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{"event":"custom_event","event_name":"view_search_result","event_category":"browse_catalog","keyword":"sternstrecken","search_type":"standard","search_bridgeman_artists":"false","search_mode":"automatic","search_zero_result":"false","search_results":153,"search_results_page_number":1}

'Sternstrecken' Bilder und Clips Suchergebnisse page 1 of 2

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Bilder zu 'Sternstrecken' gefunden, 153

Star Line - The constellation of Orion - Star trails - The constellation of Orion - Because of the Earth's rotation, leaving the camera open, the stars advance towards the background of the sky. During the installation, gradually changing the focal length of the lens, the stars spread out and reveal their true color. Here is the constellation of Orion photographed in this way during a 30-minute installation in ISO 400. Here one sees the stars of the constellation of Orion recorded in an exposure of about 30 minutes, during which time the lens focus was moved from infinity to about 1 meter in a series of 10 steps about three minutes apart. The effect is to reveal the star colours and that of the vivid red Orion nebula
Halley's comet - Halley's comet - Halley's comet seen on April 10, 1986 in Peru. Glowing at 6th magnitude, Comet Halley exhibits a faint 90 degree wide fan - shaped dust tail. The dust tail is very difficult to see in this photo because it is superimposed on the bright background of the Milky Way. The blue ion tail is a bit easier to see, trailing off to the upper right of the coma. This photo was taken on April 10 1986, the day of Halley's closest approach to the Earth. Stars appear as streaks because the photo was guided on the comet which was moving rapidly relative to the starry background
Stars - The view to the north from Siding Spring - Photographic pose of several hours made in Australia; the northern Celestial pole is here 30 degrees below the horizon. As the Earth rotates beneath them the stars appear to drift across the sky from east to west. From a dark site, a camera with its shutter left open will record the apparent movement of the stars. This is the view from Siding Spring Mountain, the site of the telescopes of Anglo - Australian Observatory. It is located about 30 degrees south of the equator, so the north celestial pole is 30 degrees below the northern horizon. Behind the camera the south celestial pole is about 30 degrees above the horizon
Star Trails - Star Trails - Lighted Trees and Star Lines. Iran Trees and star trails
Circumpolar - South Hemisphere - South celestial pole star trails - Photographic pose of several hours around the south celeste pole. As the earth spins beneath the stars they appear to move across the sky from east to west. However, if one looks in the direction of the celestial poles, the stars appear to circle a single point on the sky. This is the position of the earth's axis of rotation projected into space. This picture was made from Siding Spring Observatory in Australia, so the pivotal point is 30 degrees above the northern horizon, which is the geographical latitude of Siding Spring. In the northern sky there is a bright star very close to the celestial pole. By contrast the region of the south celestial pole is barren
Orion's belt rising over the lights of Coonabarabran - Photographic pose of several hours on the constellation Orion. From Siding Spring Mountain, Australia, there is a clear view to the eastern horizon, directly over the small town of Coonabarabran about 26 km from the telescopes. Here we see the three distinctive trails of Orion's belt rising above the town. The rightmost star of the line of three is Minkata, and it is within a degree of the celestial equator. The point on the horizon where it rises is very close to due east and similarly its setting point is almost exactly due west. Minkata has long been an important navigation star. and its trail is a straight line, while either side of Orion's belt, towards the celestial poles, the star trails become increasingly curved.
