The European Space Agency’s (ESA) Euclid Space Telescope has sent back its first scientific images, and they’re truly amazing. Each of his five images of shimmering space objects will eventually become part of his 3D map of Euclidean’s universe, with the ultimate goal of understanding the dark component of the universe.

Euclid was launched on July 1st and is currently parked approximately 1.5 million kilometers from Earth. Over the next six years, she plans to photograph about a third of the sky and build her 3D map of the universe, the most detailed ever created. This map provides researchers with an unprecedented window into the large-scale structure of the universe, revealing the behavior of dark matter and dark energy on cosmic scales and how it departs from current understanding of physics and cosmology. It will help you understand what to do.

horsehead nebula

ESA/Euclid/Euclid Consortium/NASA; J.-C. Cuillandre (CEA Paris-Saclay), G. Anselmi; CC BY-SA 3.0 IGO

Dark matter and dark energy are invisible to the naked eye, hence their nickname “dark.” Therefore, the only way to track their behavior is through images of visible objects, such as those currently published by Euclid. The first of these images shows the Horsehead Nebula in the constellation Orion, 1375 light-years from Earth. The nebula is well known, but the amazing detail in this new image may allow scientists to discover new stars and even young planets.

Globular cluster NGC 6397

ESA/Euclid/Euclid Consortium/NASA; J.-C. Cuillandre (CEA Paris-Saclay), G. Anselmi; CC BY-SA 3.0 IGO

This glittering mass of hundreds of thousands of stars It is a globular cluster called NGC 6397. Because these clusters are so large, it is difficult to capture them in detail without many observations, which Euclid’s wide field of view makes possible. Researchers are not sure whether globular clusters are embedded in halos of dark matter, but Euclid’s measurements could help answer this question.

“Hidden galaxy” IC 342 (left) and irregular galaxy NGC 6822 (right)

ESA/Euclid/Euclid Consortium/NASA; J.-C. Cuillandre (CEA Paris-Saclay), G. Anselmi; CC BY-SA 3.0 IGO

Each photo above shows a galaxy. On the left is spiral galaxy IC 342. This galaxy is called a hidden galaxy because it is located on the opposite side of the Milky Way disk from Earth and is difficult to see through all the stars, gas, and dust. This galaxy contains many globular clusters and is similar to our own galaxy, making it an excellent comparison point for understanding whether the Milky Way is normal or abnormal.

On the right is irregular galaxy NGC 6822, which represents a type of galaxy that was common in the early universe. Many of these small galaxies have less distinct structures and have merged over time to form more massive galaxies, such as the Milky Way or hidden galaxies. During the course of his mission, Euclid observed billions of galaxies and marked each galaxy’s position within the larger cosmic web.

perseus galaxy cluster

ESA/Euclid/Euclid Consortium/NASA; J.-C. Cuillandre (CEA Paris-Saclay), G. Anselmi; CC BY-SA 3.0 IGO

At first glance, this image looks like an irregular galaxy or globular cluster, but it actually shows more than 100,000 galaxies. About 1000 of them are in the foreground of the image and belong to the Perseus galaxy cluster. Many of them have never been discovered before. Such gigantic structures are only possible due to the influence of dark matter, so observations like this one are extremely important for elucidating their true nature.

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