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Celestial Navigation TheoryThe Navigational TriangleA flat plane triangle can be solved using trigonometry. Knowing 2 sides and an angle, SAS, the third side and a second angle can be determined. The Celestial Triangle, which is laid out on the face of the planet, is a spherical triangle. In this triangle we also know 2 sides and an angle, Latitude, Declination and LHA. Pub 229 is a set of tables which solves the triangle using spherical trigonometry. Enter the table with:
2. Declination 3. LHA We extract :
2. Z (azimuth) Hc is compared to Ho (height observed) along with Z converted to Zn and then plotted from your Assumed Position to give a line of position. The Celestial Triangle’s three points are defined by the Pole, your DR Position (latitude and longitude) and the Objects Geographical Position (GHA and Declination) The Component Parts Ho - Height Observed: This is the Sextant observation (Hs) corrected for height of the eye above sea level and for refraction. (Dip, Altitude Correction) ![]() Lat - Latitude: This is your DR Latitude rounded to the nearest whole latitude. Dec - Declination: This is exact Declination for the body observed at the time of the sighting. LHA - Local Hour Angle: This is Meridian Angle (t). The Angle between your Longitude and the objects GHA (Greenwich Hour Angle). It is expressed as a whole number. LHA = GHA - West Long or + East Long Navigational TriangleAP - Assumed PositionDR - Position GP - Geographical Position, GHA and Dec of the Body PUB 229 Entering Argument: LHA Local Hour Angle LHA= GHA - W Long GHA + E Long Note: Long is changed to make LHA a whole number, Lat and new Long become AP. LAT DR - Lat rounded to nearest whole Lat. DEC - Exact Declination of body. ![]() HS - Height Shot HA - Apparent Altitude Corrected for Index Error and Dip Angle HO - Height Observed All Corrections Applied
Index Correction:
See Celestial Navigation Diagram Click image for more detail
Download Sunline Worksheet Download Local Apparent Noon Worksheet Download Latitude by Polaris Worksheet Great Circle CalculatorDistance:
L2 = Destination Latitude DLO = Difference in Longitude D = Distance Notes: 1. If L1 and L2 are Contrary in name, Treat L2 as a negative. 2. If course is negative, add 180 degrees. 3. If DLO is greater than 180, enter as negative. 4. Distance in miles = = CosD x 60 5. Subtract when crossing the equator Cos D = (Cos L1 x Cos L2 x Cos DLO) + -(Sin L1 x Sin L2) Initial Course Angle:
Points along the route. Determine Lat for known Long. L1 = Departure Latitude L2 = Destination Latitude DLO1 = Diff of Dep Long to known Long DLO2 = Diff of Arrival Long to known Long DLO12 = Diff between Dep and Arr Long.
Cosine – HaversineSight Reduction
Z = Azimuth Angle L = Assumed Latitude D = Exact Declination LHA = Local Hour Angle Note: Angles must be in degrees and tenths Hc = Arcsin (sin L sin D + cos L cos D dos LHA)
Great Circle Publication 229 Solution: Enter 229 with:
Dec = Latitude of destination LHA = Difference in longitude Notes: 1. If HC and Z are of body above the horizon
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