This system was first discovered by CMDR RoyalKnight557 and first visited for EDSM by CMDR IlluM1NaT1OwL. Situated about 1,150 light-years "east" of the NGC 1491 Nebula, the system contains an ammonia world with two moons, both of which are home to Crystalline Shard fields.

Carbon dioxide geysers dot the surface of B 7 a, while B 7 b features liquid ammonia-based volcanism. The crystalline shards on both moons drop ruthenium.

Shards on B 7 a seem to populate the flat portions of the moon's surface, while they're more populous in the highlands of B 7 b.

In addition to the exobiology payout, the shards' ruthenium deposits can be used for premium Automated Field Unit Maintenance module reloads.

The name of this point of interest is inspired by dragon's teeth fortifications, first used to impede tanks and infantry vehicles in World War II. Clusters of crystalline shards have been known to similarly impede surface reconnaissance vehicles.

Situated about 1,150 light-years East of the NGC 1491 Nebula, this system contains a ringed Ammonia World with two moons, both of which are home to Crystalline Shard fields.

Carbon dioxide geysers dot the surface of B 7 a, while B 7 b features ammonia-based volcanism. The crystalline shards on both moons yield ruthenium.

The shards on B 7 a seem to populate the flat portions of the moon's surface, while they're more populous in the highlands of B 7 b.

In addition to the exobiology payout from sampling the crystalline shards, their ruthenium deposits can be used for premium Automated Field Unit Maintenance module reload synthesis.

The name of this point of interest is inspired by dragon's teeth fortifications, first used to impede tanks and infantry vehicles in World War II. Clusters of crystalline shards have been known to similarly impede surface reconnaissance vehicles.