  We study the correlations between $(u-r)$ colour, stellar mass, specific star
formation rate (sSFR) and metallicity of galaxies in different geometric
environments of the cosmic web using a volume limited sample from the SDSS. The
geometric environment at the location of each galaxy is determined using the
eigenvalues of the tidal tensor in three dimensions. We use the Pearson
correlation coefficient (PCC) and the normalized mutual information (NMI) to
quantify the correlations between these galaxy properties in sheets, filaments
and clusters after matching the stellar mass distributions of the galaxies in
these environments. A two-tailed t-test assesses the statistical significance
of the observed differences between these relations in different geometric
environments. The null hypothesis can be rejected at $>99.99\%$ significance
level in most of the cases, suggesting that the scaling relations between the
observable galaxy properties are susceptible to the geometric environments of
the cosmic web.
