More than just a pretty picture
The Eagle Nebula image was taken on April 1, 1995, by the Hubble's
Wide Field and Planetary Camera 2. Like a digital camera, the
WFPC2 uses charge-coupled devices (CCDs) rather than film to
record images. CCDs have an array of light-sensitive elements
called pixels that turn light falling on them into electrical
signals. As we'll see, all the hard work of preparing the final
image involves knowing how to interpret each of those signals,
removing the "fingerprints" of the camera itself, and turning the
signals into measurements of how bright the light is at specific
points in the sky.
The WFPC2's field of view is about 1600 by 1600 pixels, which
makes it roughly equivalent to a 2.5 megapixel digital camera.
While the final image is not true color, it is closer to what your
eye would see if you went there than the picture you would get
with color film.
Before we begin fashioning the image, I need to reveal why the
final picture seems to have had a big bite taken out of its
upper-right quadrant.