During the five-year period from January 2049 to January 2054, the focus of the Colonial Alliance turned to out-system colonization, primarily in the Sirius system. Until that point, colonization was almost entirely within the Sol system. The primary advantage of Mars as a colonist destination was its proximity to Earth, but it lacked minerals entirely and the population of 1.8 billion was already half the maximum capacity. Io, which became an ideal habitable world in August 2053, did have substantial deposits of Duranium and Corundium plus a billion in population capacity, but lacked other key minerals. Even so, the population of Io had reached ninety-five million by January 2054 and had one hundred and five manned mining complexes in operation. Earth itself was fast running out of minerals with only Duranium remaining in large, accessible quantities. Even that resource was starting to diminish as the accessibility fell.
Earth Survey ReportDuranium: 331,288 0.98
Corbomite: 1,104 0.11
Boronide: 34,853 0.29
Mercassium: 51,608 0.34
Sorium: 503 0.10
Io Survey Report Duranium: 6,365,606 0.70
Mercassium: 28,765 0.80
Corundium: 424,814 0.90
Therefore, after much debate in the Council of the Colonial Alliance, the focus turned to Sirius. With almost two billion people already evacuated from Earth, the survival of humanity was assured. The new priority was ensuring the economy could continue to support that population, which meant exploitation of resources outside the Sol system, which in turn required out-system colonies. At the start of 2049, the colonies in Sirius comprised 4.5m on Sirius-A II and tiny settlements on two moons of Sirius-A I.
Sirius-A II, a mountainous world, with large lakes covering sixteen percent of the surface, offered a number of advantages for a more substantial colony. The planet had deposits of all mineral types, albeit mainly at minimal accessibility with the exception of Duranium and Corbomite, plus it had a population capacity of six billion. Before terraforming began, the planet had a temperature of 78C and a nitrogen and oxygen atmosphere of 0.7 atm, with an oxygen content too high for humans at 38%. By January 2054, forty-six terraforming installations on the surface, supported by twenty Gaia class terraforming stations in orbit, had brought the temperature down to 42C and made the atmosphere breathable. The colony cost was 0.40 due to the hydrographic coverage, but the scale of the terraforming effort meant it would be an ideal habitable world within a year. The population was thirty-eight million.
Sirius-A II Survey ReportDuranium: 10,533,889 0.50
Neutronium: 1,831 0.60
Corbomite: 10,791,064 0.50
Tritanium: 6,350,368 0.10
Boronide: 4,473,160 0.20
Mercassium: 72,868 0.10
Vendarite: 11,696,368 0.10
Sorium: 163,993 0.10
Uridium: 10,207,993 0.10
Corundium: 10,497,568 0.10
Gallicite: 2,924,068 0.10
Another advantage of Sirius-A II was its proximity to other sources of minerals, which meant a substantial economy could be supported on the planet. In the late 2040s, Neutronium had become a serious problem, with almost all work on shipyard expansion halted as the stockpile fell to a critical level. The only significant supply on a world that could be realistically colonised from Earth in the near-term was on the first moon of Sirius-A I. The 2800 km diameter moon had almost two million tons of accessibility 0.5 Neutronium, plus over three hundred thousand tons of accessibility 0.9 Duranium and a smaller deposit of Uridium.
While the moon lacked both air and water and had a colony cost of 3.75, its small size meant it could be terraformed twenty times more quickly than an Earth-sized planet. The moon became the primary terraforming target between the completion of the operation on Io and the start of the major effort on Sirius-A II. The atmosphere was made breathable and the temperature brought into the habitable range. By January 2054 the colony cost was 0.85, with the only factor being the limited amount of surface water. Sufficient water vapour was already in the atmosphere so it was simply a matter of waiting for the condensation to take place. The moon would be an ideal habitable world by 2056. The Neutronium crisis made the moon the focus of out-system mining; three hundred and eighty mines were in operation by the end of 2053 and the population reached thirty-six million.
Sirius-A I – Moon 1 Survey ReportDuranium: 340,169 0.90
Neutronium: 1,913,979 0.50
Uridium: 55,084 0.60
Two other moons of Sirius-A I also would contribute to the ongoing industrial expansion in the system. The tenth moon was very similar to the first; 3000 km in diameter with useful mineral deposits and lacking both air and water. In this case, the deposits were accessible Duranium, Vendarite and Gallicite and the colony cost was 4.95. Once the terraforming of Sirius-A II was complete, the tenth moon would be the priority. Even without terraforming, the population had reached six million.
