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Yachtmaster Ocean revision module 2 of 10

TIME

Celestial Sphere and Time

Source-reviewed coordinate and time chain from body GP, GHA and declination through LHA, Aries and SHA, chronometer correction, UTC date and reconstructable sight records.

8 guided lessons · 8 practice questions · 8 flashcards

Lesson previewBuild the Earth–Sky Coordinate Model1 section shown

Preview lesson

Build the Earth–Sky Coordinate Model

What you will learn

Distinguish the celestial sphere, geographical position, declination, GHA, observer position, altitude and azimuth without treating related coordinates as interchangeable.

The celestial sphere is a working model that projects directions in the sky onto an Earth-centred coordinate system. It helps a navigator describe where a body is for one instant; it is not a physical shell and it does not reveal the observer's position by itself.

Project the Earth's equator and poles outward to define the celestial equator and celestial poles. A body's declination is its angular distance north or south of the celestial equator. Declination therefore behaves like latitude, but it belongs to the body, not to the yacht.

Project the body's direction inward to the Earth's surface. The point where the body would be at the zenith is its geographical position, or GP. The GP's latitude equals the body's declination. Its east–west coordinate is described by Greenwich Hour Angle, measured westward from Greenwich from 0° to 360°.

The observer has a different coordinate pair: latitude and longitude. From that observer, the body has altitude above the horizon and azimuth around the horizon. Sight reduction connects the body coordinates and the assumed observer coordinates to a computed altitude and azimuth; none of the coordinate pairs is a substitute for the others.

Celestial coordinate and time workbench

Keep the coordinate, clock and longitude operations visible

Select a worked state. The diagrams are paired with the complete signed working, result and limitation so no meaning depends on colour or on the sketch alone.

  1. 1Observation time
  2. 2Almanac GHA and Dec
  3. 3Assumed longitude
  4. 4LHA
  5. 5Reduction and plot
Coordinate modelSchematic Earth side view and north-pole dial. The complete signed calculation and limitations are written below the diagram.Declination and geographical positionCelestial equatorGPDec 20.0° NHour angles · north-pole planGreenwichBody hour circleGHA 65.0° · longitude 0.0° E · LHA 65.0°ANGLE KEYGreenwichBody GHAAssumed meridian

Inputs to keep separate

The body, UTC instant and almanac edition belong together. Declination names the body's north/south coordinate; GHA names its westward angle from Greenwich.

Signed working

Project the body's direction to the Earth's surface. Its geographical position has latitude equal to declination and longitude described by GHA.

Result

At this schematic instant the Sun's GP is 20° N with GHA 065°. An observer still needs an assumed position and a sight reduction before a line of position exists.

What it does not prove

The GP is not the observer's position, a fix or the point where the body appears in the observer's sky.

Revision calculation aid only. This schematic is not an almanac page, sight-reduction table, sextant observation, fix or navigation system. It cannot identify a body, verify UTC or chronometer error, choose an assumed position, apply altitude corrections, assess a real sight, replace the current Nautical Almanac, AP3270 or recognised instruction, or direct a real passage. Use the convention printed in the exact maintained publication and worksheet being used.

Worked example

At one stated UTC instant, an almanac entry gives the Sun declination 20°00.0′ N and GHA 065°00.0′.

  1. 1Place the Sun's GP at latitude 20°00.0′ N because GP latitude equals declination.
  2. 2Describe the GP hour circle as 065° westward from Greenwich; do not call 065° the observer's longitude.
  3. 3Keep the yacht's assumed latitude and longitude separate until the sight-reduction step.
  4. 4Keep the observed altitude separate from both coordinate pairs until it is corrected and compared with the computed altitude.

Sense check: Changing the observer's position changes altitude, azimuth and LHA, but it does not change the body's almanac GHA and declination for that same instant.

Build the Earth–Sky Coordinate Model
DeclinationCelestial bodyNorth or south of the celestial equator
GHACelestial body or AriesWestward from Greenwich, 0° to 360°
Latitude and longitudeObserver or assumed positionEarth coordinates
Altitude and azimuthBody as seen by one observerObserver's horizon and true-north reference
LHABody relative to assumed longitudeWestward from the assumed meridian, 0° to 360°

Run a coordinate-ownership check

Before beginning any reduction, write each extracted or observed value under Body, Observer, Observation or Derived result.

  1. 1. Name

    Write the coordinate name in full before using its abbreviation.

  2. 2. Own

    State whether it belongs to the body, observer, observation or calculation.

  3. 3. Reference

    Write Greenwich, celestial equator, horizon or assumed meridian beside the value.

Sense check: A second learner should be able to identify every reference line without relying on where a number happens to sit on the worksheet.

Common mistake or limitation

  • Treating the body's geographical position as the yacht's position or as a completed celestial fix.
  • Calling declination the observer's latitude because the two use north/south angular notation.
  • Mixing GHA, LHA, altitude and azimuth because all are angular quantities.

Recap

  • The celestial sphere is a coordinate model, not a physical shell.
  • GP latitude equals declination; GHA supplies the Greenwich-referenced westward angle.
  • Observer coordinates and horizon coordinates remain separate until the reduction connects them.

Optional quick check

Section 1 of 1

An almanac gives declination 18° N and GHA 074° for a body. What can be concluded immediately?

Choose one answer