LESSON%2019:%20The%20Marine%20Sextant,%20and%20Determination%20of%20Observed%20Altitude - PowerPoint PPT Presentation

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LESSON%2019:%20The%20Marine%20Sextant,%20and%20Determination%20of%20Observed%20Altitude

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a celestial body (star, sun, moon, or planet) the visible horizon. Use of the Sextant. A sextant is used to determine the sextant altitude (hs) of a celestial body. ... – PowerPoint PPT presentation

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Title: LESSON%2019:%20The%20Marine%20Sextant,%20and%20Determination%20of%20Observed%20Altitude


1
LESSON 19The Marine Sextant, and Determination
of Observed Altitude
  • Learning Objectives
  • Know the purpose of a marine sextant.
  • Apply proper procedures to determine the observed
    altitude (Ho) of a celestial body.

2
The Marine Sextant
  • A marine sextant is nothing more than a device
    designed to measure, with a great deal of
    precision, the angle between two objects.
  • In celestial navigation, these objects are
  • a celestial body (star, sun, moon, or planet)
  • the visible horizon.

3
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4
Use of the Sextant
  • A sextant is used to determine the sextant
    altitude (hs) of a celestial body.
  • First, we have to decide which stars to observe
    this is done using a Rude Starfinder or other
    methods.
  • When making an observation, the star should look
    as shown in the next slide...

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6
Determination of Observed Altitude (Ho)
  • We must make some corrections to hs to come up
    with the Ho, which we need to use the
    altitude-intercept method.

7
Determination of Observed Altitude (Ho)
  • These corrections account for the following
  • index error (error in the sextant itself)
  • difference between visible and celestial horizon,
    due to the observers height of eye
  • adjustment to the equivalent reading at the
    center of the earth and the center of the body
  • refractive effects of the earths atmosphere

8
Determination of Ho
  • The corrections needed to convert from the
    sextant altitude (hs) to observed altitude (Ho)
    are
  • 1. Index Correction (IC) - sextant error
  • 2. Dip (D) - height of eye
  • 3. Altitude Correction (Alt Corr) -refractive
    effects of the atmosphere

9
1. Index Correction (IC)
  • Error present in the sextant itself is known as
    index error (IC).
  • This error is easily determined by setting the
    sextant to zero and observing the horizon if
    there is no error, the view looks like that of
    the following slide...

10
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11
Index Correction
  • Often, however, the sextant has a slight error.
    In this case, the view is as follows

12
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13
Index Correction
  • To account for this sextant error, we apply an
    index correction (IC).
  • This correction number is a function of the
    individual sextant itself.

14
2. Dip Correction (D)
  • Next, we must account for the difference between
    the celestial horizon and the visible horizon,
    due to our height of eye.
  • This is known as the dip correction (D).
  • Values of the dip correction are tabulated inside
    the front cover of the Nautical Almanac.

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16
Apparent Altitude
  • Now, by applying the index correction (IC) and
    the dip correction (D), we can determine the
    apparent altitude (ha).
  • ha hs IC D
  • Note that this is not yet the observed altitude
    (Ho) required for our calculations.

17
3. Altitude Correction
  • The third correction accounts for the refractive
    effects of the earths atmosphere.
  • Known as the altitude correction, it is tabulated
    inside the front cover of the Nautical Almanac.
  • Ho ha Alt Corr

18
Altitude Correction
19
Determination of Ho
  • Again, the corrections needed to convert from the
    sextant altitude (hs) to observed altitude (Ho)
    were
  • IC (index correction, from sextant error)
  • D (dip, from height of eye)
  • Alt Corr (altitude correction, from refractive
    effects)

20
Additional Corrections
  • These corrections are all that are needed under
    normal circumstances to determine Ho of a star.
  • An additional correction is required if the
    observation is made under non-standard conditions
    of temperature or pressure.

21
Additional Corrections
  • If we are using the sun, moon, or planets, the
    problem becomes a bit more complicated.
  • In addition to the corrections we already
    mentioned, we must also accout for
  • horizontal parallax (sun, moon, Venus, Mars)
  • semidiameter of the body (sun and moon)
  • augmentation (moon)

22
Additional Corrections
  • These additional corrections make determination
    of Ho for the sun, moon, and planets generally
    more difficult than those for a star.
  • For simplicitys sake, well stick to
    determination of Ho for a star.

23
Use of a Strip Chart
  • To aid in making any calculations in celestial
    navigation, we normally use a form called a strip
    chart.
  • An example of a strip chart used for calculating
    Ho of Dubhe is shown on the next slide...

24
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