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Bilder zu 'Newton D' gefunden, 3,038

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The Academicians of The Royal Academy in London, copy after a painting by Johann Zoffany (1733-1810), 1773 (watercolour)

The Academicians of The Royal Academy in London, copy after a painting by Johann Zoffany (1733-1810), 1773 (watercolour)

Sanders, John (1768-1826)

DGA500731

Science in Sport, or the Pleasures of Astronomy. A New Game, 1804 (cardboard)

Science in Sport, or the Pleasures of Astronomy. A New Game, 1804 (cardboard)

Wallis, John (19th century)

MMM7339964

The academicians of The Royal Academy in London, copy after a painting by Johann Zoffany (1733-1810), 1773 (watercolour)

The academicians of The Royal Academy in London, copy after a painting by Johann Zoffany (1733-1810), 1773 (watercolour)

Sanders, John (1768-1826)

IBE5388093

Science in Sport, or the Pleasures of Astronomy. A New Game, 1804 (cardboard)

Science in Sport, or the Pleasures of Astronomy. A New Game, 1804 (cardboard)

Wallis, John (19th century)

MMM7339962

Spiral galaxy M33 in the Triangle - Spiral galaxy M33 in Triangulum - M33, the galaxy of the Triangle is located about 2 million years from Earth. It belongs to the local group, just like our galaxy or Andromede galaxy. In red, star-forming regions appear. Image obtained from the Isaac Newton telescope of La Palma. M33 is a large, almost face - on spiral galaxy about 2.5 million light years distant in the northern constellation of Triangulum. It is a member of the 'Local Group' of galaxies, which is dominated by the Milky Way and M31. Like M31, M33 is approaching the Milky Way at a velocity of about 180km/s. Although the total light M33 galaxy is that of a star of magnitude 5.3, its large diameter makes it hard to see. However, despite its low surface brightness, this galaxy was among the first to be identified as a 'spiral nebula' by Lord Rosse in the 1840s. On shorter exposures, the nucleus appears very bright and almost stellar, like that in its southern cousin, NGC 300

Spiral galaxy M33 in the Triangle - Spiral galaxy M33 in Triangulum - M33, the galaxy of the Triangle is located about 2 million years from Earth. It belongs to the local group, just like our galaxy or Andromede galaxy. In red, star-forming regions appear. Image obtained from the Isaac Newton telescope of La Palma. M33 is a large, almost face - on spiral galaxy about 2.5 million light years distant in the northern constellation of Triangulum. It is a member of the 'Local Group' of galaxies, which is dominated by the Milky Way and M31. Like M31, M33 is approaching the Milky Way at a velocity of about 180km/s. Although the total light M33 galaxy is that of a star of magnitude 5.3, its large diameter makes it hard to see. However, despite its low surface brightness, this galaxy was among the first to be identified as a 'spiral nebula' by Lord Rosse in the 1840s. On shorter exposures, the nucleus appears very bright and almost stellar, like that in its southern cousin, NGC 300

PIX4609297

Unidentified lady, early 17th century (watercolour, gum arabic, vellum, gilt)

Unidentified lady, early 17th century (watercolour, gum arabic, vellum, gilt)

Oliver, Isaac (c.1565-1617)

MMM7340109

Spiral galaxy NGC 4651 in Berenice's Hair - Spiral galaxy NGC 4651 in Coma Berenices - The galaxy NGC 4651 (Arp 189) is located about 50 million years away - light from Earth. The Umbrella Galaxy (NGC 4651 or Arp 189) exhibits a jet like spear that's strikingly coherent and narrow. The structure was previously reported by Boris Vorontsov Velyaminov in 1959 but never interpreted as a stellar tidal stream. This deep image additionally shows a spectacular crescent shaped shell surrounding the east side of the star system that corresponds to the apocenter of the dwarf galaxy. Interestingly, a possible second arc on the western side of the galaxy can also be seen in this image. This feature is less obvious because it's partially hidden by the galaxy's disk and suggests we are observing a moderately inclined structure projected into the halo of NGC 4651. This image was produced by combining an hour of exposure through the Isaac Newton Telescope, located on the Spanish island of La Palma, wit

