owniverse/data/legacy/locale-en.csv

Owniverse||interface||||
MM-Create||interface||||Menu/en/CreateUniverse
MM-Help||interface||||Menu/en/Tutorial
MM-Achievments||interface||||Menu/en/Achievements
MM-Credits||interface||||Menu/en/Credits
MM-LanguageEn||interface||||Menu/en/EnglishActive
MM-LanguageRu||interface||||Menu/en/Russian
MM-SoundActive||interface||||Menu/en/SoundActive
MM-SoundNonActive||interface||||Menu/en/SoundNonActive
MM-MusicActive||interface||||Menu/en/MusicActive
MM-MusicNonActive||interface||||Menu/en/MusicNonActive
MM-LeaveReality||interface||||Menu/en/LeaveReality
CreditsTitle||interface||||Credits/en/Credits
CreditsRoles||interface||Unitizer <br> Python Tamer <br> Painter <br> Original Score by||
CreditsNames||interface||Kirill Ivlev <br> Ilya Konovalov <br> Dmitry Uvarov <br> Tatyana Stepanenko||
Achievement-Header||interface||||Achievements/en/Achievements
Achievement-Status-Template||interface||Unlocked %Count% of %Total%||
ReportTitle||interface||||Report/en/Title
ReportNewWarning||interface||||Report/en/NewWarning
ReportNewButton||interface||||Report/en/NewButton
ReportWipeWarning||interface||||Report/en/WipeWarning
ReportWipeButton||interface||||Report/en/WipeButton
MF-FBV-ReturnButton||interface||||Dashboard/Indicators/ForceBoxes/En/Return
MF-FBV-OpenBoxButton||interface||||Dashboard/Indicators/ForceBoxes/En/OpenBox
MF-FBV-AcquireButton||interface||||Dashboard/Indicators/ForceBoxes/En/Acquire
MF-FBV-NoAdsDeliveredSign||interface||||Dashboard/Indicators/ForceBoxes/En/NoAds
Universe||interface||||
Time|Time|indicator|AboutTheGame|Time|Change the speed as you like.|
Energy|Enr|indicator|EnergyAndDensity|Energy|Spend on hydrogen and space.|
Density|Den|indicator|EnergyAndDensity|Density|Maintain balance.|
DensityRip|DenR|indicator|EnergyAndDensity|Big Rip|Increase density!|
DensityCrunch|DenC|indicator|EnergyAndDensity|Big Crunch|Decrease density!|
BurnabilityIndicator|Bur|indicator|BurnabilityAndExplosiveness|Burnability|Burning intensity of stars.|
ExplosivenessIndicator|Exp|indicator|BurnabilityAndExplosiveness|Explosiveness|Power of stellar explosions.|
AggressionIndicator|Agg|indicator|AggressionAndTrends|Aggression|Evolution and competition.|
||||1 year per second||
||||10 years per second||
||||100 years per second||
||||1 000 years per second||
||||10 000 years per second||
||||100 000 years per second||
||||1 000 000 years per second||
||||10 000 000 years per second||
||||100 000 000 years per second||
||||1 000 000 000 years per second||
||logtext||Summary of changes in the last 100 seconds.<br>Average values for the year are shown.||
ForceNavigationImage||interface||||BigBang/Dashboard/en/Forces
1-1-1-NavigationResourceImage||interface||||BigBang/Dashboard/en/Resources
Space|S|entity|SpaceAndHydrogen|Space|Needed for placing objects.|
Hydrogen|H|entity|SpaceAndHydrogen|Hydrogen|Used to create clouds and stars.|
Helium|He|entity|HeliumAndMetals|Helium|Saves hydrogen.|
Metals|Met|entity|HeliumAndMetals|Metals|Needed to create planets.|
||||Metallicity||
NavigationStarImage||interface||||BigBang/Dashboard/en/Stars
Nebula|N|entity|Clouds|Nebula|Produces hydrogen.|
Globula|G|entity|Clouds|Globula|Produces more hydrogen.|
StarNursery|STN|entity|Clouds|Star Nursery|Produces hydrogen and stars.|
MolecularCloud|MC|entity|Clouds|Molecular Cloud|Produces a lot of hydrogen.|
ActiveStarNursery|ASTN|entity|Clouds|Active Star Nursery|Produces a lot of hydrogen and stars.|
BrownDwarf|BD|entity|DwarfStars|Brown Dwarf|Useless, but doesn't take up space.|
RedDwarf|RD|entity|DwarfStars|Red Dwarf|The simplest star.|
OrangeDwarf|OD|entity|DwarfStars|Orange Dwarf|Star with planets.|
YellowDwarf|YD|entity|DwarfStars|Yellow Dwarf|Star similar to the Sun.|
WhiteYellowDwarf|WYD|entity|DwarfStars|White-Yellow Dwarf|Star with many planets.|
RedGiant|RG|entity|GiantStars|Red Giant|Degrading old star.|
YellowGiant|YG|entity|GiantStars|Yellow Giant|Optimal for metals production.|
BlueGiant|BG|entity|GiantStars|Blue Giant|Produces metals and space in a balanced manner.|
Supergiant|SG|entity|GiantStars|Supergiant|Produces space and a bit of metals quickly.|
