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A RuckSack primer
The latitude/longitude
geographic coordinate system
By Michael A. Neiger
Copyright 2005 --
2005-05-03
Last modified on
May 3, 2005
E-mail comments or corrections
to author at mneiger@hotmail.com
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Introduction
to the
latitude/longitude coordinate system
Today's latitude/longitude coordinate
system is an extremely accurate and unambiguous way to describe any location
on the earth’s surface. Of all the geographic coordinate systems, it is
the one most often found on maps, charts, and globes. It is also the most
commonly understood and often used coordinate system in existence.
The system consists of an imaginary,
two-coordinate grid overlaid on the earth’s spherical surface. The grid
framework consists of an unlimited number of parallels of latitude, which
are represented by the horizontal lines on a map or globe, and meridians
of longitude, which are represented by the vertical lines on a map or
globe.
The grid system’s zero point--0°
latitude and 0° longitude--is defined
as the place where the north-south running system base line, known as
the prime meridian, crosses the east-west system base line, known as the
equator. It is situated in the Gulf of Guinea in the Atlantic Ocean, about
375 miles south of the coast of Accra, Ghana, in western Africa.
A specific location within the latitude/longitude
grid system is described by two angular descriptors, both of which are
measured with respect to the center, or core, of the earth. A location’s
latitudinal descriptor is represented by the angular deviation of its
local parallel from the equator, or zero-degree line of latitude. A location’s
longitudinal descriptor is represented by the angular deviation of its
local meridian from the prime meridian, or zero-degree line of longitude.
By design, no two locations on the earth’s
surface can have the exact same parallel and meridian combination. In
other words, every latitude/longitude coordinate combination identifies
a unique and individual geographical location on the earth’s surface.
***Lat/lon diagrams
adapted from the U.S. Army's Map
Reading and Land Navigation Field Manual (FM 3-25.26, rev. 20
July 2001, formerly FM 21-26)
An historical overview of the
latitude/longitude coordinate system
The latitude/longitude geographical
coordinate system is the oldest known map-coordinate system in the world.
As far back as 500 BC--some 2,500 years ago--the Greeks were using a rudimentary
version to make celestial and terrestrial measurements and observations.
By observing the sun, moon, planets, and stars with angle- or altitude-measuring
devices, they were able approximate their terrestrial position. For seafarers
of the time, accurately fixing their location while underway could mean
the difference between life and death.
Through the centuries,
the latitude/longitude coordinate system has evolved into an increasingly
accurate means of locating one’s position on the earth’s surface and making
measurements between different terrestrial locations. Along with improvements
in the coordinate system, the last 2,500 years have witnessed the invention
and development of various aids to navigation such as angle-measuring
devices and the timekeeping instruments.
Quadrant. The medieval quadrant
was probably the first angle-measuring instrument utilized for measuring
latitude. As its name implies, the quadrant was configured as a quarter-of-a-circle
(90 degree) arc instrument. Made of wood or brass, this portable, planispheric
(flat), wedge-shaped instrument included two sights situated along one
of its straight edges and a degree scale along its radius. The graduated
degree scale combined with a weighted line, or plumb bob, hung from the
apex, served to indicate a celestial body’s angle, or altitude, from the
horizon.
In the northern hemisphere, latitude
was calculated by measuring the angle between the horizon and the polar
star, and then correcting this figure for the minor deviation between
the polar star and the celestial north pole. In the southern hemisphere,
latitude was calculated by measuring the angle between the horizon and
the sun, and then correcting for the sun’s declination.
Astrolabe. The astrolabe was
a medieval instrument used to measure latitude. Its name was derived from
the Latin words astro, meaning star, and labio, meaning
finder.This portable, angle-measuring instrument may have been invented
in the 3rd century BC by Apollonius of Perga. It was a whole-circle (360
degree) planispheric, angle-measuring device constructed of brass or iron.
Over the ages, it took on many forms.
In its simplest form, it consisted of
two principal parts: the "mater," which was a large, circular
base plate or frame graduated in degrees along its edge; and an "alidade,"
which was a rotating straight rule with a dual-sighting mechanism. Later
models added rotating disks--such as the "rete" and the "tympan,"
for example--that bore celestial diagrams and charts, essentially creating
a two-dimensional celestial model.
Apollonius of Perga
(circa 262 BC-circa 190 BC) was a Greek mathematician, geometrician,
and astronomer. Known as "The Great Geometer," his works included
the Conics (a series of 8 books on the field of conic sections)¸
Cutting-off of a Ratio, Cutting off of an Area, On Determinate Section,
Tangencies, Vergings, On Contacts, On Plane Loci, On the Cylindrical
Helix, Comparison of the Dodecahedron and the Icosahedron, Quick Delivery,
On Unordered Irrationals, and On the Burning Mirror.
Eratosthenes and the lat/lon system.
Some of the initial work on the latitude/longitude coordinate system
was done during the 3rd century BC by Eratosthenes of Cyrene. While he
is credited with charting lines of latitude and longitude on the earth’s
surface, his charting was rudimentary and irregular at best. His system
also relied on inaccurate, terrestrial-based measurements.
Eratosthenes of Cyrene (circa
284 BC-circa 194 BC) was a Greek astronomer, geographer, grammarian,
philosopher, mathematician, scholar of natural history, writer, and
poet. He was the chief librarian at the Alexandrian Museum in Alexandria,
Egypt and is most famous for making the first accurate, scientific measurement
of the earth’s circumference using the sun’s rays--his estimate was
accurate to within 50 miles of today's accepted standard. Hailed as
the father of geodesy--the study of the earth’s size, shape, gravity,
and surface locations--Eratosthenes is also credited with founding scientific
chronology and astronomical geography. He cataloged 675 stars. His works
included Geographica, On Ancient Comedy, Erigone,
Hermes, Hesiod, Duplication of the Cube, On
Means, Platonicus, On the Measurement of the Earth,
Chronographiai, and Catasterisms.
Hipparchus and the lat/lon system.
By the 2nd century BC, Hipparchus of Nicaea had improved upon Eratosthenes’
latitude/longitude coordinate system. He is credited with plotting the
lines of latitude and longitude at regular, fixed intervals. He also increased
the coordinate system’s accuracy by applying trigonometry and spherical
geometry, and relying upon astronomy-based measurements.
Hipparchus of Nicaea, or Hipparchos,
(circa 194 BC-circa 120 BC) was a great Greek astronomer, and mathematician.
Considered the father of the science of astronomy, Hipparchus is credited
with cataloging some 850, or possibly even 1080, stars; determining
the length of the solar year; discovering the eccentricities of solar
orbit and the procession of the equinoxes (his greatest discovery);
determining the relative size of the sun and the moon as well as their
distances from the earth; inventing the planisphere and possibly the
astrolabe; and inventing stereographic projection and chordal trigonometry.
Some of Hipparchus’ 14 works included Commentary on the "Phenomena"
of Aratus and Eudoxus, On the Magnitudes and Distances of the Sun and
Moon, The Movement of the Moon in Latitude, On Bodies
Carried Down by Weight, and On the Displacement of the Tropical
and Equinoctial Points (circa 128 BC)
Ptolemy and the lat/lon system.
In the 2nd century AD, Ptolemy of Alexandria made further improvements
upon Hipparchus’ conception of the latitude/longitude system. In Geographia,
a monumental, eight-volume treatise on general geography, which remained
authoritative until the 15th century, Ptolemy wrote about mathematical
cartography, coined the terms meridian and parallel, and cataloged a number
of place names along with their corresponding latitudes and longitudes.
