Alcohol molecules found in giant cosmic cloud capable of holding the entire Earth
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Aaj Tak
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Alcohol molecules found in giant cosmic cloud capable of holding the entire Earth

Alcohol lovers on Earth might be interested to know that 'alcohol' also exists in space. A massive gas and dust cloud was discovered near the center of our Milky Way galaxy, containing various alcohol molecules. Scientists identified propanol here, which is considered the largest alcohol molecule found in space to date.

It is important to note that this is not potable alcohol, but a chemical substance. According to researchers, this discovery may help understand the processes of forming complex organic compounds necessary for life in space.

The attention of scientists is focused on a giant molecular cloud called Sagittarius B2, located near the center of the Milky Way. It is approximately 26 thousand light-years from Earth. This region is rich in gas and dust and is a site of active formation of a large number of new stars, hence it is called a stellar nursery.

Various alcohol molecules were found in this cloud, including methanol, ethanol, vinyl alcohol, ethyl formate, and propanol. According to scientists, the amount of methanol and ethanol in Sagittarius B2 is so vast that an estimated 10 trillion liters of these substances are present. However, this does not mean that the alcohol has accumulated in liquid form, like a sea or a pond; these molecules are distributed among the cosmic gas and dust.

The characteristic of the discovered propanol is that it is the largest alcohol molecule ever found. One of its types is isopropanol, which is used in hand antiseptics. Another type is common propanol. Scientists detected the presence of isopropanol in Sagittarius B2 using a radio telescope located in Chile. These discoveries were published in two studies in the scientific journal Astronomy & Astrophysics.

Researchers involved in this project emphasize the exceptional importance of discovering both forms of propanol, as their chemical structures are very similar, and they can exist under similar conditions. By comparing their quantities, scientists can understand exactly how such complex chemical compounds are formed in space.

The main question facing scientists is how such complex organic molecules form in space. To date, about 125 different molecules have been identified in space. Scientists believe that most of them are formed by the collision and combination of small molecules or atoms. However, explaining the presence of such complex substances as vinyl alcohol and propanol solely by this process is difficult.

In 2001, scientists recorded signals of vinyl alcohol in Sagittarius B2 using a 12-meter radio telescope. This was the last of three stable molecules of the C2H4O group discovered in space. At that time, a scientist from the National Radio Astronomy Observatory of the USA, Barry Turner, stated that the discovery of vinyl alcohol was an important key to understanding the process of forming complex organic substances in space.

Another interesting discovery in the Sagittarius B2 cloud is the detection of a chemical substance called ethyl formate. This is the substance that gives raspberries their distinctive taste. Notably, it has a rum aroma. Because of this, scientists once jokingly remarked that the center of our galaxy might taste like raspberry and smell like rum. Nevertheless, this does not mean that real raspberries or rum exist in space; these are simply properties of chemical molecules.

The significance of these discoveries for scientists is not limited to the fact that alcohol-related compounds are in space. In fact, these compounds can help them understand how complex organic molecules necessary for life are formed and distributed in space. This is why they continue to closely observe giant molecular clouds like Sagittarius B2. Scientists hope this will help determine whether there are chemical conditions necessary for life in the universe besides Earth.

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Scientific explanation of gigantism in creatures inhabiting the deep ocean
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super.abril.com.br

Scientific explanation of gigantism in creatures inhabiting the deep ocean

The origin of imagination regarding giant marine creatures dates back to various ancient mythologies. In Mesopotamian mythology, the sea serpent Tiamat was seen as a primary deity linked to chaos and the sea. Hebrew tradition presents the dragon Leviathan as an immense and threatening marine creature, while in Greek mythology, the giant whale Cetus and monsters like Scylla, with their twelve legs and six necks, symbolize aquatic dangers.

The belief in colossal sea beings likely arose from the combination of three elements: the fear of the unknown ocean, contact with little-known real animals, and the human tendency to transform natural forces into monstrous figures. However, these myths have parallels in current reality, as gigantism is an observable characteristic in various species residing in the deep ocean.

Notable examples include the giant squid, capable of exceeding ten meters in total length, and the giant isopod, a crustacean similar to a garden pill bug, which can reach approximately fifty centimeters. This phenomenon is called abyssal gigantism and follows a pattern where deep-water species tend to be significantly larger than their shallow-water relatives. This raises the question: why does this occur?

The Giants of the Seas

In a 2006 study, biologist Craig R. McClain suggested analyzing this phenomenon through the lens of surface islands. Islands generally follow the principle known as the Island Rule (or Foster's Rule), which posits that the body size of animals changes when living in isolated ecosystems, such as islands.

Large animals, such as elephants and hippos, tend to reduce their size over generations (insular dwarfism) due to limited food resources on the island. Conversely, smaller species, such as rodents and insects, tend to increase in size (insular gigantism) because, without the pressure of large predators, they can expand their growth and occupy new ecological niches.