Spiral galaxy NGC 4651 in Berenice's Hair - Spiral galaxy NGC 4651 in Coma Berenices - The galaxy NGC 4651 (Arp 189) is located about 50 million years away - light from Earth. The Umbrella Galaxy (NGC 4651 or Arp 189) exhibits a jet like spear that's strikingly coherent and narrow. The structure was previously reported by Boris Vorontsov Velyaminov in 1959 but never interpreted as a stellar tidal stream. This deep image additionally shows a spectacular crescent shaped shell surrounding the east side of the star system that corresponds to the apocenter of the dwarf galaxy. Interestingly, a possible second arc on the western side of the galaxy can also be seen in this image. This feature is less obvious because it's partially hidden by the galaxy's disk and suggests we are observing a moderately inclined structure projected into the halo of NGC 4651. This image was produced by combining an hour of exposure through the Isaac Newton Telescope, located on the Spanish island of La Palma, wit

R. Jay GaBany

PIX4611786

Center of the Andromede Galaxy (M31) - Center of the Andromeda galaxy - The Andromede galaxy is located about 2 million years ago - light from Earth. Like the lactee path, the Andromede galaxy belongs to the local group. This image obtained from the 2.5m Isaac Newton telescope of La Palma shows the nucleus of the galaxy. This nucleus is double, probably the vestige of a collision with another galaxy. At the heart of the nearby spiral galaxy M31 is a tiny, bright nucleus, seen to be slightly elongated on this colour picture. Hubble Space Telescope pictures show the nucleus to be a double structure, possibly the remains of the nucleus of another galaxy which has now been almost completely absorbed in M31. Around the binary nucleus swirls a huge cloud of mostly old, faint stars. This not only reveals the inner nucleus but also shows traces of dust which seem to stream into the bright central part of the galaxy. Studies of the stars around the nucleus strongly suggest that at the heart of

Center of the Andromede Galaxy (M31) - Center of the Andromeda galaxy - The Andromede galaxy is located about 2 million years ago - light from Earth. Like the lactee path, the Andromede galaxy belongs to the local group. This image obtained from the 2.5m Isaac Newton telescope of La Palma shows the nucleus of the galaxy. This nucleus is double, probably the vestige of a collision with another galaxy. At the heart of the nearby spiral galaxy M31 is a tiny, bright nucleus, seen to be slightly elongated on this colour picture. Hubble Space Telescope pictures show the nucleus to be a double structure, possibly the remains of the nucleus of another galaxy which has now been almost completely absorbed in M31. Around the binary nucleus swirls a huge cloud of mostly old, faint stars. This not only reveals the inner nucleus but also shows traces of dust which seem to stream into the bright central part of the galaxy. Studies of the stars around the nucleus strongly suggest that at the heart of

PIX4608823

Spiral Galaxy M33 in the Triangle - Spiral galaxy M33 in Triangulum - The Galaxy of the Triangle (M33, NGC598) is located about 2 million years ago - light from Earth. It belongs to the local group, just like our galaxy or Andromede galaxy. In red, the star-forming regions appear, especially at the top left NGC 604 one of the largest and most active star-forming regions. It extends over 150 years of light. Image obtained from the Isaac Newton telescope of La Palma. M33 is a large, almost face - on spiral galaxy about 2.5 million light years distant in the northern constellation of Triangulum. It is a member of the 'Local Group' of galaxies, which is dominated by the Milky Way and M31. Like M31, M33 is approaching the Milky Way at a velocity of about 180km/s. Although the total light M33 galaxy is that of a star of magnitude 5.3, its large diameter makes it hard to see. However, despite its low surface brightness, this galaxy was among the first to be identified as a 'spiral nebula' by

