Anemones genus
Description
Despite their name, these organic structures more closely resemble the shells of sea urchins. These organic structures can tolerate a wide range of temperatures and are able to absorb energy from nearby stars.
Minimum distance between two genetic samples: 100 m
Conditions of occurrence
- Parent Star: types O, B more rarely A
- Planets types: planets with no atmosphere. Have been found punctually on planets with thin atmospheres (confirmed on thin Sulfur Dioxide).
Colored variants
Rubeum Bioluminescent
CMDR Alistair Hope, Anemone, Slegeae KT-Q e5-1, A 3
Roseum Bioluminescent
CMDR Alistair Hope, Anemone, Heart Sector DL-Y e7, 7
Prasinum Bioluminescent
CMDR Alistair Hope, Anemone, 2MASS J02350854+6109233, 3 a
CMDR Quadmo, Blatteum Bioluminescent, HIP 27016, 8 A
Anemone
Luteolum
CMDR Quadmo, Anemone, HIP 27016, 8 A
The different types of anemones depend on the type of planet, the type of star and the luminosity class of the star (information available in the system map):
| Star Class + Luminosity | Metal-Rich / HMC | Rocky | Rocky Ice / Icy |
|---|---|---|---|
| O | Prasinus/Prasinum Bioluminescent | Prasinus/Prasinum Bioluminescent | Puniceus/Puniceum |
| B I, B II, B III | Roseus/Roseum Bioluminescent | Roseus/Roseum | |
| B IV, B V | Blattinus/Blatteum Bioluminescent | Luteus/Luteolum | |
| B VI, A III | Rubens/Rubeum Bioluminescent | Croceus/Croceum |