'Creating' Bilder und Clips Suchergebnisse

Mars: Valles Marineris - Mosaic of 20 images obtained by the European probe Mars Express. This image shows the eastern part of Valles Marineris, a canyon about 4500 km long and 8 km deep. This mosaic image of eastern part of Valles Marineris - colored to resemble the martian surface - comes from Esa's Mars Express spacecraft, which repeatedly crosses the Martian equator from north to south or south to north. The High Resolution Stereo Camera (HRSC) on board Mars Express, has been taking image strips of the valley system since 2004 as it passes overhead. The individual HRSC image strips are each between 50 and 200 kilometers wide, depending on Mars Express' orbit, so this view of Valles Marineris has only been made possible by creating a mosaic using 20 separate images. To improve the presentation here, the altitudes have been exaggerated fourfold, so that the slopes and mountainsides appear steeper than they are in reality. The colours in this image are slightly false as well. By incre

PIX4616253

Impact on the Moon at the Cretace - Cretaceous lunar strike - Artist's view of an asteroid impact on the Moon illuminating a nocturnal landscape of the cretace. In the foreground, a spinosaur, a theropod dinosaur who lived in what is now Egypt 95 to 93 million years ago. What may appear here as a diamond ring effect from a solar eclipse is in fact a brilliant and momentary flash of light signaling a massive asteroid impact on the Moon. The Moon and all the inner planets of the Solar System show evidence of a long and violent history of encounters with meteorites and asteroids - leftover debris from the formation of the Solar System. This image depicts an asteroid colliding with the Moon about 95 million years ago. The perspective is from the surface of the Earth in what today is Egypt. The impact would have released millions of times more energy than today's largest nuclear weapon, creating a flash of light that would be far brighter than any star in the sky. In the foreground of this

Walter B Myers

PIX4662978

Six Senses Resort, Koh Yao Noi, Phang Nga Bay, Thailand, Asia (photo)

Sergi Reboredo

SRB3585107

The Horse Fair, late 1660s (oil on mahogany panel)

Wouwermans or Wouwerman, Philips (1619-68)

TWC5894926

St. Peter of Alcántara, c.1663-1670 (painted wood, with ivory and glass)

Mena, Pedro de (1628-88)

XCL500419

Star Formation in the dwarf galaxy NGC 1569 - Starburst galaxy NGC 1569 - NGC 1569 is a dwarf irregular galaxy in the constellation Giraffe. The Hubble space telescope measured its distance with precision, placing it 11 million years - light from Earth, or 4 million years - light beyond the distance previously established by astronomers. This new measure explains better why this galaxy has a particularly high star formation rate. It resides among a group of galaxies that by gravity compresses its gas, thus creating a hundred times more stars than in our own galaxy. NGC 1569 is located in the middle of a group of about 10 galaxies centered on the spiral galaxy IC 342. Gravitational interactions among the group's galaxies may be compressing gas in NGC 1569 and igniting the star - birthing frenzy. The galaxy is forming stars at a rate more than 100 times higher than the rate in the Milky Way. This high star - formation rate has been almost continuous for the past 100 million years. Thanks

PIX4609940

China: The Daoist immortal Zhongli Quan, from the album of 18 Daoist Paintings by Zhang Lu (1464-1538), 16th century CE. Painting sprinkled with gold leaf, Shanghai Museum, Shanghai

Zhang Lu (1464-1538)

PFH3431937

Ancient Roman city of Empúries, Catalonia, 2022 (photography)

Sergi Reboredo

SRB7334175

Ancient Roman city of Empúries, Catalonia, 2022 (photography)

Sergi Reboredo

SRB7334176

Rare bank note holder for Boucheron, 1893 (ivory, gold, enamel, rubies, sapphires & amethysts)

Sache, Georges le (b.1849)

CH3326251

Malaysia / China: Carving of Zhou Xin (King Zhou of Shang), depicting his role in the 16th Century Ming Dynasty novel 'Fengshen Yanyi' ('Investiture of the Gods'). From Ping Sien Si Temple, Pasir Panjang Laut

PFH3277955

Six Senses Resort, Koh Yao Noi, Phang Nga Bay, Thailand, Asia (photo)

Sergi Reboredo

SRB3585115

Rare bank note holder for Boucheron, 1893 (ivory, gold, enamel, rubies, sapphires & amethysts)

Sache, Georges le (b.1849)

CH3326247

The Angel of the Annunciation, 1947 (oil on cardboard)

McCahon, Colin (1919-87)

