  To settle the question of the nature of the interstellar object 1I/'Oumuamua
requires in-situ observations via a spacecraft, as the object is already out of
range of existing telescopes. Most previous proposals for reaching 1I/'Oumuamua
using near-term technologies are based on the Solar Oberth Manoeuvre (SOM), as
trajectories without the SOM are generally significantly inferior in terms of
lower mission duration and higher total velocity requirement. While the SOM
allows huge velocity gains, it is also technically challenging and thereby
increases programmatic and mission-related risks. In this paper, we identify an
alternative route to the interstellar object 1I/'Oumuamua, based on a launch in
2028, which does not require a SOM but has a similar performance as missions
with a SOM. It instead employs a Jupiter Oberth Manoeuvre (JOM) with a total
time of flight of around 26 years or so. The efficacy of this trajectory is a
result of it significantly reducing the $\Delta$V to Jupiter by exploiting the
VEEGA sequence. The total $\Delta$V of the trajectory is 15.8 $kms^{-1}$ and
the corresponding payload mass is 115 kg for a SLS Block 1B or 241 kg for a
Block 2. A further advantage of the JOM is that the arrival speed relative to
1I/'Oumuamua is approximately 18 $kms^{-1}$, much lower than the equivalent for
the SOM of around 30 $kms^{-1}$.
