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{"event":"custom_event","event_name":"view_search_result","event_category":"browse_catalog","keyword":"Dss","search_type":"standard","search_bridgeman_artists":"false","search_mode":"automatic","search_zero_result":"false","search_results":448,"search_results_page_number":1}

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Andromede Galaxy - The Andromeda Galaxy (M31) - The Andromede galaxy is located about 2.3 million years ago - light from Earth. Two satellite galaxies accompany it: M32 (NGC 221) at the top left of the nucleus, and M110 (NGC 205) at the bottom. Like the lactee path, the Andromede galaxy belongs to the local group, making up about thirty galaxies. M31, the Great galaxy in Andromeda, is a gigantic collection of more than 300 billion stars and is located about 2 million light years from Earth. Companion dwarf elliptical galaxies M32 and M110 are also visible. M31 and its companions are part of our local group of galaxies, which includes the Milky Way and Magellanic Clouds, and M33. The Andromeda Galaxy is headed towards our Milky Way Galaxy and is expected to collide with it and possibly merge into a gigantic elliptical galaxy in about 3 billion years
Double star 61 Cygni - Binary star 61 Cygni - 61 Cygni is a binary system of two stars comparable to the Sun. Located 11.4 years - light from the Earth, 61 Cygni is the first star (after the Sun) whose distance was measured thanks to its parallax. Image obtained by the Oschin telescope of Mount Palomar through several filters and composed. 61 Cygni is a binary star system in the Constellation Cygnus at approximately 11.4 light - years distance from Earth. Composite image obtained by the Oschin telescope refractor at the Palomar Observatory, USA
Summertime, 2012 (collage mixed media on paper)
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The star Fomalhaut - Star Fomalhaut - The star Fomalhaut is located 25 years - light from Earth in the constellation Southern Fish. An extrasolar planet, called Fomalhaut b, with a mass close to Jupiter, is in orbit around it. This image shows Fomalhaut, the star around which the discovered planet Fomalhaut b orbits. Fomalhaut is much hotter than our Sun, 15 times as bright, and lies 25 light - years from Earth. It is blazing through hydrogen at such a furious rate that it will burn out in only one billion years, 10% the lifespan of our star. The field of view is 2.7 x 2.9 degrees
Andromede Galaxy - Andromeda galaxy - The Andromede galaxy is located about 2.3 million years ago - light from Earth. Two satellite galaxies accompany it: M32 (NGC 221) at the top left of the nucleus, and M110 (NGC 205) at the bottom. Like the lactee path, the Andromede galaxy belongs to the local group, making up about thirty galaxies. M31, the Great galaxy in Andromeda, is a gigantic collection of more than 300 billion stars and is located about 2 million light years from Earth. Companion dwarf elliptical galaxies M32 and M110 are also visible. M31 and its companions are part of our local group of galaxies, which includes the Milky Way and Magellanic Clouds, and M33. The Andromeda Galaxy is headed towards our Milky Way Galaxy and is expected to collide with it and possibly merge into a gigantic elliptical galaxy in about 3 billion years
Turangalîla 5, 1991 (acrylic on canvas)
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 Turangalîla 3, 1991 (acrylic on canvas)
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Harbour, 2012 (collage mixed media on paper)
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Turangalîla 10, 1991 (acrylic on canvas)
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Turangalîla 21, 1991 (oil on canvas)
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 Turangalîla 13, 1991 (acrylic on canvas)
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Calypso, 2006 (acrylic on canvas)
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Sculptor's Dwarf Galaxy - Sculptor dwarf galaxy - The Sculptor's dwarf galaxy belongs to the local group, just like our galaxy or the Andromede galaxy. The Sculptor dwarf galaxy is one of our Milky Way's neighbouring dwarf galaxies. The Milky Way is, like all large galaxies, thought to have formed from smaller galaxies in the early days of the Universe. These small galaxies should also contain many very old stars, just as the Milky Way does, and a team of astronomers has now shown that this is indeed the case. This image was composed from data from the Digitized Sky Survey 2
