The intercept method allows you to calculate a full position fix using a complete set of stars at a single point in time. This method of celestial position fixing is quite complicated to explain in this article, but I have made a complete video walking you through the entire process.Īdvantages of position fixing using the intercept method Once you have at least three intercepts, spread around 60° apart, you can plot them and get a celestial position fix. The difference between the two gives you an intercept for each star. Once you have taken your sights, you compare the measured altitude to an altitude you calculate from the nautical almanac. Pro Tip: It is possible to take sights all night if there is a bright moon available to light up the horizon. It can’t be too dark though, because you need a clear and crisp horizon to measure against. The sun needs to be below the horizon so that stars and celestial bodies are clearly visible in the sky. This is why the sights can only be taken at sunrise or sunset. Then, using your sextant you measure the altitude of each one above the horizon, noting down the precise time that you take your measurement. Normally, you would plan to take six sights, in the hope that at least three of them will be available to take, and not obscured by cloud cover. The classic celestial position fix is an intercept fix, taken either at sunrise or at sunset.Įxample of the intercept method for a celestial navigation position fix. Pro Tip: I learned celestial navigation from college, but always found one book particularly useful for brushing up my skills: Celestial Navigation, by Tom Cunliffe (link to Amazon). Comparing the calculated azimuth to the compass bearing lets you calculate the error in your compass. Using a nautical almanac, you can calculate the azimuth, or bearing, of any celestial body from your position. The final use of celestial navigation is for calculating your compass error by azimuth. Combining that with your longitude at merpass, you can get a full position fix from a single sight. If you take a standard sun sight at merpass, it will also give you your latitude. The time of merpass coincides with the time when the sun is either directly north of you, or directly south of you. Table of merpass, taken from the daily pages of the Nautical Almanac available from ĭue to the rotation of the earth, the difference in time corresponds directly with your longitude. If you measure the precise time of merpass, you can compare that to the time of merpass on the Prime Meridian. Merpass is the meridian passage of the sun, which is the point at which the sun is at its highest point in the sky. Similarly, when you are on the equator, Polaris appears to have an altitude of 0°, matching your longitude.įor longitude, it is possible to use merpass. At that point, Polaris’s altitude is 90°, and your latitude is also 90°. It wobbles around a little bit, but generally, it will be directly overhead when you are at the north pole. You can find your latitude from Polaris, the North Star. Other celestial navigation techniques can be used to find either your latitude or your longitude, but not both. You transfer your first line of position using your course and speed in the same way you would with a terrestrial running fix. To complete a sun-run-sun, you need to take sights a couple of hours apart so that the angle between them is large enough to get an accurate fix. This is basically a running fix, using a celestial line of position from the sun as your position line. The other way of finding your position is to use the “sun-run-sun” technique. You can then work out your final position fix as the point where all your position lines intersect. Classic 6 star celestial position fix taken at sunrise or sunset.Įach sight gets plotted onto a chart, giving a line of position.
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