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Images of 'Jaune' found, 22,771

 
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Marmion Edward Ferrers (1813-1884): 'The squire's evening walk'

Orpen, Rebecca Dulcibella (1830-1923)

USB1160587

Marmion Edward Ferrers (1813-1884): 'The squire's evening walk'

Orpen, Rebecca Dulcibella (1830-1923)

USB1160587

 
The elliptical galaxy M84 - The elliptical galaxy M84 - The M84 galaxy (NGC 4374) is 55 million light years away from Earth, in the Virgin's cluster. This image is a composite obtained in X-rays (blue), radio (red) and visible (yellow and white). Gas material is ejected from the heart of the galaxy. A supermassive black hole would have caused this jet. This composite image shows M84, a massive elliptical galaxy in the Virgo Cluster, about 55 million light years from Earth. Hot gas around M84 is shown in a Chandra X - ray Observatory image in blue and a radio image from the Very Large Array is shown in red. A background image from the Sloan Digital Sky Survey is shown in yellow and white. A number of bubbles are visible in the hot gas, outlined with blue X - ray emission. These bubbles were blown by relativistic particles generated by the central supermassive black hole in M84. These particles travel outwards in the form of a two - sided jet. Because smaller bubbles are found inside lar

PIX4611313

The elliptical galaxy M84 - The elliptical galaxy M84 - The M84 galaxy (NGC 4374) is 55 million light years away from Earth, in the Virgin's cluster. This image is a composite obtained in X-rays (blue), radio (red) and visible (yellow and white). Gas material is ejected from the heart of the galaxy. A supermassive black hole would have caused this jet. This composite image shows M84, a massive elliptical galaxy in the Virgo Cluster, about 55 million light years from Earth. Hot gas around M84 is shown in a Chandra X - ray Observatory image in blue and a radio image from the Very Large Array is shown in red. A background image from the Sloan Digital Sky Survey is shown in yellow and white. A number of bubbles are visible in the hot gas, outlined with blue X - ray emission. These bubbles were blown by relativistic particles generated by the central supermassive black hole in M84. These particles travel outwards in the form of a two - sided jet. Because smaller bubbles are found inside lar

PIX4611313

 
Crocodile, Chobe National Park, Botswana (photo)

Sergi Reboredo

SRB1202619

Crocodile, Chobe National Park, Botswana (photo)

Sergi Reboredo

SRB1202619

 
Waterfalls Popokvil, Bokor National Park, Cambodia (photo)

Sergi Reboredo

SRB1202734

Waterfalls Popokvil, Bokor National Park, Cambodia (photo)

Sergi Reboredo

SRB1202734

 
Open cluster NGC 6242 in Scorpio - Open star cluster NGC 6242 in Scorpius - This cluster is about 3500 years old - light from the Sun and is about 50 million years old. A bright yellow star is in the foreground. This cluster is one of many in the sparkling southern constellation of Scorpius. It is marked by a bright yellow star (spectral type K5) which happens to be in the foreground at a distance of about 1000 light years. The cluster itself is about 3,500 light years from the sun. The cluster is slightly dimmed by foreground dust. This so - called interstellar extinction is common with object close to the Galactic plane. Despite this, it is possible to estimate the age of the cluster by measuring the color and relative brightness of its stars. The age turns out to be about 50 million years, which is quite mature for an open cluster of this type. By now, most of the brightest stars will have turned into supernovae and vanished, leaving this quite modest group to compete with the many

PIX4568311

Open cluster NGC 6242 in Scorpio - Open star cluster NGC 6242 in Scorpius - This cluster is about 3500 years old - light from the Sun and is about 50 million years old. A bright yellow star is in the foreground. This cluster is one of many in the sparkling southern constellation of Scorpius. It is marked by a bright yellow star (spectral type K5) which happens to be in the foreground at a distance of about 1000 light years. The cluster itself is about 3,500 light years from the sun. The cluster is slightly dimmed by foreground dust. This so - called interstellar extinction is common with object close to the Galactic plane. Despite this, it is possible to estimate the age of the cluster by measuring the color and relative brightness of its stars. The age turns out to be about 50 million years, which is quite mature for an open cluster of this type. By now, most of the brightest stars will have turned into supernovae and vanished, leaving this quite modest group to compete with the many

PIX4568311

 
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Saxony, historical, GDR, Trade, Retail trade, Care, Businesses, department …, 1985 (photo)

