Stars and planets formed within the same molecular cloud are inextricably linked in their composition. Alpha-process elements shape planetary cores and atmospheres, with studies showing that key elemental ratios (e.g. Fe/Si, Mg/Si) in planets reflect those of their host stars. While correlations between stellar chemical abundances, planet occurrence, mass and orbital properties have been suggested, definitive confirmation remains difficult due to the subtlety of these trends. Large, homogeneous, high-precision spectral datasets are essential to uncover these relationships. Bright stars (V < 11 mag), such as PLATO's priority-one targets, provide an ideal sample for high-quality stellar and chemical abundance measurements and are expected to yield thousands of new planetary discoveries in the coming years. However, modern multi-object spectroscopic (MOS) surveys often exclude these stars due to their low on-sky density, leading to inefficiencies in conventional observing strategies. The WEAVE-TwiLight Survey (WTLS) solves this problem by introducing a groundbreaking observing mode that optimises efficiency by combining multiple fields into a single fibre configuration. It is expected to produce a homogeneous spectral dataset of ~6,000 bright stars, tailored to probe the chemical relationships between host stars and their planets. In this talk, I will give a general overview of host-star planet relations and discuss the status of the upcoming WEAVE-TwiLight Survey.