LGS 3

LGS 3 is an irregular dwarf galaxy that is part of the Local Group.

The galaxy is also believed to be a satellitegalaxy of the TriangulumGalaxy (M33). Because it is in the constellation Pisces, the galaxy is called the Pisces Dwarf. It displays a blueshift, as it is approaching the MilkyWay at 287 km/s. It may be transition-type galaxy, somewhere between dwarf spheroidal and dwarf irregular. Alternatively, it may be a rare, but statistically acceptable, version of one of the two types. The star formation rate in the Pisces Dwarf has been declining for the past 10 billion years. Most of the galaxy's stars were formed in its early years, about 8 billion years ago. Studies have also shown that there has been no significant star formation for the past 100 million years. Hence, most of the stars that populate this galaxy are old, metal-rich stars aged about 2.5 billion years. But there are small clusters of young, hot, blue stars on the outer areas of the galaxy.

As of 5055 OTT, the Union has no presence in LGS 3, either by ship or gate.