TEP3084374

Italy / Holland: 'Tiberius, Emperor of Rome' (42 BCE - 37 CE), line engraving by Aegidus Sadeler (Netherlands, 1570-1629), after Titian, 17th Century

Sadeler or Saedeler, Aegidius (1570-1629)

PFH3122258

Rare bank note holder for Boucheron, 1893 (ivory, gold, enamel, rubies, sapphires & amethysts)

Sache, Georges le (b.1849)

CH3326248

Rare bank note holder for Boucheron, 1893 (ivory, gold, enamel, rubies, sapphires & amethysts)

Sache, Georges le (b.1849)

CH3326250

Rare bank note holder for Boucheron, 1893 (ivory, gold, enamel, rubies, sapphires & amethysts)

Sache, Georges le (b.1849)

CH3326252

China: Portrait of the Chinese mythical deity Pangu, from the Ming Dynasty encyclopedia <i>Sancai Tuhui</i> ('Illustrations of the Three Realms') Wang Qi, 1609

PFH3431914

Malaysia / China: Carving of King Zhou of Shang, depicting his role in the 16th Century Ming Dynasty novel 'Fengshen Yanyi' ('Investiture of the Gods'). From Ping Sien Si Temple, Pasir Panjang Laut

PFH3277774

Mississippi Delta, Louisiana, seen by satellite - Mississippi River Delta. Louisiana - Mississpi Delta, Louisiana, USA, seen by Landsat-7 satellite, November 27, 1999. The Mississippi River drains the heart of the North American continent, carrying vast quantities of sediment and depositing it along the shore of Louisiana and into the Gulf of Mexico. The sediment is composed of topsoil, sand, dead and decaying plants, and anything else washed away by a strong rainstorm far upstream. Many of these effluents are nutrients that act as fertilizer for the microscopic plants (phytoplankton) living near the surface of the Gulf waters. Each summer the phytoplankton population explodes. As the phytoplankton age, die, and decompose, bacteria absorb oxygen dissolved in the water, creating a dead zone”” along the shore at the ocean bottom. The oxygen - poor water is deadly to animals, from the microscopic zooplankton that graze on phytoplankton to crustaceans, molluscs, and fish. Once infrequent,

PIX4673124

Rare bank note holder for Boucheron, 1893 (ivory, gold, enamel, rubies, sapphires & amethysts)

Sache, Georges le (b.1849)

CH3326249

Rare bank note holder for Boucheron, 1893 (ivory, gold, enamel, rubies, sapphires & amethysts)

Sache, Georges le (b.1849)

CH3326253

Winter scene with a sledge in the foreground and figures gathering round a tent on the ice, 1653 (oil on panel)

Goyen, Jan Josephsz van (1596-1656)

MAN3900340

Satellite photo of the Rub al Khali desert - Rub 'al Khali desert seen from space - Rub al-Khali (the Empty Quarter), is one of the largest deserts and the largest uninterrupted expanse of sand in the world. It covers nearly 600,000 square kilometres in the Arabian Peninsula, located mostly in Saudi Arabia and in the territories of Yemen, Oman and the United Arab Emirates. The image obtained by the Landsat-7 satellite on 26 August 2001 shows the sand dune fields separated by flat and saline stretches, sebkha (or sabkha). The Arabian Peninsula's Empty Quarter, known as Rub 'al Khali, is the world's largest sand sea, holding about half as much sand as the Sahara Desert. The Empty Quarter covers 583,000 square kilometers (225,000 square miles), and stretches over parts of Saudi Arabia, Yemen, Oman, and the United Arab Emirates. The Enhanced Thematic Mapper on Nasa's Landsat 7 satellite captured this image of the Empty Quarter on August 26, 2001. The area shown resides in southeastern Saud

PIX4658462

Abstract Automatic Collage: 49, 2020 (paper collage)

premium — Abstract Automatic Collage: 49, 2020 (paper collage)

Abstract Automatic Collage: 49, 2020 (paper collage)

Pierides, Kika

ACG8093756

Abstract Automatic Collage: 72, 2020 (paper collage)

Abstract Automatic Collage: 72, 2020 (paper collage)

Pierides, Kika

ACG8093874

Abstract Automatic Collage: 96, 2020 (paper collage)

Abstract Automatic Collage: 96, 2020 (paper collage)

Pierides, Kika

ACG8093951

Abstract Automatic Collage: 58, 2020 (paper collage)

Abstract Automatic Collage: 58, 2020 (paper collage)

