The physical properties of galaxies — such as luminosity, stellar mass, and star formation rate — are significantly correlated with their local environment. Understanding these environmental correlations is crucial for studying the evolution of galaxies in the large-scale structure of the Universe. Traditionally, such studies rely on local density measurements defined at a specific separation scale around galaxies. However, to fully capture the impact of the environment, it is essential to examine correlations across a wide range of scales. In this talk, I will demonstrate how clustering measurements effectively trace the environmental correlations of various galaxy properties as a function of separation scale. I will present results from our studies on the correlations of luminosities (from optical to mid-IR bands), stellar mass, and star formation rate with local environment. Additionally, I will show how clustering measurements help probe the environmental dependence of galaxy mergers. Our analysis is based on stellar-mass-selected, volume-limited galaxy samples from the Galaxy And Mass Assembly (GAMA) survey. We also compare our measurements from GAMA with those from CosmoDC2, a simulated sky catalogue designed for the Rubin Observatory LSST Dark Energy Science Collaboration. Finally, I will present our recent results on the environmental correlations of low-surface-brightness galaxies (LSBGs) identified in the Dark Energy Survey.