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Digital Universe Guide - Hayden Planetarium

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108 3. THE MILKY WAY ATLAS<br />

3.3.19 Ecliptic Coordinates Sphere<br />

Group Name eclip<br />

Reference —<br />

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

Labels Yes<br />

Files eclip.speck<br />

Dependencies none<br />

Ecliptic coordinates are based on the imaginary line traced by the Sun throughout the year. This line<br />

is called the ecliptic and, in three dimensions, also defines the plane that contains the Sun and Earth.<br />

Because Earth is tilted on its axis 23. ◦ 5 to this plane, the Sun appears to move in declination<br />

throughout the year (see “Equatorial Coordinates Sphere” for definition). Two days a year, on the vernal<br />

equinox around March 21, and on the autumnal equinox around September 21, the Sun crosses the<br />

celestial equator. Around June 21, it lies over the Tropic of Cancer (the summer solstice in the Northern<br />

Hemisphere), and around December 21, it lies over the Tropic of Capricorn (winter solstice for the<br />

Northern Hemisphere). Coincidentally, the Tropics of Cancer and Capricorn are at 23. ◦ 5 north and 23. ◦ 5<br />

south latitude, respectively.<br />

Ecliptic coordinates are described by ecliptic longitude and latitude measured in degrees (labels<br />

provided every 10 ◦ ). Longitude is measured from the vernal equinox [(RA, Dec) = (0, 0) ◦ ] and the<br />

ecliptic north pole is in the constellation Draco (23. ◦ 5 from the celestial north pole and the north star,<br />

Polaris). The ecliptic north pole is the point perpendicular to the plane of the Solar System and would be<br />

the north celestial pole if Earth were not tilted 23. ◦ 5.<br />

A New Horizon In the Atlas, the ecliptic sphere is similar to the celestial sphere but is given a<br />

radius of 100 light-years. Turn on the Milky Way all-sky image (mwVis) and notice the tilt of the ecliptic to<br />

the band of the Milky Way. These two planes, the plane of the Solar System and the plane of the<br />

Galaxy, are tilted about 60 ◦ to each other (62. ◦ 87 to be precise).<br />

Many of us are used to thinking of the Solar System plane as our cosmic horizon line. All the planets<br />

lie roughly within this plane, so it makes sense that this should be the plane from which we measure up,<br />

down, over, and under. However, the Milky Way band tells us otherwise. In fact, the Sun and all its<br />

planets are orbiting the center of the Galaxy once every 225 million years. Picture the Sun and its<br />

planets tipped 60 ◦ , orbiting in the Galactic plane at 220 km/sec (or just less than 500,000 miles/hour).<br />

We now see there’s a more significant horizon to obey, that of our home Galaxy. Are there any horizons

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