Editing Celestial navigation (section)

==Example==
[[Image:Sun Moon (annotated).gif|thumb|right|300px]]
An example illustrating the concept behind the [[intercept method]] for determining position is shown to the right. (Two other common methods for determining one's position using celestial navigation are [[longitude by chronometer]] and [[ex-meridian]] methods.) In the adjacent image, the two circles on the map represent lines of position for the Sun and Moon at 12:00 [[GMT]] on October 29, 2005. At this time, a navigator on a ship at sea measured the Moon to be 56° above the horizon using a [[sextant]]. Ten minutes later, the Sun was observed to be 40° above the horizon. Lines of position were then calculated and plotted for each of these observations. Since both the Sun and Moon were observed at their respective angles from the same location, the navigator would have to be located at one of the two locations where the circles cross.

In this case, the navigator is either located on the Atlantic Ocean, about {{convert|350|nmi|km}} west of [[Madeira]], or in South America, about {{convert|90|nmi|km}} southwest of [[Asunción]], Paraguay. In most cases, determining which of the two intersections is the correct one is obvious to the observer because they are often thousands of miles apart. As it is unlikely that the ship is sailing across South America, the position in the Atlantic is the correct one. Note that the lines of position in the figure are distorted because of the map's projection; they would be circular if plotted on a globe.

An observer at the [[Gran Chaco]] point would see the Moon at the left of the Sun, and an observer at the Madeira point would see the Moon at the right of the Sun.