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The elliptical galaxy M84 - The elliptical galaxy M84 - The M84 galaxy (NGC 4374) is 55 million light years away from Earth, in the Virgin's cluster. This image is a composite obtained in X-rays (blue), radio (red) and visible (yellow and white). Gas material is ejected from the heart of the galaxy. A supermassive black hole would have caused this jet. This composite image shows M84, a massive elliptical galaxy in the Virgo Cluster, about 55 million light years from Earth. Hot gas around M84 is shown in a Chandra X - ray Observatory image in blue and a radio image from the Very Large Array is shown in red. A background image from the Sloan Digital Sky Survey is shown in yellow and white. A number of bubbles are visible in the hot gas, outlined with blue X - ray emission. These bubbles were blown by relativistic particles generated by the central supermassive black hole in M84. These particles travel outwards in the form of a two - sided jet. Because smaller bubbles are found inside lar

The elliptical galaxy M84 - The elliptical galaxy M84 - The M84 galaxy (NGC 4374) is 55 million light years away from Earth, in the Virgin's cluster. This image is a composite obtained in X-rays (blue), radio (red) and visible (yellow and white). Gas material is ejected from the heart of the galaxy. A supermassive black hole would have caused this jet. This composite image shows M84, a massive elliptical galaxy in the Virgo Cluster, about 55 million light years from Earth. Hot gas around M84 is shown in a Chandra X - ray Observatory image in blue and a radio image from the Very Large Array is shown in red. A background image from the Sloan Digital Sky Survey is shown in yellow and white. A number of bubbles are visible in the hot gas, outlined with blue X - ray emission. These bubbles were blown by relativistic particles generated by the central supermassive black hole in M84. These particles travel outwards in the form of a two - sided jet. Because smaller bubbles are found inside lar

PIX4611313

Light echo of supernova 1987A - July 1989 - The light echo of supernova 1987A - July 1989 - Image obtained with Siding Spring's 3.9m telescope. Supernova 1987A appeared in the constellation Doradus on February 23, 1987. When supernova 1987A was seen to explode in the Large Magellanic Cloud, the Milky Way's nearest companion galaxy, the brilliant flash of light from the self - destructing star had taken about 170,000 years to arrive. Some light was deflected by two sheets of dust near the supernova, and is seen after the star has faded away because it covers a longer path to reach us. The dust responsible for the rings seen here lies in two distinct sheets, about 470 and 1300 light years from the supernova. The colour picture, made by subtracting images on plates taken before and after the supernova, is an accurate reproduction of the colour of the extremely faint light echo, which in turn reflects the yellow colour of the supernova when it was at its brightest, in May 1987.

Light echo of supernova 1987A - July 1989 - The light echo of supernova 1987A - July 1989 - Image obtained with Siding Spring's 3.9m telescope. Supernova 1987A appeared in the constellation Doradus on February 23, 1987. When supernova 1987A was seen to explode in the Large Magellanic Cloud, the Milky Way's nearest companion galaxy, the brilliant flash of light from the self - destructing star had taken about 170,000 years to arrive. Some light was deflected by two sheets of dust near the supernova, and is seen after the star has faded away because it covers a longer path to reach us. The dust responsible for the rings seen here lies in two distinct sheets, about 470 and 1300 light years from the supernova. The colour picture, made by subtracting images on plates taken before and after the supernova, is an accurate reproduction of the colour of the extremely faint light echo, which in turn reflects the yellow colour of the supernova when it was at its brightest, in May 1987.

PIX4582384

Transit de Venus - 06/06/2012 - Transit of Venus (June 6 2012) - Transit of Venus in front of the Sun seen from Hungary, June 6, 2012. Venus is barely visible as a black dot on the upper center of the solar disc. The Transit of Venus is a rare celestial phenomenon happens only twice in each century and the 2012 transit was the last of our time. Image taken from Hungary

Transit de Venus - 06/06/2012 - Transit of Venus (June 6 2012) - Transit of Venus in front of the Sun seen from Hungary, June 6, 2012. Venus is barely visible as a black dot on the upper center of the solar disc. The Transit of Venus is a rare celestial phenomenon happens only twice in each century and the 2012 transit was the last of our time. Image taken from Hungary

Sebastian Voltmer

PIX4588580

Remains of supernova SN 1006 - Supernova remnant SN 1006 - Remains of supernova SN 1006 located 7000 years ago - light in the constellation Wolf. This supernova that appeared in 1006 is the result of a white dwarf star that absorbs the matter of a companion star became unstable and eventually exploded. This image is a composite of X-ray images obtained by the Chandra telescope (blue), by Cerro Tololo's 90 cm telescope (yellow) and by the Digitized Sky Survey (orange and light blue), and by the VLA and the Green Bank's telescope radio (red). Just over a thousand years ago, the stellar explosion known as supernova SN 1006 was observed. It was brighter than Venus, and visible during the day for weeks. The brightest supernova ever recorded on Earth, this spectacular light show was documented in China, Japan, Europe, and the Arab world. Astronomers now understand that SN 1006 was caused by a white dwarf star that captured mass from a companion star until the white dwarf became unstable and

Remains of supernova SN 1006 - Supernova remnant SN 1006 - Remains of supernova SN 1006 located 7000 years ago - light in the constellation Wolf. This supernova that appeared in 1006 is the result of a white dwarf star that absorbs the matter of a companion star became unstable and eventually exploded. This image is a composite of X-ray images obtained by the Chandra telescope (blue), by Cerro Tololo's 90 cm telescope (yellow) and by the Digitized Sky Survey (orange and light blue), and by the VLA and the Green Bank's telescope radio (red). Just over a thousand years ago, the stellar explosion known as supernova SN 1006 was observed. It was brighter than Venus, and visible during the day for weeks. The brightest supernova ever recorded on Earth, this spectacular light show was documented in China, Japan, Europe, and the Arab world. Astronomers now understand that SN 1006 was caused by a white dwarf star that captured mass from a companion star until the white dwarf became unstable and

