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Bilder zu 'Planck Telescope' gefunden, 16

Effelsberg radio telescope in Bad Munstereifel, North Rhine-Westphalia, 2011 (photo)

Effelsberg radio telescope in Bad Munstereifel, North Rhine-Westphalia, 2011 (photo)

SZT6201249

This image is taken looking towards a region of our Milky Way galaxy in the Eagle constellation, closer to the galactic center than our sun. At the center and the left of the image, the two massive star-forming regions G29.9 and W43 are clearly visible. Herschel.

This image is taken looking towards a region of our Milky Way galaxy in the Eagle constellation, closer to the galactic center than our sun. At the center and the left of the image, the two massive star-forming regions G29.9 and W43 are clearly visible. Herschel.

UIG867162

A low activity, star-formation region in the constellation Perseus, as seen by Planck.

A low activity, star-formation region in the constellation Perseus, as seen by Planck.

UIG867159

A low activity, star-formation region in the constellation Perseus, as seen by Planck.

A low activity, star-formation region in the constellation Perseus, as seen by Planck.

UIG867160

This long-wavelength image shows most of the constellation Orion, highlighting turbid clouds of cold material, where new stars are being stirred into existence. Planck Telescope.

This long-wavelength image shows most of the constellation Orion, highlighting turbid clouds of cold material, where new stars are being stirred into existence. Planck Telescope.

UIG867161

The radio telescope Effelsberg at the Max Planck Institute in Nordrhein-Westfalen, 2011 (photo)

The radio telescope Effelsberg at the Max Planck Institute in Nordrhein-Westfalen, 2011 (photo)

SZT6201250

The Effelsberg radio telescope, Nordrhein-Westfalen, 2016 (photo)

The Effelsberg radio telescope, Nordrhein-Westfalen, 2016 (photo)

SZT6201251

Map of Fossil Radiation Seen by Planck - The cosmic microwave background as seen by Planck - The European Space Agency's Planck space telescope is the source of the data on the most detailed map ever drawn of the Cosmological Hyperrequency background radiation - the fossil radiation of the Big Bang. This image is based on data from the first 15 months of Planck operation. It is the first image of this mission that shows on the whole sky the oldest emission of light that bathed our young Universe when it was only 380,000 years old. The Universe was then filled with a burning magma of protons, electrons, and photons intertwining at about 2700oC. The interaction between protons and electrons that gave rise to the hydrogen atoms then released light. As a result of the expansion of the Universe, this light has been extended until today reaches hyperfrequency wavelengths equivalent to a temperature of just 2.7 degrees above the absolute zero. This hyperfrequency cosmological background radia

Map of Fossil Radiation Seen by Planck - The cosmic microwave background as seen by Planck - The European Space Agency's Planck space telescope is the source of the data on the most detailed map ever drawn of the Cosmological Hyperrequency background radiation - the fossil radiation of the Big Bang. This image is based on data from the first 15 months of Planck operation. It is the first image of this mission that shows on the whole sky the oldest emission of light that bathed our young Universe when it was only 380,000 years old. The Universe was then filled with a burning magma of protons, electrons, and photons intertwining at about 2700oC. The interaction between protons and electrons that gave rise to the hydrogen atoms then released light. As a result of the expansion of the Universe, this light has been extended until today reaches hyperfrequency wavelengths equivalent to a temperature of just 2.7 degrees above the absolute zero. This hyperfrequency cosmological background radia

PIX4634328

The Effelsberg radio telescope, Nordrhein-Westfalen, 2016 (photo)

The Effelsberg radio telescope, Nordrhein-Westfalen, 2016 (photo)

Rainer Unkel

SZT6201253

The Effelsberg radio telescope, Nordrhein-Westfalen, 2016 (photo)

The Effelsberg radio telescope, Nordrhein-Westfalen, 2016 (photo)

Sepp Spiegl

SZT6201254

The Effelsberg radio telescope, Nordrhein-Westfalen, 2016 (photo)

The Effelsberg radio telescope, Nordrhein-Westfalen, 2016 (photo)

Sepp Spiegl

SZT6201252

Spiral Galaxy M83 in Hydra - M83 (NGC 5236) - The galaxy M83 (NGC 5236) is about 15 million light years away from Earth. This galaxy is intermediate between a classic spiral and a barree spiral. Composite images obtained from the Hubble Space Telescope (HST), the Subaru Telescope and the 2.2m MPG telescope of the ESO. M83 (NGC 5236) is located in the southern constellation Hydra at 15 million light years from the sun. It is classified as intermediate between normal and barred spiral galaxies. Composite image from four data sources (8.2 Meter Subaru Telescope, Hubble Space Telescope, 2.2 - meter Max Planck - ESO telescope and 14.5” RC)