Sirius-A I – Moon 10 Survey ReportDuranium: 3,976,106 0.70
Vendarite: 216,118 0.80
Sorium: 793 0.80
Uridium: 72,847 0.40
Gallicite: 216,105 0.90
Finally, the eleventh moon had deposits of all eleven minerals, including ninety-four million tons of accessibility 0.5 Duranium, eighteen million tons of accessibility 0.7 Corbomite, ten million tons of accessibility 1.00 Corundium and one point five million tons of accessibility 0.9 Gallicite. All the other deposits were at minimal accessibility. Unfortunately, the ‘moon’ was larger than Earth and had a dense Venusian atmosphere of over 100 atm, which meant terraforming was not an option and the colony cost of 27.04 precluded the use of manned mines. One hundred and twenty automated mines were in operation on the surface, plus four civilian mining complexes.
Sirius-A I – Moon 11 Survey Report Duranium: 94,118,573 0.50
Neutronium: 4,775 0.10
Corbomite: 18,834,722 0.70
Tritanium: 18,232,775 0.10
Boronide: 7,839,875 0.10
Mercassium: 35,402,375 0.10
Vendarite: 29,051,975 0.10
Sorium: 12,744,775 0.10
Uridium: 20,702,375 0.10
Corundium: 10,822,845 1.00
Gallicite: 1,586,471 0.90
In addition to the major colonies in Sirius, a colony of 600,000 was established on Osiris V, a small colony cost 2.13 planet two transits from Earth via Lacaille. Osiris V had accessible Duranium and Neutronium deposits, although the latter was not in the same quantities as the first moon of Sirius-A I and Osiris was further away from Earth. Even so, it was a useful outpost on a planet with terraforming potential that could serve as a forward base in the future.
Osiris V Survey ReportDuranium: 2,367,488 0.70
Neutronium: 139,876 0.90
Corbomite: 462,400 0.20
Sorium: 10,653,696 0.10
Corundium: 10,653,696 0.10
Between January 2049 and January 2054, Earth’s population’s fell by only twenty million as the much longer round trip to the Sirius-A system meant the colony ships could only keep up with the natural population growth on Earth. The population might even have grown slightly if it were not for the establishment of a colony on Mercury in November 2050. The Xenoarchaeology expeditions on Mercury and Alpha Centauri-A IV were successful in deciphering the language and symbology of the two destroyed outposts, which were apparently both created by a polity known as the Kitchener Kingdom, and identified a total of sixteen sites for potential recovery, once the requisite technology was developed. They also determined the two ancient constructs would provide assistance in research efforts, adding perhaps thirty percent to construction-related projects on Mercury and seventy percent to logistics-related projects on Alpha Centauri IV. With the potential for Mercury as a research-focused colony, a total of twenty-seven terraforming installations were moved to the planet to add Frigusium to the atmosphere, which reached 0.16 atm by January 2054 and reduced the colony cost to 2.49. The focus of civilian shipping lines moved to Mercury for a couple of years, before being redirected to Sirius, and the population passed thirty million in late 2053. A single research facility was moved to Mercury in 2052.
By January 2054, Earth had moved within the orbit of Venus. The distance from Earth to the Sun was one hundred and six million kilometres and falling. The temperature had risen slightly to 0.3C, which was not yet a major factor due to the 0.275 atm of Frigusium in the atmosphere. In fact, most of the terraforming effort had moved away from Earth, leaving only nineteen terraforming installations in operation on the home world. Seventy-seven research facilities were on Earth, along with six hundred financial centres and five hundred and seventy mines. As the colonies in Sirius increased their population and began to take on more responsibility for industrial production, the financial centres would move to Mars. The research facilities would move either to Mars, or to the sites of the alien structures on Mercury and Alpha Centauri IV. The mines would move to Sirius or Io.
