#cloud migration system

[tm-systems]

Get Best Cloud Migration Services

Cloud migration providers are companies or services that help businesses move their data, applications, and other IT resources from on-premises systems to cloud-based infrastructure. The services providers including assessment planning, data and application migration, etc.

[hlbsolutionsontario]

[auroraelabs]

Best Cloud Architecture Redesign Service Provider

Are you looking for best cloud architecture redesign service? Then you can count us! We provide latest technological solutions available on cloud through API’s & build innovative solutions. For more information, you can visit our website.

[kssgservices]

Maximizing Performance: Migrating Oracle PeopleSoft Application Services to Oracle Cloud Infrastructure

In the ever-evolving landscape of enterprise applications, migrating Oracle PeopleSoft Application Services to Oracle Cloud Infrastructure (OCI) has emerged as a game-changer. This shift isn't just a trend; it's a strategic move that offers a plethora of benefits while addressing certain challenges.

Why the Move?

Oracle PeopleSoft Application Solutions cater to diverse organizational needs, and migrating them to OCI amplifies their potential. Improved scalability, agility, and cost-efficiency stand out as primary drivers. OCI's elastic nature allows seamless scaling, accommodating fluctuating workloads without compromising performance. Moreover, the pay-as-you-go model ensures optimal resource utilization, reducing unnecessary expenses.

Challenges to Address:

However, this transition isn't without hurdles. The complexity of the migration process, ensuring data security, and maintaining system integrity pose significant challenges. Compatibility issues between on-premises setups and the cloud environment demand meticulous planning and execution. Addressing these concerns requires a robust strategy and leveraging Oracle's best practices.

Best Practices for Success:

Successful migration hinges on meticulous planning. Start by conducting a thorough assessment of the existing PeopleSoft environment to strategize the migration roadmap. This includes workload analysis, identifying dependencies, and selecting suitable OCI services. Leverage Oracle's Migration Accelerators and tools like Cloud Manager for streamlined migration and deployment.

Optimizing Performance:

Once migrated, optimizing PeopleSoft on OCI is crucial. Utilize OCI's advanced monitoring tools to track performance metrics in real-time, ensuring optimal system health. Implement automated backups and disaster recovery plans to safeguard critical data.

Community Support and Continuous Learning:

Leverage the vast Oracle PeopleSoft community for insights, best practices, and support. Attend relevant conferences and webinars to stay abreast of the latest advancements in maximizing PeopleSoft on OCI.

Migrating Oracle PeopleSoft Application Services to OCI is a strategic move towards future-proofing your organization's ERP landscape. By embracing best practices and leveraging OCI's robust infrastructure, organizations can unlock the true potential of their PeopleSoft solutions.

[syngrowc]

Ensuring a future-ready and resilient tech ecosystem. 🌟 Stay with us as we journey toward a seamless digital tomorrow!

visit us at - www.syngrowconsulting.com Email us at - contact@syngrowconsulting.com Call us at - +1 (917) 764 5482

[rpgprogrammers]

Ibmi Iseries/AS400 Services | AS400 Software Solutions

[appletechx]

Data Migration: Driving Digital Transformation & Enhancing Efficiency

In today's digital age, data is king. It is the lifeblood of businesses, providing insights into customer behavior, market trends, and operational efficiency. As a result, data migration is becoming increasingly important for businesses that want to stay ahead of the curve.

Data migration is the process of moving data from one system to another. This can be a complex and time-consuming process, but it can also be a valuable opportunity to improve the quality and accessibility of your data.

There are many reasons why businesses choose to migrate their data. Some common reasons include:

To improve performance. Moving data to a more efficient platform can improve performance and reduce costs.

To improve security. Moving data to a more secure environment can help protect your data from unauthorized access.

To comply with regulations. Moving data to a platform that meets regulatory requirements can help you avoid fines and penalties.

To modernize your IT infrastructure. Moving data to a newer platform can help you take advantage of new technologies and improve your overall IT efficiency.

In addition to these benefits, data migration can also help businesses drive digital transformation. By migrating data to the cloud, businesses can gain access to new analytical tools and insights that can help them make better decisions. They can also use data migration to create new products and services that meet the needs of their customers.

Of course, data migration is not without its challenges. Some of the challenges that businesses may face include:

Data compatibility. The data you are migrating may not be compatible with the new platform. This can require you to clean or transform the data before you can migrate it.

Data loss. There is always a risk of data loss during a migration. This is why it is important to have a backup plan in place.

Cost. Data migration can be a costly process. This is why it is important to carefully plan your migration and choose the right tools and services.

Despite the challenges, the benefits of data migration can be significant. By carefully planning and executing your migration, you can improve the quality and accessibility of your data, improve performance, and enhance security. You can also use data migration to drive digital transformation and create new opportunities for your business.

Here are some tips for a successful data migration:

Start by assessing your current data landscape. What data do you have? Where is it stored? What format is it in? This will help you determine the scope of your migration and identify any potential challenges.

Create a detailed migration plan. This plan should include the following:

The goals of your migration

The steps involved in the migration

The timeline for the migration

The resources you will need

Test your migration plan thoroughly. This will help you identify any potential problems and ensure that your migration is successful.

Have a backup plan in place. This will help you recover your data in the event of a problem.

Communicate with your stakeholders throughout the migration process. This will help keep them informed and avoid any surprises.

By following these tips, you can increase your chances of a successful data migration.

Conclusion

Data migration is a complex and challenging process, but it can be a valuable opportunity to improve the quality and accessibility of your data, improve performance, and enhance security. By carefully planning and executing your migration, you can reap the benefits of data migration and drive digital transformation for your business.

[writers-reach]

I have a request for joker (could you use akira for the name please).

Something like his s/o is also in the phantom thieves and when they are in safe rooms she likes to do small braids in his hair, also while chilling out at leblanc maybe :3

Might be a silly request but I thought it was cute, have a great day!

persona 5: playing with his hair (akira kurusu/ren amamiya)

notes: akira kurusu for protag, fluff, fem!reader, reader is a phantom thief, this might be sliiightly inaccurate since i haven't touched p5 in a while and idc to check myself

you were grinding through mementos one day with the rest of the phantom thieves, and things were going pretty well! shadows were being slain, treasure was being looted, and you were overall having a fun time riding around in morgana's van form.

you were grateful, though, for makoto's recent membership of the team. she was better at driving the van than akira was (bless his heart), which meant she took the wheel while akira sat in the passenger's seat, telling her where to go.

you sat behind him in the second row of seats, often leaning your head on the seat in front of you, sometimes babbling to get akira's attention. he'd always reach back to ruffle your hair or playfully offset your mask.

but your attention always drifted to his hair - his soft and undoubtedly fluffy head of black feathery hair. you'd been together for a while, so physical interactions weren't uncommon, but you've never really asked him if you could play with his hair.

you really, really wanted to play with his hair. holy shit, you wanted nothing more than to do that. but now wasn't the right time, being in mementos and all. you'd have to strategise for another time.

thankfully, that time came when after leaving mementos, akira invited you back to leblanc to destress and chill out. he'd make some coffee, you two would chat and cuddle, probably watch some tv.

you accepted, obviously, and taking his hand in yours, led you through the subway system to yongen-jaya and to leblanc. after pouring the two of you a damn good cup of coffee, you two went upstairs to his room in the attic.

after watching a few episodes of that cheesy action show you two like to riff on (and getting the neo featherman r theme song stuck in your head), you two migrated to his bed. akira sat down and extended his arms, inviting you in for a spooning sesh, but you waved your hands in denial.

after a puzzled and slightly pouty look from your boyfriend, you clarified what you meant: "i wanna be big spoon. i kinda... wanna play with your hair? is that cool?"

akira's eyes lit up and he adjusted his glasses that slipped down his face. a slightly goofy grin played across his lips and he shuffled on the bed, allowing you to slot yourself behind him.

"yeah, sure! go right ahead."

you quickly got to work, running your hands through his hair (which was still surprisingly soft and felt like heaven's clouds within your fingertips). you twirled some strands around your digits here and there and massaged his scalp.

akira leaned his head back into your touch, smiling all the while. you could've sworn you heard him purring (maybe that was your imagination, or maybe he was spending too much time with morgana).

you pressed a kiss to the side of his temple and kept playing with his hair long into the night...

a/n: cat-coded joker ftw!!! also i love writing akira being more, like, a dork? i love his canon characterisation in the anime and it's not something i see often. you'll be seeing more silly goofy joker from me if y'all request it lmao

[whirligig-girl]

Losar System

Cooking the Solar System from the Inside Out

(yeah lol it does kinda look like it says Loser)

For this system layout, I have taken the Solar System planet's orbital distance in astronomical units, and taken the reciprocal.

