'Taurus' Bilder und Clips Suchergebnisse

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Bilder zu 'Taurus' gefunden, 1,096

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Sundials, Altitude Column sundial, German, c 1550

Sundials, Altitude Column sundial, German, c 1550

UIS5085009

Sundials, Altitude Column sundial, German, c 1550

Sundials, Altitude Column sundial, German, c 1550

UIS5085018

Classic Motorbike Mignon 125 N (photo)

Classic Motorbike Mignon 125 N (photo)

GRL5614042

Classic Motorbike Mignon 125 N, Engine (photo)

Classic Motorbike Mignon 125 N, Engine (photo)

GRL5614044

Classic Motorbike Mignon 125 N (photo)

Classic Motorbike Mignon 125 N (photo)

GRL5614040

Classic Motorbike Mignon 125 N (photo)

Classic Motorbike Mignon 125 N (photo)

GRL5614041

Classic Motorbike Mignon 125 N (photo)

Classic Motorbike Mignon 125 N (photo)

GRL5614045

Classic Motorbike Mignon 125 N (photo)

Classic Motorbike Mignon 125 N (photo)

GRL5614046

Apollo 17: Harrison Schmitt on the Moon - Apollo 17: Harrison Schmitt - Harrison Schmitt takes pictures near the rock at Station 6. 13/12/1972. Scientist - astronaut Harrison H. Schmitt is photographed working beside a huge boulder at Station 6 (base of North Massif) during the third Apollo 17 Extravehicular Activity (EVA - 3) at the Taurus - Littrow landing site. The front portion of the Lunar Roving Vehicle (LRV) is visible on the left. This picture was taken by astronaut Eugene A. Cernan, Apollo 17 commander. Schmitt is the lunar module pilot. While astronauts Cernan and Schmitt descended in the Lunar Module (LM) “” Challenger”” to explore the Moon, astronaut Ronald E. Evans, command module pilot, remained with the Apollo 17 Command and Service Modules (CSM) in lunar - orbit.13 December 1972

Apollo 17: Harrison Schmitt on the Moon - Apollo 17: Harrison Schmitt - Harrison Schmitt takes pictures near the rock at Station 6. 13/12/1972. Scientist - astronaut Harrison H. Schmitt is photographed working beside a huge boulder at Station 6 (base of North Massif) during the third Apollo 17 Extravehicular Activity (EVA - 3) at the Taurus - Littrow landing site. The front portion of the Lunar Roving Vehicle (LRV) is visible on the left. This picture was taken by astronaut Eugene A. Cernan, Apollo 17 commander. Schmitt is the lunar module pilot. While astronauts Cernan and Schmitt descended in the Lunar Module (LM) “” Challenger”” to explore the Moon, astronaut Ronald E. Evans, command module pilot, remained with the Apollo 17 Command and Service Modules (CSM) in lunar - orbit.13 December 1972

PIX4598027

Classic Motorbike Mignon 125 N (photo)

Classic Motorbike Mignon 125 N (photo)

GRL5614043

Sky horizon to horizon - Light pollution is visible on both horizons. The star Sirius is reflected in the sea. Higher, the constellations of Orion, and the Bull with the Pleiades. Near the zenith, a shooting star claws the sky not far from the round spot of Holmes comet right in Persee. Towards the other horizon, the double cluster of Persee, the Andromede Galaxy, the nebula North America (very low in light pollution) and finally the Lyre near the horizon. 16 November 2007, Combrit (Finistere). The light pollution is visible above both horizons. Sirius has just risen and reflects itself in the sea. Higher, are constellations of Orion, the Taurus with Pleiades. Near the zenith, a meteor scratches the sky near the round patch of Comet Holmes in the heart of Perseus. Down to the other horizon: the double Perseus Cluster, Great Andromeda galaxy, North America nebula (hard to spot in the light pollution) and constellation of Lyra near the horizon. November 16 2007, Brittany, France

Sky horizon to horizon - Light pollution is visible on both horizons. The star Sirius is reflected in the sea. Higher, the constellations of Orion, and the Bull with the Pleiades. Near the zenith, a shooting star claws the sky not far from the round spot of Holmes comet right in Persee. Towards the other horizon, the double cluster of Persee, the Andromede Galaxy, the nebula North America (very low in light pollution) and finally the Lyre near the horizon. 16 November 2007, Combrit (Finistere). The light pollution is visible above both horizons. Sirius has just risen and reflects itself in the sea. Higher, are constellations of Orion, the Taurus with Pleiades. Near the zenith, a meteor scratches the sky near the round patch of Comet Holmes in the heart of Perseus. Down to the other horizon: the double Perseus Cluster, Great Andromeda galaxy, North America nebula (hard to spot in the light pollution) and constellation of Lyra near the horizon. November 16 2007, Brittany, France

