NauticTools2

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Sextant altitude corrections – from the reading Hs to the observed altitude Ho

The altitude read off the sextant is not yet the altitude you work with. Only after index error, dip, refraction and – depending on the body – semi-diameter and parallax do you get the observed altitude Ho. NauticTools2 works the whole chain and shows every step.

Sun's lower limb on 22 October 2026: Hs 30°00.0′ becomes Ho 30°10.3′ – with every correction in the working. The line under “Sun” shows that the lower limb is selected.

Which corrections are applied?

CorrectionSizeApplies to
Index error± a few ′all bodies
Dip− 1.779 · √HEall bodies
Refraction− 0′ to 34′all bodies
Semi-diameter± about 16′sun, moon
Parallax+ HP · cos Hmoon, Venus, Mars

The index correction compensates the error of the sextant itself. Dip arises because the eye is above the water: the visible sea horizon lies below the rational horizon. Refraction lifts every body apparently – by over half a degree near the horizon, not at all at the zenith. For the sun and moon you measure a limb; the semi-diameter refers the altitude to the centre. Parallax converts from the observer to the centre of the Earth for the nearby moon and the planets Venus and Mars.

Sketch (exaggerated): eye at height of eye above the water, rational horizon level, line of sight to the sea horizon slightly below it (dip); the sextant measures from the sea horizon to the apparent body, the true direction is a little lower because of refraction body (apparent) true direction refraction Hs dip rational horizon line to the sea horizon height of eye
Greatly exaggerated: the sextant measures from the sea horizon (Hs). The sea horizon lies below the rational horizon by the dip, and refraction makes the body appear higher than it really is. Both amounts are subtracted.

When do you need it?

Formulas and working

Ho = Hs + IC − dip − refraction ± SD + parallax
  1. Index correction

    Hs + IC – the reading corrected for the index error.

  2. Dip

    1.779 · √HE in minutes of arc, with the height of eye HE in metres; subtracted.

  3. Semi-diameter

    For the sun about 15.7′ to 16.3′ depending on the season, for the moon 0.2725 · HP. Lower limb: add, upper limb: subtract.

  4. Refraction

    Depends on the apparent altitude – about 34′ at the horizon, about 2.6′ at 20°, just under 1′ at 45°. Subtracted.

  5. Parallax

    HP · cos H for the moon, Venus and Mars; NauticTools2 calculates the horizontal parallax HP from date and time. Added.

  6. Result

    Observed altitude Ho and the total correction.

Worked examples

Star Vega: Hs = 58°33.0′, index correction −1.0′, height of eye 3 m. What is Ho?

Hs + IC = 58°33.0′ − 1.0′ = 58°32.0′
Dip = −3.1′ · refraction = −0.6′
Total correction = −3.7′
Ho = 58°28.3′

Sun, lower limb, on 22 October 2026: Hs = 30°00.0′, index correction −1.0′, height of eye 3 m.

Hs + IC = 29°59.0′
Dip −3.1′ · semi-diameter +16.1′ · refraction −1.7′
Total correction = +11.3′
Ho = 30°10.3′

Star Shaula: Hs = 26°59.0′, index correction −1.0′, height of eye 3 m.

Hs + IC = 26°58.0′ · total correction = −5.0′
Ho = 26°53.0′

Things to watch out for

How it works in NauticTools2

  1. Enter the reading

    Sextant altitude Hs in degrees and minutes, index correction and height of eye.

  2. Choose the body

    Sun, moon, Venus, Mars or star (also for Jupiter and Saturn). For the sun and moon the app asks for lower or upper limb; a line under or over the name shows the choice.

  3. Date and time

    For the sun only the date, for the semi-diameter. For the moon, Venus and Mars also the time: NauticTools2 calculates the horizontal parallax from it, which can still be overwritten.

  4. Calculate

    Altitude above the horizon, total correction and Ho appear in the result, every correction with its sign in the working. Inputs can be saved and the result printed.

Frequently asked questions

What is the difference between Hs and Ho?

Hs is the sextant reading. Corrected for index error it becomes the altitude above the sea horizon. After dip, refraction and – depending on the body – semi-diameter and parallax you get the observed altitude Ho.

How large is the dip?

1.779 · √(height of eye) in minutes of arc: about 3.1′ at 3 m, about 5.6′ at 10 m.

Why is the sun usually measured on its lower limb?

The lower limb can be set on the horizon most precisely. To refer the altitude to the centre, the semi-diameter of about 16′ is added; for the upper limb it is subtracted.

Related tools

NauticTools2 is free and runs on Windows 10 and 11. An Android version is in preparation.

Get it from the Microsoft Store