The major planets, in order of increasing distance from Los, are Enutpen, Sunaru, Nrutas, Retipuj, Sram, Thrae, Sunev, and Yrucrem.

Read more about them below the cut:

The Losar system formed through a very different mechanism to our solar system. I'm not sure entirely about the specifics, but the arrangement is not dissimilar to the Kepler-90 system, in which 6 super-earth-mass planets are extremely compact and close to their parent star, with a low-mass and a high-mass gas giant at the outer part of the solar system. Perhaps as Retipuj formed, it migrated inward, carrying with it the ice and gas necessary to form the super-earth-mass planetary cores which accreted into Enutpen and Sunaru, or perhaps there was some kind of switcharoo where the Hot Ice Giants started out on more distant orbits, before crossing orbits with Retipuj and then being coralled into lower orbits.

Either way, some kind of migration is necessary, since Enutpen and Sunaru are volatile-rich, and the outer planets are comparatively volatile-poor.

I've excluded Pluto (or "Otulp") and the other dwarf planets, not because I don't like them or think they count as planets, but because I think by the time you're accounting for every large object in the Solar system in the Losar system, it just gets really implausible. also I bet some objects end up inside of the Sun. Plus, this kind of thought experiment is playing the same kind of planetary dynamics game that splitters are playing when they say Pluto's not a planet. Suffice to say, there are definitely lots of interesting small worlds in the Losar system, but they don't have 1:1 analogues with Solar system planets.

There are only five large moons in the entire system. Aside from Retipuj, satellites and rings are not stable around any of the Hot Giants. If satellites were initially formed around the Hot Giants, they would have either crashed into the planets or were ejected into one of the asteroid belts.

The first civilization to arise in the Losar system are the Sunevians, suspiciously great-ape-like feathered aliens who walk on their upper limbs and use their lower limbs as graspers. Sunev is an oceanic world with one large australia-sized landmass and a great number of volcanic islands. The ocean is relatively shallow, with a lot of coral reefs across the planet. The world is kept warm due to an atmosphere with an Earthlike composition but over twice the atmospheric pressure. Its slow retrograde rotation period results in day/night cycles which are more like seasons, and there is plenty of time during the warm nights to peek through the relatively dense cloud cover into the nearly empty sky. Early or late in the night, one might be able to see Thrae and Noom, or Sram, or if they catch it at just the right time, they might see the incredibly bright spectacle of Retipuj or even Nrutas peek out of the treeline, brighter than any planet or star. On a really good sunset across the ocean with clear skies, some observers report seeing additional super-bright red stars next to the red Sun, but these are thought to be some kind of weather phenomenon reflecting sunlight.

In rare moments of clear skies at night, away from light pollution, one might see many faint hazy spectacles. The zodiacal light (meteoroids orbiting beyond Yrucrem) shines as a faint haze across the ecliptic. The milky way too, shines as a glittery patchy cloud across the sky. But sometimes, every few hours, early in the night, there is a bright patch near the sun, brighter than the zodiacal light. A mystery for ages, but this is now known to be the cometary tail of Enutpen. Sunaru's tail is also detectable, but substantially fainter.

Sunaru and Enutpen were the first planets to be discovered, and were detected within a week of one another by early Losar observers. After the invention of the astronomical telescope, a reflector, observers got very bored during the daytime months. That is, until someone figured out a safe way of pointing towards the Sun. At a cadence of 52 and 103 hours, little black dots would march across the Losar disk. 52 hours was also the cadence of the brightening and dimming of the twilight zodiacal light. And suddenly, two brand new planets were discovered!

Millions of years later on the cold ice-age planet Thrae, astronomers would have an easier time with Enutpen and Sunaru, having known them to be planets since antiquity, due to their apparitions during total solar eclipses. Thrae's comparative cloudlessness also helps.

Sunev has three tiny asteroid moons, which was a helpful jumpstart to Sunevian space exploration, providing early wins for all four space programs. But these little asteroids were not truly other worlds, merely refueling outposts on the way to the rest of the Losar system.

Every few years, there would be a perfect alignment between Sunev and the Hot Giants to allow for a grand tour to be completed using only flybys of the gas giants, with minimal propellant expenditure. The first grand tour attempt got no further than Retipuj--contact was lost due to overheating before the probe made its Nrutas flyby. Specially developed solar flyby probes had to be developed that could survive hotter temperatures before the Hot Giants could be properly explored. These probes would resemble the Parker Solar Probe in some ways, albeit with very different scientific instruments designed for planetary science as opposed to Oilehphysics. Nrutas, Sunaru, and Enutpen turned out all to be much less massive than originally thought, having been puffed up to a larger diameter by being cooked by solar radiation. Nrutas, thought to be the king of the planets, turned out to be merely puffing up its crest to appear regal, so to speak.

Retipuj's moons were incredibly interesting. Retipuj turned out to have 8 satellites--four tiny inner asteroid moons, and four large satellite planets. Otsillac, the innermost turned out to be a volcanic world, yellow-brown in color and pitted with dull-red volcanoes, and a thin atmosphere constantly replenished by volcanic plumes. The next three are in a Ecalpal Resonance of 1:2:4. Being both larger than Otsillac (and, in fact, Yrucrem) and in a more eccentric orbit, Edymenag was even more volcanically active, with a molten surface and exposed mantle. The smaller and more distant Aporue and Oi turned out to be less active, with only a few active volcanoes and many extinct ones. Oi was the least active--although the most recent eruptions were only half a million years old, it was practically dead. It was also the only one with a substantial amount of impact craters, and like Thrae's satellite, Noom, there is likely some volatile ices stuck in the permanent darkness of polar craters.

Hot Giant exploration was best appreciated by specialists, but the other outer planets were much more appreciated. Sram was thought to be warm enough to potentially support liquid water, but its atmosphere ended up being 1/20th of the pressure initially expected, the majority of it having been blown away into space by the Losar winds and the Enutpen tail. But Thrae was a sweet spot--it may have had a thinner atmosphere, but that was compensated by being nearer to Los. In addition, a giant impact it sustained billions of years ago lead to it having a powerful magnetic dynamo to survive the onslaught of the Losar and Enutpen winds. Thrae was a habitable biosphere of similar complexity to Sunev's, albeit with deeper oceans and all the alien horrors that comes with the territory.

Even Yrucrem turned out to be a surprise--despite a dull appearance in telescopes, it was found to have cryovolcanoes and pockets of subsurface oceans, which could potentially support a biosphere. It's a dark brown color due to ice having been aged by solar radiation, with white spots and rays spraying out from recent asteroid impacts and cryovolcanic plumes. The small planets of the trans-Yrucrem asteroid belt were a similar treasure trove, although the nearest large trans-Yrucrem planets were a dozen au away, and requiring RTG power sources. Initial flyby probes to the Trans-Yrucrem-Objects required both being capable of surviving the oppressive heat of Los-shine near Retipuj, and the cold of deep deep space, in order to take advantage of Sunev-Thrae-Sunev-Retipuj gravity assists.

The Sunevians never had a chance to discover the deepest secrets of the Losar system. Their planet froze over due to anthropogenic aerosol production intended to reverse anthropogenic carbon emission, civilization fell, and it never recovered.

But millions of years later, perhaps the Thraelings have a chance to discover, whether through direct imaging or through analyzing the weirdly arrayed orbits of certain trans-yrucrem objects, the four Cold Giant planets, and the distant brown dwarf companion of the Losar system...

[chroniclingworlds]

Auranauts

As the Viatora evolved wings to take advantage of atmospheric water, their predators soon followed. Now, huge clouds of arboreal Viatora travel the planet as “air plankton”, following the moisture-filled clouds that sustain them. In turn, these are hunted by some of the strangest animals on Strix. With one lung adapted into a buoyant gas sac and bodies modified to be as lightweight as possible, the Auranauts glide through the air without ever touching a solid surface.

Silverwings

Pictured: the greater kite-bird, found across the skies of the northern hemisphere.

With lazily undulating wings, the Silverwings fly through the lower atmosphere, beneath the cloud cover, searching for any air plankton that get caught in downdrafts. Unlike all other Auranauts, who brood their young attached to their own bodies until their gas bladders develop, the Silverwings are a more primitive lineage who must deposit their eggs on a tree. They do this with impressive aerial acrobatics, swooping down and laying an egg in the canopy without ever landing until they have deposited all their young. The eggs stick to the leaves and hatch into tiny versions of the adults, who take flight almost immediately after birth.