Hypergiant|HG|entity|GiantStars|Hypergiant|Burns violently, creating a lot of space.|
WhiteDwarf|WD|entity|DegenerateObjects|White Dwarf|Remnant of a dwarf star.|
NeutronStar|NS|entity|DegenerateObjects|Neutron Star|Remnant of a burned-out giant.|
Magnetar|MGT|entity|DegenerateObjects|Magnetar|Remnant of a large giant.|
BlackHole|BH|entity|DegenerateObjects|Black Hole|The result of a stellar catastrophe. Needed for structures.|
SupermassiveBlackHole|SMBH|entity|DegenerateObjects|Supermassive Black Hole|Merged from black holes. Needed for galaxies.|
1-3-1-NavigationStructureImage||interface||||BigBang/Dashboard/en/Structures
StarClusterScattered|SCD|entity|StarClusters|Scattered Star Cluster|A little structure of irregular shape.<br>Space: +10%.|
StarClusterSmall|SCS|entity|StarClusters|Small Star Cluster|Has globular shape.<br>Space: +20%.|
StarClusterMedium|SCM|entity|StarClusters|Medium Star Cluster|Noticeable from afar off.<br>Space: +30%.|
StarClusterLarge|SCL|entity|StarClusters|Large Star Cluster|Makes an impression.<br>Space: +50%.|
StarClusterGiant|SCG|entity|StarClusters|Giant Star Cluster|Causes awe.<br>Space: +80%.|
GalaxyEllipticalDwarf|GED|entity|Galaxies|Dwarf Elliptical Galaxy|The size of the Small Magellanic Cloud.<br>Space: +100%.|
GalaxyEllipticalSmall|GES|entity|Galaxies|Small Elliptical Galaxy|The size of the Large Magellanic Cloud.<br>Space: +150%.|
GalaxyEllipticalMedium|GEM|entity|Galaxies|Medium Elliptical Galaxy|The size of the Milky Way.<br>Space: +200%.|
GalaxyEllipticalLarge|GEL|entity|Galaxies|Large Elliptical Galaxy|The size of the Andromeda Galaxy.<br>Space: +300%.|
GalaxyEllipticalGiant|GEG|entity|Galaxies|Giant Elliptical Galaxy|Similar to the IC 1101.<br>Space: +450%.|
GalaxySpiralDwarf|GSD|entity|Galaxies|Dwarf Spiral Galaxy|Similar to the Small Magellanic Cloud.|
GalaxySpiralSmall|GSS|entity|Galaxies|Small Spiral Galaxy|Similar to the Large Magellanic Cloud.|
GalaxySpiralMedium|GSM|entity|Galaxies|Medium Spiral Galaxy|Similar to the Milky Way.|
GalaxySpiralLarge|GSL|entity|Galaxies|Large Spiral Galaxy|Similar to the Andromeda Galaxy.|
GalaxySpiralGiant|GSG|entity|Galaxies|Giant Spiral Galaxy|The size of the IC 1101.|
GalacticGroup|LGG|entity|LargeStructures|Galactic Group|Aggregates galaxies.|
GalacticSupercluster|LSC|entity|LargeStructures|Galactic Supercluster|Basis for the structure of the universe.|
GalacticFilament|LGF|entity|LargeStructures|Galactic Filament|Balances density with voids.|
GalacticWall|LGW|entity|LargeStructures|Great Wall|Creates the structure of the universe.|
UniverseBubble|LUB|entity|LargeStructures|Universe Bubble|That's the extent of it.|
1-4-1-NavigationLifeImage||interface||||BigBang/Dashboard/en/Planets
GasGiant|GG|entity|Planets|Gas Giant|Too big.|
AsteroidBelt|AB|entity|Planets|Asteroids|A bunch of rocks.|
RockyPlanet|RP|entity|Planets|Rocky Planet|Not suitable for life.|
HabitablePlanet|HP|entity|Planets|Habitable Planet|Has the potential for life.|
LivingPlanet|LP|entity|Planets|Living Planet|There is life on this planet!|
|Star|||Star||
|SC|||Star Cluster||
|GAL|||Galaxy||
AboutTheGame||help||About The Game|In this game you can <b>create a universe</b> and control its development. The final goal is designated by yourself. Don't forget to check out the list of game achievements and try to reach some of the ones that seem interesting. Read hints, explore possibilities and don't be afraid to experiment. In the worst case you can always start from scratch.<br><br>Numbers greater than 1 000 are displayed using <b>scientific notation</b>. 1e4 – this is a 10 000, meaning “one with 4 zeroes”. 1e6 – a million, 1e9 – a billion and so on. 13.77e9 – this is 13 billions 770 millions.<br><br>The game plays in <b>real time</b> with changeable scaling. One second of real time can pass a year, a decade, a century and so on. Change the pace of time by using buttons “−” and “+”.|Help/en/AboutTheGame
