  The behaviour of a static thin shell embedded in dS space is investigated. To
satisfy the junction conditions at the boundary, one rescales the time
variable. The surface energy $\sigma$ on the shell is positive but its surface
tension $\tau$ is negative when $r << a$, where $a$ is the horizon radius. The
repulsive character of the radial acceleration of a static inner observer is
fortified by the process of sinking in the Sitter universe. An upper limit for
$\sigma$ has to be imposed for the shell mass to remain positive.