Devilbirds

Pictured: the magnificent devilbird, the largest species, migrates seasonally between the northern and southern hemispheres with the rain.

Although their name is intimidating, these are harmless creatures which feed only on air plankton. However, their large size and angular jet-black bodies have created ominous legends about them, including that they are omens of death. These are the largest of the Auranauts, typically living in groups of five to ten and cruise relatively low in the atmosphere, often just above the surface of the Southern Sea. These creatures migrate huge distances with the seasonal rains, behaving almost like small versions of the Papyracetae, potentially an example of convergent evolution between these two different lineages.

Stormriders

Pictured: the yellow-spotted stormrider, which has been seen all across the planet but most frequently sighted in the south.

While most Auranauts avoid the strong winds and dangerous lightning found inside storms, Stormriders take advantage of these conditions. With a highly sensitive electrical sensory system, they can detect the lightning coming and avoid strikes, and the shape of their bodies allows them to remain balanced and return to an upright position even in turbulence. Utilizing the chaos that storms enact upon clouds of air plankton, they snap up the disoriented Viatora and will also feed on Darts that are sucked into the storm cloud. These exquisitely adapted animals are captivating to witness flying in and out of storms.

Darts

Pictured: the iridescent stripe-wing, which migrates seasonally with the rain between the Moon Sea and the Southern Sea.

Like a dragonfly, these animals can fly in any direction they please. While many Auranauts evolved to be larger and gulp huge mouthfuls of air plankton, Darts took the opposite approach and became tiny and highly maneuverable to catch individual Viatora. They live in all levels of the habitable atmosphere, following swarms of air plankton wherever they go, and are frequently preyed upon by larger Auranauts. Some scientists consider them to be air plankton themselves, given their abundance, small size, and status as prey animals. Certain species also follow around the Papyracetae, feeding on parasites that attach to the giants.

Cruisers

Pictured: the orange-headed cruiser, which patrols the regions between the Southern Sea and the Black Mountains.

A larger relative of the Darts, Cruisers are incredibly fast and agile, and unlike their relatives, are macro-predators. They hunt and feed on smaller Auranauts, including juveniles of bigger species. These intelligent pack-hunters communicate with high-pitched trills and clicks, and seem to have complex social structures within their groups. Although formidable predators, they are preyed upon by the larger and more voracious Terebroids, so one member of the pack always serves as a lookout when others are hunting or resting. Aside from the Rostertia, these may be the most intelligent animals on Strix.

[hlbsolutionsontario]

Managed IT Service Solutions for Modern Businesses

TITLE: Managed IT Service Solutions for Modern Businesses Today's commercial landscape demands technological proficiency and seamless operations. Companies of all sizes acknowledge the need for comprehensive technology solutions to maintain their competitive edge and optimize productivity. Among these essential services, Managed IT service has emerged as a steadfast solution to the complex challenges businesses face daily. Here’s how you can ensure that your business stays ahead in today's tech-driven world. 1. Embrace Advanced Managed IT Services: In major cities like Toronto, where competition among businesses is fierce, employing robust managed IT services ensures continuous operation and minimal downtime. Partnering with a reputable IT company in Guelph or Toronto provides you access to cutting-edge technologies, proactive system monitoring, and strategic planning that aligns with your specific business objectives. 2. Streamline Communication with Business Phone Systems: Effective communication forms the bedrock of any thriving enterprise. Modern business phone systems offer more than just voice calls; they facilitate video conferencing, instant messaging, and customer management tools integrated into one platform. By leveraging these systems, your company can boost internal collaboration while providing exceptional customer service. 3. Secure Your Operations with Cloud Solutions: As cyber threats evolve, safeguarding data has never been more important. Cloud solutions offer scalable and flexible infrastructure that enables secure data storage, backup, disaster recovery plan—all while allowing employees to collaborate efficiently regardless of location. 4. Navigate Complexity with Business IT Support: Staying on top of the latest software updates and hardware requirements can be daunting for companies without dedicated technical support teams. A reliable IT services provider in Toronto or elsewhere grants you peace of mind with comprehensive support plans tailored to address hardware issues, software glitches, and overall tech maintenance. 5. Invest in a Strategic Partnership with an IT Services Firm: The value of a strategic partnership with an experienced IT company cannot be overstated. Such partnerships allow for proactive planning around technology initiatives that keep your business at the forefront of innovation while managing operational costs effectively. By engaging a trusted partner like HLB System Solutions specialized in offering advanced managed IT service solutions including cloud technologies and state-of-the-art business phone systems—a move which not only enhances day-to-day workflows but also secures long-term growth prospects through innovative technologies adapted to your unique business needs—ensure your organization is poised for success amidst an ever-changing technological era.

For More Details:

Contact us: HLB System Solutions Address : 291 Woodlawn Rd W Unit C3,Vancouver,British Columbia,N1H 7L6 Email : sales@hlbsolutions.com Hours : Monday : Friday:8:00 : 5:00

[boinkingbattlemechs]

Viper

The Viper is a fast, highly-maneuverable medium OmniMech originally designed by Clan Fire Mandrill on Shadow. Code-named the Dragonfly by the Inner Sphere forces that first encountered this small but fierce OmniMech, the name stuck because of its ability to move swiftly over the battlefield. The Viper is fast and well-armored, but significantly undergunned compared with other Clan OmniMechs massing 35–45 tons (including the Adder, Battle Cobra, Grendel, Shadow Cat, Pouncer, and Cougar).

Clan Ghost Bear came into possession of the design in 3002 when they traded several production runs of Executioner OmniMechs for the design and production facilities on Shadow. Rather than Trial for land rights to Shadow, and become embroiled in the internecine struggles of the Fire Mandrills, the Bears restructured the facility, making the lines modular, and relocated production to Strana Mechty - this modular technology proved very useful when the Ghost Bears migrated back to the Inner Sphere in the late 3050s. Surprisingly, the Bears left their first modular production facility on Strana Mechty. Production continued on Strana Mechty for Clan Ghost Bear until the mid-3060s when the Hell's Horses won the production rights and the facility (and then promptly lost the facility to Clan Ice Hellion in 3068). In addition to the manufacturing plant on Strana Mechty, at least one other planet in the Homeworlds was home to a manufacturing line producing Vipers; in 3071 Clan Goliath Scorpion captured a Viper factory from Clan Coyote on Delios, although it is unknown if the planet survived the Wars of Reaving, Goliath Scorpion Abjurement and the subsequent abandonment of the planet by the Coyotes and Cloud Cobras.

Following the Wars of Reaving, the remaining Home Clans would continue to field the design as the Ice Ferret was phased out, possibly due to its association with the Spheroid Clans.

The Viper is built on a lightweight Endo Steel chassis and powered by a weight saving 320 XL engine that propels the Viper to a top speed of 129.6 km/h. The Viper augments its impressive ground speed with eight jump jets that allow it to jump up to a distance of two hundred and forty meters. The Viper has seven tons of ferro-fibrous armor to absorb any damage from shots that are lucky enough to strike it and has eight and a half tons of podspace for its weapons payload.

In its primary weapons configuration, the Viper is configured to fill a variety of close combat roles. The Viper has an anti-missile system for added defense capabilities and two machine guns for use against soft targets and anti-infantry work. The Viper's main guns are two Medium Pulse Lasers and an SRM-4 launcher that allow it to harass other 'Mechs and vehicles.

[dailyanarchistposts]

I wanted to share some thoughts I’ve been having recently about the idea of a “Universal Basic Income” or UBI that has become an important topic of discussion in the US recently.

This January, a Silicon Valley venture capitalist firm called Y Combinator issued a “Request for Research” to explore the idea of a guaranteed income. [1] In the proposal, the firm requests applications from researchers interested in examining what happens when you give a set of people a basic income for a five-year period. The underlying assumption is that they want to know if people will blow free money on heroin, basically.

Paul Graham, founder of Y Combinator and its “philosopher king” according to the Awl, summarized his interest in the problem of income inequality in an essay called “Economic Inequality”: “when I hear people saying that economic inequality is bad and should be eliminated, I feel rather like a wild animal overhearing a conversation between hunters.” [2] After facing criticism for saying this, Graham removed this language in an updated version of the text. [3] The essay is a gripping read. Graham begins by acknowledging himself as a “manufacturer of income inequality” and “an expert on how to increase income inequality.” Graham strikes me as an important, articulate figure explaining how contemporary robber barons in the early 21st century understand the capitalist system.

