GHA
Well-known member
I've never actually got the hang of spherical trig, cartesian 2 dimensional makes sense with the sin etc just ratios but spherical... so lets have a look over morning coffee (need an excited emoji!)Agree with these. It isn’t Rocket Science. For many, rote is the only way, hence why they think that a Template is a gift from Neptune. With a little more effort and coaching by Poseidon, figure out the basics of spherical trig and it becomes straightforward.
So from memory the Admiralty AP3270 rapid sight reduction tables I have require 3 things, your Lat, the body Lat & difference in longs, LHA.
first stop perplexity> "Give an overview of the spherical trig involved in reducing a celestial sextant sight"
Answer
Celestial navigation using a sextant involves complex spherical trigonometry to convert the observed altitude of a celestial body into a position on Earth. The process, known as sight reduction, relies on solving the celestial navigation triangle, also called the PZX triangle
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The PZX Triangle
The PZX triangle is a spherical triangle formed on the celestial sphere by three points:
The sides and angles of this triangle correspond to important navigational elements:
- P: The celestial pole (North or South)
- Z: The observer's zenith (directly overhead)
- X: The celestial body being observed (sun, star, planet, or moon)
- PZ: Co-latitude (90° - latitude)
- PX: Co-declination (90° - declination of the celestial body)
- ZX: Co-altitude (90° - observed altitude)
- Angle at P: Local Hour Angle (LHA)
- Angle at Z: Azimuth
- Angle at X: Parallactic angle (not typically used in navigation)
So far so good, that makes sense, same angles just from a different datum.
Spherical Trigonometry Formulas
The fundamental formula used in celestial navigation is the cosine formula for sides
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cos(a)=cos(b)cos(c)+sin(b)sin(c)cos(A)cos(a)=cos(b)cos(c)+sin(b)sin(c)cos(A)
Where a, b, and c are the sides of the spherical triangle, and A is the angle opposite side a.
For the PZX triangle, this formula can be expressed as:
sin(Ho)=sin(Lat)sin(Dec)+cos(Lat)cos(Dec)cos(LHA)
Where:
- Ho is the observed altitude
- Lat is the observer's latitude
- Dec is the celestial body's declination
- LHA is the Local Hour Angle
Beyond me, can't visualise that so will just have to accept it, means remembering cos () no way could I figure that out from scratch. So "cosine formula for sides" sides means the angles if the GPs are extended to the centre of the earth?
Perplexity has access to Wolfram|Alpha Examples: Mathematics so should be able to do the sums.
So picking one from ap3270..been a long while since this book was opened-
Lets pick LAT =20º, Dec = 15º (same name as LAT), LHA = 45º.In the Rapid Sight Reduction Tables for Navigation (AP3270), LAT., LHA, and declination are key parameters used for celestial navigation calculations. Let's break down each of these terms:
LAT. (Latitude)
LAT. refers to the assumed latitude of the observer's position on Earth. It is one of the primary arguments used to enter the sight reduction tables. In AP3270, latitude is typically given in whole degrees, ranging from 0° to 89° North or South
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LHA (Local Hour Angle)
LHA is the angle between the observer's meridian and the celestial body's hour circle, measured westward from 0° to 360°. It represents the apparent angular distance of the celestial body from the observer's meridian
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. LHA is calculated by combining the Greenwich Hour Angle (GHA) of the celestial body with the observer's assumed longitude:
If the result exceeds 360°, subtract 360° to obtain the final LHA
- For western longitudes: LHA = GHA - Longitude West
- For eastern longitudes: LHA = GHA + Longitude East
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Declination
Declination is the angular distance of a celestial body north or south of the celestial equator, similar to latitude on Earth. In AP3270, declination is typically given in whole degrees, ranging from 0° to 29° North or South
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Book says Hc = 46º 55'
So>
sin(Ho)=sin(Lat)sin(Dec)+cos(Lat)cos(Dec)cos(LHA)
sin(Ho)=sin(20)sin(15)+cos(20)cos(15)cos(45)
= 0.7303 from perplexity
from .wolframalpha ^
So finally.... "what is arcsine(0.730343322772540813741134936233901786275378419357341693685266035513254507) in degrees and decimal minutes"
The arcsine of 0.730343322772540813741134936233901786275378419357341693685266035513254507 is approximately 46.7499999999999999999999999999999999999999999999999999999999999999999999°
or 46° 45'.
Close!!!! But should be closer, wonder why that is Still close enough to get the dopamine hit though
(Edit. Ask it to calc trig to 10 decimal degrees it comes up with 46° 54.91102')
Ah, wolframs
46.915183737359028075860755247167244855221419164415881621786507337574790225 degrees
0.915183737359028075860755247167244855221419164415881621786507337574790225*60 = 54.911024241541684551
46º54.91102424154168455'
YAY!!!!!!
Full dopamine!!!!
That must have been about 3 days in an astro nav classroom
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