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Approximately 60 miles
The Earth's atmosphere is approximately 60 miles (about 86 kilometers) thick from the surface to the edge of space. It consists of several layers, with the troposphere being the most active layer, where weather occurs, and the stratosphere above it, where ozone is abundant.
Wiki

Vertical mixing occurs when different layers of the ocean mix due to temperature and density differences. Wind-driven waves and storms can break down the thermocline (the barrier between warm surface waters and cold deep waters), allowing nutrient-rich deep water to mix with nutrient-depleted surface waters. This process is particularly active in temperate regions during winter months when surface waters cool and sink.

Upwelling, a more dramatic process, happens when deep, nutrient-rich water rises to replace surface water pushed away by winds or currents. The most productive marine ecosystems are found in upwelling zones, such as off the west coasts of continents. For example, the Peruvian Coast experiences intense upwelling, supporting one of the world’s largest fisheries.

May 20, 2024
AI Training vs. Inferencing: A Comparison of the Data Center Infrastructure Each Requires
In the past few years, AI has seized the spotlight, leading groundbreaking research and catalyzing transformative progress across many industries. As organizations at all scales continue to tackle complex challenges and unlock new possibilities, the ability to meet distinct infrastructural requirements for various AI workloads becomes increasingly crucial.

AI training and inferencing are two such workloads, each with distinct functions and requirements. While both play crucial roles and often function hand in hand, they entail different computational demands and necessitate varying infrastructural setups within the data center.

Here is a Swedish associated device, I believe: https://medium.com/@curiosityai/corpowe … 06e296bc33
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So, you have an energy source and a thermal radiator sink.  While this will redistribute the heat that ultimately comes from the waves, the heat was going to show up somewhere on the planet anyway.

Radiotrophic fungus

Radiosynthesis (metabolism)

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From Wikipedia, the free encyclopedia
Radiosynthesis is the theorized capture and metabolism, by living organisms, of energy from ionizing radiation, analogously to photosynthesis. Metabolism of ionizing radiation was theorized as early as 1956 by the Russian microbiologist S. I. Kuznetsov.[1]

Beginning in the 1990s, researchers at the Chernobyl Nuclear Power Plant uncovered some 200 species of apparently radiotrophic fungi containing the pigment melanin on the walls of the reactor room and in the surrounding soil.[2][3][4] Such "melanized" fungi have also been discovered in nutrient-poor, high-altitude areas which are exposed to high levels of ultraviolet radiation.[5]

Following the Ukrainian results, an American team at the Albert Einstein College of Medicine of Yeshiva University in New York began experimenting with radiation exposure of melanin and melanized fungi. They found that ionizing radiation increased the ability of melanin to support an important metabolic reaction, and that Cryptococcus neoformans fungi grew three times faster than normal.[6][5] Microbiologist Ekaterina Dadachova suggested such fungi could serve as a food supply and source of radiation protection for interplanetary astronauts, who would be exposed to cosmic rays.[5][4]

In 2014, the American research group was awarded a patent for a method of enhancing the growth of microorganisms through increasing melanin content. The inventors of this process claimed their fungi were employing radiosynthesis, and hypothesized that radiosynthesis may have played a role in early life on Earth, by allowing melanized fungi to act as autotrophs.[7]

From October 2018 through March 2019, NASA conducted an experiment aboard the International Space Station to study radiotrophic fungi as a potential radiation barrier to the harmful radiation in space. Radiotrophic fungi have many possible applications on Earth as well, potentially including a disposal method for nuclear waste or use as high-altitude biofuel or a nutrition source.[8]

Mars receives about 43–44% of the sunlight that Earth does, due to its greater distance from the Sun and thin, dusty atmosphere.
Solar Irradiance
The average solar irradiance on Mars is approximately 590 W/m², compared to about 1,367 W/m² at the top of Earth's atmosphere and roughly 1,000 W/m² at Earth's surface under clear conditions. This means Mars gets less than half the sunlight Earth receives, primarily because it orbits at an average distance of 1.5 astronomical units (AU) from the Sun, compared to Earth’s 1 AU. The inverse square law explains this reduction: sunlight intensity decreases with the square of the distance from the Sun.