So UBI is an idea that’s floating around and it’s no surprise that it’s coming from an economic sector, venture capitalists, who make money by investing in companies which are exploring ways to eliminate jobs on an enormous scale. The idea is emerging at the outset of what bourgeois economists are calling “Industry 4.0.” [5] This fourth industrial revolution (after mechanization, water/steam power; mass production, the assembly line, and electricity, and computers and automation) will involve cyber-physical systems, the “Internet of things” and cloud computing, according to its contemporary prophets. But in addition to the enormous profits capitalists hope to make from this transformation in the foundations of the contemporary economy, they are also recognizing the political problems it might produce, in particular the very real possibility of substantial increases in unemployment as new technology enables companies to eliminate jobs once previously considered untouchable.

Truck driving is an important example of how this transformation might take place. Auto companies, as I’m sure everyone knows, are actively pursuing partnerships with Silicon Valley in order to bring computers into cars. In spite of all evidence of the problems of global warming from carbon-based fuel consumption, these companies are actively pursuing self-driving cars. [6][7][8][9]

The problem with this technology, which relates to truck driving, is that driverless technology is actually extremely expensive. Recently, a company called Otto launched with a view toward migrating the technology for driverless cars to trucks. In an interview I heard on the radio, one of its founders noted the expense associated with driverless technology, something like $50,000. For a consumer vehicle, such technology would effectively more than double the cost of a car. But for a semi-truck, that might only add an additional 33% to a truck that would otherwise cost $150,000 or so. The article cites the public health risk that trucks pose — they account for 5.6 percent of miles driven while causing 9.5 percent of the country’s accidents. The article also notes that driverless technology could allow drivers to nap, allowing the trucks to stop less frequently. But the article also notes that there are over 4 million trucks on the road, transporting over 70 percent of the country’s cargo. Let’s face it: there is a real chance that some ambitious trucking companies will seek to eliminate jobs by implementing this technology. Even that modification — sleeping and never stopping — would eliminate jobs. Initially developed as a palliative to long, lone commutes by individual workers, driverless technology can be almost seamlessly converted into an engine of massive job loss. [10][11]

So what is at stake with a Universal Basic Income is that capitalists are recognizing the potential to automate through “Industry 4.0” and want to pursue it. But they also recognize the enormous social dislocations automation on this scale would unleash. And, as Graham says, they would like to not be hunted in the streets and eaten.

The left, as ever, is divided into thousands of competing camps on this issue. One Jacobin article distinguishes between a “livable basic income” (LBI) and a “non-livable basic income” (NLBI), arguing that a UBI would need to be established on a level “high enough to eliminate the need to work for a wage.” [12] I’m not convinced by this, and it also seems, in the context of this article, to support the Jacobin’s interest in reviving not so much a basic income but full employment. The Endnotes collective has criticized this approach as the “primary contradiction” of the labor movement, that is, “that the generalization of one form of domination was seen as the key to overcoming all domination.” [13] Or, more pithily, “Everyone is being proletarianized, and so, to achieve communism, we must proletarianize everyone!”

This approach, Endnotes claims, understands the factory “as the foundation of socialism, not as the material embodiment of abstract domination.” Endnotes demurs on providing strategic guidelines, however, and that vacuum ends up being filled by thinkers like Nick Snick and Alex Williams, authors of Inventing the Future: Postcapitalism and a World Without Work and the #Accelerate manifesto. The latter argues for unleashing “latent productive forces” in technology that a capitalism economic system holds in check. [14] The manifesto suggests that technology has no politics, basically, and the authors want to explore its expansion as a way of creating an alternative to capitalism. I’m not entirely convinced, however, that this technological accelerationism won’t ultimately result in a Matrix-style scenario in which the working class basically functions as batteries fueling a “clean” or environmental future for a few capitalists.

Anyway, I hope this provides some basis for future discussion on another important aspect of contemporary transformations in capitalism, alongside our discussion of the emerging “green” economy.

Footnotes

[1] blog.ycombinator.com

[2] theawl.com

[3] paulgraham.com ; paulgraham.com

[5] en.wikipedia.org

[6] www.freep.com

[7] fortune.com

[8] www.seattletimes.com

[9] www.brookings.edu

[10] www.cnbc.com

[11] medium.com

[12] www.jacobinmag.com

[13] endnotes.org.uk

[14] criticallegalthinking.com

[spacenutspod]

The orbit of Earth around the Sun is always changing. It doesn’t change significantly from year to year, but over time the gravitational tugs of the Moon and other planets cause Earth’s orbit to vary. This migration affects Earth’s climate. For example, the gradual shift of Earth’s orbit and the changing tilt of Earth’s axis leads to the Milankovitch climate cycles. So if you want to understand paleoclimate or the shift of Earth’s climate across geologic time, it helps to know what Earth’s orbit was in the distant past.Fortunately, Newtonian mechanics and the law of gravity work backward in time as well as forward. We can use Newtonian dynamics to predict eclipses and the trajectories of spacecraft to the outer solar system, but we can also use it to turn back the clock and map Earth’s orbit into the deep past. Within limits.Since there is no exact solution for the orbital motion of more than two bodies, we have to run our calculations computationally. A bit of chaos comes into the works, so any uncertainty we have in the current positions and motions of large solar system bodies decreases the accuracy of our retrodiction the further back in time we go. Fortunately with radar ranging and other measurements, our computations are so accurate we can trace Earth’s orbit back 100 million years into the past with some confidence. Or so we thought because a new paper demonstrates we’ve been overlooking the gravitational effect of passing stars.The uncertainty of Earth’s orbit 54 million years ago. Credit: N. Kaib/PSIMost stars are too distant to have any measurable effect on Earth’s orbit. They tug upon our world no more than the distant rocks of the Oort Cloud. But now and then a star will make a close approach. Not close enough to throw our solar system into chaos, but close enough to give the solar planets a gravitational nudge. The most recent close approach was HD 7977. Right now the star is about 250 light-years away, but 2.8 million years ago it passed within 30,000 AU or half a light-year of the Sun. It may have passed as close as 4,000 AU from the Sun. At the larger distance, the gravitational effect of HD 7977 would be negligible, but at the closer end of the range, it would be significant. When you add this into the computational mix, the uncertainties of Earth’s past orbit make it difficult to be confident more than 50 million years. And that has a significant impact on paleoclimate studies.For example, about 56 million years ago Earth entered a period known as the Paleocene-Eocene Thermal Maximum, where global temperatures rose 5 – 8 °C. Orbital models point to the fact that Earth’s orbit was particularly eccentric during that time, which could be the underlying cause. But this new study raises the uncertainty of that conclusion, meaning that other factors such as geologic activity may have played a major role.It’s estimated that a star passes within 10,000 AU of the Sun every 20 million years or so. This means that as we map Earth’s orbital motion deeper into the past, we must also look for effects that may be written in the stars.Reference: Kaib, Nathan A. and Raymond, Sean N. “Passing Stars as an Important Driver of Paleoclimate and the Solar System’s Orbital Evolution.” Astrophysical Journal Letters 962 (2024): L28.The post Passing Stars Changed the Orbits of Planets in the Solar System appeared first on Universe Today.

[blueboxsimulator]

Blue Box Simulator 0.9: The Graphics Update, is already available for PC and Mac

At long last, after months of bugfixing and optimizations for the mobile version which was probably released a bit too early... the latest version of Blue Box Simulator (0.9.33) is already available for desktop!

What's new in version 0.9?

Visual changes:

Migration to the Universal Render Pipeline. It implied redoing every material and custom shader, but in return, it will allow stunning visuals, post-processing effects and...

Bigger on the inside effect! Enable it in Graphics Settings.

Started using Space Graphics Toolkit to improve planets visual quality.

New atmosphere and cloud layers in the Google Earth world scene.

Added subtle animations to some NPCs.

The Cyberman and K9 have a more metallic look.

Updated Io (Jupiter moon) texture.

Changes in Settings:

Removed Render Distance setting, as it would break immersion for little to no performance impact.

Added Render Scale slider, which should actually help with performance!

Separate settings for texture quality and lighting quality in Graphics Settings.

Added Earth Terrain Detail Distance setting in Graphics Settings. Good for detailed landscapes, but the higher the detail distance, the more bandwidth and RAM it will consume.

New settings panel to choose between touch controls and keyboard and mouse controls.

New Features:

Character models on the top of the Cardiff building can now be pushed into the inside of the TARDIS! Yes, materializing around them gets them inside too!

The lighting status of interior windows is now synchronized with exterior windows.

>>Download links<<

What's next?

As of today, I'll start work on version 0.10: The Space Update, a groundbreaking update that will convert this game in no longer just a solar system simulator, but a universe simulator, thanks to the power of the Space Graphics Toolkit asset that I bought which will allow full scale planet terrains, more realistic stars, nebulae, black holes, galaxies, etc.

