logo
Europe ‘Frankly Insane' To Keep Importing Fossil Fuels, Scientist Says

Europe ‘Frankly Insane' To Keep Importing Fossil Fuels, Scientist Says

Forbes15-04-2025

Soldiers search wrecked cars in Massassana, eastern Spain, in the aftermath of deadly floods in ... More November 2024.
Leading scientists have reacted with exasperation to a major new climate change report showing that Europe experienced its warmest year on record in 2024, confirming its status as the world's fastest-warming continent.
The report, from two leading EU science bodies, reveals unprecedented climate challenges across the continent, with severe weather events, from flooding to wildfires, affecting over 413,000 people and claiming 335 lives.
The European State of the Climate 2024 report, released by the Copernicus Climate Change Service (C3S) and the World Meteorological Organization (WMO), shows that 2024 brought record-breaking temperatures across nearly half of Europe; record-breaking sea surface temperatures, with the Mediterranean Sea 1.2 degrees Celsius above average; and widespread flooding affecting 30% of Europe's river network.
Warning that governments had been complacent about the levels of global warming already seen, which now exceed 1.3 degrees Celsius above pre-industrial levels, Friederike Otto, senior lecturer at the Centre for Environmental Policy and co-lead of World Weather Attribution, Imperial College London, said leaders were "insane" to keep importing fossil fuels such as LNG.
"Think 1.3 degrees of warming is safe? This report lays bare the pain Europe's population is already suffering from extreme weather," Otto told media. "But we're on track to experience 3 degrees Celsius by 2100. You only need to cast your mind back to the floods in Spain, the fires in Portugal, or the summer heatwaves last year to know how devastating this level of warming would be."
Turning to Europe's reliance on imported gas and LNG, Otto went on: "In a volatile global economy, it is frankly insane to keep relying on imported fossil fuels—the main cause of climate change—when renewable energy offers a cheaper and cleaner alternative."
"The EU can't afford to put its climate commitments on the backburner," she added. "It needs to lead the charge and accelerate the shift to evidence-based politics, actually helping low-income people and not oligarchs."
On the shift away from fossil fuels, the Copernicus report found some cause for optimism, noting that the European renewable energy sector had achieved a record 45% of electricity generation from renewable sources in 2024, up from 43% in 2023. Twenty EU countries now generate more electricity from renewables than fossil fuels—nearly double the number from 2019.
European climate adaptation efforts showed promise, too, with 51% of European cities now having dedicated climate adaptation plans, up from 26% in 2018.
But experts warn that renewables are not replacing fossil fuels quickly enough to head off further warming. In January, energy think-tank Ember warned that "an acceleration is needed between now and 2030" if the continent is to achieve its emission-cutting goals.
Responding to the Copernicus report, Sir David King, chair of the Climate Crisis Advisory Group and the U.K.'s former chief science officer, said: "Europe is heating faster than any other continent. This, combined with widespread flooding and record losses of glacial ice, underlines how profoundly Europe is being affected—and why its response to the climate crisis will have global consequences."
King went on to single out the U.S. administration of Donald Trump, which has drastically cut funding and staff from climate and health programs, and has moved to block the development of renewable energy projects.
"As the current U.S. administration fails to even acknowledge the existence of human-caused climate change, Europe must take the reins," King said. "In doing so, countries like the UK, Germany and Norway can set a standard for all progressive countries to match—regardless of US policy. Political bodies and private organizations across Europe must take urgent, decisive action to avoid further catastrophic temperature rises."

Orange background

Try Our AI Features

Explore what Daily8 AI can do for you:

Comments

No comments yet...

Related Articles

The sun: Facts about the bright star at the center of the solar system
The sun: Facts about the bright star at the center of the solar system