Ukraine Just Did Something That Will UNBLOCK the Strait of Hormuz… Iran Can’t Stop It!
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Radiotrophic fungus

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Lightning has been confirmed on Mars, primarily occurring as small electrical discharges in dust storms and dust devils.
Evidence of Martian Lightning
NASA’s MAVEN spacecraft detected a whistler wave, a low-frequency electromagnetic signal typically caused by lightning, in Mars’ ionosphere. This event was recorded over a localized crustal magnetic field at an altitude of 349 kilometers on the night side of the planet, lasting 0.4 seconds and spanning up to 110 Hz, representing the first direct evidence of lightning-like activity on Mars (NASA, 2026). MAVEN’s detection was extremely rare, with only one event found among over 108,000 measurements, highlighting the elusive nature of Martian lightning.
Phys.org
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Mechanism of Lightning Formation
Unlike Earth, Mars lacks a global magnetic field and has a thin, dry carbon dioxide atmosphere. Lightning on Mars does not form in rain clouds but is generated by triboelectric charging during dust storms and dust devils. As dust grains collide and rub together, they accumulate electrical charge, which can discharge as small sparks or “mini-lightning” (Nature, 2025; EarthSky, 2025). Laboratory experiments and simulations confirm that these conditions can produce electrical discharges similar to those observed in terrestrial volcanic eruptions or dust devils.
CBS News
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Observations from the Surface
The Perseverance rover recorded 55 instances of electrical discharges over two Martian years, with seven events capturing full acoustic signatures, including tiny sonic booms akin to miniature thunderclaps. These discharges were typically very small, ranging from 0.1 to 150 nanojoules, with one larger event at 40 millijoules, far weaker than typical Earth lightning (ScienceAlert, 2025; CBS News, 2025). The events occurred mostly during the strongest winds at the leading edges of dust storms or within dust devils, confirming that both dust and wind are necessary for lightning formation.
ScienceAlert
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Implications
Martian lightning is much weaker and more localized than Earth’s, posing minimal risk to future human explorers but potentially affecting sensitive equipment. The discovery also provides insights into atmospheric chemistry, as electrical discharges can drive reactions that form oxidizing compounds like perchlorates, which are common on Mars (Nature, 2025). Understanding these discharges helps scientists model Mars’ atmosphere and plan future missions, including ESA’s proposed M-MATISSE mission.
Nature
Summary
Lightning on Mars exists but is rare, weak, and mostly near the surface.
It occurs primarily in dust storms and dust devils through triboelectric charging.
MAVEN detected a whistler wave from orbit, while Perseverance recorded miniature lightning and sonic signatures on the surface.
These findings enhance our understanding of Martian atmospheric dynamics and have implications for future exploration and planetary chemistry.
This discovery confirms that Mars, despite its thin atmosphere and lack of a global magnetic field, can generate electrical discharges similar to lightning, albeit on a much smaller scale than on Earth.

Electric bacteria
Life that lives on electricity
Electric bacteria are a unique example of life forms that thrive on electricity. These bacteria, such as Shewanella and Geobacter, can survive on pure energy, consuming electrons from rocks and metals. They are not dependent on sugars or other nutrients, making them a fascinating subject of study in the field of microbiology. The discovery of electric bacteria shows that some basic forms of life can handle energy in its purest form, which is a significant advancement in our understanding of life's energy requirements.
New Scientist
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Life
Meet the electric life forms that live on pure energy
Unlike any other life on Earth, these extraordinary bacteria use energy in its purest form – they eat and breathe electrons – and they are everywhere

By Catherine Brahic

16 July 2014

Antarctic microbes have been discovered that can eat air, specifically using atmospheric gases like hydrogen, carbon dioxide, and carbon monoxide. These bacteria, known for their ability to perform atmospheric chemosynthesis, thrive in low-nutrient environments, such as polar deserts, where they convert atmospheric gases into organic compounds for growth. This process allows them to survive in extreme conditions where traditional food sources are scarce, potentially playing a significant role in the ecosystem by contributing to carbon cycling.

Biology
Bacteria that "eat" only air found in cold deserts around the world
By Michael Irving
August 19, 2020 05:53 pm

Strange Bacteria That Survive Only on Air May Be More Prevalent Than We Realised
Nature
20 August 2020
ByTessa Koumoundouros

Melania Trump walks side by side with humanoid robot at White House summit
Melania Trump pitched a vision of the future in which robots serve as educators who teach students about philosophy and art.

