  We report relations between inner ($<1$ au) super Earths (planets with
mass/radius between Earth and Neptune) and outer ($>1$ au) giant planets (mass
$>0.3~M_{\rm J}$, or cold Jupiters) around Sun-like stars, based on data from
both ground-based radial velocity (RV) observations and the Kepler mission. We
find that cold Jupiters appear three times more often around hosts of super
Earths than they do around field stars. Given the prevalence of the super Earth
systems, their cold Jupiters can account for nearly all cold Jupiters. In other
words, cold Jupiters are almost certainly ($\sim90\%$) companied by super
Earths. A few corollaries follow: (1) around metal-rich ([Fe/H]$>0.1$) stars,
the fraction of super Earths with cold Jupiters can rise to $60\%$ or higher;
(2) the inner architecture can be strongly impacted by the outer giant and we
report some observational evidence for this; (3) planetary systems like our
own, with cold Jupiters but no super Earths, should be rare ($\sim1\%$). The
strong correlation between super Earths and cold Jupiters establish that super
Earths and cold Jupiters do not compete for solid material, rather, they share
similar origins, with the cold Jupiter formation requiring a somewhat more
stringent condition. Lastly, we propose a few immediate observational tests of
our results, using ground-based RV observations and ongoing/planned space
missions.