Let me also mention that developing each small patch can take long days of programming, and although I am juggling this work with other ways to make a living, my income is still well below minimum wage. So, please, spread the word about my Patreon so I can continue releasing updates for many years to come!

[suns-water]

Asteroids, especially carbonaceous chondrites, provide crucial insights into the Earth's water history and the dynamics of planet formation. These meteorites are rich in hydrous minerals, such as clays and hydrated silicates, as well as complex organic molecules. Formed in the outer regions of the Solar System, where water ice and organic compounds remained stable, these asteroids migrated inward and encountered the early Earth, playing an important role in its evolution. The rocky bodies orbiting the Sun, mainly in the asteroid belt between Mars and Jupiter, contain significant amounts of hydrated minerals, indicating the presence of water. Carbonaceous chondrites are particularly important because their isotopic composition is very close to that of water on Earth. Interstellar dust particles, tiny grains of material found in the space between stars, can contain water ice and organic compounds that can be incorporated into the forming Solar System. During the evolution of the Solar System, these particles contributed to the water inventory of planetesimals and planets.

Comets, which have long fascinated astronomers with their spectacular phenomena, also play a crucial role in supplying the Earth with water. Comets are composed of water ice, dust and various organic compounds and originate from the outer regions of the Solar System, such as the Kuiper Belt and Oort Cloud. These pristine materials, remnants of the early solar nebula, offer a glimpse into the conditions that prevailed during the formation of the Solar System over 4.6 billion years ago. Comets, with their highly elliptical orbits, occasionally come close to the Sun, sublimating volatile ice and releasing gas and dust into space. Isotopic compositions of water in comets, such as comet 67P/Churyumov-Gerasimenko studied by the Rosetta mission, are slightly different from Earth's oceans, suggesting that comets are not the only source of terrestrial water, but probably made a significant contribution to early Earth formation. Impacts from comets on during the Late Heavy Bombardment period about 3.9 billion years ago are thought to have deposited significant amounts of water and volatile compounds that supplemented Earth's early oceans and created a favorable environment for the emergence of life. The founder of Greening Deserts and the Solar System Internet project has developed a simple theory about Earth's main source of water, called the "Sun's Water Theory", which has explored that much of space water was generated by our star. According to this theory, most of the planet's water, or cosmic water, came directly from the Sun with the solar winds and was formed by hydrogen and other particles. Through a combination of analytical skills, a deep understanding of complex systems and simplicity, the founder has developed a comprehensive understanding of planetary processes and the Solar System. In the following text you will understand why so much space water was produced by the Sun and sunlight.

Helium and Oxygen From the Sun

While hydrogen is the main component of the solar wind, helium ions and traces of heavier elements are also present. The presence of oxygen ions in the solar wind is significant because it provides another potential source of the constituents necessary for water formation. When oxygen ions from the solar wind interact with hydrogen ions from the solar wind or from local sources, they can form water molecules.

The detection of oxygen from the solar wind together with hydrogen on the Moon supports the hypothesis that the Sun contributes to the water content of the lunar surface. The interactions between these implanted ions and the lunar minerals can lead to the formation of water and hydroxyl compounds, which are then detected by remote sensing instruments.

Magnetosphere and Atmospheric Interactions

The Earth's magnetosphere and atmosphere are a complex system and are significantly influenced by solar emissions. The magnetosphere deflects most of the solar wind particles, but during geomagnetic storms caused by solar flares and CMEs, the interaction between the solar wind and magnetosphere can become more intense. This interaction can lead to phenomena such as auroras and increase the influx of solar particles into the upper atmosphere. In the upper atmosphere, these particles can collide with atmospheric constituents such as oxygen and nitrogen, leading to the formation of water and other compounds. This process contributes to the overall water cycle and atmospheric chemistry of the planet. Interstellar dust particles also provide valuable insights into the origin and distribution of water in the Solar System. In the early stages of the formation of the Solar System, the protoplanetary disk picked up interstellar dust particles containing water ice, silicates and organic molecules. These particles served as building blocks for planetesimals and larger bodies, influencing their composition and the volatile inventory available to terrestrial planets like Earth.

NASA's Stardust mission, which collected samples from comet Wild 2 and interstellar dust particles, has demonstrated the presence of crystalline silicates and hydrous minerals. The analysis of these samples provides important data on the isotopic composition and chemical diversity of water sources in the Solar System.

Solar Wind and Solar Hydrogen

The theory of solar water states that a significant proportion of the water on Earth originates from the Sun and came in the form of hydrogen particles through the solar wind. The solar wind, a stream of charged particles consisting mainly of hydrogen ions (protons), constantly flows from the Sun and strikes planetary bodies. When these hydrogen ions hit a planetary surface, they can combine with oxygen and form water molecules. This process has been observed on the Moon, where the hydrogen ions implanted by the solar wind react with the oxygen in the lunar rocks to form water. Similar interactions have taken place on the early Earth and contributed to its water supply. Studying the interactions of the solar wind with planetary bodies using missions such as NASA's Parker Solar Probe and ESA's Solar Orbiter provides valuable data on the potential for water formation from the Sun.

Theoretical Models and Simulations

Advanced theoretical models and simulations can play a crucial role to understand the processes that contribute to the formation and distribution of water in the Solar System. Models of planet formation and migration, such as the Grand Tack hypothesis, suggest that the motion of giant planets influenced the distribution of water-rich bodies in the early Solar System. These models help explain how water may have traveled from the outer regions of the Solar System to the inner planets, including Earth. Simulations of the interactions between solar wind and planetary surfaces shed light on the mechanisms by which solar hydrogen could contribute to water formation. By recreating the conditions of the early system, these simulations help scientists estimate the contribution of solar-derived hydrogen to Earth's water supply.

The journey of water from distant cosmic reservoirs to planets has also profoundly influenced the history of our planet and its potential for life. Comets, asteroids and interstellar dust particles each offer unique insights into the dynamics of the early Solar System, providing water and volatile elements that have shaped Earth's geology and atmosphere. Ongoing research, advanced space missions, and theoretical advances are helping to improve our understanding of the cosmic origins of water and its broader implications for planetary science and astrobiology. Future studies and missions will further explore water-rich environments in our Solar System and the search for habitable exoplanets, and shed light on the importance of water in the search for the potential of life beyond Earth.

Theoretical models and simulations provide insights into the processes that have shaped Earth's water reservoirs and the distribution of volatiles. The Grand Tack Hypothesis states that the migration of giant planets such as Jupiter and Saturn has influenced the orbital dynamics of smaller bodies, including comets and asteroids. This migration may have directed water-rich objects from the outer Solar System to the inner regions, contributing to the volatile content of the terrestrial planets. Intense comet and asteroid impacts about billions of years ago, likely brought significant amounts of water and organic compounds to Earth, shaping its early atmosphere, oceans, and possibly the prebiotic chemistry necessary for the emergence of life.

To understand the origins of water on Earth, the primary sources that supplied our planet with water must be understood. The main hypotheses focus on comets, asteroids and interstellar dust particles. Each of these sources is already the subject of extensive research, providing valuable insights into the complex processes that brought water to planets. Comets originating in the outer regions of the Solar System, such as the Kuiper Belt and the Oort Cloud, are composed of water ice, dust and organic compounds. As comets approach the sun, they heat up and release water vapor and other gases, forming a visible coma and tail. Comets have long been seen as potential sources of Earth's water due to their high water content.

The Sun's Contribution to the Earth's Water

Further exploration and research are essential to confirm and refine the theory of solar water or sun's water. Future missions to analyze the interactions of the solar wind with planetary bodies and advanced laboratory experiments will provide deeper insights into this process. Integrating the data from these endeavors with theoretical models will improve our understanding of the formation and evolution of water in the Solar System. Recent research in heliophysics and planetary science has begun to shed light on the possible role of the Sun in supplying water to planetary bodies. For example, studies of lunar samples have shown the presence of hydrogen transported by the solar wind. Similar processes have occurred on the early Earth, particularly during periods of increased solar activity when the intensity and abundance of solar wind particles was greater. This hypothesis is consistent with observations of other celestial bodies, such as the Moon and certain asteroids, which show signs of hydrogen transported by the solar wind. Solar wind, which consist of charged particles, mainly hydrogen ions, constantly emanate from the Sun and move through the Solar System. When these particles encounter a planetary body, they can interact with its atmosphere and surface. On the early Earth, these interactions may have favored the formation of very much water molecules. Hydrogen ions from the solar wind have reacted with oxygen-containing minerals and compounds upon reaching the surface, leading to a gradual accumulation of water. Although slow, this process occurred over billions of years, contributing to the planet's water supply. Theoretical models simulate the early environment of the Solar System, including the flow of solar wind particles and their possible interactions with the planet. By incorporating data from space missions and laboratory experiments, these models can help scientists estimate the contribution of solar-derived hydrogen to Earth's water inventory. Isotopic analysis of hydrogen in ancient rocks and minerals on Earth provides additional clues. If a significant proportion of the planetary hydrogen has isotopic signatures consistent with solar hydrogen, this would support the idea that the Sun played a crucial role in providing water directly by solar winds.

