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Star Clusters
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Clusters and superclusters of galaxies-Illustratio
Star clusters, 1814
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Clusters and superclusters of galaxies-Illustratio
Calcite (photo)
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Phenakite (photo)
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1856, Burritt, Huntington Chart of Star Clusters and Double Stars
Salt formations (photo)
Stibnite (photo)
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Salt formations (photo)
Cinnabar (photo)
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1856, Burritt, Huntington Chart of Comets, Star Clusters, Galaxies, and Nebulae
Erythrite (photo)
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Salt formations (photo)
1960s: Organisms under a microscope, some in giant cluster and some in wormlike shapes.
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Wall hanging showing two star clusters, 1850-60 (cotton, brass)
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Hyades and Pleiades open clusters - Hyades and Pleiades open clusters - The Hyades cluster, on the left, with the brilliant star Aldebaran. On the right, the Pleiades cluster. These two clusters belong to the constellation of the Taurus of which Aldebaran is the brightest star; it is a red giante. The Hyades is seen at left, containing the bright star Aldeberan. The Pleiades is at right. Both are open clusters in the constellation of Taurus. This skyview is corresponding to binoculars and small telescopes
Heulandite (photo)
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1960s: Organisms under a microscope, some in giant cluster and some in wormlike shapes.
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Amethyst crystals (photo)
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Salt Clusters, Dead Sea, Israel (photo)
Add MS 41623 f.111v Pine, from a 'A herbal', Belluno (ink & colour on vellum)
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Mesolite (photo)
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Nebula Sh2 - 142 in Cephee - Star formation region in Cephee and star clusters NGC 7380
Sarcophagus from the 'Tomb of the Nazirite', Mount Scopus, Jerusalem, Herodian Period (hard limestone)
Open clusters M6 and M7 in Scorpio - Open clusters M6 and M7 in Scorpius - The star clusters M6 (NGC 6405), at the top right, and M7 (NGC 6475), at the bottom of the image, are two open clusters located in the constellation Scorpio. M6, the Butterfly Cluster, at upper right, is a wonderful open cluster, it can be seen about 4 degrees northwest of M7, with both clusters being located in Scorpius. M7, at bottom, consists of 80 stars brighter than magnitude 10 in a field of about 1.3 degrees apparent diameter. It was known to Ptolemy who mentioned it in 130 AD. Both clusters are visible with the unaided eye in a rich area of Milky Way located between Sagittarius and Scorpius
The dreamer, 2000 (acrylic on board)
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Hyades and Pleiades open clusters - Hyades and Pleiades open clusters - The Hyades cluster, bottom left, with the bright star Aldebaran. In the center, the Pleiades cluster. These two clusters belong to the constellation of the Taurus of which Aldebaran is the brightest star; it is a red giante. The Pleiades is a relatively nearby open cluster, which is located at a distance of 440 light years. The Hyades (at bottom left) is another open cluster located even closer at a distance of 153 light years
Hyades and Pleiades open clusters - Hyades and Pleiades open clusters - The Hyades cluster, on the left, with the brilliant star Aldebaran. On the right, the Pleiades cluster. These two clusters belong to the constellation of the Taurus of which Aldebaran is the brightest star; it is a red giante. The Pleiades is a relatively nearby open cluster, which according to new data from the Hipparcos satellite is located at a distance of 370 light years. The Hyades (at left) is another open cluster located even closer at a distance of 153 light years
Nebula IC 4628 and star clusters in Scorpio - Nebula IC 4628 and star clusters in Scorpio - Nebula IC 4628 in the middle left of the image is surrounded at the bottom by the star cluster NGC 6231, and by the NGC 6242 cluster at the top of the image. A beautiful collection of open clusters and nebulosity is seen here in Scorpius, just north of the double star Zeta Scorpii. Zeta is visible at the far bottom right and is also know as the “Little Cat's Eyes””. NGC 6231 is a lovely open cluster above Zeta. IC 4628 is the emission nebula just northeast of two loose open clusters, Cr 316 and Tr 24 in the center of the photo. NGC 6242 is the other small open cluster at top left. (c) 2006 Jerry Lodriguss/www.astropix.co
