Astronav: essential tools and documents

This is the first in a series of articles on celestial navigation. It covers the tools and documents required for celestial navigation, namely:

1. A sextant;
2. An astronomical almanac;
3. A reduction table (Ho 249);
4. A calculator;
5. A precision watch;
6. A ruler;
7. Paper for recording your observations;
8. A star chart.

You don’t need anything else. A basic scientific calculator with trigonometric functions (sin, cos, tan, etc.) costs around $20. A ruler costs next to nothing, but it might be worth investing in a set square or a breton plotter. These tools make it easier to draw lines at specific angles. Depending on the quality, a sextant can cost between $200 and $5,000. As for a watch, you can buy a quartz model, but it’s handy to use your mobile phone. Everything else is free and available online.

As an extra, you might want to get a mobile app for identifying stars, or a starfinder.

Below, I detail where I source the documents needed for celestial navigation, as well as their purpose. I also outline a few considerations specific to buying a sextant.

Astronomical almanac

An almanac is an astronomical calendar. It is an annual document, much like a tide table. For every day and every hour of the day, the almanac will give the position of the sun, the planets and the main stars used for navigation. An almanac also includes additional information, such as the times of sunset and sunrise, as well as the corrections required for interpolating positions. In later sections, we will learn how to use an almanac. As this stage, the most important aspect to learn is the coordinate system for stars and planets.

The Bauer and Rodegerdts astronomical almanac is free, updated annually and based on established scientific libraries. Its main limitation is the lack of a guarantee. If you are sailing on a pleasure yacht, this almanac is sufficient. If you are sailing professionally on a vessel worth several million dollars, your insurance company may require a publication with a guarantee of reliability.

Pages from the Almanac

A two-page extract from the Almanac is shown below, covering the 21st, 22nd and 23rd of February 2026. The first page shows the position of the vernal equinox (Aries) and the positions of the planets Venus, Mars, Jupiter and Saturn. The geographic position of the planets are listed in the almanac for every hour and day of the year.

The geographical position (GP) of a star is its projection onto the surface of Earth. It is the position on the Earth’s surface determined by the line connecting the star to the centre of the Earth. Finding the GP of a star is an intermediate step for determining its position.

The almanac also presents the coordinates of the brightest stars in the sky in the celestial sphere coordinate system. The coordinates are given by the day, hour by hour (0 to 23) in Greenwich Mean Time (UTC-0).

Coordinates of celestial bodies

The GP of celestial bodies is positioned on earth. Its coordinates are in terms of Greenwich hour angle (GHA) and Declination (Dec). The Greenwich hour angle is equivalent to longitude, but ranges from 0° to 360° as one moves westwards. It should be noted that longitude, on the other hand, ranges from 180°E to 180°W.

Declination is the same as latitude. It ranges from 90°S to 90°N. The only difference is that it is used exclusively for celestial bodies. We therefore use it to describe the position of stars, planets or the Sun.

The position of stars is expressed in terms of the Sidereal hour angle (SHA). This is a coordinate specific to stars. Like longitude, it measures a star’s position from east to west. However, the SHA ranges from 0° to 360°.

Below, we can see that on 21 February 2026 at midnight (UTC-0), the GP of Venus is GHA 165° 49.7′, Dec S07° 55.6′. We can also see that the start Alpheratz as a sideral hour angle of 357° 34.1′ and a declination of 29° 14.1′. We will see in another text how to interpret these positions. For now, the aim is to familiarise ourselves with the documents.

The following page shows the GP of the Sun and the Moon, as well as the times of sunrise and sunset at the Greenwich meridian. We can deduce from this second page that on 22 February 2026 at 1100 (UTC-0), the GP of the Sun will be at GHA 341° 38.3′, Dec 10° 06.2′.

Without an astronomical almanac, we do not know where the stars are. At this point, you should be able to find the coordinates of any celestial body for any date and any whole hour. If need be, pick a celestial body and a date randomly and find the coordinates.

Correction table

As the name suggests, correction tables details corrections to be made to various angles. The most important corrections are for the GP coordinates and for the sextant readings.

Interpolation corrections

These correction pages are used to interpolate the GP of celestial bodies outside of whole hours. An example of a correction page from the Almanac is given below.

For example, we can see that the correction to the GHA of the Sun’s GP, for 15 minutes 23 seconds, is 3° 50.7′. This means that this correction must be added to the whole hour coordinate found in the Almanac if the time is 15min23s past the hour.

