Since contemporary astronomy
focuses on understanding physical processes
in the universe, the data collected usually
do not match what the human eye would perceive.
For example, our eyes detect radiation over
a range bounded on one end by blue light (high
energies) and the other by red light (low
energies). One can use the instruments and
filters on telescopes to replicate this range.
If this is done, natural color images can
be constructed. However, in astrophysics a
filter is more often used to isolate particular
energies of radiation. For example, astronomers
will use a filter to isolate gas of a specific
temperature from other sources of light. Gas
of a second temperature could also be imaged
by using filter which isolates a different
energy range. Despite the difference in the
energy of the radiation passed by these 2
filters, it may be the case that both gases
appear to be the same color of light to the
human eye! So if only these sort of filtered
observations exist, then only composite
color images are useful. Therefore each
filtered image is assigned a distinct color
in order to illustrate the difference in temperatures
existing in the astronomical object. |
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Copyright T. Bonev,
K. Jockers, and T. Credner |
Astronomers T. Bonev, K. Jockers, and
T. Credner at Max-Planck-Institut
fur Aeronomie have also made a composite
color image of the Bubble Nebula from their observations
of the radiation from hot gases. |