PIX4583213

Constellation Cancer - Cancer constellation - In the center of the picture, the Creche cluster, M44. Composite of two images. The sky is enlarged in relation to reality. Composite image. Stars are bigger than in reality

Constellation Cancer - Cancer constellation - In the center of the picture, the Creche cluster, M44. Composite of two images. The sky is enlarged in relation to reality. Composite image. Stars are bigger than in reality

B&S.Fletcher

PIX4589381

'1884; Eighteen Hundred Gems of British Columbia Greet You!'; composite photo made up of children's portraits taken the previous year, 1885 (b/w photo)

'1884; Eighteen Hundred Gems of British Columbia Greet You!'; composite photo made up of children's portraits taken the previous year, 1885 (b/w photo)

Maynard, Hannah (1834-1918)

RBC2637624

Solar eruption seen by SOHO 02/04/2001 - Large solar flare seen by SOHO on april 2 2001 - Solar eruption seen by SOHO satellite; the Sun is masked by a coronographer. An image of the Sun taken at the same time by another satellite instrument was superimposed. A large solar flare occurred at 4:51 p.m. EDT, on Monday, April 2, 2001. as Observed by the Solar and Heliospheric Observatory (SOHO) satellite. Solar flares, among the solar systems mightiest eruptions, are tremendous explosions in the atmosphere of the Sun capable of releasing as much energy as a billion megatons of TNT. Caused by the sudden release of magnetic energy, in just a few seconds, solar flares can accelerate solar particles to very high velocities, almost to the speed of light, and heat solar material to tens of millions of degrees. The recent explosion from the active region near the sun's northwest limb hurled a coronal mass ejection into space at a whopping speed of roughly 7.2 million kilometers per hour. Luckily,

Solar eruption seen by SOHO 02/04/2001 - Large solar flare seen by SOHO on april 2 2001 - Solar eruption seen by SOHO satellite; the Sun is masked by a coronographer. An image of the Sun taken at the same time by another satellite instrument was superimposed. A large solar flare occurred at 4:51 p.m. EDT, on Monday, April 2, 2001. as Observed by the Solar and Heliospheric Observatory (SOHO) satellite. Solar flares, among the solar systems mightiest eruptions, are tremendous explosions in the atmosphere of the Sun capable of releasing as much energy as a billion megatons of TNT. Caused by the sudden release of magnetic energy, in just a few seconds, solar flares can accelerate solar particles to very high velocities, almost to the speed of light, and heat solar material to tens of millions of degrees. The recent explosion from the active region near the sun's northwest limb hurled a coronal mass ejection into space at a whopping speed of roughly 7.2 million kilometers per hour. Luckily,

PIX4627092

Active galaxy NGC 1068 in the Whale - Composite X - visible - Active galaxy NGC 1068 seen in visible and X - ray - This visible X composite image shows that a strong stellar wind escapes from the heart of the galaxy NGC 1068. This active galaxy houses a massive black hole and is the object of intense star formation in its spiral arms. NGC 1068 stands at about 50 million years - light. Image obtained by the Chandra satellite in December 2000. This composite X - ray (blue and green) and optical (red) image of the active galaxy, NGC 1068, shows gas blowing away in a high - speed wind from the vicinity of a central supermassive black hole. Regions of intense star formation in the inner spiral arms of the galaxy are highlighted by both optical and X - ray emission

Active galaxy NGC 1068 in the Whale - Composite X - visible - Active galaxy NGC 1068 seen in visible and X - ray - This visible X composite image shows that a strong stellar wind escapes from the heart of the galaxy NGC 1068. This active galaxy houses a massive black hole and is the object of intense star formation in its spiral arms. NGC 1068 stands at about 50 million years - light. Image obtained by the Chandra satellite in December 2000. This composite X - ray (blue and green) and optical (red) image of the active galaxy, NGC 1068, shows gas blowing away in a high - speed wind from the vicinity of a central supermassive black hole. Regions of intense star formation in the inner spiral arms of the galaxy are highlighted by both optical and X - ray emission

PIX4609567

'Gems of British Columbia 1881', composite photo of children's portraits taken in the previous year, 1882 (b/w photo)

'Gems of British Columbia 1881', composite photo of children's portraits taken in the previous year, 1882 (b/w photo)

Maynard, Hannah (1834-1918)

RBC2637623

Panathenaic procession, horses and chariots, frieze in Parthenon cell, illustration from Teatro universale, Raccolta enciclopedica e scenografica, No 341, January 16, 1841

Panathenaic procession, horses and chariots, frieze in Parthenon cell, illustration from Teatro universale, Raccolta enciclopedica e scenografica, No 341, January 16, 1841

DGA3954005

Andromede galaxy (M31) seen in X and infrared - Andromeda galaxy infrared and X - Ray composite - Andromede spiral galaxy seen in X-ray (blue) by the XMM - Newton space telescope and in infrared (orange) by the Herschel space telescope. This mosaic of the Andromeda spiral galaxy highlights explosive stars in its interior, and cooler, dusty stars forming in its many rings. The image is a combination of observations from the Herschel Space Observatory taken in infrared light (seen in orange hues), and the XMM - Newton telescope captured in X - rays (seen in blues). Herschel provides a detailed look at the cool clouds of star birth that line the galaxy's five concentric rings. Massive young stars are heating blankets of dust that surround them, causing them to glow in the longer - wavelength infrared light, known as far - infrared, that Herschel sees. In contrast, XMM - Newton is capturing what happens at the end of the lives of massive stars. It shows the high - energy X - rays that come

