'Ultraviolet Ray' images and/or videos results page 1 of 1

Laser Robotics, 2016 (Collage on canvas)

premium — Laser Robotics, 2016 (Collage on canvas)

Laser Robotics, 2016 (Collage on canvas)

AUH7392106

The electromagnetic spectrum - Electromagnetic spectrum -Artwork - Artist's view of the different means of observing the electromagnetic spectrum on the ground and in space. Artistic view showing the different instruments used to study the electromagnetic spectrum

D. Ducros

PIX4650395

Crab Nebula seen in different wavelength - The Crab Nebula in multi wavelength: M1, the Crab Nebula, is the rest of a supernova that exploded on July 4, 1054. It is located about 6500 light years from Earth in the constellation Taurus. At the heart of this nebula is a pulsar. To obtain this photo, different observatories and telescopes combined their observations; the VLA provided the radio image (in red), the Spitzer telescope the infrared image (in yellow), the Hubble telescope for the visible part (here in green), XMM-Newton the ultraviolet image (in blue) and the Chandra telescope for X-ray data (purple). The pulsar is the bright spot in the center of the image. The unusual image was produced by combining data from telescopes spanning almost the entire electromagnetic spectrum, from radio waves to X-rays. The Karl G. Jansky Very Large Array (VLA) provided information about the nebula gathered in the radio regime (colored in red). Nasa's Spitzer Space Telescope took images in the in

PIX4626499

WTW, TX, TY, YT, TTY, TZ, UU, UV, VU (engraving)

English School, (20th century)

LLM11692391

Light refraction, 2019 (photomanipulation)

Light refraction, 2019 (photomanipulation)

Caminker, Alex

AHN5936116

Two planets, 2019 (mixed media)

Caminker, Alex

AHN6096359

Re-action, 2019 (mixed media)

Caminker, Alex

AHN6096373

Uv vsion,2019,(collage)

Caminker, Alex

AHN5932512

Allways and everywhere, 2019 (collage)

Caminker, Alex

AHN5932513

Blue fog, 2019 (mixed media)

Caminker, Alex

AHN6096364

Untitled, 2019 (mixed media)

Caminker, Alex

AHN6096376

Garden, 2019 (collage)

Caminker, Alex

AHN5918358

Invert, 2019 (mixed media)

Caminker, Alex

AHN6096367

The Sun as seen by SDO on October 2, 2014

PIX7223384

Invisible, 2019 (mixed media)

Caminker, Alex

AHN6096362

Levels, 2019 (photography)

Caminker, Alex

AHN6096363

Silver plants, 2019 (photo)

Caminker, Alex

AHN6096375

Silver mushrooms, 2019 (photo)

Caminker, Alex

AHN6096371

Natural carpet, 2019 (mixed media)

Caminker, Alex

AHN6096378

Crystal pink flower, 2019 (photography)

Caminker, Alex

AHN6096360

Untitled, 2019 photography)

Caminker, Alex

AHN6096361

Rocks and minerals glow under UV light in laboratory workshop.

AVE8890471

Rocks and minerals glow under UV light in laboratory workshop.

AVE8890481

Radial Iridescent Interpenetration, 1913-14 (oil on canvas)

Balla, Giacomo (1871-1958)

Luisa Ricciarini

LRI4612928

Bridge, 2019 (phtography)

Caminker, Alex

AHN6096380

Traitement therapeutique d'un chien aux rayons ultraviolets dans une ecole veterinaire a Londres

UIS5081977

Far Galaxies - Chandra Deep Field South - Distant Galaxies - GOODS Chandra Deep Field South - A myriad of distant galaxies, accompanied by a few stars of our Lactee Way, covers almost the entire picture. Some detected galaxies are a billion times weaker than the human eye can perceive without instrument. Many new galaxies are so distant that they appear to us as they were when the Universe was only two billion years old. The image was made by the Very Large Telescope and the 2.2m telescope of La Silla within the framework of the GOODS programme, an extensive programme of study of primordial galaxies conducted by different terrestrial and spatial observatories, in a field of the boreal constellation of the Great Bear and in a field of the southern hemisphere, as here in the constellation of the Furnace. November 2008. Obtained in part with the Very Large Telescope, the image contains more than 27 million pixels and is the result of 55 hours of observations with the VIMOS instrument. Thi

PIX4613813

Sirius A and Sirius B in the Big Dog - Sirius A and Sirius B seen in X - ray - Sirius A and Sirius B in the Big Dog seen in X-ray by the Chandra telescope. The brightest source on this image is Sirius B, a white dwarf star whose surface, heated at a temperature of 25,000 degres, emits huge X-rays. The other point is Sirius A, the brightest star in the sky in visible light, but practically non-existent in this wavelength. An X - ray image of the Sirius star system located 8.6 light years from Earth. This image shows two sources and a spike - like pattern due to the support structure for the transmission grating. The bright source is Sirius B, a white dwarf star that has a surface temperature of about 25,000 degrees Celsius which produces very low energy X - rays. The dim source at the position of Sirius A, a normal star more than twice as massive as the Sun, may be due to ultraviolet radiation from Sirius A leaking through the filter on the detector. In contrast, Sirius A is the brighte