Star line - Star trails - Long pose on the constellation of Orion that marks the Celestial Ecuador. Iran. Long exposure on the constellation of Orion. Iran
Circumpolar - Star trails around north celestial pole - Photographic pose around the polar star
Stars - The Southern Cross - Alpha and Beta of Centaur - Southern Cross and pointers - Star trails - Because of the Earth's rotation, leaving the camera open, the stars advance towards the background of the sky. During the installation, gradually changing the focal length of the lens, the stars spread out and reveal their true color. Here it is the constellation of the Southern Cross (center right) and the Centaurus Alpha and Beta stars, in the center below, that are photographed in this way during a 30-minute pose. Star images are point sources of light of widely varying intensity. Normally, no single photographic exposure on colour film can capture their subtle colours. Those stars whose intensity is just right for their colour to be recorded appear insignificant on the photograph, while anything brighter is overexposed and washed out. By changing the focus of the lens during a star trail exposure, star images are spread out over the film surface. This effectively changes the amount of light in each star image as well as making it bigger. If this is done in a series of steps, as here, sooner or later all the star images will be recorded with an exposure that will reveal the star colours. Here we see the stars of the Southern Cross and pointers (alpha and beta Cen) recorded in an exposure of about 30 minutes, during which the lens focus was moved from infinity to about 1m in about 15 equally spaced steps
Eclipse de Lune - 28/09/2015 - Lunar eclipse September 28 2015: Total Eclipse of Moon of 28 September 2015
Stars - The Southern Cross - Alpha and Beta of Centaur - Southern Cross and pointers - Star trails - Because of the Earth's rotation, leaving the camera open, the stars advance towards the background of the sky. During the installation, gradually changing the focal length of the lens, the stars spread out and reveal their true color. Here, the constellation of the Southern Cross and the Alpha and Beta stars of the Centaurus, on the left, are photographed this way during a 40mn pose. Star images are point sources of light of widely varying intensity. Normally, no single photographic exposure on colour film can capture their subtle colours. Those stars whose intensity is just right for their colour to be recorded appear insignificant on the photograph, while anything brighter is overexposed and washed out. By changing the focus of the lens during a star trail exposure, star images are spread out over the film surface. This effectively changes the amount of light in each star image as well as making it bigger. If this is done in a series of steps, as here, sooner or later all the star images will be recorded with an exposure that will reveal the star colours. Here we see the stars of the Southern Cross and pointers (alpha and beta Cen) recorded in an exposure of about 40 minutes, during which the lens focus was moved from infinity to about 2m in six steps five minutes apart
Star line - Star trails - Long pose on the constellation of Orion that marks the Celestial Ecuador. Iran. Long exposure on the constellation of Orion. Iran
Star Line - Star trail
Star trails with Moon rise - Moon rise seen in long pose. Iran. Moon and Antares rising. Long exposure image. Iran
Star line - Star trails - Long pose on the constellation of Orion that marks the Celestial Ecuador. Iran. Long exposure on the constellation of Orion. Iran
Star line - Star trails - Long pose on the constellation of Orion that marks the Celestial Ecuador. Iran. Long exposure on the constellation of Orion. Iran
Star line - Star trails - Long pose on the constellation of Orion that marks the Celestial Ecuador. Iran. Long exposure on the constellation of Orion. Iran
Star line - Star trails - Long pose on the constellation of Orion that marks the Celestial Ecuador. Iran. Long exposure on the constellation of Orion. Iran
Circumpolar above the dome of the 1.93 m of the Observatory of Haute - Provence - Haute - Provence Observatory, the 1.93 m telescope dome - Photographic pose showing the apparent rotation of stars around the polar star (circumpolar). Below, the dome of the 1.93 m telescope of the Observatory of Haute Provence. This is where the first exoplanet was discovered in 1995. The Observatory of Haute-Provence is located in the south-east of France, near the village of St. Michel l'Observatoire, a hundred kilometers north of Marseille, on a plateau with an average altitude of 650 meters. Long exposure image of starry sky around the pole star (circumpolar). Below, the 1.93 m telescope dome. Here has been discovered the first extrasolar planet (51 Peg b) in 1995. OHP is situated in the southeast of France, it lies at an altitude of about 650 m, near the village of Saint-Michel l'Observatoire
Zodiacal light - Star Trainee - Zodiacal light - Star trails - The visible glow in the sky is called the zodiacal light. It comes from the reflection of the light of the Sun on the countless interplanetary dust; it draws the plan of the Solar System. 9 March 2007 at sunset, Treguennec (Finistere - France). The faint cone of light extending from the horizon along the ecliptic is known as zodiacal light. It comes from the reflexion of the sun's light off tiny interplanetary dust particles in the plane of the solar system. 6 minutes exposure, March 9 2007, sunset, Treguennec (Finistere - France)