Yahoo

time2 days ago

  • Yahoo

The sun: Facts about the bright star at the center of the solar system

When you buy through links on our articles, Future and its syndication partners may earn a commission. Quick facts about the sun How big it is: 865,000 miles (1.392 million kilometers) across How far away it is: 93 million miles (150 million km) What type of star it is: A yellow dwarf star The sun is the star at the center of our solar system. It's the largest, brightest and most massive object in the solar system, and it provides the light and heat that life on Earth depends on. Powered by a process called nuclear fusion, the sun can get hotter than 27 million degrees Fahrenheit (15 million degrees Celsius). The sun has been around for over 4 billion years, but one day, it will run out of fuel. Read on to learn more about what our local star is made of, how it formed and what will happen when it dies. Over 1 million Earths could fit inside the sun. The sun may look yellow from Earth, but it actually releases every color of light, meaning its true color is white. The sun is unique in that it's the only star in our solar system. Up to 85% of stars have at least one companion star. The sun contains over 99% of the mass of our entire solar system. Like Earth, the sun also rotates on its axis. Each rotation takes about 27 Earth days. The sun is a ball of gas and plasma made mostly of hydrogen. The sun uses these vast stores of hydrogen to generate the heat and light that sustain our planet. It does this through a process called nuclear fusion, in which two hydrogen atoms combine to create a different element, helium. The sun is about three-quarters hydrogen and one-quarter helium, with tiny amounts of metals. The larger a star is, the more rapidly it burns through its hydrogen. Some of the largest known stars — such as those with masses 40 times that of the sun — will live just 1 million years. By contrast, the sun will have a lifetime of around 10 billion years. Different parts of the sun reach different temperatures. The sun's core gets as hot as 27 million F (15 million C). The part of the sun we can see from Earth is called the photosphere, which is the "surface" of the huge ball of plasma. The temperature of the photosphere is about 9,900 F (5,500 C). Above the photosphere is the loose outer atmosphere of the sun, known as the corona. We can't see the corona from Earth under ordinary conditions, though it can be photographed during a total solar eclipse. The sun formed around 4.5 billion years ago. At that time, the area of the Milky Way galaxy that would become the solar system was a dense cloud of gas — the leftovers of an earlier generation of stars. The densest region of this cloud collapsed and created a seed, called a protostar, that would become the sun. As this young protostar grew, planets, moons and asteroids formed from the remaining raw material, and then began circling around the growing sun as they were sucked into orbit by the star's powerful gravity. At the heart of the sun, this same force sparked nuclear fusion. The heat and light from this nuclear reaction allowed life on Earth to evolve and prosper. However, this reaction will eventually lead to the sun's death when it runs out of nuclear fuel. The sun is around halfway through its lifetime. Our star is locked in a constant battle as outward pressure from nuclear fusion fights the inward pull of gravity. When the sun runs out of hydrogen in about 5 billion years, the inward force of gravity will win. The center of the sun will collapse, compressing into a dense core. Helium will start fusing into even denser elements, like carbon, nitrogen and oxygen. While this happens, the heat generated by the fusing of these elements will push the sun's outer shell to swell. This will be bad news for the inner planets of the solar system — including Earth. As the sun becomes a type of star called a red giant, its outer shell will expand to the orbit of Mars, gobbling up Mercury, Venus, Earth and Mars. But the red-giant phase is not when the sun will die. The outer layers that swell during the red-giant phase will become a shell of gas called a surrounding planetary nebula. This shell will be shed after approximately 1 billion years. This will expose the star's smoldering core, which, by this point, will be a dense ball called a white dwarf. As a white dwarf, the sun will dim. The material from the planetary nebula will spread out into the galaxy and form the building blocks of the next generation of stars and planets. Image 1 of 5 Space agencies have launched many spacecraft that help us observe and gather data about the sun. Pictured here is an artist's concept of the sun being observed by NASA's Parker Solar Probe. Image 2 of 5 The red giant star Camelopardalis. The sun will eventually become a red giant, and as it expands, it will engulf its nearest planets, including Earth. Image 3 of 5 Sunspots are darker, cooler areas that temporarily appear on the sun. They're caused by changes in the sun's magnetic field. Image 4 of 5 Solar storms happen when the sun releases flares of energy and particles. Image 5 of 5 Auroras on Earth happen when charged particles from the sun interact with our planet's atmosphere. Is Earth getting closer to the sun, or farther away? Where on Earth does the sun rise first? What color is the sun?

European Mars orbiter spies crumbling crater 'soaked in layers of Martian history' (photo)
European Mars orbiter spies crumbling crater 'soaked in layers of Martian history' (photo)

Yahoo

time2 days ago

  • Yahoo

European Mars orbiter spies crumbling crater 'soaked in layers of Martian history' (photo)

