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CHAPTER 1
INTRODUCTION TO MARINE NAVIGATION
DEFINITIONS
100. The Art And Science Of Navigation
with frequent or constant determination of position
relative to nearby geographic and hydrographic
features.
Marine navigation blends both science and art. A good
navigator constantly thinks strategically, operationally, and
tactically. He plans each voyage carefully. As it proceeds,
he gathers navigational information from a variety of
sources, evaluates this information, and determines his
ship’s position. He then compares that position with his
voyage plan, his operational commitments, and his pre-
determined “dead reckoning” position. A good navigator
anticipates dangerous situations well before they arise, and
always stays “ahead of the vessel.” He is ready for naviga-
tional emergencies at any time. He is increasingly a
manager of a variety of resources--electronic, mechanical,
and human. Navigation methods and techniques vary with
the type of vessel, the conditions, and the navigator’s
experience. The navigator uses the methods and techniques
best suited to the vessel, its equipment, and conditions at
hand.
Some important elements of successful navigation
cannot be acquired from any book or instructor. The science
of navigation can be taught, but the art of navigation must
be developed from experience.
Celestial navigation involves reducing celestial
measurements taken with a sextant to lines of
position using calculators or computer programs, or
by hand with almanacs and tables or using spherical
trigonometry.
Radio navigation uses radio waves to determine
position through a variety of electronic devices.
Radar navigation uses radar to determine the
distance from or bearing of objects whose position is
known. This process is separate from radar’s use in
collision avoidance.
Satellite navigation uses radio signals from
satellites for determining position.
Electronic systems and integrated bridge concepts are
driving navigation system planning. Integrated systems
take inputs from various ship sensors, electronically and
automatically chart the position, and provide control
signals required to maintain a vessel on a preset course. The
navigator becomes a system manager, choosing system
presets, interpreting system output, and monitoring vessel
response.
In practice, a navigator synthesizes different method-
ologies into a single integrated system. He should never
feel comfortable utilizing only one method when others are
also available. Each method has advantages and
disadvantages. The navigator must choose methods
appropriate to each situation, and never rely completely on
only one system.
With the advent of automated position fixing and
electronic charts, modern navigation is almost completely
an electronic process. The mariner is constantly tempted to
rely solely on electronic systems. But electronic navigation
systems are always subject to failure, and the professional
mariner must never forget that the safety of his ship and
crew may depend on skills that differ little from those
practiced generations ago. Proficiency in conventional
piloting and celestial navigation remains essential.
101. Types of Navigation
Methods of navigation have changed throughout
history. New methods often enhance the mariner’s ability to
complete his voyage safely and expeditiously, and make his
job easier. One of the most important judgments the
navigator must make involves choosing the best methods to
use. Each method or type has advantages and
disadvantages, while none is effective in all situations.
Commonly recognized types of navigation are listed below.
Dead reckoning (DR) determines position by
advancing a known position for courses and
distances. A position so determined is called a dead
reckoning (DR) position. It is generally accepted that
only course and speed determine the DR position.
Correcting the DR position for leeway, current
effects, and steering error result in an estimated
position (EP) .
Piloting involves navigating in restricted waters
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INTRODUCTION TO MARINE NAVIGATION
102. Phases of Navigation
The navigator’s position accuracy requirements, his fix
interval, and his systems requirements differ in each phase.
The following table can be used as a general guide for
selecting the proper system(s).
Four distinct phases define the navigation process. The
mariner should choose the system mix that meets the
accuracy requirements of each phase.
Inland Waterway Phase : Piloting in narrow canals,
channels, rivers, and estuaries.
Inland
Harbor/
Approach
Coastal
Ocean
Harbor/Harbor Approach Phase : Navigating to a
harbor entrance through bays and sounds, and
negotiating harbor approach channels.
DR
X
X
X
X
Piloting
X
X
X
Celestial
X
X
Radio
X
X
X
Coastal Phase : Navigating within 50 miles of the
coast or inshore of the 200 meter depth contour.
Radar
X
X
X
Satellite
X*
X
X
X
Ocean Phase : Navigating outside the coastal area in
the open sea.
