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Images of 'Diameter 200' found, 44

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1+1=2, 1971 (mixed media)

1+1=2, 1971 (mixed media)

Merz, Mario (1925-2003)

XKH156476

Venus: Aine corona - Volcanic Formation 200 km in diameter.

Venus: Aine corona - Volcanic Formation 200 km in diameter.

PIX4635325

Arecibo Radiotelescope - Puerto Rico - The largest radio telescope in the world, 305m diameter antenna. 03 - 200

Arecibo Radiotelescope - Puerto Rico - The largest radio telescope in the world, 305m diameter antenna. 03 - 200

Christophe Lebedinsky

PIX4651661

Arecibo Radiotelescope - Puerto Rico - The largest radio telescope in the world, 305m diameter antenna. 03 - 200

Arecibo Radiotelescope - Puerto Rico - The largest radio telescope in the world, 305m diameter antenna. 03 - 200

Christophe Lebedinsky

PIX4651751

Arecibo Radiotelescope - Puerto Rico - The largest radio telescope in the world, 305m diameter antenna. 03 - 200

Arecibo Radiotelescope - Puerto Rico - The largest radio telescope in the world, 305m diameter antenna. 03 - 200

Christophe Lebedinsky

PIX4651720

Arecibo Radiotelescope - Puerto Rico - The largest radio telescope in the world, 305m diameter antenna. 03 - 200

Arecibo Radiotelescope - Puerto Rico - The largest radio telescope in the world, 305m diameter antenna. 03 - 200

Christophe Lebedinsky

PIX4651637

Arecibo Radiotelescope - Puerto Rico - The largest radio telescope in the world, 305m diameter antenna. 03 - 200

Arecibo Radiotelescope - Puerto Rico - The largest radio telescope in the world, 305m diameter antenna. 03 - 200

Christophe Lebedinsky

PIX4651666

Arecibo Radiotelescope - Puerto Rico - The largest radio telescope in the world, 305m diameter antenna. 03 - 200

Arecibo Radiotelescope - Puerto Rico - The largest radio telescope in the world, 305m diameter antenna. 03 - 200

Christophe Lebedinsky

PIX4651634

Arecibo Radiotelescope - Puerto Rico - The largest radio telescope in the world, 305m diameter antenna. 03 - 200

Arecibo Radiotelescope - Puerto Rico - The largest radio telescope in the world, 305m diameter antenna. 03 - 200

Christophe Lebedinsky

PIX4651654

Arecibo Radiotelescope - Puerto Rico - The largest radio telescope in the world, 305m diameter antenna. 03 - 200

Arecibo Radiotelescope - Puerto Rico - The largest radio telescope in the world, 305m diameter antenna. 03 - 200

Christophe Lebedinsky

PIX4651678

Arecibo Radiotelescope - Puerto Rico - The largest radio telescope in the world, 305m diameter antenna. 03 - 200

Arecibo Radiotelescope - Puerto Rico - The largest radio telescope in the world, 305m diameter antenna. 03 - 200

Christophe Lebedinsky

PIX4651680

Arecibo Radiotelescope - Puerto Rico - The largest radio telescope in the world, 305m diameter antenna. 03 - 200

Arecibo Radiotelescope - Puerto Rico - The largest radio telescope in the world, 305m diameter antenna. 03 - 200

Christophe Lebedinsky

PIX4651625

Arecibo Radiotelescope - Puerto Rico - The largest radio telescope in the world, 305m diameter antenna. 03 - 200

Arecibo Radiotelescope - Puerto Rico - The largest radio telescope in the world, 305m diameter antenna. 03 - 200

Christophe Lebedinsky

PIX4651649

Arecibo Radiotelescope - Puerto Rico - The largest radio telescope in the world, 305m diameter antenna. 03 - 200

Arecibo Radiotelescope - Puerto Rico - The largest radio telescope in the world, 305m diameter antenna. 03 - 200

Christophe Lebedinsky

PIX4651695

Arecibo Radiotelescope - Puerto Rico - The largest radio telescope in the world, 305m diameter antenna. 03 - 200

Arecibo Radiotelescope - Puerto Rico - The largest radio telescope in the world, 305m diameter antenna. 03 - 200

Christophe Lebedinsky

PIX4651746

Arecibo Radiotelescope - Puerto Rico under the Moon - The largest radiotelescope in the world, 305m in diameter antenna. 03 - 200

