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Venus zone
noun
A
theoretical
orbital
zone
around
a
star
that
will
result
in
an
Earth-like
planet
existing
in
an
orbit
in
the
zone
having
a
runaway
greenhouse
effect,
similar
to
that
found
on
Venus
in
our
Solar
System.
The
inner
edge
of
the
zone
is
where
solar
radiation
is
intense
enough
to
strip
the
atmosphere
of
a
planet
away.
The
outer
edge
is
where
solar
radiation
is
insufficient
to
power
a
runaway
greenhouse.
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