Sächsische Zeitung

IMO8758618

Saxony, historical, GDR, Trade, Retail trade, Care, Businesses, department …, 1985 (photo)

Sächsische Zeitung

IMO8758618

 
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Called The Hon. Harriet Molesworth, The Hon. Mrs John Staples (1745-1812) but most probably Harriett Conolly, Mrs. John Staples (d.1771)

Cotes, Francis (1726-70)

USB1158476

Called The Hon. Harriet Molesworth, The Hon. Mrs John Staples (1745-1812) but most probably Harriett Conolly, Mrs. John Staples (d.1771)

Cotes, Francis (1726-70)

USB1158476

 
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Staircase in a Palace

Spanish School, (19th century)

USB1159677

Staircase in a Palace

Spanish School, (19th century)

USB1159677

 
Black hole collision in NGC 6240 - Black holes colliding in NGC 6240 - The galaxy NGC 6240, is located about 400 million light years away from Earth in the constellation Ophiuchus. This system consists of two colliding galaxies each with a central black hole; in several millions of years, they will form only one galaxy. A composite X-ray image (red, orange and yellow) and visible from the space telescopes Chandra and Hubble. This image of NGC 6240 contains X - ray data from Chandra (shown in red, orange, and yellow) that has been combined with an optical image from the Hubble Space Telescope. In 2002, the discovery of two merging black holes was announced based on Chandra data in this galaxy. The two black holes are a mere 3,000 light years apart and are seen as the bright point - like sources in the middle of the image. Scientists think these black holes are in such close proximity because they are in the midst of spiraling toward each other - a process that began about 30 million yea

PIX4612910

Black hole collision in NGC 6240 - Black holes colliding in NGC 6240 - The galaxy NGC 6240, is located about 400 million light years away from Earth in the constellation Ophiuchus. This system consists of two colliding galaxies each with a central black hole; in several millions of years, they will form only one galaxy. A composite X-ray image (red, orange and yellow) and visible from the space telescopes Chandra and Hubble. This image of NGC 6240 contains X - ray data from Chandra (shown in red, orange, and yellow) that has been combined with an optical image from the Hubble Space Telescope. In 2002, the discovery of two merging black holes was announced based on Chandra data in this galaxy. The two black holes are a mere 3,000 light years apart and are seen as the bright point - like sources in the middle of the image. Scientists think these black holes are in such close proximity because they are in the midst of spiraling toward each other - a process that began about 30 million yea

PIX4612910

 
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Saint Elizabeth of Portugal (1271-1336)

Zurbaran, Francisco de (1598-1664) (studio of)

USB1156939

Saint Elizabeth of Portugal (1271-1336)

Zurbaran, Francisco de (1598-1664) (studio of)

USB1156939

 
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Margaret Gerard, Lady Legh (m. 1584 - d. 1603)

Geeraerts, Marcus, the younger (1561-1635) (manner of)

USB1157332

Margaret Gerard, Lady Legh (m. 1584 - d. 1603)

Geeraerts, Marcus, the younger (1561-1635) (manner of)

USB1157332

 
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Morning dresses. "Two Ladies, en neglige, taking an airing in a phaeton." They wear plain calico morning dresses and ribbon and feather-trimmed bonnets with ostrich feathers. Description of the left figure reads: "Headdress: white stamp- paper hat, trimmed with a green riband and tied down with the same. One green and one yellow feather placed on the left side. Green gauze veil. The hair in small curls; plain chignon. Plain calico morning dress with long sleeves; the petticoat trimmed with a narrow flounce. Plain lawn handkerchief, green sash, lawn cloak trimmed with lace and tied behind, york tan gloves, yellow shoes." Description of the right figure reads: "Headdress: straw-coloured hat, trimmed with orange and purple ribands, and a white lawn handkerchief, embroidered in lilac, tied down with a white riband. One lilac and white cross-striped large ostrich feather on the left side, the hair in light curls and hanging down in ringlets behind, bound with a half-handkerchief tied into

BL3294763

Morning dresses. "Two Ladies, en neglige, taking an airing in a phaeton." They wear plain calico morning dresses and ribbon and feather-trimmed bonnets with ostrich feathers. Description of the left figure reads: "Headdress: white stamp- paper hat, trimmed with a green riband and tied down with the same. One green and one yellow feather placed on the left side. Green gauze veil. The hair in small curls; plain chignon. Plain calico morning dress with long sleeves; the petticoat trimmed with a narrow flounce. Plain lawn handkerchief, green sash, lawn cloak trimmed with lace and tied behind, york tan gloves, yellow shoes." Description of the right figure reads: "Headdress: straw-coloured hat, trimmed with orange and purple ribands, and a white lawn handkerchief, embroidered in lilac, tied down with a white riband. One lilac and white cross-striped large ostrich feather on the left side, the hair in light curls and hanging down in ringlets behind, bound with a half-handkerchief tied into