However, inaccuracies abounded, including his estimate of Eurasia’s longitude,
an error that was said to have encouraged Christopher Columbus to make
his famous 1492 westward sailing voyage, which ultimately resulted in
the discovery of the New World.
Ptolemy of Alexandria (circa
AD 100-circa AD 180), whose full Latin name was Claudius Ptolemaeus,
was a brilliant Greek-Egyptian astronomer, astrologer, mathematician,
geographer, and scientist. A librarian in Alexandria, Egypt, and second
only to Aristotle in influence, Ptolemy’s theories remained immensely
popular for some 1,400 years. His works included Almagest (his
most famous work), Analemma, Planisphaerium, Optica,
Tetrabiblos, and Harmonica.
The magnetic compass. By the
11th century AD--if not earlier--the magnetic compass had been discovered
and was in use. The first compasses were fashioned of lodestone--a naturally-occurring
iron-bearing ore with magnetic properties. The lodestone was attached
to the top of a splinter of wood or a piece of straw, reed, or cork, which
was then floated in a container of water so it could rotate freely and
orient itself in a north-south direction.
Eventually lodestone was used to magnetize
a needle-shaped piece of iron or steel. By the 13th century, rotating
compass needles and compass cards, balanced atop pin-like posts in bowl-shaped
containers, were in use. It was not until the 15th century that compass
users began to realize that their compasses did not point directly to
the terrestrial north pole but to some other nearby location, which came
to be known as the magnetic north pole. By the 19th century, liquid-filled
compasses had replaced dry compasses.
Navigational maps and charts. While
crude maps were drawn on clay tablets and animal skins as far back as
2500 BC by the ancient Babylonians, the Chinese are credited with printing
the first maps during the 12th century AD.
Mercator maps. In 1569, the Mercator
map was developed by Gerardus Mercator. His revolutionary maps used the
Mercator projection--a technique which was named after him--to represent
the earth’s three-dimensional, sphere-shaped surface on two-dimensional
paper. The Mercator projection used the cylindrical projection method
in which both parallels and meridians were represented as straight lines.
This groundbreaking discovery allowed navigators to calculate both distance
and direction from their maps.
Gerhardus Mercator (1512-1594),
or Gerardus or Gerard (his given name was Gerhard or Gerard De Cremer
[or Kremer], but he chose to use his Latin name), was a Flemish cartographer,
court cosmographer (geographer), calligrapher, mathematician, talented
scientific-instrument maker, professor, engraver, and surveyor who is
credited with creating the first modern, 18-sheet world map using his
Mercator projection technique. He created the Atlas, or Cosmographical
Meditations on the Structure of the World, the first modern
atlas (a term he invented for a work envisioned to explain the creation
of the world as well as lay out its complete history). In addition to
publishing numerous notable maps and charts, and constructing celestial
and terrestrial globes, his other works included a thorough guide to
italic lettering as well as On the Use of the Astronomical Ring,
Chronologia, and Tabulae Geographica.
Cross-staff. During the 16th
century AD, the portable cross-staff widely replaced the astrolabe for
calculating latitude. Also known as the Jacob’s staff, the cross-staff
was nothing more than a graduated vertical staff with an adjustable crosspiece
that allowed the user to measure the angle between the horizon and a celestial
body, usually the north star or the sun.
Backstaff. By 1594, John Davis
had improved upon the cross-staff with the development of the portable
backstaff, or shadow-staff, which did not require the user to look directly
into the sun. It was popular for nearly 150 years.
John Davis (circa 1550-1605),
or Davys, was a proficient English seaman, explorer, first-rate navigator,
naval combatant, writer, and inventor. He commanded the Black Dog
against the Spanish Armada in 1588, invented the double quadrant, and
devised the ship’s log, which became a standard tool for future navigators.
Before his death at the hands of Japanese pirates near Singapore, his
discoveries included the Davis Strait, which is located between Greenland
and Canada’s Baffin Island and bears his name, and the Falkland Islands.
Known as the father of arctic discovery for his efforts to find a northwest
passage to India, his nautical works included The Seaman’s Secrets
(1594) and The World’s Hydrographical Description (1595).
Vernier scale. In 1631, Pierre
Vernier invented the graduated scale--or vernier scale--which represented
a tremendous improvement over the transversals method (a geometric technique
where a straight line cuts a system of other lines) of reading angular
scales and linear rules. This mechanical device consisted of two parallel,
sliding scales--a large main scale and a smaller auxiliary, or vernier,
scale--that greatly increased the accuracy with which fractional parts
or subdivisions of a single division on a fixed scale could be read.
Pierre Vernier (circa 1580-1637)
was a French mathematician, government official, and inventor who published
a number of works including The Construction, Uses, and Properties
of a New Mathematical Quadrant (1631).
Descartes and the lat/lon system.
By the 17th century AD, Rene Descartes had further refined and systemized
the latitude/longitude coordinate system. In Geometry, his famous
1637 work, Descartes laid out the principles of co-ordinate or analytical
geometry and applied them to the latitude/longitude coordinate system.
Rene Descartes (1596-1650)
was a celebrated French philosopher, mathematician, and scientist. Known
as the father of modern, rationalistic philosophy, Descartes’ philosophy
came to be called Cartesianism. His accomplishments included inventing
co-ordinate or analytic geometry through the merging of algebra and
geometry. An opponent of Scholastic Aristotelianism, Descartes devoted
himself to explaining man and the universe through the application of
mathematics, logical reasoning, and experimentation. He became famous
for the Latin axiom, cogito, ergo sum, which translated to "I
think, therefore I am." Descartes’ works included Discourse
on the Method for Rightly Conducting One’s Reason, and Searching for
Truth in the Sciences (1637; his most famous work), which became
known as the Discourse on Method; Meditations on First Philosophy
(1641; his principal philosophical work); and Principles of Philosophy
(1644).
Telescopic sighting mechanism.
In 1640, William Gascoigne invented the telescopic sight, which greatly
improved the accuracy with which a telescope could be aimed. His design
combined crosshairs fashioned from spider web material with a refractor.
William Gascoigne (circa 1612-1644),
or Gascoygne, was an English amateur astronomer, inventor, and soldier
who invented the micrometer in 1641 and developed glass-grinding methods.
Meridian transit. Also known
as a meridian circle, transit circle, transit instrument, transit telescope,
or Roemer’s transit, the meridian transit was a non-portable, angle-measuring
instrument used in astronomical observatories. Invented around 1684 by
Ole Roemer, the meridian transit consisted of a refracting telescope with
cross-hair sights mounted in such a way that it could only pivot in a
north-south manner along the plane of the meridian. It also included a
finely-graduated vertical circle for making accurate readings of a celestial
body’s ascension and declination.
Olaus Roemer (1644-1710), also
known as Ole or Olaf Romer, was a Danish professor, politician, astronomer,
and mathematician who was most famous for measuring the velocity of
light. He also invented the altazimuth, the equatorial telescope, and
may have helped Daniel Fahrenheit develop the Fahrenheit mercury thermometer.
Octant or double-reflecting quadrant.
About 1731, a portable device called the octant--which was first proposed
by Sir Isaac Newton in the late 1600s--was simultaneously invented by
an Englishman named John Hadley and an American named Thomas Godfrey.
As its name implies, the portable octant was configured as an eighth-of-a-circle
(45 degree) arc instrument. It could measure angles or altitudes of up
to 90 degrees and quickly replaced the backstaff developed by John Davis
in 1594.
