  The photometric analysis of sample Am stars is carried out to determine the
stellar characteristics and to constrain the stellar dynamics. The
spectroscopic analysis of the studied Am stars confirms their general
characteristics of Am stars. The available data on elemental abundances for HD
113878 and HD 118660 have shown different characteristics during different
epochs of observations. The basic stellar parameters (mass, luminosity, radius,
life time, distance, proper-motion, etc.) are also determined to identify the
stellar habitat zones for earth like exoplanet. Such information is important
to identify suitable planets for human settlement in the near future. In this
connection, the tidal radius and boundaries of the habitable zone of each star
have been computed to support the search of an extra-terrestrial life around
them. Asteroseismic mass scale test shows greater stellar masses comparable to
the solar mass.
