'Creating' images and/or videos results

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

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

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

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: 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

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

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

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

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

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

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

Jürgen Schadeberg

AMD8679362

Pulsar of Crab in Taurus seen in X - The Crab nebula pulsar - Pulsar of Crab in Taurus seen in X by satellite Chandra. The pulsar is the white dot in the center of the image. This neutron star generates a powerful magnetic field creating material jets at the poles, as well as a strong stellar wind. This image gives the first clear view of the faint boundary of the Crab Nebula's X - ray - emitting pulsar wind nebula. The nebula is powered by a rapidly rotating, highly magnetized neutron star, or pulsar (white dot near the center). The combination of rapid rotating and strong magnetic field generates an intense electromagnetic field that creates jets of matter and anti - matter moving away from the north and south poles of the pulsar, and an intense wind flowing out in the equatorial direction. The inner X - ray ring is thought to be a shock wave that marks the boundary between the surrounding nebula and the flow of matter and antimatter particles from the pulsar. Energetic electrons and

PIX4583131

The Rho Ophiuchi nebula seen in infrared - Rho Ophiuchi in infrared - This coloree nebula represents part of a very vast molecular cloud, the Ophiuchus cloud. This star-forming region is about 520 years old - light. The triple star Rho Ophiuchus is located in the top center of the image. Below, a very bright nebula is visible, accompanied by a group of very young stars. At the bottom right, surrounded by a reddish nebula, the star Sigma Scorpii. The globular clusters NGC 6144 (bottom, center of the image) and M80 (top right of the image) are also visible on this infrared image obtained from the Wide - field Infrared Explorer (WISE) satellite. A rich collection of colorful astronomical objects is revealed in this picturesque image of the Rho Ophiuchi cloud complex from Nasa's Wide - field Infrared Explorer, or WISE. The Rho Ophiuchi cloud (pronounced 'oh - fee - yoo - ki' and named after a bright star in the region) is found rising above the plane of the Milky Way in the night sky, bord

PIX4621533

Planetary nebula NGC 6543 in the Dragon/HST - This NASA Hubble Space Telescope image shows one of the most complex planetary nebulae ever seen, NGC 6543, nicknamed the “Cat's Eye Nebula.””” Hubble reveals surprisingly intricate structures including concentric gas shells, jets of high - speed gas and unusual shock - induced knots of gas. Estimated to be 1,000 years old, the nebula is a visual “” fossil record”” of the dynamics and late evolution of a dying star. A preliminary interpretation suggests that the star might be a double - star system. The dynamical effects of two stars orbiting one another most easily explains the intricate structures, which are much more complicated than features seen in most planetary nebulae. (The two stars are too close together to be individually resolved by Hubble, and instead, appear as a single point of light at the center of the nebula.) According to this model, a fast “” stellar wind””” of gas blown off the central star created the elongated shell o

PIX4623213

Richat structure - Mauritania - satellite view - Richat structure, Mauritania, seen by satellite - Richat structure is a geological formation of volcanic origin in Mauritania. This “eye” measures 50 km in diameter. This image is a combination of an image obtained by the Landsat satellite in 1987 and a radar image obtained from the Space Shuttle (SRTM) in 2000. The relief is exaggerated by about 6 times. The picture covers an area of 68 km by 112 km. This prominent circular feature, known as the Richat Structure, in the Sahara desert of Mauritania is often noted by astronauts because it forms a conspicuous 50 - kilometer - wide (30 - mile - wide) bull's - eye on the otherwise rather featureless expanse of the desert. Initially mistaken for a possible impact crater, it is now known to be an eroded circular anticline (structural dome) of layered sedimentary rocks. Extensive sand dunes occur in this region and the interaction of bedrock topography, wind, and moving sand is evident in this

PIX4659064

Wrapped in blankets to ward off the cold, women and a child sit together in a shallow pit, the first step in creating a tent shelter for themselves in the Maslakh camp for an estimated 140,000 displaced persons, set up amidst the ruins of an abandoned village near the western city of Herat, capital of the province of the same name. Despite low temperatures that often drop below freezing at night, many new arrivals to the camp have no shelter at all. Until they find some kind of assistance from either their equally poor neighbours, or from international agencies working in the camp, they have to spend night under the open skies in temperatures that often reaches several degrees below freezing. As a result often children and older people die from the cold. Lack of access to a food and water only aggravates these miseries. Afghanistan. With ongoing conflicts and emergencies like draughts in Afghanistan and some 7.5 million people requiring international support -- two-thirds of who are ch

UIG795801

Field	Search term	Example
Asset title	title:	title:pony
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]
Agency name	coll:	coll:history
Medium	medium:	medium:oil
Century	century:	century:20th
Keywords	kw:	kw:dog
Artist name	artist: or ?	artist:monet or ?monet
Artist nationality	??	??French
Creator ID	creatorid:	creatorid:37
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]

Display options

View

Image Size

Images of 'Creating' found, 2,236

Copyright

Copyright

Copyright

Copyright

Copyright

Copyright

Copyright

Copyright

Copyright

Copyright

Copyright

Copyright

Copyright

Copyright

Copyright

Copyright

Copyright

Copyright

Copyright

Image Restrictions

Usage restrictions from our Content Partners

Special Instructions

Art. Culture. History.

Simple. Fast. Reliable.

Discover millions of images and videos for your creative projects.