Table 102. The relationship of the types and phases of
navigation. * With SA off and/or using DGPS
NAVIGATION TERMS AND CONVENTIONS
103. Important Conventions and Concepts
observatory as a reference. The publication by the
Observatory of the first British Nautical Almanac in 1767
further entrenched Greenwich as the prime meridian. An
unsuccessful attempt was made in 1810 to establish
Washington, D.C. as the prime meridian for American
navigators and cartographers. In 1884, the meridian of
Greenwich was officially established as the prime meridian.
Today, all maritime nations have designated the Greenwich
meridian the prime meridian, except in a few cases where
local references are used for certain harbor charts.
Charts are graphic representations of areas of the
Earth, in digital or graphic form, for use in marine or air
navigation. Nautical charts, whether in digital or paper
form, depict features of particular interest to the marine
navigator. Charts have probably existed since at least 600
B.C. Stereographic and orthographic projections date from
the 2nd century B.C. In 1569 Gerardus Mercator published
a chart using the mathematical principle which now bears
his name. Some 30 years later, Edward Wright published
corrected mathematical tables for this projection, enabling
other cartographers to produce charts on the Mercator
projection. This projection is still the most widely used.
Sailing Directions or pilots have existed since at least
the 6th century B.C. Continuous accumulation of naviga-
tional data, along with increased exploration and trade, led
to increased production of volumes through the Middle
Ages. “Routiers” were produced in France about 1500; the
English referred to them as “rutters.” In 1584 Lucas
Waghenaer published the Spieghel der Zeevaerdt (The
Mariner’s Mirror) , which became the model for such
publications for several generations of navigators. They
were known as “Waggoners” by most sailors.
The compass was developed about 1000 years ago.
The origin of the magnetic compass is uncertain, but
Throughout the history of navigation, numerous terms
and conventions have been established which enjoy
worldwide recognition. The professional navigator, to gain
a full understanding of his field, should understand the
origin of certain terms, techniques, and conventions. The
following section discusses some of the important ones.
Defining a prime meridian is a comparatively recent
development. Until the beginning of the 19th century, there
was little uniformity among cartographers as to the
meridian from which to measure longitude. But it mattered
little because there existed no method for determining
longitude accurately.
Ptolemy, in the 2nd century AD, measured longitude
eastward from a reference meridian 2 degrees west of the
Canary Islands. In 1493, Pope Alexander VI established a
line in the Atlantic west of the Azores to divide the
territories of Spain and Portugal. For many years, cartog-
raphers of these two countries used this dividing line as the
prime meridian. In 1570 the Dutch cartographer Ortelius
used the easternmost of the Cape Verde Islands. John
Davis, in his 1594 The Seaman’s Secrets , used the Isle of
Fez in the Canaries because there the variation was zero.
Most mariners paid little attention to these conventions and
often reckoned their longitude from several different capes
and ports during a voyage.
The meridian of London was used as early as 1676, and
over the years its popularity grew as England’s maritime
interests increased. The system of measuring longitude both
east and west through 180
°
may have first appeared in the
middle of the 18th century. Toward the end of that century,
as the Greenwich Observatory increased in prominence,
English cartographers began using the meridian of that
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INTRODUCTION TO MARINE NAVIGATION
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Norsemen used it in the 11th century, and Chinese
navigators used the magnetic compass at least that early and
probably much earlier. It was not until the 1870s that Lord
Kelvin developed a reliable dry card marine compass. The
fluid-filled compass became standard in 1906.
Variation was not understood until the 18th century,
when Edmond Halley led an expedition to map lines of
variation in the South Atlantic. Deviation was understood
at least as early as the early 1600s, but adequate correction
of compass error was not possible until Matthew Flinders
discovered that a vertical iron bar could reduce certain
types of errors. After 1840, British Astronomer Royal Sir
George Airy and later Lord Kelvin developed
combinations of iron masses and small magnets to
eliminate most magnetic compass error.
The gyrocompass was made necessary by iron and
steel ships. Leon Foucault developed the basic gyroscope in
1852. An American (Elmer Sperry) and a German (Anshutz
Kampfe) both developed electrical gyrocompasses in the
early years of the 20th century. Ring laser gyrocompasses
and digital flux gate compasses are gradually replacing
traditional gyrocompasses, while the magnetic compass
remains an important backup device.
