Spanking clean
This is the final, fully cleaned-up version of the PC1
image—or at least one of the PC1 images. Remember that a
picture was taken with the PC1 through each of four filters. Each
filter records light emanating from the target object—in our
case the Eagle Nebula—in very specific parts of the
visible-light spectrum.
Different types of atoms, it turns out, emit light at very
specific wavelengths—that is, very specific colors. (For
more on this, see the "Decoding Cosmic Spectra" feature elsewhere
on this Web site.) This allows astronomers like me to take images
that only show the light coming from specific types of atom. For
the Eagle Nebula image, the WFPC2 used filters that took images in
the light of three kinds of atoms: hydrogen atoms, sulfur atoms
with one electron removed (sulfur ions), and oxygen atoms with two
electrons removed (doubly ionized oxygen). A fourth filter sees
only starlight, which lights up the dust that is mixed in with the
nebula's gas.
The PC1 image that we've been manipulating was taken with the
oxygen filter. The first step in getting the PC1 image together
with its Wide Field mates is to obtain cleaned-up versions of the
three WF images also taken with the oxygen filter.