The Sun's Water Theory assumes that a significant proportion of the water on Earth and other objects in space originates from the Sun and was transported in the form of hydrogen particles. This hypothesis states that the solar hydrogen combined with the oxygen present on the early Earth to form water. By studying the isotopic composition of planetary hydrogen and comparing it with solar hydrogen, scientists can investigate the validity of this theory. Understanding the mechanisms by which the Sun have contributed directly to Earth's water supply requires a deep dive into the processes within the Solar System and the interactions between solar particles and planetary bodies. This theory also has implications for our understanding of water distribution in the Solar System and beyond. If solar-derived hydrogen is a common mechanism for water formation, other planets and moons in the habitable zones of their respective stars could also have water formed by similar processes. This expands the possibilities for astrobiological research and suggests that water, and possibly life, may be more widespread in our galaxy than previously thought.

To investigate the theory further, scientists should use a combination of observational techniques, laboratory simulations and theoretical modeling. Space missions to study the Sun and its interactions with the Solar System, such as NASA's Parker Solar Probe and the European Space Agency's Solar Orbiter, provide valuable data on the properties of the solar wind and their effects on planetary environments. Laboratory experiments recreate the conditions under which the solar wind interacts with various minerals and compounds found on Earth and other rocky bodies. These experiments aim to understand the chemical reactions that could lead to the formation of water under the influence of the solar wind.

The Sun's Water Theory for Space and Planetary Research

Understanding the origin of water on Earth not only sheds light on the history of our planet, but also provides information for the search for habitable environments elsewhere in the galaxy. The presence of water is a key factor in determining the habitability of a planet or moon. If solar wind-driven water formation is a common process, this could greatly expand the number of celestial bodies that are potential candidates for the colonization of life. The study of the cosmic origins of water also overlaps with research into the formation of organic compounds and the conditions necessary for life. Water in combination with carbon-based molecules creates a favorable environment for the development of prebiotic chemistry. Studying the sources and mechanisms of water helps scientists understand the early conditions that could lead to the emergence of life. Exploring water-rich environments in our Solar System, such as the icy moons of Jupiter and Saturn, is a priority for future space missions. These missions, equipped with advanced instruments capable of detecting water and organic molecules, aim to unravel the mysteries of these distant worlds. Understanding how the water got to these moons and what state it is in today will provide crucial insights into their potential habitability.

The quest to understand the role of water in our galaxy also extends to the study of exoplanets. Observing exoplanets and their atmospheres with telescopes such as the James Webb Space Telescope (JWST) allows scientists to detect signs of water vapor and other volatiles. By comparing the water content and isotopic composition of exoplanets with those of Solar System bodies, researchers can draw conclusions about the processes that determine the distribution of water in different planetary systems.

Most of the water on planet Earth was most likely emitted from the Sun as hydrogen and helium. For many, it may be unimaginable how so much hydrogen got from the Sun to the Earth. In the millions of years there have certainly been much larger solar flares and storms than humans have ever recorded. CMEs and solar winds can transport solid matter and many particles. The solar water theory can certainly be proven by ice samples! Laboratory experiments and computer simulations continue to play an important role in this research. By recreating the conditions of early Solar System environments, scientists can test various hypotheses about the formation and transport of water. These experiments help to refine our understanding of the chemical pathways that lead to the incorporation of water into planetary bodies.

In summary, the study of the origin of water on Earth and other celestial bodies is a multidisciplinary endeavor involving space missions, laboratory research, theoretical modeling, and exoplanet observations. The integration of these approaches provides a comprehensive understanding of the cosmic journey of water and its implications for planetary science and astrobiology. Continued exploration and technological advances will further unravel the mysteries of water in the universe and advance the search for life beyond our planet.

Solar Flares and Coronal Mass Ejections

Solar flares are intense bursts of radiation and energetic particles caused by magnetic activity on the Sun. Coronal mass ejections (CMEs) are violent bursts of solar wind and magnetic fields that rise above the Sun's corona or are released into space. Both solar flares and CMEs release significant amounts of energetic particles, including hydrogen ions, into the Solar System.The heat, high pressure and extreme radiation can create water molecules of space dust or certain particles.

When these high-energy particles reach our planet or other planetary bodies, they can trigger chemical reactions in the atmosphere and on the surface. The energy provided by these particles can break molecular bonds and trigger the formation of new compounds, including water. On Earth, for example, the interaction of high-energy solar particles with atmospheric gases can produce nitric acid and other compounds, which then precipitate as rain and enter the water cycle. On moons, comets and asteroids the impact of high-speed solar particles can form water isotopes and molecules. Some particles of the solar eruptions can be hydrogen anions, nitrogen and forms of space water. This can be proven by examples or solar particle detectors.

More Theoretical Models and Simulations

It should be clear to everyone that many space particles in space can be - and have been - guided to the poles of planets by magnetic fields. Much space water and hydrogen in or on planets and moons has thus reached the polar regions. Magnetic, polar and planetary research should be able to confirm these connections. Many of the trains of thought, ideas and logical connections to the origin of the water in our Solar System were explored and summarized by the researcher, physicist and theorist who wrote this article. Simulations of solar-induced water formation can also be used to investigate different scenarios, such as the effects of planetary magnetic fields, surface composition and atmospheric density on the efficiency of water production. These models provide valuable predictions for future observations and experiments and help to refine our understanding of space water formation.

The development of sophisticated theoretical models and simulations is essential for predicting and explaining the processes by which solar hydrogen contributes to water formation. Models of the interactions between solar wind and planetary surfaces, incorporating data from laboratory experiments and space missions, help scientists understand the dynamics of these interactions under different conditions.

The advanced theory shows that the Sun is a major source of space water in the Solar System through solar hydrogen emissions and provides a comprehensive framework for understanding the origin and distribution of water. This theory encompasses several processes, including solar wind implantation, solar flares, CMEs, photochemistry driven by UV radiation, and the contributions of comets and asteroids. By studying these processes through space missions, laboratory experiments and theoretical modeling, scientists can unravel the complex interactions that have shaped the water content of planets and moons. This understanding not only expands our knowledge of planetary science, but also aids the search for habitable environments and possible life beyond Earth. The Sun's role in water formation is evidence of the interconnectedness of stellar and planetary processes and illustrates the dynamic and evolving nature of our Solar System

The sun's influence on planetary water cycles goes beyond direct hydrogen implantation. Solar radiation drives weathering processes on planetary surfaces and releases oxygen from minerals, which can then react with solar hydrogen to form water. On Earth, the interaction of solar radiation with the atmosphere contributes to the water cycle by influencing evaporation, condensation and precipitation processes. The initiator of this theory has spent many years researching and studying the nature of things. In early summer, he made a major discovery and documented the formation and shaping process of an element and substance similar to hydrogen, which he calls solar granules. A scientific name for the substance was also found: "Solinume". The Sun's Water Theory was developed by the founder of Greening Deserts, an independent researcher and scientist from Germany. The innovative concepts and specific ideas are protected by international laws.

The introducing article text is a scientific publication and a very important paper for further studies on astrophysics and space exploration. We free researchers believe that many answers can be found in the polar regions. This is also a call to other sciences to explore the role of cosmic water and to rethink all knowledge about planetary water bodies and space water, especially Arctic research and ancient ice studies. This includes evidence and proof of particle flows with hydrogen or space water to the poles. Gravity and the Earth's magnetic field concentrate space particles in the polar zones. The theory can solve and prove other important open questions and mysteries of science - such as why there is more ice and water in the Antarctic than in the Arctic.

Very Important Article Updates

The pre-publication of some article drafts formed the basis for the final preparation of the study papers and subsequent publication in July. The translations were done with the help of DeepL and some good people. Everyone who really contributed will of course be mentioned in the future.

Updates and corrections can be done here and for further editions. You can find the most important sources and references at the end, they are not directly linked in this research study, this can be done in the second edition.