The log is the mariner’s speedometer. Mariners
originally measured speed by observing a chip of wood
passing down the side of the vessel. Later developments
included a wooden board attached to a reel of line. Mariners
measured speed by noting how many knots in the line
unreeled as the ship moved a measured amount of time;
hence the term knot. Mechanical logs using either a small
paddle wheel or a rotating spinner arrived about the middle
of the 17th century. The taffrail log still in limited use today
was developed in 1878. Modern logs use electronic sensors
or spinning devices that induce small electric fields propor-
tional to a vessel’s speed. An engine revolution counter or
shaft log often measures speed aboard large ships. Doppler
speed logs are used on some vessels for very accurate speed
readings. Inertial and satellite systems also provide highly
accurate speed readings.
The Metric Conversion Act of 1975 and the Omnibus
Trade and Competitiveness Act of 1988 established the
metric system of weights and measures in the United
States. As a result, the government is converting charts to
the metric format. Notwithstanding the conversion to the
metric system, the common measure of distance at sea is the
nautical mile .
The current policy of the National Imagery and
Mapping Agency (NIMA) and the National Ocean
Service (NOS) is to convert new compilations of
nautical, special purpose charts, and publications to the
metric system. All digital charts use the metric system.
This conversion began on January 2, 1970. Most modern
maritime nations have also adopted the meter as the
standard measure of depths and heights. However, older
charts still on issue and the charts of some foreign
countries may not conform to this standard.
The fathom as a unit of length or depth is of obscure
origin. Posidonius reported a sounding of more than 1,000
fathoms in the 2nd century B.C. How old the unit was then
is unknown. Many modern charts are still based on the
fathom, as conversion to the metric system continues.
The sailings refer to various methods of mathemat-
ically determining course, distance, and position. They
have a history almost as old as mathematics itself. Thales,
Hipparchus, Napier, Wright, and others contributed the
formulas that permit computation of course and distance by
plane, traverse, parallel, middle latitude, Mercator, and
great circle sailings.
104. The Earth
The Earth is an irregular oblate spheroid (a sphere
flattened at the poles). Measurements of its dimensions and
the amount of its flattening are subjects of geodesy.
However, for most navigational purposes, assuming a
spherical Earth introduces insignificant error. The Earth’s
axis of rotation is the line connecting the north and south
geographic poles.
A great circle is the line of intersection of a sphere and
a plane through its center. This is the largest circle that can
be drawn on a sphere. The shortest line on the surface of a
sphere between two points on the surface is part of a great
circle. On the spheroidal Earth the shortest line is called a
geodesic. A great circle is a near enough approximation to
Figure 104a. The planes of the meridians at the polar axis.
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INTRODUCTION TO MARINE NAVIGATION
a geodesic for most problems of navigation. A small circle
is the line of intersection of a sphere and a plane which does
not pass through the center. See F igure 104a.
The term meridian is usually applied to the upper
branch of the half-circle from pole to pole which passes
through a given point. The opposite half is called the lower
branch.
. It is designated east (E) or west (W) to
indicate the direction of measurement.
The difference of longitude (DLo) between two
places is the shorter arc of the parallel or the smaller angle
at the pole between the meridians of the two places. If both
places are on the same side (east or west) of Greenwich,
DLo is the numerical difference of the longitudes of the two
places; if on opposite sides, DLo is the numerical sum
unless this exceeds 180
minus the sum.
The distance between two meridians at any parallel of
latitude, expressed in distance units, usually nautical miles,
is called departure (p, Dep.) . It represents distance made
good east or west as a craft proceeds from one point to
another. Its numerical value between any two meridians
decreases with increased latitude, while DLo is numerically
the same at any latitude. Either DLo or p may be designated
east (E) or west (W) when appropriate.
°
, when it is 360
°
106. Distance on the Earth
Figure 104b. The equator is a great circle midway
between the poles.
Distance, as used by the navigator, is the length of the
rhumb line connecting two places. This is a line making
the same angle with all meridians. Meridians and parallels
which also maintain constant true directions may be con-
sidered special cases of the rhumb line. Any other rhumb
line spirals toward the pole, forming a loxodromic curve
or loxodrome . See Figure 106 . Distance along the great
A parallel or parallel of latitude is a circle on the
surface of the Earth parallel to the plane of the equator.
It connects all points of equal latitude. The equator is a
great circle at latitude 0
. See Figure 104b. The poles are
single points at latitude 90
°
°
. All other parallels are small
circles.
105. Coordinates
at the poles. It is
designated north (N) or south (S) to indicate the direction of
measurement.