This handheld astronomical instrument
utilized two mirrors; index or vernier scales; plane or telescopic sights;
and a plumb line or spirit level to measure the altitude of celestial
bodies such as the moon, sun, and stars. Also known as the seaman’s reflecting
quadrant, this instrument was often referred to by the surname of its
inventor or the person who happened to improve upon its design (e.g.,
Hadley’s quadrant, Godfrey’s quadrant, etc.).
John Hadley (1682-1744) was
a British mathematician, mechanician (mechanic), astronomer, and inventor
who took the rudimentary reflecting telescope of his time and improved
its power and precision to a point where the instrument was favored
by astronomers into the 18th century. His first telescope, built in
1721, was called the Gregorian reflector telescope.
Thomas Godfrey (1704-1749)
was an American mathematician, astronomer, plumber, glazier, artisan,
mechanician, and inventor who at one time rented a room from his friend,
Benjamin Franklin. Despite having no formal education, Godfrey was described
in the July 1758 issue of American Magazine as a "singular
phenomenon" in the "learned world." He was said to be
gifted with "a kind of natural or intuitive knowledge of the abstrusest
parts of mathematics and astronomy."
Sextant. The sextant, which had
its origins in Hadley’s and Godfrey’s reflecting quadrants, was perfected
around 1757 and quickly replaced the octant. As its name implies, the
portable sextant was configured as a sixth-of-a-circle (60 degree) arc
instrument. It could measure angles or altitudes of up to 120 degrees.
Some sextants were constructed with arcs measuring 45 degrees, 72 degrees,
and 90 degrees.
The sextant consisted of a frame and
cross braces made of metal--often brass--or ebony wood, a rotating radial
arm, an edge graduated in degrees, two mirrors--called the horizon glass
and the index glass--and a sighting telescope.
Nautical almanac. In 1766, Nevil
Maskelyne compiled the Nautical Almanac, the first accurate nautical
tables that provided navigators with the day-to-day positions of celestial
bodies necessary for accurate latitude and longitude calculations.
Nevil Maskelyne (1732-1811)
was an English astronomer, ordained minister, and author. He is credited
with devising a means to measure the density of the earth as well as
inventing the prismatic micrometer. His astronomical works included
The British Mariner’s Guide (1763), Philosophical Transactions,
and a standard catalog of the stars.
Marine chronometer. Despite the
compilation of almanacs and tables to predict the day-to-day positions
of celestial bodies and the development of "lunar-distance"
techniques, accurate longitudinal readings were not possible until the
18th century when John Harrison invented a precise timekeeping instrument.
Known as a portable marine chronometer, it allowed sailors to accurately
tell time at sea and thereby more precisely calculate their longitude.
Harrison’s invention was motivated in
large part by the British Board of Longitude, which in 1713 had posted
a reward of 20,000 lira to anyone who developed a timepiece that could
keep precise time while at sea. Inaccurate longitudinal calculations had
been blamed for a string of deadly maritime disasters during this period.
In 1728, Harrison began working on a marine clock known as timepiece No.
1. By 1761, he had perfected a marine chronometer called timepiece No.
4--a five-inch diameter pocket watch. He did not receive the entire, 20,000-lira
award until King George III intervened on his behalf in 1773, just three
years before the inventor’s death.
John Harrison (1693-1776) was
an English carpenter, horologist (clock and watchmaker), inventor, and
mechanician. In addition to dedicating much of his life to perfecting
the marine chronometer, he also constructed clocks and surveying instruments.
He is credited with inventing the compound pendulum in 1726. Called
the gridiron compensating pendulum, this clock mechanism could self-compensate
for error-causing climatic (temperature) changes. Harrison also invented
the recoil escapement mechanism and a clock spring mechanism that allowed
a clock to continue keeping time while it was being wound.
Parallels of latitude
Parallels of latitude are the horizontal
lines that often appear on maps, charts, and globes. They are also referred
to as lines of latitude, latitude lines, or simply parallels. The word
latitude--which is often abbreviated as lat.--is a Middle English word
derived from the Latin terms latitudo, which meant breadth or width,
and latus, which meant broad.
Parallels are imaginary, equally-spaced,
rings that encircle the earth’s surface in an east-west fashion. They
run perpendicular to meridians of longitude and parallel to both the equator
and each other. Put another way, a line of latitude cuts across the north-south
axis of the earth much like a knife cuts across the core of an onion as
it is sliced. 
No matter what their longitudinal coordinates,
all locations on a specific parallel have exactly the same latitudinal
coordinate. Following this same principle, every location on a specific
meridian has a unique and individual latitudinal coordinate. While it
is customary for cartographers to show only major parallels, and possibly
their major subdivisions, on maps, charts, and globes, there is no set
number of parallels: the number of parallels is unlimited.
Since the earth is not a perfect sphere,
but is somewhat flattened near its geographic poles, the length of a degree
of latitude (or distance between two parallels spaced one degree apart)
varies slightly from 68.703 statute miles (110.567 kilometers) at the
equator to 69.407 statute miles (111.699 kilometers) at the north and
south poles.
Around the 46th parallel in Michigan's
Upper Peninsula, one second of latitude equals about 100 feet (while one
second of longitude equals about 69 feet).
***Lat/lon diagram
adapted from the U.S. Army's Map
Reading and Land Navigation Field Manual (FM 3-25.26, rev. 20
July 2001, formerly FM 21-26)
Notable parallels
Arctic Circle
Located at 66 degrees, 30 minutes north
latitude, the arctic circle marks the line of demarcation between the
northern frigid zone, or north polar region, and the northern temperate
zone. This imaginary circle around the earth also marks the point north
of which the sun is not visible every day of the year. Situated about
1,624 miles from the geographic north pole, this parallel of latitude
passes through Alaska, Canada, Greenland, the northern Atlantic Ocean,
Norway, Sweden, Finland, Russia, and the Bering Sea.
Tropic of Cancer
Located at 23 degrees, 27 minutes
north latitude, the Tropic of Cancer marks the northern limit of the earth’s
tropical--or torrid--zone. This imaginary line around the earth--or parallel
of latitude--passes through the North Pacific Ocean, Mexico, the Gulf
of Mexico, the Bahamas, the northern Atlantic Ocean, the Western Sahara,
Mauritania, Mali, Algeria, Libya, Egypt, the Red Sea, Saudi Arabia, the
United Arab Emirates, Oman, the Arabian Sea, India, Bangladesh, Myanmar,
China, the South China Sea, and Taiwan.
Cancer. The Tropic of Cancer
takes its name from the Cancer constellation, which occupies a 30-degree-segment
of the 18-degree-wide zoidacal constellation--a swath of the heavens,
known as the elliptic, that the sun traverses annually. The Cancer constellation
is the fourth of 12 zodiacal constellations. This extremely faint, spring
constellation is located in the equatorial region of the northern hemisphere,
directly overhead, between Gemini and Leo. This constellation is also
known as the Crab since the English term Cancer is derived from the Latin
word Cancer, which means Crab.
Summer solstice. The Tropic
of Cancer represents the northernmost point, north of the equator, where
the sun appears directly overhead. When this occurs at noon on June 20,
21, or 22 of each year, it marks the arrival of the summer solstice and
the longest day of the year in its hemisphere. The summer solstice represents
the start of summer in the northern hemisphere (and winter in the southern
hemisphere) and is sometimes referred to as the June solstice. The English
word solstice is derived from the Latin term solstitium, which
originated from the Latin terms sol and stit, meaning "sun"
and "to stop or make stand," respectively, which is what the
sun appears to do on that day.
