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Tekros Expanse
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The Tekros Expanse is a region of space approximately three hundred light years in diameter which lies slightly beyond the borders of Federation and Klingon territory. This region of space was briefly surveyed by the USS Celestial in 2256, but no further exploratory efforts have been made since then. The Klingon Empire established a small outpost on its fringes during hostilities with the Federation in 2223 but abandoned it shortly afterwards.
This region of space is known as the ‘Dustbin’ for its high density of stellar nebulae and asteroid fields as well as its lack of anything to draw the attention of neighboring civilizations. During its survey, the USS Celestial reported no habitable planets and only sparse mineral deposits. Its location near to the edge of the galactic rim and away from trade routes also makes it a poor strategic location for establishing military outposts or other facilities.
Due to the recent cessation of conflicts between the Federation and the Hur’q, Starfleet has decided to continue the exploratory push which was initiated with the conclusion of the Iconian conflict. Several ships are scheduled to make a more detailed survey of the Expanse to make a more detailed astrometric survey of the region. As a prelude to this effort, the USS Beowulf has recently deployed a subspace amplifier in the area to facilitate communication between the Federation and Starfleet ships within the Expanse.
HAZARDS: The Expanse contains a large number of nebulae and other gaseous anomalies. A preliminary analysis by LtC. Lendaria on board the USS Eminence found that these clouds contain a high concentration of dilithium carbides, which give them sensor scattering properties. Starships travelling through the region will find their long-range sensor telemetry is greatly reduced. Short range scanners are also affected, albeit to a lesser degree.
Both the USS Celestial and USS Eminence have encountered subspace eddies within the Expanse. These energy currents can cause subspace turbulence for ships travelling at warp. The effect becomes more pronounced at higher velocities. Mapping efforts by Lt. Seral aboard the USS Eminence determined that these currents span the entirety of the Expanse and occur at relatively high densities. The source is currently unknown.
This region of space is known as the ‘Dustbin’ for its high density of stellar nebulae and asteroid fields as well as its lack of anything to draw the attention of neighboring civilizations. During its survey, the USS Celestial reported no habitable planets and only sparse mineral deposits. Its location near to the edge of the galactic rim and away from trade routes also makes it a poor strategic location for establishing military outposts or other facilities.
Due to the recent cessation of conflicts between the Federation and the Hur’q, Starfleet has decided to continue the exploratory push which was initiated with the conclusion of the Iconian conflict. Several ships are scheduled to make a more detailed survey of the Expanse to make a more detailed astrometric survey of the region. As a prelude to this effort, the USS Beowulf has recently deployed a subspace amplifier in the area to facilitate communication between the Federation and Starfleet ships within the Expanse.
HAZARDS: The Expanse contains a large number of nebulae and other gaseous anomalies. A preliminary analysis by LtC. Lendaria on board the USS Eminence found that these clouds contain a high concentration of dilithium carbides, which give them sensor scattering properties. Starships travelling through the region will find their long-range sensor telemetry is greatly reduced. Short range scanners are also affected, albeit to a lesser degree.
Both the USS Celestial and USS Eminence have encountered subspace eddies within the Expanse. These energy currents can cause subspace turbulence for ships travelling at warp. The effect becomes more pronounced at higher velocities. Mapping efforts by Lt. Seral aboard the USS Eminence determined that these currents span the entirety of the Expanse and occur at relatively high densities. The source is currently unknown.

Species 2562
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Species 2562 is a unicellular spaceborne lifeform which is native to the Tekros expanse. It is unusually large for a single celled lifeform and has been observed to grow as large as 1mm in diameter, although much of this area is composed of fringes of specialized cilia which it uses as solar sails. These cilia provide Species 2562 with its primary means of motility.
The organism appears to derive sustenance from EM radiation. It absorbs the radiation by means of chloroplast-like structures which line the interior of its cell membrane and is capable of feeding on a wide range of the EM spectrum. Its lifecycle appears to consist of two primary phases. The first involves drifting over vast distances as it absorbs and stores energy from its environment in phosphorylated protein lattices.
After it has absorbed enough energy, Species 2562 seeks out nebulae and utilizes the stored energy in combination with raw materials it harvests from the gases in order to reproduce. The microbe is capable of rapid reproduction, with each individual replicating its DNA and cellular structures many times over. The organism then proceeds to cluster divide, with each cell giving rise to as many as ten daughter cells.
Species 2562 has been observed throughout the Expanse. However, it occurs in higher densities near stars or other radiation sources and also near nebulae where the organisms harvest needed raw material from the gases. Its sensory capabilities appear to be limited to the detection of radiation or particle density gradients.
HAZARDS: While Species 2562 is incapable of doing direct harm to starships or personnel, it is attracted to both powered communications and sensor arrays. Sufficient density of Species 2562 is capable of drawing Species 2563 to an area.
Species 2563
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Image Credit: CBS
Species 2563 is a large cosmozoan which is native to the Tekros Expanse. Adults average approximately three kilometers in length with a mass of 2.7 million metric tonnes. It bears a passing resemblance to a Terran whale, with a long and streamlined body and multiple sets of fins along its sides. The ‘fins’ are composed of thin folded membranes stretched between bony supports, and the creature is capable of unfurling these structures to many times their compressed size. It uses these fins as sails to move itself along currents of solar radiation while conserving energy.
Species 2563 also possesses two more forms of locomotion should the need arise. It is capable of surprising bursts of speed, which it achieves by expelling nebular gases from vents in its posterior. These gases are obtained from the various nebulae that dot the Expanse and are stored in large internal sacs until needed.
The organism is also capable of limited FTL travel via the numerous subspace eddies which are present in the Tekros Expanse. It appears to harness these eddies using a type of naturally generated subspace bubble, though the exact mechanism is unknown. It is also unknown whether it is capable of unassisted FTL travel. The tough outer layer of Species 2563’s hide contains a high amount of various dilithium compounds, presumably to help shield it from radiation during FTL travel.
Species 2563 preys almost exclusively on the unicellular Species 2562, which it filters from space and traps using mucous covered membranes which line the interior of its throat. Its preferred hunting method is to cruise at warp until it detects a sufficient quantity of prey. It then proceeds to slow to sublight and approach to within striking distance using its sails before accelerating suddenly and devouring the entire swarm at once.
Presently little is known about the behavior and other biological characteristics of these organisms. Lone adults are found scattered throughout the Expanse as they search for prey. Juveniles of the species are theorized to spend much of their time hidden in nebulae. It is possible that they feed on the small amounts of prey in these areas, while absorbing dilithium compounds in order to grow their radiation resistant dermal layers.
HAZARDS: Species 2563 is largely docile and has not been observed engaging in intentionally aggressive behavior towards Starfleet ships or personnel. However, its sensory perception is limited, and it may attempt to ingest any objects which are in proximity to its prey while feeding.
Personnel regardless of protection will most likely die within hours if not recovered. Should this occur to a starship, the creature will likely die either of internal trauma if the vessel attempts to free itself or of starvation as it is unable to digest the alloys that comprise the hull.
Starfleet personnel should also be aware that the subspace field generated by Species 2563 also interferes with the generation of a stable warp field by vessels within its perimeter.