
Help! There is a comet in my computer! 7
2 Detection of emitted light
Our eyes, supported by our brain, are amazing instruments. We process incredible amounts
of visual information and store a lot of what we see in our memory. We can see very small
details. We can focus to near and far objects. There is one problem with our eyes, though –
we are not very good at judging the quantitative aspects of all the information we receive.
By only looking, we cannot tell whether two similar pencils located at different parts of a
table are of the same length or not, or how many centimetres they have. We are even worse
at measuring light intensities with our eyes. When we walk into a dimly-lit room from
sunshine, it seems to be very dark. A few moments later, we see perfectly well. When
observing a comet slide under a microscope, we cannot say how much light comes from
the head and how much from the tail. Our eyes are also not sensitive enough to see very
weak light.
We need to use technology for precise measurement of the intensity of light emitted from
comets. We can direct the emitted light through a microscope to a device that can detect
light intensity - a camera can do this (Figure 2C). A detector located in the camera is
composed of a rectangular array of small light-sensitive elements. The size of each detector
element is only a few micrometers across. Each element converts the measured light
intensity to a digital format, i.e. to numbers. By definition, small numbers represent a low
light intensity (few photons hit the detecting element), and high numbers a high light
intensity (many photons hit the detecting element). If we now connect the camera to a
computer and record the image, the camera sends the numbers representing each detector
element together with its coordinates on the detection array to the computer. The camera
sends all numbers representing one image as a package of digital data (an image file). The
computer decodes the received digital (numerical) information and displays it as an image
on the monitor screen (Figure 3A).
An image is composed of small dots called pixels. Each pixel represents one light-
sensitive element of the camera, and the numbers corresponding to light intensity
detected for each pixel are stored in a computer file.
We will use a simplified model image of a comet (Figures 3B, 3C) to explain how the
comet intensity is measured. This image was generated artificially and has extremely large
pixels for easier explanation of the discussed procedures.
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