Sun's Water Theory – Chapter 2

Solar System Science and Space Water

Another approaches and summaries of the most important findings for the ongoing study you can read here and in attached papers for the theory.

Can solar winds be the main source for water formation in space, on comets, asteroids, moons and planets?

Carbonaceous chondrites are especially important because their isotopic composition closely matches that of Earth's water. Interstellar dust particles, tiny grains of material found in the space between stars, can contain water ice and organic compounds, which can be incorporated into the forming Solar System. As the Solar System evolved, these particles contributed to the water inventory of planetesimals.

Comets, long fascinating to astronomers for their spectacular appearances, also played a crucial role in delivering water to Earth. Composed of water ice, dust, and various organic compounds, comets originate from the outer regions of the Solar System, such as the Kuiper Belt and the Oort Cloud. These pristine materials, remnants from the early solar nebula, offer a window into the conditions prevailing during the Solar System's formation over 4.6 billion years ago. The impacts of comets on Earth during the Late Heavy Bombardment period, around 3.9 billion years ago, are believed to have deposited significant amounts of water and volatile compounds, supplementing the early oceans and creating a conducive environment for the emergence of life.

Interstellar and interplanetary dust particles offer valuable insights into the origins and distribution of water across the Solar System. During the early stages of the Solar System's formation, the protoplanetary disk captured interstellar dust particles containing water ice, silicates, and organic molecules. These particles served as building blocks for planetesimals and larger bodies, influencing their compositions and the volatile inventory available for terrestrial planets.

Earth's Water Budget and Origins

Understanding the current distribution and budget of water on Earth helps contextualize its origins. The water is distributed among oceans, glaciers, groundwater, lakes, rivers, and the atmosphere. The majority of the water, about 97%, is in the oceans, with only 3% as freshwater, mainly locked in glaciers and ice caps. The balance of water between these reservoirs is maintained through the hydrological cycle, which includes processes such as evaporation, precipitation, and runoff. This cycle is influenced by various factors, including solar radiation, atmospheric dynamics, and geological processes.

Water formation in the Solar System occurs through several processes:

Comet and Asteroid Impacts: Impact events from water-rich comets and asteroids deliver water to planetary surfaces. The kinetic energy from these impacts can also induce chemical reactions, forming additional water molecules.

Grain Surface Reactions: Water can form on the surfaces of interstellar dust grains through the interaction of hydrogen and oxygen atoms. These grains act as catalysts, facilitating the formation of water molecules in cold molecular clouds.

Solar Wind Interactions: Hydrogen ions from the solar wind can interact with oxygen in planetary bodies, forming water molecules. This process is significant for bodies like the Moon and potentially early Earth.

Volcanism and Outgassing: Volcanic activity on planetary bodies releases water vapor and other volatiles from the interior to the surface and atmosphere. This outgassing contributes to the overall water inventory. High pressure and heat can push chemical reactions.

Future Research and Exploration

To further investigate the origins and distribution of water in the Solar System, future missions and research endeavors are essential. Key areas of focus include:

Isotopic Analysis: Advanced techniques for isotopic analysis of hydrogen and oxygen in terrestrial and extraterrestrial samples. Isotopic signatures help differentiate between water sources and understand the contributions from different processes.

Laboratory Experiments: Simulating space conditions in laboratory settings to study water formation processes, such as solar wind interactions and grain surface reactions. These experiments provide controlled environments to test theoretical models and refine our understanding of water chemistry in space.

Lunar and Martian Exploration: Missions to the Moon and Mars to study their water reservoirs, including polar ice deposits and subsurface water. These studies provide insights into the processes that have preserved water on these bodies and their potential as resources for future exploration.

Sample Return Missions: Missions that return samples from comets, asteroids, and other celestial bodies to Earth for detailed analysis. These samples provide direct evidence of the isotopic composition and water content, helping to trace the history of water in the Solar System.

Theoretical Models and Simulations: Continued development of theoretical models and simulations to study the dynamics of the early Solar System, planet formation, and water delivery processes. These models integrate observational data and experimental results to provide comprehensive insights.

Heliophysics Missions:

Solar Observatories: Missions like the Parker Solar Probe and ESA's Solar Orbiter are studying the solar wind and its interactions with planetary bodies. These missions provide critical data on the composition of the solar wind and the mechanisms through which it can deliver water to planets.

Space Weather Studies: Understanding the impact of solar activity on Earth's magnetosphere and atmosphere helps elucidate how solar wind particles contribute to atmospheric chemistry and the water cycle. There are great websites and people who providing daily news on these topics.

Implications for Astrobiology

The study of water origins and distribution has profound implications for astrobiology, the search for life beyond Earth. Water is a key ingredient for life as we know it, and understanding its availability and distribution in the Solar System guides the search for habitable environments. Potentially habitable exoplanets are identified based on their water content and the presence of liquid water. The study of water on Earth and other celestial bodies informs the criteria for habitability and the likelihood of finding life elsewhere.

The Sun's Water Theory offers a compelling perspective on the origins of planetary water, suggesting that the Sun, through solar wind and hydrogen particles, played a significant role in delivering water to our planet. This theory complements existing hypotheses involving comets, asteroids, and interstellar dust, providing a more comprehensive understanding of water's cosmic journey. Ongoing research, space missions, and technological advancements continue to unravel the complex processes that brought water to Earth and other planetary bodies. Understanding these processes not only enriches our knowledge of planetary science but also enhances our quest to find habitable environments and life in space.

Hydrogen Transport and Water Formation

Hydrogen ions from solar winds and CMEs play a crucial role in the formation of water molecules in Earth’s atmosphere. This process can be summarized in several key steps:

Chemical Reactions: Once in the atmosphere, hydrogen ions engage in chemical reactions with oxygen and other atmospheric constituents. A significant reaction pathway involves the combination of hydrogen ions with molecular oxygen to form hydroxyl radicals:

H++O2→OH+OH++O2→OH+O

Further reactions can lead to the formation of water:

OH+H→H2OOH+H→H2O

Hydrogen Anions in Atmospheres: The hydrogen anion is a negative hydrogen ion, H−. It can be found in the atmosphere of stars like our sun.

Hydrogen Influx: Hydrogen ions carried by solar winds and CMEs enter Earth’s atmosphere primarily through the polar regions where the geomagnetic field lines are more open. This influx is heightened during periods of intense solar activity.

Water Molecule Formation: The newly formed water molecules can either remain in the upper atmosphere or precipitate downwards, contributing to the overall water cycle. In polar regions, this process is particularly significant due to the higher density of incoming hydrogen ions – negative + positive.

o

Hydrogen is the primary component of the solar wind, helium ions, oxygen and traces of heavier elements are also present. The presence of oxygen ions in the solar wind is significant because it provides another potential source of the necessary ingredients for water formation. When oxygen ions from the solar wind interact with hydrogen ions, either from the solar wind or from local sources, they can form water molecules.

Hydration of Earth's Mantle

Much of the solar hydrogen and many solar storms contributed to the water building on planet Earth but also on other planets like we know now. One of the significant challenges in understanding the water history is quantifying the amount of water stored in the planet's mantle. Studies of mantle-derived rocks, such as basalt and peridotite, have revealed the presence of hydroxyl ions and water molecules within mineral structures. The process of subduction, where oceanic plates sink into the mantle, plays a critical role in cycling water between Earth's surface and its interior.

Water carried into the mantle by subducting slabs is released into the overlying mantle wedge, causing partial melting and the generation of magmas. These magmas can transport water back to the surface through volcanic eruptions, contributing to the surface and atmospheric water budget. The deep Earth water cycle is a dynamic system that has influenced the evolution of the geology and habitability over billions of years.

Impact on Earth's Polar Regions

During geomagnetic storms and periods of high solar activity, the polar regions experience increased auroral activity, visible as the Northern and Southern Lights (aurora borealis and aurora australis). These auroras are the result of charged particles colliding with atmospheric gases, primarily oxygen and nitrogen, which emit light when excited.

The Earth's polar regions are particularly sensitive to the influx of solar particles due to the configuration of the magnetic field. The geomagnetic poles are areas where the magnetic field lines converge and dip vertically into the Earth, providing a pathway for charged particles from the solar wind, CMEs, and SEPs to enter the atmosphere.

The increased particle flux in these regions can lead to enhanced chemical reactions in the upper atmosphere, including the formation of water and hydroxyl radicals. These processes contributed to the overall water budget of the polar atmosphere and influence local climatic and weather patterns.

Implications for Planetary Water Distribution

For planets and moons with magnetic fields and atmospheres, the interaction with solar particles could influence their water inventories and habitability. Studying these processes in our Solar System provides a foundation for exploring water distribution and potential habitability in exoplanetary systems.

