The Longitude Problem.
Navigating by the Stars.
Well one could ask why do people go to sea in small boats, climb mountains, etc?Perhaps we all have an inbuilt need to connect to our environment or even an aspiration to the divine.
For the purposes of celestial navigation on the surface of our planet you donâ€™t need to know about any of those crazy Copernican ideas of the universe.
As far as we are concerned the pre-Copernican, Ptolemaic notions of what we see up there are sufficient.
Of course it is always good to know what really is going on, but for now all we need is to be aware of what we can see.
And what we see up there are the Sun, Moon, Stars, and Planets marching in step across the sky.
They all rise to our east and set in the west.
Now, imagine that all these celestial bodies are on the inside surface of an immense crystal globe which encloses the earth.
And imagine that this crystal globe has an equator, north and south poles, latitude and longitude which reflect those of the earth.
Our celestial sphere now has a grid system which we can use, just like the lat and long on earth, to locate the position of celestial objects in relation to us.
So, now we earth bound navigators have two spheres to consider.
The first is the surface of the earth, the second is the inside surface of that imaginary crystal globe surrounding the earth.
On both spheres we use the same imaginary sets of coordinates, latitude and longitude.
We use this grid system to pinpoint the location of anything on either sphere.
The grid on the celestial sphere is a projection of the grid on the terrestrial sphere.
So if you were stood at the Earthâ€™s North Pole directly above your head would be the Celestial North Pole.
And by the same token the Celestial equator would be directly above someone stood on the earthâ€™s equator.
OK, so far so good, now it starts to get a bit complicated.
The equivalents of the terrestrial latitude lines are called lines of Declination on the celestial sphere.
While longitude line equivalents become Hour Circles on the celestial sphere.
And where longitude, on the terrestrial sphere is measured through 180 degrees east or west of the Greenwich meridian, on the celestial sphere it is numbered from 0â° all the way around to 360â° .
And the 0â° hour circle known as the Celestial Meridian is known as the First Point of Aries.There is also quite a bit of strange archaic language used in Astro Navigation but to begin with there are a few terms which are worth understanding.
These are to do with how you or I relate to the celestial bodies.
First is the point directly over your or my head this is known as your or my Zenith, and the bit of the surface you are standing on is your bodyâ€™s Geographical Position or GP.
The imaginary line running, due north or south from my or your Zenith is known as your or my own Meridian.
And the distance of any celestial body above your or my horizon is known as its Altitude, this is the angle which is measured with a sextant.
If you imagine a line from the centre of any celestial body to the centre of the earth where it passes through the surface of the earth is known as that celestial bodyâ€™s Geographical Position or GP.
The GP for a celestial body is measured in degrees of latitude and longitude.
The latitude measured north or south of the equator is known as its Declination.
Its longitude is measured in degrees westward from the Greenwich meridian and is known as the Greenwich Hour Angle (GHA) .
The Declination and GHA for the celestial bodies which are used for navigation can be found in the Almanac.
And Iâ€™m sure you are more than capable of working out from that the direction of north and south.
So, you are already something of an Astro Navigator!
OK, itâ€™s not quite that
simple as that as the place the sun appears to rise from will vary
slightly throughout the year.
At the equinoxes 21st of March and 23rd of September it will rise at due east and set due west.
But by 21st June the â€˜summer solsticeâ€™ it will rise 23.5â° further to the north of east then by 22nd December the winter solstice it will be 23.5â° south of east.
This is because the earthâ€™s axis is tilted by approximately 23.5â° and remains tilted in roughly the same direction throughout the year, and it is also why we have seasons.
The rate of change is approximately 1â° every four days.
Now donâ€™t rush out to buy a sextant, you can make a rough measurement of the suns angle using your hand.
Your fist will give you a rough angle of 10â° this can be subdivided by each finger being the equivalent of 2â°.
So if you want to find due east on the morning of the 1st March, (20 days before the equinox) you know that the sun will be rising 5â° south of east, so you need to measure half a fist to the north, of where it rises, to find due east.
OK, so that tells you where east and therefore all the other compass directions are but it doesnâ€™t tell you where you are.
But what we have learned so far is that the GP of the sun and therefore is Declination changes throughout the year.
And, that this information
is predicted for us in the Nautical Almanac.
Well letâ€™s stay with the sun for now as it is the easiest celestial body to find and consider the ocean navigators bedrock, the Noon Sight.
