Scan More than 60 Million Stars in the Most Detailed Photo of the Milky Way Ever Taken
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TL;DR

The European Space Agency’s Euclid mission has taken the most detailed image of the Milky Way’s core, capturing more than 60 million stars. This achievement enhances our understanding of the galaxy’s structure and potential exoplanets, with further analysis ongoing.

The European Space Agency’s Euclid mission has produced the most detailed image of the dense, glowing center of the Milky Way galaxy to date, capturing over 60 million stars. This achievement provides new opportunities for studying the galaxy’s structure and searching for exoplanets, marking a notable development in astronomical imaging.

The image, taken in visible light, reveals the galactic bulge—a densely packed region filled mainly with old, cooler stars that give it a yellow hue, according to ESA. It also captures various phenomena such as nebulae, bright star clusters, and molecular clouds, which appear as dark splotches against the brighter background. The photograph was made possible by ESA’s Euclid spacecraft, which can survey large areas of the galaxy with high sensitivity and sharpness.

Compared to the Hubble Space Telescope, Euclid’s images are similarly detailed but cover a much larger field of view—each pointing spans an area 270 times greater than Hubble’s. To observe the same region with Euclid, the Keck Observatory would require approximately 2,000 hours of observation time, highlighting Euclid’s efficiency and capability.

At a glance
breakingWhen: announced March 2025
The developmentIn March 2025, the Euclid mission captured the highest-resolution image of the Milky Way’s center, revealing over 60 million stars and other phenomena.

Implications for Galactic and Exoplanet Research

This image represents an advancement in astronomical imaging, enabling scientists to analyze the structure of the Milky Way’s core with greater detail. The ability to monitor over 60 million stars simultaneously can assist in efforts to identify exoplanets via microlensing, where small fluctuations in starlight may indicate orbiting planets. Additionally, understanding the distribution and properties of stars in the galactic bulge can contribute to studies of the galaxy’s formation and evolution.

The data collected could support the discovery of new exoplanets and improve models of galactic dynamics. This progress also highlights the capabilities of ESA’s Euclid mission in expanding our understanding of the universe, with potential influence on future observational strategies and space telescopes.

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Milestone in Space Imaging Capabilities

The Euclid mission, launched by ESA in 2022, aims to map the large-scale structure of the universe and study dark matter and dark energy. Its recent imaging achievement builds on previous high-resolution observations but surpasses them in scope and detail. The March 2025 image signifies a step forward in galactic imaging, comparable in clarity to the Hubble Space Telescope but covering a larger area.

The galactic bulge of the Milky Way, a primary target of the survey, has been studied extensively, but the large number of stars captured in this image—more than 60 million—provides a substantial dataset for analysis. Earlier efforts relied on smaller fields of view or lower resolution, which limited the scope of research. ESA’s technological advancements and the design of the Euclid spacecraft have facilitated this progress.

“The Euclid image of the galactic bulge provides a detailed map of a large number of stars in a single observation.”

— ESA spokesperson

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Outstanding Questions About Data Analysis

While the image’s resolution and scope are confirmed, detailed analysis of the data, including the identification of new exoplanets or insights into galactic formation, is still underway. The full scientific implications are yet to be published, and further studies are necessary to interpret the dataset comprehensively.

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Upcoming Analysis and Future Observations

Researchers will analyze the image data over the coming months to identify potential exoplanets and refine models of the Milky Way’s structure. ESA plans to continue utilizing Euclid for extensive surveys, with additional high-resolution imaging sessions scheduled. The findings from this dataset could inform future space missions and ground-based observations.

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Key Questions

How does Euclid’s imaging compare to Hubble’s?

Euclid’s images are similar in clarity and sensitivity but cover a field of view 270 times larger than Hubble’s in each pointing, enabling broader surveys.

What is the significance of capturing over 60 million stars?

This allows scientists to study the structure, composition, and dynamics of the galaxy’s core in greater detail, aiding in the search for exoplanets and understanding galactic evolution.

Will this image help find new exoplanets?

Yes, by monitoring small fluctuations in starlight through microlensing, researchers aim to identify new exoplanets orbiting stars within the dense galactic bulge.

When will the full scientific analysis be available?

Detailed analysis is expected to be published over the next several months as scientists examine the dataset collected by Euclid.

What are the next steps for the Euclid mission?

Euclid will continue its survey operations, capturing additional high-resolution images to further investigate the universe’s structure and dark matter distribution.

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