  The Alfv\'{e}n speed and plasma beta in photospheric bright points observed
by the Broadband Filter Imager (BFI) of the Solar Optical Telescope (SOT) on
board the \textit{Hinode} satellite, are estimated seismologically. The
diagnostics is based on the theory of slow magnetoacoustic waves in a
non-isothermally stratified photosphere with a uniform vertical magnetic field.
We identify and track bright points in a G-band movie by using the 3D region
growing method, and align them with blue continuum images to derive their
brightness temperatures. From the Fourier power spectra of 118 continuum light
curves made in the bright points, we find that light curves of 91 bright points
have oscillations with properties which are significantly different from
oscillation in quiet regions, with the periods ranging 2.2--16.2~min. We find
that the model gives a moderate value of the plasma beta when $\gamma$ lies at
around 5/3. The calculated Alfv\'{e}n speed is 9.68$\pm$2.02~km~s$^{-1}$,
ranging in 6.3--17.4~km~s$^{-1}$. The plasma beta is estimated to be of
0.93$\pm$0.36, ranging in 0.2--1.9.