***Lat/lon diagram
adapted from the U.S. Army's Map
Reading and Land Navigation Field Manual (FM 3-25.26, rev. 20
July 2001, formerly FM 21-26)
Equator
Located at zero degrees latitude, the
equator represents the imaginary line around the earth--or parallel of
latitude--that lies an equal distance from both the geographic north and
south poles. It serves to divide the earth into two hemispheres: the southern
and northern. Measuring about 24,901 miles in length, the equator passes
through the Pacific Ocean, Ecuador, Columbia, Brazil, the Atlantic Ocean,
Gabon, the Congo, Zaire, Uganda, Kenya, Somalia, the Indian Ocean, and
Indonesia.
Tropic of Capricorn
Located at 23 degrees, 27 minutes
south latitude, the Tropic of Capricorn marks the southern limit of the
earth’s tropical--or torrid--zone. This imaginary line around the earth--a
parallel of latitude--passes through the southern Pacific Ocean, Chile,
Argentina, Paraguay, Brazil, South Atlantic Ocean, Namibia, Botswana,
South Africa, Mozambique, Indian Ocean, Madagascar, Indian Ocean, and
Australia.
Capricorn. The Tropic of Capricorn,
or Capricornus, takes its name from the 30-degree-long Capricorn constellation,
which is the tenth of 12 zodiacal constellations situated in an 18-degree-wide
swath of the heavens--known as the elliptic--that the sun traverses annually.
Also known as the Sea Goat or Horned Goat, this faint, autumn constellation
is located in the equatorial region of the southern hemisphere, directly
overhead, between Aquarius and Sagittarius. The English term Capricorn
is derived from the Latin term Capricornus, which originated from
the Latin terms caper and cornu, meaning "goat"
and "horn," respectively.
Winter solstice. The Tropic
of Capricorn represents the southernmost point, south of the equator,
where the sun appears directly overhead. When this occurs at noon on December
21 or 22 of each year, it marks the arrival of the winter solstice and
the shortest day of the year in the northern hemisphere. The winter solstice
represents the start of winter in the northern hemisphere (and summer
in the southern hemisphere) and is sometimes referred to as the December
solstice. The English word solstice is derived from the Latin term solstitium,
which originated from the Latin terms sol and stit, meaning
"sun" and "to stop or make stand," respectively, which
is what the sun appears to do on that day.
Antarctic Circle
Located at 66 degrees, 30 minutes south
latitude, the antarctic circle marks the line of demarcation between the
southern frigid zone, or south polar region, and the southern temperate
zone. This imaginary circle around the earth also marks the point south
of which the sun is not visible every day of the year. Situated about
1,624 miles from the geographic south pole, this imaginary line around
the earth--or parallel of latitude--passes through the ice-encrusted continent
of Antartica as well as the Southern Ocean, or the Antarctic Ocean.
Latitudinal coordinates
A specific location’s latitudinal coordinate
is its northerly, or southerly, angular distance along the earth’s surface
relative to the equator. It is measured as an arc, along a meridian of
longitude, perpendicular to the equator, which is by convention the zero
degree parallel.
The
numerical coordinate
Latitudinal coordinates--which can range
up to one-quarter of the earth’s circumference, from zero degrees (at
the equator) to 90 degrees (at the north, or south, terrestrial poles)--are
angles traditionally expressed in a degrees-minutes-seconds format: 45°
30’ 30.30"N. By custom, degree units are signified by the degree
° symbol; minutes are signified by the
minutes ‘ symbol, a single tick mark or apostrophe; and seconds are signified
by the seconds " symbol, or a double tick mark or quotation mark.
In the degree-based latitude and longitude measurement system, a circle
is made up of 360 degrees; a degree is made up of 60 minutes (a minute
equals 1/60 of a degree); and a minute is made up of 60 seconds (a second
equals 1/60 of a minute, or 1/3600 of a degree).
In addition to a "degrees, minutes,
seconds" format, latitudinal coordinates are sometimes expressed
in shortened forms such as a "degrees and minutes" format, where
the parts of a minute are represented in a decimal-fraction form (e.g.,
45° 30.5001’N), or a "degrees"
format, where the parts of a degree are represented in decimal-fraction
form (e.g., 45.5084166° N).
While decimal-fraction format coordinates
are a common coordinate format option in Global Positioning System (GPS)
units and mapping software programs, they are very cumbersome for plotting
on topographic maps, especially in the field. Information on how to convert
latitude/longitude coordinates from one format to another, or convert
them to or from the UTM coordinate system, is discussed below.
***Lat/lon diagram
adapted from the U.S. Army's Map
Reading and Land Navigation Field Manual (FM 3-25.26, rev. 20
July 2001, formerly FM 21-26)
The
hemispherical designator
Latitudinal coordinates are typically
followed by a single letter or symbol that designates whether they are
located north of the equator--in the northern hemisphere--or south of
the equator--in the southern hemisphere. North latitudinal coordinates
are customarily followed by either the letter "N" or the plus
"+" symbol. South latitudinal coordinates are customarily followed
by either the letter "S" or the minus "-" symbol.
Since the continental United States
lies entirely within the northern hemisphere for latitudinal purposes,
many U.S. maps and charts do not include a northern hemisphere designator
with the latitudinal coordinates printed along the neatlines in the margins
of the map or chart. Cartographers assume the user will know the latitudinal
coordinate is in the northern hemisphere.
By convention, latitude/longitude coordinate
combinations always list the latitudinal coordinate first and the longitudinal
coordinate second.
Meridians of longitude
Meridians of longitude are the vertical
lines that often appear on maps, charts, and globes. They are also referred
to as lines of longitude, longitudinal lines, meridians of longitude,
geographic meridians, or simply meridians. The word longitude--which is
often abbreviated as lon. or long.--is a Middle English word derived from
the Latin terms longitudo, which meant length, and longus,
which meant long.
Meridians are the imaginary, equally-spaced,
half-circles that are drawn on the earth's surface in a north-south fashion,
from pole to pole. They run perpendicular to the parallels of latitude.
All meridians converge at the north and south geographic poles. Put another
way, a line of longitude cuts through the north-south axis of the earth
much like a knife cuts through the core of an apple when it is sliced.
No matter what their latitudinal coordinates,
all locations on a specific meridian have exactly the same longitudinal
coordinate. Following this same principle, every location on a specific
parallel has a unique and individual longitudinal coordinate. While it
is customary for cartographers to show only major meridians, and possibly
their major subdivisions, on maps, charts, and globes, there is no set
number of meridians: the number of meridians is unlimited.
The length of a degree of longitude
(or width between two meridians spaced one degree apart) varies depending
on the location and is a function of the cosine of its latitude. At the
equator--or the zero parallel at zero degrees latitude--where the lines
of longitude are their furthest apart, one degree of longitude measures
69.172 statue miles (111.321 kilometers). Near the middle of the Lower
Peninsula of Michigan--or the 45th parallel at 45 degrees north latitude--one
degree of longitude measures 48.995 statute miles (78.849 kilometers).
At the north geographic pole--or the 90th parallel at 90 degrees north
latitude--all the lines of longitude converge and one degree of longitude
measures 0.000 statute miles (0.000 kilometers).
Around the 46th parallel in Michigan's
Upper Peninsula, one second of longitude equals about 69 feet (while one
second of latitude equals about 100 feet).
***Lat/lon diagram
adapted from the U.S. Army's Map
Reading and Land Navigation Field Manual (FM 3-25.26, rev. 20
July 2001, formerly FM 21-26)
Notable
meridians
The prime meridian
The prime meridian is defined as the
meridian from which all of the earth’s other meridians are reckoned or
measured. It is also known as the Greenwich Meridian, meridian of Greenwich,
zero meridian, first meridian, standard meridian, reference meridian,
or base meridian. 
