The very phrase - "May there always be Sunshine" and the emotional charge of the associated song is all about ensuring that the Earth which is giving us life now and the Sun that is giving the Earth and us the energy for life to be possible, continue to do so for us and our systemic siblings for all of eternity.
The MTABS model can be mapped on the Kardashev Scale but it isn't clear exactly what level later Phases fit in. Phases below 6 can be safely assumed to be below 2 on Kardashev's Scale. Phases below 9 can also be pretty easily mapped below 3 Kardashev. The question then becomes do Phases 9 and especially 10 require over 3 Kardashev?
Phase 10 is probably so far away from our capabilities that it's just not worth focusing on at this point - we just can't see far enough out of the Milky Way to understand the full picture. But, no matter what the Andromeda situation is (and it has recently been questioned) Phase 9 business requires enormous amounts of energy. And if Phase 9 can be accomplished on a level closer to Kardashev 2, using machines that power directly from stars, can the combined civilizations of a Galaxy accomplish Phase 9 goals while Linked 8/23/2024 remaining solely on their home planets? The answer to this question is hard to arrive at logically given only what we commonly know now.
From this logic follows - if we (collectively as a Galaxy) must build Earth-like artificial habitats and exist in many interstellar locations to prevent Galactic Cataclysms, does that conflict with MTABS eternal focus on Earth and Sun?
The answer is simple - we are nowhere near the level of societal and technological development necessary to contribute to galactic projects. On the contrary, the MTABS hypothesis is that by focusing on our own planet first and ensuring the most optimal arrival at Kardashev 1 we will set the most optimal course for the next step. Subsequently then, by concentrating our focus on the Sun we will naturally plot the most optimal course to arrive at Kardashev 2.
The key assumption present in MTABS is that it will take time (lots of time by our measure) to arrive at Kardashev 1. And subsequently, it will continue to take even more time to arrive at Kardashev 2. But, without focusing on our own planet first and then on our own star it could be argued that we would arrive at those milestones either too late or never at all.
Thus the MTABS model Phases map to the Kondrashev scale in the following timeline progression, which when combined with other factors forms a hypothetical matrix:
MTABS Phase | Time Frame from fusion net engineering gain |
Civilizational stage | Environment management | Kardashev Value | (Optimal) Energy Source Schedule | Planet-Predominant / Human / ?Solar System? Sovereignty status | Typical Violent Sovereign Conflicts |
~ -70M - ~ -7M | 0 | Pre-Human Family Group balance of forces | Naturally occuring Pre-Human violence | ||||
~ -7M - ~ -700K | Local arrival and positioning | Up to .1 | Early scattered fuel usage | Inter (Proto-Human) Family Group balance of forces | Semi-naturally occuring Proto-Human violence | ||
~ -700K - ~ -70K | Local/Regional infancy | Up to .15 | Mid scattered fuel usage |
Inter-Family Froup safety
Inter-Clan balance of forces |
Sporadic violent engagements
Early Organized violent engagements (the assumed worst stage of the Human-on-Human "Total Violence") |
||
~ -70K - ~ -7K | Early Local/Regional Childhood | Early Local management | Up to .25 |
Late scattered fuel usage
Early Earth surface fuel |
Inter-Family Group secuirty
Inter-Clan safety Inter-Tribe balance of forces |
Sporadic violent engatements
Mid Organized violent engagements Early Local war |
|
~ -7K - ~ -700 |
Late Regional childhood, early adulthood, adulthood
Global arrival and positioning |
Mid Local management | Up to ~.4 | Mid Earth surface fuel |
Inter-Clan security
Inter-Tribe safety Inter-City/Area balance of forces |
Late Organized violent engagements
Mid Local war Early Regional war |
|
~ -700 - ~ 70 |
Late Regional adulthood
Global infancy |
Late Local management
Early Regional management |
Up to ~.6 | ~
Late Earth surface fuel
Early fossil fuel |
Inter-Tribe security
Inter-City/Area safety Inter-State/Principality balance of forces |
Late Local war
Mid Regional war Early/Direct Global war |
|
~ -70 - 0 | Early Global childhood | Mid Regional management | Up to ~.7 | Mid fossil fuel |
Inter-City/Area security
Inter-State/Principality safety Inter-Nation balance of forces |
Late Regional war
Mid/Proxy Global war Early deterrence war |
|
1 | 0 - ~ 70 |
Late Global childhood, early adulthood, adulthood
Solar System arrival and positioning |
Full Regional management
Early Earth management |
Up to ~.8 |
Late fossil fuel
Early Earth deuterium fusion |
Inter-State/Principality security
Inter-Nation safety Inter-Sub-Continent balance of forces |
Late/Concealed Global war
Mid deterrence war Early restrained ?maneuvering engagement? |
2 | ~ 70 - ~ 700 |
Late Global adulthood
Solar Systemic infancy |
Partial Earth management | Up to ~.9 | Mid Earth deuterium fusion |
Inter-Nation security
Inter-(Sub-)Continent safety Inter-Planetary balance of forces (between native dry-surface dominant (human) and extraplanetry aquatic dominant species on Earth) |
Late deterrence war
Mid restrained ?maneuvering engagement? Early Oribal ?protection? & NLNM combat |
3 | ~ 700 - ~ 7K | Early Solar Systemic childhood |
Full Earth management
Early Solar System management |
Up to ~1 |
Late Earth deuterium fusion
Early Solar-System resource fusion |
Inter-Continental security
Inter-Planetary safety (between Solar System native dry-surface dominant [human] on Earth and extra-solar dry-surface dominant [on Venus and/or Mars] species) Entering (as a planet - Earth) into Inter-"Nearby interstellar space-faring, relatively close level of development civilization" balance of forces |
Late restrained ?maneuvering engagement?