PIX4571724

Telescopes Astro - 1 - ASTRO - 1 telescopes - View of telescopes in orbit around the Earth. Installed aboard the space shuttle Columbia, they observed the sky in ultraviolet and X-ray for 10 days in December 1990. ASTRO - 1 telescopes are documented in the payload bay of the space shuttle Columbia, and backdropped against the cloud - covered surface of the Earth. In the center of the frame are three ultraviolet telescopes mounted and precisely coaligned on a common structure, called the cruciform, that is attached to the instrument pointing system. December 1990

PIX4646265

Nebula NGC 604 in the galaxy M33 - NGC 604 star forming nebula - NGC 604, is a very large star-forming region located in the galaxy M33 of the Triangle. This image is a composite of X-ray images (blue) obtained by the Chandra Space Telescope and visible (green and red) by the Hubble Space Telescope. The study of very hot gas observed in X-ray allows us to better understand the star formation activity within this nebula. NGC 604, is one of the largest known seething cauldrons of star birth in a nearby galaxy. NGC 604 is similar to familiar star - birth regions in our Milky Way galaxy, such as the Orion Nebula, but it is vastly larger in extent and contains many more recently formed stars. This monstrous star - birth region contains more than 200 brilliant blue stars within a cloud of glowing gases some 1,300 light - years across, nearly 100 times the size of the Orion Nebula. The bright stars in NGC 604 are extremely young having formed a mere 3 million years ago. The most massive stars

PIX4617509

Satellites, Scientific, Netherlands The Astronomical Netherlands Satellite (ANS 1), 1974

UIS5070774

Instruments Placed in the Noseof Sputnik 2 for the Measurement of Solar Radiation in the Hard Spectrum, 1957 (photo)

UIG3904046

Nebula NGC 6726 - 27 - 29 in the Southern Crown - The Corona Australis nebula (NGC 6726 - 27 - 29) Image of R Coronae Australis region in the southern Milky Way, obtained with the Wide Field Imager (WFI) (camera) at the 2.2 - m MPG/ESO Telescope on La Silla (Chile). The sky field shown measures approx. 33.7 x 31.9 arcmin2 (about the diameter of the full moon). The R Coronae Australis complex of young stars and interstellar gas clouds is one of the nearest star - forming regions, at a distance of approx. 500 light - years from the Sun. It is seen in the southern constellation of that name (The “Southern Crown”). R Coronae Australis, the bright star from which the entire complex is named, is located at the center of the field and illuminates the reddish nebula around it. The bright star in the lower part, illuminating a somewhat bluer nebula, is known as TY Coronae Australis. The brightness of these two stars and several others in the same field is variable. They belong to the so - calle

PIX4620222

Southern Crown Nebula - The Corona Australis nebula (NGC 6726 - 27 - 29) - R Coronae Australis is one of the closest and most intense star-forming regions; visible in the southern hemisphere, it is located about 500 years from Earth. R Coronae Australis is the star in the center of the image that illuminates a reddish nebula around it. Image obtained in Chile at the observatory of La Silla with the 2.2 meter MPG/ESO telescope. Image of R Coronae Australis region in the southern Milky Way, obtained with the Wide Field Imager (WFI) (camera) at the 2.2 - m MPG/ESO Telescope on La Silla (Chile). The R Coronae Australis complex of young stars and interstellar gas clouds is one of the nearest star - forming regions, at a distance of approx. 500 light - years from the Sun. It is seen in the southern constellation of that name (The “Southern Crown”). R Coronae Australis, the bright star from which the entire complex is named, is located at the center of the field and illuminates the reddish ne

PIX4620317

Centaurus A Elliptical Galaxy (NGC 5128) in the Centaur - Galaxy Centaurus A - The NGC 5128 galaxy is about 11 million years away - light from Earth. This image from the Hubble Space Telescope (HST) shows the star flames that occur in the dark band of the galaxy. This giant galaxy is a powerful radio source known as Centaurus A. It is an active galaxy whose energy comes from a supermassive black hole. Centaurus A, also known as NGC 5128, is well known for its dramatic dusty lanes of dark material. Hubble's observations, using its most advanced instrument, the Wide Field Camera 3, are the most detailed ever made of this galaxy. They have been combined here in a multi - wavelength image that reveals never - before - seen detail in the dusty portion of the galaxy. As well as features in the visible spectrum, this composite shows ultraviolet light from young stars, and near - infrared light, which lets us glimpse some of the detail otherwise obscured by the dust. The dark dust lane that cr

PIX4612191

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