By modern convention, the prime meridian--the
zero-degree, north-south line of longitude--is defined as the meridian
that passes through the optical axis (crosshairs) of the Airy Transit
Circle telescope at the old Royal Greenwich Observatory located in Greenwich,
England. The coordinates of the Airy transit are 51°
28’ 38.1" north latitude and 000°
00’ 00" longitude.
Greenwich is a residential and industrial
borough of east-central Greater London. It is situated along the south
bank of the 210-mile-long River Thames, which is locally known as the
London River.
The Royal Greenwich Observatory, originally
known as the Observatory of Greenwich, was located in Greenwich from 1675
until the 1950s when light pollution from the Greater London area limited
the observatory’s astronomical effectiveness and forced its relocation
to Hurstmonceux Castle, a village located in England’s East Sussex County.
In 1990, the observatory was moved to Cambridge where it remained operational
until its closure in 1998.
Prior to 1884, the location of the prime
meridian varied from country to country. Nations often designated their
capital (e.g., Washington, Paris, Madrid, Copenhagen, Rome, Beijing, etc.)
as the location of the prime meridian, and it became known as their national
meridian. Sometimes convenient location or historic sites--such as the
Canary Islands--were designated as an area’s prime meridian.
To eliminate the problems multiple prime
meridians created for timekeeping, cartography, and navigation, the Washington
Meridian Conference was held in Washington, D.C. in 1884. The result of
this international meeting was a treaty that fixed the official location
for the earth’s prime meridian as "the meridian passing through the
centre of the transit instrument" at the United Kingdom’s Royal Astronomical
Observatory located in Greenwich, England.
Time zones and the prime
meridian
In addition to being the geographical
location of the modern-day prime meridian, Greenwich, England also serves
as the place from which Greenwich Mean Time (GMT)--the world timekeeping
standard and basis for the world’s time zone system--is calculated.
Greenwich Mean Time is also known as Universal Time.
Each of the world’s 24 time zones
occupies a 15-degree slice of longitude. Time zones west of the Greenwich
zone have times that are progressively earlier--one hour earlier per
each time zone--the farther they are located west of the Greenwich zone.
Time zones east of the Greenwich zone have times that are progressively
later--one hour later per time zone--the farther they are located east
of the Greenwich zone.
Put another way, every second, the
earth rotates through 15 seconds of longitude; every minute, the earth
rotates through 15 minutes of longitude; every hour, the earth rotates
through 15 degrees of longitude; and every 24 hours, the earth rotates
through 360 degrees of longitude, or one complete revolution.
***Lat/lon diagrams
adapted from the U.S. Army's Map
Reading and Land Navigation Field Manual (FM 3-25.26, rev. 20
July 2001, formerly FM 21-26)
International Date
Line
The International Date Line, sometimes
simply known as the date line, is an irregular, imaginary line running
between the north and south geographical poles. This north-south-running
line is largely represented by the 180 degree east longitude meridian,
or the 180 degree west longitude meridian, both of which are situated
180 degrees opposite the prime meridian. The current location of the International
Date Line was officially agreed upon when the position of the prime meridian
was established in 1884 at the Washington Meridian Conference in Washington,
D.C. 
While the location of the date line
generally follows the 180-degree meridian, it does depart to the east
or west in certain areas to prevent landmasses, islands, or archipelagos
from straddling the dateline and having two different dates, a situation
that would seriously disrupt an area’s daily life and commerce. Starting
from the arctic circle, the International Date Line diverges eastward
from the 180th meridian to avoid splitting Russia’s Siberia near it eastern
border; westward to avoid splitting the Aleutian Islands from Alaska in
the United States; and westward again to avoid splitting the Fiji Islands
and to avoid separating New Zealand from it smaller islands.
As the world’s official date line, the
180th meridian marks the location on the earth’s surface where the date
changes, where one day ends and the next day begins. This occurs when
the sun is directly over the prime meridian, which is located on the opposite
side of the earth at the zero degree line of longitude. Locations just
west of the International Date Line are one day ahead of points just east
of it.
***Lat/lon diagrams
adapted from the U.S. Army's Map
Reading and Land Navigation Field Manual (FM 3-25.26, rev. 20
July 2001, formerly FM 21-26)
Longitudinal
coordinates
A specific location’s longitudinal coordinate
is its easterly or westerly angular distance along the earth’s surface
relative to the prime meridian. It is measured as an arc, along a parallel
of latitude, perpendicular to the prime meridian, which by modern convention
is the zero degree meridian.
The numerical coordinate
Longitudinal coordinates--which can
range up to one-half of the earth’s circumference, from zero degrees (at
the prime meridian) to 180 degrees (at the international date line)--are
angles traditionally expressed in a degrees-minutes-seconds format: 145°
30’ 30.30"W. By custom, degree units are signified by the degree
° symbol; minutes are signified by the
minutes ‘ symbol, a single tick mark or apostrophe; and seconds are signified
by the seconds " symbol, or a double tick mark or quotation mark.
In the degree-based latitude and longitude measurement system, a circle
is made up of 360 degrees; a degree is made up of 60 minutes (a minute
equals 1/60 of a degree); and a minute is made up of 60 seconds (a second
equals 1/60 of a minute, or 1/3600 of a degree). 
In addition to a "degrees, minutes,
seconds" format, latitudinal coordinates are sometimes expressed
in shortened forms such as a "degrees and minutes" format, where
the parts of a minute are represented in a decimal-fraction form (e.g.,
145° 30.5001’W), or a "degrees"
format, where the parts of a degree are represented in decimal-fraction
form (e.g., 145.5084166° W).
While decimal-fraction format coordinates
are a common coordinate format option in Global Positioning System (GPS)
units and mapping software programs, they are very cumbersome for plotting
on topographic maps, especially in the field. Information on how to convert
latitude/longitude coordinates from one format to another, or convert
them to or from the UTM coordinate system, is discussed below.
***Lat/lon diagram
adapted from the U.S. Army's Map
Reading and Land Navigation Field Manual (FM 3-25.26, rev. 20
July 2001, formerly FM 21-26)
The hemispherical designator
Longitudinal coordinates are typically
followed by a single letter or symbol that designates whether they are
located east of the prime meridian--in the eastern hemisphere--or west
of the prime meridian--in the western hemisphere. West longitudinal coordinates
are customarily followed by either the letter "W" or the plus
"+" symbol. East longitudinal coordinates are customarily followed
by either the letter "E" or the minus "-" symbol.
Note: Some lat/lon coordinate systems
use the minus symbol to designate westerly coordinates and the plus symbol
to designate easterly coordinates.
Since the continental United States
lies entirely within the western hemisphere for longitudinal purposes,
many U.S. maps and charts do not include a western hemisphere designator
with the longitudinal coordinates printed along the neatlines in the margins
of the map or chart. Cartographers assume the user will know the longitudinal
coordinate is in the western hemisphere.
By convention, latitude/longitude coordinate
combinations always list the latitudinal coordinate first and the longitudinal
coordinate second.
Calculating
& plotting
lat/lon coordinates on maps
Learning how to plot lat/lon coordinates--identify
the specific location the coordinates refer to on a map--and calculate
lat/lon coordinates--figure out what the coordinates are for a specific
location on a map--can be an valuable skill for advanced-level wilderness
trippers.
For example, sometimes wilderness
trippers will be given coordinates in a lat/lon format only and it will
be necessary to either use them as they are or convert them to another
format. At other times, wilderness trippers will find themselves using
maps or charts--especially NOAA nautical charts used by sea kayakers--that
only include the lat/lon coordinate grid system.