GameplayBasics||help||Gameplay Basics|You have access to a very large, but still limited <b>cache of energy</b> that is used to create the whole matter in the universe and the expanse of the universe's space itself. At the start of the game the vast majority of this energy is not in your direct control. But during the game you will take more and more energy from the cache. The less filled the cache is, the harder it is to obtain new energy. The energy shortage won’t become an urgent problem in the first billion years or so: the cache is really very large.<br><br>The matter is harvested from the energy cache in the form of <b>hydrogen</b> by clouds. Hydrogen may be spent to create new clouds and also to create stars. During their burning stars create <b>space</b> that can be used to place additional stars and clouds. This creation of space also spends some energy from the cache.|Help/en/GameplayBasics
StarsAndStructures||help||Stars and Structures|The heavier the star is, the faster it burns and the more space it produces. However, on the contrary, the most cost-efficient way of spending hydrogen to obtain new space, is investment into the smallest stars. Unfortunately they burn for a very long time and produce space very slowly. Also each star takes a unit of space, no matter which type the star is.<br><br>There is a reason to arrange stars and nebulae of the growing universe into galaxies and even larger <b>structures</b>. The production of space by stars is increased inside structures.<br><br>The proportion between universe matter and space is called density. The universe is only stable when the <b>density</b> is inside a certain range. If it is too packed or too empty, problems come into being.|Help/en/StarsAndStructures
LifeAndForces||help||Life and Forces|<b>Planets</b> form around certain stars, and life may emerge there. In specific circumstances life can evolve to sapience, and sapience can advance to high technology. Life's next step is to try to reclaim the universe, which she assumes as her own.<br><br>There are many events in the universe that don't happen all the time, only with certain probability. You have access to special <b>forces</b>, which you can use to “tweak” chances of events that are important to you, changing the laws of nature in the process.|Help/en/LifeAndForces
Achievements||help||Achievements|During the gameplay you will definitely be able to reach certain <b>achievements</b>. While simpler ones come by themselves, ones that are more complex may be more tricky. You can use the achievements list as a roadmap of hints and suggestions for possible next steps.<br><br>It is unnecessary to try to finish each and every achievement. This is your own universe and you can do whatever you like with it. However, achievements are a nice thing in general, and besides just having a personal feeling of pride and accomplishment you can easily <b>share</b> it with friends!|Help/en/Achievements
Karma||help||Karma|Each obtained achievement grants you a certain number of <b>karmic points</b>. During the new universe creation you may spend these points to gain some small bonuses that will definitely help you to gain better results.<br><br>Spent karmic points are not lost: they will be <b>available</b> for spending again in the next universe. There is a chance that there will be even more of them at that moment.|Help/en/Karma
Gauges||help||Gauges|<b>Gauges</b> of measures that are especially important for an active objects page are located on the dashboard. To check other gauges just swipe the page.|Help/en/Gauges
EnergyAndDensity||help||Energy and Density|<b>Energy</b> from the cache is converted into hydrogen and space. The lower the proportion of remaining cache, indicated in the middle of the bar, the lower is the efficiency of the resource generators, such as clouds for hydrogen and stars for space.<br>The energy cache really is immense, however it is not infinite.<br><br>Average <b>density</b> of the universe is the ratio of total matter mass, meaning all stars, clouds and so on, to the empty space. It increases alongside the mass and decreases when the space grows. If the “ρ” gauge will leave the “middle zone” and become inclined to any of the two extremeties, then the outcome might surprise you in a bad way.|Help/en/EnergyAndDensity
