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Arabian desert seen by satellite 01/2016 - Eastern Desert - Egypt: Part of the Arabian desert in Egypt seen by Sentinel-2A satellite on 17 January 2016. The vegetation appears in red near the Nile. The Sentinel-2A satellite takes us over central-eastern Egypt with this image from 17 January. The image is dominated by arid desert - namely the Eastern Desert between the Nile River the Red Sea. The distinctive pattern of water erosion from rivers and streams is clearly visible as they make their way towards the Nile, at which point the rolling sandy highlands drop abruptly at the Nile valley, visible along the bottom of the image. Fields of intensive farming along the Nile appear red owing to this false-colour image being processed to include the near-infrared. The varying shades of red indicate how sensitive the multispectral instrument on Sentinel-2 is to differences in chlorophyll content, providing key information on plant health. Zooming in along the bottom we can see clusters of bla

Arabian desert seen by satellite 01/2016 - Eastern Desert - Egypt: Part of the Arabian desert in Egypt seen by Sentinel-2A satellite on 17 January 2016. The vegetation appears in red near the Nile. The Sentinel-2A satellite takes us over central-eastern Egypt with this image from 17 January. The image is dominated by arid desert - namely the Eastern Desert between the Nile River the Red Sea. The distinctive pattern of water erosion from rivers and streams is clearly visible as they make their way towards the Nile, at which point the rolling sandy highlands drop abruptly at the Nile valley, visible along the bottom of the image. Fields of intensive farming along the Nile appear red owing to this false-colour image being processed to include the near-infrared. The varying shades of red indicate how sensitive the multispectral instrument on Sentinel-2 is to differences in chlorophyll content, providing key information on plant health. Zooming in along the bottom we can see clusters of bla

PIX4630475

The scattered remains of an exploded star named Cassiopeia A. Much of the star's original layering had been preserved. NASA's Spitzer Space Telescope.

The scattered remains of an exploded star named Cassiopeia A. Much of the star's original layering had been preserved. NASA's Spitzer Space Telescope.

UIG867013

The scattered remains of an exploded star named Cassiopeia A. Much of the star's original layering had been preserved. NASA's Spitzer Space Telescope.

The scattered remains of an exploded star named Cassiopeia A. Much of the star's original layering had been preserved. NASA's Spitzer Space Telescope.

UIG867011

This infrared image showed a "snake" (upper left) and its surrounding stormy environment. The object is actually the core of a thick, sooty cloud large enough to swallow dozens of solar systems. NASA's Spitzer Space Telescope.

This infrared image showed a "snake" (upper left) and its surrounding stormy environment. The object is actually the core of a thick, sooty cloud large enough to swallow dozens of solar systems. NASA's Spitzer Space Telescope.

UIG867007

This infrared image showed a "snake" (upper left) and its surrounding stormy environment. The object is actually the core of a thick, sooty cloud large enough to swallow dozens of solar systems. NASA's Spitzer Space Telescope.

This infrared image showed a "snake" (upper left) and its surrounding stormy environment. The object is actually the core of a thick, sooty cloud large enough to swallow dozens of solar systems. NASA's Spitzer Space Telescope.

UIG867006

This infrared image showed a "snake" (upper left) and its surrounding stormy environment. The object is actually the core of a thick, sooty cloud large enough to swallow dozens of solar systems. NASA's Spitzer Space Telescope.

This infrared image showed a "snake" (upper left) and its surrounding stormy environment. The object is actually the core of a thick, sooty cloud large enough to swallow dozens of solar systems. NASA's Spitzer Space Telescope.

UIG867008

Galaxy cluster Abell 1656 - Coma cluster - The Coma cluster (Abell 1656) - A large cluster of galaxies consists of about a thousand galaxies located 330 million years - light in the constellation Coma Berenices (Berenice hair). This cluster is dominated by two large elliptical galaxies NGC 4874 on the right and NGC 4889 on the left. Image obtained near infrared by a 1.3m (2Mass) telescope. The Coma cluster (Abell 1656) is a particularly rich cluster of individual galaxies (over 1000 members), most prominently the two giant ellipticals, NGC 4874 (right) and NGC 4889 (left). The remaining members are mostly smaller ellipticals, but spiral galaxies are also evident in this 2MASS image. The cluster is seen towards the constellation Coma Berenices, and is actually at a distance of about 100 Mpc (330 million light years, or a redshift of 0.023) from us. Near infrared image

Galaxy cluster Abell 1656 - Coma cluster - The Coma cluster (Abell 1656) - A large cluster of galaxies consists of about a thousand galaxies located 330 million years - light in the constellation Coma Berenices (Berenice hair). This cluster is dominated by two large elliptical galaxies NGC 4874 on the right and NGC 4889 on the left. Image obtained near infrared by a 1.3m (2Mass) telescope. The Coma cluster (Abell 1656) is a particularly rich cluster of individual galaxies (over 1000 members), most prominently the two giant ellipticals, NGC 4874 (right) and NGC 4889 (left). The remaining members are mostly smaller ellipticals, but spiral galaxies are also evident in this 2MASS image. The cluster is seen towards the constellation Coma Berenices, and is actually at a distance of about 100 Mpc (330 million light years, or a redshift of 0.023) from us. Near infrared image

PIX4565251

A star's spectacular death in the constellation Taurus was observed on Earth as the supernova of 1054 A.D. NASA's Spitzer Space Telescope.