Spiral Galaxy M33 in the Triangle - Spiral galaxy M33 in Triangulum - The Galaxy of the Triangle (M33, NGC598) is located about 2 million years ago - light from Earth. It belongs to the local group, just like our galaxy or Andromede galaxy. In red, the star-forming regions appear, especially at the top left NGC 604 one of the largest and most active star-forming regions. It extends over 150 years of light. Image obtained from the Isaac Newton telescope of La Palma. M33 is a large, almost face - on spiral galaxy about 2.5 million light years distant in the northern constellation of Triangulum. It is a member of the 'Local Group' of galaxies, which is dominated by the Milky Way and M31. Like M31, M33 is approaching the Milky Way at a velocity of about 180km/s. Although the total light M33 galaxy is that of a star of magnitude 5.3, its large diameter makes it hard to see. However, despite its low surface brightness, this galaxy was among the first to be identified as a 'spiral nebula' by

PIX4609292

Exterior of Quad Gallery, Derby, UK (photo)

Exterior of Quad Gallery, Derby, UK (photo)

ARD2538874

The Hepworth Wakefield, West Yorkshire, UK (photo)

The Hepworth Wakefield, West Yorkshire, UK (photo)

ARD2539668

Galaxy NGC 891 in Andromede - Edge - on spiral galaxy NGC 891 in Andromeda - Spiral galaxy seen by the slice located at a distance of 10 million years - light.. This image obtained with the 2.5m Isaac Newton telescope of La Palma. If we could view the Milky Way from a distance of about 30 million light years it would look something like NGC 891. But galaxies that look like this are quite rare because the chance alignment of the thin disk of a spiral galaxy with our line of sight is unusual. A few degrees either side of its orientation and NGC 891 would be just another highly inclined spiral galaxy. From this unusual vantage point we can see in NGC 891 the surprising narrowness of the obscuring dust lane, a dark, slightly irregular band across the galaxy. We also see that it is yellowish, confirming that it is dust, which absorbs blue light, as in the Milky Way. Also similar to the Milky Way is the prominent central 'bulge' corresponding to the rich star clouds in Sagittarius. However,

Galaxy NGC 891 in Andromede - Edge - on spiral galaxy NGC 891 in Andromeda - Spiral galaxy seen by the slice located at a distance of 10 million years - light.. This image obtained with the 2.5m Isaac Newton telescope of La Palma. If we could view the Milky Way from a distance of about 30 million light years it would look something like NGC 891. But galaxies that look like this are quite rare because the chance alignment of the thin disk of a spiral galaxy with our line of sight is unusual. A few degrees either side of its orientation and NGC 891 would be just another highly inclined spiral galaxy. From this unusual vantage point we can see in NGC 891 the surprising narrowness of the obscuring dust lane, a dark, slightly irregular band across the galaxy. We also see that it is yellowish, confirming that it is dust, which absorbs blue light, as in the Milky Way. Also similar to the Milky Way is the prominent central 'bulge' corresponding to the rich star clouds in Sagittarius. However,

PIX4609481

Galaxy NGC 891 in Andromede - Edge - on spiral galaxy NGC 891 in Andromeda - Spiral galaxy seen by the slice located at a distance of 10 million years - light. This image was obtained with the Isaac Newton 2.5m telescope of La Palma. If we could view the Milky Way from a distance of about 30 million light years it would look something like NGC 891. But galaxies that look like this are quite rare because the chance alignment of the thin disk of a spiral galaxy with our line of sight is unusual. A few degrees either side of its orientation and NGC 891 would be just another highly inclined spiral galaxy. From this unusual vantage point we can see in NGC 891 the surprising narrowness of the obscuring dust lane, a dark, slightly irregular band across the galaxy. We also see that it is yellowish, confirming that it is dust, which absorbs blue light, as in the Milky Way. Also similar to the Milky Way is the prominent central 'bulge' corresponding to the rich star clouds in Sagittarius. Howeve

Galaxy NGC 891 in Andromede - Edge - on spiral galaxy NGC 891 in Andromeda - Spiral galaxy seen by the slice located at a distance of 10 million years - light. This image was obtained with the Isaac Newton 2.5m telescope of La Palma. If we could view the Milky Way from a distance of about 30 million light years it would look something like NGC 891. But galaxies that look like this are quite rare because the chance alignment of the thin disk of a spiral galaxy with our line of sight is unusual. A few degrees either side of its orientation and NGC 891 would be just another highly inclined spiral galaxy. From this unusual vantage point we can see in NGC 891 the surprising narrowness of the obscuring dust lane, a dark, slightly irregular band across the galaxy. We also see that it is yellowish, confirming that it is dust, which absorbs blue light, as in the Milky Way. Also similar to the Milky Way is the prominent central 'bulge' corresponding to the rich star clouds in Sagittarius. Howeve

