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A Homo habilis hammerstone

A Homo habilis hammerstone

NHM1452631

Homo habilis in action

Homo habilis in action

McBride, Angus (1931-2007)

NHM1452632

Homo habilis in action

Homo habilis in action

McBride, Angus (1931-2007)

NHM1452633

Homo habilis in action

Homo habilis in action

McBride, Angus (1931-2007)

NHM1450193

Homo habilis in action

Homo habilis in action

NHM1458612

Elizabeth Taylor Wearing For The First Time her 6 Millions Diamond (Taylor-Burton Diamond) November 17, 1969 at Scorpios Ball in Monte-Carlo (b/w photo)

Elizabeth Taylor Wearing For The First Time her 6 Millions Diamond (Taylor-Burton Diamond) November 17, 1969 at Scorpios Ball in Monte-Carlo (b/w photo)

XRA1656562

One hundred million billion pengd note

One hundred million billion pengd note

UIG2910265

A child is being fed with vitamin A capsule at a health care centre in Chittagong, Bangladesh. June 6, 2009. About 20 million children of 1-5 years and 10.9 million children of 2-5 years will be fed Vitamin A capsule and de-worming tablets from the 120,000 permanent and 20,000 mobile centers throughout the country. (photo)

A child is being fed with vitamin A capsule at a health care centre in Chittagong, Bangladesh. June 6, 2009. About 20 million children of 1-5 years and 10.9 million children of 2-5 years will be fed Vitamin A capsule and de-worming tablets from the 120,000 permanent and 20,000 mobile centers throughout the country. (photo)

UIG801057

Carboniferous landscape - Calamites & Drepanophycus - Carboniferous landscape with calamites of different sizes and a variety of Drepanophycus, a smaller plant that appeared 20 million years ago, and coexisted with calamites for 35 million years. Calamites of varying size (10 to 50 feet tall) populate lowlands near the brackish waters of an inland sea. Closer to the ground at about 6 feet tall is a variety of Drepanophycus, ancient plants that preceded the Calamites by about 20 million years and coexisted with them for another 35 million years

Carboniferous landscape - Calamites & Drepanophycus - Carboniferous landscape with calamites of different sizes and a variety of Drepanophycus, a smaller plant that appeared 20 million years ago, and coexisted with calamites for 35 million years. Calamites of varying size (10 to 50 feet tall) populate lowlands near the brackish waters of an inland sea. Closer to the ground at about 6 feet tall is a variety of Drepanophycus, ancient plants that preceded the Calamites by about 20 million years and coexisted with them for another 35 million years

Walter B Myers

PIX4632910

Impact Crater Gosses Bluff, Australia - Impact Crater Gosses Bluff, Australia, seen by the International Space Station on February 6, 2007. Its diameter is 5 km; it would have been formed about 142 million years ago.

Impact Crater Gosses Bluff, Australia - Impact Crater Gosses Bluff, Australia, seen by the International Space Station on February 6, 2007. Its diameter is 5 km; it would have been formed about 142 million years ago.

PIX4630617

Kasha-Katuwe Tent Rocks National Monument, New Mexico Was Designated A National Monument In January 17, 2001. The Cone Shaped Tent Rock Formations Were Formed By Volcanic Eruptions About 6 To 7 Million Years Ago.

Kasha-Katuwe Tent Rocks National Monument, New Mexico Was Designated A National Monument In January 17, 2001. The Cone Shaped Tent Rock Formations Were Formed By Volcanic Eruptions About 6 To 7 Million Years Ago.

UIG536122

Kasha-Katuwe Tent Rocks National Monument, New Mexico Was Designated A National Monument In January 17, 2001. The Cone Shaped Tent Rock Formations Were Formed By Volcanic Eruptions About 6 To 7 Million Years Ago.

Kasha-Katuwe Tent Rocks National Monument, New Mexico Was Designated A National Monument In January 17, 2001. The Cone Shaped Tent Rock Formations Were Formed By Volcanic Eruptions About 6 To 7 Million Years Ago.

UIG536116

Kasha-Katuwe Tent Rocks National Monument, New Mexico Was Designated A National Monument In January 17, 2001. The Cone Shaped Tent Rock Formations Were Formed By Volcanic Eruptions About 6 To 7 Million Years Ago.

Kasha-Katuwe Tent Rocks National Monument, New Mexico Was Designated A National Monument In January 17, 2001. The Cone Shaped Tent Rock Formations Were Formed By Volcanic Eruptions About 6 To 7 Million Years Ago.

UIG536119

Dresden, historical, Economy Industry, Companies Leipzig Strass 6, former …, 1993 (photo)

Dresden, historical, Economy Industry, Companies Leipzig Strass 6, former …, 1993 (photo)

Sächsische Zeitung

IMO8754896

Psittacosaurus and pond - The psittacosaur (Psittacosaurus) is a ceratopsian dinosaur from the early Cretace that lived in Asia about 130 to 100 million years ago. A Jurassic Psittacosaurus prepares to dine on a scrubland cycad 130 million years ago in what is today central Asia. Psittacosaurus was one of the earliest known ceratopsians, a family of horned, frilled dinosaurs that includes the better known Triceratops. Psittacosaurus was about 3 to 6 feet long and weighed 50 to 175 pounds, depending on species. At least one species had long, quill-like structures on its tail and lower back. With a parrot-like beak it is believed that Psittacosaurus was a plant-eater

Psittacosaurus and pond - The psittacosaur (Psittacosaurus) is a ceratopsian dinosaur from the early Cretace that lived in Asia about 130 to 100 million years ago. A Jurassic Psittacosaurus prepares to dine on a scrubland cycad 130 million years ago in what is today central Asia. Psittacosaurus was one of the earliest known ceratopsians, a family of horned, frilled dinosaurs that includes the better known Triceratops. Psittacosaurus was about 3 to 6 feet long and weighed 50 to 175 pounds, depending on species. At least one species had long, quill-like structures on its tail and lower back. With a parrot-like beak it is believed that Psittacosaurus was a plant-eater

Walter B Myers

PIX4662900

Women members lead a 1928 Ku Klux Klan parade on Pennsylvania Avenue. After D. W. Griffith's film 'Birth of A Nation', portrayed Klansmen as heroes, the KKK was revived and grew to an estimated membership between 6 to 3 million at its height in 1925.

Women members lead a 1928 Ku Klux Klan parade on Pennsylvania Avenue. After D. W. Griffith's film 'Birth of A Nation', portrayed Klansmen as heroes, the KKK was revived and grew to an estimated membership between 6 to 3 million at its height in 1925.

EVB2947505

Cryolophosaurus - Cryolophosaurus (Cryolophosaurus ellioti) is the first dinosaur found in Antarctica by paleontologists. Measuring 6 to 8 metres long, this carnivore lived at the beginning of the Jurassic about 190 million years ago. Cryolophosaurus ellioti is one of the few dinosaurs known from Antarctica

Cryolophosaurus - Cryolophosaurus (Cryolophosaurus ellioti) is the first dinosaur found in Antarctica by paleontologists. Measuring 6 to 8 metres long, this carnivore lived at the beginning of the Jurassic about 190 million years ago. Cryolophosaurus ellioti is one of the few dinosaurs known from Antarctica

Julius Csotonyi

PIX4661949

Spiral galaxy NGC 6946 in Cephee - Spiral galaxy NGC 6946 in Cepheus - Spiral galaxy NGC 6946 located about 10 million years ago - light in Cephee. Image obtained with a 50 cm telescope. 6 hours of installation

Spiral galaxy NGC 6946 in Cephee - Spiral galaxy NGC 6946 in Cepheus - Spiral galaxy NGC 6946 located about 10 million years ago - light in Cephee. Image obtained with a 50 cm telescope. 6 hours of installation

R. Gendler

PIX4613048

General Dwight Eisenhower raises both arms and acknowledges the New York crowd's cheers, June 6, 1945

General Dwight Eisenhower raises both arms and acknowledges the New York crowd's cheers, June 6, 1945

EVB2922807

Camptosaurus - Artist - Camptosaurus (or twisted lezard “”) was a genus of dinosaurs of the order of ornithisdogs. It was up to 6 m tall, weighed about 500 kg and lived in the upper Jurassic and lower cretace (about 160 to 140 million years ago) in England, France and the United States. In the sky fly two pterosaurs. Plant-eating ornithischian dinosaurs of the genus Camptosaurus graze in a forest of cycads and ferns 160 million years ago in what is today Wyoming. In the cloudy sky above a pair of pterosaurs soar by. Adult Camptosaurus grew to 26 feet long, nearly seven feet tall at the hip, and weighed over 1,500 pounds. These dinosaurs had sturdy beaks in addition to closely packed teeth which would have helped them to dine on tough Jurassic vegetation.

Camptosaurus - Artist - Camptosaurus (or twisted lezard “”) was a genus of dinosaurs of the order of ornithisdogs. It was up to 6 m tall, weighed about 500 kg and lived in the upper Jurassic and lower cretace (about 160 to 140 million years ago) in England, France and the United States. In the sky fly two pterosaurs. Plant-eating ornithischian dinosaurs of the genus Camptosaurus graze in a forest of cycads and ferns 160 million years ago in what is today Wyoming. In the cloudy sky above a pair of pterosaurs soar by. Adult Camptosaurus grew to 26 feet long, nearly seven feet tall at the hip, and weighed over 1,500 pounds. These dinosaurs had sturdy beaks in addition to closely packed teeth which would have helped them to dine on tough Jurassic vegetation.

