Let

be a standard planar Brownian motion
and

be the diameter of the projection of
![$\mathrm{B}\left([0,1]\right)$](img35.png)
on the line generated by the unit
vector

, where

. In this short note, we find the common
cumulative distribution function

of the random variables

. Namely, we prove that
for every

. As immediate consequence, lower bound for the
expected diameter of the set
![$\mathrm{B}\left([0,1]\right)$](img35.png)
, better
than known, is obtained. Namely, it is known that

, where

is the diameter
of the set
![$\mathrm{B}\left([0,1]\right)$](img35.png)
. In this note we show

.