PIX4609474

Harbor of Boston, with the City in the Distance, c.1846-47 (oil on canvas)

Harbor of Boston, with the City in the Distance, c.1846-47 (oil on canvas)

Lane, Fitz Henry (1804-65)

XCL500339

Liquid mirror telescope on the Moon - Lunar liquid mirror telescope - Illustration of an astronomical observatory on the Moon. Installs near the southern pole of the Moon, a giant telescope with liquid mirror, one kilometre in diameter. A giant liquid mirror telescope 1 kilometer wide (6 tenths of a mile) and 1 kilometer tall lies nestled in an approximately 1 kilometer wide crater near the Moon's south pole. In the foreground is a kind of lunar city for human habitation composed of pressurized and radiation-hardened living units. On the upper right are landing pads for transports arriving to and departing from the lunar surface. A liquid mirror telescope is a Newtonian reflecting type telescope that employs a reflecting liquid as the primary mirror. A concept first identified 300 years ago by Isaac Newton himself, the reflecting liquid assumes the proper paraboloidal shape by rotating the container the liquid is in. On Earth working liquid mirror telescopes have been created with diam

Liquid mirror telescope on the Moon - Lunar liquid mirror telescope - Illustration of an astronomical observatory on the Moon. Installs near the southern pole of the Moon, a giant telescope with liquid mirror, one kilometre in diameter. A giant liquid mirror telescope 1 kilometer wide (6 tenths of a mile) and 1 kilometer tall lies nestled in an approximately 1 kilometer wide crater near the Moon's south pole. In the foreground is a kind of lunar city for human habitation composed of pressurized and radiation-hardened living units. On the upper right are landing pads for transports arriving to and departing from the lunar surface. A liquid mirror telescope is a Newtonian reflecting type telescope that employs a reflecting liquid as the primary mirror. A concept first identified 300 years ago by Isaac Newton himself, the reflecting liquid assumes the proper paraboloidal shape by rotating the container the liquid is in. On Earth working liquid mirror telescopes have been created with diam

Walter B Myers

PIX4639385

Red Dwarf Star Proxima of Centauri - Proxima Centauri in X - Ray - Proxima of Centaur (in the center of the image) is the closest star to the Sun, at a distance of 4.2 years - light. It belongs to the triple Alpha star system of the Centaurus being the least bright star of this system; it is a red dwarf star. X-ray image obtained by the Chandra space telescope. Chandra and XMM - Newton observations of the red dwarf star Proxima Centauri have shown that its surface is in a state of turmoil. Flares, or explosive outbursts, occur almost continually. This behavior can be traced to Proxima Centauri's low mass, about a tenth that of the Sun. In the cores of low mass stars, nuclear fusion reactions that convert hydrogen to helium proceed very slowly, and create a turbulent, convective motion throughout their interiors. This motion stores up magnetic energy which is often released explosively in the star's upper atmosphere where it produces flares in X - rays and other forms of light. The same

Red Dwarf Star Proxima of Centauri - Proxima Centauri in X - Ray - Proxima of Centaur (in the center of the image) is the closest star to the Sun, at a distance of 4.2 years - light. It belongs to the triple Alpha star system of the Centaurus being the least bright star of this system; it is a red dwarf star. X-ray image obtained by the Chandra space telescope. Chandra and XMM - Newton observations of the red dwarf star Proxima Centauri have shown that its surface is in a state of turmoil. Flares, or explosive outbursts, occur almost continually. This behavior can be traced to Proxima Centauri's low mass, about a tenth that of the Sun. In the cores of low mass stars, nuclear fusion reactions that convert hydrogen to helium proceed very slowly, and create a turbulent, convective motion throughout their interiors. This motion stores up magnetic energy which is often released explosively in the star's upper atmosphere where it produces flares in X - rays and other forms of light. The same