Walter B Myers

PIX4662115

A Malaysian bidder, Angela Ng, looks at gold plated-toiletry items on sale at a multi-million dollar.., 2001 (photo)

A Malaysian bidder, Angela Ng, looks at gold plated-toiletry items on sale at a multi-million dollar.., 2001 (photo)

Zainal Abd Halim

REU7465556

Diabloceratops and White Rhinoceros - Comparison - Diabloceratops & White Rhinoceros compared - An adult Diabloceratops who lived 70 million years ago is compared to today's adult White Rhinoceros (Ceratotherium simum). The Diabloceratops was 2.5 metres high at the withers and weighed 3.6 tonnes, while the white rhinoceros was 1.8 metres high at the withers and weighed 3.2 tonnes. An adult Diabloceratops from 70 million years ago is compared to a modern adult White Rhinoceros (Ceratotherium simum). The Diabloceratops is a little over 8 feet tall at the shoulder and weighs 8,000 pounds*, while the White Rhinoceros is 6 feet tall at the shoulder and weighs 7,000 pounds.* Values are estimates only based upon available paleontological data

Diabloceratops and White Rhinoceros - Comparison - Diabloceratops & White Rhinoceros compared - An adult Diabloceratops who lived 70 million years ago is compared to today's adult White Rhinoceros (Ceratotherium simum). The Diabloceratops was 2.5 metres high at the withers and weighed 3.6 tonnes, while the white rhinoceros was 1.8 metres high at the withers and weighed 3.2 tonnes. An adult Diabloceratops from 70 million years ago is compared to a modern adult White Rhinoceros (Ceratotherium simum). The Diabloceratops is a little over 8 feet tall at the shoulder and weighs 8,000 pounds*, while the White Rhinoceros is 6 feet tall at the shoulder and weighs 7,000 pounds.* Values are estimates only based upon available paleontological data

Walter B Myers

PIX4663175

Cotylorhynchus - Cotylorhynchus was a large mammalian reptile (Synapside, Pelycosaur) living herbivorous from early Permian to mid-Permian (299 to 265 million years). They were the largest terrestrial animals of their time, measuring 6 metres long and weighing two tons. Giant, 20-foot-long and one-ton synapsids of the genus Cotylorhynchus forage in an Early Permian swamp 275 million years ago in what is today North America. Also in this image on the lower left is a 3-foot long lepospondyl amphibian of the genus Diplocaulus. Vegetation includes ferns and horsetails in the foreground and on the horizon is a forest of ginkgos. Cotylorhynchus is the largest known non-mammalian synapsid and was the largest land animal of its time. An herbivore, Cotylorhynchus had a massive barrel-shaped body and limbs with a relatively small head, making it perhaps one of the most unattractive land animals to have ever walked the Earth. Standing about 6 feet tall at the shoulder Cotylorhynchus probably had no predators; even the fierce Dimetrodon (also a synapsid) weighed little more than 300 pounds compared to Cotylorhynchus' 2,000 — Cotylorhynchus - Cotylorhynchus was a large mammalian reptile (Synapside, Pelycosaur) living herbivorous from early Permian to mid-Permian (299 to 265 million years). They were the largest terrestrial animals of their time, measuring 6 metres long and weighing two tons. Giant, 20-foot-long and one-ton synapsids of the genus Cotylorhynchus forage in an Early Permian swamp 275 million years ago in what is today North America. Also in this image on the lower left is a 3-foot long lepospondyl amphibian of the genus Diplocaulus. Vegetation includes ferns and horsetails in the foreground and on the horizon is a forest of ginkgos. Cotylorhynchus is the largest known non-mammalian synapsid and was the largest land animal of its time. An herbivore, Cotylorhynchus had a massive barrel-shaped body and limbs with a relatively small head, making it perhaps one of the most unattractive land animals to have ever walked the Earth. Standing about 6 feet tall at the shoulder Cotylorhynchus probably had

Cotylorhynchus - Cotylorhynchus was a large mammalian reptile (Synapside, Pelycosaur) living herbivorous from early Permian to mid-Permian (299 to 265 million years). They were the largest terrestrial animals of their time, measuring 6 metres long and weighing two tons. Giant, 20-foot-long and one-ton synapsids of the genus Cotylorhynchus forage in an Early Permian swamp 275 million years ago in what is today North America. Also in this image on the lower left is a 3-foot long lepospondyl amphibian of the genus Diplocaulus. Vegetation includes ferns and horsetails in the foreground and on the horizon is a forest of ginkgos. Cotylorhynchus is the largest known non-mammalian synapsid and was the largest land animal of its time. An herbivore, Cotylorhynchus had a massive barrel-shaped body and limbs with a relatively small head, making it perhaps one of the most unattractive land animals to have ever walked the Earth. Standing about 6 feet tall at the shoulder Cotylorhynchus probably had

Walter B Myers

PIX4661707

The First Trees on Earth - Artist View - First Trees - Artist view - 385 million years ago, in the upper Devonian, the first trees began to appear on Earth. In this illustration, the archaeopteris, considered the first tree, is present at different stages of its evolution, with on the left a young specimen of 6 metres, in the centre a tree twice as large, on the right, an even older specimen. At the extreme right, a strain of an old Archaeopteris collapse. 385 million years ago, near the end of the Devonian period, the first trees began to populate the Earth. Considered the first modern trees, the Archaeopteris were a part of the Earth's primitive forests for the next 25 million years. Unlike the trees we know today, Archaeopteris was in fact a primitive fern that reproduced by means of spores instead of seeds. While terrestrial plants had been around for 130 million years prior to Archaeopteris, this was the first plant to solve the biomechanical challenges of supporting and nurturing ever larger sizes, enabling these Archaeopteris to grow to heights of 70 feet and more, over twice the height of the Calamites. In this image, four stages of the life of the Archaeopteris are illustrated. On the far left nearest our vantage point is a young, 20 - foot Archaeopteris, and in the center at twice that height is a medium - aged Archaeopteris, and on the right is a fully mature specimen. Furthest right is the collapsed and decaying trunk of a mature tree, a contribution the biomassy that will eventually become the oil, coal and natural gas we exploit today — The First Trees on Earth - Artist View - First Trees - Artist view - 385 million years ago, in the upper Devonian, the first trees began to appear on Earth. In this illustration, the archaeopteris, considered the first tree, is present at different stages of its evolution, with on the left a young specimen of 6 metres, in the centre a tree twice as large, on the right, an even older specimen. At the extreme right, a strain of an old Archaeopteris collapse. 385 million years ago, near the end of the Devonian period, the first trees began to populate the Earth. Considered the first modern trees, the Archaeopteris were a part of the Earth's primitive forests for the next 25 million years. Unlike the trees we know today, Archaeopteris was in fact a primitive fern that reproduced by means of spores instead of seeds. While terrestrial plants had been around for 130 million years prior to Archaeopteris, this was the first plant to solve the biomechanical challenges of supporting and nurturing

The First Trees on Earth - Artist View - First Trees - Artist view - 385 million years ago, in the upper Devonian, the first trees began to appear on Earth. In this illustration, the archaeopteris, considered the first tree, is present at different stages of its evolution, with on the left a young specimen of 6 metres, in the centre a tree twice as large, on the right, an even older specimen. At the extreme right, a strain of an old Archaeopteris collapse. 385 million years ago, near the end of the Devonian period, the first trees began to populate the Earth. Considered the first modern trees, the Archaeopteris were a part of the Earth's primitive forests for the next 25 million years. Unlike the trees we know today, Archaeopteris was in fact a primitive fern that reproduced by means of spores instead of seeds. While terrestrial plants had been around for 130 million years prior to Archaeopteris, this was the first plant to solve the biomechanical challenges of supporting and nurturing

Walter B Myers

PIX4632789

Galaxies NGC 5078 and IC 879 in Hydra - Galaxies NGC 5078 and IC 879 in Hydra - NGC 5078 is a spiral galaxy located about 95 million years ago - light. A small galaxy, IC 879, on its left, is probably interacting with it. Image obtained with a 35 cm telescope, 6 hours of poses. NGC 5078 is a lenticular (lens - shaped) galaxy crossed by a distinct dusty band which is seen against the bright background of the galaxy itself. The dust lane is warped and broadened, probably by interaction with the faint companion galaxy IC 879, which is itself distorted into an 'S' shape by the interaction. The galaxies are about 95 million light years distant. Image taken with 14.5”” RCOS telescope, 6 Hours of exposure

Galaxies NGC 5078 and IC 879 in Hydra - Galaxies NGC 5078 and IC 879 in Hydra - NGC 5078 is a spiral galaxy located about 95 million years ago - light. A small galaxy, IC 879, on its left, is probably interacting with it. Image obtained with a 35 cm telescope, 6 hours of poses. NGC 5078 is a lenticular (lens - shaped) galaxy crossed by a distinct dusty band which is seen against the bright background of the galaxy itself. The dust lane is warped and broadened, probably by interaction with the faint companion galaxy IC 879, which is itself distorted into an 'S' shape by the interaction. The galaxies are about 95 million light years distant. Image taken with 14.5”” RCOS telescope, 6 Hours of exposure

R. Gendler

PIX4612142

Zuniceratops and White Rhinoceros - Comparison - Zuniceratops & White Rhinoceros compared - An adult Zuniceratops who lived 90 million years ago is compared to today's adult white rhinoceros (Ceratotherium simum). The Zuniceratops was 90 centimetres high at the withers and weighed 110 kilograms, while the white rhinoceros was 1.8 metres high at the withers and weighed 3.2 tons. An adult Zuniceratops from 90 million years ago is compared to a modern adult White Rhinoceros (Ceratotherium simum). The Zuniceratops is 3 feet tall at the shoulder and weighs 250 pounds*, while the White Rhinoceros is 6 feet tall at the shoulder and weighs 7,000 pounds.* Values are estimates only based upon available paleontological data

Zuniceratops and White Rhinoceros - Comparison - Zuniceratops & White Rhinoceros compared - An adult Zuniceratops who lived 90 million years ago is compared to today's adult white rhinoceros (Ceratotherium simum). The Zuniceratops was 90 centimetres high at the withers and weighed 110 kilograms, while the white rhinoceros was 1.8 metres high at the withers and weighed 3.2 tons. An adult Zuniceratops from 90 million years ago is compared to a modern adult White Rhinoceros (Ceratotherium simum). The Zuniceratops is 3 feet tall at the shoulder and weighs 250 pounds*, while the White Rhinoceros is 6 feet tall at the shoulder and weighs 7,000 pounds.* Values are estimates only based upon available paleontological data

