The Leo Triplet

The Leo Triplet
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The Hyades star cluster, with bright yellow Aldebaran star.
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Messier 88 and Messier 91 in the constellation Coma Berenices
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The open cluster NGC 7243 in Lacerta.
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Albireo, bouble star in Cygnus.
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Messier galaxies M95, M96 and M105 in Leo.
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Stretch of galaxies known as Markarian's Chain.
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NGC 457, the ET or Owl Cluster in Cassiopeia.
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NGC 6397 globular cluster in Ara, with stars Beta Arae and Gamma Arae.
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A wide-field image of the field around the North Star, Polaris, at upper right.
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A galactic star scene with Omega Centauri, NGC 5128 and NGC 4945.
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Messier 5, a globular cluster in the constellation Serpens.
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The constellation of Corona Borealis, the Northern Crown, in the northern spring sky.
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Messier 44, the Beehive Cluster.
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The large Hyades star cluster with the giant star Aldebaran and star cluster NGC 1647.
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Messier 44, the Beehive Cluster, with stars Asellus Borealis and Asellus Australis.
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A huge elliptical galaxy.
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Panta rhei is a simplified version of the famous Greek philosopher Heraclitus' teachings. It basically means, everything flows. And everything in the Universe is indeed continually on the move, spiraling and shifting through space. Some cosmic objects move a little further than others take the subject of this NASA/ESA Hubble Space Telescope image, a globular cluster of stars known as Palomar 12. Although it currently lies on the outskirts of the Milky Way’s halo, Palomar 12 was not born here. When astronomers first studied this cluster, they were puzzled by its strangely young age when compared to the other clusters in the galaxy. It appeared to be around 30 percent younger than other Milky Way globulars. Surely if it had been born within our galaxy, it would have sprung to life at a similar time to its cluster companions A bit more digging revealed that Palomar 12 was actually ripped from its initial home, the Sagittarius Dwarf Elliptical galaxy, around 1.7 billion years ago via tid
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The glowing object in this Hubble Space Telescope image is an elliptical galaxy called NGC 3923. It is located over 90 million light-years away in the constellation of Hydra. NGC 3923 is an example of a shell galaxy where the stars in its halo are arranged in layers. Finding concentric shells of stars enclosing a galaxy is quite common and is observed in many elliptical galaxies. In fact, every tenth elliptical galaxy exhibits this onion-like structure, which has never been observed in spiral galaxies. The shell-like structures are thought to develop as a consequence of galactic cannibalism, when a larger galaxy ingests a smaller companion. As the two centers approach, they initially oscillate about a common center, and this oscillation ripples outwards forming the shells of stars just as ripples on a pond spread when the surface is disturbed. NGC 3923 has over twenty shells, with only a few of the outer ones visible in this image, and its shells are much more subtle than those of othe
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The Splinter Galaxy (NGC 5907), located in the constellation Draco, is viewed edge on from our perspective of 39 million light years away, features looping structures that represent the orbit of a former satellite galaxy that finally became aborbed
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Stars, dust and gas nebula in a far galaxy Stars, dust and gas nebula in a far galaxy. Elements of this image furnished by NASA Copyright: xZoonar.com/gannaxacheretx 11584269
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NGC 1275 in the constellation Perseus.
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Image Number: 4239-57495803Royalty FreeCredit Line:Roberto Colombari/Stocktrek Images/StockTrek/SuperStockCollection:Stocktrek ImagesStory:Stellar Clusters and GalaxiesContributor:Roberto ColombariModel Release:NoProperty Release:NoResolution:3690×2726
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