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Celestial Applications

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... procedures for computing times of sunrise, sunset, and twilight. ... at sunset or sunrise. ... of Times of Sunrise and Sunset. Important for the navigator. ... – PowerPoint PPT presentation

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Title: Celestial Applications


1
Celestial Applications
  • Learning Objectives
  • Know the information that can be obtained from
    the practice of celestial navigation at sea.
  • Know the correct procedures for computing times
    of sunrise, sunset, and twilight.

2
Determination of Latitude
  • As we have already seen, determining position
    using celestial navigation is a lot of work.
  • Under certain circumstances, it is possible to
    determine latitude by using methods which are
    much less time consuming.

3
Determination of Latitude
  • A latitude line (an LOP) can obtained by
    observing a body at meridian passage.
  • Two bodies are commonly used for this type of
    latitude determination
  • Polaris, since it is always due north (and
    therefore always at meridian passage)
  • the sun, when it reaches its highest altitude
    during the day (Local Apparent Noon)

4
Determination of Latitude
  • By observing a body when it is at meridian
    passage, the navigation triangle is reduced to a
    line, greatly simplifying our solution.

5
Determination of Latitude
6
Latitude by Polaris
  • Polaris (the pole star) is so named because it
    lies almost directly above the north pole.
  • Colatitude and coaltitude are one and the same.
  • As a result, when in the northern hemisphere,
    Polaris may be observed, and the altitude of
    Polaris is equivalent to the observers latitude.

7
Latitude by Polaris
8
Latitude by Polaris
  • A cutaway, side view of the earth is helpful in
    showing the relationships involved...

9
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10
Latitude by Polaris
  • In reality, of course, Polaris and the celestial
    Pn are not exactly coincident Polaris wanders a
    bit with respect to the north pole.
  • To account for this, a correction table is
    provided in the Nautical Almanac.

11
Latitude by Local Apparent Noon (LAN)
  • Observation of the sun at meridian transit (high
    noon) is a very convenient method for
    determining latitude.
  • The sun latitude line thus obtained is considered
    one of the most accurate LOPs available.

12
Latitude by Local Apparent Noon (LAN)
  • The suns declination changes from N 23.5 o to S
    23.5 o in the course of each year.
  • As a result, there are a number of different
    relationships possible between the elevated
    celestial pole, position of the sun, and
    observers zenith at LAN.

13
Latitude by LAN
14
Latitude by Local Apparent Noon (LAN)
  • Now well work through an example to illustrate
    the concept.
  • Keep in mind that, in reality, some corrections
    must be applied to our calculations to come up
    with an accurate latitude by LAN. Here we are
    just addressing the theory behind LAN.

15
Determination of Gyro Error
  • Gyro error by Polaris
  • used in Northern latitudes between the equator
    and 65 oN.
  • True azimuth of Polaris is extracted from the
    Nautical Almanac, and compared to the observed
    azimuth of Polaris.

16
Determination of Gyro Error
  • Sun Amplitude Sight
  • sun is observed at sunset or sunrise.
  • At this time, it is easy to measure the true
    azimuth of the sun, since its right on the
    horizon.
  • True azimuth can be found without using a sight
    reduction form, by using either an amplitude
    table or the amplitude angle formula.

17
Gyro Error by Sun Amplitude
18
Gyro Error by Sun Amplitude
  • The previous slide showed the sun at the time of
    equinox at other times of the year, the suns
    declination will be above or below the equator.

19
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20
Gyro Error by Sun Amplitude
  • Obviously, if were not at the equator, the
    geometry is a bit more complicated, but the idea
    is the same.

21
Determination of Gyro Error
  • Azimuth of the Sun
  • Similar to the sun amplitude sight, but can be
    done any time of the day. The true azimuth of
    the sun is calculated using a sight reduction
    form, and compared to the measured value of true
    azimuth.
  • Calculations are more involved since a complete
    sight reduction is required.

22
Determination of Times of Sunrise and Sunset
  • Important for the navigator.
  • Determines the time of twilight, both in the
    morning and evening, when a celestial fix may be
    obtained.
  • May also be important for other operational
    reasons.
  • Calculation requires use the Nautical Almanac and
    the DR plot.

23
Determination of Times of Sunrise and Sunset
  • Good examples are in your text book. Well work
    through one in class.
  • Terms with which you should be familiar
  • Civil twilight (sun6o below the horizon).
  • Nautical twilight (sun 12o below the horizon).
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