The dwarf galaxy of the furnace - Fornax dwarf galaxy - The dwarf galaxy of the furnace belongs to the local group, just like our galaxy or the galaxy of Andromede. The Fornax dwarf galaxy is one of our Milky Way's neighbouring dwarf galaxies. The Milky Way is, like all large galaxies, thought to have formed from smaller galaxies in the early days of the Universe. These small galaxies should also contain many very old stars, just as the Milky Way does, and a team of astronomers has now shown that this is indeed the case. This image was composed from data from the Digitized Sky Survey 2
Globular cluster M107 in Ophiuchus - Globular cluster M107 in Ophiuchu
Galaxies Maffei 1 and Maffei 2 in Cassiopee - Maffei Galaxies in Cassiopeia - Maffei 1 (right) is an elliptical galaxy, Maffei 2 (left) is a barree spiral galaxy. These two galaxies are located about 8 million light years away from Earth. Image obtained by the Oschin telescope of Mount Palomar through several filters and composed. The picture show two galaxies lying at 2.5 degrees northeast of h and Chi Persei the famous Double Cluster in Cassiopeia. Although the galaxies has been obstructed by inner galactic matters, their actual sizes are larger than 10 arc minutes, fairly large - sized neighboring galaxies. The Maffei I (on the right) is an elliptic, and the Maffei II (on the left) is classified as a bared galaxy. The galaxies are estimated about 8 million light years away. They were discovered by the Italian astronomer Paolo Maffei in 1968. Now we know about 20 galaxies belonging to Maffei Group. This image is based on data acquired by the Oschin Telescope at the Mount Palomar Observatory
Globular cluster M70 in Sagittarius - Globular cluster M70 in Sagittarius - Star cluster located about 29,300 years - light from Earth. Star cluster located at about 29,000 light years away
Globular cluster M68 in Hydra - Globular cluster M68 in Hydr
Galaxy M88 in the Hair of Berenice - Spiral galaxy M88 in Coma Berenices - M88 is a spiral galaxy located in the cluster of the Virgin. Spiral galaxy located in the Virgo cluster of galaxies
Globular cluster M55 in Sagittarius - Globular cluster M55 in Sagittarius - Star cluster located about 17,000 years away from Earth. Star cluster located at about 17,000 light years away
Open cluster M21 in Sagittarius - Open cluster M21 in Sagittarius - The cluster of stars M21 (NGC 6531) is composed of about sixty stars located in the constellation Sagittarius. Image obtained by the Oschin telescope of Mount Palomar through several filters and composed. The open cluster M21, or NGC 6531, in the constellation Sagittarius shows a strong central concentration and a wide range of star brightnesses, despite its limited membership of probably fewer than 60 stars. Most likely quite young (for a star cluster, that means only a few million years), its distance is uncertain. M21 is quite close on the sky to M20, the Trifid Nebula
Alpha Centauri - Alpha Centauri - Alpha Centauri is a double star (Alpha Centauri A and B) near the Sun, 4.36 years - light. These two stars are relatively similar to the Sun. Alpha Centauri is a binary star (Alpha Centauri A and B) located at a distance of 4.36 light - years, or 41 million km, in the direction of the southern constellation Centaurus (The Centaur). Alpha Centauri A and Alpha Centauri B, are rather similar to the Sun; their stellar spectral types are “” G2V”” and “” K1V””, respectively. Alpha Centauri A and B orbit each other at a distance of about 3600 million km, or somewhat more than the distance of planet Uranus from the Sun. The orbital period is almost exactly 80 years
Andromede Galaxy - Detail - The Andromede galaxy is located about 2.3 million years ago - light from Earth. On this composite image obtained by the Hubble Space Telescope (HST), one hundred million stars are visible. M31, the Great galaxy in Andromeda, is a gigantic collection of more than 300 billion stars and is located about 2 million light years from Earth. This image, captured with the NASA/ESA Hubble Space Telescope, is the largest and sharpest image ever taken of the Andromeda galaxy - - otherwise known as M31. It is the biggest Hubble image ever released and shows over 100 million stars and thousands of star clusters embedded in a section of the galaxy's pancake - shaped disc stretching across over 40 000 light - years. Additional data: The Subaru Telescope (NAOJ), DSS, NOA