Andromede galaxy (M31) seen in X and infrared - Andromeda galaxy infrared and X - Ray composite - Andromede spiral galaxy seen in X-ray (blue) by the XMM - Newton space telescope and in infrared (orange) by the Herschel space telescope. This mosaic of the Andromeda spiral galaxy highlights explosive stars in its interior, and cooler, dusty stars forming in its many rings. The image is a combination of observations from the Herschel Space Observatory taken in infrared light (seen in orange hues), and the XMM - Newton telescope captured in X - rays (seen in blues). Herschel provides a detailed look at the cool clouds of star birth that line the galaxy's five concentric rings. Massive young stars are heating blankets of dust that surround them, causing them to glow in the longer - wavelength infrared light, known as far - infrared, that Herschel sees. In contrast, XMM - Newton is capturing what happens at the end of the lives of massive stars. It shows the high - energy X - rays that come

PIX4609049

Total Eclipse of Sun 07/1991 - Composite 1991 Total Solar Eclipse - The different phases of the total eclipse of Sun of 11 July 1991. Composite Image, July 11, 1991 Total Eclipse of the Sun. Partial phases and corona and mid totality. A total eclipse of the Sun occurs when the orbits of the Sun and Moon line up and the Moon moves in front to the Sun, totally blocking its light from reaching a narrow path on the Earth

Total Eclipse of Sun 07/1991 - Composite 1991 Total Solar Eclipse - The different phases of the total eclipse of Sun of 11 July 1991. Composite Image, July 11, 1991 Total Eclipse of the Sun. Partial phases and corona and mid totality. A total eclipse of the Sun occurs when the orbits of the Sun and Moon line up and the Moon moves in front to the Sun, totally blocking its light from reaching a narrow path on the Earth

Jerry Lodriguss

PIX4627386

M87 elliptical galaxy in Virgo - M87 elliptical galaxy in Virgo - The M87 galaxy (NGC 4486) is 54 million years ago - light from Earth, in the heart of the Virgin's cluster. This composite image obtained by the Hubble space telescope in 2003 and 2006 shows a gigantic jet of gas material ejected from the heart of the galaxy. A supermassive black hole would have caused this jet. The monstrous elliptical galaxy M87 is the home of several trillion stars, a supermassive black hole, and a family of 13,000 globular star clusters. M87 is the dominant galaxy at the center of the neighboring Virgo cluster of galaxies, which contains some 2,000 galaxies. Amid the smooth, yellow population of older stars, the two features that stand out most in this Hubble Space Telescope image of M87 are its soft blue jet and the myriad of starlike globular clusters scattered throughout the image. The jet is a black - hole - powered stream of material that is being ejected from the core of the galaxy. As gaseous

M87 elliptical galaxy in Virgo - M87 elliptical galaxy in Virgo - The M87 galaxy (NGC 4486) is 54 million years ago - light from Earth, in the heart of the Virgin's cluster. This composite image obtained by the Hubble space telescope in 2003 and 2006 shows a gigantic jet of gas material ejected from the heart of the galaxy. A supermassive black hole would have caused this jet. The monstrous elliptical galaxy M87 is the home of several trillion stars, a supermassive black hole, and a family of 13,000 globular star clusters. M87 is the dominant galaxy at the center of the neighboring Virgo cluster of galaxies, which contains some 2,000 galaxies. Amid the smooth, yellow population of older stars, the two features that stand out most in this Hubble Space Telescope image of M87 are its soft blue jet and the myriad of starlike globular clusters scattered throughout the image. The jet is a black - hole - powered stream of material that is being ejected from the core of the galaxy. As gaseous

PIX4611437

Black hole collision in NGC 6240 - Black holes colliding in NGC 6240 - The galaxy NGC 6240, is located about 400 million light years away from Earth in the constellation Ophiuchus. This system consists of two colliding galaxies each with a central black hole; in several millions of years, they will form only one galaxy. A composite X-ray image (red, orange and yellow) and visible from the space telescopes Chandra and Hubble. This image of NGC 6240 contains X - ray data from Chandra (shown in red, orange, and yellow) that has been combined with an optical image from the Hubble Space Telescope. In 2002, the discovery of two merging black holes was announced based on Chandra data in this galaxy. The two black holes are a mere 3,000 light years apart and are seen as the bright point - like sources in the middle of the image. Scientists think these black holes are in such close proximity because they are in the midst of spiraling toward each other - a process that began about 30 million yea

Black hole collision in NGC 6240 - Black holes colliding in NGC 6240 - The galaxy NGC 6240, is located about 400 million light years away from Earth in the constellation Ophiuchus. This system consists of two colliding galaxies each with a central black hole; in several millions of years, they will form only one galaxy. A composite X-ray image (red, orange and yellow) and visible from the space telescopes Chandra and Hubble. This image of NGC 6240 contains X - ray data from Chandra (shown in red, orange, and yellow) that has been combined with an optical image from the Hubble Space Telescope. In 2002, the discovery of two merging black holes was announced based on Chandra data in this galaxy. The two black holes are a mere 3,000 light years apart and are seen as the bright point - like sources in the middle of the image. Scientists think these black holes are in such close proximity because they are in the midst of spiraling toward each other - a process that began about 30 million yea

PIX4612910

Infrared view of the Andromeda galaxy - Infrared view of the Andromeda galaxy - This image shows the difference in infrared radiation between the light emitted by the aged stars (blue) and that emitted by the dust (star-forming zone, red). By measuring the infrared radiation emitted by a galaxy, more or less important depending on the nature of the stars, the mass of that galaxy can be reduced. According to this method, the mass of stars in the Andromede galaxy would be 110 billion times that of the Sun, which means that this galaxy would have 1 trillion stars (our galaxy had 400 billion). In this image we distinguish the two satellite galaxies of Andromede, M32 at the bottom and NGC 205 (M110) at the top. Infrared composite at the following wavelengths: 3.6 and 4.5 microns: sensitive to star light (blue and green), and 8 micron sensitive to dust in red. 3000 different poses obtained by the Spitzer space telescope in January and August 2005 were required to achieve this complete view o

