Euclid Space Telescope Captures Stunning Razor-Sharp Images in Debut

Euclid Space Telescope Captures Stunning Razor-Sharp Images in Debut


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2023-11-08 09:43:24

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Table
  1. New Space Telescope Euclid Beams Back First Razor-Sharp Images
    1. The Perseus Cluster Of Galaxies
    3. Irregular Galaxy NGC 6822
    4. The Horsehead Nebula
    5. Globular Cluster NGC 6397

New Space Telescope Euclid Beams Back First Razor-Sharp Images

Euclid, the newly launched space telescope by the European Space Agency, has revealed its first set of images. Equipped with highly sensitive sensors, Euclid captures razor-sharp images across a wide field of view. The telescope's visible instrument, composed of 36 detectors, can capture the equivalent of nearly 70 4K resolution screens in one shot, covering an area of the night sky comparable to two-and-a-half full moons seen from Earth.

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Euclid's mission is to study dark matter and energy, and over the next six years, it will create a massive cosmic 3D map using its two instruments: the visible instrument and a Near-Infrared Spectrometer and Photometer. This data will help scientists gain a better understanding of how dark matter shapes and influences the universe.

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"Dark matter pulls galaxies together and causes them to spin more rapidly than visible matter alone can account for; dark energy is driving the accelerated expansion of the Universe," explained Carole Mundell, the Director of Science at the European Space Agency.

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The Perseus Cluster Of Galaxies

The image shows 1000 galaxies belonging to the Perseus Cluster, and more than 100,000 additional galaxies further away in the background, each containing up to hundreds of billions of stars.
The image shows 1000 galaxies belonging to the Perseus Cluster, and more than 100,000 additional galaxies further away in the background, each containing up to hundreds of billions of stars.

Spiral Galaxy IC 342, AKA The "Hidden Galaxy"

The 'Hidden Galaxy,' also known as IC 342 or Caldwell 5, is difficult to observe because it lies behind the busy disc of our Milky Way, and so dust, gas and stars obscure our view.
The 'Hidden Galaxy,' also known as IC 342 or Caldwell 5, is difficult to observe because it lies behind the busy disc of our Milky Way, and so dust, gas and stars obscure our view.

Euclid's infrared view has already revealed crucial information about stars in the "Hidden Galaxy."

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Irregular Galaxy NGC 6822

This image of the irregular galaxy known as 'NGC 6822' shows characteristics of a galaxy in its early development. Unlike the Milky Way, which has a distinct shape, NGC 6822 is irregular and small.
This image of the irregular galaxy known as 'NGC 6822' shows characteristics of a galaxy in its early development. Unlike the Milky Way, which has a distinct shape, NGC 6822 is irregular and small.

Euclid aims to observe galaxies up to 10 billion light-years away, including irregular dwarf galaxies like NGC 6822.

The Horsehead Nebula

Euclid shows us a spectacularly panoramic and detailed view of the Horsehead Nebula, also known as Barnard 33 and part of the constellation Orion. At approximately 1375 light-years away, the Horsehead – visible as a dark cloud shaped like a horse’s head – is the closest giant star-forming region to Earth.
Euclid shows us a spectacularly panoramic and detailed view of the Horsehead Nebula, also known as Barnard 33 and part of the constellation Orion. At approximately 1375 light-years away, the Horsehead – visible as a dark cloud shaped like a horse’s head – is the closest giant star-forming region to Earth.

Globular Cluster NGC 6397

This sparkly image shows Euclid’s view on a globular cluster called NGC 6397. Globular clusters are collections of hundreds of thousands of stars held together by gravity and are some of the oldest objects in the Universe.
This sparkly image shows Euclid’s view on a globular cluster called NGC 6397. Globular clusters are collections of hundreds of thousands of stars held together by gravity and are some of the oldest objects in the Universe.

Euclid's unique capabilities allow it to observe entire globular clusters and distinguish numerous stars within them.

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