Monday, April 20, 2026

‘Interstellar Glaciers’: NASA’s SPHEREx Maps Vast Galactic Ice Regions -UNIVERSE

Water ice highlighted

Interstellar dust highlighted

These observations made by NASA’s SPHEREx mission reveal vast frozen complexes in the Cygnus X star-forming region of the Milky Way galaxy. Water ice, shown as bright blue structures at left, exactly overlays the dark lanes of interstellar dust, shown in different wavelengths at right.

NASA’s SPHEREx (Spectro-Photometer for the History of the Universe, Epoch of Reionization, and Ices Explorer) mission has mapped interstellar ice at an unprecedented scale. Covering regions in our Milky Way galaxy more than 600 light-years across, the ice was found inside giant molecular clouds — vast regions of gas and dust where dense clumps of matter collapse under gravity, giving birth to stars. A study describing these findings published Wednesday in The Astrophysical Journal.

One of SPHEREx’s main goals is to map the chemical signatures of various types of interstellar ice. This ice includes molecules like water, carbon dioxide, and carbon monoxide, which are vital to the chemistry that allows life to develop. Researchers believe these ice reservoirs, attached to the surfaces of tiny dust grains, are where most of the universe’s water is formed and stored. The water in Earth’s oceans — and the ices in comets and on other planets and moons in our galaxy — originates from these regions.

“These vast frozen complexes are like ‘interstellar glaciers’ that could deliver a massive water supply to new solar systems that will be born in the region,” said study coauthor Phil Korngut, the instrument scientist for SPHEREx at Caltech in Pasadena, California. “It’s a profound idea that we are looking at a map of material that could rain on nascent planets and potentially support future life.” 

Thanks to its spectral capabilities, SPHEREx can measure the amounts of various ices and molecules, such as polycyclic aromatic hydrocarbons, in and around molecular clouds, helping scientists better understand their composition and environment.  

Although space telescopes such as NASA’s James Webb Space Telescope and the agency’s retired Spitzer have detected water, carbon dioxide, carbon monoxide, and other icy molecules throughout our galaxy, the SPHEREx observatory is the first infrared mission specifically designed to find such molecules over the entire sky via the mission’s large-scale spectral survey. 

“We expected to detect these ices in front of individual bright stars: The light from a star acts like a spotlight, revealing any ice in the space between us and that star. But this is something different,” said lead author Joseph Hora, an astronomer at the Center for Astrophysics (CfA) at Harvard & Smithsonian in Cambridge, Massachusetts. “When looking along the galactic plane — where most of the stars, gas, and dust of our galaxy are concentrated — there’s a lot of diffuse background light shining through entire dust clouds, and SPHEREx can see the spatial distribution of the ices they contain in incredible detail.” 

Managed by NASA’s Jet Propulsion Laboratory in Southern California, the SPHEREx observatory launched March 11, 2025, and has the unique ability to see the sky in 102 colors, each representing a different wavelength of infrared light that offers distinctive information about galaxies, stars, planet-forming regions, and other cosmic features. By late 2025, SPHEREx had completed the first of four all-sky infrared maps of the universe, charting the positions of hundreds of millions of galaxies in 3D to help answer major questions about the cosmos, including those about the origins of water and life.

Icy origins

Using the SPHEREx maps of various icy molecules, the study’s authors were able to look deep into many molecular clouds in the Cygnus X and North American Nebula regions of the Milky Way. In the densest areas, where the amount of dust is greatest, dark filamentary lanes block the visible light from the stars behind. With its infrared eye, the space telescope also revealed where the different ices — which absorb specific wavelengths of infrared light that would pass through the clouds if they consisted only of dust — are at their densest.  

This finding supports the hypothesis that interstellar ice forms on the surface of tiny dust particles, which are no larger than particles found in candle smoke, and that the dense regions of dust shield the ices from the intense ultraviolet radiation emitted by newborn stars. However, not all ices are treated the same way in the interstellar medium.

“We can investigate the environmental factors that contribute to different ice formation rates across large areas of interstellar space,” said study coauthor Gary Melnick, also an astronomer at the CfA. “The SPHEREx mission’s ‘big picture’ view provides valuable new information you can’t get when zooming in on a small region.” 

Within this broad perspective, adds Melnick, SPHEREx can do something ground-based observatories cannot: detect varying amounts of water and carbon dioxide, two ices that respond differently to environmental factors. For example, the presence of intense ultraviolet light from nearby massive young stars or the heating of these dust grains by that light affects the abundances of different ices in distinct ways. 