Infrared view of the Andromeda galaxy - Infrared view of the Andromeda galaxy - This image shows the difference in infrared radiation between the light emitted by the aged stars (blue) and that emitted by the dust (star-forming zone, red). By measuring the infrared radiation emitted by a galaxy, more or less important depending on the nature of the stars, the mass of that galaxy can be reduced. According to this method, the mass of stars in the Andromede galaxy would be 110 billion times that of the Sun, which means that this galaxy would have 1 trillion stars (our galaxy had 400 billion). In this image we distinguish the two satellite galaxies of Andromede, M32 at the bottom and NGC 205 (M110) at the top. Infrared composite at the following wavelengths: 3.6 and 4.5 microns: sensitive to star light (blue and green), and 8 micron sensitive to dust in red. 3000 different poses obtained by the Spitzer space telescope in January and August 2005 were required to achieve this complete view o

PIX4608960

Total solar eclipse -Turkey 29 March 2006 - Total solar eclipse -Turkey -March 29, 2006 - Total solar eclipse observed in Turkey on 29 March 2006. Composite image showing the different phases of the eclipse

Total solar eclipse -Turkey 29 March 2006 - Total solar eclipse -Turkey -March 29, 2006 - Total solar eclipse observed in Turkey on 29 March 2006. Composite image showing the different phases of the eclipse

Alex Conu

PIX4583370

Earth and Sun - artist view - Earth and Sun - Artwork

Earth and Sun - artist view - Earth and Sun - Artwork

PIX4669693

Total Eclipse de Soleil. 01/08/2008 - Total Solar Eclipse of 2008 august 01 - All phases of the total eclipse of Sun from August 1st 2008. One image every 5 minutes before and after Total Solar Eclipse of 2008 august 01 seen in Mongolia. The different phases are shown in this composite of images taken every 5 minutes

Total Eclipse de Soleil. 01/08/2008 - Total Solar Eclipse of 2008 august 01 - All phases of the total eclipse of Sun from August 1st 2008. One image every 5 minutes before and after Total Solar Eclipse of 2008 august 01 seen in Mongolia. The different phases are shown in this composite of images taken every 5 minutes

G. Cannat

PIX4628172

Midnight Sun on Mars seen by Phoenix - Midnight Sun on Mars seen by Phoenix - Panorama obtained by Phoenix probe showing the sun's race in the sky of Mars. The foreground image was taken on the 54th day of the mission (Ground 54, July 20, 2008). The different images of the Sun were taken between 10 pm and 2 am (local time) during soils 46 to 56 (12 to 22 July 2008 on Earth). The Phoenix probe landed on May 25, 2008 in the Vastitas Borealis region in the polar circle of Mars. This panorama mosaic of images was taken by the Surface Stereo Imager on board Nasa's Phoenix Mars Lander. This mosaic documents the midnight sun during several days of the mission. The foreground and sky images were taken on Sol 54, or the 54th Martian day of the mission (July 20, 2008). The solar images were taken between 10 p.m. and 2 a.m., local solar time, during the nights of sols 46 to 56. During this period of 11 sols, the sun's path got slightly lower over the northern horizon, causing the lack of smoothne

Midnight Sun on Mars seen by Phoenix - Midnight Sun on Mars seen by Phoenix - Panorama obtained by Phoenix probe showing the sun's race in the sky of Mars. The foreground image was taken on the 54th day of the mission (Ground 54, July 20, 2008). The different images of the Sun were taken between 10 pm and 2 am (local time) during soils 46 to 56 (12 to 22 July 2008 on Earth). The Phoenix probe landed on May 25, 2008 in the Vastitas Borealis region in the polar circle of Mars. This panorama mosaic of images was taken by the Surface Stereo Imager on board Nasa's Phoenix Mars Lander. This mosaic documents the midnight sun during several days of the mission. The foreground and sky images were taken on Sol 54, or the 54th Martian day of the mission (July 20, 2008). The solar images were taken between 10 p.m. and 2 a.m., local solar time, during the nights of sols 46 to 56. During this period of 11 sols, the sun's path got slightly lower over the northern horizon, causing the lack of smoothne

PIX4616625

Moonrise - September 2016 - Distorted Moonrise - Moonrise on the sea. Lofoten, Norway, 16 September 2016. The full moon rises in a photo sequence from Lofoten Islands. The mountains in the image are part of the Norwegian mainland, some 100 km from Lofoten. September 16, 2016

Moonrise - September 2016 - Distorted Moonrise - Moonrise on the sea. Lofoten, Norway, 16 September 2016. The full moon rises in a photo sequence from Lofoten Islands. The mountains in the image are part of the Norwegian mainland, some 100 km from Lofoten. September 16, 2016

Alex Conu

PIX4578399

Andromede Galaxy (M31) infrared view - The Andromeda galaxy seen in infrared - This image shows the difference in infrared radiation between the light emitted by the aged stars (blue) and that emitted by the dust (star-forming zone, yellow and red). This image obtained by the WISE satellite also distinguishes the two Andromede satellite galaxies, M32 (above the nucleus of the Andromede galaxy) and NGC 205 (M110) below. Infrared composite at the following wavelengths: 3.4 and 4.6 microns (blue), 12 microns (green), and 22 microns dust sensitive, red. M31, is captured in full in this new image from Nasa's Wide - field Infrared Survey Explorer, or WISE. The mosaic covers an area equivalent to more than 100 full moons, or five degrees across the sky. WISE used all four of its infrared detectors to capture this picture (3.4 - and 4.6 - micron light is colored blue; 12 - micron light is green; and 22 - micron light is red). Blue highlights mature stars, while yellow and red show dust heated