On the majority of maps, the
perimeter boundary lines--called neatlines--along the left and right sides
and the tops and bottoms are represented by lines of longitude and lines
of latitude, respectively. However, many maps, especially large-scale
topographic maps suitable for wilderness land navigation, don’t come preprinted
with a grid of such lines--called a graticule--across the interior of
the map.
Topographic maps are often called
quadrangles--or quads--because they represent four-sided polygons known
as quadrilaterals. While it may not be readily apparent, a quad does not
form a true rectangle--a parallelogram composed of four right angles--because,
unlike the parallels of latitude that run parallel to each other as they
form the top and bottom of a map, the meridians of longitude that form
the left and right sides of the map are not straight lines and they don't
run parallel to each other. Instead, the meridians of longitude bend ever
so slightly as they converge at the poles.
Drawing the lat/lon grid
Before a map can be used with the latitude/longitude
geographic coordinate system, a grid of parallels and meridians should
be overlaid on the map proper. Since most maps include a series of tick
or hash marks--known as graticule marks--along the neatlines in all four
margins, and sometimes within the interior of the map itself in the form
of small crosses or plus "+" sign symbols, the user can simply
draw the parallels and meridians across the surface of the map by using
a pencil and a straightedge, such as an aluminum yardstick, to connect
these preprinted marks.
In the field, lines of latitude and
longitude can be drawn across a map by simply folding a corresponding
map edge over onto the surface of the map to create an improvised straight
edge.
Using a lat/lon coordinate plotter
To calculate the latitude/longitude
coordinates for a specific location on a map, or to plot known latitude/longitude
coordinates--say from a GPS unit--on a map, a latitude/longitude plotter
should be used.
Commercially manufactured latitude/longitude
plotters, calibrated in minutes and seconds, can be purchased from a number
of sources, some of which are listed below. Homemade plotters and improvised,
field-expedient latitude/longitude plotters can also be fashioned as described
below.
While it is possible to calculate or
plot approximate latitudinal and longitudinal coordinates without a plotter
through interpolation--estimating coordinates or their plots using a proportional,
geometric technique--it is often much more complicated and time-consuming,
not to mention less accurate, than using a latitude/longitude coordinate
plotter.
To use a latitude/longitude coordinate
plotter, simply position the device so each end of the appropriate scale
is aligned between two, adjacent lines of latitude, or longitude, depending
on which coordinate is being calculated or plotted. Often, especially
when plotting longitudinal coordinates, the scale will have to be positioned
at an angle between the lines, not perpendicularly, as is the custom when
using most conventional rulers.
For Michigan, Canadian, and other North
American quads, latitudinal coordinates increase from bottom to top, or
from south to north; longitudinal coordinates increase from right to left,
or from east to west.
The number of divisions on a latitude/longitude
plotter often depends on the map scale for which it was designed. For
example, The Coordinator, a commercial latitude/longitude plotter, is
configured with the following scales:
- 1:24,000 plotter (7 & 9/16 inches long)--150 one-second
divisions for grid lines spaced up to 2 minutes, 30 seconds apart.
- 1:25,000 plotter (7 & 1/4 inches long)--150 one-second
divisions for grid lines spaced up to 2 minutes, 30 seconds apart
- 1:30,000 plotter (6 & 1/16 inches long)--150 one-second
divisions for grid lines spaced up to 2 minutes, 30 seconds apart
- 1:50,000 plotter (7 & 1/4 inches long)--300 one-second
divisions for grid lines spaced up to 5 minutes, 00 seconds apart
- 1:62,500 plotter (5 & 13/16 inches long)--300 one-second
divisions for grid lines spaced up to 5 minutes, 00 seconds apart
- 1:63,360 plotter (5 & 3/4 inches long)--300 one-second
divisions for grid lines spaced up to 5 minutes, 00 seconds apart
- 1:100,000 plotter (11 inches long)--450 two-second divisions
for grid lines spaced up to 15 minutes, 00 seconds apart
- 1:250,000 plotter (4 & 3/8 inches long)--180 five-second
divisions for grid lines spaced up to 15 minutes, 00 seconds apart
Once one coordinate is calculated, or
plotted, depending on the case, the latitude/longitude plotter can then
be repositioned to calculate, or plot, the remaining coordinate. While
a single plotter works well for calculating the coordinates of a fixed
position on a map, two plotters, used simultaneously--one to plot the
latitudinal coordinate and one to plot the longitudinal coordinate--are
handy for plotting a known coordinate--say from a GPS unit--on a map.
Since calculating and/or plotting latitudinal
and longitudinal coordinates on topographical maps in the bush is a rather
cumbersome and complicated process (due in large part to the non-symmetrical
nature of the graticule), most experienced, long-range, wilderness trippers
avoid this awkward system and instead rely on the easy-to-use Universal
Transverse Mercator (UTM) coordinate system for rapid, on-the-go geographical
calculations and plots.
Commercial
lat/lon &
UTM coordinate plotter vendors
Adventure GPS
1-888-477-4386
http://www.gps4fun.com
Ben Meadows Company
1-800-241-6401
http://www.benmeadows.com
Brunton Company
1-800-443-4871
http://www.brunton.com/
See "map quad tool"
Forestry Suppliers,
Inc.
1-800-647-5368
http://www.forestry-suppliers.com
GPS Navigator Magazine.com
1-800-275-7526
http://www.gpsnavigatormagazine.com
Sells the Topo Companion
Lat.26Inc
1-800-305-0036
http://www.lat26inc.com
The Map Store
1-877-921-6277
http://www.maptown.com
Map Tools
1-650-529-9410
http://www.maptools.com
Ranger Joe's
1-800-247-4541
http://www.rangerjoes.com
Search Gear
1-800-474-2612
http://www.searchgear.com
Waypoint Enterprises
1-888-412-2600
http://www.waypoint-ent.com
Improvised
lat/lon plotters
1:20,000 (5.4’ by 8’) Ontario quads
The quad. The Ontario Ministry
of Natural Resources 1:20,000-scale quad is a topographic base map published
by the Province of Ontario, Canada. This 19.75-inch-wide by 19.75-inch-high
map depicts 5.4 minutes of latitude and 8 minutes of longitude. Since
the majority of these maps are not configured with latitudinal and longitudinal
tick marks, most are not suitable for use with the latitude/longitude
coordinate system.
Some of the older 1:20,000-scale quads
have graticule tick marks placed at two minute--or 120 second--intervals.
The neatlines along the maps’ boundaries, however, do not correspond with
the parallels and meridians needed for use with the latitude/longitude
coordinate system. Instead, they represent the easting and northing lines
necessary for use with the Universal Transverse Mercator (UTM) system,.
1:24,000 (7.5’ by 7.5’) USGS quads
The quad. The USGS 1:24,000-scale
quad is the most common topographic map in Michigan. This 15.75-inch-wide
by 22.75-inch-high map depicts 7.5 minutes of latitude and 7.5 minutes
of longitude. Because of its 7.5-minute size, it is often referred to
as a 7.5-minute quad.
Lat/lon tick marks. On the 1:24,000-scale
quad, the latitude and longitude coordinate system tick marks are located
on the neatlines in all four of the map’s margins. As an aid to drawing
lines between these marginal tick marks, corresponding crosses, or plus
"+" sign symbols, often appear between the neatlines, within
the map proper. Typically, these graticule tick marks are placed at 2.5-minute--or
150 second--intervals. Since the latitude/longitude coordinate system
is not symmetrical, 2.5 minutes of latitude equals about 7.5 inches while
2.5 minutes of longitude equals about 5.25 inches.