According to McClain, the deep marine environment operates analogously to an island. After a mass extinction event during the Cenozoic, much of the deep-water fauna evolved from species originating in shallow waters. Some of these species decreased in size due to food scarcity, while others became giants.

For those that showed an increase in size, McClain and other researchers propose four possible explanations. It is important to note that there is no single proven cause for abyssal gigantism; the hypotheses raised may act together, justifying different cases. Additionally, inhabiting the abyss does not necessarily imply being gigantic, as the depths host organisms of various sizes, including many tiny species.

Giant Abyssal Animals

Below are some of the most notable examples of this group of creatures.

Ethiopian Renaissance Dam and the Nile: Conflicts between water scarcity and energy
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archdaily.com.br

Ethiopian Renaissance Dam and the Nile: Conflicts between water scarcity and energy

The Grand Ethiopian Renaissance Dam, known by the acronym GERD, is a colossal work of engineering and architecture that, despite connecting, also generates significant divisions. This mega-dam calls into question who holds the right to sovereignty over the river's water and energy resources, challenging the old Nile treaties established during the colonial era.

Inaugurated in September 2025, the GERD is a massive concrete structure located on the Blue Nile, in western Ethiopia, specifically in the Benishangul-Gumuz region. It is situated just 30 kilometers upstream and east of the border with Sudan. Its construction aims to make it one of the largest hydroelectric power sources on the planet, symbolizing Ethiopia's technological autonomy and economic advancement.

Dam Architecture Details

To understand the debate, it is essential to know its structure. The GERD was built under the administration of the civil engineering company Webuild (formerly Salini Impregilo) for the Ethiopian Electric Power. It consists of a main roller-compacted concrete (RCC) dam, an earth-fill arch dam with concrete lining, as well as spillway and hydroelectric power plant systems at the base.

With a designed capacity of 6,000 MW (although recent literature registers 5,150 MW), the dam is 1.8 kilometers long and reaches 175 meters in height. The main dam, only 14 kilometers from Sudan, contains a reservoir called Lake Nigat, with a capacity of 74 billion cubic meters of water, an surface area three times larger than Addis Ababa.

Additionally, there is a 5-kilometer-long and 50-meter-high earth-fill arch dam that serves for passive water containment in a lower area of the basin. The total average annual flow of the reservoir is about 50 billion cubic meters. Two hydroelectric power plants, equipped with 13 Francis turbines on both banks of the river, generate an average annual output of 15,700 GWh.

The spillway system ensures the dam's safety by allowing the safe discharge of floodwaters, keeping the reservoir level within planned limits. These include a main service spillway with gates, a freeboard spillway, and a side emergency spillway without gates, prepared for extreme events.

Internal Webuild laboratories were responsible for testing and developing materials to ensure structural stability and long-term mechanical performance. This was achieved through an advanced mix of RCC, developed internally and internationally, characterized by low cement and water content, and prolonged setting times. A network of galleries in the main dam houses high-sensitivity instruments, such as vertical pendulums, to monitor hydrostatic pressure, structural displacements, joint integrity, and turbine operation in real time. This data is sent to a centralized database at the right bank control center, enabling preventive maintenance and ensuring maximum structural reliability.

The reservoir's storage capacity allows GERD to modify seasonal flow patterns, manage floods, and produce energy. However, being part of an international and transboundary river system, the reservoir filling process raises questions about water needs and storage schedules. Filling cycles have been carried out unilaterally, without transparency between the upstream country and its downstream neighbors, intensifying geopolitical tensions.

GERD operation requires hydrological regulation, as lack of coordination and non-transparent data sharing can harm downstream infrastructure, such as the Roseires Dam in Sudan, due to its proximity to GERD.

Egypt alleges that Ethiopia's unilateral actions could reduce water flow, representing a national threat to its economy and population. The country also points to Ethiopia's 'unilateral exploitation' of transboundary waters in the Omo, Jubba, and Shebelle basins, in addition to the damage caused to its neighbors Somalia and Kenya.

Peaceful resolution of this issue could foster crucial regional cooperation on the White Nile. The disorganized release of water from Ugandan dams, for example, has already caused downstream flooding in South Sudan, resulting in forced displacement of people and disease outbreaks.

Historical Hegemony

In the initial planning of GERD, conducted in the 1960s, Ethiopia lacked internal stability to proceed with the project. The initiative was kept secret until a significant amount of work was completed, as it was known that its development would have a strong geopolitical impact, especially on nations located downstream in the basin.

This weight is amplified when considering that the Nile Basin countries total 11, distributed upstream, downstream, or in both positions. Nations strictly upstream include Burundi, Democratic Republic of Congo, Rwanda, Uganda, Tanzania, Kenya, Eritrea, and Ethiopia. Egypt is the only exclusively downstream country. Sudan and South Sudan occupy mixed positions: South Sudan is upstream relative to Sudan and Egypt, but downstream relative to Uganda, given that the White Nile receives rivers that flow into Lake Victoria.