Arecibo Radiotelescope - Puerto Rico under the Moon - The largest radiotelescope in the world, 305m in diameter antenna. 03 - 200

Christophe Lebedinsky

PIX4651682

Mirror, 101 AD200 AD (reflective disk: bronze; repoussé disk: brass)

Mirror, 101 AD200 AD (reflective disk: bronze; repoussé disk: brass)

Roman, (2nd century)

XCC5861417

Arecibo Radiotelescope - Puerto Rico - Tourist Tour - The largest radio telescope in the world, 305m diameter antenna. 03 - 200

Arecibo Radiotelescope - Puerto Rico - Tourist Tour - The largest radio telescope in the world, 305m diameter antenna. 03 - 200

Christophe Lebedinsky

PIX4651683

Tamalameque culture (200-600 / 16th century). Clay anthropomorphic figure. From Colombia.

Tamalameque culture (200-600 / 16th century). Clay anthropomorphic figure. From Colombia.

TRK2922577

Arecibo Radiotelescope - Puerto Rico - Close up on single antenna. The world's largest radio telescope, 305m diameter antenna. 03 - 200

Arecibo Radiotelescope - Puerto Rico - Close up on single antenna. The world's largest radio telescope, 305m diameter antenna. 03 - 200

Christophe Lebedinsky

PIX4651664

Tête au masque (A.R. 362), 1956 (ceramic)

Tête au masque (A.R. 362), 1956 (ceramic)

Picasso, Pablo (1881-1973)

CH6371230

Tamalameque culture (200-600 / 16th century). Clay anthropomorphic figure. From Colombia.

Tamalameque culture (200-600 / 16th century). Clay anthropomorphic figure. From Colombia.

TRK2922582

Pre-Incan. Guangala Culture.300/200 a 700/800 DC. Ceramic vessel. From Ecuador.

Pre-Incan. Guangala Culture.300/200 a 700/800 DC. Ceramic vessel. From Ecuador.

TRK2922579

Aorounga Meteor Impact Crater, Chad, True Colour Satellite Image

Aorounga Meteor Impact Crater, Chad, True Colour Satellite Image

UIG602006

Aorounga Crater, Chad, True Colour Satellite Image

Aorounga Crater, Chad, True Colour Satellite Image

UIG601867

Terracotta anthropomorphic container showing an ansa serving as a spout, height 22.8cm, width 14.2cm, diameter opening 7.6cm. Artifact originating from the Valley of Sula (Honduras). Mayan Civilization, pre-classical period 900 BC-200 AD.

Terracotta anthropomorphic container showing an ansa serving as a spout, height 22.8cm, width 14.2cm, diameter opening 7.6cm. Artifact originating from the Valley of Sula (Honduras). Mayan Civilization, pre-classical period 900 BC-200 AD.

DGA534592

Io seen by the probe Voyager 1 - Region of the south pole - At the bottom of the image Haemus Mons, not far from the southern pole of Io, is one of the largest mountains in the solar system. It extends 200 km in diameter and is more than 10 000m; it is completely covered with sulfur frost. Mosaic of images obtained by the Voyager 1 probe

Io seen by the probe Voyager 1 - Region of the south pole - At the bottom of the image Haemus Mons, not far from the southern pole of Io, is one of the largest mountains in the solar system. It extends 200 km in diameter and is more than 10 000m; it is completely covered with sulfur frost. Mosaic of images obtained by the Voyager 1 probe

PIX4574650

Switzerland Music Sammy Davis Jr., 1978 (b/w photo)

Switzerland Music Sammy Davis Jr., 1978 (b/w photo)

Stringer (STR)

KES6248565

Vincent Lunardi airborne after his ascent from Moorfields, September 1784 (coloured engraving)

Vincent Lunardi airborne after his ascent from Moorfields, September 1784 (coloured engraving)

English School, (18th century)

BL3960213

Switzerland Music Sammy Davis Jr., 1978 (b/w photo)

Switzerland Music Sammy Davis Jr., 1978 (b/w photo)

Stringer (STR)

