'Optical Phenomena' Bilder und Clips Suchergebnisse

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Bilder zu 'Optical Phenomena' gefunden, 84

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Sunset, 10 May 1884

Sunset, 10 May 1884

UIS5086156

Sunset, 4 September 1885

Sunset, 4 September 1885

UIS5086155

Sunset, 10 May 1884

Sunset, 10 May 1884

UIS5086164

Afterglow caused by the eruption of Krakatoa, 9 November 1883

Afterglow caused by the eruption of Krakatoa, 9 November 1883

UIS5086103

Sunset and afterglow, Chelsea, London, 12 July 1886

Sunset and afterglow, Chelsea, London, 12 July 1886

UIS5086111

Sustained light after sunset, 12 July 1886

Sustained light after sunset, 12 July 1886

UIS5086120

Rose flush following sunset, 10 May 1884

Rose flush following sunset, 10 May 1884

UIS5086146

Amber afterglow with crepuscular rays, September 1885

Amber afterglow with crepuscular rays, September 1885

UIS5086108

Sunset at Chelsea, London, 14 July 1886

Sunset at Chelsea, London, 14 July 1886

UIS5086123

Sunset and noctilucent cloud, 6 July 1885

Sunset and noctilucent cloud, 6 July 1885

UIS5086125

Afterglow two hours after sunset, 13 September 1886

Afterglow two hours after sunset, 13 September 1886

UIS5086129

Afterglow following sunset, 10 May 1884

Afterglow following sunset, 10 May 1884

UIS5086139

Sunset and afterglow caused by the eruption of Krakatoa, November 1883

Sunset and afterglow caused by the eruption of Krakatoa, November 1883

UIS5086099

Afterglow caused by the eruption of Krakatoa, 9 November 1883

Afterglow caused by the eruption of Krakatoa, 9 November 1883

UIS5086089

Sunset with 'Bishop's Ring' clearly defined, 10 May 1884

Sunset with 'Bishop's Ring' clearly defined, 10 May 1884

UIS5086128

Twilight and Afterglow Effects at Chelsea, 26 November 1883', 1888

Twilight and Afterglow Effects at Chelsea, 26 November 1883', 1888

UIS5090773

Sky sketches, Chelsea, London, 9-10 May 1884

Sky sketches, Chelsea, London, 9-10 May 1884

UIS5090782

Sunset showing amber afterglow with rays, 11 September 1886

Sunset showing amber afterglow with rays, 11 September 1886

UIS5086117

Afterglow with crepuscular rays, 13 September 1885

Afterglow with crepuscular rays, 13 September 1885

UIS5086207

Afterglow an hour after official sunset time, Chelsea, London, 14 July 1886

Afterglow an hour after official sunset time, Chelsea, London, 14 July 1886

UIS5086135

Coeur de la nebula de la Lagoon dans le sagittarius/HST - This NASA Hubble Space Telescope (HST) image reveals a pair of one - half light - year long interstellar “” twisters”” in the heart of the Lagoon Nebula (Messier 8) which lies 5,000 light - years away in the direction of the constellation Sagittarius. The central hot O type star, Herschel 36 (lower right), is the primary source of the ionizing radiation for the brightest region in the nebula, called the Hourglass. Other hot stars, also present in the nebula, are ionizing the extended optical nebulosity. The ionizing radiation induces photo - evaporation of the surfaces of the clouds and drives away violent stellar winds tearing into the cool clouds. Analogous to the spectacular phenomena of Earth tornadoes, the large difference in temperature between the hot surface and cold interior of the clouds, combined with the pressure of starlight, may produce strong horizontal shear to twist the clouds into their tornado - like appearanc

Coeur de la nebula de la Lagoon dans le sagittarius/HST - This NASA Hubble Space Telescope (HST) image reveals a pair of one - half light - year long interstellar “” twisters”” in the heart of the Lagoon Nebula (Messier 8) which lies 5,000 light - years away in the direction of the constellation Sagittarius. The central hot O type star, Herschel 36 (lower right), is the primary source of the ionizing radiation for the brightest region in the nebula, called the Hourglass. Other hot stars, also present in the nebula, are ionizing the extended optical nebulosity. The ionizing radiation induces photo - evaporation of the surfaces of the clouds and drives away violent stellar winds tearing into the cool clouds. Analogous to the spectacular phenomena of Earth tornadoes, the large difference in temperature between the hot surface and cold interior of the clouds, combined with the pressure of starlight, may produce strong horizontal shear to twist the clouds into their tornado - like appearanc

