Climate Change is Impacting the Deepest Reaches of the Arctic Ocean

Deep Waters of the Arctic Ocean Are Warming

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Warm waters from the Atlantic near Greenland are now heating the deep layers of the Arctic Ocean, an area once considered relatively insulated from climate change.

The Arctic Ocean has seen a reduction of about 40% in its sea ice cover over the past 40 years, primarily due to the impact of atmospheric warming on sea levels. Researchers at the Ocean University of China evaluated the latest data collected by icebreakers to assess the temperature increase of the ocean floor.

In the Eurasian Basin, which is one of the ocean’s two principal sections, temperatures at depths ranging from 1500 meters to 2600 meters have increased by 0.074 degrees Celsius since 1990.

While this temperature rise may seem minor, it equates to nearly 500 trillion megajoules of energy. Such energy could potentially melt up to one-third of the least extensive sea ice area.

“The deep ocean is more dynamic than previously assumed,” states Chen Xianyao, one of the research team members. “We suspected that the deep ocean was warming, but not at this pace.”


An underwater ridge separating Greenland and Siberia divides the Arctic Ocean into two basins. The Amerasian Basin is primarily cut off from the Pacific Ocean by the shallow Bering Strait. However, warm Atlantic waters can still flow north along the Scandinavian coast into the upper Eurasian Basin through an extension of the Atlantic Meridional Overturning Circulation (AMOC). During winter, when seawater freezes, the salts are released, resulting in denser water that sinks and drags some warmer Atlantic water down with it.

Geothermal heat from the Earth warms the deep waters of the Eurasian Basin.

Previously, these warming trends were balanced by cold water flowing down from a neighboring basin east of Greenland. Yet, as the Greenland ice sheet continues to melt, more freshwater is entering the Greenland Basin. This influx has slowed the downward movement of cold, salty water, raising the temperature of deep waters in the Greenland Basin from -1.1°C to -0.7°C—a significantly rapid increase. Consequently, the influx of cold Greenland waters is no longer counteracting the heat from geothermal sources or the warm Atlantic waters sinking into the Arctic.

“The rising temperatures in the Greenland Basin are now reaching the Arctic,” says Son Louise, another research team member.

This research uncovers new warming mechanisms deep within the Arctic Ocean, “indicating a broader trend of global warming,” according to James McWilliams from UCLA.

The ongoing warming might eventually contribute to the melting of both sea ice and permafrost found on the ocean floor, which contains ice-like structures known as clathrates. If disturbed, these can release methane into the atmosphere, a phenomenon believed to have contributed to the Permian mass extinction.

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Source: www.newscientist.com

The Tarantula Nebula is captured in the deepest X-ray images ever by Chandra

The Tarantula Nebula is the most important star-forming complex in local galaxy groups, including the Milky Way, the large Magellan cloud and the Andromeda galaxy. At its heart is the highly rich young star cluster R136, which contains the most huge known stars. The stellar wind and supernova carved the tarantula nebula into an astonishing display of arcs, pillars and bubbles.



This image of Chandra shows the Tarantula Nebula. Image credits: NASA/CXC/Penn State/Townsley et al.

The Tarantula Nebula is approximately 170,000 light years away from the southern constellation of Dorado.

The nebula, also known as the NGC 2070 or 30 Dorados, is part of the large Magellan cloud.

“The Tarantula Nebula is the most powerful and large star-forming region in the local galaxy group,” says Matthew Povich, astronomers at Polytechnic University in California, and Pennsylvania State University astronomers Raysa Townsley and Patrick Brose. I said that.

“The nebulae differ from the massive star-forming regions of the Milky Way galaxy. There is no different galactic rotation to tear the complex, so it provides fuel for at least 25 million years to supply large star-forming. It lasts and grows at the confluence of two super-huge shells, reaching a starburst percentage.”

“Today, it is dominated by a central large cluster R136, 1-2 million years ago, and includes the wealthiest young star population of the local group, and the largest star included It's here.”

“In contrast to the large star-forming regions of the galaxy, the location of the large Magellan tarantula nebula provides a low metallic starburst laboratory with low absorption and well-known distances. I'll do that.”

https://www.youtube.com/watch?v=ivd_gmu9p8c

New X-ray images of the tarantula nebula contain data from the large Chandra program, including observation times of approximately 23 days, with Chandra previously performed in the nebula for over 1.3 days.

The 3,615 x-ray sources detected by Chandra include large stars, double star systems, bright stars still in the process of formation, and much smaller clusters of young stars.

The authors also identified the oldest X-ray pulsar candidate ever detected in Tarantula Nebula, PSR J0538-6902.

“There are a ton of diffuse hot gases found in x-rays that come from various sources that arise from the giant star winds and gases expelled by supernova explosions,” the astronomer said.

“This dataset is ideal for the near future to study diffuse X-ray emissions in star-forming regions.”

Team's paper It will be published in Astrophysical Journal Supplement Series.

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Raysa K. Townsley et al. 2025. TARANTULA – Revealed by X-ray (T-REX). APJin press; Arxiv: 2403.16944

Source: www.sci.news