The three 25,000-ton Lexington class carriers, Lexington, Ark Royal and Akagi, were launched in January 2050. It was almost a year before the first Cobra class fighter landed on the Lexington in December 2050. Over the next three years, a total of four different Cobra class fighters were designed, with construction of the Cobra MK IV beginning in January 2054. The Cobra MK I was a bare-bones design, intended to provide the Alliance with at least a minimal combat capability. The Tarasov MK I 10cm Railgun only had a range of 10,000 km while the operational range of the fighter was less than 200m km. The Cobra did not have an inherent engineering capability but did carry sufficient spares to effect repairs. Despite its limited offensive potential, the Cobra could serve in a missile defence role where weapon range and endurance were not a factor. The APD-6 Active Search Sensor was designed with that role in mind, sacrificing range for a missile-detection capability. Twenty Cobra MK Is were constructed.
Cobra MK I class Fighter 500 tons 23 Crew 72.6 BP TCS 10 TH 72 EM 0
7214 km/s Armour 1-5 Shields 0-0 HTK 3 Sensors 0/0/0/0 DCR 0 PPV 3
Maint Life 2.09 Years MSP 40 AFR 100% IFR 1.4% 1YR 12 5YR 184 Max Repair 36.00 MSP
Lieutenant Commander Control Rating 1
Intended Deployment Time: 6 days Morale Check Required
Kirk-72F Improved Nuclear Pulse Drive (1) Power 72.0 Fuel Use 754.25% Signature 72.00 Explosion 20%
Fuel Capacity 8,000 Litres Range 0.38 billion km (14 hours at full power)
Tarasov MK I 10cm Railgun (1x4) Range 10,000km TS: 7,214 km/s Power 3-3 RM 10,000 km ROF 5
AWG-5 Beam Fire Control (1) Max Range: 32,000 km TS: 7,200 km/s 69 38 6 0 0 0 0 0 0 0
R3 Improved Pebble Bed Reactor (1) Total Power Output 3 Exp 5%
APD-6 Active Search Sensor (1) GPS 1 Range 1.3m km MCR 113.5k km Resolution 1
The Cobra MK II upgraded the power plant from the pebble bed reactor of the Mk I to the recently-developed gas-cooled fast reactor, providing the same power while saving mass. The extra payload capacity was devoted to fuel, allowing a seventy-six percent increase in range. Ten Cobra MK IIs were constructed before the advent of the MK III.
Cobra MK II class Fighter 500 tons 22 Crew 73.1 BP TCS 10 TH 72 EM 0
7206 km/s Armour 1-5 Shields 0-0 HTK 3 Sensors 0/0/0/0 DCR 0 PPV 3
Maint Life 2.09 Years MSP 40 AFR 100% IFR 1.4% 1YR 12 5YR 184 Max Repair 36 MSP
Lieutenant Commander Control Rating 1
Intended Deployment Time: 6 days Morale Check Required
Kirk-72F Improved Nuclear Pulse Drive (1) Power 72 Fuel Use 754.25% Signature 72 Explosion 20%
Fuel Capacity 14,000 Litres Range 0.67 billion km (25 hours at full power)
Tarasov MK I 10cm Railgun (1x4) Range 10,000km TS: 7,206 km/s Power 3-3 RM 10,000 km ROF 5
AWG-5 Beam Fire Control (1) Max Range: 32,000 km TS: 7,200 km/s 69 38 6 0 0 0 0 0 0 0
R3 Gas-Cooled Fast Reactor (1) Total Power Output 3 Exp 5%
APD-6 Active Search Sensor (1) GPS 1 Range 1.3m km MCR 113.5k km Resolution 1
The Cobra Mk III design was a more substantial improvement in performance. The Kirk-72F Improved Nuclear Pulse Drive was replaced with the Kirk-80F Ion Drive, increasing engine power by eleven percent while reducing engine mass by the same percentage. Although a more powerful engine could have been included, the Kirk-80F remained within the maximum repair capacity of the Cobra and freed up sufficient mass for a larger fire control with a greater tracking speed, plus an eighty-five percent increase in fuel capacity. With endurance exceeding a billion kilometres, the Cobra MK II could operate at interplanetary ranges. The Tarasov MK I 10cm Railgun was replaced with the MK II, which doubled the weapon range to 20,000 kilometres. Fifteen Cobra MK Is were constructed. With the availability of Ion technology, developed by Jason Kirk in July 2052, the parent carriers were taken back into the shipyard for an upgrade to the new engines, increasing their speed to 4000 km/s.