KES6248564

Halo around the Sun - Sun Halo - Halos are due to the light of the Sun reflected by high-altitude clouds, cirrostratus, composed of ice crystals. They bend the light and thus cause a perfect circle around the Sun. 30 May 2007. Halos are caused by sunlight being refracted by cirro - stratus clouds. These are thin clouds, very high in the atmosphere, and are composed of ice crystals. They bend light at a 22 degree angle, which creates a halo around the sun that is 44 degrees in diameter. May 30 200

Halo around the Sun - Sun Halo - Halos are due to the light of the Sun reflected by high-altitude clouds, cirrostratus, composed of ice crystals. They bend the light and thus cause a perfect circle around the Sun. 30 May 2007. Halos are caused by sunlight being refracted by cirro - stratus clouds. These are thin clouds, very high in the atmosphere, and are composed of ice crystals. They bend light at a 22 degree angle, which creates a halo around the sun that is 44 degrees in diameter. May 30 200

G. Cannat

PIX4670990

Aerial view of CERN with the trace of the LEP tunnel and the future LHC - CERN's aerial view - Aerial view of CERN near Geneva. The large circle of 27 km in diameter shows the trace of the LEP tunnel and the LHC. The LEP (Large Electron Positron) was operational until 2000 and was launched to give way to the LHC (Large Hadron Collider). Date: 01 Jan 2001 Aerial view of the CERN site just outside Geneva, Switzerland. The large circle shows the line of the LEP tunnel, 27 km in circumference. The LEP (Large Electron Positron) was operational until 2000, then dismantled to build the LHC (Large Hadron collider). January 1, 200

Aerial view of CERN with the trace of the LEP tunnel and the future LHC - CERN's aerial view - Aerial view of CERN near Geneva. The large circle of 27 km in diameter shows the trace of the LEP tunnel and the LHC. The LEP (Large Electron Positron) was operational until 2000 and was launched to give way to the LHC (Large Hadron Collider). Date: 01 Jan 2001 Aerial view of the CERN site just outside Geneva, Switzerland. The large circle shows the line of the LEP tunnel, 27 km in circumference. The LEP (Large Electron Positron) was operational until 2000, then dismantled to build the LHC (Large Hadron collider). January 1, 200

PIX4650450

Thailand: A mature jackfruit hangs from the trunk of a jackfruit tree, southern Thailand

Thailand: A mature jackfruit hangs from the trunk of a jackfruit tree, southern Thailand

David Henley

PFH4072221

George Ellery Hale, American astronomer, 1918

George Ellery Hale, American astronomer, 1918

UIS5075109

Earth during a Total Solar Eclipse - Earth during a Total Solar Eclipse - Artist's view of the planet Earth during the night, seen above the Indian Ocean. The artificial lights of the cities appear. On the right, the part illuminated by the Sun shows an area of shadow caused by a total eclipse of the Sun. The perspective in this image is looking down on the Indian Ocean from an altitude of 25,000 miles. On the Earth's night side artificial lights clearly define the Mediterranean Sea, Red Sea, and almost the entire African continent, while clouds obscure some of Europe and India. The alignment with the Moon and Sun is such that at this moment a total eclipse of the Sun is visible revealing the Sun's brilliant corona. However the area of totality, i.e., the darkest part of the Moon's shadow, is so small - - less than 200 miles wide - - that observers on the Earth would not be able to see this total eclipse. The only portion of the eclipse visible from the Earth is in the eastern Indian O

Earth during a Total Solar Eclipse - Earth during a Total Solar Eclipse - Artist's view of the planet Earth during the night, seen above the Indian Ocean. The artificial lights of the cities appear. On the right, the part illuminated by the Sun shows an area of shadow caused by a total eclipse of the Sun. The perspective in this image is looking down on the Indian Ocean from an altitude of 25,000 miles. On the Earth's night side artificial lights clearly define the Mediterranean Sea, Red Sea, and almost the entire African continent, while clouds obscure some of Europe and India. The alignment with the Moon and Sun is such that at this moment a total eclipse of the Sun is visible revealing the Sun's brilliant corona. However the area of totality, i.e., the darkest part of the Moon's shadow, is so small - - less than 200 miles wide - - that observers on the Earth would not be able to see this total eclipse. The only portion of the eclipse visible from the Earth is in the eastern Indian O