Walter B Myers

PIX4663005

Einiosaurus and White Rhinoceros - Comparison - Einiosaurus & White Rhinoceros compared - An adult Einiosaurus who lived 77 million years ago is compared to today's adult white rhinoceros (Ceratotherium simum). The Einiosaurus was 2 metres high at the withers and weighed 3.6 tonnes, while the white rhinoceros was 1.8 metres high at the withers and weighed 3.2 tonnes. An adult Einiosaurus from 77 million years ago is compared to a modern adult White Rhinoceros (Ceratotherium simum). The Einiosaurus is 6 and a half feet tall at the shoulder and weighs 8,000 pounds*, while the White Rhinoceros is 6 feet tall at the shoulder and weighs 7,000 pounds.* Values are estimates only based upon available paleontological data

Einiosaurus and White Rhinoceros - Comparison - Einiosaurus & White Rhinoceros compared - An adult Einiosaurus who lived 77 million years ago is compared to today's adult white rhinoceros (Ceratotherium simum). The Einiosaurus was 2 metres high at the withers and weighed 3.6 tonnes, while the white rhinoceros was 1.8 metres high at the withers and weighed 3.2 tonnes. An adult Einiosaurus from 77 million years ago is compared to a modern adult White Rhinoceros (Ceratotherium simum). The Einiosaurus is 6 and a half feet tall at the shoulder and weighs 8,000 pounds*, while the White Rhinoceros is 6 feet tall at the shoulder and weighs 7,000 pounds.* Values are estimates only based upon available paleontological data

Walter B Myers

PIX4662925

Torosaurus and White Rhinoceros - Comparison - Torosaurus & White Rhinoceros compared - An adult Torosaurus who lived 75 million years ago is compared to today's adult white rhinoceros (Ceratotherium simum). The Torosaurus was 2 metres high at the withers and weighed 4.5 tonnes, while the white rhinoceros was 1.8 metres high at the withers and weighed 3.2 tonnes. An adult Torosaurus from 75 million years ago is compared to a modern adult White Rhinoceros (Ceratotherium simum). The Torosaurus is 6 and a half feet tall at the shoulder and weighs 10,000 pounds*, while the White Rhinoceros is 6 feet tall at the shoulder and weighs 7,000 pounds.* Values are estimates only based upon available paleontological data

Torosaurus and White Rhinoceros - Comparison - Torosaurus & White Rhinoceros compared - An adult Torosaurus who lived 75 million years ago is compared to today's adult white rhinoceros (Ceratotherium simum). The Torosaurus was 2 metres high at the withers and weighed 4.5 tonnes, while the white rhinoceros was 1.8 metres high at the withers and weighed 3.2 tonnes. An adult Torosaurus from 75 million years ago is compared to a modern adult White Rhinoceros (Ceratotherium simum). The Torosaurus is 6 and a half feet tall at the shoulder and weighs 10,000 pounds*, while the White Rhinoceros is 6 feet tall at the shoulder and weighs 7,000 pounds.* Values are estimates only based upon available paleontological data

Walter B Myers

PIX4662994

Elasmotherium and White Rhinoceros - Comparison - Elasmotherium and Rhino Compared - An adult Elasmotherium that lived 2 million years ago is compared to today's adult White Rhinoceros (Ceratotherium simum). Elasmotherium was 2.1 metres high at withers and weighed 3.6 tonnes, while white rhinoceros was 1.8 metres high at withers and 3.2 tonnes. An adult Elasmotherium from 2 million years ago is compared to a modern adult White Rhinoceros (Ceratotherium simum). The Elasmotherium is over 7 feet tall at the shoulder and weighs 8,000 pounds*, while the White Rhinoceros is 6 feet tall at the shoulder and weighs 7,000 pounds.* Values are estimates only based upon available paleontological data

Elasmotherium and White Rhinoceros - Comparison - Elasmotherium and Rhino Compared - An adult Elasmotherium that lived 2 million years ago is compared to today's adult White Rhinoceros (Ceratotherium simum). Elasmotherium was 2.1 metres high at withers and weighed 3.6 tonnes, while white rhinoceros was 1.8 metres high at withers and 3.2 tonnes. An adult Elasmotherium from 2 million years ago is compared to a modern adult White Rhinoceros (Ceratotherium simum). The Elasmotherium is over 7 feet tall at the shoulder and weighs 8,000 pounds*, while the White Rhinoceros is 6 feet tall at the shoulder and weighs 7,000 pounds.* Values are estimates only based upon available paleontological data

Walter B Myers

PIX4664296

Brontotherium and White Rhinoceros - Comparison - Brontotherium and Rhino Compared - An adult Brontotherium who lived 35 million years ago is compared to today's adult White Rhinoceros (Ceratotherium simum). The Brontotherium was 2.4 metres high at the withers and weighed more than 4 tonnes, while the white rhinoceros was 1.8 metres high at the withers and weighed 3.2 tonnes. An adult Brontotherium from 35 million years ago is compared to a modern adult White Rhinoceros (Ceratotherium simum). The Brontotherium is 8 feet tall at the shoulder and weighs 9,000 pounds*, while the White Rhinoceros is 6 feet tall at the shoulder and weighs 7,000 pounds.* Values are estimates only based upon available paleontological data

Brontotherium and White Rhinoceros - Comparison - Brontotherium and Rhino Compared - An adult Brontotherium who lived 35 million years ago is compared to today's adult White Rhinoceros (Ceratotherium simum). The Brontotherium was 2.4 metres high at the withers and weighed more than 4 tonnes, while the white rhinoceros was 1.8 metres high at the withers and weighed 3.2 tonnes. An adult Brontotherium from 35 million years ago is compared to a modern adult White Rhinoceros (Ceratotherium simum). The Brontotherium is 8 feet tall at the shoulder and weighs 9,000 pounds*, while the White Rhinoceros is 6 feet tall at the shoulder and weighs 7,000 pounds.* Values are estimates only based upon available paleontological data

Walter B Myers

PIX4664417

Auctioneers point to the successful bidder at a multi-million dollar auction being held in Brunei, A.., 2001 (photo)

Auctioneers point to the successful bidder at a multi-million dollar auction being held in Brunei, A.., 2001 (photo)

Zainal Abd Halim

REU7457528

Pentaceratops and White Rhinoceros - Comparison - Pentaceratops & White Rhinoceros compared - An adult Pentaceratops who lived 75 million years ago is compared to today's adult white rhinoceros (Ceratotherium simum). The Pentaceratops was 2.4 metres high at the withers and weighed 5.9 tonnes, while the white rhinoceros was 1.8 metres high at the withers and weighed 3.2 tonnes. An adult Pentaceratops from 75 million years ago is compared to a modern adult White Rhinoceros (Ceratotherium simum). The Pentaceratops is 8 feet tall at the shoulder and weighs 13,000 pounds*, while the White Rhinoceros is 6 feet tall at the shoulder and weighs 7,000 pounds.* Values are estimates only based upon available paleontological data

Pentaceratops and White Rhinoceros - Comparison - Pentaceratops & White Rhinoceros compared - An adult Pentaceratops who lived 75 million years ago is compared to today's adult white rhinoceros (Ceratotherium simum). The Pentaceratops was 2.4 metres high at the withers and weighed 5.9 tonnes, while the white rhinoceros was 1.8 metres high at the withers and weighed 3.2 tonnes. An adult Pentaceratops from 75 million years ago is compared to a modern adult White Rhinoceros (Ceratotherium simum). The Pentaceratops is 8 feet tall at the shoulder and weighs 13,000 pounds*, while the White Rhinoceros is 6 feet tall at the shoulder and weighs 7,000 pounds.* Values are estimates only based upon available paleontological data

Walter B Myers

PIX4663145

Two child labourers are working on a autorickshaw at a road side auto rickshaw repairing centre in Kolkata, India. About one and half of India's 230 million children age 6-14 do not attend school and qualify as child labourers. For many, poverty, lack of awarness among parents, inadequacy of school facilities and teachers, ineffective enforcement of child labour laws block access to education. India, September 5, 2005. (photo)

Two child labourers are working on a autorickshaw at a road side auto rickshaw repairing centre in Kolkata, India. About one and half of India's 230 million children age 6-14 do not attend school and qualify as child labourers. For many, poverty, lack of awarness among parents, inadequacy of school facilities and teachers, ineffective enforcement of child labour laws block access to education. India, September 5, 2005. (photo)

UIG796376

Albertaceratops and White Rhinoceros - Comparison - Albertaceratops & White Rhinoceros compared - An adult Albertaceratops who lived 77 million years ago is compared to today's adult white rhinoceros (Ceratotherium simum). The Albertaceratops was 2 metres high at the withers and weighed more than 2 tonnes, while the white rhinoceros was 1.8 metres high at the withers and weighed more than 3 tonnes. An adult Albertaceratops from 77 million years ago is compared to a modern adult White Rhinoceros (Ceratotherium simum). The Albertaceratops is 6 and a half feet tall at the shoulder and weighs 4,500 pounds*, while the White Rhinoceros is 6 feet tall at the shoulder and weighs 7,000 pounds.* Values are estimates only based upon available paleontological data

Albertaceratops and White Rhinoceros - Comparison - Albertaceratops & White Rhinoceros compared - An adult Albertaceratops who lived 77 million years ago is compared to today's adult white rhinoceros (Ceratotherium simum). The Albertaceratops was 2 metres high at the withers and weighed more than 2 tonnes, while the white rhinoceros was 1.8 metres high at the withers and weighed more than 3 tonnes. An adult Albertaceratops from 77 million years ago is compared to a modern adult White Rhinoceros (Ceratotherium simum). The Albertaceratops is 6 and a half feet tall at the shoulder and weighs 4,500 pounds*, while the White Rhinoceros is 6 feet tall at the shoulder and weighs 7,000 pounds.* Values are estimates only based upon available paleontological data

