  The advent of global mm-band Very Long Baseline Interferometry (VLBI) in
recent years has finally revealed the morphology of the base of the two most
prominent nearby, bright, extragalactic radio jets in M\,87 and 3C\,84. The
images are quite surprising considering the predictions of jet theory and
current numerical modeling. The jet bases are extremely wide compared to
expectations and the nucleus of 3C\,84 is very complicated. It appears as a
double in 86\,GHz observations with 50\,$\mu$as resolution and a triple nucleus
with 30\,$\mu$as resolution with space-based VLBI by RadioAstron at 22\,GHz.
What is even odder is that the double and triple are arranged along an
east-west line that is approximately orthogonal to the north-south large scale
jet on 150\,$\mu$as $-$ 4\,mas scales. We explore the emergence of an
(east-west) double nucleus in the lower resolution 43\,GHz Very Long Baseline
Array (VLBA) imaging from August 2018 to April 2020. The double is marginally
resolved. We exploit the east-west resolution associated with the longest
baselines, $\sim 0.08$\,mas, to track a predominantly east-west separation
speed of $\approx 0.086\pm 0.008$\,c. We estimate that the observed mildly
relativistic speed persists over a de-projected distance of $\sim 1900-9800$
times the central, supermassive black hole, gravitational radius ($\sim
0.3-1.5$\,lt-yrs) from the point of origin.
