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| train:lectures:siderealtime [2024/03/18 14:44] – Roy Prouty | train:lectures:siderealtime [2024/03/18 16:10] (current) – Roy Prouty | ||
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| Since DEC($\delta$) is measured from the CEq, we find that lines of constant DEC trace out concentric circles on the CNP and CSP. The radius of these circles of constant DEC decrease with $\cos{\delta}$. So at $\delta=\pm 90^\circ$ (at either CNP or CSP) the circle of constant DEC is a point and at $\delta=0^\circ$ (along the CEq), the circumference of the circle of constant DEC is maximized. In the same way, the rate of motion along these circles of constant DEC also decreases off of the Celestial Equator with the $\cos{\delta}$. | Since DEC($\delta$) is measured from the CEq, we find that lines of constant DEC trace out concentric circles on the CNP and CSP. The radius of these circles of constant DEC decrease with $\cos{\delta}$. So at $\delta=\pm 90^\circ$ (at either CNP or CSP) the circle of constant DEC is a point and at $\delta=0^\circ$ (along the CEq), the circumference of the circle of constant DEC is maximized. In the same way, the rate of motion along these circles of constant DEC also decreases off of the Celestial Equator with the $\cos{\delta}$. | ||
| + | ===Challenge=== | ||
| + | The next time you are participating in an Observing Session, calculate how long it will take for a star (not near the CNP) to move from one side of the frame to the other side. | ||
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| + | Written by Roy Prouty 20240318\\ | ||
| + | Reviewed by | ||