Laurent Laveder

PIX4637831

Remains of the Crab Supernova (M1) in the Taurus - This image, made by the Very Large Telescope in November 1999, shows in detail the gas remains of the supernova that exploded in 1054. In the center of the picture, the pulsar of the Crab. M1 with the FORS2 instrument in imaging mode in the morning of November 10, 1999. It is the remnant of a supernova explosion at a distance of about 6,000 light - years, observed almost 1000 years ago, in the year 1054. It contains a neutron star near its center that spins 30 times per second around its axis In this picture, the red light is predominantly produced by hydrogen emission from material ejected by the star that exploded. The blue light is predominantly emitted by very high - energy (“relativistic”) electrons that spiral in a large - scale magnetic field (so - called syncrotron emission). It is believed that these electrons are continuously accelerated and ejected by the rapidly spinning neutron star at the centre of the nebula and which is

Remains of the Crab Supernova (M1) in the Taurus - This image, made by the Very Large Telescope in November 1999, shows in detail the gas remains of the supernova that exploded in 1054. In the center of the picture, the pulsar of the Crab. M1 with the FORS2 instrument in imaging mode in the morning of November 10, 1999. It is the remnant of a supernova explosion at a distance of about 6,000 light - years, observed almost 1000 years ago, in the year 1054. It contains a neutron star near its center that spins 30 times per second around its axis In this picture, the red light is predominantly produced by hydrogen emission from material ejected by the star that exploded. The blue light is predominantly emitted by very high - energy (“relativistic”) electrons that spiral in a large - scale magnetic field (so - called syncrotron emission). It is believed that these electrons are continuously accelerated and ejected by the rapidly spinning neutron star at the centre of the nebula and which is

PIX4582982

Constellation Cancer - Cancer constellation - At the top right, the star Pollux des Gemeaux. Cancer (the Crab) is a rather small constellation of 506 square degrees without any bright stars, however, the stick figure above strongly hints at a crab - like shape. The ecliptic runs through the middle of the main stars, which makes it one of the 12 zodiacal constellations. It is best seen in the early evening in March. The most obvious feature in the image above is the large open cluster Messier 44, also known as Praesepe, which appears to the unaided eye as a fuzzy patch. It is easly resolved into numerous faint stars in binoculars, hence its popular name, the Beehive cluster. Although inconspicuous, the constellation gave its name to the Tropic of Cancer. In ancient times Cancer was where the Sun appeared at its maximum mid - day elevation at the time of the (northern) summer solstice. Because of the precession of the equinoxes the northern summer solstice now occurs when the Sun is in T

Constellation Cancer - Cancer constellation - At the top right, the star Pollux des Gemeaux. Cancer (the Crab) is a rather small constellation of 506 square degrees without any bright stars, however, the stick figure above strongly hints at a crab - like shape. The ecliptic runs through the middle of the main stars, which makes it one of the 12 zodiacal constellations. It is best seen in the early evening in March. The most obvious feature in the image above is the large open cluster Messier 44, also known as Praesepe, which appears to the unaided eye as a fuzzy patch. It is easly resolved into numerous faint stars in binoculars, hence its popular name, the Beehive cluster. Although inconspicuous, the constellation gave its name to the Tropic of Cancer. In ancient times Cancer was where the Sun appeared at its maximum mid - day elevation at the time of the (northern) summer solstice. Because of the precession of the equinoxes the northern summer solstice now occurs when the Sun is in T

PIX4589441

Constellation Cancer - Cancer constellation - At the top right, the star Pollux des Gemeaux. Cancer (the Crab) is a rather small constellation of 506 square degrees without any bright stars, however, the stick figure above strongly hints at a crab - like shape. The ecliptic runs through the middle of the main stars, which makes it one of the 12 zodiacal constellations. It is best seen in the early evening in March. The most obvious feature in the image above is the large open cluster Messier 44, also known as Praesepe, which appears to the unaided eye as a fuzzy patch. It is easly resolved into numerous faint stars in binoculars, hence its popular name, the Beehive cluster. Although inconspicuous, the constellation gave its name to the Tropic of Cancer. In ancient times Cancer was where the Sun appeared at its maximum mid - day elevation at the time of the (northern) summer solstice. Because of the precession of the equinoxes the northern summer solstice now occurs when the Sun is in T

