1. A LITTLE HISTORY,
2.TIME - GMT, UT. UTC & TIME ZONES
3. TIME AND GPS
4 .THE ART OF FIXING YOUR POSITION USING CELESTIAL BODIES
5. SIGHT REDUCTION USING A CALCULATOR
A LITTLE HISTORY
Using the sun and stars to find our way is a very old art. It is known the Vikings used the sun and the pole star to sail a line of latitude on their voyages to North America. However until the mid -18th century there was no certain method of fixing a ships position. Ocean navigation remained a hit and miss affair with explorers dying of thirst sailing to and fro along lines of latitude looking for islands.
In October 1707
Admiral Sir Clowdisley Shovell on the Association was sailing homeward
bound from the Mediterranean past the hazards of the
Scilly Isles on their way back to England. After making an error in judging
their longitude, the Admiral headed north with the three other warships under
his command. Tthe fleet was wrecked on the Isles of Scilly. Most of the crews
died including the Admiral.
This tragedy was mainly due to a lack a practical method of establishing longitude at sea. A Royal Committee was formed to gather ideas. In 1714 a Board of Longitude was set up in Britain and a prize of £20000 was offered to encourage the discovery of a means of accurately determining longitude at sea. Between 1735 and 1760 John Harrison, a Yorkshire man, clockmaker and genius developed clocks and watches that worked at sea. Thus seafarers could take Greenwich time with them around the world. Captain Cook used a copy of Harrison's watch on his second world voyage returning in 1775 to pronounce it to be a very accurate method of establishing longitude. Harrison eventually won the prize. The full story is told in the very readable book, Longitude by Dava Sobel.
How did time solve longitude? Having Greenwich time enables seafarers to time their local noon in Greenwich time. (rather than local time which would just tell you is was local noon!) The time of noon at Greenwich is found from tables (Almanac) as it varies slightly daily. The time difference between the local and Greenwich noon can be converted to longitude. The sun travels 15 degrees around the earth every hour. Therefore if your local noon occurred one hour later than Greenwich noon you would be 15 degrees west.
By the end of the 18th century celestial navigation had taken off. The navigator was now armed with a copy of Harrison's accurate time piece, a sextant, (invented in 1757, a development of the earlier quadrant,) and tables giving the accurate positions of the heavenly bodies. These items along with increasingly accurate charts surveyed by the likes of Captain Cook meant that the navigator was able fix his position out in the ocean with a fair degree of accuracy. . In 1837 Captain Thomas Sumner of Boston, USA developed a method of establishing position lines from sights. He coupled these lines using the transferred position line method to get more versatile fixes.
The modern method of celestial navigation was developed by the French navel officer Captain (later Admiral) Marcq St. Hilaire in 1875. This is know as the Intercept Method. Like Sumner's method it uses the transferred position line principle and does not depend on a noon altitude of the sun. Very handy when the sun is not out all day.
The RYA Ocean Course follows the Marcq St Hilaire Intercept method, as do most modern text books.
Finally, why do we need to use the celestial bodies when we have the GPS?. Some navigators, perhaps because of an interest in the history of navigation, will just want to know. Some may have a healthy mistrust of electronic gear and want a reliable backup out there in the ocean.. Others, perhaps aiming for higher qualifications, need to have the RYA Ocean Yachtmaster qualification..
Celestial navigation can be straightforward. Using the Air Navigation Sight Reduction tables and pro-formas it requires only simple arithmetic. A knowledge of the night skies is not necessary
This is important, buy the smallest book you can find. I recommend Tom Cunliffe's Ocean Sailing. Master the basics of the subject, then if you want to know more, buy a thick book.
Ian Crowson 2003
GMT Greenwich Mean Time
In 1880 international agreement accepted Greenwich as the prime meridian from which all time at sea should be measured.
GMT is based on the 'average time' the sun takes to go around the world. i.e. one day (solar time) In fact noon, (when the sun it at its highest altitude due south) at Greenwich varies daily . Whilst the sun is not an accurate time keeper it is predictable. The time of the sun's meridian passage (noon) at Greenwich is given in the Nautical Almanac for each day of the year.
GMT is also known as Zulu time (mostly by the services)
Most British tide tables and Almanacs use GMT (UT). But take care Reeds for example uses, for example, French Standard Time (1 hour ahead of GMT) for times of tides at French ports.
BST British Summer Time
Between the last weekend in March and last weekend in October we add an hour to GMT (or UT) for daylight saving.
Remember to add an hour to tide times in Reeds during daylight saving time.
UT Universal Time
Same as GMT.
Nothing new, actually introduced in 1928 but GMT continued to be used for navigational publications and radio communications until recently.