Walter B Myers

PIX4663084

Nedoceratops and White Rhinoceros - Comparison - Nedoceratops & White Rhinoceros compared - An adult Nedoceratops (Diceratops) who lived 70 million years ago is compared to today's adult white rhinoceros (Ceratotherium simum). The Nedoceratops was 2.5 metres high at the withers and weighed 5.4 tons, while the white rhinoceros was 1.8 metres high at the withers and weighed 3.2 tons. An adult Nedoceratops (FKA Diceratops) from 70 million years ago is compared to a modern adult White Rhinoceros (Ceratotherium simum). The Nedoceratops is a little over 8 feet tall at the shoulder and weighs 12,000 pounds*, while the White Rhinoceros is 6 feet tall at the shoulder and weighs 7,000 pounds.* Values are estimates only based upon available paleontological data

Nedoceratops and White Rhinoceros - Comparison - Nedoceratops & White Rhinoceros compared - An adult Nedoceratops (Diceratops) who lived 70 million years ago is compared to today's adult white rhinoceros (Ceratotherium simum). The Nedoceratops was 2.5 metres high at the withers and weighed 5.4 tons, while the white rhinoceros was 1.8 metres high at the withers and weighed 3.2 tons. An adult Nedoceratops (FKA Diceratops) from 70 million years ago is compared to a modern adult White Rhinoceros (Ceratotherium simum). The Nedoceratops is a little over 8 feet tall at the shoulder and weighs 12,000 pounds*, while the White Rhinoceros is 6 feet tall at the shoulder and weighs 7,000 pounds.* Values are estimates only based upon available paleontological data

Walter B Myers

PIX4662983

Triceratops and White Rhinoceros - Comparison - Triceratops & White Rhinoceros compared - An adult Triceratops who lived 68 million years ago is compared to today's adult white rhinoceros (Ceratotherium simum). The Triceratops was 3 metres high at the withers and weighed 11 tonnes, while the white rhinoceros was 1.8 metres high at the withers and weighed 3.2 tonnes. An adult Triceratops from 68 million years ago is compared to a modern adult White Rhinoceros (Ceratotherium simum). The Triceratops is nearly 10 feet tall at the shoulder and weighs 25,000 pounds*, while the White Rhinoceros is 6 feet tall at the shoulder and weighs 7,000 pounds.* Values are estimates only based upon available paleontological data

Triceratops and White Rhinoceros - Comparison - Triceratops & White Rhinoceros compared - An adult Triceratops who lived 68 million years ago is compared to today's adult white rhinoceros (Ceratotherium simum). The Triceratops was 3 metres high at the withers and weighed 11 tonnes, while the white rhinoceros was 1.8 metres high at the withers and weighed 3.2 tonnes. An adult Triceratops from 68 million years ago is compared to a modern adult White Rhinoceros (Ceratotherium simum). The Triceratops is nearly 10 feet tall at the shoulder and weighs 25,000 pounds*, while the White Rhinoceros is 6 feet tall at the shoulder and weighs 7,000 pounds.* Values are estimates only based upon available paleontological data

Walter B Myers

PIX4663031

Upon Liberation, The SS was put to Work (b/w photo)

Upon Liberation, The SS was put to Work (b/w photo)

UIG2904536

Eurohippus and horse compared - Eurohippus is a prehistoric mammal, ancestor of the horse, living from the middle to the end of the eocene. He is represented here compared to a modern horse. Mature Eurohippus 42 million years ago are compared to a modern adult horse (Equus ferus caballus). Eurohippus is only about 20 inches long and weighs just a few pounds*, while the modern horse is 6 feet tall at the shoulder and weighs 1,000 pounds.* Values are estimates only based upon available paleontological data

Eurohippus and horse compared - Eurohippus is a prehistoric mammal, ancestor of the horse, living from the middle to the end of the eocene. He is represented here compared to a modern horse. Mature Eurohippus 42 million years ago are compared to a modern adult horse (Equus ferus caballus). Eurohippus is only about 20 inches long and weighs just a few pounds*, while the modern horse is 6 feet tall at the shoulder and weighs 1,000 pounds.* Values are estimates only based upon available paleontological data

Walter B Myers

PIX4664469

The Bavarian justice minister of the Christian Social Union Party (CSU), Alfred Sauter drinks beer prior to a news conference in Munich, September 6, 1999 (photo)

The Bavarian justice minister of the Christian Social Union Party (CSU), Alfred Sauter drinks beer prior to a news conference in Munich, September 6, 1999 (photo)

Michael Dalder

REU7448918

Remnants of the Supernova of Sails - The Vela Supernova Remnant - Remnant of the Supernova of Sails. The supernova exploded 12,000 years ago. The rest of the supernova is approximately 815 years away from Earth. Image obtained with FSQ 106 bezel, 6 hours of installation. About 120 centuries ago an inconspicuous star in what is now the constellation of Vela brightened by about 100 million times to rival the Moon as the brightest object in the night sky. This photograph shows a portion of the north - western quadrant of an expanding nebulous shell, which now surrounds the site of the explosion

Remnants of the Supernova of Sails - The Vela Supernova Remnant - Remnant of the Supernova of Sails. The supernova exploded 12,000 years ago. The rest of the supernova is approximately 815 years away from Earth. Image obtained with FSQ 106 bezel, 6 hours of installation. About 120 centuries ago an inconspicuous star in what is now the constellation of Vela brightened by about 100 million times to rival the Moon as the brightest object in the night sky. This photograph shows a portion of the north - western quadrant of an expanding nebulous shell, which now surrounds the site of the explosion

Stephane Guisard

PIX4582851

Remnants of the supernova Cassiopee A en X by Chandra - Object Description: Cas A is the remnant of a star that exploded about 300 years ago. The X - ray image shows an expanding shell of hot gas produced by the explosion. This gaseous shell is about 10 light years in diameter, and has a temperature of about 50 million degrees. Scale: Image is 6 arcmin on a side. Cassiopeia A: The 320 year old remnant of a massive star that exploded. Located in the constellation Cassiopeia, it is 10 light years across and 10,000 light years from Earth

Remnants of the supernova Cassiopee A en X by Chandra - Object Description: Cas A is the remnant of a star that exploded about 300 years ago. The X - ray image shows an expanding shell of hot gas produced by the explosion. This gaseous shell is about 10 light years in diameter, and has a temperature of about 50 million degrees. Scale: Image is 6 arcmin on a side. Cassiopeia A: The 320 year old remnant of a massive star that exploded. Located in the constellation Cassiopeia, it is 10 light years across and 10,000 light years from Earth

PIX4582917

Two small coffins being carried on stretchers to a cemetery in the Volga famine district of Bolshevist Russia, 1921

Two small coffins being carried on stretchers to a cemetery in the Volga famine district of Bolshevist Russia, 1921

Unknown photographer, (20th century)

UIG1574884

Irregular galaxy NGC 6822 in Sagittarius - Irregular galaxy NGC 6822 in Sagittarius - The galaxy NGC 6822 is about 1.6 million years away - light from Earth. She belongs to our local group. Image obtained with a telescope of 35 cm, 12 hours of poses. The irregular dwarf galaxy NGC 6822 is located at only 1,6 million light year. It is a member of our local group and the third nearest galaxy to the Milky Way after the Sagittarius Dwarf Elliptical and the Magellanic Clouds. The galaxy was discovered by Barnard in 1881 using a 6 inch refractor. It is very similar to the LMC with its weak bar and its irregular distribution of bright OB associations and HII regions. In 1925 in a classic paper, Edwin Hubble reported on several bright objects in NGC 6822, later found to represent a grouping of bright star clusters and HII regions. The galaxy is rich in neutral hydrogen gas, the essential fuel of star formation. NGC 6822 started forming stars some 10 billion years ago. Similar to the LMC it has a large intermediate age population of stars of about 3 billion years old, although the galaxy has picked up its star forming rate over the last 100 to 200 million years. Prominent HII regions and scattered clusters of young blue stars are testament to its current constant rate of star formation. Image taken with 14.5”” RCOS telescope, 12 Hours of exposure — Irregular galaxy NGC 6822 in Sagittarius - Irregular galaxy NGC 6822 in Sagittarius - The galaxy NGC 6822 is about 1.6 million years away - light from Earth. She belongs to our local group. Image obtained with a telescope of 35 cm, 12 hours of poses. The irregular dwarf galaxy NGC 6822 is located at only 1,6 million light year. It is a member of our local group and the third nearest galaxy to the Milky Way after the Sagittarius Dwarf Elliptical and the Magellanic Clouds. The galaxy was discovered by Barnard in 1881 using a 6 inch refractor. It is very similar to the LMC with its weak bar and its irregular distribution of bright OB associations and HII regions. In 1925 in a classic paper, Edwin Hubble reported on several bright objects in NGC 6822, later found to represent a grouping of bright star clusters and HII regions. The galaxy is rich in neutral hydrogen gas, the essential fuel of star formation. NGC 6822 started forming stars some 10 billion years ago. Similar to the LMC it has

Irregular galaxy NGC 6822 in Sagittarius - Irregular galaxy NGC 6822 in Sagittarius - The galaxy NGC 6822 is about 1.6 million years away - light from Earth. She belongs to our local group. Image obtained with a telescope of 35 cm, 12 hours of poses. The irregular dwarf galaxy NGC 6822 is located at only 1,6 million light year. It is a member of our local group and the third nearest galaxy to the Milky Way after the Sagittarius Dwarf Elliptical and the Magellanic Clouds. The galaxy was discovered by Barnard in 1881 using a 6 inch refractor. It is very similar to the LMC with its weak bar and its irregular distribution of bright OB associations and HII regions. In 1925 in a classic paper, Edwin Hubble reported on several bright objects in NGC 6822, later found to represent a grouping of bright star clusters and HII regions. The galaxy is rich in neutral hydrogen gas, the essential fuel of star formation. NGC 6822 started forming stars some 10 billion years ago. Similar to the LMC it has

R. Gendler

PIX4613022

Los Angeles

Los Angeles

UTD2840762

Concestor 1

Concestor 1

NHM1457962

Dresden, historical, Prague Street, construction, building site Overview …, 1996 (photo)

Dresden, historical, Prague Street, construction, building site Overview …, 1996 (photo)

Sächsische Zeitung

IMO8754815

POP STARS ATTEND FUNERAL OF PRINCESS IN LONDON, 1997-09-06 (photo)

POP STARS ATTEND FUNERAL OF PRINCESS IN LONDON, 1997-09-06 (photo)