The Blue Nile, which constitutes 85% of the total volume of the Nile River, originates in Lake Tana, in the Ethiopian Plateau, flows towards Sudan, and finally joins the White Nile in Khartoum to form the main course of the Nile, which passes through Egypt until discharging into the Mediterranean Sea.

Historically, water policy in the Nile Basin was dominated by Egypt's water hegemony, a legal pattern consolidated over a century of colonial-era 'treaties'—the Nile Treaties—in contrast to the search for a multilateral agreement that still conflicts with water use rights.

The Anglo-Ethiopian Treaty of 1902 initially secured Egypt's control over the Nile, prohibiting Ethiopia from altering the course of the Blue Nile without British permission. This supremacy was reinforced by the Anglo-Egyptian Treaty of 1929—which functioned more like an exchange of notes than a formal treaty, giving Egypt veto power over upstream projects or unilateral initiatives—and the subsequent Nile Water Agreement of 1959, which granted Egypt exclusive annual quotas of 55.5 billion cubic meters and Sudan 18.5 billion cubic meters.

However, the reality is more complex: although these unequal colonial-era treaties should be revised or revoked, Egypt remains a country with severe water scarcity, depending on the Nile for over 90% of its freshwater needs, with about 95% of the population living along its banks.

Furthermore, unlike other riparian nations in the basin—except Eritrea (which participates as an observer in the Nile Basin Initiative due to its low water impact) and Sudan (which suffers from infrastructure collapse)—Egypt depends on the Nile as a vital line of survival. Since GERD is on the Blue Nile, responsible for the majority of the river's total volume, the project implies a drastic shift in the regional balance of power, ending the 'monopoly' of water and generating apprehension for the agriculture and water security of downstream countries, especially during prolonged droughts.

To challenge this asymmetric control, the Nile Basin Initiative (NBI) was launched in 1999, followed by the Cooperative Framework Agreement (CFA) in 2010, just one year before the start of the Renaissance Dam works in 2011.

Due to the internal tensions of the Arab Spring, Egypt was unable to effectively oppose or block the project. Its isolation increased when Sudan softened its old objections, adopting a posture of moderate neutrality. Since then, the Sudanese position has frequently varied—between rejection, neutrality, or support—influenced mainly by its own internal political fragmentation. The debate over the pros and cons of the dam has also shaped these shifts in position. On one hand, the dam promises more stable irrigation, reduced dredging costs, and better flood management. On the other, it presents serious long-term risks: impoverishment of alluvial plains due to sediment accumulation in the reservoir, disturbances to local ecosystems, and the persistent lack of cooperation among the three nations.

Political pressure culminated in the Principles Declaration on GERD in 2015, which is the main trilateral milestone between Ethiopia, Sudan, and Egypt. In this document, the three countries recognized the existence of the dam and committed to the principles of international water law. However, to date, they have not reached a binding agreement on the rate of reservoir filling or on managing drought periods.

Disagreements persist on a broader scale. When the Nile Basin Cooperative Framework Agreement (CFA) came into force in October 2024, Egypt and Sudan refused to sign it, seeking to protect access to a vital resource and the veto rights they claim based on colonial treaties.

The Architecture of Geopolitics

Concrete structures can control physical flows of water, but they rarely solve political friction. Ethiopia presents GERD as a shared resource, built for its population and for neighboring countries, committing to exporting excess energy to boost its own economy and support the continent. However, hydrological uncertainty remains the biggest obstacle due to the absence of a clear and definitive agreement for the dam's operation.

A sustainable and equitable transboundary water governance model can be observed in the Senegal River Basin Organization (OMVS), which implements a model of collaborative benefit sharing and co-ownership of infrastructure.

In summary, unlocking the true potential of GERD as a driver of East African economic integration depends on overcoming impasses to ensure the security of downstream neighbors and establishing a new paradigm of equitable water governance, environmental security, and lasting trilateral cooperation. Otherwise, how can a shared river basin reconcile the right of one nation to build its economic future with the right of its neighbors to water security?

Cosmic explosion 2.4 billion light-years from Earth may have affected the planet's atmosphere
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Cosmic explosion 2.4 billion light-years from Earth may have affected the planet's atmosphere

An intense cosmic explosion, known as BOAT (The Brightest of All Time), occurred on October 9, 2022, and reached Earth with a radiation wave capable of altering the ionosphere, one of the atmospheric layers. This phenomenon has attracted the attention of astronomers and continues to spark debate regarding its actual impact on the planet.

This event was identified as GRB 221009A and belongs to the category of Gamma-Ray Bursts (GRBs)—some of the most powerful energy releases in the Universe. They occur when very massive stars collapse, forming a black hole and ejecting jets of particles at speeds close to the speed of light.

