We report the discovery of a new member of the Local Group in the cons
tellation of Antlia. Optically the system appears to be a typical dwar
f spheroidal galaxy of type dE3.5 with no apparent young blue stars or
unusual features. A color-magnitude diagram in I, V-I shows the tip o
f the red giant branch, giving a distance modulus of 25.3+/-0.2 (1.15
Ripe +/-0.1) and a metallicity of -1.6+/-0.3. Although Antlia is in a
relatively isolated part of the Local Group it is only 1.2 degrees awa
y on the sky from the Local Group dwarf NGC 3109 and may be an associa
ted system. (C) 1997 American Astronomical Society.