A new climate study was just being released that had the potential to brush out the global warming we’re experiencing like so many eraser crumbs on notebook paper, revealing what might be our future if the ambient warming wasn’t part of the equation: much more extreme regional happenings. The model also forecasts Arctic Ocean warming as high as 5°C and intense rainfall strengthening over areas such as the Himalayas, Andes, and eastern Asia. This jump in detail, made possible by high-powered simulations, provides sharper tools to adapt to local climates, plan energy needs, and prepare for disasters — especially in places like small island nations and mountain communities that are already feeling the effects of climate change and rely on cell towers more than landlines.

Supercomputing Climate Model Unveils Regional Extremes Under 1°C Global Warming

As per a report published in Earth System Dynamics, the breakthrough was made by researchers from the IBS Centre for Climate Physics in South Korea and the Alfred Wegener Institute in Germany. They employed the AWI-CM3 Earth system model, running it on South Korea’s top supercomputers to simulate climate conditions at 9 km atmospheric and 4–25 km ocean resolution—far finer than the ~100 km resolution models commonly used by the IPCC.

The weather forecast now takes into account region-specific patterns never studied before: local conditions on islands, types of oceanfront rain, and the way turbulence forms in ocean eddies. Warming is expected to intensify at a rate 45%–60% higher than the global mean in high mountain ranges, including the Hindu Kush and Andes. In Siberian and Canadian Arctic regions, temperatures may rise by about 2°C under a 1°C global average increase.

The researchers also predict increased climate fluctuations. El Niño, La Niña, and the Madden Julian Oscillation (MJO) will increase, and the state of both phenomena will be on a faster track with larger frequency and impact, which will cause a great number of days with heavy rain (rainfall > 50 mm/day). That motion could trigger floods and landslides in heavily populated and environmentally delicate areas.

And for that insight to be actionable, the lab has created an interactive tool that is basically maps of climate projections in the form of data overlaid on Google Earth. These datasets are vital for policymakers who build solar & wind infrastructure & develop disaster response & water management plans in varied geographies.

Astronomers call ancient star clusters like NGC 1786 “time capsules” for their galaxy, preserving some of its oldest stars. A new image from NASA’s Hubble Space Telescope offers an unprecedented close-up of this dense cluster 160,000 light-years away in the Large Magellanic Cloud. Hubble’s data show that NGC 1786 contains stars of different ages – a surprising find, since such clusters were once thought to hold a single stellar generation. This multi-age discovery is reshaping our view of how galaxies built their first stars, and suggests more complex early history.

Mixed-Age Stars in a Galactic Time Capsule

According to the official source, this Hubble image shows the globular cluster NGC 1786, a ball of densely packed stars in the Large Magellanic Cloud about 160,000 light-years from Earth. Astronomers captured this picture as part of a program comparing ancient clusters in nearby dwarf galaxies (like the LMC) with clusters in our own Milky Way. The surprising discovery is that NGC 1786 hosts stars of multiple ages. In fact, astronomers expected all stars in such a cluster to form at the same time, so finding multiple stellar generations was unexpected. This suggests even ancient clusters in other galaxies have more complex, layered histories than scientists expected.

Clues to Galaxy Evolution

For astronomers, the discovery provides clues to galaxy formation. Each globular cluster is like a snapshot of its galaxy’s past, so finding multiple stellar generations implies the Large Magellanic Cloud built its stars in stages rather than all at once. By comparing NGC 1786 to clusters in the Milky Way, researchers can retrace how both galaxies assembled their oldest stars. As one NASA scientist notes, this study “can tell us more not only about how the LMC was originally formed, but the Milky Way Galaxy, too”. Overall, the discovery supports a picture of gradual galactic growth through multiple waves of star formation and mergers, rather than a single early burst.