Cobra MK III class Fighter 500 tons 21 Crew 84.6 BP TCS 10 TH 80 EM 0
8015 km/s Armour 1-5 Shields 0-0 HTK 3 Sensors 0/0/0/0 DCR 0 PPV 3
Maint Life 1.97 Years MSP 40 AFR 100% IFR 1.4% 1YR 14 5YR 204 Max Repair 40 MSP
Lieutenant Commander Control Rating 1
Intended Deployment Time: 6 days Morale Check Required
Kirk-80F Ion Drive (1) Power 80 Fuel Use 800% Signature 80 Explosion 20%
Fuel Capacity 26,000 Litres Range 1.17 billion km (40 hours at full power)
Tarasov MK II 10cm Railgun (1x4) Range 20,000km TS: 8,015 km/s Power 3-3 RM 20,000 km ROF 5
AWG-7 Beam Fire Control (1) Max Range: 32,000 km TS: 8,100 km/s 69 38 6 0 0 0 0 0 0 0
R3 Gas-Cooled Fast Reactor (1) Total Power Output 3 Exp 5%
APD-6 Active Search Sensor (1) GPS 1 Range 1.3m km MCR 113.5k km Resolution 1
The design of the Cobra MK IV was finalised in December 2053. The only change was the replacement of the AWG-7 Beam Fire Control with the more modern AWG-11, which provided greater fire control range and therefore improved accuracy at shorter ranges. As of January 2054, no MK IVs had been constructed.
Cobra MK IV class Fighter 500 tons 21 Crew 91 BP TCS 10 TH 80 EM 0
8015 km/s Armour 1-5 Shields 0-0 HTK 3 Sensors 0/0/0/0 DCR 0 PPV 3
Maint Life 1.89 Years MSP 40 AFR 100% IFR 1.4% 1YR 14 5YR 215 Max Repair 40 MSP
Lieutenant Commander Control Rating 1
Intended Deployment Time: 6 days Morale Check Required
Kirk-80F Ion Drive (1) Power 80 Fuel Use 800% Signature 80 Explosion 20%
Fuel Capacity 26,000 Litres Range 1.17 billion km (40 hours at full power)
Tarasov MK II 10cm Railgun (1x4) Range 20,000km TS: 8,015 km/s Power 3-3 RM 20,000 km ROF 5
AWG-11 Beam Fire Control (1) Max Range: 48,000 km TS: 8,100 km/s 79 58 38 17 0 0 0 0 0 0
R3 Gas-Cooled Fast Reactor (1) Total Power Output 3 Exp 5%
APD-6 Active Search Sensor (1) GPS 1 Range 1.3m km MCR 113.5k km Resolution 1
The development of ion drive technology also had an impact on the design of commercial shipping, in particular the large numbers of colony ships and freighters responsible for setting up the colonies in Sirius. The first Diaspora V class colony ships were launched in July 2053, with four in service by January 2054. The Diaspora V was much larger than the first three Diaspora designs, but was identical to the Diaspora IV with the exception of the Kirk-200C Ion Drive replacing the Kirk-160C Nuclear Pulse Engine. The Diaspora III-B was intended as a refit for the earlier Diaspora II and Diaspora III classes, replacing their Spielmann-128C and Kirk-128C engines respectively with the Kirk-200C. By January 2054, sixty-two colony ships in total were in service, all but twelve of which were the smaller, earlier designs.
Diaspora V class Colony Ship 82,243 tons 546 Crew 2,796.5 BP TCS 1,645 TH 3,800 EM 0
2310 km/s Armour 1-168 Shields 0-0 HTK 158 Sensors 5/0/0/0 DCR 1 PPV 0
MSP 21 Max Repair 100 MSP
Cryogenic Berths 150,000 Cargo Shuttle Multiplier 8
Lieutenant Commander Control Rating 1 BRG
Intended Deployment Time: 3 months
Kirk-200C Ion Drive (19) Power 3800 Fuel Use 4.05% Signature 200 Explosion 4%
Fuel Capacity 750,000 Litres Range 40.5 billion km (203 days at full power)
SQR-2 Thermal Sensor (1) Sensitivity 5 Detect Sig Strength 1000: 17.7m km
Diaspora III - B class Colony Ship 40,263 tons 268 Crew 1,448.6 BP TCS 805 TH 1,600 EM 0
1986 km/s Armour 1-104 Shields 0-0 HTK 78 Sensors 0/0/0/0 DCR 1 PPV 0
MSP 22 Max Repair 100 MSP
Cryogenic Berths 80,000 Cargo Shuttle Multiplier 5
Lieutenant Commander Control Rating 1 BRG
Intended Deployment Time: 3 months
Kirk-200C Ion Drive (8) Power 1600 Fuel Use 4.05% Signature 200 Explosion 4%
Fuel Capacity 400,000 Litres Range 44.2 billion km (257 days at full power)
The Mars V was the freighter equivalent of the Diaspora V; twice as large as the first three Mars designs, but equivalent to the Mars IV except for the upgrade to ion engines. A Mars III – B fulfilled the same role as the Diaspora III – B, acting as a refit option for the Mars II and Mars III. Ninety-eight freighters were in service in January 2054, including twenty-eight Mars IV and four Mars V.