Understanding the role of CMEs, solar winds, and solar eruptions in water formation has broader implications for planetary science and the study of exoplanets. If these processes are effective in delivering and generating water on Earth, they may also play a significant role in other planetary systems with similar stellar activity.

Interplanetary Dust and Its Contribution to Water

Interplanetary dust particles (IDPs), also known as cosmic dust, are small particles in space that result from collisions between asteroids, comets, and other celestial bodies. These particles can contain water ice and organic compounds, and they continually bombard Earth and other planets. The accumulation of IDPs over geological timescales could have contributed to Earth's water inventory.

As IDPs enter Earth's atmosphere, they undergo thermal ablation, a process in which the particles are heated to high temperatures, causing them to release their volatile contents, including water vapor. This water vapor can then contribute to the atmospheric and hydrological cycles on Earth. This process, albeit slow, represents another potential source of water.

Magnetospheric and Atmospheric Interactions

Geomagnetic storms, triggered by interactions between CMEs and Earth’s magnetosphere, result in enhanced auroral activity and increased particle precipitation in polar regions. These storms are critical in modulating the upper atmosphere's chemistry and dynamics.

Auroral Precipitation: During geomagnetic storms, energetic particles are funneled into the polar atmosphere along magnetic field lines. The resulting auroras are not just visually spectacular but also chemically significant, leading to increased production of reactive species such as hydroxyl radicals (OH) and hydrogen oxides (HOx).

Ionization and Chemical Reactions: The increased ionization caused by energetic particles alters the chemical composition of the upper atmosphere. Hydrogen ions, in particular, interact with molecular oxygen (O2) and ozone (O3) to produce water and hydroxyl radicals. This process is especially active in the polar mesosphere and lower thermosphere.

The Earth’s magnetosphere and atmosphere serve as a complex system that mediates the impact of solar emissions. The magnetosphere deflects most of the solar wind particles, but during geomagnetic storms caused by solar flares and Coronal Mass Ejections (CMEs), the interaction between the solar wind and the magnetosphere can become more intense. This interaction can lead to phenomena such as auroras and can enhance the influx of solar particles into the upper atmosphere. In the atmosphere, these particles can collide with atmospheric constituents, including oxygen and nitrogen, leading to the formation of water and other compounds. This process contributes to the overall water cycle and atmospheric chemistry of the planet.

Moon and Solar Wind Interactions

On the Moon, the detection of solar wind-implanted oxygen, along with hydrogen, further supports the hypothesis that the Sun contributed and still contributes to the Moon’s surface water content. The interactions between these implanted ions and lunar minerals can lead to the production of water and hydroxyl compounds, which are then detected by remote sensing instruments. Similar interactions could have occurred on early Earth, contributing to its water inventory. The study of solar wind interactions with planetary bodies using space missions, orbiter, probes and satellites can provide more valuable data on the potential for solar-derived water formation.

Solar Wind and Solar Hydrogen

Coronal Mass Ejections (CMEs) are massive bursts of solar wind and magnetic fields rising above the solar corona or being released into space. They are often associated with solar flares and can release billions of tons of plasma, including protons, electrons, and heavy ions, into space. When CMEs are directed towards Earth, they interact with the planet's magnetosphere, compressing it on the dayside and extending it on the nightside, creating geomagnetic storms.

These geomagnetic storms enhance the influx of solar particles into Earth's atmosphere, particularly near the polar regions where Earth's magnetic field lines converge and provide a direct path for these particles to enter the space atmosphere. The hydrogen ions carried by CMEs can interact with atmospheric oxygen, potentially contributing to the formation of water and hydroxyl radicals (OH).

Summary: Water is essential for life as we know it, and its presence is a key indicator in the search for habitable environments beyond Earth. If the processes described by the Sun's Water Theory and other mechanisms are common throughout the galaxy, then the likelihood of finding water-rich exoplanets and moons increases significantly.

The quest to understand the origins and distribution of water in the cosmos is a journey that spans multiple scientific disciplines and explores the fundamental questions of life and habitability. The Sun's Water Theory, along with other hypotheses, offers a promising framework for investigating how water might have formed and been distributed across the Solar System and beyond. Through these efforts, we move closer to answering the profound questions of our origins and the potential for life beyond Earth, expanding our knowledge and inspiring wonder about the vast and mysterious cosmos.

The Sun, as the primary source of energy and particles in our Solar System, has a profound impact on planetary environments through its emissions. Coronal Mass Ejections (CMEs), solar winds, and solar eruptions are significant contributors to the delivery of hydrogen to Earth's atmosphere, particularly influencing the polar regions where the magnetic field lines converge.

Solar wind is a continuous flow of charged particles from the Sun, consisting mainly of electrons, protons, and alpha particles. The solar wind varies in intensity with the solar cycle, which lasts about 11 years. During periods of high solar activity, the solar wind is more intense, and its interactions with Earth's magnetosphere are more significant.

At the polar regions, the solar wind can penetrate deeper into the atmosphere due to the orientation of Earth's magnetic field. This influx of hydrogen from the solar wind can combine with atmospheric oxygen, contributing to the water cycle in these regions. The continuous flow by solar wind particles plays a role in the production of hydroxyl groups and parts of water molecules, especially in upper parts of the atmosphere.

Space Dust, Fluids, Particles and Rocks

Space dust, including micrometeoroids and interstellar particles, is another important source of material for atmospheric chemistry. These particles, often rich in volatile compounds, ablate upon entering Earth’s atmosphere, releasing their constituent elements, including hydrogen.

Ablation and Chemical Release: As space dust particles travel through the atmosphere, frictional heating causes them to ablate, releasing hydrogen and other elements. This process is particularly active in upper parts of the atmosphere and contributes to the local chemical environment.

Catalytic Surfaces: Space dust particles can also act as catalytic surfaces, facilitating chemical reactions between atmospheric constituents. These reactions can enhance the formation of water and other compounds, particularly in regions with high dust influx, such as during meteor showers.

Fluid Dynamics in Space: In astrophysics, the behavior of fluids is critical in the study of stellar and planetary formation. The movement of interstellar gas and dust, driven by gravitational forces and magnetic fields, leads to the birth of stars and planets. Simulations of these processes rely on fluid dynamics to predict the formation and evolution of celestial bodies.

Flux in Physical Systems: The concept of flux, the rate of flow of a property per unit area, is fundamental in both physical and biological systems. In physics, magnetic flux and heat flux describe how magnetic fields and thermal energy move through space. In biology, nutrient flux in ecosystems determines the distribution and availability of essential elements for life.

Plus and Minus Charged Hydrogen Particles: More about magnetic fields, particles flows, solar hydrogen and other space particles are attached in additional papers. +-_-+

Potential Sources of Planetary Water

The discovery of water in the form of ice on asteroids and other celestial bodies indicates that water was present in the early Solar System and has been transported across different regions. This evidence supports the idea that multiple processes, including solar hydrogen interactions, delivery by asteroids and comets, and interstellar dust particles, have collectively contributed to the water inventory of Earth and other planetary bodies.

The theory that much of the planetary water could have originated from solar hydrogen is an intriguing proposition that aligns with several key observations. The isotopic similarities between Earth's water and the water found in carbonaceous chondrites and comets suggest a common origin – they were charged by the sun. Additionally, the presence of water in the lunar regolith, generated by solar wind interactions, supports the notion that solar particles can contribute to water formation on planetary surfaces.

Scientific Observations and Evidence

Scientific observations have provided evidence supporting the role of solar particles in contributing to water formation on Earth and other planetary bodies. For instance, measurements from lunar missions have detected hydroxyl groups and water molecules on the lunar surface, particularly in regions exposed to the solar wind. This suggests that similar processes could be occurring on our planet.

Studies of isotopic compositions of hydrogen in Earth's atmosphere also indicate contributions from solar wind particles. The distinct isotopic signatures of solar hydrogen can be traced and compared with terrestrial sources, providing insights into the relative contributions of solar wind and other sources to Earth's waters.

Understanding the origins of Earth's water and the dynamics of planetary formation has long been a focus of scientific inquiry. A critical part of this investigation involves the study of asteroids, particularly carbonaceous chondrites, which provide essential insights into Earth's water history. These meteorites, rich in water-bearing minerals such as clays and hydrated silicates, and complex organic molecules, formed in the outer regions of the Solar System where water ice and organic compounds remained stable. As these asteroids migrated inward and impacted early Earth, they played a significant role in its development.

The text here is an extract of the ongoing study and very important papers were published in the first preprint version some time ago. There you can find also further information, links, references and sources.