  We present a UBV I and H alpha photometric study of the young open cluster
NGC 1893 in the H II region W8 (IC 410 or Sh 2-236). A total of 65 early-type
members are selected from photometric diagrams. A mean reddening of the stars
is <E(B-V)> = 0.563 +/- 0.083 mag. The published photometric data in the near-
and mid-infrared passbands are used to test the reddening law toward the
cluster, and we confirm that the reddening law is normal (R_V = 3.1). Zero-age
main sequence fitting gives a distance modulus of V_0 - M_V = 12.7 +/- 0.2 mag,
equivalent to 3.5 +/- 0.3 kpc. From H alpha photometry 125 H alpha emission
stars and candidates are identified as pre-main sequence (PMS). The lists of
young stellar objects and X-ray sources published by previous studies allow us
to select a large number of PMS members down to 1 M_sun. Isochrone fitting in
the Hertzsprung-Russell diagram gives a turn-off age of 1.5 Myr and the median
age of 1.9 Myr from the PMS members with a spread of 5 Myr. We derive the
initial mass function (IMF) for stars with mass larger than 1 M_sun. The slope
of the IMF (Gamma = -1.3 +/- 0.1) is well consistent with the Salpeter/Kroupa
IMF. A total mass of the cluster appears to be in excess of 1,300 M_sun.
Finally, we estimate the mass accretion rate of 82 PMS members in the mass
range of 0.6 M_sun to 5 M_sun.