Star Line - Star trail
Circumpolar - South Hemisphere - Star trails around the south celestial pole - 10h30 photographic installation on 400 ISO film around the south celeste pole. Siding Spring's 3.9m telescope dome in the foreground. By pointing a camera towards the south (or to the north in the northern hemisphere) at night, we can record the paths of stars which never set. They appear to circle the apparent position of the Earth's axis of rotation projected on the sky. The elevation of this position above the local horizon indicates our local geographical latitude, about 30 degrees south at Siding Spring. The angle swept out by the arcs is an indication of the exposure time, which was about 10.5 hours on 400 ISO colour film. This kind of exposure is only possible from an extremely dark site
Circumpolar - hemisphere sud - Dawn and evening twilights reflected on the AAT dome - Photographic pose of 6 hours during a summer night, around the south Celeste pole. Siding Spring's 3.9m telescope dome in the foreground. From a truly dark site like Siding Spring, Australia, the duration of star trail exposures is governed only by the length of the night. The shortest nights are in December, at the height of summer, when it is truly dark for a little over six hours. “True darkness” for astronomers is defined as the period between “” astronomical twilights” when the sun is 18 or more degrees below the horizon. This exposure was a little over six hours long on one December night, and the AAT dome reflects both the evening twilight on the west (right) of the dome and the morning twilight from the eastern glow on the left
Circumpolar - Hemisphere south and hemisphere north - North and South celestial pole star trails - Photographic pose of several hours around the south celeste pole (left) in Australia and around the north pole in La Palma, Canary Islands. As the earth spins beneath the stars they appear to move across the sky from east to west. However, if one looks in the direction of the celestial poles, the stars appear to circle a single point on the sky. This is the position of the earth's axis of rotation projected into space. These pictures were made from Siding Spring Observatory in Australia, and from the La Plama Observatory in the Canary Islands, so the pivotal points are about 30 degrees above their respective horizons, which reflects their geographical latitudes
Circumpolar - South Hemisphere - Star trails around the south celestial pole - Photographic pose of several hours around the south celeste pole. Siding Spring's 3.9m telescope dome in the foreground. The reddish color of the sky is due to the volcanic eruption of the Pinatubo. On June 15, 1991, after weeks of rumbling and venting steam and poisonous gas, Mt Pinatubo exploded on the island of Luzon, in the Phillipines. This was the largest volcanic eruption for nearly a century. The eruption killed over 700 people and ejected several cubic kilometers of dust and gas over 35 km high into the stratosphere. The effects were felt around the world and included a temporary global cooling and a thinning of the ozone layer as well as other changes in the global weather pattern. However, the most obvious effect for many people was a milkiness in the daytime sky due to scattering by high altitude aerosols, and corresponding anomalous sunsets and twilights that were noticable for years. This picture was made in early 1992, two hours after sunset, when it is usually completely dark. However, high altitude dust in the stratosphere reflected sunset colours strongly enough for them to be seen (in the sky, at right) and to be reflected again, by the AAT dome. The red reflection was captured in this six - hour exposure. Here the camera is pointing due south, directly at the south celestial pol
Circumpolar above the dome of the 1.93 m of the Observatory of Haute - Provence - Haute - Provence Observatory, the 1.93 m telescope dome - Photographic pose showing the apparent rotation of stars around the polar star (circumpolar). Below, the dome of the 1.93 m telescope of the Observatory of Haute Provence. This is where the first exoplanet was discovered in 1995. The Observatory of Haute-Provence is located in the south-east of France, near the village of St. Michel l'Observatoire, a hundred kilometers north of Marseille, on a plateau with an average altitude of 650 meters. Long exposure image of starry sky around the pole star (circumpolar). Below, the 1.93 m telescope dome. Here has been discovered the first extrasolar planet (51 Peg b) in 1995. OHP is situated in the southeast of France, it lies at an altitude of about 650 m, near the village of Saint-Michel l'Observatoire
Circumpolar - Circumpolar - Photographic pose showing the apparent rotation of stars around the polar star. Iran. Long exposure image of starry sky around the pole star. Iran
Circumpolar - Circumpolar - Photographic pose showing the apparent rotation of stars around the polar star. Iran. Long exposure image of starry sky around the pole star. Iran
