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  2. Euclid (spacecraft) - Wikipedia

    en.wikipedia.org/wiki/Euclid_(spacecraft)

    This release contains images and catalogs of star-forming regions, globular clusters, nearby galaxies, fields of the Fornax cluster and Perseus cluster, as well as more distant galaxy clusters. [35] The content of the ERO is described in one paper submitted to Astronomy & Astrophysics .

  3. Shimmering galaxies revealed in new photos by European space ...

    www.aol.com/news/shimmering-galaxies-revealed...

    In one picture, Euclid captured a group shot of 1,000 galaxies in a cluster 240 million light-years away, against a backdrop of more than 100,000 galaxies billions of light-years away. A light ...

  4. IC 342 - Wikipedia

    en.wikipedia.org/wiki/IC_342

    IC 342 (also known as Caldwell 5) is an intermediate spiral galaxy in the constellation Camelopardalis, located relatively close to the Milky Way.Despite its size and actual brightness, its location behind dusty areas near the galactic equator makes it difficult to observe, leading to the nickname "The Hidden Galaxy", [4] [1] though it can readily be detected even with binoculars. [5]

  5. Euclid telescope's first images offer full-color look at the ...

    www.aol.com/news/euclid-telescopes-first-images...

    The Euclid telescope's view of a spiral galaxy known as IC 342. ... The Euclid telescope spied a globular cluster — a huge collection of hundreds of thousands of stars bound together by gravity ...

  6. Euclid telescope’s first images reveal new cosmic details - AOL

    www.aol.com/euclid-telescope-first-images-reveal...

    The first five color images captured by the European Space Agency’s Euclid telescope were revealed Tuesday, capturing previously unseen cosmic details.

  7. MACS J0025.4-1222 - Wikipedia

    en.wikipedia.org/wiki/MACS_J0025.4-1222

    MACS J0025.4-1222 is a galaxy cluster created by the collision of two galaxy clusters, and is part of the MAssive Cluster Survey (MACS). Like the earlier discovered Bullet Cluster, this cluster shows a clear separation between the centroid of the intergalactic gas (of majority of the normal, or baryonic, mass) and the colliding clusters.