PIX4619687

Galaxy clusters Abell 2744 - Black material - X - rays, dark matter and galaxies in cluster Abell 2744

Galaxy clusters Abell 2744 - Black material - X - rays, dark matter and galaxies in cluster Abell 2744

PIX4565787

Galaxy NGC 4631 in Hunting Dogs - Spiral galaxy NGC 4631 in Canes Venatici - Spiral galaxy seen by the slice located at a distance of 30 million years - light. Image obtained by the Hubble Space Telescope (HST). The NASA/ESA Hubble Space Telescope has peered deep into NGC 4631, better known as the Whale Galaxy. Here, a profusion of starbirth lights up the galactic centre, revealing bands of dark material between us and the starburst. The galaxy's activity tapers off in its outer regions where there are fewer stars and less dust, but these are still punctuated by pockets of star formation. The Whale Galaxy is about 30 million light - years away from us in the constellation of Canes Venatici (The Hunting Dogs) and is a spiral galaxy much like the Milky Way. From our vantage point, however, we see the Whale Galaxy edge - on, seeing its glowing centre through dusty spiral arms. The galaxy's central bulge and asymmetric tapering disc have suggested the shape of a whale or a herring to past

Galaxy NGC 4631 in Hunting Dogs - Spiral galaxy NGC 4631 in Canes Venatici - Spiral galaxy seen by the slice located at a distance of 30 million years - light. Image obtained by the Hubble Space Telescope (HST). The NASA/ESA Hubble Space Telescope has peered deep into NGC 4631, better known as the Whale Galaxy. Here, a profusion of starbirth lights up the galactic centre, revealing bands of dark material between us and the starburst. The galaxy's activity tapers off in its outer regions where there are fewer stars and less dust, but these are still punctuated by pockets of star formation. The Whale Galaxy is about 30 million light - years away from us in the constellation of Canes Venatici (The Hunting Dogs) and is a spiral galaxy much like the Milky Way. From our vantage point, however, we see the Whale Galaxy edge - on, seeing its glowing centre through dusty spiral arms. The galaxy's central bulge and asymmetric tapering disc have suggested the shape of a whale or a herring to past

PIX4611784

Heart of the Nebula of the Lagoon (M8) in Sagittarius seen by HST - This NASA Hubble Space Telescope (HST) image reveals a pair of one - half light - year long interstellar “” twisters”” - - eerie funnels and twisted - rope structures (upper left) - - in the heart of the Lagoon Nebula (Messier 8) which lies 5,000 years - - away in the direction of the constellation Sagittarius. The central hot O type star, Herschel 36 (upper left in photo), is the primary source of the ionizing radiation for the brightest region in the nebula, called the Hourglass. Other hot stars, also present in the nebula, are ionizing the extended optical nebulosity. The ionizing radiation induces photo - evaporation of the surfaces of the clouds (seen as a blue “” mist”” at the right of the image), and drives away violent stellar winds tearing into the cool clouds.Analogous to the spectacular phenomena of Earth tornadoes, the large difference in temperature between the hot surface and cold interior of the clouds,

Heart of the Nebula of the Lagoon (M8) in Sagittarius seen by HST - This NASA Hubble Space Telescope (HST) image reveals a pair of one - half light - year long interstellar “” twisters”” - - eerie funnels and twisted - rope structures (upper left) - - in the heart of the Lagoon Nebula (Messier 8) which lies 5,000 years - - away in the direction of the constellation Sagittarius. The central hot O type star, Herschel 36 (upper left in photo), is the primary source of the ionizing radiation for the brightest region in the nebula, called the Hourglass. Other hot stars, also present in the nebula, are ionizing the extended optical nebulosity. The ionizing radiation induces photo - evaporation of the surfaces of the clouds (seen as a blue “” mist”” at the right of the image), and drives away violent stellar winds tearing into the cool clouds.Analogous to the spectacular phenomena of Earth tornadoes, the large difference in temperature between the hot surface and cold interior of the clouds,

PIX4619680

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