith) and down to the south pole. Because we are rotating, this line will move with us. Every 24 hours, it will cross the same point that it started at.

On the celestial sphere, lines of right ascension don't rotate with us, unlike the one that we just made. There are 24 hours of right ascension, each one broken into 60 minutes, and each minute broken into 60 seconds. So, if you looked at your zenith, and you knew that you were looking at 00h 00m 00s of right ascension, one second later you would be looking at 00h 00m 01s of right ascension, another second and it would be 00h 00m 02s, etc.

Declination
Declination (dec) is much simpler than right ascension. It works just like our system of latitude. It is measured in degrees, minutes, and seconds. As you go above the celestial equator, numbers start at 0° and work up to 90° at the north celestial pole. As you go below the celestial equator, numbers start as 0° and go down to -90° at the south celestial pole.

So Where Am I Looking?
Knowing coordinates of stars is very useful for using star maps. If you know the coordinates of a star, you can then look them up on a star map, and then find them in the sky. For example, if you saw the coordinates 16h 45m 08.9s RA -16° 42' 58" dec you could look them up on a star chart and find Sirius, the brightest star outside our solar system. Here is one you should go and look at: 05h 36m 12.8s RA -1° 12' 07" dec.

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[Key Words] [General] [Right Ascension] [Declination]
[So Where Am I Looking]



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