Even the closest stars are
so far away as to appear as nothing but little dots in the sky.
Stars dwarf their planets, so our ability to see planets of other
solar systems is minimal.
We can, however, infer
their existence, by looking at minor, cyclical changes in the signals
from the stars themselves.
A planet orbiting a star
will exert a small tug upon it’s parent, towards or away from us,
at different points of it’s orbit. This wobble is just large enough
to be picked up as changes in the star’s radial velocity.
Inferring the presence of
a planet from these changes in the light is difficult. where several
planets orbit the star, at different frequencies, the changes in
signal are laid on top of one another. it is necessary to look for
evidence of a repeated pattern, and subtract it from the sum of the
signal, gradually working backwards, uncovering evidence of further
regularities, and hopefully of further, less influential planets.
Other entirely unrelated
factors may also contribute to the changes in signal, further
compounding the problem.
The search for life on
systems outside our own is fraught with false hope and
disappointment.
The Gliese 581 star is a
close neighbour, only 20 light years away. In 2007, strong evidence
of a third exoplanet, within the goldilocks zone, was discovered. A
year later, a radio signal sending greetings from Earth was sent
there.
More recently, better data
has allowed us to factor in the presence of sunspot activity from the
signal, peeling back another layer of noise. Subtracting that
strengthened the regularity of the signal detected for the planets
dubbed B, C and E, but D, previously considered to be a strong
candidate for life, has faded from the picture entirely. (The others
are well outside the Goldilocks zone.)
By the time our signal of
hope reaches Gliese, it is likely that we will know that it’s
intended target was nothing but a mirage, an artefact of our
inability to see more clearly when we were younger.
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