Mid Oribal ?protection? & NLNM combat Early Solar System ?force positioning? & ? Solar-System-Inter-Planetary NLNM combat ? |
4 | ~ 7K - ~ 70K |
Late Solar Systemic childhood, early adulthood, adulthood
? Sub-Galactic (internal) arrival and co-positioning ? |
Partial Solar System management | Low 1.Ns | Mid Solar System resource fusion |
Inter-Planetary security (inside the Solar System)
Participating in Inter-"Nearby ... civilization" safety Entering (as the Solar System) into Inter-Multi Parsec balance of forces (for a grouping of "Nearbly ... civilizations") |
Late Orbital ?protection? & NLNM combat
Mid Solar System ?force positioning? & ? Solar-System-Inter-Planetary NLNM combat ? Early Multi-Parsec (?systemically?) collaborative ?force projection? & ?? Cross-Star-System NLNM combat ?? |
5 | ~ 70K - ~ 700K |
Late Solar Systemic adulthood
? (Internal) Sub-Galactic infancy ? |
Full Solar system management
Early Sun management |
Mid 1.Ns |
Late Solar System resource fusion
Early Solar extraction fusion |
Contributing to Inter-Star System security
Participating in Inter-Multi Parsec safety ? Entering (as a ?grouping of "Nearby ... civilizations"?) into Inter-Greater Parsec balance of forces "for sufficiently developed+" civilizations? |
Late Solar System ?force positioning?? & ? Solar-System-Inter-Planetary NLNM
combat ?
Mid Multi-Parsec (?systemically?) collaborative ?force projection? & ?? Cross-Star-System NLNM combat ?? ? Early Greater Parsec (?systemically?) joint ?force expeditioning? ? & ??? Cross-Star-System-grouping NLNM combat ??? |
6 | ~ 700K - ~ 7M | ? Early (internal) Sub-Galactic childhood ? | Mid Sun management | High 1.Ns | Mid Solar extraction fusion |
Contributing to Inter-Multi Parsec security
? Participating in Inter-Greater Parsec safety ? ?? Entering (as a ??grouping of Multi-Parsec sufficiently+ developed civilizations??) into (internal) Sub-Galactic balance of forces (for "a wide range of development" civilizations) ?? |
Late Multi-Parsec (?systemically?) collaborative ?force projection? & ??
Cross-Star-System NLNM combat ??
? Mid Greater Parsec (?systemically?) joint ?force expeditioning? ? & ??? Cross-Star-System-grouping NLNM combat ??? ?? Early stage participation in (internal) Sub-Galactic ?guarding? ?? & ¯\_(ツ)_/¯ |
7 | ~ 7M - ~ 70M | ? Late (internal) Sub-Galactic childhood, early adulthood, adulthood ?
?? (Internal) Galactic arrival ?? |
Late Sun management
? Minor-excessively-metallic star management ? |
Collaborative 2 |
Late Solar extraction fusion
? Minor-excessively-metallic star (core material extraction and) fusion ? |
? Contributing to Greater Parsec security ?
?? Participating in (internal) Sub-Galactic safety ?? ??? Entering (as a ???grouping of Greater-Parsec civilizations with a wide range of development???) into (internal) Galactic balance of forces ??? |
? Late Greater Parsec (?systemically?) joint ?force expeditioning? ? & ???
Cross-Star-System-grouping NLNM
combat ???
