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'6 And 2 Million Years Ago' Bilder und Clips Suchergebnisse

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Bilder zu '6 And 2 Million Years Ago' gefunden, 15

 
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  • Urheberrechtlich Geschützt
Homo habilis in action

McBride, Angus (1931-2007)

NHM1452632

Homo habilis in action

McBride, Angus (1931-2007)

NHM1452632

 
Zusätzliche Genehmigungen
  • Permission required for non-editorial use (inc book and magazine covers). Please contact us
Homo habilis in action

NHM1458612

Homo habilis in action

NHM1458612

 
Zusätzliche Genehmigungen
  • Permission required for non-editorial use (inc book and magazine covers). Please contact us
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  • Urheberrechtlich Geschützt
Homo habilis in action

McBride, Angus (1931-2007)

NHM1452633

Homo habilis in action

McBride, Angus (1931-2007)

NHM1452633

 
Zusätzliche Genehmigungen
  • Permission required for non-editorial use (inc book and magazine covers). Please contact us
Homo habilis in action

NHM1450193

Homo habilis in action

NHM1450193

 
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

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

 
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

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

 
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

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

Walter B Myers

PIX4662994

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

 
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

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

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

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

R. Gendler

PIX4618379

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

 
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

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

 
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

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

 
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

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

 
Galaxy cluster Abell 1689 - Gravitational lenses in Abell 1689 galaxy cluster - Galaxy cluster Abell 1689 is about 2.2 billion years ago - light in the constellation of the Virgin. This image shows, by a gravitational mirage effect, the deformed image of many galaxies located behind the cluster. Near infrared and visible image obtained by the Hubble space telescope in June 2002. 13 hours of installation. This representative color image is a composite of visible - light and near - infrared exposures taken in June 2002. Hubble peered straight through the center of one of the most massive galaxy clusters known, called Abell 1689. This required that Hubble gaze at the remote cluster, located 2.2 billion light - years away, for over 13 hours. The gravity of the cluster's trillion stars - - plus dark matter - - acts as a 2 - million - light - year - wide “” lens”” in space. This “” gravitational lens””” bends and magnifies the light of galaxies located far behind it. Although much more analy

PIX4565577

Galaxy cluster Abell 1689 - Gravitational lenses in Abell 1689 galaxy cluster - Galaxy cluster Abell 1689 is about 2.2 billion years ago - light in the constellation of the Virgin. This image shows, by a gravitational mirage effect, the deformed image of many galaxies located behind the cluster. Near infrared and visible image obtained by the Hubble space telescope in June 2002. 13 hours of installation. This representative color image is a composite of visible - light and near - infrared exposures taken in June 2002. Hubble peered straight through the center of one of the most massive galaxy clusters known, called Abell 1689. This required that Hubble gaze at the remote cluster, located 2.2 billion light - years away, for over 13 hours. The gravity of the cluster's trillion stars - - plus dark matter - - acts as a 2 - million - light - year - wide “” lens”” in space. This “” gravitational lens””” bends and magnifies the light of galaxies located far behind it. Although much more analy

PIX4565577

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