Open cluster M25 (IC 4725) in Sagittarius - Open cluster M25 (IC 4725) in Sagittarius - Image obtained by the Oschin telescope of Mount Palomar through several filters and composed
Open cluster NGC 5715 in the Compas - Open cluster NGC 5715 in Circinus - Image obtained by the Oschin telescope of Mount Palomar through several filters and composed
Spiral galaxy M101 in the Great Bear - Large field - Wide field view of the Pinwheel Galaxy (M101) - The galaxy M101 (NGC 5457) is located about 27 million years away - light from Earth. It spans more than 170,000 light years, almost double the size of our galaxy. We think that of the trillion stars in it, 100 billion stars could be similar to our Sun. In this image, other galaxies are visible: NGC 5474 (below M101), NGC 5473 (just above M101), NGC 5485 (upper left), NGC 5422 (upper center) and UGC 8837 (near star 86 uA, lower left). Image obtained by the Oschin telescope of Mount Palomar through several filters and composed. Catalogued as M101, the Pinwheel is a nice face - on spiral galaxy. It lies in the northern circumpolar constellation Ursa Major (The Big Bear), at a distance of about 25 million light - years from Earth. The bright blue star at right is 86 Uma, barely visible at the naked eye from a dark site. Also visible some other nice galaxies like NGC 5474 (below under M101), NGC 5473 (just above M101), NGC 5485 (at left edge), NGC 5422 (at top edge) and UGC 8837 (near 86 UMA, the bright star at bottom right). This image is based on data acquired by the Oschin Telescope at the Mount Palomar Observatory
Cometary Globula CG30 in the Stern - Cometary Globule CG30 - Cometary cells are small clouds of isolated gases. These, called CG30/31/38, are located about 1300 light years ago in the constellation Pupus. The Cometary Globules CG 30/31/38 are located 1300 light years away in Vela/Puppis constellations; they appear as finger - like extensions extending out in different directions. Bright rimmed globules and their more evolved cousin the cometary globule represent fascinating dynamic structures formed by the interplay of cold molecular clouds and hot ionizing stars. Typically the head of the globule faces a hot O - type star. The blood cells are known to be the birthplace of low mass stars. The globule head of CG 30 contains the Herbig Haro object HH 120, which is the outflow signature of a pre - main sequence star
Nebula NGC 6334 in Scorpio - Cat's Paw nebula (NGC 6334) in Scorpius - The nebula NGC 6334 is located about 5500 years - light from Earth. It is a vast region of star formation. The Cat's Paw Nebula (NGC 6334) is a vast region of star formation. NGC 6334 lies about 5500 light - years from Earth in the constellation of Scorpius. The whole gas cloud is about 50 light - years across. NGC 6334 is one of the most active nurseries of massive stars in our galaxy and has been extensively studied by astronomers
Field around the galaxy NGC 1672 in the bream - Wide field around galaxy NGC 1672 - The barree spiral galaxy NGC 1672 is located 60 million years - light in the southern constellation of the bream. Intense star formations are observed and many clusters of young stars are visible in the arms of the galaxy. NGC 1672 is a galaxy of Seyfert, whose core houses a supermassive black hole. Wide field ground - based image of NGC 1672's region in the Southern constellation of Dorado. This image is a colour composite taken by the Digitized Sky Survey
Open cluster CR 399 in Little Fox - The Coathanger (CR 399) in Vulpecula - The Hanger cluster or Brocchi cluster is not a true cluster of stars but an asterism in the constellation Little Fox. Image obtained by the Oschin telescope of 1.2m of Mount Palomar through several filters and composed. Cr 399, Brocchi's Cluster, is also known as the “” Coathanger””. It is a distinctive asterism, but not a true star cluster. It is visible to the unaided eye off the head of Cygnus, the Swan in Vulpecula, and resolved into its namesake shape in a telescope or pair of binoculars. Image from Oschin telescope of Palomar observatory
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