Andromede Galaxy (M31) infrared view - The Andromeda galaxy seen in infrared - This image shows the difference in infrared radiation between the light emitted by the aged stars (blue) and that emitted by the dust (star-forming zone, yellow and red). This image obtained by the WISE satellite also distinguishes the two Andromede satellite galaxies, M32 (above the nucleus of the Andromede galaxy) and NGC 205 (M110) below. Infrared composite at the following wavelengths: 3.4 and 4.6 microns (blue), 12 microns (green), and 22 microns dust sensitive, red. M31, is captured in full in this new image from Nasa's Wide - field Infrared Survey Explorer, or WISE. The mosaic covers an area equivalent to more than 100 full moons, or five degrees across the sky. WISE used all four of its infrared detectors to capture this picture (3.4 - and 4.6 - micron light is colored blue; 12 - micron light is green; and 22 - micron light is red). Blue highlights mature stars, while yellow and red show dust heated

PIX4608987

Composite image of the colliding galaxies VV 340 North and VV 340 South (photo)

Composite image of the colliding galaxies VV 340 North and VV 340 South (photo)

SMT1217262

Galactic Center Region - Center of our galaxy (photo)

Galactic Center Region - Center of our galaxy (photo)

PIX4637973

Corymb, composite diagram

Corymb, composite diagram

DGA1259365

Total Eclipse of Sun 22/07/2009 - Total Solar Eclipse - July 22 2009 - Total Eclipse of Sun of 22 July 2009 seen in the Pacific Ocean (Enewetak Atoll, Marshall Islands). Composite of 38 images showing the solar crown, ash light (the Moon lit by the Earth) and some stars (the weakest visible here are magnitude 10). Total Solar Eclipse of July 22 2009 seen in the Pacific ocean (Enewetak Atoll, Marshall Islands). Composition of 38 images showing the solar corona, lunar surface and stars, highly beyond the ability of human vision during the eclipse. The weakest stars visible in the image are of about magnitude 10. The stars are a little bit blurred by the motion of the Sun during the very long eclipse

Total Eclipse of Sun 22/07/2009 - Total Solar Eclipse - July 22 2009 - Total Eclipse of Sun of 22 July 2009 seen in the Pacific Ocean (Enewetak Atoll, Marshall Islands). Composite of 38 images showing the solar crown, ash light (the Moon lit by the Earth) and some stars (the weakest visible here are magnitude 10). Total Solar Eclipse of July 22 2009 seen in the Pacific ocean (Enewetak Atoll, Marshall Islands). Composition of 38 images showing the solar corona, lunar surface and stars, highly beyond the ability of human vision during the eclipse. The weakest stars visible in the image are of about magnitude 10. The stars are a little bit blurred by the motion of the Sun during the very long eclipse

PIX4628221

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

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

Ring of black matter in the cluster of galaxies Cl 0024+17 - Dark matter ring in distant galaxy cluster - The cluster of galaxies Cl 0024+17 is located about 5 billion years - light in the constellation Pisces. By studying visible gravitational mirages, astronomers were able to demonstrate a ring of black matter around this cluster. On this image, the ring of black material (in blue) was digitally superimposed on the image obtained by the Hubble space telescope in November 2004 with the ACS camera. Discovery of a ring of dark matter in the cluster ZWCL0024+1652. The ring's discovery is among the strongest evidence yet that dark matter exists.The ring, which measures 2.6 million light - years across, was found in the cluster ZWCL0024+1652, located 5 billion light - years away from Earth. The astronomers team found the ring unexpectedly while they were mapping the distribution of dark matter within the cluster. Although astronomers cannot see dark matter, they can infer its existence in

Ring of black matter in the cluster of galaxies Cl 0024+17 - Dark matter ring in distant galaxy cluster - The cluster of galaxies Cl 0024+17 is located about 5 billion years - light in the constellation Pisces. By studying visible gravitational mirages, astronomers were able to demonstrate a ring of black matter around this cluster. On this image, the ring of black material (in blue) was digitally superimposed on the image obtained by the Hubble space telescope in November 2004 with the ACS camera. Discovery of a ring of dark matter in the cluster ZWCL0024+1652. The ring's discovery is among the strongest evidence yet that dark matter exists.The ring, which measures 2.6 million light - years across, was found in the cluster ZWCL0024+1652, located 5 billion light - years away from Earth. The astronomers team found the ring unexpectedly while they were mapping the distribution of dark matter within the cluster. Although astronomers cannot see dark matter, they can infer its existence in

PIX4565677

Galaxy Centaurus A (NGC 5128) x-ray view - radio - visible - Galaxy Centaurus A in different wavelengths - false-coloured view of the 30,000-year long jet - light escaping from the nucleus of the Centaurus A galaxy where a massive black hole is suspected. On this composite image obtained in X, radio, and visible, two large X-emission arcs surround this jet over a diameter of 25,000 years - light. These hot arcs could be the result of a gigantic explosion that occurred 10 million years ago in the nucleus of the galaxy. The galaxy NGC 5128 is located about 13 million light years away from Earth. A composite X - ray (blue), radio (pink and green), and optical (orange and yellow) image of the galaxy Centaurus A presents a stunning view of a galaxy in turmoil. A broad band of dust and cold gas is bisected at an angle by opposing jets of high - energy particles blasting away from the supermassive black hole in the nucleus. Two large arcs of X - ray emitting hot gas were discovered in the out

Galaxy Centaurus A (NGC 5128) x-ray view - radio - visible - Galaxy Centaurus A in different wavelengths - false-coloured view of the 30,000-year long jet - light escaping from the nucleus of the Centaurus A galaxy where a massive black hole is suspected. On this composite image obtained in X, radio, and visible, two large X-emission arcs surround this jet over a diameter of 25,000 years - light. These hot arcs could be the result of a gigantic explosion that occurred 10 million years ago in the nucleus of the galaxy. The galaxy NGC 5128 is located about 13 million light years away from Earth. A composite X - ray (blue), radio (pink and green), and optical (orange and yellow) image of the galaxy Centaurus A presents a stunning view of a galaxy in turmoil. A broad band of dust and cold gas is bisected at an angle by opposing jets of high - energy particles blasting away from the supermassive black hole in the nucleus. Two large arcs of X - ray emitting hot gas were discovered in the out