A star's spectacular death in the constellation Taurus was observed on Earth as the supernova of 1054 A.D. NASA's Spitzer Space Telescope.

UIG867010

A star's spectacular death in the constellation Taurus was observed on Earth as the supernova of 1054 A.D. NASA's Spitzer Space Telescope.

A star's spectacular death in the constellation Taurus was observed on Earth as the supernova of 1054 A.D. NASA's Spitzer Space Telescope.

UIG867009

Located 1,000 light years from Earth in the constellation Perseus, a reflection nebula called NGC 1333 epitomizes the beautiful chaos of a dense group of stars being born. Spitzer Space Telescope.

Located 1,000 light years from Earth in the constellation Perseus, a reflection nebula called NGC 1333 epitomizes the beautiful chaos of a dense group of stars being born. Spitzer Space Telescope.

UIG867031

The many sides of the supernova remnant Cassiopeia A. Located 10,000 light-years away in the northern constellation Cassiopeia, Cassiopeia A is the remnant of a once massive star that died in a violent supernova explosion 325 years ago. Hubble Space Telescope (HST), Spitzer Space Telescope.

The many sides of the supernova remnant Cassiopeia A. Located 10,000 light-years away in the northern constellation Cassiopeia, Cassiopeia A is the remnant of a once massive star that died in a violent supernova explosion 325 years ago. Hubble Space Telescope (HST), Spitzer Space Telescope.

UIG867028

The Visible Infrared Imaging view of the Americas in daytime, 2000

The Visible Infrared Imaging view of the Americas in daytime, 2000

UIG3508118

Located 1,000 light years from Earth in the constellation Perseus, a reflection nebula called NGC 1333 epitomizes the beautiful chaos of a dense group of stars being born. Spitzer Space Telescope.

Located 1,000 light years from Earth in the constellation Perseus, a reflection nebula called NGC 1333 epitomizes the beautiful chaos of a dense group of stars being born. Spitzer Space Telescope.

UIG867030

This image shows the Large Magellanic Cloud galaxy in infrared light as seen by the Herschel Space Observatory.

This image shows the Large Magellanic Cloud galaxy in infrared light as seen by the Herschel Space Observatory.

UIG867354

The Visible Infrared Imaging view of the Americas at night, 2000

The Visible Infrared Imaging view of the Americas at night, 2000

UIG3508117

This image, PIA06908, and PIA06910 represent views of Kepler's supernova remnant taken in X-rays, visible light, and infrared radiation

This image, PIA06908, and PIA06910 represent views of Kepler's supernova remnant taken in X-rays, visible light, and infrared radiation

UIG3524422

Titan, Saturn satellite seen by Cassini - Saturn's moon Titan as seen by Cassini spacecraft: Titan images obtained by the Cassini probe on 21 March 2017. On the left, Titan seen in real colors. On the right, infrared image showing surface details as well as clouds in the northern hemisphere. These views were obtained with the Cassini spacecraft narrow-angle camera on March 21, 2017. Images taken using red, green and blue spectral filters were combined to create the natural-color view at left. The false-color view at right was made by substituting an infrared image (centered at 938 nanometers) for the red color channel. A large, bright and feathery band of summer clouds can be seen arcing across high northern latitudes in the view at right. The views were acquired at a distance of approximately 613,000 miles (986,000 kilometers) from Titan. Image scale is about 4 miles (6 kilometers) per pixel

Titan, Saturn satellite seen by Cassini - Saturn's moon Titan as seen by Cassini spacecraft: Titan images obtained by the Cassini probe on 21 March 2017. On the left, Titan seen in real colors. On the right, infrared image showing surface details as well as clouds in the northern hemisphere. These views were obtained with the Cassini spacecraft narrow-angle camera on March 21, 2017. Images taken using red, green and blue spectral filters were combined to create the natural-color view at left. The false-color view at right was made by substituting an infrared image (centered at 938 nanometers) for the red color channel. A large, bright and feathery band of summer clouds can be seen arcing across high northern latitudes in the view at right. The views were acquired at a distance of approximately 613,000 miles (986,000 kilometers) from Titan. Image scale is about 4 miles (6 kilometers) per pixel