PIX4571790

Turning Out the Light, 1905 (etching)

Turning Out the Light, 1905 (etching)

Sloan, John (1871-1951)

PHL2910120

Planetary nebula NGC 6543 dans le Dragon/HST - The nebula, formally cataloged NGC 6543 was one of the first planetary nebulae to be discovered; it is one of the most complex such nebulae seen in space. A planetary nebula forms when Sun - like stars gently eject their outer gaseous layers that form bright nebulae with amazing and confounding shapes. In 1994, Hubble first revealed NGC 6543's surprisingly intricate structures, including concentric gas shells, jets of high - speed gas, and unusual shock - induced knots of gas. As if the Cat's Eye itself isn't spectacular enough, this new image taken with Hubble's Advanced Camera for Surveys (ACS) reveals the full beauty of a bull's eye pattern of eleven or even more concentric rings, or shells, around the Cat's Eye. Each 'ring' is actually the edge of a spherical bubble seen projected onto the sky - - that's why it appears bright along its outer edge. Observations suggest the star ejected its mass in a series of pulses at 1,500 - year inte

Planetary nebula NGC 6543 dans le Dragon/HST - The nebula, formally cataloged NGC 6543 was one of the first planetary nebulae to be discovered; it is one of the most complex such nebulae seen in space. A planetary nebula forms when Sun - like stars gently eject their outer gaseous layers that form bright nebulae with amazing and confounding shapes. In 1994, Hubble first revealed NGC 6543's surprisingly intricate structures, including concentric gas shells, jets of high - speed gas, and unusual shock - induced knots of gas. As if the Cat's Eye itself isn't spectacular enough, this new image taken with Hubble's Advanced Camera for Surveys (ACS) reveals the full beauty of a bull's eye pattern of eleven or even more concentric rings, or shells, around the Cat's Eye. Each 'ring' is actually the edge of a spherical bubble seen projected onto the sky - - that's why it appears bright along its outer edge. Observations suggest the star ejected its mass in a series of pulses at 1,500 - year inte

PIX4623222

Galaxy NGC 4631 in Hunting Dogs - Spiral galaxy NGC 4631 in Canes Venatici - Spiral galaxy seen by the slice located at a distance of 30 million years - light. Image obtained by the Hubble Space Telescope (HST). The NASA/ESA Hubble Space Telescope has peered deep into NGC 4631, better known as the Whale Galaxy. Here, a profusion of starbirth lights up the galactic centre, revealing bands of dark material between us and the starburst. The galaxy's activity tapers off in its outer regions where there are fewer stars and less dust, but these are still punctuated by pockets of star formation. The Whale Galaxy is about 30 million light - years away from us in the constellation of Canes Venatici (The Hunting Dogs) and is a spiral galaxy much like the Milky Way. From our vantage point, however, we see the Whale Galaxy edge - on, seeing its glowing centre through dusty spiral arms. The galaxy's central bulge and asymmetric tapering disc have suggested the shape of a whale or a herring to past

Galaxy NGC 4631 in Hunting Dogs - Spiral galaxy NGC 4631 in Canes Venatici - Spiral galaxy seen by the slice located at a distance of 30 million years - light. Image obtained by the Hubble Space Telescope (HST). The NASA/ESA Hubble Space Telescope has peered deep into NGC 4631, better known as the Whale Galaxy. Here, a profusion of starbirth lights up the galactic centre, revealing bands of dark material between us and the starburst. The galaxy's activity tapers off in its outer regions where there are fewer stars and less dust, but these are still punctuated by pockets of star formation. The Whale Galaxy is about 30 million light - years away from us in the constellation of Canes Venatici (The Hunting Dogs) and is a spiral galaxy much like the Milky Way. From our vantage point, however, we see the Whale Galaxy edge - on, seeing its glowing centre through dusty spiral arms. The galaxy's central bulge and asymmetric tapering disc have suggested the shape of a whale or a herring to past

PIX4611784

Two Women of the Marquesas Islands, c.1902 (monotype)

Two Women of the Marquesas Islands, c.1902 (monotype)

Gauguin, Paul (1848-1903)

PHL3597107

Mrs. Herbert Duckworth, 1867 (albumen silver print)