PIX4612202

The Moon and Stars Above the Earth - Moon and starry sky over Earth - Artwork - The Moon and Stars Above the Earth's Atmosphere

The Moon and Stars Above the Earth - Moon and starry sky over Earth - Artwork - The Moon and Stars Above the Earth's Atmosphere

PIX4675255

Galaxy M82 view in different wavelength - Galaxy M82 in multi - wavelength - Composite of different images: in blue the image obtained by Chandra in X-rays, in red the infrared image obtained by Spitzer, in yellow, orange, green, the image of Hubble. M82 is an irregular galaxy distant about 12 million years - light from Earth. Its nucleus, which appears to have suffered from the passage of the neighbouring galaxy M81, is in a phase of violent star activity. Its central regions are rich in star formation. These hot stars blow a stellar wind that becomes a very violent galactic wind. Composite of multi - wavelength images of the active galaxy M82 from the three Great Observatories. X - ray data recorded by Chandra appears here in blue; infrared light recorded by Spitzer appears in red; Hubble's observations of hydrogen emission appears in orange, and the bluest visible light appears in yellow - green. Another Hubble observation designed to image 10,000 degree Celsius hydrogen gas (orange

Galaxy M82 view in different wavelength - Galaxy M82 in multi - wavelength - Composite of different images: in blue the image obtained by Chandra in X-rays, in red the infrared image obtained by Spitzer, in yellow, orange, green, the image of Hubble. M82 is an irregular galaxy distant about 12 million years - light from Earth. Its nucleus, which appears to have suffered from the passage of the neighbouring galaxy M81, is in a phase of violent star activity. Its central regions are rich in star formation. These hot stars blow a stellar wind that becomes a very violent galactic wind. Composite of multi - wavelength images of the active galaxy M82 from the three Great Observatories. X - ray data recorded by Chandra appears here in blue; infrared light recorded by Spitzer appears in red; Hubble's observations of hydrogen emission appears in orange, and the bluest visible light appears in yellow - green. Another Hubble observation designed to image 10,000 degree Celsius hydrogen gas (orange

PIX4610442

Total solar eclipse -Turkey 29 March 2006 - Total solar eclipse -Turkey -March 29, 2006 - Total solar eclipse observed in Turkey on 29 March 2006. Composite image to show details in the crown and on the moon

Total solar eclipse -Turkey 29 March 2006 - Total solar eclipse -Turkey -March 29, 2006 - Total solar eclipse observed in Turkey on 29 March 2006. Composite image to show details in the crown and on the moon

Alex Conu

PIX4583396

M87 elliptical galaxy in Virgo - M87 elliptical galaxy in Virgo - The M87 galaxy (NGC 4486) is 54 million years ago - light from Earth, in the heart of the Virgin's cluster. This image is a composite obtained in X-rays, radio and visible. Gas material is ejected from the heart of the galaxy. A supermassive black hole would have caused this jet. This image is a composite of visible (or optical), radio, and X - ray data of the giant elliptical galaxy, M87. M87 lies at a distance of 54 million light years and is the largest galaxy in the Virgo cluster of galaxies. Bright jets moving at close to the speed of light are seen at all wavelengths coming from the massive black hole at the center of the galaxy. It has also been identified with the strong radio source, Virgo A, and is a powerful source of X - rays as it resides near the center of a hot, X - ray emitting cloud that extends over much of the Virgo cluster. The extended radio emission consists of plumes of fast - moving gas from the j

M87 elliptical galaxy in Virgo - M87 elliptical galaxy in Virgo - The M87 galaxy (NGC 4486) is 54 million years ago - light from Earth, in the heart of the Virgin's cluster. This image is a composite obtained in X-rays, radio and visible. Gas material is ejected from the heart of the galaxy. A supermassive black hole would have caused this jet. This image is a composite of visible (or optical), radio, and X - ray data of the giant elliptical galaxy, M87. M87 lies at a distance of 54 million light years and is the largest galaxy in the Virgo cluster of galaxies. Bright jets moving at close to the speed of light are seen at all wavelengths coming from the massive black hole at the center of the galaxy. It has also been identified with the strong radio source, Virgo A, and is a powerful source of X - rays as it resides near the center of a hot, X - ray emitting cloud that extends over much of the Virgo cluster. The extended radio emission consists of plumes of fast - moving gas from the j

PIX4611440

Nebulae NGC 2024 and Horse's Head - Flame nebula and the Horsehead Nebula - This image shows the nebula NGC 2024 (left), the small nebula NGC 2023 (right middle) and the nebula of the horse's head (top right). The bright star on the top left is the star Alnitak. Visible infrared composite image. This image shows the spectacular star - forming region known as the Flame Nebula, or NGC 2024, in the constellation of Orion (the Hunter) and its surroundings. The view also includes the glow of the reflection nebula NGC 2023, middle right, and the ghostly outline of the Horsehead Nebula (Barnard 33) towards the upper right. The bright bluish star top left is one of the three bright stars forming the Belt of Orion, Alnitak. The image was created from VISTA in the near - infrared part of the spectrum and optical datas

Nebulae NGC 2024 and Horse's Head - Flame nebula and the Horsehead Nebula - This image shows the nebula NGC 2024 (left), the small nebula NGC 2023 (right middle) and the nebula of the horse's head (top right). The bright star on the top left is the star Alnitak. Visible infrared composite image. This image shows the spectacular star - forming region known as the Flame Nebula, or NGC 2024, in the constellation of Orion (the Hunter) and its surroundings. The view also includes the glow of the reflection nebula NGC 2023, middle right, and the ghostly outline of the Horsehead Nebula (Barnard 33) towards the upper right. The bright bluish star top left is one of the three bright stars forming the Belt of Orion, Alnitak. The image was created from VISTA in the near - infrared part of the spectrum and optical datas