Mars V class Freighter 102,016 tons 450 Crew 1,519.5 BP TCS 2,040 TH 4,600 EM 0
2254 km/s Armour 1-194 Shields 0-0 HTK 165 Sensors 5/0/0/0 DCR 1 PPV 0
MSP 9 Max Repair 50 MSP
Cargo 50,000 Cargo Shuttle Multiplier 6
Lieutenant Commander Control Rating 1 BRG
Intended Deployment Time: 3 months
Kirk-200C Ion Drive (23) Power 4600 Fuel Use 4.05% Signature 200 Explosion 4%
Fuel Capacity 1,000,000 Litres Range 43.6 billion km (223 days at full power)
SQR-2 Thermal Sensor (1) Sensitivity 5 Detect Sig Strength 1000: 17.7m km
Three new shipping lines were formed between January 2049 and January 2054; Blue Origin, the Sierra Nevada Corporation and OneSpace. Between the three companies, they had ten ships in operation. The original two civilian shipping lines, SpaceX and Boeing, each had forty-two ships in operation, for a total of nine-four civilian ships across the five companies.
The number of known systems increased from twenty-one in January 2049 to fifty-six by January 2054, with more systems discovered in the ‘Greek Arm’, compared to the areas named for Egyptian and Norse mythology. A connection was made between the Greek and Egyptian arms at the systems of Sekhmet and Hestia, which created a loop of eight systems, including Sol.
In June 2052, the Anubis system, comprising an orange K4-V primary and nine planets, was discovered at the end of a chain of systems in the Egyptian Arm. Except for Earth, Anubis II was the first non-terraformed planet with a breathable atmosphere. In terms of physical characteristics, the planet was similar to Earth, with a nitrogen – oxygen atmosphere of 1.12 atm, gravity of 1.06G and diameter of 11,200 km. The major difference was the climate; Anubis II was a desert world with a temperature of 90C and small seas covering nineteen percent of the surface. As the planet was tide-locked, the temperature was less of an issue, resulting in a colony cost of 0.44. The planet had deposits of all eleven minerals, including seven million tons of accessibility 0.8 Duranium, sixteen million tons of accessibility 0.8 Mercassium and seven million tons of accessibility 1.0 Vendarite. At some point in the future, Anubis II would be a valuable colony for the Colonial Alliance. For now, it was six transits and seventeen billion kilometres away and lay outside the stabilised jump network.
Anubis II Survey ReportDuranium: 7,250,432 0.80
Neutronium: 614,656 0.60
Corbomite: 15,808,576 0.10
Tritanium: 112,896 0.10
Boronide: 8,809,024 0.10
Mercassium: 16,711,744 0.80
Vendarite: 7,225,344 1.00
Sorium: 15,366,400 0.10
Uridium: 8,809,024 0.10
Corundium: 6,927,424 0.10
Gallicite: 12,544 0.10
Other interesting systems included Tau Ceti in the Greek Arm, a yellow G8-V star with thirteen planets, the outermost of which orbited at over a trillion kilometres. Ragnarök, in the Norse Arm, had only four planets and ten moons, yet had six bodies with colony costs between 2.00 and 2.77, including a moon with a large ice sheet and substantial mineral deposits. The Zeus system, a trinary with a G5-IV sub-giant and two red dwarfs, had seventeen planets and more than a hundred moons, including seven bodies of colony cost 2.00. Although a geological survey was underway at the start of 2054, red dwarfs, which had twelve planets between them, were forty billion kilometres from the primary. Zeus-B had the only Lagrange point in the system, so Zeus-A III, a gas giant, would be the site of the first LaGrange point to be stabilised by the Colonial Alliance, opening up the B and C components to survey.