Paul Hackett

REU7930017

Tanystropheus - Two Tanystropheus, six-metre-long marine reptiles, swim in a bay in China 230 million years ago. A pair of 20-foot-long, 300 pound reptiles of the genus Tanystropheus swim in an ocean bay 230 million years ago in what is today China. On the shore are a pair of 6-foot-long bipedal basal saurischian dinosaurs and beyond them on the horizon are 60-foot-tall araucarians, an ancient family of coniferous trees. Horsetails and ferns flourish near the water. Tanystropheus was not a dinosaur, rather it was an ancient marine reptile, an archosaur, that hunted ocean shores at a time when true dinosaurs were only making their first appearance on land. Tanystropheus was likely a fish-eater due to its long, narrow snout and sharp interlocking teeth typical of marine predators. Tanystropheus had an extraordinarily long neck, as long as its body and tail combined, though with only ten vertebrae it was likely not very flexible. Here Tanystropheus are shown extending their head and necks fully out of the water, which may have indeed been possible due to a heavy and muscular counter-balancing tail — Tanystropheus - Two Tanystropheus, six-metre-long marine reptiles, swim in a bay in China 230 million years ago. A pair of 20-foot-long, 300 pound reptiles of the genus Tanystropheus swim in an ocean bay 230 million years ago in what is today China. On the shore are a pair of 6-foot-long bipedal basal saurischian dinosaurs and beyond them on the horizon are 60-foot-tall araucarians, an ancient family of coniferous trees. Horsetails and ferns flourish near the water. Tanystropheus was not a dinosaur, rather it was an ancient marine reptile, an archosaur, that hunted ocean shores at a time when true dinosaurs were only making their first appearance on land. Tanystropheus was likely a fish-eater due to its long, narrow snout and sharp interlocking teeth typical of marine predators. Tanystropheus had an extraordinarily long neck, as long as its body and tail combined, though with only ten vertebrae it was likely not very flexible. Here Tanystropheus are shown extending their head and necks

Tanystropheus - Two Tanystropheus, six-metre-long marine reptiles, swim in a bay in China 230 million years ago. A pair of 20-foot-long, 300 pound reptiles of the genus Tanystropheus swim in an ocean bay 230 million years ago in what is today China. On the shore are a pair of 6-foot-long bipedal basal saurischian dinosaurs and beyond them on the horizon are 60-foot-tall araucarians, an ancient family of coniferous trees. Horsetails and ferns flourish near the water. Tanystropheus was not a dinosaur, rather it was an ancient marine reptile, an archosaur, that hunted ocean shores at a time when true dinosaurs were only making their first appearance on land. Tanystropheus was likely a fish-eater due to its long, narrow snout and sharp interlocking teeth typical of marine predators. Tanystropheus had an extraordinarily long neck, as long as its body and tail combined, though with only ten vertebrae it was likely not very flexible. Here Tanystropheus are shown extending their head and necks

Walter B Myers

PIX4661932

Spiral galaxy of Sombrero M104 in the Virgin - The Sombrero galaxy (M104) in Virgo - The spiral galaxy M104 (NGC 4594, Sombrero galaxy) is located about 28 million years ago - light. Assembled 6 images obtained with the Hubble Space Telescope in May and June 2003. The “” Sombrero”” is located in the constellation Virgo. This magnificent galaxy is almost one - fifth the diameter of the full moon. The team used Hubble's Advanced Camera for Surveys to take six pictures of the galaxy and then stitched them together to create the final composite image. The photo reveals a myriad of stars in a pancake - shaped disk as well as a glowing central bulge of stars

Spiral galaxy of Sombrero M104 in the Virgin - The Sombrero galaxy (M104) in Virgo - The spiral galaxy M104 (NGC 4594, Sombrero galaxy) is located about 28 million years ago - light. Assembled 6 images obtained with the Hubble Space Telescope in May and June 2003. The “” Sombrero”” is located in the constellation Virgo. This magnificent galaxy is almost one - fifth the diameter of the full moon. The team used Hubble's Advanced Camera for Surveys to take six pictures of the galaxy and then stitched them together to create the final composite image. The photo reveals a myriad of stars in a pancake - shaped disk as well as a glowing central bulge of stars

PIX4611616

Colorful Pentaceratops - The Pentaceratops lived 75 million years ago in the southwestern United States. Herbivore, it was 8 meters long and weighed 6 tons. The usefulness of his collar is not clearly defined. A protective shield against predators is a possibility, but relatively fragile, it is likely that it was used as an attribute of visual intimidation to rivals or to attract opposing sex. Although no pigment of colour has been preserved in the fossil remains, it is not unreasonable to imagine that these collars may have been very coloured. A six ton, 27 foot long Pentaceratops wonders a Cretaceous forest 75 million years ago in what is today the southwestern United States. Like the better known Triceratops, Pentaceratops was a Ceratopsid, a large four-legged plant-eating dinosaur characterized by beaks, rows of shearing teeth in the back of the jaw, and elaborate horns and frills. While they resemble defensive shields, the frills are in fact relatively fragile, suggesting that they may have served a purpose other than protecting against a brute force attack. One possibility is that the frills were employed as visual displays in order to intimidate rivals and attract the opposite sex. While no color pigmentation has been preserved in the fossil remains of Ceratopsids, it's not unreasonable to suggest that they may have been very colorful, like many reptiles and birds today — Colorful Pentaceratops - The Pentaceratops lived 75 million years ago in the southwestern United States. Herbivore, it was 8 meters long and weighed 6 tons. The usefulness of his collar is not clearly defined. A protective shield against predators is a possibility, but relatively fragile, it is likely that it was used as an attribute of visual intimidation to rivals or to attract opposing sex. Although no pigment of colour has been preserved in the fossil remains, it is not unreasonable to imagine that these collars may have been very coloured. A six ton, 27 foot long Pentaceratops wonders a Cretaceous forest 75 million years ago in what is today the southwestern United States. Like the better known Triceratops, Pentaceratops was a Ceratopsid, a large four-legged plant-eating dinosaur characterized by beaks, rows of shearing teeth in the back of the jaw, and elaborate horns and frills. While they resemble defensive shields, the frills are in fact relatively fragile, suggesting that the

Colorful Pentaceratops - The Pentaceratops lived 75 million years ago in the southwestern United States. Herbivore, it was 8 meters long and weighed 6 tons. The usefulness of his collar is not clearly defined. A protective shield against predators is a possibility, but relatively fragile, it is likely that it was used as an attribute of visual intimidation to rivals or to attract opposing sex. Although no pigment of colour has been preserved in the fossil remains, it is not unreasonable to imagine that these collars may have been very coloured. A six ton, 27 foot long Pentaceratops wonders a Cretaceous forest 75 million years ago in what is today the southwestern United States. Like the better known Triceratops, Pentaceratops was a Ceratopsid, a large four-legged plant-eating dinosaur characterized by beaks, rows of shearing teeth in the back of the jaw, and elaborate horns and frills. While they resemble defensive shields, the frills are in fact relatively fragile, suggesting that the

Walter B Myers

PIX4663157

Star cluster M46 and planetary nebula NGC 2438 - Open cluster M46 and planetary nebula NGC 2438 - M46 (NGC 2437) is an age cluster located at 5400 years - light. It contains about 500 stars, 150 of which are brilliant. It is about 300 million years old. The planetary nebula NGC 2438 does not appear to belong to this cluster, and must be closer although its distance is unknown. Image obtained by Siding Spring's 3.9m telescope The open cluster NGC 2437 (M46) has an angular diameter of almost half a degree and is quite beautiful in even quite a modest telescope. It has an integrated magnitude of about 6 and so is on the threshold of naked - eye visibility. The cluster is quite old as these things go, about 300 million light years. It is about 5000 light years distant, in the northern part of the constellation of Puppis. Although planetary nebula distances are notoriously difficult to measure, NGC 2438 seems to be in the foreground and is not connected to the cluster. Planetaries are in any case the result of the demise of an old, low mass stars and are thus not seen in relatively young open clusters — Star cluster M46 and planetary nebula NGC 2438 - Open cluster M46 and planetary nebula NGC 2438 - M46 (NGC 2437) is an age cluster located at 5400 years - light. It contains about 500 stars, 150 of which are brilliant. It is about 300 million years old. The planetary nebula NGC 2438 does not appear to belong to this cluster, and must be closer although its distance is unknown. Image obtained by Siding Spring's 3.9m telescope The open cluster NGC 2437 (M46) has an angular diameter of almost half a degree and is quite beautiful in even quite a modest telescope. It has an integrated magnitude of about 6 and so is on the threshold of naked - eye visibility. The cluster is quite old as these things go, about 300 million light years. It is about 5000 light years distant, in the northern part of the constellation of Puppis. Although planetary nebula distances are notoriously difficult to measure, NGC 2438 seems to be in the foreground and is not connected to the cluster. Planetaries are in an

Star cluster M46 and planetary nebula NGC 2438 - Open cluster M46 and planetary nebula NGC 2438 - M46 (NGC 2437) is an age cluster located at 5400 years - light. It contains about 500 stars, 150 of which are brilliant. It is about 300 million years old. The planetary nebula NGC 2438 does not appear to belong to this cluster, and must be closer although its distance is unknown. Image obtained by Siding Spring's 3.9m telescope The open cluster NGC 2437 (M46) has an angular diameter of almost half a degree and is quite beautiful in even quite a modest telescope. It has an integrated magnitude of about 6 and so is on the threshold of naked - eye visibility. The cluster is quite old as these things go, about 300 million light years. It is about 5000 light years distant, in the northern part of the constellation of Puppis. Although planetary nebula distances are notoriously difficult to measure, NGC 2438 seems to be in the foreground and is not connected to the cluster. Planetaries are in an