UT is based on the spin of the earth. It is the mean solar time and the time scale needed for celestial navigation.
UTC Co-ordinated Universal Time
This is the time that time signals worldwide are co-ordinated to.
For practical purposes it can be regarded to be the same time as GMT and UT. (Note: UT and UTC are kept within 0.9 sec of each other and be regarded as the same as at Nov 2003. Changes in future may require a correction to be applied)
The world is divided into 24 time zones each spanning 15 degrees of longitude. Time zone Z or 0 goes 7.5 degrees each way from Greenwich. Many larger countries group areas together into one zone for domestic reasons.
New York is in Time Zone +5. This means to work out Greenwich Time 5 hours must be added. e.g. if it is 0500 hours in the morning in New York, add 5 hours to discover it is 1000 hours in London.
For those interested in Greenwich and time a good book is Greenwich Time and the Longitude by Derek Howse.
Even better might be a visit to the Old Royal Observatory at 0 degrees longitude, Greenwich.
3. TIME AND GPS
GPS uses atomic time (TAI time scale). GPS time was identical to UTC on 6th January 1980. Since that date corrections have been made to UTC for leap seconds (atomic time being more accurate) but not to GPS time. Therefore a difference of over 13 seconds has built up between UTC and GPS time.
A correction is given in the nav messages transmitted by GPS every 12.5 seconds to automatically correct the time difference and allow UTC to be obtained from the GPS accurate to +/- 1 second.
However it is possible to get a time from the GPS receiver that is not accurate enough for celestial navigation where the correction has not made for various reasons.
A chronometer or good quality quartz watch should used for celestial navigation
4. THE ART OF FIXING YOUR POSITION USING CELESTIAL BODIES
To get started lets look at the equipment required. A sextant (for measuring the angle of celestial objects above the horizon,) an accurate clock or watch that can be read to hours, minutes and seconds (four seconds error can put you off a mile) and, finally, a copy of the Nautical Almanac for the current year. The almanac contains the exact positions of the sun, moon, planets or stars for every second of the year. Sight Reduction tables will normally also be required, more later.
THE NOON SIGHT
The noon sight for latitude where the navigator observes the sun while it is passing through its highest point for the day is a good place for us to start. The angle of the sun above the horizon at its highest point is measured with the sextant and easily (using declination from the Nautical Almanac) converted to latitude. The time when the sun reaches its highest point can be converted to longitude with reference to the exact time of noon at Greenwich (using the Meridian passage time at Greenwich from the almanac). The RYA syllabus does not include noon sight for longitude. In practice several sights would be required as it is difficult to precisely time noon from just a noon sight. So, if you stick to noon sights there’s not that much to it. An hour or so of instruction, a few hours of practice, and you're on your way. However don’t rely on this method to cross the North Sea in winter!
You can also measure the altitude (and time of observation) of the north star (Polaris) and calculate your latitude easily. The altitude of Polaris is similar to your latitude and requires just a few corrections.
You can also measure the altitude (angle above the horizon) of the sun at other times during the day. For the moon, stars, and the planets you need to stick to brief periods of twilight around sunrise and sunset when both stars and horizon are visible. These sights are a little more involved, but their reduction requires only more arithmetic.
THE INTERCEPT METHOD
Read the next paragraphs carefully, this is the heart of the matter. This is the standard approach (attributed to Admiral Marcq Saint Hilaire) and is called the intercept method of sight reduction. This is the method the RYA Course is based on and is the one used in most modern text books such as Tom Cunliffe’s excellent Ocean Sailing.
Firstly a sight (measured with the sextant) is taken of the celestial body to get an observed altitude (Ho). Note: the exact UT time of the sight must be recorded. Various corrections are applied to the sextant altitude to get Ho.
Secondly you work out the calculated altitude (Hc) of the body from an assumed position. Your assumed position is based on your DR or EP but ‘doctored’ slightly to allow you to enter the sight reduction tables in whole numbers. To do this, use the Nautical Almanac to find the position of the body at the time of observation. Then you take the bodies position and use the sight reduction tables to obtain the altitude (Hc) (angle above the horizon) and azimuth (Zn) (angle from true north) that the body would have had if it had been sighted from your assumed position.
The aim of the sights is to obtain position lines in order to get a fix.. Comparison of this calculated (Hc) and the observed value (Ho) of the altitude gives rise to a position line which when plotted with other position lines gives you a fix. The altitudes (Ho & Hc) give position circles around the geographical position (GP) of the body. The difference between Hc and Ho is the intercept. That is how far from the calculated position (circle) the observed position (circle) lies. The azimuth gives the bearing from the body and shows which part of the circles to use. Because the circle is so large the small part used (as indicated by the azimuth) appears as a straight line. This is the position line on our plot. We use the position line in the same way as if it was from a bearing on a church spire taken with the familiar hand bearing compass. Two or more are required to get a fix.