Mrs. Herbert Duckworth, 1867 (albumen silver print)

Cameron, Julia Margaret (1815-79)

PHL450461

Sharecropper, 1952 (linocut)

Sharecropper, 1952 (linocut)

Catlett, Elizabeth (1915-2012)

PHL451127

Self Portrait (oil on canvas)

Self Portrait (oil on canvas)

Pickersgill, Henry William (1782-1875)

SYD250437

Countess Shannon, 18th century (oil on canvas)

Countess Shannon, 18th century (oil on canvas)

Cotes, Francis (1726-70) (attr. to)

MAM712819

Portrait of Madame Franc-Nohain, c.1905 (oil on canvas)

Portrait of Madame Franc-Nohain, c.1905 (oil on canvas)

Bonnard, Pierre (1867-1947)

PHL434610

Wellington Harbour, 1894 (oil on panel)

Wellington Harbour, 1894 (oil on panel)

Nairn, James McLachlan (1859-1904)

TEP352936

"I Rose Up in the Silent Night; I made my Dagger Sharp and Bright", c. 1859-60 (pen & ink over graphite with touches of heightening on ivory wove paper)

"I Rose Up in the Silent Night; I made my Dagger Sharp and Bright", c. 1859-60 (pen & ink over graphite with touches of heightening on ivory wove paper)

Burne-Jones, Edward Coley (1833-98)

PHL450911

Tess, 1893 (oil on canvas)

Tess, 1893 (oil on canvas)

Nairn, James McLachlan (1859-1904)

TEP352914

The Pulpit of the Cathedral of Saint-André in Bordeaux, 1907 (transparent & opaque w/c, with black chalk, on heavy wove paper)

The Pulpit of the Cathedral of Saint-André in Bordeaux, 1907 (transparent & opaque w/c, with black chalk, on heavy wove paper)

Boldini, Giovanni (1842-1931)

PHL450932

Cartoon for "The Liberation of the Peon", c.1931 (charcoal & graphite on paper mounted on canvas)

Cartoon for "The Liberation of the Peon", c.1931 (charcoal & graphite on paper mounted on canvas)

Rivera, Diego (1886-1957)

HST1075181

The Vanishing Race Navaho Plate 1, Volume 1 from the series The North American Indian, c. 1904 (orotone)

The Vanishing Race Navaho Plate 1, Volume 1 from the series The North American Indian, c. 1904 (orotone)

Curtis, Edward Sheriff (1868-1952)

HST2634109

Portrait of the Bertolini Son, 1914 (graphite & black crayon, on beige wove paper, mounted down)

Portrait of the Bertolini Son, 1914 (graphite & black crayon, on beige wove paper, mounted down)

Gemito, Vincenzo (1852-1929)

PHL451084

Portrait of Laura Bertolini, 1913 (graphite & black crayon, on beige wove paper, mounted down)

Portrait of Laura Bertolini, 1913 (graphite & black crayon, on beige wove paper, mounted down)

Gemito, Vincenzo (1852-1929)

PHL451083

Marilyn, 1967 (color photoscreenprint & color screenprint)

Marilyn, 1967 (color photoscreenprint & color screenprint)

Warhol, Andy (1928-87)

PHL441744

General Z. Taylor (Rough and Ready), 1846 (lithograph)

General Z. Taylor (Rough and Ready), 1846 (lithograph)

Sarony & Major (fl.1846-1857)

HST2634413

Cambridge, England

Cambridge, England

Doughty, C.L. (1913-85)

LAL295325

Elysium and Sartarus or the State of Final Retribution, 1791 (etching)

Elysium and Sartarus or the State of Final Retribution, 1791 (etching)

Barry, James (1741-1806)

XYC291021

Elysium, or the State of Final Retribution, sixth in the series 'The Progress of Human Culture and Knowledge', c.1777-84 (oil on canvas) (see 101467 and 101468)

Elysium, or the State of Final Retribution, sixth in the series 'The Progress of Human Culture and Knowledge', c.1777-84 (oil on canvas) (see 101467 and 101468)

Barry, James (1741-1806)

RSA101465

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