Star clusters M46 and M47 and planetary nebula NGC 2438 in stern - Open clusters M46 and M47 - M46 (NGC 2437) and M47 (NGC 2422), are two open clusters located in the constellation Stern. M46, which contains the planetary nebula NGC 2438, is on the left, M47, on the right. M46 and M47 are two interesting open clusters that lie a little more than 1 degree apart in the sky in the constellation of Pupis. M46, containing planetary nebula NGC 2438, is seen at left in this photo, and M47 is at right. M47 is a bright cluster that can be seen with the unaided eye under dark skies. It is comprised of about 30 stars, and is 30 arc minutes in diameter and has an overall brightness of 4.4 magnitude
The Latrobe nugget, 1850
The Latrobe nugget, 1850
New Continent, 1962 (painted wood)
Copyright/Diritti d'Autore
  • In Copyright
Anglo-American incendiary bombs fall on Hamburg, 1942-45 (b/w photo)
Globular cluster M5 in Serpens - Globular cluster M5 in Serpens - This cluster of stars is located about 25,000 light years away from Earth. It is one of the most extensive (165 years - light) and one of the oldest known globular clusters. M5 is perhaps the most spectacular globular cluster visible from the northern hemisphere, and can even be seen under excellent conditions with the naked eye, in the constellation Serpens. It is elongated, one of the largest and one of the oldest clusters (maybe 13 billion years), and at a distance of almost 25000 light - years from us
Globular cluster M5 in Serpens - Globular cluster M5 in Serpens - This cluster of stars is located about 25,000 light years away from Earth. It is one of the most extensive (165 years - light) and one of the oldest known globular clusters. M5 is perhaps the most spectacular globular cluster visible from the northern hemisphere, and can even be seen under excellent conditions with the naked eye, in the constellation Serpens. It is elongated, one of the largest and one of the oldest clusters (maybe 13 billion years), and at a distance of almost 25000 light - years from us
Star cluster NGC 6791 in Lyra - Open cluster NGC 6791 in Lyra - NGC 6791 is one of the oldest and largest open clusters; it contains about 10,000 stars. Here, a detail of the cluster obtained by the Hubble space telescope. The stars present would be 8 billion years old. A galaxy in the background is also visible at the top left. NGC 6791 is one of the oldest and largest open clusters known, about 10 times larger than most open clusters and containing roughly 10,000 stars. The cluster is located 13 000 light years in the constellation Lyra. The full Hubble Advanced Camera for Surveys field is full of stars estimated to be 8 billion years old. Two background galaxies can be seen at upper left
Globular cluster M5 in Serpens - Globular cluster M5 in Serpens - This cluster of stars is located about 25,000 light years away from Earth. It is one of the most extensive (165 years - light) and one of the oldest known globular clusters. M5 is perhaps the most spectacular globular cluster visible from the northern hemisphere, and can even be seen under excellent conditions with the naked eye, in the constellation Serpens. It is elongated, one of the largest and one of the oldest clusters (maybe 13 billion years), and at a distance of almost 25000 light - years from us
Group of Galaxies HCG 31 - Hickson Compact Group 31 - This group of interacting galaxies is located 166 million years of light from Earth in the constellation Eridan. Dwarf galaxies are merging causing intense star formation. This long fusion process will lead to the birth of a large elliptical galaxy. Image obtained by the Hubble Space Telescope on August 8, 2006. These four dwarf galaxies waited billions of years to come together, setting off a fireworks show as thousands of new star clusters come to life. The distorted galaxies are quickly producing massive, hot, young stars that are pumping out ultraviolet radiation, heating up surrounding gas clouds, and causing them to glow. Such encounters between dwarf galaxies are normally seen billions of light - years away and therefore occurred billions of years ago. But these galaxies, members of Hickson Compact Group 31, are relatively nearby, only 166 million light - years away. In this image, taken by Nasa's Hubble Space Telescope, the bright, distorted object at middle, left, is actually two colliding dwarf galaxies. Myriad star clusters have formed in the streamers of debris pulled from the galaxies and at the site of their head - on collision. The cigar - shaped object above the galaxy duo is another member of the group. A bridge of star clusters connects the trio. A long rope of bright star clusters points to the fourth member of the group, at lower right. The bright object in the center is a foreground star. Astronomers used Hubble's Advanced Camera for Surveys to resolve the youngest and brightest of star clusters, which allowed them to calculate the clusters' ages, map the star - formation history, and determine that the galaxies are starting the final stages of galaxy assembly. Hubble reveals that the brightest clusters, hefty groups each holding at least 100,000 stars, are less than 10 million years old. Astronomers say the interacting galaxies will form