Walter B Myers

PIX4628553

The Formation of the Earth - Artist's View - Meteorite strike on infant Earth - The Earth was formed 4.6 billion years ago from a gigantic cloud of gas and dust. These dust accreted to form our planet; it was subjected to a large bombardment of meteorites. A molten, infant Earth is impacted by an object about 10 miles in diameter, releasing 200 million times a much energy as the largest manmade explosion. While this collision appears negligible when compared to the scars of much larger encounters, a similar impact four billion years later may have resulted in the extinction of the dinosaurs. The Earth accrued the majority of its mass during the 100 million years following the formation of the Sun, a period referred to as the cosmic bombardment. During this era of frequent impacts and radioactive heating, the entire Earth remained molten long enough for the heavy metals iron and nickel to settle to the center of the Earth while lighter silicates floated to the surface. Today, over four

The Formation of the Earth - Artist's View - Meteorite strike on infant Earth - The Earth was formed 4.6 billion years ago from a gigantic cloud of gas and dust. These dust accreted to form our planet; it was subjected to a large bombardment of meteorites. A molten, infant Earth is impacted by an object about 10 miles in diameter, releasing 200 million times a much energy as the largest manmade explosion. While this collision appears negligible when compared to the scars of much larger encounters, a similar impact four billion years later may have resulted in the extinction of the dinosaurs. The Earth accrued the majority of its mass during the 100 million years following the formation of the Sun, a period referred to as the cosmic bombardment. During this era of frequent impacts and radioactive heating, the entire Earth remained molten long enough for the heavy metals iron and nickel to settle to the center of the Earth while lighter silicates floated to the surface. Today, over four

Walter B Myers

PIX4633457

Nebula NGC 6726 - 27 - 29 in the Southern Crown - The Corona Australis nebula (NGC 6726 - 27 - 29) Image of R Coronae Australis region in the southern Milky Way, obtained with the Wide Field Imager (WFI) (camera) at the 2.2 - m MPG/ESO Telescope on La Silla (Chile). The sky field shown measures approx. 33.7 x 31.9 arcmin2 (about the diameter of the full moon). The R Coronae Australis complex of young stars and interstellar gas clouds is one of the nearest star - forming regions, at a distance of approx. 500 light - years from the Sun. It is seen in the southern constellation of that name (The “Southern Crown”). R Coronae Australis, the bright star from which the entire complex is named, is located at the center of the field and illuminates the reddish nebula around it. The bright star in the lower part, illuminating a somewhat bluer nebula, is known as TY Coronae Australis. The brightness of these two stars and several others in the same field is variable. They belong to the so - calle

Nebula NGC 6726 - 27 - 29 in the Southern Crown - The Corona Australis nebula (NGC 6726 - 27 - 29) Image of R Coronae Australis region in the southern Milky Way, obtained with the Wide Field Imager (WFI) (camera) at the 2.2 - m MPG/ESO Telescope on La Silla (Chile). The sky field shown measures approx. 33.7 x 31.9 arcmin2 (about the diameter of the full moon). The R Coronae Australis complex of young stars and interstellar gas clouds is one of the nearest star - forming regions, at a distance of approx. 500 light - years from the Sun. It is seen in the southern constellation of that name (The “Southern Crown”). R Coronae Australis, the bright star from which the entire complex is named, is located at the center of the field and illuminates the reddish nebula around it. The bright star in the lower part, illuminating a somewhat bluer nebula, is known as TY Coronae Australis. The brightness of these two stars and several others in the same field is variable. They belong to the so - calle

PIX4620222

Planetary nebula M2 - 9 in Ophiuchus/HST - M2 - 9 is a striking example of a “” butterfly”” or a bipolar planetary nebula. Another more revealing name might be the “Twin Jet Nebula.”” If the nebula is sliced across the star, each side of it appears much like a pair of exhausts from jet engines. Indeed, because of the nebula's shape and the measured velocity of the gas, in excess of 200 miles per second, astronomers believe that the description as a super - super - sonic jet exhaust is quite apt. Ground - based studies have shown that the nebula's size increases with time, suggesting that the stellar outburst that formed the lobes occurred just 1,200 years ago. The central star in M2 - 9 is known to be one of a very close pair which orbit one another at perilously close distances. It is even possible that one star is being engulfed by the other. Astronomers suspect the gravity of one star pulls weakly bound gas from the surface of the other and flings it into a thin, dense disk which su