BurnabilityAndExplosiveness||help||Burnability and Explosiveness|<b>Burnability</b> displays the current burning rate of stars. It can be influenced by the universe density (the denser the greater), the actions of superadvanced civilizations and the forces used by the player.<br><br><b>Explosiveness</b> displays the current probability of the gamma-ray bursts and the space yield produced by any sort of star collapses. It can be influenced by universe density (the denser the lower), actions of superadvanced civilizations and forces used by the player.|Help/en/BurnabilityAndExplosiveness
AggressionAndTrends||help||Aggression and Trends|<b>Aggression</b> displays the intensity of competition between species, civilizations and their inner factions. It governs the progress and stability of life and societies. It can be influenced by universal trends and forces used by the player.<br>By default the average universal aggression is shown. But you can select any civilization level and observe the average aggression for this level, which can be different from the universal one.<br><br><b>Trends</b> are the results of prolonged civilization influences. There are five trends in total.|Help/en/AggressionAndTrends
SpaceAndHydrogen||help||Space and Hydrogen|The majority of creative actions require spending <b>resources</b>.<br><br><b>Space</b> is needed to place everything you are creating. To add new space lit up some stars! Also don't forget to combine the created stars into structures to get even more space.<br><br><b>Hydrogen</b> is required to create nebulae and stars. Nebulae allow you to obtain more hydrogen. Stars are used to make more space and also to harbor planets. Both of these object types also serve as building blocks to create more complex structures.|Help/en/SpaceAndHydrogen
HeliumAndMetals||help||Helium and Metals|Helium and metals are obtained when stars finish their life cycle.<br><b>Helium</b> is not especially useful, but it is inevitable. It is automatically spent in a line of hydrogen if possible, conserving the more valuable resource.<br><br><b>Metals</b> “contaminate” your hydrogen and helium by heavier elements. And usually it is a good thing, because the high proportion of metals to hydrogen and helium, also known as “metallicity”, provides for a greater chance for planets to emerge near new stars.<br>Metals are added when stars burn out, especially larger ones. But total metellicity may shrink down when the universe is filled by new objects made from pure hydrogen and helium, such as nebulae and stars.|Help/en/HeliumAndMetals
Clouds||help||Clouds|Clouds are used to produce hydrogen, which is required to construct the universe. Simplest nebulae can be arranged into more complex cloud structures.<br><br><b>Nebula:</b> the simplest of clouds.<br><b>Globula:</b> provides hydrogen at a slower rate than nebulae, but persists for longer, and also takes less space. Used in creation of larger clouds.<br><b>Star nursery:</b> automatically creates stars from a fraction of provided hydrogen.<br><b>Molecular cloud:</b> large and long-lasting hydrogen generator.<br><b>Active star nursery:</b> very large automatic hydrogen and stars generator.|Help/en/Clouds
DwarfStars||help||Dwarf Stars|Dwarf stars are cheap, they last for a long time and produce space efficiently. They can have planets that sometimes may harbor life at some point.<br><br><b>Brown dwarf:</b> useless rejects that happen during the star creation process. They appear by themselves and do not take space as opposed to all the other stars. Can’t be created manually, and you don’t need to.<br><b>Red dwarf:</b> It is cost-effective in space creation, but works very slowly.<br><b>Orange dwarf:</b> perfect for the development of life.<br><b>Yellow dwarf:</b> good for the emergence of life.<br><b>White-yellow dwarf:</b> has a largest habitable zone, but burns out rapidly.|Help/en/DwarfStars