To recap and go over the procedure step by step:
You measure the altitude of a celestial body (Ho), noting the exact time. (UT)
You get the position of the celestial body at the time of observation from the Nautical Almanac.
Using your assumed position you calculate what the altitude (Hc) and the azimuth (direction of the object) would have been from that assumed position.
Comparison of the altitude you measured (Ho) with the one you calculated (Hc) gives you an offset that can be plotted on a chart as a position line.
A fix is obtained by plotting two or more position lines. Where two or more stars are observed in one session an immediate fix is obtained. ( just like taking bearings of say a church, chimney, and water tower) When just the sun is used a running fix (transferred position line fix) is worked up with a position line being obtained, say in the morning, and another later in the day.
SIGHT REDUCTION AND ASSUMED POSITION
Sight reduction is the process used to determine the altitude and azimuth the celestial object would have at your assumed position. Your assumed position is based on your DR or EP but ‘doctored’ slightly to allow you to enter the sight reduction table in whole numbers.
The method of sight reduction used in the RYA Course is straight forward and use’s tables. These are AP 3270NP303 Sight Reduction Tables for (Air) Navigation Vols. I, II & III. Volume II latitudes 0 – 39 degrees north or south. Volume III latitudes 40 – 89 degrees north or south. Volumes II & III are limited to celestial objects whose declination (angle above or below the celestial equator) is less than 29 degrees. This is good enough for the sun, moon, planets and some stars.
Volume I. Selected Stars is something completely different. Each day a changing set of seven stars (out of the 41 best navigation stars) are presented along with their altitudes and azimuths. Volume I is great, it makes it easy to find the correct star without a knowledge of the night skies.
Why Air Navigation Tables? – although these tables are slightly less accurate than the 6 books of Marine tables, fewer and lighter books are required. In fact recently published copies are not titled Air as they have become popular for general maritime use.
OTHER METHODS OF SIGHT REDUCTION
Sight reduction is the solving of the PZX triangle. This the spherical triangle traditionally solved by using spherical trigonometry. There are various methods of sight reduction including using tables, trigonometry, calculators, and computer software. There are Concise Sight Reduction tables in the Nautical Almanac, these maybe useful in an emergency, but can be difficult to use and are less accurate. The Sight Reduction Tables for Marine Navigation come in six big, heavy and expensive volumes. After using the Air Table these should be straight forward to use.
One way of doing the sight reduction is with an inexpensive hand calculator (that has "sin" and "cos" keys) using two easy, one line formulas from spherical trigonometry These formulas can be found below. There are also a number of pre programmed calculators which include Almanac information. Computers offer not just sight reduction programes but software which includes Almanac information, sight reduction and fix calculators. Just enter the sextants angles from your sights, date/times and your DR/EP, touch a few keys and out comes your fix in lat and long. Fun maybe, but remember did your machine ever pack up at home?
SIGHT REDUCTION USING A POCKET CALCULATOR
This requires a scientific calculator. It should have sin, cos and tan functions and be able to handle degrees and minutes. The Casio fx-83WA which should cost less than £10 is suitable.
1. Sun Sights.
A. To find Hc (calculated altitude) (Do this calculation first as the Hc is required to find Azimuth)
Required: (a) LHA of body (b) DR Latitude (c) Declination of body
sin Hc =
(cos LHA x cos DR lat x cos dec) + or - (sin DR lat x sin dec)
Note: use + if lat and dec are same names.
B. To find Azimuth (Zn)
Required: (a) DR Latitude (b) Declination of body (c) Hc (from first calculation)
cos Az * =
sin dec +/- (sin Hc x sin DR lat) divided by (cos Hc x cos DR lat)
Note: use + when lat and dec are of opposite names.
* Remember Az is the azimuth angle. To get Zn (Azimuth) apply the rules:
Northern Lat: LHA > 180 deg. Azimuth = Azimuth Angle. LHA < 180 deg. Zn = 360 - Az
Southern Lat. LHA > 180 deg. Zn = 180 deg. - Az. LHA< 180 deg. Zn = 180 + Az
Link to site with free soft ware for PC sight reduction
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Volume I. Selected Stars is something completely different. Each day a changing set of seven stars (out of the 57 best navigation stars) are presented along with their altitudes and azimuths. Volume I is great, it makes it easy to find the correct star without a knowledge of the night skies. Why Air Navigation Tables? - although these tables are slightly less accurate than the 6 books of Marine tables, fewer and lighter books are required.