When you buy through links on our articles, Future and its syndication partners may earn a commission. A European Mars probe captured a stunning view of a Martian crater that's rich in many of the features that help scientists reconstruct the planet's dynamic history over billions of years. The image, taken in October 2024 using the High Resolution Stereo Camera (HRSC) on the European Space Agency's (ESA) Mars Express orbiter, shows a crumbling crater called Deuteronilus Cavus. It is "soaked in layers of Martian history," having been exposed to volcanic lava flows, erosion from liquid water, repeated freeze-thaw cycles that expanded its edges, and layers of wind-blown volcanic dust settling over time, according to a statement from the space agency. Located in a transitional zone between the planet's rugged southern highlands and smoother northern lowlands, Deuteronilus Cavus is believed to originally have formed following an impact roughly 4.1 to 3.7 billion years ago, when Mars and other planets were being bombarded by huge numbers of asteroids and comets. Over time, the nearly circular 75-mile-wide (120 kilometers) depression has been eroded by water and ice, enlarging it to nearly twice its initial size. ESA shared a fun "recipe" outlining the series of events that shaped the crater, offering valuable insights into the planet's climatic and geological evolution. For example, the presence of clay minerals indicates past interactions between volcanic materials and water, hinting at the possibility of ancient habitable environments, according to the statement. This is further supported by channels cut through the crater's rim, likely formed by surface water flow or the collapse of weakened ground above draining subsurface water. Meanwhile, grooves in the crater rim suggest that ice once formed when Mars' axis tilted more sharply away from the sun than it does now. Related Stories: — Mars: Everything you need to know about the Red Planet — Facts about ESA's Mars Express orbiter — What happened to all the water on Mars? Here's why the debate continues "The linear grooves indicate where boulders frozen into the base of a glacier were dragged along, gouging out the troughs visible today," ESA officials said in the statement. "Around the base of the crater's inner walls, we can see the smooth, tongue-shaped ends of rock-covered glaciers. These 'debris aprons' formed when ice mixed together with rocky debris along the crater walls during a period of glaciation, and slowly crept downslope." The crater's interior also exhibits a mix of rock knobs, mesas, channels and plains, believed to be remnants of a collapsed central peak. Dark volcanic ash covers much of the crater floor, while surrounding wrinkle ridges mark ancient lava flows. "This feature-rich crater has all the ingredients for exploring Mars' varied geological processes, giving us a tantalizing taste of its complex history," ESA officials said in the statement.

UH: Urgent response required to save world's coral reefs
UH: Urgent response required to save world's coral reefs

Yahoo

time2 days ago

  • Yahoo

UH: Urgent response required to save world's coral reefs

HONOLULU (KHON2) — A study by researchers at University of Hawaiʻi at Mānoa's Hawaiʻi Institute of Marine Biology found that coral reefs are less frequent in the tropics due to warming oceans. The research found that the reefs are unable to beat the heat and effects of climate change, which rings the emergency alarm for conservationists. 8 takeaways from Hawaiʻi's top ranking for school lunches However, there is still hope, as the research showed that immediate actions to reduce greenhouse gas emissions can improve the future of these iconic ocean scenes across the planet. 'As the ocean warms, species tend to move poleward,' said lead author Noam Vogt-Vincent, lead author of the study. 'We know from the fossil record that coral reefs have previously expanded their ranges in response to past climate change, but we didn't know whether this was a matter of decades or millennia.' In order to predict changes in the distribution of these reefs, the research team used complex simulation models running on UH's high-performance computing cluster. The team created a global model including approximately 50,000 coral reef sites to the model, the researches tested three future emissions scenarios: one with low warming, around two degrees Celsius, a moderate warming scenario, around three degrees Celsius and a high warming model, which is greater than four degrees Celsius. 'By modeling coral reefs globally and incorporating evolution and connectivity, this study provides an unprecedented long-term view of how these complex ecosystems will respond to climate change,' said research professor Lisa McManus. Provided the current condition of the climate on coral reefs, the researchers found both good news and bad news. Download the free KHON2 app for iOS or Android to stay informed on the latest news 'Unfortunately, while we've confirmed that coral reef range expansion will indeed eventually occur, the biggest coral losses are expected in the next 60 years, meaning these new, higher-latitude reefs won't form fast enough to save most tropical coral species,' Vogt-Vincent said. While northern Florida, southern Australia and southern Japan may see new reefs in the future, they will not be in existence soon enough to help corals survive through the century, UH said. While the future seems bleak, there is still hope, with significant cuts in emissions, such as those outlined in the Paris Climate Agreement, could dramatically reduce the loss of coral. Aliʻi Drive to revert to a two-way street Currently, coral reduction is on track to lose up to 86% of coral reefs; but with lower emissions, losses could be reduced to only around 33% of coral reefs. 'Our study suggests that reductions in greenhouse gas emissions will not just improve coral reef futures this century, but for hundreds to thousands of years into the future,' Vogt-Vincent said. 'Our actions over the next few decades will therefore have incredibly long-lasting consequences for coral reefs globally.' Researchers will continue to monitor reef levels with their supercomputer power to try to better understand both threats and solutions surrounding the world's coral reefs. For more information, visit the Hawaiʻi Institute of Marine Biology's website. Copyright 2025 Nexstar Media, Inc. All rights reserved. This material may not be published, broadcast, rewritten, or redistributed.

DOWNLOAD THE APP

Get Started Now: Download the App

Ready to dive into the world of global news and events? Download our app today from your preferred app store and start exploring.
app-storeplay-store