Star Trains on the Observatory of Siding Spring - Star trails above Anglo - Australian Observatory - Photographic installation of several hours and dome of Siding Spring's 3.9m telescope. As the earth rotates the stars appear to move across the sky, as do the more obvious sun and Moon This effect is easily recorded by leaving a camera outdoors with its shutter open during the night. To make this picture, the camera was pointed to the southwest, towards the dome of the AAT, from the UK Schmidt building on Siding Spring Mountain in New South Wales
Circumpolar in Ecuador - Star Trail from the Equator (Ecuador) - Star line taken from Ecuador, Ecuador. 10 hours of cumulative poses show us more than 90% of all the visible sky (the remaining 10% are drowned in solar light). A shooting star indicates the South Pole to the horizon to the left of the image. The north pole is on the right horizon. This image is an unprecedented star trail image taken from the Equator (this imaginary line that splits the Earth into the two hemispheres) in Ecuador (the country). If you stand on the Equator line you can see the Southern Pole at the horizon to the South (left of the image) and the Northern pole at the horizon on the opposite direction. The Earth rotation will make all the sky and stars look like they rotate around these two points, making them appear as concentric circles (which look like ellipses on this distorsioning fish eye image). Note that on this image, that cumulates 10 hours of exposure starting 1 hour after sunset and finishing 1 hour before sunrise (nights and days always last 12 hours on the Equator, it is a permanent equinox), more than 90% of the sky is 'visible', this is another particularity of being on the ecuator line: you can observe the largest part of the sky during any night. An extremely bright meteor appeared during that night and seems to be pointing at the Southern Pole (extreme left of the image)
Queue d'étoiles - Moonset in the Warrumbungles - Photographic pose of several hours on the stars and the crescent moon. The picture here was made on one partially cloudy night at Siding Spring. In the foreground are the distinctive shapes of the Warrumbungle mountains in outback New South Wales. The exposure, on 400 ISO transparency film, was begun at the end of astronomical twilight, when the sun has descended 18 degrees below the horizon. There was a crescent moon and cloud around the south - western horizon. The exposure continued for several hours after the moon had set, and breaks in the star trails reveal that cloud had come and gone during the night
Star Line - Moon - Venus - Star trails - Moon and Venus - Sunset and Venus photography in long pose. Moon and Venus setting, Alamoot valley, west of Tehran
Polar ciricumpole above the dome of the GTC - La Palma Observatory: The GTC (Gran Telescopio Canarias) is a 10.4 m telescope
Stars on the SIRENE Observatory - Star trails above the amateur observatory SIRENE - France - Several decades of military presence have limited urban settlements and thus light pollution on the Albion plateau. This photographic pose of over an hour, showing the rotation of the stars of the constellations of Cassiopee and Persee above the domes of the SIRENE observatory, testifying to the absence of genant halos of light. As far as the horizon is concerned, one can even guess a few peaks of the Alps, which glow slightly under the light of a gibbous Moon. During the installation, the nightlife of an active observation site was recorded: the domes rotated, the telescopes moved, red lamps were lit to read maps or set instruments, and an animator used a green laser to design a few stars for the public. One hour exposure star trails above the SIRENE amateur observatory in Luberon (Vaucluse - France). Located on the Albion plateau, an ancient military base, this place is well preserved from light pollution. During the exposure, activities of a public observation night have been recorded: dome has turned, red lights have been turned on, green laser to show stars has been used
Stars on the castle of Peyrepertuse (11) - Star trails over the castle of Peyrepertuse - Stars on the castle of Peyrepertuse in the Aude. Long exposure trail of stars over the Cathar castle of Peyrepertuse
Star trails over the castle of Arques (11) - Star trails over the castle of Arques - Star stars above the chateau cathare d'Arques in the Aude. Long exposure trail of stars over the Cathar castle of Arques
Circumpolar - hemisphere sud - Star trails around the south celestial pole - 10h30 photographic installation on 400 ISO film around the south celeste pole. Siding Spring's 3.9m telescope dome in the foreground. By pointing a camera towards the south (or to the north in the northern hemisphere) at night, we can record the paths of stars which never set. They appear to circle the apparent position of the Earth's axis of rotation projected on the sky. The elevation of this position above the local horizon indicates our local geographical latitude, about 30 degrees south at Siding Spring. The angle swept out by the arcs is an indication of the exposure time, which was about 10.5 hours on 400 ISO colour film. This kind of exposure is only possible from an extremely dark site