Pierides, Kika

ACG8093780

Abstract Automatic Collage: 66, 2020 (paper collage)

Abstract Automatic Collage: 66, 2020 (paper collage)

Pierides, Kika

ACG8093857

Abstract Automatic Collage: 91, 2020 (paper collage)

Abstract Automatic Collage: 91, 2020 (paper collage)

Pierides, Kika

ACG8093900

Galaxies NGC 5426 and NGC 5427 in the Virgin - Galaxies NGC 5426 and NGC 5427 in Virgo - Arp 271 desks the two spiral galaxies of similar sizes in interaction NGC 5426 and NGC 5427. Located 90 million years ago - light in the constellation of Virgo, Arp 271 is about 130,000 years - light in diameter. Although it is uncertain whether this interaction leads to a fusion of galaxies, the galaxies are already gravitationally affected by each other and a bridge of matter has formed between the two. Image obtained with a telescope of 80 cm. NGC 5426 and NGC 5427 are two spiral galaxies of similar sizes engaged in a dramatic dance. It is not certain that this interaction will end in a collision and ultimately a merging of the two galaxies, although the galaxies have already been affected. Together known as Arp 271, this dance will last for tens of millions of years, creating new stars as a result of the mutual gravitational attraction between the galaxies, a pull seen in the bridge of stars al

Adam Block

PIX4612650

Mars - View of the south pole - Mars South pole - Image of part of the southern polar cap of Mars obtained by the Mars Express probe on December 17, 2012. The bright white region of this image shows the icy cap that covers Mars' south pole, composed of frozen water and carbon dioxide. While it looks smooth in this image, at close quarters the cap is a layered mix of peaks, troughs and flat plains, and has been likened in appearance to swiss cheese. The southern cap reaches some 3 km thick in places, and is around 350 km in diameter. This icy region is permanent; in the martian winter another, thinner ice cap forms over the top of it, stretching further out across the planet and disappearing again when the weather warms up. The cap is around 150 km north of Mars' geographical south pole and Mars Express has shed light on why this ice cap is displaced. Deep impact craters - notably the Hellas Basin, the largest impact structure on the entire planet at 7 km deep and 2300 km across - funne

PIX4616189

Star field in the constellation Sagittarius - Scattered stars in Sagittarius: Stars in Sagittarius seen by the space telescope Hubble. This stunning image, captured by the NASA/ESA Hubble Space Telescope's Advanced Camera for Surveys (ACS), shows part of the sky in the constellation of Sagittarius (The Archer). The region is rendered in exquisite detail - deep red and bright blue stars are scattered across the frame, set against a background of thousands of more distant stars and galaxies. Two features are particularly striking: the colours of the stars, and the dramatic crosses that burst from the centres of the brightest bodies. While some of the colours in this frame have been enhanced and tweaked during the process of creating the image from the observational data, different stars do indeed glow in different colours. Stars differ in colour according to their surface temperature: very hot stars are blue or white, while cooler stars are redder. They may be cooler because they are sma

PIX4572253

Abstract Automatic Collage: 20, 2020 (paper collage)

Abstract Automatic Collage: 20, 2020 (paper collage)

Pierides, Kika

ACG8093737

Abstract Automatic Collage: 36, 2020 (paper collage)

Abstract Automatic Collage: 36, 2020 (paper collage)

Pierides, Kika

ACG8093741

Abstract Automatic Collage: 37, 2020 (paper collage)

Abstract Automatic Collage: 37, 2020 (paper collage)

Pierides, Kika

ACG8093746

Abstract Automatic Collage: 60, 2020 (paper collage)

Abstract Automatic Collage: 60, 2020 (paper collage)

Pierides, Kika

ACG8093841

Abstract Automatic Collage: 71, 2020 (paper collage)

Abstract Automatic Collage: 71, 2020 (paper collage)

Pierides, Kika

ACG8093864

Abstract Automatic Collage: 48, 2020 (paper collage)

Abstract Automatic Collage: 48, 2020 (paper collage)

Pierides, Kika

ACG8093752

Abstract Automatic Collage: 50, 2020 (paper collage)

Abstract Automatic Collage: 50, 2020 (paper collage)

Pierides, Kika

ACG8093761

Abstract Automatic Collage: 52, 2020 (paper collage)

Abstract Automatic Collage: 52, 2020 (paper collage)

Pierides, Kika

ACG8093765

Abstract Automatic Collage: 59, 2020 (paper collage)

Abstract Automatic Collage: 59, 2020 (paper collage)