Planetary nebula M2 - 9 in Ophiuchus/HST - M2 - 9 is a striking example of a “” butterfly”” or a bipolar planetary nebula. Another more revealing name might be the “Twin Jet Nebula.”” If the nebula is sliced across the star, each side of it appears much like a pair of exhausts from jet engines. Indeed, because of the nebula's shape and the measured velocity of the gas, in excess of 200 miles per second, astronomers believe that the description as a super - super - sonic jet exhaust is quite apt. Ground - based studies have shown that the nebula's size increases with time, suggesting that the stellar outburst that formed the lobes occurred just 1,200 years ago. The central star in M2 - 9 is known to be one of a very close pair which orbit one another at perilously close distances. It is even possible that one star is being engulfed by the other. Astronomers suspect the gravity of one star pulls weakly bound gas from the surface of the other and flings it into a thin, dense disk which su

PIX4623720

Pistol star - Massive star in the constellation Sagittarius - The massive star Pistol star in Sagittarius - Pistol star is one of the most massive stars in our galaxy. Located about 25,000 years ago - the light of the Earth in the constellation of Sagittarius, this star shines like 10 million Sun consuming in six seconds as much energy as our star in a year. This star is masked by the numerous interstellar dust present in the Sagittarius near the galactic center and appears only in infrared wavelengths, as in this image obtained with the NICMOS instrument embark on the Hubble space telescope. The nebula that surrounds it (in the shape of a gun), extends over 4 years - light. Image obtained in 1997. Astronomers using Nasa's Hubble Space Telescope have identified what may be the most luminous star known “” a celestial mammoth which releases up to 10 million times the power of the Sun and is big enough to fill the diameter of Earth's orbit. The star unleashes as much energy in six seconds

Pistol star - Massive star in the constellation Sagittarius - The massive star Pistol star in Sagittarius - Pistol star is one of the most massive stars in our galaxy. Located about 25,000 years ago - the light of the Earth in the constellation of Sagittarius, this star shines like 10 million Sun consuming in six seconds as much energy as our star in a year. This star is masked by the numerous interstellar dust present in the Sagittarius near the galactic center and appears only in infrared wavelengths, as in this image obtained with the NICMOS instrument embark on the Hubble space telescope. The nebula that surrounds it (in the shape of a gun), extends over 4 years - light. Image obtained in 1997. Astronomers using Nasa's Hubble Space Telescope have identified what may be the most luminous star known “” a celestial mammoth which releases up to 10 million times the power of the Sun and is big enough to fill the diameter of Earth's orbit. The star unleashes as much energy in six seconds

PIX4572084

Meteor Crater - Arizona - USA - Impact Crater Meteor Crater, Arizona, USA. This crater measures 1,200 metres in diameter and 180 metres in depth. It would have formed about 50,000 years ago as a result of the impact of an asteroid 30 to 50 meters in diameter. A panorama of Meteor Crater, near Flagstaff, Arizona. It was formed about 50,000 years ago following the impact of a 30 to 50 meter diameter asteroid; its diameter currently stands at 1,2 km and its depth is about 180m

Meteor Crater - Arizona - USA - Impact Crater Meteor Crater, Arizona, USA. This crater measures 1,200 metres in diameter and 180 metres in depth. It would have formed about 50,000 years ago as a result of the impact of an asteroid 30 to 50 meters in diameter. A panorama of Meteor Crater, near Flagstaff, Arizona. It was formed about 50,000 years ago following the impact of a 30 to 50 meter diameter asteroid; its diameter currently stands at 1,2 km and its depth is about 180m

Alex Conu

PIX4661536

Meteor Crater - Arizona - USA - Anaglyph - Meteor Crater - Arizona - USA - Anaglyph - Impact Crater Meteor Crater, Arizona, USA. This crater measures 1,200 metres in diameter and 180 metres in depth. It would have formed about 50,000 years ago as a result of the impact of an asteroid 30 to 50 meters in diameter. It was formed about 50,000 years ago following the impact of a 30 to 50 meter diameter asteroid; its diameter currently stands at 1,2 km and its depth is about 180m. Anaglyph image, use 3D Eyeglasse

