Earth's Coordinate System
From SciencePickle
(Copyright, Jodi Pickle)
Earth is a rotating sphere, so its coordinate system uses latitude and
longitude to locate positions on the planet. Earth's axis of rotation orients
latitude so that the axis is the center of every latitude circle. Since a
latitude circle is perpendicular to the axis of rotation, every point along a
given latitude experiences the same illumination patterns of the Sun on any
given day of the year: location of sunrise and sunset, amount of daylight and
darkness, angle of the Sun above the horizon at local noon, etc. The National
Geographic website shows the range of definitions for the horizon. We will
use the astronomical horizon: the perpendicular horizontal plane to the
observer's zenith (the point directly above the observer).
Click to open or close a topic below.
Latitude
Latitude circles, which are points around the globe with the same
latitude, are perpendicular to Earth's axis of rotation. The North and South
Poles are where the axis of rotation intersects the Earth's surface. The North
Pole is 90°N, and the South Pole is 90°S. Because the Earth is
rotating, every person at a given latitude experiences the same pattern of the
Sun's apparent motion throughout the day.
Conventions of Latitude
- The North Pole is 90°N, the South Pole is 90°S, and the
Equator, halfway between the Poles [green], is 0°.
- Latitudes have positive and negative values. Northern Hemisphere
latitudes are positive, and negative latitudes occur in the
Southern Hemisphere.
- The largest latitude circle (greatest radius and perimeter) occurs
at the Equator (0°), the smallest at the Poles.
- The distance between one degree of latitude is a constant 60 nautical
miles or 111 km.
- If you look in the direction of constant latitude, you are facing
either east or west.
There are many ways to think about latitude, and each has value in how
we navigate and how the Sun warms the Earth. Examine the three images
that follow for examples.
Labeled latitudes every 15° extending from the North Pole to the South
Pole. Notice that the latitude circles are evenly spaced apart. The
latitude with the largest radius is the Equator (0°). At the Poles,
the circle is a point, so the radius is 0 km.
- Imagine standing at the center of the Earth and oriented parallel
to the Earth's axis. Looking straight ahead, you would be viewing the
Equator (0°). You would see the North Pole (90°N) directly overhead,
and the South Pole (90°S) would be straight down. If you looked 30°
above the Equator (magenta line), you would be looking at 30°N.
- The horizon
is the flat piece of real estate surrounding you when
standing at a particular location. The green line in this example is
the horizon for a person standing at 30°N. Latitude determines the
orientation of the horizon relative to the axis of rotation.
- The point directly overhead a person is the zenith. Notice that it
is an extension of the line of latitude (magenta) extending from the
center of the Earth to the point directly overhead someone (zenith)
standing at 30°N.
The zenith line and the horizon are always perpendicular to each other.
Notice how the orientations of the horizon and zenith change as
latitude changes from 90°N to 90°S. At the poles, the horizon is
perpendicular to the axis of rotation, and at the Equator (0°), the
horizon is parallel to it.
These spatial connections will be essential to apply in the Sun-Earth
Connection and Star-Planet Connection sections.
The orientation of the horizon (green) and zenith (magenta) depend on
one's latitude.
Latitude exercises
Longitude
Longitude is parallel
to the axis of rotation, but political, geographic, economic, aesthetic and/or
logical reasons dictate the location of 0°. For Earth, 0° goes
through the British Royal Observatory in Greenwich, England. A line of
longitude, or a meridian, creates a half-circle between the North and South
Poles.
Conventions of Longitude
- The Prime Meridian [green] is 0°, and the International Date Line
is 180°.
- Longitudes have positive and negative values. Positive longitudes are in
the Eastern Hemisphere (east of the Prime Meridian), and negative ones
occur in the Western Hemisphere (west of 0°).
- All lines of longitude meet at the Poles, so the distance between
one degree of longitude is not constant. It is 0 km at the Poles and
60 nm (111 km) at the Equator.
- If you look in the direction of constant longitude, you are facing
either north or south.
The Earth rotates counterclockwise in the Northern
Hemisphere but
clockwise in the Southern Hemisphere. To be more consistent, the Earth
rotates from west to east since this works in both hemispheres. This
is easy to remember since the east coasts of continents experience
sunrise before the west coasts.
Longitude defines our time zones, where, discounting geopolitical
boundaries, each hour is 15° longitude wide (360° / 24 hours =
15°). The time zone that includes the Prime Meridian extends between
7.5°W and 7.5°E.
Above are longitudes every 15° extending around the globe. The Prime
Meridian is 0°, and the International Dateline is 180°.
Longitude exercises