Large solar panel arrays can create localized conditions that promote rainfall by altering temperature, airflow, and moisture patterns.
Mechanism of Rain Formation from Solar Panels
Solar panels affect the local microclimate primarily through temperature and airflow changes. Dark photovoltaic panels absorb sunlight, converting 10–20% into electricity while the rest contributes to heat. This creates thermal gradients, where the air above the panels warms slightly while the ground beneath remains cooler due to shading. The rising warm air generates updrafts and convection currents, which can lift moisture into the atmosphere and enhance cloud formation.
biologyinsights.com
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The panels also increase surface roughness, slowing near-ground winds and promoting vertical mixing of air. This combination of rising warm air and altered wind patterns can lead to greater atmospheric instability, which is a key factor in precipitation formation.
biologyinsights.com
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Positive Feedback in Desert Environments
In arid regions like the Sahara, large solar farms have been observed to trigger rainfall and vegetation growth. The process works as a positive feedback loop: solar panels lower ground temperatures, warm air rises, clouds form, and rainfall increases. This rainfall supports plant growth, which further enhances local moisture levels, potentially leading to a gradual “greening” of desert areas.
EcoPortal.net
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Scale and Limitations
While these effects are noticeable in massive solar farms, the current scientific consensus indicates that typical solar installations are too small to significantly alter regional weather or precipitation patterns. Most observed impacts are localized, affecting the thermal boundary layer and dew point rather than causing widespread rainfall changes. Simulations suggest that only solar arrays covering extremely large areas, such as a significant portion of the Sahara, could meaningfully influence rainfall and global climate patterns.
biologyinsights.com
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Summary
Solar panels can indirectly cause rain by:
Creating thermal updrafts that lift air and moisture.
Modifying local wind and airflow through surface roughness.
Shading the ground, which reduces evaporation and enhances convection.
Supporting a positive feedback loop in deserts, where rainfall encourages vegetation growth, further increasing moisture.
These effects are most pronounced in large-scale solar farms in arid regions, while smaller installations mainly influence microclimates rather than regional weather.
3

New cooling gel could raise PV module efficiency by 12%
Researchers in Saudi Arabia have developed a hydrogel composite that absorbs moisture in solar modules overnight and facilitates evaporative cooling throughout daylight hours. The system has undergone lab tests and outdoor experiments on two continents.

June 9, 2025 Lior Kahana

Solar panels are creating an unexpected effect by forming rainfall clouds and thriving oases in the middle of the desert
Warren van der Sandt by Warren van der Sandt  April 11, 2026 in Energy

Researchers and farmers working together to understand permafrost-agriculture interactions.

Farming on permafrost soil presents unique challenges and opportunities. The Permafrost Grown Project is a significant initiative that aims to understand the interactions between permafrost and agriculture in Alaska. The project focuses on developing sustainable, adaptable, and resilient permafrost-agroecosystems by co-producing knowledge with farmers and researchers. It employs a combination of field data collection, sensor networks, remote sensing techniques, agricultural experiments, existing agriculture experience, interviews, and socio-economic risk modeling to address various objectives related to permafrost and agriculture. The project is funded by the US National Science Foundation's Navigating the New Arctic Initiative and has a budget of 3 million USD over 5 years.
permafrostgrown.org

The project's research team includes experts from the University of Alaska Fairbanks and Alaskan farmers, who collaborate to investigate the impacts of permafrost on agricultural infrastructure and cultivation activities. They aim to understand how permafrost affects soils used for agriculture and how agriculture affects permafrost. The team conducts ground penetrating radar (GPR) surveys and collects ground cores to assess permafrost conditions. The project's findings can benefit from the ~120-year legacy of farming on permafrost in Alaska and the predicted intensification of high-latitude agriculture in response to climate changes.
Futurum Careers

Transient lunar phenomena
Outgassing events on the Moon are associated with transient lunar phenomena (TLPs), which are short-lived changes in light, color, or appearance on the lunar surface. These phenomena can include brightenings, dimmings, and color changes, often described as "mists," "clouds," or "volcanoes." The physical mechanism responsible for creating TLPs is not fully understood, but theories suggest they are the outcome of lunar outgassing, where gases are released from the surface of the Moon. This outgassing can be influenced by seismic activities, such as moonquakes, which may release gases that reflect sunlight and cause luminous phenomena.

This map, based on a survey of 300 TLPs by Barbara M. Middlehurst and Patrick Moore, shows the approximate distribution of observed events. Red-hued events are in red; the remainder are in yellow.

Science
Japan Plans to Create a Solar Ring Around the Moon to Power Earth for Eternity
Shimizu Corporation’s Luna Ring concept could transform global energy by harnessing the Moon’s solar power and beaming it back to Earth.

Published on February 8, 2026 at 08:45
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Lydia Amazouz
Written by Lydia Amazouz
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Reading time : 4 minutes

Article
Open access
Published: 05 April 2019
An extremely heavy chlorine reservoir in the Moon: Insights from the apatite in lunar meteorites