The difference of latitude ( l , DLat.) between two
places is the angular length of arc of any meridian between
their parallels. It is the numerical difference of the latitudes
if the places are on the same side of the equator; it is the sum
of the latitudes if the places are on opposite sides of the
equator. It may be designated north (N) or south (S) when
appropriate. The middle or mid-latitude (Lm) between
two places on the same side of the equator is half the sum
of their latitudes. Mid-latitude is labeled N or S to indicate
whether it is north or south of the equator.
The expression may refer to the mid-latitude of two
places on opposite sides of the equator. In this case, it is
°
at the equator to 90
°
Figure 106. A loxodrome.
equal to half the difference between the two latitudes and
takes the name of the place farthest from the equator.
Longitude (l, long.) is the angular distance between
the prime meridian and the meridian of a point on the Earth,
measured eastward or westward from the prime meridian
through 180
°
Coordinates of latitude and longitude can define any
position on Earth. Latitude (L, lat.) is the angular distance
from the equator, measured northward or southward along
a meridian from 0
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INTRODUCTION TO MARINE NAVIGATION
5
circle connecting two points is customarily designated
great-circle distance . For most purposes, considering the
nautical mile the length of one minute of latitude introduces
no significant error
Speed (S) is rate of motion, or distance per unit of time.
A knot (kn.) , the unit of speed commonly used in
navigation, is a rate of 1 nautical mile per hour. The
expression speed of advance (SOA) is used to indicate the
speed to be made along the intended track. Speed over the
ground (SOG) is the actual speed of the vessel over the
surface of the Earth at any given time. To calculate speed
made good (SMG) between two positions, divide the
distance between the two positions by the time elapsed
between the two positions.
. In this case it is designated
course angle (C) and should be properly labeled to indicate
the origin (prefix) and direction of measurement (suffix).
Thus, C N35
°
or 180
°
°
E=Cn035
°
(000
°
+35
°
), C N155
°
W=Cn
205
°
(360
°
- 155
°
), C S47
°
E = Cn 133
°
(180
°
-47
°
). But Cn
260
°
may be either C N100
°
W or C S80
°
W, depending
upon the conditions of the problem.
Track (TR) is the intended horizontal direction of travel
with respect to the Earth. The terms intended track and
trackline are used to indicate the path of intended travel. See
Figure 107a. The track consists of one or a series of course
lines, from the point of departure to the destination, along
which one intends to proceed. A great circle which a vessel
intends to follow is called a great-circle track , though it
consists of a series of straight lines approximating a great circle
Heading (Hdg., SH) is the direction in which a vessel
is pointed at any given moment, expressed as angular
distance from 000
107. Direction on the Earth
Direction is the position of one point relative to
another. Navigators express direction as the angular
difference in degrees from a reference direction, usually
north or the ship’s head. Course (C, Cn) is the horizontal
direction in which a vessel is intended to be steered,
expressed as angular distance from north clockwise through
360
. It is easy to
confuse heading and course. Heading constantly changes as
a vessel yaws back and forth across the course due to sea,
wind, and steering error.
Bearing (B, Brg.) is the direction of one terrestrial
point from another, expressed as angular distance from
000
°
clockwise through 360
°
. Strictly used, the term applies to direction through the
water, not the direction intended to be made good over the
ground.The course is often designated as true, magnetic,
compass, or grid according to the reference direction.
Track made good (TMG) is the single resultant
direction from the point of departure to point of arrival at
any given time. Course of advance (COA) is the direction
intended to be made good over the ground, and course over
ground (COG) is the direction between a vessel’s last fix
and an EP. A course line is a line drawn on a chart
extending in the direction of a course. It is sometimes
convenient to express a course as an angle from either north
°
(North) clockwise through 360
°
. When measured
from either north or south, it is called
bearing angle (B). Bearing and azimuth are sometimes used
interchangeably, but the latter more accurately refers to the
horizontal direction of a point on the celestial sphere from
a point on the Earth. A relative bearing is measured relative
to the ship’s heading from 000
°
or 180
°
°
(dead ahead) clockwise
. However, it is sometimes conveniently mea-
sured right or left from 000
°
°
at the ship’s head through
. This is particularly true when using the table for Dis-
tance of an Object by Two Bearings.
°
Figure 107a. Course line, track, track made good, and heading.
or south, through 90
°
through 90
through 360
180
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