This is just the beginning for the mission. Observations from SPHEREx will provide scientists with a powerful tool to explore the various components of our galaxy, the physics of the interstellar medium that lead to star and planet formation, and the chemical processes that deliver molecules essential for life to newly formed planets.

More about SPHEREx

The mission is managed by JPL for the agency’s Astrophysics Division within the Science Mission Directorate in Washington. The telescope and the spacecraft bus were built by BAE Systems in Boulder, Colorado. The science analysis of the SPHEREx data is being conducted by a team of scientists at 13 institutions across the U.S. and in South Korea and Taiwan, led by Principal Investigator Jamie Bock, who is based at Caltech with a joint JPL appointment, and by JPL Project Scientist Olivier Doré. Data is processed and archived at IPAC at Caltech in Pasadena, which manages JPL for NASA. The SPHEREx dataset is freely available to scientists and the public. 

For more information about the SPHEREx mission visit: https://science.nasa.gov/mission/spherex/ 

Source: ‘Interstellar Glaciers’: NASA’s SPHEREx Maps Vast Galactic Ice Regions - NASA 

Gone with the wind: Turbine parameters drive significant differences in offshore wind power forecasts - Engineering - Energy & Green Tech

Credit: Pixabay/CC0 Public Domain

Offshore wind energy generation is a central pillar of Europe's energy transition. At the same time, it is placing increasing demands on models that are expected to reliably predict future wind power production and its impact on the atmosphere. A study by the Helmholtz-Zentrum Hereon now shows that both atmospheric boundary conditions and technical decisions made during the development of wind farms can lead to significant differences. The various turbine parameters have a particularly strong influence on the calculations, as the associated reduction in wind speeds has a substantial impact on the results. The researchers' findings were published in the journal Wind Energy Science.

For the study, the established regional model COSMO6.0 CLM was further developed and combined with an expanded wind farm module that offers greater flexibility than previous versions. For the first time, different turbine types and rotor sizes, as well as staggered commissioning schedules of individual wind farms over time, can be represented within a single model. In parallel, the researchers investigated how the spatial arrangement of turbine arrays affects the simulated total power production.

Larger turbines alter both the wind field and energy yields

"The results show that, assuming a total installed capacity of 150 gigawatts in the North Sea, there are clear differences in the simulated power production. The differences between the scenarios amount to around 15 gigawatts in total, which corresponds to a remarkable 10% of the overall capacity," says Prof Corinna Schrum, who contributed to the study as head of the Hereon Institute of Coastal Systems—Analysis and Modelling.

The largest deviations occur between different turbine types, particularly between older models with lower rated capacity and modern installations with very large rotors. The technological shift toward ever larger turbines shows pronounced effects. The study compares two extreme cases: small 3.6 MW turbines and modern 15 MW turbines.

Power curves for turbines with different rated capacities. Idealized power (solid lines), uncorrected curves calculated directly from the provided turbine power coefficients (dashed-dotted lines), and corrected curves obtained following the application of the scale factor (dashed lines). Credit: Wind Energy Science (2026). DOI: 10.5194/wes-11-1077-2026

Extended wake effects assumed

A key aspect of the study is the analysis of the wake effects behind wind turbines, which are characterized by reduced wind speeds and increased turbulence, as the turbines extract kinetic energy from the wind. As shown in previous studies—including those conducted by Hereon—the wake effects of wind farms can extend more than 50 kilometers downstream of the wind farms, significantly reducing wind speeds in those areas.

However, until now, the influence of different boundary conditions used to drive regional simulations has largely been neglected in those studies. Additionally, it was demonstrated for the first time that realistic modeling of wind fields under the influence of the wind farms built between 2008 and 2021 could be performed, with variations of approximately 20% depending on the location, weather conditions, and wind farm configuration.

The results of the study have direct relevance for offshore wind power planning and for forecasting the total amount of offshore wind energy to be generated. They provide an assessment of the accuracy of simulation results and show that different modeling approaches can lead to substantially different forecasts: wind farms need to be explicitly represented in both weather forecasting models and the generation of historical, so-called reanalysis data. To achieve a realistic assessment of energy yields and to adequately address the ecological and infrastructural context of future expansion, it is essential to take these uncertainties into account. 

Provided by Helmholtz Association of German Research Centres 

Source: Gone with the wind: Turbine parameters drive significant differences in offshore wind power forecasts