Pierides, Kika

ACG8093832

Remains of the Supernova of Vails - The Vela supernova remnant: Nearly 12,000 years ago, a massive star exploded in the constellation of Vails. The star reaches the end of life and expels its material to become a small star only a few kilometres in diameter. This stellar corpse is a neutron star, the pulsar of Voiles, barely visible in the image. The gas shell that surrounds it today extends over more than 100 light years. Mosaic of 117 images - Approximately 11,000 to 12,000 years ago a massive star exploded in the southern constellation of Vela. The matter ejected by the supernova scattered the contents of the star into the surrounding interstellar medium creating shock fronts of multimillion degree gas and high energy particles. The heated matter produces brilliant visible light as well as radio and x-ray emission which will continue for thousands of years until the entire remnant of the dying star completely dissipates into space. Supernovas enrich the surrounding interstellar medi

R. Gendler

PIX4626466

Abstract Automatic Collage: 57, 2020 (paper collage)

Abstract Automatic Collage: 57, 2020 (paper collage)

Pierides, Kika

ACG8093776

Abstract Automatic Collage: 62, 2020 (paper collage)

Abstract Automatic Collage: 62, 2020 (paper collage)

Pierides, Kika

ACG8093847

Abstract Automatic Collage: 81, 2020 (paper collage)

Abstract Automatic Collage: 81, 2020 (paper collage)

Pierides, Kika

ACG8093882

Six Senses Resort, Koh Yao Noi, Phang Nga Bay, Thailand, Asia (photo)

Sergi Reboredo

SRB3585117

Globular cluster M54 in Sagittarius - Globular cluster M54 in Sagittarius - The globular cluster M54 photographed by the Hubble space telescope (HST). M54 resides about 90,000 light years from Earth, in the dwarf galaxy of Sagittarius. The object shown in this beautiful Hubble image, dubbed Messier 54, could be just another globular cluster, but this dense and faint group of stars was in fact the first globular cluster found that is outside our galaxy. Discovered by the famous astronomer Charles Messier in 1778, Messier 54 belongs to a satellite of the Milky Way called the Sagittarius Dwarf Elliptical Galaxy. Messier had no idea of the significance of his discovery at the time, and it wasn't until over two centuries later, in 1994, that astronomers found Messier 54 to be part of the miniature galaxy and not our own. Current estimates indicate that the Sagittarius dwarf, and hence the cluster, is situated almost 90 000 light - years away - - more than three times as far from the centre

PIX4565011

Nebula N44 in the Large Magellan Cloud - Superbubble LHA 120 - N 44 in the Large Magellanic Cloud - This image obtained by the Very Large Telescope (VLT) shows the nebula N44 surrounding the cluster of stars NGC 1929. It is a star-forming region located in the galaxy of the Great Magellan Cloud, about 170,000 light years from Earth. Eso's Very Large Telescope captured this striking view of the nebula around the star cluster NGC 1929 within the Large Magellanic Cloud, a satellite galaxy of our own Milky Way. A colossal example of what astronomers call a superbubble dominates this stellar nursery. It is being carved by the winds from bright young stars and the shockwaves from supernova explosions. This nebula is officially known as LHA 120 - N 44, or just N 44 for short. Hot young stars in NGC 1929 are emitting intense ultraviolet light and causing the gas to glow. This effect highlights the aptly - named superbubble, a vast shell of material around 325 by 250 light - years across. For c

PIX4620802

Geyser sur Enceladus - Artist's view - Water geyser on Enceladus - Artist's view of an ice geyser on the surface of the Enceladus satellite. In the sky, the planet Saturn and its satellite Mimas. Liquid water reaches the surface of Enceladus' south pole and drives a massive plume of ice crystals into the sky. The combination of Enceladus' low surface gravity and the geyser's force accelerate the crystals to escape velocity, where sunlight breaks the water molecules down into their constituent atoms of hydrogen and oxygen. Saturn itself appears low on the horizon due to the proximity to Enceladus' pole. The small object immediately to Saturn's left is another icy moon named Mimas. Somewhat smaller than Enceladus and closer to Saturn, Mimas sprints around Saturn in slightly less than one Earth day. In March 2006 Nasa's Cassini probe revealed evidence of water - driven geysers on the surface of Enceladus. At first glance Enceladus doesn't seem to be a likely host for liquid water as the s