Estimates suggest that this event could have been the brightest observed on Earth in approximately the last ten thousand years. According to NASA data, the explosion was so powerful that it temporarily overloaded gamma-ray detectors on various spacecraft.

One example is NASA's Fermi Gamma-ray Space Telescope. Two instruments on the observatory—the Gamma-ray Burst Monitor (GBM) and the Large Area Telescope (LAT)—encountered limitations in registering radiation during the most intense moments of the event.

The INTEGRAL mission, representing the European Space Agency's (ESA) International Laboratory for Gamma-ray Astrophysics, was also affected by BOAT. A study conducted by the Institute of Astrophysics of Andalusia in Spain and published in the journal Astronomy & Astrophysics in 2024 showed that the received radiation was sufficient to saturate the Anti-Coincidence Shield (ACS) and parts of the Imaging Spectrometer (ISGRI) detectors, which degraded data collection during the burst.

To overcome this issue, researchers used data from another INTEGRAL detector—the Microcalorimeter (MCAL)—which was not affected by saturation, to estimate the radiation intensity. Furthermore, they referred to data from the European probe BepiColombo, heading to Mercury, which registered the burst using the Mercury Gamma-ray and Neutron Spectrometer (MGNS). This instrument detected radiation in the energy range of 280 to 460 kilo-electron volts, recording a sequence of pulses lasting about 6.6 minutes.

Scientists combined measurements from two spacecraft to estimate the burst intensity during times when other INTEGRAL detectors were overloaded. This comparison allowed for the reconstruction of part of the signal that could not be measured directly.

Despite the exceptional intensity of the radiation, no signs of permanent physical damage to the spacecraft were found; the problem lay in the temporary overloading of the detectors, which affected some measurements.

The first signal was recorded at 13:16:59 UTC by the Fermi GBM instrument. Other space installations, including the Neil Gehrels Swift Observatory, also detected this radiation. The combination of observations allowed for the study of the phenomenon across different wavelengths and tracking the radiation after the initial flare.

Data indicated that the explosion occurred in a distant galaxy, approximately 2.4 billion light-years from Earth, although this distance may vary depending on the cosmological measurement method used. Even traversing such a vast distance, the radiation reached Earth with enough intensity to cause detectable effects in the atmosphere.

A spectroscopic measurement published in 2025 estimated the light distance at approximately 745 megaparsecs, equivalent to about 2.43 billion light-years. The ionosphere is a region of the atmosphere located between altitudes of 50 and 1000 kilometers. In it, solar radiation and other energy sources knock electrons out of atoms and molecules, forming charged particles. These changes affect the propagation of radio waves and can be detected by scientific instruments.

In November 2025, a study published in Geophysical Research Letters presented evidence that the explosion increased the electron density in the lower ionosphere, at an altitude of 50 to 90 kilometers. Researchers noticed changes in the propagation speed of extremely low frequency radio waves caused by lightning. This disturbance lasted for about 40 minutes.

The team also identified discrepancies between monitoring methods: some measurements showed signals related to radiation passage, while others, such as Schumann resonance observations, did not show obvious changes. The results suggested that the explosion caused a specific reaction in the ionosphere, different from what is usually observed during solar storms.

However, a study placed in the arXiv preprint repository in May of this year revised other changes previously attributed to BOAT. The authors analyzed data from different altitudes and concluded that some anomalies in satellite measurements, electron content, and equatorial electric circulation could be explained by natural conditions and instrumental limitations. The work did not find a consistent increase in total electron content that could be directly linked to the explosion. The authors also identified variations that occurred regularly under certain lighting conditions or began before the event itself. Since the text is still awaiting peer review, its conclusions should be considered in the context of independent scientific evaluation.

According to Marcelo Zurita, president of the Paraiban Astronomy Association (APA), member of the Brazilian Astronomical Society (SAB), technical director of the Brazilian Meteor Observation Network (BRAMON), and columnist for Olhar Digital, it is important to emphasize that this study does not call into question the fact of BOAT or the data recorded by the Institute of Astrophysics of Andalusia's gamma-ray detectors.

The expert explained: 'It disputes the effects of this GRB, and consequently, other gamma-ray bursts on the Earth's ionosphere in the 2025 paper.' He added: 'The ability of these explosions to affect the atmosphere has been discussed in the scientific community for many years. Thus, this study may finally resolve this controversy. If it is proven that the most powerful gamma-ray burst did not cause significant effects in our ionosphere, we can conclude that none of the others will be able to do so.'

This event remains important for astronomy as it helps investigate the interaction of extragalactic explosions with the Earth's environment. The research also highlights the need to use various instruments and independent analyses to separate the effects of cosmic phenomena from natural atmospheric fluctuations.

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