PIX4622107

Galaxies Group: Stephan's Quintet in Pegase - Stephan's Quintet group of galaxies - This group of 5 galaxies is located about 260 million years ago - light from Earth. These galaxies interact, however NGC 7320 (upper left) would be 7 times closer to us. Composite image obtained in visible light and infrared by the Hubble space telescope in August 2009. This portrait of Stephan's Quintet, also known as the Hickson Compact Group 92, was taken by the new Wide Field Camera 3 (WFC3) aboard the NASA/ESA Hubble Space Telescope. Stephan's Quintet, as the name implies, is a group of five galaxies. The name, however, is a bit of a misnomer. Studies have shown that group member NGC 7320, at upper left, is actually a foreground galaxy that is about seven times closer to Earth than the rest of the group. Three of the galaxies have distorted shapes, elongated spiral arms, and long, gaseous tidal tails containing myriad star clusters, proof of their close encounters. These interactions have sparked a

Galaxies Group: Stephan's Quintet in Pegase - Stephan's Quintet group of galaxies - This group of 5 galaxies is located about 260 million years ago - light from Earth. These galaxies interact, however NGC 7320 (upper left) would be 7 times closer to us. Composite image obtained in visible light and infrared by the Hubble space telescope in August 2009. This portrait of Stephan's Quintet, also known as the Hickson Compact Group 92, was taken by the new Wide Field Camera 3 (WFC3) aboard the NASA/ESA Hubble Space Telescope. Stephan's Quintet, as the name implies, is a group of five galaxies. The name, however, is a bit of a misnomer. Studies have shown that group member NGC 7320, at upper left, is actually a foreground galaxy that is about seven times closer to Earth than the rest of the group. Three of the galaxies have distorted shapes, elongated spiral arms, and long, gaseous tidal tails containing myriad star clusters, proof of their close encounters. These interactions have sparked a

PIX4565504

Hannah Maynard and her grandson Maynard McDonald in several poses in a composite photo, c.1895 (b/w photo)

Hannah Maynard and her grandson Maynard McDonald in several poses in a composite photo, c.1895 (b/w photo)

Maynard, Hannah (1834-1918)

RBC2637608

Cyclones encircle Jupiter's North Pole (photo)

Cyclones encircle Jupiter's North Pole (photo)

XOS3742366

Total Eclipse of Sun. 01/08/2008 - Total Solar Eclipse of 2008 august 01 - Composite of 23 images showing the solar crown, the ash light (the Moon lit by the Earth) and the stars. Solar corona, Earth - lit Moon and stars It is a composition of 23 images showing the solar corona in very high resolution and also the Earth - lit Moon and stars up to 11 magnitude. The brightest star (4 magn.) is slightly blurred by the motion of the Sun during the eclipse. The position of the Moon represents the situation 54 seconds after the second contact (18:04:29 local time in Mongolia). Both the display of the solar corona and the lunar surface in the resulting image are beyond the ability of human vision during the eclipse

Total Eclipse of Sun. 01/08/2008 - Total Solar Eclipse of 2008 august 01 - Composite of 23 images showing the solar crown, the ash light (the Moon lit by the Earth) and the stars. Solar corona, Earth - lit Moon and stars It is a composition of 23 images showing the solar corona in very high resolution and also the Earth - lit Moon and stars up to 11 magnitude. The brightest star (4 magn.) is slightly blurred by the motion of the Sun during the eclipse. The position of the Moon represents the situation 54 seconds after the second contact (18:04:29 local time in Mongolia). Both the display of the solar corona and the lunar surface in the resulting image are beyond the ability of human vision during the eclipse

PIX4628057

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

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

Designs for a System of Composite Shipbuilding Recommended by Lloyd's UK 1867

Designs for a System of Composite Shipbuilding Recommended by Lloyd's UK 1867

LZT1014876

Composite image of the 1903 Wright Flyer and Lockheed SR-71A Blackbird through the Apollo Lunar Module No. 2 window (photo)

Composite image of the 1903 Wright Flyer and Lockheed SR-71A Blackbird through the Apollo Lunar Module No. 2 window (photo)

SMT1217081

Active Galaxy NGC 1068 in the Whale - Active galaxy NGC 1068 - This composite image shows that a strong stellar wind escapes from the heart of the galaxy NGC 1068 or resides a massive black hole. NGC 1068 is located about 50 million light years away from Earth. Images obtained in X-ray by the Chandra satellite (red), visible by the Hubble space telescope (green) and radio waves (blue). This is a composite image of NGC 1068, one of the nearest and brightest galaxies containing a rapidly growing supermassive black hole. X - ray data from the Chandra X - ray Observatory are shown in red, optical data from the Hubble Space Telescope in green and radio data from the Very Large Array in blue. The spiral structure of NGC 1068 is shown by the X - ray and optical data, and a jet powered by the central supermassive black hole is shown by the radio data. The X - ray images and spectra obtained using Chandra's High Energy Transmission Grating Spectrometer show that a strong wind is being driven aw

Active Galaxy NGC 1068 in the Whale - Active galaxy NGC 1068 - This composite image shows that a strong stellar wind escapes from the heart of the galaxy NGC 1068 or resides a massive black hole. NGC 1068 is located about 50 million light years away from Earth. Images obtained in X-ray by the Chandra satellite (red), visible by the Hubble space telescope (green) and radio waves (blue). This is a composite image of NGC 1068, one of the nearest and brightest galaxies containing a rapidly growing supermassive black hole. X - ray data from the Chandra X - ray Observatory are shown in red, optical data from the Hubble Space Telescope in green and radio data from the Very Large Array in blue. The spiral structure of NGC 1068 is shown by the X - ray and optical data, and a jet powered by the central supermassive black hole is shown by the radio data. The X - ray images and spectra obtained using Chandra's High Energy Transmission Grating Spectrometer show that a strong wind is being driven aw