Improvising a plotter. To improvise
a latitude/longitude coordinate plotter for a 1:24,000-scale quad in the
field, simply cut off a 1-inch-wide by 9-inch-long, ruler-shaped piece
of the map’s blank margin. Using the statute-mile scale in the map’s bottom
margin, measure off and mark 30, 1/10-of-a-mile increments (which should
total exactly 3 miles) along one edge of the improvised paper ruler as
shown in the following diagram. 
Each one of these 0.1-mile segments
will correspond with 5 seconds of latitude, or longitude, depending upon
which coordinate the ruler is used to measure. Similarly, 12 of these
0.1-mile segments will correspond with one minute of latitude, or longitude.
Once the ruler is marked off in 0.1-mile
segments, label the first two 12-segment sections (measuring 1.2 miles
and representing 60 seconds--or 1 minute--each) with the second designators
of 0, 5, 10, 15, 20, 25, 30, 35, 40, 45, 50, 55, and 60 (the 60 would
also correspond with the zero starting mark of the next segment). Once
these two, 12-segment sections--measuring 1.2 miles each and representing
60 seconds (or 1 minute) each--have been marked off, mark off the remaining
6-segment section (measuring 0.6 miles and representing 30 seconds) with
the second designators of 0, 5, 10, 15, 20, 25, and 30.
Using the plotter. To calculate
or plot a latitudinal (or longitudinal) coordinate with this improvised
ruler, simply align the zero mark on the ruler with the lower or southernmost
line of latitude (or right or easternmost line of longitude) and then
angle the opposite end of the ruler until the 30th mark--the 2.5-minute
(150-second) mark--lines up with the adjacent upper or northern line of
latitude (or the adjacent line of longitude to the left or west), which
should be located 2.5 minutes away. Because of the non-symmetrical nature
of the latitude/longitude coordinate system, this improvised plotter is
designed to be used at an angle between two lines of latitude (or longitude),
not perpendicularly.
1:25,000 (7.5’ by 7.5’) USGS quads
The quad. The USGS 1:25,000-scale
quad is a less common topographic map in Michigan. This 15-inch-wide by
21.75-inch-high map depicts 7.5 minutes of latitude and 7.5 minutes of
longitude. Like the 1:24,000-scale quad, this map is often referred to
as a 7.5-minute quad.
Lat/lon tick marks. On the 1:25,000-scale
quad, the latitude and longitude coordinate system tick marks are located
on the neatlines in all four of the map’s margins. As an aid to drawing
lines between these marginal tick marks, corresponding crosses, or plus
"+" sign symbols, often appear between the neatlines, within
the map proper. Typically, these graticule tick marks are placed at 2.5-minute--or
150 second--intervals. Since the latitude/longitude coordinate system
is not symmetrical, 2.5 minutes of latitude equals about 7.25 inches while
2.5 minutes of longitude equals about 5.25 inches.
Improvising a plotter. (Note:
A 1:24,000-scale quad plotter will work on 1:25,000-scale quads.) To improvise
a latitude/longitude coordinate plotter for a 1:24,000-scale quad in the
field, simply cut off a 1-inch-wide by 9-inch-long, ruler-shaped piece
of the map’s blank margin. Using the statute-mile scale in the map’s bottom
margin, measure off 30, 1/10-of-a-mile increments (which should total
exactly 3 miles) along one edge of the improvised paper ruler (see diagram
in the 1:24,000 plotter instructions above).
Each one of these 0.1-mile segments
will correspond with 5 seconds of latitude, or longitude, depending upon
which coordinate the ruler is used to measure. Similarly, 12 of these
0.1-mile segments will correspond with one minute of latitude, or longitude.
Once the ruler is marked off in 0.1-mile
segments, label the first two 12-segment sections (measuring 1.2 miles
and representing 60 seconds--or 1 minute--each) with the second designators
of 0, 5, 10, 15, 20, 25, 30, 35, 40, 45, 50, 55, and 60 (the 60 would
also correspond with the zero starting mark of the next segment). Once
these two, 12-segment sections--measuring 1.2 miles each and representing
60 seconds (or 1 minute) each--have been marked off, mark off the remaining
6-segment section (measuring 0.6 miles and representing 30 seconds) with
the second designators of 0, 5, 10, 15, 20, 25, and 30.
Using the plotter. To calculate
or plot a latitudinal (or longitudinal) coordinate with this improvised
ruler, simply align the zero mark on the ruler with the lower or southernmost
line of latitude (or right or easternmost line of longitude) and then
angle the opposite end of the ruler until the 30th mark--the 2.5-minute
(150-second) mark--lines up with the adjacent upper or northern line of
latitude (or the adjacent line of longitude to the left or west), which
should be located 2.5 minutes away. Because of the non-symmetrical nature
of the latitude/longitude coordinate system, this improvised plotter is
designed to be used at an angle between two lines of latitude (or longitude),
not perpendicular to the edges of the map.
1:50,000 (15’ by 30’) Canadian quads
The quad. The Canadian 1:50,000-scale
quad is the most common topographic map in Canada. This 30-inch-wide by
21.75-inch-high map depicts 15 minutes of latitude and 30 minutes of longitude.
Lat/lon tick marks. On the 1:50,000-scale
quad, the latitude and longitude coordinate system tick marks are located
on the neatlines in all four of the map’s margins. There are normally
no intermediate tick marks within the map proper. Typically, these graticule
tick marks are placed at 5-minute--or 300 second--intervals. For convenience,
the neatlines on the 1:50,000-scale quads also include a handy, checkered
border that readily denotes each intermediate minute of latitude and longitude.
Since the latitude/longitude coordinate system is not symmetrical, 5 minutes
of latitude equals about 7.25 inches while 5 minutes of longitude equals
about 5 inches.
Improvising a plotter. To improvise
a latitude/longitude coordinate plotter for a 1:50,000-scale quad in the
field, simply cut off a 1-inch-wide by 9-inch-long, ruler-shaped piece
of the map’s blank margin. Using the statute-mile scale in the map’s bottom
margin, measure off 30, 2/10-of-a-mile increments (which should total
exactly 6 miles) along one edge of the improvised paper ruler (see diagram
in the 1:24,000 plotter instructions above).
Each one of these 0.2-mile segments
will correspond with 10 seconds of latitude, or longitude, depending upon
which coordinate the ruler is used to measure. Similarly, 6 of these 0.2-mile
segments will correspond with one minute of latitude, or longitude.
Once the ruler is marked off in 0.2-mile
segments, label all five 6-segment sections (measuring 1.2 miles and representing
60 seconds--or 1 minute--each) with the second designators of 0, 10, 20,
30, 40, 50, and 60 (the 60 would also correspond with the zero starting
mark of the next segment).
Using the plotter. To calculate
or plot a latitudinal (or longitudinal) coordinate with this improvised
ruler, simply align the zero mark on the ruler with the lower or southernmost
line of latitude (or right or easternmost line of longitude) and then
angle the opposite end of the ruler until the 30th mark--the 5-minute
(300-second) mark--lines up with the adjacent upper or northern line of
latitude (or the adjacent line of longitude to the left or west), which
should be located 5 minutes away. Because of the non-symmetrical nature
of the latitude/longitude coordinate system, this improvised plotter is
designed to be used at an angle between two lines of latitude (or longitude),
not perpendicularly.
Lat/lon
format
conversion
Converting between different formats
in the latitude/longitude geographical coordinate system is a somewhat
complicated process since the system uses degree-based measurements. As
such, it requires making computations based not on multiples of 10, to
which we are accustomed, but on multiples of 60.
