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There are different types of asteroid cosmic anomalies, named by what kinds of ores are contained within. Each type comes in three variants (small, average, and large) - the "larger" the anomaly, the more asteroids (and hence the more ore) it contains. A "Small Kernite and Omber Deposit" therefore contains a small number of Kernite and Omber asteroids, while a "Large Bistot Deposit" contains a large number of Bistot asteroids. Ore anomalies will contain all three variants of the ores they contain. | There are different types of asteroid cosmic anomalies, named by what kinds of ores are contained within. Each type comes in three variants (small, average, and large) - the "larger" the anomaly, the more asteroids (and hence the more ore) it contains. A "Small Kernite and Omber Deposit" therefore contains a small number of Kernite and Omber asteroids, while a "Large Bistot Deposit" contains a large number of Bistot asteroids. Ore anomalies will contain all three variants of the ores they contain. | ||
The following chart illustrates the makeup of cosmic anomolies. "Small", "Average" and "Large" are defined above: | |||
==== High security space ==== | ==== High security space ==== | ||