PIX4609662

Marrakech, Morocco, True Colour Satellite Image

Marrakech, Morocco, True Colour Satellite Image

UIG521324

Total Eclipse of Sun. 01/08/2008 - Total Solar Eclipse of 2008 august 01 - Composite of images showing the solar crown, the ash light (the Moon lit by the Earth) the stars around the Sun (with the cluster of stars M44 at the top right) and the planet Mercury (bright dot on the left). 01/08/2008, Mongolia. Data from two different cameras were used for this image creation. The open cluster M 44 Praesepae (NGC 2632) dominates the star field. The bright object in the left part of the image is Mercury. The solar corona is traceable up to the distance of 20 solar radii. The position of the Moon represents the situation 62 seconds after the second contact (18:04:37 mongolia local time). Display of the solar corona, lunar surface and stars in the resulting image are highly beyond the ability of human vision during the eclipse

Total Eclipse of Sun. 01/08/2008 - Total Solar Eclipse of 2008 august 01 - Composite of images showing the solar crown, the ash light (the Moon lit by the Earth) the stars around the Sun (with the cluster of stars M44 at the top right) and the planet Mercury (bright dot on the left). 01/08/2008, Mongolia. Data from two different cameras were used for this image creation. The open cluster M 44 Praesepae (NGC 2632) dominates the star field. The bright object in the left part of the image is Mercury. The solar corona is traceable up to the distance of 20 solar radii. The position of the Moon represents the situation 62 seconds after the second contact (18:04:37 mongolia local time). Display of the solar corona, lunar surface and stars in the resulting image are highly beyond the ability of human vision during the eclipse

PIX4628063

Galactic Center Region - The Galactic Center - The Galactic Center Region of the center of our galaxy seen the Chandra, Spitzer and Hubble satellites. The galactic center (Sagittarius A*) is located in the white area in the middle to the right of the image. In yellow, near-infrared images obtained by the Hubble Space Telescope; in red, infrared images obtained by the Spitzer Space Telescope; in blue and purple, X-ray observations obtained by the Chandra Space Telescope. Nasa's Great Observatories - the Hubble Space Telescope, the Spitzer Space Telescope, and the Chandra X-ray Observatory - have collaborated to produce an unprecedented image of the central region of our Milky Way galaxy. In this spectacular image, observations using infrared light and X-ray light see through the obscuring dust and reveal the intense activity near the galactic core. Note that the center of the galaxy is located within the bright white region to the right of and just below the middle of the image. The ent

Galactic Center Region - The Galactic Center - The Galactic Center Region of the center of our galaxy seen the Chandra, Spitzer and Hubble satellites. The galactic center (Sagittarius A*) is located in the white area in the middle to the right of the image. In yellow, near-infrared images obtained by the Hubble Space Telescope; in red, infrared images obtained by the Spitzer Space Telescope; in blue and purple, X-ray observations obtained by the Chandra Space Telescope. Nasa's Great Observatories - the Hubble Space Telescope, the Spitzer Space Telescope, and the Chandra X-ray Observatory - have collaborated to produce an unprecedented image of the central region of our Milky Way galaxy. In this spectacular image, observations using infrared light and X-ray light see through the obscuring dust and reveal the intense activity near the galactic core. Note that the center of the galaxy is located within the bright white region to the right of and just below the middle of the image. The ent

PIX4637984

Houston, Texas, Usa, True Colour Satellite Image

Houston, Texas, Usa, True Colour Satellite Image

UIG601783

Bosumtwi Meteor Impact Crater, Ghana, True Colour Satellite Image

Bosumtwi Meteor Impact Crater, Ghana, True Colour Satellite Image

UIG602012

Globe Europe, True Colour Satellite Image

Globe Europe, True Colour Satellite Image

UIG601600

Vredefort Meteor Impact Crater, South Africa, True Colour Satellite Image

Vredefort Meteor Impact Crater, South Africa, True Colour Satellite Image

UIG520484

Volcano Tousside In 3D, Chad, True Colour Satellite Image

Volcano Tousside In 3D, Chad, True Colour Satellite Image

UIG601956

The spiral galaxy Messier 101, from composite of views from Spitzer, Hubble, and Chandra.

The spiral galaxy Messier 101, from composite of views from Spitzer, Hubble, and Chandra.

UIG867124

Vietnam: A composite satellite image of Vietnam, together with all of Cambodia, eastern and southern Laos, Northeast Thailand and part of southern China

Vietnam: A composite satellite image of Vietnam, together with all of Cambodia, eastern and southern Laos, Northeast Thailand and part of southern China

PFH1174069

Surtsey Volcano, Iceland, True Colour Satellite Image

Surtsey Volcano, Iceland, True Colour Satellite Image

UIG601969

Tousside Volcano, Chad, True Colour Satellite Image

Tousside Volcano, Chad, True Colour Satellite Image

UIG601986

Lake Malawi, Africa, True Colour Satellite Image

Lake Malawi, Africa, True Colour Satellite Image

UIG521234

Lake Onega, Russia, True Colour Satellite Image

Lake Onega, Russia, True Colour Satellite Image

UIG521247

Yasur Volcano, Vanuatu, Pacific, True Colour Satellite Image

Yasur Volcano, Vanuatu, Pacific, True Colour Satellite Image

UIG601996

Lake Winnipeg, Canada, True Colour Satellite Image

Lake Winnipeg, Canada, True Colour Satellite Image

UIG521241

Libyan Desert, Egypt, True Colour Satellite Image

Libyan Desert, Egypt, True Colour Satellite Image

UIG601882

Lake Victoria, Africa, True Colour Satellite Image

Lake Victoria, Africa, True Colour Satellite Image

UIG521250

Titanic striking the iceberg, illustration from the front cover of 'The Sphere' newspaper, 20th April, 1912 (litho) (see also 450770)

Titanic striking the iceberg, illustration from the front cover of 'The Sphere' newspaper, 20th April, 1912 (litho) (see also 450770)

English School, (20th century)

UIG450771

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