Spiral galaxy M33 in the Triangle - Spiral galaxy M33 in Triangulum - M33, (NGC 598), the galaxy of the Triangle, is located about 2 million years ago - light from Earth. It belongs to the local group, just like our galaxy or Andromede galaxy. This image is a composite of two black and white images obtained from the 1.2m telescope of Mount Palomar, California. Spiral galaxy M33 is a mid - sized member of our Local Group of Galaxies. M33 is also called the Triangulum Galaxy for the constellation in which it resides. About four times smaller (in radius) than our Milky Way Galaxy and the Andromeda Galaxy (M31), it is much larger than the many of the local dwarf spheroidal galaxies. M33's proximity to M31 causes it to be thought by some to be a satellite galaxy of this more massive galaxy. M33's proximity to our Milky Way Galaxy causes it to appear more than twice the angular size of the Full Moon, and be visible with a good pair of binoculars. <BR>This image is a composite from black and white images taken with the Palomar Observatory's 48 - inch (1.2 - meter) Samuel Oschin Telescope as a part of the second National Geographic Palomar Observatory Sky Survey (POSS II). The images were recorded on two type of glass photographic plates - one sensitive to red light and the other to blue and later they were digitized
Star HD 209458 in Pegase - Star HD 209458 in Pegasus - This star, located in the center of the image, is about 150 years from Earth and is observable with a pair of binoculars. In orbit around this star, invisible in this image, we discovered a giant planet called Osiris (HD 209458b). This extrasolar planet of a new type is a hot Jupiter, a massive planet very close to its star. The star located in the center of this image is called HD 209458. It is similar to our Sun and lies 150 light - years from Earth. It is visible with binoculars as a seventh magnitude star in the constellation of Pegasus. In orbit around this star (but invisible on this picture) is an exoplanet named Osiris (HD 209458b). It is a hot jupiter, a giant planet orbiting very close to its star
Remains of supernova located about 1400 light years ago in the constellation Swan. The supernova would have exploded less than 10,000 years ago. Image obtained by the Oschin telescope of Mount Palomar through several filters and composed - The Veil Nebula, also known as the Cygnus Loop, is a large supernova remnant, relatively faint supernova remnant in the constellation Cygnus. The source supernova exploded some 5000 to 8000 years ago. The distance to the nebula is not precisely known, with estimates ranging from 1400 to 2600 light years. It was discovered on 1784 September 5 by William Herschel. This image is based on data acquired by the Oschin Telescope at the Mount Palomar Observatory.: Les laces du Swan - The Veil nebula
Galaxy Cluster Abell 1656 - Coma Cluster - Wide - field image around the Coma galaxy cluster - Large field around the Coma galaxy cluster. This cluster consists of about a thousand galaxies and is located 330 million light years away in the constellation Coma Berenices (Berenice hair). This cluster is dominated by two large elliptical galaxies (NGC 4874 on the right and NGC 4889 on the left). Below the middle of the image, to the right, is the galaxy NGC 4921. Mosaic of images obtained by the Oschin telescope of 1.2m from Mount Palomar through several filters and composed. The Coma cluster (Abell 1656) is a particularly rich cluster of individual galaxies (over 1000 members), most prominently the two giant ellipticals, NGC 4874 (right) and NGC 4889 (left). NGC 4921 is the small circular galaxy below and a little to the right of the centre of the image. The remaining members are mostly smaller ellipticals. The cluster is seen towards the constellation Coma Berenices, and is actually at a distance of about 100 Mpc (330 million light years, or a redshift of 0.023) from us. Image based on data acquired by the Oschin Telescope at the Mount Palomar Observatory
Untitled 1973 (DSS 319), 1973 (copper)
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Untitled, 1970 (DSS 219), 1970 (brass)