Spiral Galaxy M83 in Hydra - M83 (NGC 5236) - The galaxy M83 (NGC 5236) is about 15 million light years away from Earth. This galaxy is intermediate between a classic spiral and a barree spiral. Composite images obtained from the Hubble Space Telescope (HST), the Subaru Telescope and the 2.2m MPG telescope of the ESO. M83 (NGC 5236) is located in the southern constellation Hydra at 15 million light years from the sun. It is classified as intermediate between normal and barred spiral galaxies. Composite image from four data sources (8.2 Meter Subaru Telescope, Hubble Space Telescope, 2.2 - meter Max Planck - ESO telescope and 14.5” RC)

PIX4612542

Planetary nebula Helix (NGC 7293), located in Aquarius, is one of the closest to Earth (c. 690 light years) Image by the 2.2m Max Planck Society/ESO/MPG telescope of the La Silla Observatory in Chile.

Planetary nebula Helix (NGC 7293), located in Aquarius, is one of the closest to Earth (c. 690 light years) Image by the 2.2m Max Planck Society/ESO/MPG telescope of the La Silla Observatory in Chile.

PIX4623684

Composite image of the galaxy Centaurus A (photo)

Composite image of the galaxy Centaurus A (photo)

SMT1217250

Cone Nebula NGC 2264 in the Unicorn - The Cone Nebula NGC 2264 in Monoceros - The Cone Nebula is a region H II located about 2600 years from Earth. It is accompanied by a cluster of stars called the Christmas tree. The bright star at the top is S Monocerotis, a star of magnitude 4.7. Image obtained by the 2.2m telescope of La Silla. NGC 2264 and the Christmas Tree cluster lies about 2600 light - years from Earth in the constellation of Monoceros, the Unicorn, not far from the more familiar figure of Orion, the Hunter. The image shows a region of space about 30 light - years across. The cluster is very bright and can easily be seen with binoculars. With a small telescope (whose lenses will turn the view upside down) the stars resemble the glittering lights on a Christmas tree. The dazzling star at the top is S Monocerotis, bright enough to be seen with the unaided eye. It is a massive multiple star system that only emerged from the dust and gas a few million years ago. At the bottom of

Cone Nebula NGC 2264 in the Unicorn - The Cone Nebula NGC 2264 in Monoceros - The Cone Nebula is a region H II located about 2600 years from Earth. It is accompanied by a cluster of stars called the Christmas tree. The bright star at the top is S Monocerotis, a star of magnitude 4.7. Image obtained by the 2.2m telescope of La Silla. NGC 2264 and the Christmas Tree cluster lies about 2600 light - years from Earth in the constellation of Monoceros, the Unicorn, not far from the more familiar figure of Orion, the Hunter. The image shows a region of space about 30 light - years across. The cluster is very bright and can easily be seen with binoculars. With a small telescope (whose lenses will turn the view upside down) the stars resemble the glittering lights on a Christmas tree. The dazzling star at the top is S Monocerotis, bright enough to be seen with the unaided eye. It is a massive multiple star system that only emerged from the dust and gas a few million years ago. At the bottom of

PIX4618657

Space Exploration: Soyuz and Orion Ships - Artist's View - CEV-Soyuz Joint Mission - An American Orion ship mooring has a Soyuz TMA-M spaceship during a distant space exploration mission. Here, the ship is approaching a satellite stationed at a point in Lagrange. Illustration. An Orion class Crew Exploration Vehicle (AKA Deep Space Vehicle) is paired with a Soyuz TMA-M manned spacecraft for a joint deep space rendezvous with a satellite parked in a gravitationally stable Lagrangian point about 1 million miles beyond the orbit of the Earth's Moon. At this position, in this case a Lagrangian point 2, or L2, the Earth is between the spacecraft and the Sun resulting in the Earth eclipsing much of the Sun's light, however at this distance the Earth does not subtend an angle large enough to cover the entire disk of the Sun. What's visible of the Sun is a brilliant ring of light illuminating the spacecraft. (The streamers of light around the Sun are not the Sun's corona, but rather a way of i

Space Exploration: Soyuz and Orion Ships - Artist's View - CEV-Soyuz Joint Mission - An American Orion ship mooring has a Soyuz TMA-M spaceship during a distant space exploration mission. Here, the ship is approaching a satellite stationed at a point in Lagrange. Illustration. An Orion class Crew Exploration Vehicle (AKA Deep Space Vehicle) is paired with a Soyuz TMA-M manned spacecraft for a joint deep space rendezvous with a satellite parked in a gravitationally stable Lagrangian point about 1 million miles beyond the orbit of the Earth's Moon. At this position, in this case a Lagrangian point 2, or L2, the Earth is between the spacecraft and the Sun resulting in the Earth eclipsing much of the Sun's light, however at this distance the Earth does not subtend an angle large enough to cover the entire disk of the Sun. What's visible of the Sun is a brilliant ring of light illuminating the spacecraft. (The streamers of light around the Sun are not the Sun's corona, but rather a way of i

Walter B Myers

PIX4639150

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