BL3294763

 
Permissions
  • Permission required for non-editorial use (inc book and magazine covers). Please contact us
Apollo crowning a Poet and joining him with a Consort, witnessed by Hercules and by four other Females

Tintoretto, Jacopo Robusti (1518-94)

USB1157020

Apollo crowning a Poet and joining him with a Consort, witnessed by Hercules and by four other Females

Tintoretto, Jacopo Robusti (1518-94)

USB1157020

 
Remains of supernova SN 1006 - Supernova remnant SN 1006 - Remains of supernova SN 1006 located 7000 years ago - light in the constellation Wolf. This supernova that appeared in 1006 is the result of a white dwarf star that absorbs the matter of a companion star became unstable and eventually exploded. This image is a composite of X-ray images obtained by the Chandra telescope (blue), by Cerro Tololo's 90 cm telescope (yellow) and by the Digitized Sky Survey (orange and light blue), and by the VLA and the Green Bank's telescope radio (red). Just over a thousand years ago, the stellar explosion known as supernova SN 1006 was observed. It was brighter than Venus, and visible during the day for weeks. The brightest supernova ever recorded on Earth, this spectacular light show was documented in China, Japan, Europe, and the Arab world. Astronomers now understand that SN 1006 was caused by a white dwarf star that captured mass from a companion star until the white dwarf became unstable and

PIX4583213

Remains of supernova SN 1006 - Supernova remnant SN 1006 - Remains of supernova SN 1006 located 7000 years ago - light in the constellation Wolf. This supernova that appeared in 1006 is the result of a white dwarf star that absorbs the matter of a companion star became unstable and eventually exploded. This image is a composite of X-ray images obtained by the Chandra telescope (blue), by Cerro Tololo's 90 cm telescope (yellow) and by the Digitized Sky Survey (orange and light blue), and by the VLA and the Green Bank's telescope radio (red). Just over a thousand years ago, the stellar explosion known as supernova SN 1006 was observed. It was brighter than Venus, and visible during the day for weeks. The brightest supernova ever recorded on Earth, this spectacular light show was documented in China, Japan, Europe, and the Arab world. Astronomers now understand that SN 1006 was caused by a white dwarf star that captured mass from a companion star until the white dwarf became unstable and

PIX4583213

 
Star Formation in the DR21 Region - Star Formation in the DR21 Region - This star formation region is about 6200 years old - light. Hidden in light visible by interstellar dust, this region rises in infrared light. Gas filaments appear in red; they emphasize the presence of aromatic polycyclic hydrocarbons (PAH); they are organic molecules composed of carbon atoms and hydrogen that could be the germs on which the first bricks of life appeared. Composite image in different wavelengths obtained by the Spitzer space telescope; in blue the visible light, in yellow and red the infrared light. Hidden behind a shroud of dust in the constellation Cygnus is a stellar nursery called DR21, which is giving birth to some of the most massive stars in our galaxy. Visible light images reveal no trace of this interstellar cauldron because of heavy dust obscuration. This image from Nasa's Spitzer Space Telescope allow us to peek behind the cosmic veil and pinpoint one of the most massive natal stars yet

PIX4621115

Star Formation in the DR21 Region - Star Formation in the DR21 Region - This star formation region is about 6200 years old - light. Hidden in light visible by interstellar dust, this region rises in infrared light. Gas filaments appear in red; they emphasize the presence of aromatic polycyclic hydrocarbons (PAH); they are organic molecules composed of carbon atoms and hydrogen that could be the germs on which the first bricks of life appeared. Composite image in different wavelengths obtained by the Spitzer space telescope; in blue the visible light, in yellow and red the infrared light. Hidden behind a shroud of dust in the constellation Cygnus is a stellar nursery called DR21, which is giving birth to some of the most massive stars in our galaxy. Visible light images reveal no trace of this interstellar cauldron because of heavy dust obscuration. This image from Nasa's Spitzer Space Telescope allow us to peek behind the cosmic veil and pinpoint one of the most massive natal stars yet

PIX4621115

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