Likewise, the correction to the GHA for the point of Aries is, for 16 minutes and 17 seconds, of 4° 04.9′. This means that if the time 16min17s past the hour, this correction must be added to the GHA to find the proper position of the point of Aries.

The logic is the same for other celestial bodies. These pages will become clearer with use. At this stage, it is important to remember that corrections must be applied to the positions obtained when the time is not a whole hour.

Corrections to sextant readings

Measuring an angle using a sextant requires corrections. For example, the Sun is a relatively large disc in the sky. Depending on whether the angle is measured from the upper limb or the lower limb, the measured angle will differ. Depending on the measurement chosen, a correction must be applied to measure the angle from the centre of the Sun.

Similarly, corrections must be made for low-altitude stars, for refraction, and for the fact that taking a measurement at a sufficiently high altitude above sea level can influence our results (dip). These corrections are incorporated into the calculations and are necessary to establish a reliable position. The tables below are used to make these corrections. A full text is dedicated to understanding these corrections.

Ho 249 Reduction Table

Volumes 2 and 3

The Ho 249 reduction table is free and comprises three volumes. Volumes 2 and 3 are timeless and are used to solve intermediate calculations. If we prefer mathematics, these tables can be replaced by two equations. In practice, one looks for a page to read the relevant table entry based on the information one has. A full explanation of what these tables mean will be the subject of a separate text.

Volume 1

The first volume of Ho 249 gives the direction (Z_n) and the altitude (H_c) of various stars as a function of latitude and longitude. It is an invaluable aid for identifying which stars will be visible in a given part of the world, as well as their approximate position relative to your location on Earth. It is a practical publication for planning sextant observations. It will be detailled in the text about planning star sights.

Below is an extract from the table for a latitude of 87°N. It shows the calculated altitude (H_c) and the direction (Z_n) of various visible stars depending on the relative position of the vernal equinox (LHA ♈). For example, if the relative hour angle of the vernal equinox (LHA ♈) is 28°, then the star Pollux will be visible to the east (Z_n = 090°), at a calculated altitude of (H_c) of 27° 59′ above the horizon (if you are at a latitude of 87°N).

At this stage, you should be able to read this type of table and extract the relevant information.

Obtaining a sextant

The price of sextants varies greatly depending on the quality of manufacture. In Canada, Tamaya sextants are the maritime industry standard (made of steel, at $4,500 each). Mark plastic sextants are perfect for taking (and passing!) a course in celestial navigation with a practical exam. They are, of course, of lower quality. In particular, they warp with temperature changes. As a result, the accuracy of the angles measured is lower.

My personal sextant is a Mark 25 (accurate to 0.2′) and it spends more time than not in its storage box. If I need to take astronomical observations at sea, the vessel I’m on usually has professional-grade sextants. When I took my first course in celestial navigation, I chose the highest-quality plastic model because I knew I would have to use it for the practical exam. If you only need to take a classroom course, the cheapest model is probably sufficient. However, your calculated position will be less accurate.

How to use a sextant is covered in a full text. There’s no need to spend 1000$ to get started. If you become a professional navigator, chances are your employer will provide you with a sextant.

Paper for plotting bearings

The last page of the Nautical Almanac includes paper for plotting bearings for celestial navigation. If there is enough space on your chart table, it is best to print these pages in landscape format (11″ x 17″) and allow for the possibility of making mistakes. It is therefore best to use a graphite pencil and have a good supply of printed sheets. If your chart table is small, you may need to use the 8.5″ x 11″ format.

Bear in mind that the latitude is fixed (the scale is graduated), but the longitude still needs to be drawn in. This is because the units of longitude distance vary with latitude. Consequently, you must use the scale shown at the bottom right of the image, depending on the latitude where the drawing will be made.

Eventually, you will be able to create your own masterpieces, such as the image below. Note that the latitude is 47°N (near Newfoundland) and that the longitude scale is drawn according to this latitude. You can see that the scale at the bottom right includes an interpolated length at 47°N, allowing for a better approximation of the longitude scale.

A star chart

The US Naval Observatory provides a star chart free of charge. I include an introduction to it in a text on the theory of celestial navigation and we will use it in the text about planning star sights.

Conclusion

This text provides a brief overview of the tools and instruments that will be essential for astronomical navigation. At this stage, you should know these documents exists and roughly be able to extract information from given tables.

Interpreting what the information they contain means will be covered in specific texts. It is therefore normal, at this stage, not to know what the calculated altitude H_c is or not to know why corrections are needed. These concepts will become clearer as you read the other texts. If you want to do an astronavigation class, you however need these tools with you.