This is what earth looks like when you take a picture of it from 29,000 kilometers away. This is the original Blue Marble photo, taken from Apollo 17.
Multiple distortions from idealized sphere:
-Topography
-Gravity Differentials
-Centrifugal Force
In most applications, topography isn't explicitly needed.
- We can account for it separately if necessary using digital elevation models or contour lines.
Simplification of Earth:
-Smooths topography
-Gravity differences measured by satellites
-Differences in surface heights (180 m)
A close approximation of Earth's shape
-Topography
-Gravity Differentials
-Centrifugal Force
A system to link the oblate spheroid to the geoid
-Connect the coordinates to the earth’s surface
For some cases, either datum is suitable.
A local datum is better for small areas like a city. For global maps, you always need a global datum.
Spherical Coordinate System for identifying locations on the spheroid.
-All GCS are tied to a specific datum.
Latitude/Longitude
Distance in degrees form Equator: -90°(South) to +90°(North)
Distance in degrees Prime Meridian: -180° (West); to +180° (East)
Decimal Degrees
Degrees Minutes Seconds
Meridians converge!
Displaying Lat/Lon in 2D doesn't work well
We have to apply a projection
A map projection is a flattened GCS. Imagine sending rays of light through the ellipsoid onto a flat surface, the resulting image is a projection.