For example, in the degree-based,
latitude and longitude measurement system, a circle is made up of 360
degrees; a degree is made up of 60 minutes (a minute equals 1/60 of a
degree); and a minute is made up of 60 seconds (a second equals 1/60 of
a minute, or 1/3600 of a degree).
To make in-the-field decimal-format
conversions easier, keep the following equivalents in mind:
15 minutes = 1/4 of a (hour) degree, which is 0.25 degrees
30 minutes = 1/2 of a (hour) degree, which is 0.50 degrees
45 minutes = 3/4 of a (hour) degree, which is 0.75 degrees
15 seconds = 1/4 of a minute, which is 0.25 minutes
30 seconds = 1/2 of a minute, which is 0.50 minutes
45 seconds = 3/4 of a minute, which is 0.75 minutes
Latitudinal and longitudinal coordinates
in a format other than "degrees, minutes, seconds"--such as
where the degrees or minutes are expressed with decimal fractions--are
very difficult to plot on maps. This is one of the reasons why many experienced
wilderness trippers prefer to work with the Universal Transverse Mercator
(UTM) coordinate system.
Lat/lon & UTM coordinate
format conversion Web sites
Lat/lon to lat/lon format converters
Montana State Library
Latitude Longitude Conversion Application
http://nris.state.mt.us/wis/location/latlong.asp
Jeep.Com
Coordinate Translation Page
http://jeeep.com/details/coord/
Lat/lon to UTM format converters
Jeep.Com
Coordinate Translation Page
http://jeeep.com/details/coord/
Montana State Library
Graphical Locator: XY-Data (DMS) Page
http://www.esg.montana.edu/gl/xy-data2.html
U.S. Department of
Commerce
National Geodetic Survey
NGS Geodetic to UTM Page
http://www.ngs.noaa.gov/cgi-bin/utm_getut.prl
Oasis.com
Coordinate Converter Page
http://www.gpsinformation.net/
UTM to lat/lon format converters
Jeep.Com
Coordinate Translation Page
http://jeeep.com/details/coord/
Montana State Library
Graphical Locator: XY-Data (UTM) Page
http://www.esg.montana.edu/gl/xy-data3.html
U.S. Department of
Commerce
National Geodetic Survey
NGS UTM to Geodetic Page
http://www.ngs.noaa.gov/cgi-bin/utm_getgp.prl
Oasis.com
Coordinate Converter Page
http://www.gpsinformation.net/
Downloadable format conversion
utilities
U.S. Department of Commerce
National Geodetic Survey
NGS Geodetic Tool Kit Page
http://www.ngs.noaa.gov/TOOLS/
Offers UTM, LAT/LON, & USNG conversion utilities
National Geospatial-Intelligence Agency
GeoTrans Translator
http://earth-info.nga.mil/GandG/geotrans/
GeoTrans utility converts wide array of coordinate formats
Lat/lon
& UTM coordinate
format conversion via a GPS unit
A Global Positioning System (GPS) unit
can be used to convert latitude and longitude coordinates from one format
to another. Simply set the coordinate format display (go to system setup
menu) of your GPS unit to the format of your coordinates and input your
coordinates. Then set the coordinate format display of your GPS unit to
the desired coordinate display format and read the conversion from it.
Lat/lon to lat/lon
format
manual conversion formulas
DEG-MIN-SEC
to DEG-MIN
Convert "degrees, minutes, seconds"
format (e.g., 45° 30’ 30.31"N)
to "degrees, decimal minutes" format (e.g., 45°
30.5052’N):
Objective: convert 45° 30' 30.31"N
to "degree, decimal minutes" format
Step 1: "degrees" (45°)
remains unchanged
Step 2: "decimal minutes"
= minutes + (seconds/60)
"decimal minutes" =
30 + (30.31/60) = 30.5052'
Result: "degree, decimal minutes"
format = 45° 30.5052’N
DEG-MIN-SEC
to DEG
Convert
"degrees, minutes, seconds" format (e.g., 45°
30’ 30.31"N)
to "decimal degrees" format (e.g., 45.5084194°
N)
Objective: convert 45°
30’ 30.31"N to "decimal degrees" format
Step 1: "decimal degrees"
= degrees + (minutes/60) + (seconds/3600)
"decimal degrees" = 45
+ (30/60) + (30.31/3600) = 45.5084194°
Result: "decimal degrees" = 45.5084194°
DEG-MIN to DEG
Convert "degrees, decimal
minutes" format (e.g., 45° 30.5052’N)
to "decimal degrees" format (e.g., 45.5084°
N):
Objective: convert 45°
30.5052’N to "decimal degrees" format
Step 1: "decimal degrees"
= degrees + (minutes/60)
"decimal degrees" = 45
+ (30.5052/60) = 45.5084°
Result: "decimal degrees"
= 45.5084°
DEG-MIN to DEG-MIN-SEC
Convert
"degrees, decimal minutes" format (e.g., 45°
30.5052’N)
to "degrees, minutes, seconds" format (e.g., 45°
30’ 30.31"N):
Objective: convert 45° 30.5052’N
to "degrees, minutes, seconds" format
Step 1: "degrees" (45°)
remains unchanged
Step 2: "minutes" = MM.mmmm
- 00.mmmm
"minutes" = 30.5052 -
00.5052 = 30’
Step 3: "seconds" = 00.mmmm
* 60
"seconds" = 00.5052 *
60 = 30.31"
Result: "degrees, minutes,
seconds" format = 45° 30' 30.31"N
DEG
to DEG-MIN
Convert
"decimal degrees" format (e.g., 45.5084°N)
to "degrees, decimal minutes" format (e.g., 45°
30.5040’N):
Objective: convert 45.5084°N
to "degrees, decimal minutes" format
Step 1: "degrees" = DD.dddd
- 00.dddd
"degrees" = 45.5084 -
00.5084 = 45°
Step 2 : "decimal minutes"
= 00.dddd * 60
"decimal minutes" = 00.5084
* 60 = 30.5040’
Result: "degrees, decimal minutes"
format = 45° 30.5040'N
DEG
to DEG-MIN-SEC
Convert "decimal degrees"
format (e.g., 45.5084° N)
to "degrees, minutes,
seconds" format (e.g., 45° 30' 30.24"N):
Objective: convert 45.5084°N
to "degrees, minutes, seconds" format
Step 1: "degrees" = DD.dddd
- 00.dddd
"degrees" = 45.5084 -
00.5084 = 45°
Note: the "decimal minutes"
figure must be calculated first in order to calculate the "minutes"
figure
Step 2 : "decimal minutes"
= 00.dddd * 60
"decimal minutes" = 00.5084
* 60 = 30.5040’
Step 3: "minutes" = MM.mmmm
- 00.mmmm
"minutes" = 30.5040 -
00.5040 = 30’
Step 4: "seconds" = 00.mmmm
* 60
"seconds" = 00.5040 *
60 = 30.24"
Result: "degrees, minutes,
seconds" format = 45° 30' 30.24"N
Lat/lon look-up Web sites
Lat/lon lookup by place-name:
USGS: Geographic Names Information System
(GNIS)
http://geonames.usgs.gov/index.html
Lists latitude and longitude for 2 million place-names
and features in the United States.
Come to Bali
http://www.indo.com/distance/
Lists latitude and longitude by city place-name
Latitude/longitude lookup by zip code or place-name:
U.S. Census Bureau:
U.S. Gazetteer
http://www.census.gov/cgi-bin/gazetteer
Lists latitude and longitude for zip codes or place-names
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2005-05-03
by Michael A. Neiger
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