PIX4568052

Open Cluster of Pleiades - The Pleiades star cluster - The Pleiades cluster is a cluster of about 500 young stars nees 150 million years ago. Visible in the constellation Taurus, this cluster is 440 years from the Earth. Object number 45 in Messier's catalog is the Pleiades, also know as the Seven Sisters for the seven stars that can be easily seen with excellent eyesight.The Pleiades is a relatively nearby open cluster, which according to new data from the Hipparcos satellite is located at a distance of 370 light years. The cluster is surrounded by blue nebulosity illuminated by the light reflected from the nearby stars. Astro - Physic's 130EDT F/8 Triplet Refractor working at f/6 two 20 minute exposures

Open Cluster of Pleiades - The Pleiades star cluster - The Pleiades cluster is a cluster of about 500 young stars nees 150 million years ago. Visible in the constellation Taurus, this cluster is 440 years from the Earth. Object number 45 in Messier's catalog is the Pleiades, also know as the Seven Sisters for the seven stars that can be easily seen with excellent eyesight.The Pleiades is a relatively nearby open cluster, which according to new data from the Hipparcos satellite is located at a distance of 370 light years. The cluster is surrounded by blue nebulosity illuminated by the light reflected from the nearby stars. Astro - Physic's 130EDT F/8 Triplet Refractor working at f/6 two 20 minute exposures

Jerry Lodriguss

PIX4568688

Nebula NGC 2170 in Unicorn - Nebula NGC 2170 in Monoceros - Nebula by reflexion located in the constellation Unicorn. This rich collection of predominantly reflection and sparse emission nebulosity exists in the western part of a vast star forming region known as the Mon R 2 association. The “” R”” designation stands for reflection and indicates an association of stars illuminating reflection nebulae. Most of the members of Mon R 2 are type B stars located along an east - west line stretching across 2 degrees of the winter sky, situated about 8 degrees east of the Orion Nebula. The Mon R 2 association resides at a distance of 830 pc and formed about 6 to 10 million years ago along the edge of the Mon R2 molecular cloud

Nebula NGC 2170 in Unicorn - Nebula NGC 2170 in Monoceros - Nebula by reflexion located in the constellation Unicorn. This rich collection of predominantly reflection and sparse emission nebulosity exists in the western part of a vast star forming region known as the Mon R 2 association. The “” R”” designation stands for reflection and indicates an association of stars illuminating reflection nebulae. Most of the members of Mon R 2 are type B stars located along an east - west line stretching across 2 degrees of the winter sky, situated about 8 degrees east of the Orion Nebula. The Mon R 2 association resides at a distance of 830 pc and formed about 6 to 10 million years ago along the edge of the Mon R2 molecular cloud

Adam Block

PIX4618377

Nebula NGC 2170 in Unicorn - Nebula NGC 2170 in Monoceros - Nebula by reflexion located in the constellation Unicorn. This rich collection of predominantly reflection and sparse emission nebulosity exists in the western part of a vast star forming region known as the Mon R 2 association. The “” R”” designation stands for reflection and indicates an association of stars illuminating reflection nebulae. Most of the members of Mon R 2 are type B stars located along an east - west line stretching across 2 degrees of the winter sky, situated about 8 degrees east of the Orion Nebula. The Mon R 2 association resides at a distance of 830 pc and formed about 6 to 10 million years ago along the edge of the Mon R2 molecular cloud

Nebula NGC 2170 in Unicorn - Nebula NGC 2170 in Monoceros - Nebula by reflexion located in the constellation Unicorn. This rich collection of predominantly reflection and sparse emission nebulosity exists in the western part of a vast star forming region known as the Mon R 2 association. The “” R”” designation stands for reflection and indicates an association of stars illuminating reflection nebulae. Most of the members of Mon R 2 are type B stars located along an east - west line stretching across 2 degrees of the winter sky, situated about 8 degrees east of the Orion Nebula. The Mon R 2 association resides at a distance of 830 pc and formed about 6 to 10 million years ago along the edge of the Mon R2 molecular cloud

R. Gendler

PIX4618356

Nebula NGC 2170 in Unicorn - Nebula NGC 2170 in Monoceros - Nebula by reflexion located in the constellation Unicorn. This rich collection of predominantly reflection and sparse emission nebulosity exists in the western part of a vast star forming region known as the Mon R 2 association. The “” R”” designation stands for reflection and indicates an association of stars illuminating reflection nebulae. Most of the members of Mon R 2 are type B stars located along an east - west line stretching across 2 degrees of the winter sky, situated about 8 degrees east of the Orion Nebula. The Mon R 2 association resides at a distance of 830 pc and formed about 6 to 10 million years ago along the edge of the Mon R2 molecular cloud

Nebula NGC 2170 in Unicorn - Nebula NGC 2170 in Monoceros - Nebula by reflexion located in the constellation Unicorn. This rich collection of predominantly reflection and sparse emission nebulosity exists in the western part of a vast star forming region known as the Mon R 2 association. The “” R”” designation stands for reflection and indicates an association of stars illuminating reflection nebulae. Most of the members of Mon R 2 are type B stars located along an east - west line stretching across 2 degrees of the winter sky, situated about 8 degrees east of the Orion Nebula. The Mon R 2 association resides at a distance of 830 pc and formed about 6 to 10 million years ago along the edge of the Mon R2 molecular cloud

R. Gendler

PIX4618379

Lufengosaurus

NHM1452625

Telephone call, 1927 (b/w photo)

Telephone call, 1927 (b/w photo)

SJB7288483

Nebula NGC 3372 in the Carene - NGC 3372, Eta Carinae nebula - The nebula of the Carene is located about 8000 years - light from the Earth. It is home to many hot massive stars, including the star Eta Carinae in the centre of the nebula. This nebula is larger than the Great Nebula in Orion, but is not visible from most northern latitudes. It is a giant complex of emission and dark nebulae surrounding the unique variable star Eta Carinae, which scientists believe is the most massive and energetic star in the Milky Way galaxy. Located about 8,500 light years from the Earth, the star is about 100 times as massive as our own Sun, but produces 6 million times the light output. It was observed producing a remarkable burst of X - ray emissions that doubled its X - ray output in only four months. In the 1840's, Eta Carinae erupted visibly and was the second brightest star in the sky during this time

Nebula NGC 3372 in the Carene - NGC 3372, Eta Carinae nebula - The nebula of the Carene is located about 8000 years - light from the Earth. It is home to many hot massive stars, including the star Eta Carinae in the centre of the nebula. This nebula is larger than the Great Nebula in Orion, but is not visible from most northern latitudes. It is a giant complex of emission and dark nebulae surrounding the unique variable star Eta Carinae, which scientists believe is the most massive and energetic star in the Milky Way galaxy. Located about 8,500 light years from the Earth, the star is about 100 times as massive as our own Sun, but produces 6 million times the light output. It was observed producing a remarkable burst of X - ray emissions that doubled its X - ray output in only four months. In the 1840's, Eta Carinae erupted visibly and was the second brightest star in the sky during this time

Jerry Lodriguss

PIX4618875

Gallimimus (colour litho)

Gallimimus (colour litho)

Konopelko, Jo (21st century)

NHM1455809

Gallimimus skeleton (colour litho)

Gallimimus skeleton (colour litho)

Konopelko, Jo (21st century)

NHM1455797

Tyrannosaurus rex (colour litho)

Tyrannosaurus rex (colour litho)

Konopelko, Jo (21st century)

NHM1455815

Elliptical galaxy NGC 1275 in Persee - Elliptical galaxy NGC 1275 in Perseus - This image obtained by the Hubble space telescope in 1995 shows a system of two colliding galaxies; in the foreground, a spiral galaxy seen almost from the edge, with many stars forming in the background, a giant, very bright elliptical galaxy, special because it has a spiral structure in its center. Its core probably houses a black hole. NGC 1275 is located about 230 million years ago - light; it belongs to the large cluster of galaxies of Persee. These images, taken with Hubble's Wide Field Planetary Camera 2 (WFPC2), show traces of spiral structure accompanied by dramatic dust lanes and bright blue regions that mark areas of active star formation. Detailed observations of NGC 1275 indicate that the dusty material belongs to a spiral system seen nearly edge - on in the foreground. The second galaxy, lying beyond the first, is actually a giant elliptical with peculiar faint spiral structure in its nucleus. These galaxies are believed to be colliding at over 6 million miles per hour. NGC 1275 is about 230 million light - years away in the constellation Perseus. Embedded in the center of a large cluster of galaxies known as the Perseus Cluster, it is also known to emit a powerful signal at both X - ray and radio frequencies. The galaxy collision causes the gas and dust already existing in the central bright galaxy to swirl into the center of the object. The X - ray and radio emission indicates the probable existence of a black hole at the bright galaxy's center. While the dark dusty material in the Hubble image falls inward, NGC 1275 displays intricate filamentary structures at a much larger scale outside the image. This is a typical feature of bright cluster galaxies — Elliptical galaxy NGC 1275 in Persee - Elliptical galaxy NGC 1275 in Perseus - This image obtained by the Hubble space telescope in 1995 shows a system of two colliding galaxies; in the foreground, a spiral galaxy seen almost from the edge, with many stars forming in the background, a giant, very bright elliptical galaxy, special because it has a spiral structure in its center. Its core probably houses a black hole. NGC 1275 is located about 230 million years ago - light; it belongs to the large cluster of galaxies of Persee. These images, taken with Hubble's Wide Field Planetary Camera 2 (WFPC2), show traces of spiral structure accompanied by dramatic dust lanes and bright blue regions that mark areas of active star formation. Detailed observations of NGC 1275 indicate that the dusty material belongs to a spiral system seen nearly edge - on in the foreground. The second galaxy, lying beyond the first, is actually a giant elliptical with peculiar faint spiral structure in its nucleus.

Elliptical galaxy NGC 1275 in Persee - Elliptical galaxy NGC 1275 in Perseus - This image obtained by the Hubble space telescope in 1995 shows a system of two colliding galaxies; in the foreground, a spiral galaxy seen almost from the edge, with many stars forming in the background, a giant, very bright elliptical galaxy, special because it has a spiral structure in its center. Its core probably houses a black hole. NGC 1275 is located about 230 million years ago - light; it belongs to the large cluster of galaxies of Persee. These images, taken with Hubble's Wide Field Planetary Camera 2 (WFPC2), show traces of spiral structure accompanied by dramatic dust lanes and bright blue regions that mark areas of active star formation. Detailed observations of NGC 1275 indicate that the dusty material belongs to a spiral system seen nearly edge - on in the foreground. The second galaxy, lying beyond the first, is actually a giant elliptical with peculiar faint spiral structure in its nucleus.