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Apatite, a phosphate mineral, has been found in lunar rocks and meteorites, revealing the Moon’s complex volatile history, including water and chlorine content.
Presence and Composition
Apatite on the Moon is primarily fluorapatite (Ca5(PO4)3F), though hydroxylapatite and chlorapatite have also been identified in some samples. It occurs in nearly all lunar rock types, including basalts and breccias, but is generally a trace mineral, ranging in size from sub-micron to 2 mm. Apatite serves as a key reservoir for phosphorus and rare earth elements on the Moon and is the most common volatile-bearing mineral in lunar rocks.
NASA
Insights into Lunar Volatiles
The discovery of apatite in lunar meteorites has provided evidence that the Moon’s early crust, over 4 billion years ago, was more water-rich than previously thought. Apatite contains hydrogen, fluorine, and chlorine, which allows scientists to study the volatile content and isotopic composition of lunar materials. Analyses show water contents ranging from 220 to 5200 ppm, with δD values from −100 to +550‰ and δ37Cl values from +3.8 to +81.1‰, indicating a heterogeneous distribution of volatiles and complex lunar formation processes.
Science Times
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Isotopic Significance
Lunar apatite exhibits a wide range of chlorine isotopic ratios (δ37Cl), much broader than terrestrial or chondritic values, suggesting the Moon contains an extremely heavy chlorine reservoir. This isotopic fractionation may result from volatile loss during the Moon-forming Giant Impact and subsequent differentiation of the lunar magma ocean, with late accretion of hydrous components contributing to the observed variability.
Nature
Debates on Water Content
While apatite has been used to infer water content in lunar rocks, some studies suggest it may overestimate water levels. Computer models indicate that hydrogen-rich apatite could form during crystallization from magma even in relatively dry conditions, meaning the high hydrogen content may not directly reflect a water-rich lunar environment. Nonetheless, the presence of water-bearing apatite in meteorites like AP 007 confirms that the Moon’s crust contained significant volatiles in its early history.
UCLA
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Scientific Importance
Studying apatite on the Moon helps scientists understand:
The volatile history of the Moon, including water, chlorine, and other elements.
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The formation and differentiation of the lunar crust and magma ocean.
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The distribution of phosphorus and rare earth elements, which are critical for understanding lunar geochemistry.
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In summary, lunar apatite is a crucial mineral for reconstructing the Moon’s early volatile inventory, providing insights into water content, chlorine isotopes, and the processes that shaped the Moon’s crust over 4 billion years ago.

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Carbon exists on the Moon in trace amounts, primarily in polar ices, regolith, and recently discovered graphene layers, but it is far less abundant than on Mars or Earth.
Forms and Sources of Lunar Carbon
Carbon on the Moon is present in several forms. Polar regions may contain subsurface carbon-bearing ices, which could provide a source of carbon, hydrogen, and oxygen for propellant production, though these deposits are limited and could be quickly exhausted on longer timescales. Lunar regolith and pyroclastic glasses also contain carbon, but at very low concentrations, making them less viable for large-scale resource extraction. Additionally, recent analysis of Chang’e-5 samples revealed thin layers of natural graphene in lunar dust, marking the first confirmation of few-layer graphene on the Moon.
arXiv.org
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Trace gases in the lunar exosphere, including carbon dioxide (CO₂) and methane (CH₄), exist in extremely low concentrations and are unlikely to be useful for in-situ resource utilization. These gases may originate from solar wind interactions, cometary deposits, or outgassing from the Moon’s interior.
Wikipedia
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Potential Uses
Carbon is essential for supporting a sustained human presence on the Moon. It can be used to produce methalox propellant (methane and oxygen) for spacecraft refueling. NASA experiments have demonstrated that carbothermal reduction of lunar regolith can produce carbon monoxide, which can serve as a precursor for oxygen and fuel production, using solar energy to drive the reaction. The discovery of graphene also opens possibilities for advanced materials and electronics in lunar habitats.
arXiv.org
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Challenges
The Moon is extremely poor in carbon compared to Mars, and most accessible sources are concentrated in a few polar regions. Extraction would require careful site selection, energy input, and infrastructure to harvest and process the carbon efficiently. Bulk regolith and pyroclastic glasses are not practical sources due to low carbon content.
arXiv.org
Summary
While carbon is present on the Moon, it is scarce and unevenly distributed. Polar ices, regolith, and graphene layers represent the main sources, with polar ices being the most promising for near-term propellant production. Advances in extraction technologies, such as solar-driven carbothermal reduction, could enable sustainable lunar operations, but large-scale utilization will be limited by the Moon’s low carbon abundance.

Carbon in the Moon
The presence of carbon in the Moon has been a topic of interest due to the detection of water and other volatile elements in lunar volcanic glasses. These glasses, formed from fire-fountain eruptions, contain hydrogen, fluorine, sulphur, and chlorine, indicating an origin from source magmas with similar volatile concentrations as parts of Earth’s upper mantle. This discovery challenges the long-held assumption of a volatile-free Moon and suggests that the Earth and Moon may share a common volatile source. The carbon content in these glasses is detectable, with similar abundances to those found in Earth’s mid-ocean ridge basalts, further supporting the idea of a Moon that contains at least some volatiles.
Wikipedia