Walter B Myers

PIX4625896

The Omega nebula (M17) seen in infrared - M17 nebula in infrared - The Omega nebula (M17) seen in infrared by the Spitzer space telescope. M17 is a star-forming region about 6000 light years ago in the constellation Sagittarius. In the center of the nebula is a group of massive stars. The dust appears in red, the hot gas in green, the regions or this gas and the dust mixes in white. Nasa's Spitzer Space Telescope has captured an infrared view of the star - making cloud called M17, or the Swan nebula. The cloud, located about 6,000 light - years away in the constellation Sagittarius, is dominated by a central group of massive stars - - the most massive stars in the region. These central stars give off intense flows of expanding gas, which rush like rivers against dense piles of material, carving out the deep pocket at center of the picture. Winds from the region's other massive stars push back against these oncoming rivers, creating bow shocks like those that pile up in front of speedin

PIX4620190

Geyser sur Enceladus - Artist view - Water geyser on Enceladus - Artist view - Artist view of an ice geyser on the surface of the Enceladus satellite. In the sky, the planet Saturn and its satellite Mimas. Liquid water reaches the surface of Enceladus' south pole and drives a massive plume of ice crystals into the sky. The combination of Enceladus' low surface gravity and the geyser's force accelerate the crystals to escape velocity, where sunlight breaks the water molecules down into their constituent atoms of hydrogen and oxygen. Saturn itself appears low on the horizon due to the proximity to Enceladus' pole. The small object immediately to Saturn's left is another icy moon named Mimas. Somewhat smaller than Enceladus and closer to Saturn, Mimas sprints around Saturn in slightly less than one Earth day. In March 2006 Nasa's Cassini probe revealed evidence of water - driven geysers on the surface of Enceladus. At first glance Enceladus doesn't seem to be a likely host for liquid wate

Walter B Myers

PIX4625850

Six Senses Resort, Koh Yao Noi, Phang Nga Bay, Thailand, Asia (photo)

Sergi Reboredo

SRB3585116

Bok's cells in NGC 281 (Cassiopee) - Bok globules in NGC 281 - View of a detail of the nebula NGC 281 in Cassiopee center on Bok's Globules. A Bok's blood cell is a dark interstellar cloud of gases and dust that absorb light. If it condenses enough, it gives birth to new stars. Near these blood cells shine blue stars; they belong to the young cluster of stars IC 1590. Image obtained by the Hubble Space Telescope in October 2005. These opaque, dark knots of gas and dust are called “” Bok globules,””” and they are absorbing light in the center of the nearby emission nebula and star - forming region. Bok hypothesized that giant molecular clouds, on the order of hundreds of light - years in size, can become perturbed and form small pockets where the dust and gas are highly concentrated. These small pockets become gravitationally bound and accumulate dust and gas from the surrounding area. If they can capture enough mass, they have the potential of creating stars in their cores; however, no

PIX4617491

Childhood in Bulgaria, 1977 (16mm negative, 2K/Sound scan)

MOD6428920

Star T - Tauri in Orion - Bow Shock around T - Tauri Star in the Orion Nebula - LL Ori is a star T - Tauri located about 1500 years ago - light from Earth in Orion's nebula. This young star emits a powerful stellar wind that hits the surrounding gas creating an arc-shaped shock wave Image obtained by the Hubble space telescope in February 1995. A bow shock can be created in space when two streams of gas collide. The star LL Ori emits a vigorous solar wind, a stream of charged particles moving rapidly outward from the star. Our own Sun has a less energetic version of this wind that is responsible for auroral displays on the Earth. The material in the fast wind from LL Ori collides with slow - moving gas evaporating away from the center of the Orion Nebula, which is located to the lower right in this Heritage image. The surface where the two winds collide is the crescent - shaped bow shock seen in the image. Unlike a water wave made by a ship, this interstellar bow shock is a three - dim

PIX4572363

Dolly Rathebe - Dolly and Her Men! - The World Does Not Suspect That Film Star Dolly…, 1957 (photo)

Jürgen Schadeberg

AMD8679363

Paul Loebe House, Berlin, Germany2018 (photo)

Sergi Reboredo

SRB5056248

Dolly Rathebe - Dolly and Her Men! - The World Does Not Suspect That Film Star Dolly…, 1957 (photo)

Jürgen Schadeberg

AMD8679285

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Asset title and keywords	~	~pony
Asset description text	description:	description:london
Agency prefix	prfx: or $	prfx:lal or $LAL
Asset id	imageid:	imageid:250297 or imageid:[2500 TO 4000]
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Location	loc: or @	loc:exeter or @exeter
Classification	class: or #	class:57 or #57. Use # for unclassified assets
Year	year:	year:1850 or year:[1700 TO 1800]

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