?? Mid-stage participation in (internal) Sub-Galactic ?guarding? ?? & ¯\_(ツ)_/¯ ??? Early-stage participation in (internal) Galactic ?garrisoning? ??? & ¯\_(ツ)_/¯ |
NOTE:
Stage | Predominant security guarantees between the dominating being groups of the entities (and with moving of the earlier stage to the next formation level up) |
Balance of forces | No total war |
Safety | No systemic war |
Security | No war |
There may be a multitude of very good, even nobile reasons why older civilizations could choose nomadic lifestyles, (logically) in environments with perfectly reproduced conditions. Localized presence may be required to pull and push dark matter towards or away from the galactic center to control its speed and acceleration, or maintaining clusters of manageable black holes may be required to control galaxy's direction. Or maybe it's sub-galactic or even just regional matters - we just don't know. No matter the level of work would require that, loosing focus on our home world and star is not the way forward. With that attitude MTABS principles argue that before we join the galactic workforce our time is best spent focusing on what is and will always be important to us - our planet, with all of its natural imperfections and problems. And, once we are managing Earth our time will be best spent focusing on managing our star. The MTABS hypothesis is that only by sequentially focusing on those two things first we'll we trully be able to contribute to regional and eventually sub-galactic and even galactic projects.
Added 8/23/2024 Of course, other scenarios are possible. Maybe early Kardashev 2 civilizations face a crisis of ascension into that level, at which point one of the possible outcomes is growing your population via building very large habitats that are gravitationally and atmospherically equivalent to their homeworlds but can support an order of magnitude (or even two orders of magnitude) higher population (perhaps given a much larger surface area). And of course, in a good way, there would be any number of functional reasons for such habitats, ranging from providing material support and security to lesser developed yet still very busy civilizations to (potentially) dealing with geographic issues.
Added 8/23/2024 One can only hope that building inter-stellar habitats is not a dead-end way that prevents a civilization from ever joining (the other galactic civilizations) in building (or maintaining, as we just don't know the state of things in the Milky Way) a Kardashev 3 level system.
MTABS draws parallels between a human lifecycle and the lifecycle of humanity as a whole, but without a terminal death, arguing that just as humans should eventually live to 700 years of age, and with passing eons potentially achieve (besides the given at spiritual level) physical and mental immortality, so should should humanity. This is the other necessary component of MTABS:
May there always be Sun(shine),Just as everyone should enjoy the luxury of having their parents around (at least while they bring up their children and grandchildren) we should (at the very least in our infancy and childhood) have the luxury of being on our mother planet, with our star. MTABS argues that joining the galactic workforce in "stellar infancy" (per the model < 700,000 years from now, Update 8/23/2024 given the broad assumption that equates 1 million rotations around the Sun to one year of a galactic-level civilization, specifically for our civilization) would not contribute to the solution of galactic problems. Subsequently, the lifecycle parallel continues that like of reasoning: Why go to "regional childcare" at 3 weeks if nothing is forcing your mother to shift her attention until you are 3 years of age?
And the argument extends that doing so in "early galactic childhood" won't do much good either: why go to a boarding school from first grade? And even beyond, in near-Kandrashev 2 "school and college years" - why go to an elite university (to build connections that you can just as easily build later with far fewer mistakes) if what you really need is a good education and the support of your family (occasional, exploratory travel based friendships aside). And even as we take on long term parenting roles over newer species and "build and grow our new interstellar family", our primary focus should be the challenges of our family not those of the city. Even as adults who take care of our children, we miss "mom's cooking and father's advice". Hence, if you are not disabled by "old age", why serve your country (wider galactic region - a large fraction of the galaxy) and planet (the galaxy) before you've helped with your (?wider galactic-regional?) grandchildren and maybe even played with your (?galactic?) great-grandchildren?
Added 8/23/2024 Or, perhaps more correctly, as we get involved in facilitating the development of younger species (which the MTABS model assumes to be the natural course of things) (after a good period of "growing up time", ~25 million years from now) directly, we will likely be involved in lesser-regional affairs that deal with our region and the region of the "parented" intelligent (at least technologically, or yet semi-intelligent) species. Then subsequently, as we progress to more of a support role of a larger number of the "brought up" early stage "parents", and further develop our technological and industrial capabilities (~50 million years from now) we would naturally be involved in the affairs of our greater region of the galaxy. Subsequently, via the logically following, natural expansion of influence, combined with a more hands-off approach, and as we gain the necessary (very mass scale) equipment and galactic-maintenance capacities, we would finally start to be involved in galactic matters.
Thus, MTABS hypothesis argues that it will take (per the model) at least 70+ million years of "family work" before we can trully take on wider community projects.
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