Planete pres d'un amas globulaire - Artist view - Planet close to a globular cluster - Artist view - A globular cluster seen from the surface of a hypothetical planet. This cluster contains about 50,000 stars and is riding high above our own Milky Way galaxy. Like other globular clusters, it may be the remnant of the core of a small galaxy long ago adsorbed by the larger Milky Way. There may even be a black hole lurking at its center. Globular clusters usually contain very old stars. Any planets to be found in one would likely be much older than the Earth
One of the countless granite clusters that Mongolians call “Kyrgyz Nests” (Kyrgyz Our), August 23 - Mission in North West Mongolia - Album of the mission of Bouillane de Lacoste commander in 1909 in Mongolia, photo by Henry de Bouillane de Lacoste (1867-1937)
Interacting galaxies NGC 3256 - Interacting galaxies NGC 3256 - The special galaxy NGC 3256 is located about 100 million light years away from Earth in the southern constellation of Sails. A vestige of the collision of two galaxies, this system presents a double nucleus and many young clusters of stars. Image obtained by the Hubble Space Telescope on November 5, 2001. NGC 3256 is an impressive example of a peculiar galaxy that is actually the relict of a collision of two separate galaxies that took place in a distant past. The telltale signs of the collision are two extended luminous tails swirling out from the galaxy. NGC 3256 belongs to the Hydra - Centaurus supercluster complex and provides a nearby template for studying the properties of young star clusters in tidal tails. The system hides a double nucleus and a tangle of dust lanes in the central region. The tails are studded with a particularly high density of star clusters. Image taken by the Hubble space telescope on November 5, 2001
The Small Magellanic Cloud - The Small Magellanic Cloud - The Small Magellanic Cloud galaxy is about 210,000 light years away from Earth in the southern constellation of Toucan. It's one of the closest galaxies of the Lactee Way. Two globular clusters are visible in this image, on the left the Toucan cluster, at the bottom of the galaxy the NGC 362 cluster. The Small Magellanic Cloud is a dwarf irregular galaxy located at a distance of about 210,000 light years; it is one of the Milky Way's nearest neighbors. Two globular clusters are visible: at left NGC 104, better known as 47 Tucanae, at the bottom NGC 362
Globular clusters M9 and NGC 6356 in Ophiuchus - Globular clusters M9 and NGC 6356 in Ophiuchus - Globular clusters M9 (NGC 6333, right) and NGC 6356 (top). M9 is one of the closest globular clusters to the center of our galaxy. NGC 6356 is twice as far away from us, about 50,000 years of light from Earth. Globular clusters M9 (NGC 6333), on the right and NGC 6356, on the top. M9 is one of the nearer globular clusters to the center of our Galaxy. NGC 6356 is two times distant from us, at about 50,000 light years
The Small Magellanic Cloud (NGC 292) - The Small Magellanic Cloud (NGC 292) - The Small Magellanic Cloud galaxy is about 240,000 years from Earth in the southern constellation of Toucan. It's one of the closest galaxies of the Lactee Way. Two globular clusters are visible in this image, on the right the Toucan cluster, at the top of the galaxy the NGC 362 cluster. The Small Magellanic Cloud is about 210,000 light years in the constellation of Tucana. It is one of the Milky Way's nearest neighbors. The globular clusters 47 Tucana (on the right) and NGC 362 (on the upper left corner) are also visible on this image
Star cluster M46 and M47 and NGC 2438 in the stern - Open clusters M46 and M47 - M46 (NGC 2437), on the left, is a cluster of age stars located at 5400 years - light. It contains about 500 stars, 150 of which are brilliant. It is about 300 million years old. The planetary nebula NGC 2438 does not appear to belong to this cluster, and must be closer although its distance is unknown. On the right, cluster M47 (NGC 2422). Between the two clusters we can see a third one: NGC 2425. M46 and M47 are two open clusters that lie a little more than 1 degree apart in the sky in the constellation of Pupis. M46, containing planetary nebula NGC 2438, is seen at left in this photo, and M47 is at right. M47 is a bright cluster that can be seen with the unaided eye under dark skies. It is comprised of about 30 stars, and is 30 arc minutes in diameter and has an overall brightness of 4.4 magnitude