The reason for taking the Noon Sight is to determine the exact time when the sun has risen to its highest point in the sky.
This is known as your Local Noon.At your Local Noon the sun is directly north or south of you depending on where you are on the globe.
This means that its Celestial Meridian will correspond with your Longitude at that particular moment in time.
Now longitude is measured in degrees around the globe but one circuit of the globe is also equal to one solar day.
So if you have an accurate watch (chronometer) set to UT (Universal Time) or GMT as it used to be called, the difference between your Local Noon and UT Noon can be converted into degrees and distance west or east of the Greenwich meridian.
The distance of a body's GP from the Greenwich Meridian is its Greenwich Hour Angle (GHA).
So for every hour your local noon is after UT noon you are 15â° further west of the Greenwich meridian and conversely every hour your local noon is before noon UT you 15â° further east.
Unfortunately the sun isnâ€™t a very good time keeper, it can be as much as 20 minutes slower or faster than UT.
And any error in time will give us an error in longitude.
This is why we need that Almanac, it will give us the UT or Greenwich Mean Time that the sun reaches its highest point at Greenwich, for every hour of the day and for every day of the year.
This is the sunâ€™s Greenwich Hour Angle (GHA).
We can then use that time as our starting point.
And the need for accuracy is also why the sextant and an accurate watch are so important to celestial navigation.
In practice there are minor corrections which need to be applied but these only require some simple addition and subtraction and there are simple forms which can be used to make it even easier.
For now, itâ€™s the concept we are concerned with.
But regardless how accurate you are or how simple it is, having only one coordinate wonâ€™t tell us where we are, we could be anywhere along that meridian line between the north and south poles.
The lack of an accurate way of telling the time is why sailors in days of yore had problems determining their longitude.
What they were able to do, with considerable accuracy, was work out their latitude.
The SHA is the star's distance from the First Point of Aries, (represented by the sign of the ram) which using simple worksheets and some simple maths we can then convert.
So, the almanac only needs to tabulate the movement of this one position then by giving us the angular distance to all the navigational stars, we can easily calculate the GHA for any star at any time.
So, what is this First Point of Aries?It is a point on the celestial sphere which is used as a reference point, it is in fact where the â€˜Eclipticâ€™ and the Celestial Equator cross one another.
Venus, Mars, Jupiter, and Saturn plus of course the Sun are the only ones used for navigation unless we include the Moon with this group.
The method used to reduce an observation of a planet is similar to taking a sun sight, except that as you also need to see the horizon to measure the altitude this must be done at twilight.
The Moon, if I can be forgiven for including it here under Planets, can also be used for navigation.
However because it is so much closer to the earth than the other object we use, many more â€˜correctionsâ€™ have to be made when reducing the sight.
Anyone who has read Joshua Slocumâ€™s account of his sail around the world will know that he used Moon sights as his main way of telling the time, his only clock was an old wind up alarm clock with no minute hand.
A reasonable quality sextant such as the one I bought years ago will cost about the same as four or five hand held GPS sets.
There are some much cheaper plastic sextants on the market which I am led to believe are just as accurate.
I am also led to believe (never having used one) that care must be taken over the storage of the plastic ones as they are much more susceptible to developing errors, so might need adjusting more often.
The sextant as I'm sure you are aware by now is used to measure the angle between the horizon and a celestial body.
It can also be used to measure the any sighted angle, such as the angular distance between two landmarks or the height of a lighthouse, when coastal sailing.
Like any good magic
trick itâ€™s all done with mirrors.
It is called a sextant because the calibrated arc is one sixth of a circle 60â° , however because of the mirrors it can actually measure angles up to 120â° .
The frame of the sextant looks a bit like a slice of pizza.
The scale, the curved bottom part is fixed to the frame as is the telescope and the Horizon Mirror and the shades.
The Index Mirror pivots at the apex of the frame and is attached to the index arm so they both move together.Boat Books on-line
At the other end of the Index Arm is the measuring micrometer.
The fixed Horizon Mirror is only half mirror the other half of it is clear glass.
It is fixed so that when you look through the telescope one half of the view is straight ahead the other half is the reflection of whatever is showing in the Index Mirror.
When taking a sight the index mirror is adjusted so that the celestial object is reflected down into the mirror side of the horizon mirror while the horizon is visible through the clear side.
The shades are there to protect your eyes when taking Sun Sights.The micrometer is there to enable very precise angular adjustments and measurements to be made.