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Digital Universe Guide - Hayden Planetarium

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106 3. THE MILKY WAY ATLAS<br />

3.3.18 Equatorial Coordinates Sphere<br />

Group Name radec<br />

Reference —<br />

Prepared by Carter Emmart, Brian Abbott (AMNH/<strong>Hayden</strong>)<br />

Labels Yes<br />

Files radec.speck<br />

Dependencies none<br />

Notes Also represents Earth’s radio sphere (see below).<br />

The equatorial coordinate system is a projection of our Earth-based coordinate system of latitude<br />

and longitude onto the “celestial sphere.” The celestial sphere is an imaginary shell that surrounds Earth<br />

upon which all objects in the sky lie. Astronomers describe an object’s position in the sky by its right<br />

ascension (RA) and declination (Dec). Declination is simply a projection of our latitude on Earth. The<br />

point directly above the North Pole (the zenith point) is the north celestial pole and is located at +90 ◦<br />

declination. If you’re standing on Earth’s equator, your zenith—that point directly overhead—would lie<br />

on the celestial equator.<br />

Right ascension is based on Earth’s longitude but is expressed in hours instead of degrees.<br />

Astronomers have split the sky into 24 hours (15 ◦ per hour) measured from the vernal equinox. An<br />

object’s location is then described in hours, arcminutes, and arcseconds. For example, the star Sirius in<br />

the constellation Canis Major, the brightest star in the sky as seen from Earth, is located at right<br />

ascension 6 hours, 46 arcminutes, and −16 ◦ , 45 minutes declination.<br />

We use arcminutes and arcseconds for right ascension to remind ourselves that the length of these<br />

units depends on your declination. Close to the pole, an hour of right ascension will be quite small, while<br />

at the equator, it will be at its maximum. As with lines of longitude on Earth, lines of right ascension are<br />

not parallel with one another.<br />

Drawing the Sphere From Earth’s perspective, the wire-frame sphere perfectly represents the<br />

equatorial coordinates. If you examine the radec.speck file, you’ll see four main sections. The first<br />

section is the ellipsoid command that draws the main sphere:<br />

0 0 0 ellipsoid -s line -c 1 -r 20.245 -n 24,19<br />

The second part contains a mesh statement that draws a line around the celestial equator; this has a<br />

color index of 2. Following this is another ellipsoid statement that draws lines every 15 arcminutes in

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