Meteor Crater - Arizona - USA - Anaglyph - Meteor Crater - Arizona - USA - Anaglyph - Impact Crater Meteor Crater, Arizona, USA. This crater measures 1,200 metres in diameter and 180 metres in depth. It would have formed about 50,000 years ago as a result of the impact of an asteroid 30 to 50 meters in diameter. It was formed about 50,000 years ago following the impact of a 30 to 50 meter diameter asteroid; its diameter currently stands at 1,2 km and its depth is about 180m. Anaglyph image, use 3D Eyeglasse

Stefan Seip

PIX4630534

Tourist at Meteor Crater - Tourist at Meteor Crater, Arizona, USA. This crater measures 1,200 metres in diameter and 180 metres in depth. It would have formed about 50,000 years ago as a result of the impact of an asteroid 30 to 50 meters in diameter. A female tourist on the rim of Meteor Crater. Meteor Crater, near Flagstaff, Arizona was formed about 50,000 years ago following the impact of a 30 to 50 meter diameter asteroid; its diameter currently stands at 1,2 km and its depth is about 180m

Tourist at Meteor Crater - Tourist at Meteor Crater, Arizona, USA. This crater measures 1,200 metres in diameter and 180 metres in depth. It would have formed about 50,000 years ago as a result of the impact of an asteroid 30 to 50 meters in diameter. A female tourist on the rim of Meteor Crater. Meteor Crater, near Flagstaff, Arizona was formed about 50,000 years ago following the impact of a 30 to 50 meter diameter asteroid; its diameter currently stands at 1,2 km and its depth is about 180m

Alex Conu

PIX4661539

Titan Exploration - Illustration - Titan's low surface gravity - Astronauts on the surface of Titan. On Saturn's satellite, gravity is lower than on the Moon, an astronaut weights ten times less than on Earth. While Titan is one of the largest terrestrial worlds in the Solar System, larger even than any of the known dwarf planets, the pull of gravity at its surface is only 1/10th the Earth's. Titan's surface gravity is lower than even the Moon's (which is 1/6th the Earth's), and yet Titan's diameter is about 50% larger than the Moon's.

Titan Exploration - Illustration - Titan's low surface gravity - Astronauts on the surface of Titan. On Saturn's satellite, gravity is lower than on the Moon, an astronaut weights ten times less than on Earth. While Titan is one of the largest terrestrial worlds in the Solar System, larger even than any of the known dwarf planets, the pull of gravity at its surface is only 1/10th the Earth's. Titan's surface gravity is lower than even the Moon's (which is 1/6th the Earth's), and yet Titan's diameter is about 50% larger than the Moon's.

Walter B Myers

PIX4626133

Barree spiral galaxy NGC 1365 in the Furnace - Barred spiral galaxy NGC 1365 in Fornax - NGC 1365 is a barree spiral galaxy that extends over 200,000 years - light. Located 60 million years ago - light, it belongs to the cluster of galaxies of the Furnace. Image obtained in 1999 by the European telescope Antu of the VLT in Chile. NGC 1365 is one of the most prominent “” barred”” galaxies in the sky. It is a supergiant galaxy with a diameter of about 200,000 light - years, seen in the direction of the southern constellation Fornax. It is a major member of the Fornax Cluster of Galaxies. The distance is about 60 million light - years. A massive straight bar runs through this galaxy and contains the nucleus at the centre. It consists mostly of older stars that give a reddish colour to the bar.The gravitational perturbation from the bar causes interstellar gas and dust clouds to form a pair of spiral arms that extend from the ends of the bar. Young luminous hot stars, born out of the inter

Barree spiral galaxy NGC 1365 in the Furnace - Barred spiral galaxy NGC 1365 in Fornax - NGC 1365 is a barree spiral galaxy that extends over 200,000 years - light. Located 60 million years ago - light, it belongs to the cluster of galaxies of the Furnace. Image obtained in 1999 by the European telescope Antu of the VLT in Chile. NGC 1365 is one of the most prominent “” barred”” galaxies in the sky. It is a supergiant galaxy with a diameter of about 200,000 light - years, seen in the direction of the southern constellation Fornax. It is a major member of the Fornax Cluster of Galaxies. The distance is about 60 million light - years. A massive straight bar runs through this galaxy and contains the nucleus at the centre. It consists mostly of older stars that give a reddish colour to the bar.The gravitational perturbation from the bar causes interstellar gas and dust clouds to form a pair of spiral arms that extend from the ends of the bar. Young luminous hot stars, born out of the inter

PIX4609836

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