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See Milky Way’s core in most detailed photo yet

Milky Way's core: A crowded starfield showing countless stars in white and yellow with a few dark nebulae.
The Euclid space telescope has captured the largest and most detailed view of our Milky Way’s core yet. This is just a portion of the image, which Euclid made on March 23, 2025. The European Space Agency (ESA) released the image on June 24, 2026. Explore the image in its highest resolution here. Image via ESA/Euclid/Euclid Consortium/NASA, CFHT, image processing by J.-C. Cuillandre and E. Bertin (CEA Paris-Saclay).

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See Milky Way’s core in most detailed photo yet

On June 24, 2026, the European Space Agency (ESA) shared the largest and most detailed photo yet of our Milky Way galaxy’s heart. Captured by the Euclid space telescope, this view contains more than 60 million stars. Incredibly, that is still much less than even 1% of the stars that make up our Milky Way galaxy.

The Euclid telescope’s normal target is the faraway galaxies in our distant universe. The goal of the mission is to track the expansion of the universe, and in so doing, uncover the mysteries of dark matter and dark energy.

But for one day – March 23, 2025 – Euclid was tasked with a different mission. Euclid surveyed a part of our galaxy’s core that amounted to an area equal to 22 full moons in our sky. And the result is breathtaking.

View with irregular edges showing an area packed with stars and some dark nebulae or clouds.
This view shows Euclid’s full survey area. It is equal to 22 times the area of the full moon. Image via ESA/ Euclid/ Euclid Consortium/ NASA/ CFHT. Image processing by J.-C. Cuillandre and E. Bertin (CEA Paris-Saclay).

What part of the Milky Way does the image cover?

This packed, incredibly dense region of the Milky Way’s central zone is only a tiny portion of the galactic bulge. But zooming in on Euclid’s image shows just how much detail we can see among the stars. The dark areas in the insets are black, obscuring clouds of gas and dust that astronomers call dark nebulae.

Wide view of the plane of the Milky Way with insets showing location of the new image.
This wide-field view of the Milky Way is from Gaia, and the inset shows that Euclid’s new image is just a tiny portion of the core. Two more insets show just how much you can zoom in on Euclid’s image to identify individual stars. Image via ESA/ Euclid/ Euclid Consortium/NASA, CFHT/ ESA/ Gaia/ DPAC. Image processing by J.-C. Cuillandre and E. Bertin (CEA Paris-Saclay).

Why point Euclid at the Milky Way’s core?

Although the Euclid mission was not designed to observe the Milky Way’s core, astronomers wanted a view of this dense region without light from the stars overpowering one another. And Euclid has this capability. Getting a good look at individual stars near the galactic center allows astronomers to look for planets using microlensing. Microlensing is a phenomenon where the light from a more distant star bends around the nearer star. If the star that’s closest to us has a planet circling it, the light curve from the more distant star will show a spike. This technique only works when two stars happen to lie in the same path from Earth. And what better region to look at than one teeming with stars?

Graphic with 2 stars stacked and light curves below. On the right is the same but a small planet in the front and a spike in the light curve.
Microlensing allows astronomers to detect the presence of a planet around a near star by looking at the light curve of the more distant star. In the example on the right, a planet causes a spike in the light curve of the background star. Image via ESA.

Following up with future missions

Because it takes time for astronomers to see microlensing events, the Euclid image will provide a starting point for future surveys with instruments such as the Nancy Grace Roman Space Telescope. The leader of the Euclid galactic bulge survey, Natalia Rektsini, said:

In 24 hours, Euclid has already captured the stars involved in all the future microlensing events that the Roman space telescope will detect, but before the stars and planets involved have aligned. This means that anyone who detects a microlensing event in the same region, for example with Roman, will be able from now on to use Euclid data as a time reference in the past and see how the stars looked before they overlapped. Since Euclid can clearly separate individual stars, one can then measure how fast they move over time and use that information to confirm the existence of a planet and determine its mass. This would not be possible with data from one point in time.

Enjoy the beauty of the dense starfield in our galactic heart

The new image from Euclid will support future investigations into planets lurking around stars near the center of our galaxy. But it also allows us – right now – to bask in the beauty that is our home galaxy. Enjoy this video of the crowded, starry region near the Milky Way’s core.

Bottom line: ESA released a new image of the Milky Way’s core. This view, from the Euclid space telescope, is the largest and most detailed image yet of the galactic center.

Via ESA

Posted 
June 26, 2026
 in 
Today's Image

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