GiantStars||help||Giant Stars|Giant stars burn rapidly and produce a lot of space. At the end of their existence they collapse. These events can damage planets at nearby stars, but they produce metals.<br><br><b>Red giant:</b> a star that has consumed the majority of its fuel. You can’t create these manually, they emerge themselves.<br><b>Yellow giant:</b> the most modest of giant stars. Produces a lot of metals, collapse is weak.<br><b>Blue giant:</b> a common giant star. Produces a good amount of space and metals. Collapse is average.<br><b>Supergiant:</b> huge giant star. Lives short, collapses violently, produces a lot of space and few metals.<br><b>Hypergiant:</b> extremely giant star. Always collapses into a black hole, producing a huge amount of space, which is accompanied by insane destruction.|Help/en/GiantStars
DegenerateObjects||help||Degenerate Objects|Stars that have exhausted their fusion fuel. They occupy space and do not produce anything, but can be used in forming structures.<br><br><b>White dwarf:</b> the remains of a dwarf star.<br><b>Neutron star:</b> exceptionally compact remains of a giant star.<br><b>Magnetar:</b> the most dense object that is not a black hole.<br><b>Black hole:</b> the remains of a giant star that experienced a destructive collapse. They may be merged into supermassive black holes.<br><b>Supermassive black hole:</b> the result of multitudes of the stellar mass black holes merged into one. Required for galactic formation. They do grow in time, consuming other stars, but do so very slowly.|Help/en/DegenerateObjects
StarClusters||help||Star Clusters|Star clusters are the most modest of available structures. As a matter of fact these are just a lot of stars which are co-located closer to each other than usual, and therefore they are gravitationally bound. But even such simple lumps already bring noticeable variety into the homogenous landscape of the universe.<br><br><b>Scattered:</b> little structure of irregular shape.<br><b>Small:</b> globular shape.<br><b>Medium:</b> noticeable from afar off.<br><b>Large:</b> makes an impression.<br><b>Giant:</b> causes awe.<br><br>Clusters, like other structures, increase the production of space for their constituent stars. Stars in structures exist as usual. Over time, the clusters disintegrate, releasing the stars they are composed of. Large clusters last longer than small ones and provide a larger bonus to space production.|Help/en/StarClusters
Galaxies||help||Galaxies|<b>Elliptical galaxies</b> resemble colossal star clusters. They have lenticular shapes, rotate slowly and look very much alike to each other. The stars in them produce more space than in spiral galaxies. Gradually, elliptical galaxies disintegrate into separate stars.<br><br><b>Spiral galaxies</b> spin faster than elliptical ones, they have diverse structures with arms and keep active star formation. They are better fit for the emergence and development of life. In time spiral galaxies exhaust their storage of free gas, they slow down and become more stable and boring ellipticals.<br><br>As in the case of other structures, the stars included in the composition of galaxies continue to function as usual. They produce space, and dwarf stars can have planets.|Help/en/Galaxies
LargeStructures||help||Large Structures|<b>Large structures</b> are called that for a reason: whole galaxies are used there as building blocks. They are needed to arrange the universe on the largest scales. Without them the space, uniformly filled by stars and galaxies, becomes too monotonous and sparse, meanwile these structures create a packing gradient with more and less dense regions. This arrangement is better fit for being claimed and developed by superadvanced sapient beings.<br><br>Over time, large structures disintegrate into their components, but this does not happen very soon.|Help/en/LargeStructures
Planets||help||Planets|Planets emerge around dwarf stars when metals are sufficient. In a sense all this space construction is being made with a purpose of making planets with potential of bearing life.<br><br><b>Gas giant:</b> large planet with a very thick atmosphere, unsuitable for life.<br><b>Asteroid belt:</b> a bunch of rocks that lacks mass to form a planet.<br><b>Rocky planet:</b> a planet unsuitable for life. Too cold, hot or wrong chemical makeup.<br><b>Habitable planet:</b> there is liquid water here and life may emerge in the long run.<br><b>Living planet:</b> denizens of this planet show great promise!|Help/en/Planets