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Cluster of galaxies Abell 1656 - Coma cluster - The Coma cluster (Abell 1656) - Large cluster of galaxies consists of about a thousand galaxies located 330 million years - light in the constellation of Coma Berenices (Berenice hair). This cluster is dominated by two large elliptical galaxies NGC 4874 on the right and NGC 4889, left. The Coma cluster (Abell 1656) is a particularly rich cluster of individual galaxies (over 1000 members), most prominently the two giant ellipticals, NGC 4874 (right) and NGC 4889 (left). The remaining members are mostly smaller ellipticals. The cluster is seen towards the constellation Coma Berenices, and is actually at a distance of about 100 Mpc (330 million light years, or a redshift of 0.023) from us. Image based on data acquired by the Oschin Telescope at the Mount Palomar Observatory
Spiral Galaxy M31 in Andromede - Spiral galaxy M31 in Andromeda - The galaxy of Andromede is located about 2.3 million years ago - light from Earth. Two satellite galaxies accompany him: M32 (NGC 221) on the left, and M110 (NGC 205) on the lower right. Like the lactee path, the Andromede galaxy belongs to the local group, making up about thirty galaxies. Image based on data obtained with the Oschin telescope of Mount Palomar. Andromeda is the nearest major galaxy to our own Milky Way Galaxy. M31 is about 2.3 million light years far from us in the constellation Andromeda. It is the biggest member in our Local Group. Its diameter is more than 150,000 light years, compared to the Milky Way's 100,000 light years. M31 has two satellite galaxies: M110 (NGC 205) the elliptic galaxy at bottom right respect M31 core and M32 (NGC 221), the bright star - like object just below the M31 core. The bright blue star at top is the 4.5th magnitude nu Andromedae. This image is based on data acquired by the Oschin Telescope at the Mount Palomar Observatory
Nebula California (NGC 1499) in Persee - The California Nebula (NGC 1499) in Perseus - NGC 1499 is a very large emission nebula located 1140 years - light from Earth in the constellation Persee. Image obtained by the Oschin telescope of Mount Palomar through several filters and composed. The north is at top. This is a huge emission nebula in Perseus constellation. It is a cloud of gas, mainly hydrogen, which glows due to the ionization by radiation from a hot nearby star. The California Nebula is made glowing by the 4th magnitude star Menkib (Xi Persei, the bright blue star in center right). The nebula is named because recall the shape of the US state when viewed from the west. This image is based on data acquired by the Oschin Telescope at the Mount Palomar Observatory
Open cluster of Pleiades - Open cluster of Pleiades - The north is at top. The Pleiades star cluster, also known as the Seven Sisters and Messier 45, is one of the brightest and famous star clusters visible in the northern hemisphere. It consists of about 500 bright, hot, young stars that were all born at the same time between 75 and 150 million years ago within a large cloud of dust and gas. The cluster contains many stars, of which only a handful are commonly visible to the naked eye. The blue haze that accompanies them is due to very fine dust which still remains and preferentially reflects the blue light from the stars. This star cluster lies some 440 light years away from the Earth, in the constellation of Taurus. This image is based on data acquired by the Oschin Telescope at the Mount Palomar Observatory
Nebula IC 2177dans la Unicorn - IC 2177 The Seagull nebula - IC 2177, is a large emission nebula located at the edge of the constellations of the Unicorn and the Great Dog. IC 2177, also known as the Eagle or Seagull Nebula, is a large emission nebulosity located on the border between Monoceros and Canis Major, about 7.5 degrees northeast of Sirius. The brightest portion is the “” head”” of the bird, NGC 2327, measuring some 19 x 17 arc minutes, surrounding an 8th magnitude star, and nearly bisected by an interesting dark lane that stretches from the star eastward, and also including some blue reflection nebulosity. Several open clusters are also involved in this area of nebulosity, the most prominent being NGC 2335, located on the northern “” wing”” of the figure of the Seagull nebula