PIX4609694

Two child labourers are working on a autorickshaw at a road side auto rickshaw repairing centre in Kolkata, India, September 5, 2005. (photo)

Two child labourers are working on a autorickshaw at a road side auto rickshaw repairing centre in Kolkata, India, September 5, 2005. (photo)

UIG796378

Nebula NGC 2170 in Unicorn - Nebula NGC 2170 in Monoceros - Nebula by reflexion located in the constellation Unicorn. This rich collection of predominantly reflection and sparse emission nebulosity exists in the western part of a vast star forming region known as the Mon R 2 association. The “” R”” designation stands for reflection and indicates an association of stars illuminating reflection nebulae. Most of the members of Mon R 2 are type B stars located along an east - west line stretching across 2 degrees of the winter sky, situated about 8 degrees east of the Orion Nebula. The Mon R 2 association resides at a distance of 830 pc and formed about 6 to 10 million years ago along the edge of the Mon R2 molecular cloud. NGC2170 is a common nebula imaged and yet with long exposures it takes on a whole new look. Many of the nebulae seen here appear to be uncataloged and not previously imaged. This image has been carefully processed to reveal the many faint and dusty nebulae in this region of Monoceros — Nebula NGC 2170 in Unicorn - Nebula NGC 2170 in Monoceros - Nebula by reflexion located in the constellation Unicorn. This rich collection of predominantly reflection and sparse emission nebulosity exists in the western part of a vast star forming region known as the Mon R 2 association. The “” R”” designation stands for reflection and indicates an association of stars illuminating reflection nebulae. Most of the members of Mon R 2 are type B stars located along an east - west line stretching across 2 degrees of the winter sky, situated about 8 degrees east of the Orion Nebula. The Mon R 2 association resides at a distance of 830 pc and formed about 6 to 10 million years ago along the edge of the Mon R2 molecular cloud. NGC2170 is a common nebula imaged and yet with long exposures it takes on a whole new look. Many of the nebulae seen here appear to be uncataloged and not previously imaged. This image has been carefully processed to reveal the many faint and dusty nebulae in this regio

Nebula NGC 2170 in Unicorn - Nebula NGC 2170 in Monoceros - Nebula by reflexion located in the constellation Unicorn. This rich collection of predominantly reflection and sparse emission nebulosity exists in the western part of a vast star forming region known as the Mon R 2 association. The “” R”” designation stands for reflection and indicates an association of stars illuminating reflection nebulae. Most of the members of Mon R 2 are type B stars located along an east - west line stretching across 2 degrees of the winter sky, situated about 8 degrees east of the Orion Nebula. The Mon R 2 association resides at a distance of 830 pc and formed about 6 to 10 million years ago along the edge of the Mon R2 molecular cloud. NGC2170 is a common nebula imaged and yet with long exposures it takes on a whole new look. Many of the nebulae seen here appear to be uncataloged and not previously imaged. This image has been carefully processed to reveal the many faint and dusty nebulae in this regio

Tom Davis

PIX4618385

Möhnetalsperre

Möhnetalsperre

UTD2840032

A woman looks at lamps made of gold-plated crystal on sale at a multi-million dollar auction being h.., 2001 (photo)

A woman looks at lamps made of gold-plated crystal on sale at a multi-million dollar auction being h.., 2001 (photo)

Zainal Abd Halim

REU7464955

A Pakistani nurse adjusts the nappy of a newborn baby at an Islamabad hospital October 12. According.., 1999-10-12 (photo)

A Pakistani nurse adjusts the nappy of a newborn baby at an Islamabad hospital October 12. According.., 1999-10-12 (photo)

Muzammil Pasha

REU7585173

M46 star cluster and planetary nebula NGC 2438 in the stern - Open Cluster M46 and Planetary Nebula NGC 2438 - M46 (NGC 2437) is a cluster of stars aged 5400 years - light. It contains about 500 stars, 150 of which are brilliant. It is about 300 million years old. The planetary nebula NGC 2438 does not appear to belong to this cluster, and must be closer although its distance is unknown. M46 is a rich open cluster that contains a real jewel, planetary nebula NGC 2438. At 6th magnitude, M46 contains about 100 bright stars, the brightest of which is magnitude 8.7. It is about one - half degree in apparent diameter, the same size as the full moon. It is estimated to be about 300 million years old. Planetary nebula NGC 2438 is about one arc minute in diameter and shines at 10th magnitude. A planetary nebula is a shell of gas puffed off by a star late in its life cycle. Three bright stars are visible inside of the nebula, although none of them are the true central star which shed the gas. The central star in NGC 2438 has a magnitude of 17.7, so the stars visible inside of the ring are members of the cluster M46, which lies behind the planetary nebula, but along the same line of sight. The true central star of NGC 2438 is probably more than a billion years old, another indication that it is not a member of the cluster. NGC 2438, discovered by William Herschel in 1786, is located at a distance of about 2,900 light years. M46 is located about 5,400 light years away and was discovered by Charles Messier in 1771. Both cluster and planetary nebula are located in the constellation of Puppis — M46 star cluster and planetary nebula NGC 2438 in the stern - Open Cluster M46 and Planetary Nebula NGC 2438 - M46 (NGC 2437) is a cluster of stars aged 5400 years - light. It contains about 500 stars, 150 of which are brilliant. It is about 300 million years old. The planetary nebula NGC 2438 does not appear to belong to this cluster, and must be closer although its distance is unknown. M46 is a rich open cluster that contains a real jewel, planetary nebula NGC 2438. At 6th magnitude, M46 contains about 100 bright stars, the brightest of which is magnitude 8.7. It is about one - half degree in apparent diameter, the same size as the full moon. It is estimated to be about 300 million years old. Planetary nebula NGC 2438 is about one arc minute in diameter and shines at 10th magnitude. A planetary nebula is a shell of gas puffed off by a star late in its life cycle. Three bright stars are visible inside of the nebula, although none of them are the true central star which shed the gas. T

M46 star cluster and planetary nebula NGC 2438 in the stern - Open Cluster M46 and Planetary Nebula NGC 2438 - M46 (NGC 2437) is a cluster of stars aged 5400 years - light. It contains about 500 stars, 150 of which are brilliant. It is about 300 million years old. The planetary nebula NGC 2438 does not appear to belong to this cluster, and must be closer although its distance is unknown. M46 is a rich open cluster that contains a real jewel, planetary nebula NGC 2438. At 6th magnitude, M46 contains about 100 bright stars, the brightest of which is magnitude 8.7. It is about one - half degree in apparent diameter, the same size as the full moon. It is estimated to be about 300 million years old. Planetary nebula NGC 2438 is about one arc minute in diameter and shines at 10th magnitude. A planetary nebula is a shell of gas puffed off by a star late in its life cycle. Three bright stars are visible inside of the nebula, although none of them are the true central star which shed the gas. T

Jerry Lodriguss

PIX4568057

AN OVERWEIGHT CHINESE WOMAN FAINTS DURING A CROWDED WEIGHT-LOSS
COMPETITION IN BEIJING, 2002-04-06 (photo) — AN OVERWEIGHT CHINESE WOMAN FAINTS DURING A CROWDED WEIGHT-LOSS COMPETITION IN BEIJING, 2002-04-06 (photo)

AN OVERWEIGHT CHINESE WOMAN FAINTS DURING A CROWDED WEIGHT-LOSS COMPETITION IN BEIJING, 2002-04-06 (photo)

Guang Niu

REU7850742

BORIS BECKER FILE PHOTO, 2000-08-06 (photo)

BORIS BECKER FILE PHOTO, 2000-08-06 (photo)

Henry Romero

REU7736026

THE FABERGE WINTER EGG ON DISPLAY IN MOSCOW, 2001-03-27 (photo)

THE FABERGE WINTER EGG ON DISPLAY IN MOSCOW, 2001-03-27 (photo)

William Webster

REU7816744

OVERWEIGHT CHINESE QUEUE UP FOR A COMPETITION IN BEIJING, 2002-04-06 (photo)

OVERWEIGHT CHINESE QUEUE UP FOR A COMPETITION IN BEIJING, 2002-04-06 (photo)

Guang Niu

REU7948569

ANDREW GROVE INTEL CHAIRMAN GESTURES AT NEW BRIEFING IN BEIJING, 1998-05-06 (photo)

ANDREW GROVE INTEL CHAIRMAN GESTURES AT NEW BRIEFING IN BEIJING, 1998-05-06 (photo)

Natalie Behring

REU8093541

GUAN CHEN IS WEIGHTED IN AT A COMPETITION IN BEIJING, 2002-04-06 (photo)

GUAN CHEN IS WEIGHTED IN AT A COMPETITION IN BEIJING, 2002-04-06 (photo)

Guang Niu

REU7846544

GUAN CHEN WAITS AFTER BEING WEIGHTED IN AT A COMPETITION IN BEIJING, 2002-04-06 (photo)

GUAN CHEN WAITS AFTER BEING WEIGHTED IN AT A COMPETITION IN BEIJING, 2002-04-06 (photo)