Eons||help||Eons|Life slowly evolves through eons from the most primitive one to the one with sapience potential. Not all planets are successful in completing this process to the end, because stars do not burn forever.<br><br><b>Archean:</b> it is difficult to notice, but these planets are full of archaea and cyanobacteria.<br><b>Paleozoic:</b> alongside ubiquitous amoeba these planets host algae, sponges and even molluscs.<br><b>Proterozoic:</b> ferns, worms, trilobites and fishes.<br><b>Mezozoic:</b> conifers, lizards, dinosaurs and therapsids.<br><b>Cenozoic:</b> flowering plants and various mammals, some of which show signs of sapience.|Help/en/Eons
Type0Civilizations||help||Type 0 Civilizations|Pre-space epoch – from a tribe to a federation.<br><br><b>c0.0:</b> Lower Paleolithic. Control of fire, stone tools.<br><b>c0.1:</b> Middle Paleolithic. Developed stone tools.<br><b>c0.2:</b> Upper Paleolithic. Advanced stone tools, art.<br><b>c0.3:</b> Mesolithic. Bow and arrows, fishing, boats.<br><b>c0.4:</b> Early Neolithic. Agriculture.<br><b>c0.5:</b> Middle Neolithic. Animal husbandry, ceramics.<br><b>c0.6:</b> Late Neolithic. Large settlements.<br><b>c0.7:</b> First kingdoms of copper and bronze ages. Wheel.<br><b>c0.8:</b> Ancient empires of the iron age. Philosophy.<br><b>c0.9:</b> Industrial age. Electronics and nuclear energy.|Help/en/Type0Civilizations
Type1Civilizations||help||Type 1 Civilizations|Civilizations are busy with settling their own solar system.<br><br><b>c1.0:</b> A civilization that has completely mastered its home planet. Superconductivity, controlled nuclear fusion.<br><b>c1.1:</b> Research compounds in the home system. Launch loop, space elevator.<br><b>c1.2:</b> Complete genetic tailoring. Cyborgization.<br><b>c1.3:</b> Industrial asteroid mining. Colonies on the other planets of the home system.<br><b>c1.4:</b> Harvesting of matter from atmospheres of gas giants.<br><b>c1.5:</b> Space cities. Picotechnologies.<br><b>c1.6:</b> Industrial manufacturing of antimatter. First starships.<br><b>c1.7:</b> Terraforming. Gamma-lasers.<br><b>c1.8:</b> Space stations of continental scale.<br><b>c1.9:</b> Partial Dyson swarm.|Help/en/Type1Civilizations
Type2Civilizations||help||Type 2 Civilizations|Civilizations that can expand to other stars.<br><br><b>c2.0:</b> A civilization that completely exploits the energy output of its own sun.<br><b>c2.1:</b> Change of planetary orbits.<br><b>c2.2:</b> Control over inertia.<br><b>c2.3:</b> Starlifting, harvesting matter from stars.<br><b>c2.4:</b> Femtotechnologies: manipulations on individual fermions.<br><b>c2.5:</b> Deconstruction and creation of planets.<br><b>c2.6:</b> Complete domination of astroarchitecture over planets.<br><b>c2.7:</b> Giant stars resources exploitation.<br><b>c2.8:</b> Control over gravity.<br><b>c2.9:</b> Movement of stars.|Help/en/Type2Civilizations
Type3Civilizations||help||Type 3 Civilizations|Civilizations of galactic scale.<br><br><b>c3.0:</b> Expansion into a galactic group is available.<br><b>c3.1:</b> Creation of stars.<br><b>c3.2:</b> Utilization of white dwarfs.<br><b>c3.3:</b> Creation of black holes by focused radiation.<br><b>c3.4:</b> Expansion into a galactic supercluster is available.<br><b>c3.5:</b> Utilization of neutron stars.<br><b>c3.6:</b> Expansion into a galactic filament is available.<br><b>c3.7:</b> Utilization of magnetars.<br><b>c3.8:</b> Expansion into a great wall is available.<br><b>c3.9:</b> Utilization of black holes.|Help/en/Type3Civilizations
Type4Civilizations||help||Type 4 Civilizations|Civilizations of the universe scale.<br><br><b>c4.0:</b> Temporal manipulations.<br><b>c4.1:</b> Expansion into the whole universe scale is available.<br><b>c4.2:</b> Utilization of supermassive black holes.<br><b>c4.3:</b> Folding space.<br><b>c4.4:</b> Improbability field.<br><br>And so on, bigger and bigger, so long as there is space.|Help/en/Type4Civilizations