Ragnarök IV – Moon 10 Survey ReportDuranium: 6,624,800 0.70
Tritanium: 2,016,400 0.90
Boronide: 1,960,000 0.30
Uridium: 270,400 0.90
Corundium: 1,081,600 0.30
Gallicite: 1,600 0.40
The system of Beta Canum Venaticorum, six transits from Sol in the Greek Arm, was discovered in September 2052 by the survey ship Leif Erikson. As this was a well-known yellow G0-V star, there was no need for a new ‘Greek’ designation and it retained its pre-existing name. Five terrestrial planets and a gas giant orbited the star, along with eleven moons. Five bodies were colony cost 2.00 and ten more were 2.00 LG, leaving only the gas giant and the outermost planet, which was colony cost 4.96. Beta Canum Venaticorum V had a nitrogen – oxygen atmosphere of 0.4 atm, including 0.036 atm of oxygen. With a temperature of -56C, an ice sheer covering eight-five percent of the surface and a diameter of 9200 km, it was a good terraforming prospect. The sixth planet, almost entirely covered in ice, had a temperature of -129C and a nitrogen – oxygen atmosphere of 0.67 atm, including 0.24 atm of oxygen. The percentage of oxygen content was too high but as Aestusium would be required anyway to increase the temperature, it was also a good terraforming prospect. Leif Erikson headed in-system to begin a geological survey followed by a gravitational survey.
In June 2053, the stabilisation ship Bulwand Darwaza followed Leif Erikson into the system after completing the stabilisation of the far side of the jump point in the Astraeus system. She immediately detected the wreck of the survey ship between the orbits of the fifth and sixth planets. Bulwand Darwaza had no jump drive, so the only way out of the system was to stabilise the Beta Canum Venaticorum side of the jump point. After a tense five months passed without incident, the stabilisation ship transited back into Astraeus and raised the alarm via the stable jump network on November 18th 2053.
The news caused a huge amount of concern in the Council of the Colonial Alliance. The Colonial Alliance navy, known as the Colonial Fleet, had a considerable number of vessels in service, totalling over eighteen million tons of shipping and orbital stations. However, the only armed vessels were the fifty-five Cobra fighters of various types, totalling twenty-seven thousand tons; hardly a formidable force. Even the carriers required to transport them were unarmed. The Council resolved to focus research efforts on defensive technologies and begin the long and arduous task of forming a real navy, even at the expense of the colonisation effort. The only good news was the unknown hostile force was six transits away and had shown no interest in the Astraeus jump point during the five months in which Bulwand Darwaza was present in the system. Given sufficient time, the Colonial Alliance had the industrial potential to build a substantial force. The key questions were whether the Alliance had that time and what impact the diversion of resources would have on the plan to evacuate Earth.
Colonial Fleet – January 20543x Lexington II class Carrier:
Lexington, Ark Royal, Akagi20x Cobra MK I
10x Cobra MK II
15x Cobra MK III
5x Magellan class Survey Ship:
Christopher Columbus, Ferdinand Magellan, James Cook, Marco Polo, Sacagawea4x Magellan II class Survey Ship:
George Vancouver, Vasco de Gama, Yuri Gagarin, Zheng He1x Agincourt class Troop Transport:
Agincourt1x Agincourt II class Troop Transport:
Gettysburg2x Agincourt III class Troop Transport:
Stalingrad, Waterloo4x Kamikawa Maru class Jump Tender:
Kamikawa Maru, Kiyokawa Maru, Hirokawa Maru, Kimikawa Maru2x Amazon class Tanker:
Amazon, Nile3x Rappahannock class Tanker:
Rappahannock, Roanoke, Shenandoah6x Gateway class Stabilisation Ship:
Arch of Constantine, Brandenburg Gate, Bulwand Darwaza, Golden Gate, Ishtar Gate, Meridian Gate30 x Diaspora - B class Colony Ship
1x Diaspora II class Colony Ship
16x Diaspora III class Colony Ship
3x Diaspora III - B class Colony Ship
8x Diaspora IV class Colony Ship
4x Diaspora V class Colony Ship
30x Mars - B class Freighter
6x Mars II class Freighter
24x Mars III class Freighter
6x Mars III - B class Freighter
28 x Mars IV class Freighter
4x Mars V class Freighter
63x Saturn class Fuel Harvester Base
4x Gaia class Terraforming Station
16x Gaia II class Terraforming Station