Guang Niu

REU7891265

Star field in the halo of the Andromede galaxy - Deep field image in the halo of Andromeda galaxy - Deep field in the halo of the Andromede galaxy obtained by the Hubble space telescope in 2003. 300,000 stars as well as thousands of background galaxies are visible. Astronomers using Nasa's Hubble Space Telescope (HST) have reliably measured the age of the spherical halo of stars surrounding the neighboring Andromeda galaxy (M31). To their surprise, they have discovered that approximately one - third of the stars in Andromeda's halo formed only 6 to 8 billion years ago. That's a far cry from the 11 - to - 13 billion - year age of the stars in the Milky Way's halo. Why the difference in halo ages? Apparently, M31 must have gone through a major “” corporate merger”” with another large galaxy, or a series of mergers with smaller galaxies, billions of years ago. Astronomers cannot yet tell whether this was one tumultuous event or a more continual acquisition of smaller galaxies. The newly discovered younger stars in Andromeda's halo are richer in heavier elements than the stars in our Milky Way's halo, or in most of the small dwarf galaxies that surround the Milky Way. Indeed the level of chemical enrichment seen in these younger stars is characteristic of relatively massive galaxies, containing at least a billion stars. This suggests three possibilities: (1) Collisions destroyed the young disk of M31 and dispersed many of its stars into the halo; (2) a single collision destroyed a relatively massive invading galaxy and dispersed its stars and some of Andromeda's disk stars into the halo; and/or (3) many stars formed during the collision itself. Astronomers say it will take more detailed observations to unravel the acquisition history of these early cataclysmic events. Located only 2.5 million light - years away, the magnificent Andromeda galaxy, visible as a naked - eye spindle of light in the autumn sky has long been considered a near twin to our — Star field in the halo of the Andromede galaxy - Deep field image in the halo of Andromeda galaxy - Deep field in the halo of the Andromede galaxy obtained by the Hubble space telescope in 2003. 300,000 stars as well as thousands of background galaxies are visible. Astronomers using Nasa's Hubble Space Telescope (HST) have reliably measured the age of the spherical halo of stars surrounding the neighboring Andromeda galaxy (M31). To their surprise, they have discovered that approximately one - third of the stars in Andromeda's halo formed only 6 to 8 billion years ago. That's a far cry from the 11 - to - 13 billion - year age of the stars in the Milky Way's halo. Why the difference in halo ages? Apparently, M31 must have gone through a major “” corporate merger”” with another large galaxy, or a series of mergers with smaller galaxies, billions of years ago. Astronomers cannot yet tell whether this was one tumultuous event or a more continual acquisition of smaller galaxies. The newly d

Star field in the halo of the Andromede galaxy - Deep field image in the halo of Andromeda galaxy - Deep field in the halo of the Andromede galaxy obtained by the Hubble space telescope in 2003. 300,000 stars as well as thousands of background galaxies are visible. Astronomers using Nasa's Hubble Space Telescope (HST) have reliably measured the age of the spherical halo of stars surrounding the neighboring Andromeda galaxy (M31). To their surprise, they have discovered that approximately one - third of the stars in Andromeda's halo formed only 6 to 8 billion years ago. That's a far cry from the 11 - to - 13 billion - year age of the stars in the Milky Way's halo. Why the difference in halo ages? Apparently, M31 must have gone through a major “” corporate merger”” with another large galaxy, or a series of mergers with smaller galaxies, billions of years ago. Astronomers cannot yet tell whether this was one tumultuous event or a more continual acquisition of smaller galaxies. The newly d

PIX4572242

CSU election poster, 1983 (photo)

CSU election poster, 1983 (photo)

Dietrich, Rudolf

SZT11799668

EPA ADMINISTRATOR BROWNER TALKS ABOUT THE HUDSON RIVER CLEAN UP, 2000-12-06 (photo)

EPA ADMINISTRATOR BROWNER TALKS ABOUT THE HUDSON RIVER CLEAN UP, 2000-12-06 (photo)

Jeff Christensen

REU7691188

TO GO WITH FEATURE STORY BC-GERMANY-DEPOPULATION, 2003-07-06 (photo)

TO GO WITH FEATURE STORY BC-GERMANY-DEPOPULATION, 2003-07-06 (photo)

Manuela Hartling

REU7854493

TO GO WITH FEATURE STORE BC-GERMANY-DEPOPULATION, 2003-07-06 (photo)

TO GO WITH FEATURE STORE BC-GERMANY-DEPOPULATION, 2003-07-06 (photo)

Manuela Hartling

REU7855145

Victor Garcia, a three-year-old Peruvian, lifts a brick in an informal brickyard in a shantytown in .., 2002-07-13 (photo)

Victor Garcia, a three-year-old Peruvian, lifts a brick in an informal brickyard in a shantytown in .., 2002-07-13 (photo)

Pilar Olivares

REU7496484

TO GO WITH FEATURE STORE BC-GERMANY-DEPOPULATION, 2003-07-06 (photo)

TO GO WITH FEATURE STORE BC-GERMANY-DEPOPULATION, 2003-07-06 (photo)

Manuela Hartling

REU7900082

The Bavarian justice minister of the Christian Social Union Party (CSU), Alfred Sauter eats traditio.., 1999-09-06 (photo)

The Bavarian justice minister of the Christian Social Union Party (CSU), Alfred Sauter eats traditio.., 1999-09-06 (photo)

Michael Dalder

REU7586072

A COUPLE WALKS PASSED A DESTROYED BICYCLE IN A WITTENBERGE STREET IN
EASTERN GERMANY, 2003-07-06 (photo) — A COUPLE WALKS PASSED A DESTROYED BICYCLE IN A WITTENBERGE STREET IN EASTERN GERMANY, 2003-07-06 (photo)

A COUPLE WALKS PASSED A DESTROYED BICYCLE IN A WITTENBERGE STREET IN EASTERN GERMANY, 2003-07-06 (photo)

Manuela Hartling

REU7683506

A MAN PUSHES HIS DAUGHTER ON A TRICYCLE THROUGH A DERELICT STREET IN
WITTENBERGE IN EASTERN GERMANY, 2003-07-06 (photo) — A MAN PUSHES HIS DAUGHTER ON A TRICYCLE THROUGH A DERELICT STREET IN WITTENBERGE IN EASTERN GERMANY, 2003-07-06 (photo)

A MAN PUSHES HIS DAUGHTER ON A TRICYCLE THROUGH A DERELICT STREET IN WITTENBERGE IN EASTERN GERMANY, 2003-07-06 (photo)

Manuela Hartling

REU7821920

A WOMAN WALKS HER DOG IN A DERELICT WITTENBERGE STREET IN EASTERN
GERMANY, 2003-07-06 (photo) — A WOMAN WALKS HER DOG IN A DERELICT WITTENBERGE STREET IN EASTERN GERMANY, 2003-07-06 (photo)

A WOMAN WALKS HER DOG IN A DERELICT WITTENBERGE STREET IN EASTERN GERMANY, 2003-07-06 (photo)

Manuela Hartling

REU7821711

FOR RELEASE WITH STORY PERU-CHILDREN, 2002-06-15 (photo)

FOR RELEASE WITH STORY PERU-CHILDREN, 2002-06-15 (photo)

Pilar Olivares

REU7865957

Phobos and Mars - Illustration - Phobos and Mars - Illustration - Artist's view of Phobos, the largest of Mars's two satellites. This is how Mars and its tiny satellite Phobos might appear from a distance of about 100 miles from Phobos' surface. Phobos is over the low martian plains of Syrtis Major. Below the plains extending down to Mars' terminator and beyond is the heavily cratered Terra Sabaea. Clouds of water - ice crystals are forming at the terminator between light and dark. Looking more like a common potato than a celestial body, Phobos is actually the larger of Mars' two satellites, with a length of about 16 miles and about 11 miles across its smallest dimension. Phobos does not have enough mass for gravity to pull it into a uniform sphere like the larger satellites and planets in the Solar System. Phobos may be an asteroid long ago captured by Mars' gravity, orbiting a mere 5,800 miles above Mars' surface, making it the closest satellite to its host planet in the Solar System. Phobos' orbit is so low that it completes one revolution in less than eight hours, easily outpacing by threefold Mars' rotation period of 24 hours, 40 minutes. The resulting tidal forces are causing Phobos' altitude to decay at the relatively rapid rate of 6 feet per century; in about 50 million years Phobos will either crash into the martian surface, or be torn apart by Mars' gravity — Phobos and Mars - Illustration - Phobos and Mars - Illustration - Artist's view of Phobos, the largest of Mars's two satellites. This is how Mars and its tiny satellite Phobos might appear from a distance of about 100 miles from Phobos' surface. Phobos is over the low martian plains of Syrtis Major. Below the plains extending down to Mars' terminator and beyond is the heavily cratered Terra Sabaea. Clouds of water - ice crystals are forming at the terminator between light and dark. Looking more like a common potato than a celestial body, Phobos is actually the larger of Mars' two satellites, with a length of about 16 miles and about 11 miles across its smallest dimension. Phobos does not have enough mass for gravity to pull it into a uniform sphere like the larger satellites and planets in the Solar System. Phobos may be an asteroid long ago captured by Mars' gravity, orbiting a mere 5,800 miles above Mars' surface, making it the closest satellite to its host planet in the Solar System

Phobos and Mars - Illustration - Phobos and Mars - Illustration - Artist's view of Phobos, the largest of Mars's two satellites. This is how Mars and its tiny satellite Phobos might appear from a distance of about 100 miles from Phobos' surface. Phobos is over the low martian plains of Syrtis Major. Below the plains extending down to Mars' terminator and beyond is the heavily cratered Terra Sabaea. Clouds of water - ice crystals are forming at the terminator between light and dark. Looking more like a common potato than a celestial body, Phobos is actually the larger of Mars' two satellites, with a length of about 16 miles and about 11 miles across its smallest dimension. Phobos does not have enough mass for gravity to pull it into a uniform sphere like the larger satellites and planets in the Solar System. Phobos may be an asteroid long ago captured by Mars' gravity, orbiting a mere 5,800 miles above Mars' surface, making it the closest satellite to its host planet in the Solar System

Walter B Myers

PIX4616778

SHIPYARD WORKERS LISTEN TO SPEECHES DURING A RALLY, 1997-03-06 (photo)

SHIPYARD WORKERS LISTEN TO SPEECHES DURING A RALLY, 1997-03-06 (photo)

Str Old

REU8054652

KAMALA MANDAL SHOWS HER HANDS WRINKLED BECAUSE OF DRINKING ARSENIC CONTAMINATED WATER IN CALCUTTA, 2000-03-30 (photo)

KAMALA MANDAL SHOWS HER HANDS WRINKLED BECAUSE OF DRINKING ARSENIC CONTAMINATED WATER IN CALCUTTA, 2000-03-30 (photo)

Jayanta Shaw

REU7547349

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