Constellation Cancer - Cancer constellation - At the top right, the star Pollux des Gemeaux. Cancer (the Crab) is a rather small constellation of 506 square degrees without any bright stars, however, the stick figure above strongly hints at a crab - like shape. The ecliptic runs through the middle of the main stars, which makes it one of the 12 zodiacal constellations. It is best seen in the early evening in March. The most obvious feature in the image above is the large open cluster Messier 44, also known as Praesepe, which appears to the unaided eye as a fuzzy patch. It is easly resolved into numerous faint stars in binoculars, hence its popular name, the Beehive cluster. Although inconspicuous, the constellation gave its name to the Tropic of Cancer. In ancient times Cancer was where the Sun appeared at its maximum mid - day elevation at the time of the (northern) summer solstice. Because of the precession of the equinoxes the northern summer solstice now occurs when the Sun is in T

PIX4589405

Remains of the Crab Supernova (M1) in the Taurus and Crab Pulsar - This picture shows a time sequence for the pulsar in the Crab nebula, shown in context against an image, also taken with the Kitt Peak 4 - meter Mayall telescope. Both the nebula and its central pulsar were created by a supernova explosion in the year 1054 A.D. The enlarged region is a mosaic of 33 time slices, ordered from top to bottom and from left to right. Each slice represents approximately one millisecond in the period of the pulsar. The brighter, primary pulse is visible in the first column: the weaker, broader inter - pulse can be seen in the second column. These data were taken with the Kitt Peak Photon Counting Array (KPCA) at the Kitt Peak 4 - meter Mayall telescope during the night of 20 October 1989, using a standard B - band optical filter, and represent a phased accumulation of almost two hours of observation. The observed period at the telescope was 33.36702 milliseconds. Due to poor weather and a long

Remains of the Crab Supernova (M1) in the Taurus and Crab Pulsar - This picture shows a time sequence for the pulsar in the Crab nebula, shown in context against an image, also taken with the Kitt Peak 4 - meter Mayall telescope. Both the nebula and its central pulsar were created by a supernova explosion in the year 1054 A.D. The enlarged region is a mosaic of 33 time slices, ordered from top to bottom and from left to right. Each slice represents approximately one millisecond in the period of the pulsar. The brighter, primary pulse is visible in the first column: the weaker, broader inter - pulse can be seen in the second column. These data were taken with the Kitt Peak Photon Counting Array (KPCA) at the Kitt Peak 4 - meter Mayall telescope during the night of 20 October 1989, using a standard B - band optical filter, and represent a phased accumulation of almost two hours of observation. The observed period at the telescope was 33.36702 milliseconds. Due to poor weather and a long

PIX4583092

Remnants of the Crab Supernova (M1) in the Taurus - This is a mosaic image, one of the largest ever taken by Nasa's Hubble Space Telescope of the Crab Nebula, a six - light - year - wide expanding remnant of a star's supernova explosion. Japanese and Chinese astronomers recorded this violent event nearly 1,000 years ago in 1054, as did, almost certainly, Native Americans. The orange filaments are the tattered remains of the star and consist mostly of hydrogen. The rapidly spinning neutron star embedded in the center of the nebula is the dynamo powering the nebula's eerie interior bluish glow. The blue light comes from electrons whirling at nearly the speed of light around magnetic field lines from the neutron star. The neutron star, like a lighthouse, ejects twin beams of radiation that appear to pulse 30 times a second due to the neutron star's rotation. A neutron star is the crushed ultra - dense core of the exploded star. The Crab Nebula derived its name from its appearance in a dra

Remnants of the Crab Supernova (M1) in the Taurus - This is a mosaic image, one of the largest ever taken by Nasa's Hubble Space Telescope of the Crab Nebula, a six - light - year - wide expanding remnant of a star's supernova explosion. Japanese and Chinese astronomers recorded this violent event nearly 1,000 years ago in 1054, as did, almost certainly, Native Americans. The orange filaments are the tattered remains of the star and consist mostly of hydrogen. The rapidly spinning neutron star embedded in the center of the nebula is the dynamo powering the nebula's eerie interior bluish glow. The blue light comes from electrons whirling at nearly the speed of light around magnetic field lines from the neutron star. The neutron star, like a lighthouse, ejects twin beams of radiation that appear to pulse 30 times a second due to the neutron star's rotation. A neutron star is the crushed ultra - dense core of the exploded star. The Crab Nebula derived its name from its appearance in a dra

PIX4583010

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