Rosette nebula (NGC 2237) in the Unicorn - The Rosette nebula in Monoceros - The Rosette nebula is a vast cloud of dust and gas. In its center, the cluster of stars NGC 2244. Image obtained by the Oschin telescope of Mount Palomar through several filters and composed. The north is at top. Discovered by John Flamsteed about 1690, the Rosetta Nebula is a vast cloud of dust and gas, extending over an area of more than 1 degree across, or about 5 times the area covered by the full moon. Within the nebula, open star cluster NGC 2244 is situated, consisted of the young stars which recently formed from the nebula's material, and the brightest of which make the nebula shine by exciting its atoms to emit radiation. Star formation is still in progress in this vast cloud of interstellar matter. Although various values for its distance occur in the literature, an avarage value of about 5,500 light - years is generally accepted. This image is based on data acquired by the Oschin Telescope at the Mount Palomar Observatory
Nebula IC 1318 in the Swan - IC 1318 Butterfly nebula in Cygnus - IC 1318 is a very large emission nebula that surrounds the supergiant star Gamma Cygni (Sadr), visible towards the middle of the image. LDN 889 is a vast region of dark nebulae that separates the nebula on the left from Sadr. On the extreme right, another dark nebula, B343. Image obtained by the Oschin telescope of Mount Palomar through several filters and composed. Supergiant star Gamma Cygni lies at the center of the Northern Cross, famous asterism in the constellation Cygnus the Swan. Known by the proper name Sadr, the bright star also lies at the center of this gorgeous skyscape, featuring a complex of stars, dust clouds, and glowing nebulae along the plane of our Milky Way galaxy. The field of view spans over 4 degrees (eight Full Moons) on the sky and includes emission nebula IC 1318 and open star cluster NGC 6910. Left of Gamma Cyg and shaped like two glowing cosmic wings divided by a long dark dust lane, IC 1318's popular name is understandably the Butterfly Nebula. Above and left of Gamma Cyg, are the young, still tightly grouped stars of NGC 6910. Some distance estimates for Gamma Cyg place it at around 750 light - years while estimates for IC 1318 and NGC 6910 range from 2,000 to 5,000 light - years. The color image is based on data coming from a number of different photographic plates taken in 1991 and 1992 by the Palomar Observatory's 48 - inch (1.2 - meter) Samuel Oschin Telescope as a part of the second National Geographic Palomar Observatory Sky Survey (POSS II)
Nebulae around the cluster NGC 2264 and the nebula of the Cone - Wide field around NGC 2264 in Monoceros - Region of star formation located in the constellation of Unicorn about 2700 years old - light from Earth. Image obtained by the Oschin telescope of Mount Palomar through several filters and composed. Wide field around the open cluster NGC 2264 with the brilliant star S Monocerotis (center of the image) and Cone nebula. Image made from 2 different photographic plates taken at Palomar Observatory between 1989 and 1992
Frank Borman visiting a Seguimento DSS 61 space station in Robledo de Chavela near Madrid in Spain
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The Virgo cluster of galaxies - The Virgo cluster of galaxies - The Virgin cluster contains about 2000 galaxies. In the middle of the picture, the giant elliptical galaxy M87. Image obtained by the Oschin telescope of Mount Palomar through several filters and composed. Image of the central portion of the great Virgo/Coma cluster including Markarians chain. Located about 70 million light years away, The Virgo cluster is a gigantic collection of several thousand galaxies that dominate our local part of the universe. Image taken with the Palomar Observatory 48 - inch Schmidt telescope as part of the Digitized Sky Survey
The last Yugoslav President and leader of Democratic Party of Serbia (DSS) Vojislav Kostunica casts .., 2003-12-28 (photo)
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PEOPLE WALK UNDER SNOW COVERED TREES IN SARAJEVO, 1999-02-09 (photo)
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AN OLD LADY AND A YOUNG COUPLE SIT IN THE PARK ON INTERNATIONAL WOMEN'S DAY IN SARAJEVO, 1999-03-08 (photo)
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BOSNIAN ORTHODOX BELIEVERS CELEBRATE EASTER, 2001-04-15 (photo)
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SAMIR MURATOVIC OF BOSNIA FIGHTS FOR BALL WITH ROMANIAN CAP GHEORGHE
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SERBIAN PRIME MINISTER DJINDJIC ARRIVES AT A GOVERNMENT SESSION IN
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