PIX4582276

Detroit of Gibraltar seen by satellite - Strait of Gibraltar seen from space - The Detroit of Gibraltar seen by the Terra satellite with the ASTER instrument on 5 July 2000. The visible and infrared image covers an area of 34 km by 59 km. To the north, Spain and the rock of Gibraltar at the end of the tip, to the south, Morocco. The Strait of Gibraltar separates Spain from Morocco. This image, acquired on July 5, 2000, covers an area 34 kilometers (21 miles) wide and 59 kilometers (37 miles) long in three bands of the reflected visible and infrared wavelength region. The promontory on the eastern side of the conspicuous Spanish port is the Rock of Gibraltar. Once one of the two classical Pillars of Hercules, the Rock was crowned with silver columns by Phoenician mariners to mark the limits of safe navigation for the ancient Mediterranean peoples. The rocky promontory still commands the western entrance to the Mediterranean Sea. The rocky limestone and shale ridge rises abruptly from th

Detroit of Gibraltar seen by satellite - Strait of Gibraltar seen from space - The Detroit of Gibraltar seen by the Terra satellite with the ASTER instrument on 5 July 2000. The visible and infrared image covers an area of 34 km by 59 km. To the north, Spain and the rock of Gibraltar at the end of the tip, to the south, Morocco. The Strait of Gibraltar separates Spain from Morocco. This image, acquired on July 5, 2000, covers an area 34 kilometers (21 miles) wide and 59 kilometers (37 miles) long in three bands of the reflected visible and infrared wavelength region. The promontory on the eastern side of the conspicuous Spanish port is the Rock of Gibraltar. Once one of the two classical Pillars of Hercules, the Rock was crowned with silver columns by Phoenician mariners to mark the limits of safe navigation for the ancient Mediterranean peoples. The rocky promontory still commands the western entrance to the Mediterranean Sea. The rocky limestone and shale ridge rises abruptly from th

PIX4665868

The many sides of the supernova remnant Cassiopeia A. Located 10,000 light-years away in the northern constellation Cassiopeia, Cassiopeia A is the remnant of a once massive star that died in a violent supernova explosion 325 years ago. Hubble Space Telescope (HST), Spitzer Space Telescope.

The many sides of the supernova remnant Cassiopeia A. Located 10,000 light-years away in the northern constellation Cassiopeia, Cassiopeia A is the remnant of a once massive star that died in a violent supernova explosion 325 years ago. Hubble Space Telescope (HST), Spitzer Space Telescope.

UIG867026

This image shows the Large Magellanic Cloud galaxy in infrared light as seen by the Herschel Space Observatory.

This image shows the Large Magellanic Cloud galaxy in infrared light as seen by the Herschel Space Observatory.

UIG867357

Saturn seen in infrared by Cassini spacecraft - Saturn seen in infrared by Cassini spacecraft - Composite image of Saturn in false colours obtained from infrared observations collected by the Cassini probe on 24 February 2007 at a distance of 1.58 million km from the planet. Flying over the unlit side of Saturn's rings, the Cassini spacecraft captures Saturn's glow, represented in brilliant shades of electric blue, sapphire and mint green, while the planet's shadow casts a wide net on the rings. This striking false - color mosaic was created from 25 images taken by Cassini's visual and infrared mapping spectrometer over a period of 13 hours, and captures Saturn in nighttime and daytime conditions. The visual and infrared mapping spectrometer acquires data simultaneously at 352 different wavelengths, or spectral channels. Data at wavelengths of 2.3, 3.0 and 5.1 microns were combined in the blue, green and red channels of a standard color image, respectively, to make this false - color m

Saturn seen in infrared by Cassini spacecraft - Saturn seen in infrared by Cassini spacecraft - Composite image of Saturn in false colours obtained from infrared observations collected by the Cassini probe on 24 February 2007 at a distance of 1.58 million km from the planet. Flying over the unlit side of Saturn's rings, the Cassini spacecraft captures Saturn's glow, represented in brilliant shades of electric blue, sapphire and mint green, while the planet's shadow casts a wide net on the rings. This striking false - color mosaic was created from 25 images taken by Cassini's visual and infrared mapping spectrometer over a period of 13 hours, and captures Saturn in nighttime and daytime conditions. The visual and infrared mapping spectrometer acquires data simultaneously at 352 different wavelengths, or spectral channels. Data at wavelengths of 2.3, 3.0 and 5.1 microns were combined in the blue, green and red channels of a standard color image, respectively, to make this false - color m

PIX4624969

Saturn in false colours - Saturn in infrared - The planet Saturn seen in visible and infrared by the Cassini probe on November 1, 2008. This false - color composite image, constructed from data obtained by Nasa's Cassini spacecraft, shows Saturn's rings and southern hemisphere. The composite image was made from 65 individual observations by Cassini's visual and infrared mapping spectrometer in the near - infrared portion of the light spectrum on Nov. 1, 2008. The observations were each six minutes long. In this image constructed from data collected in the near - infrared wavelengths of light, scientists designated blue to indicate sunlight reflected at a wavelength of 2 microns, green to indicate sunlight reflected at 3 microns and red to indicate thermal emission at 5 microns. Saturn's rings reflect sunlight at 2 microns, but not at 3 and 5 microns, so they appear deep blue. Saturn's high altitude haze reflects sunlight at both 2 and 3 microns, but not at 5 microns, and so it appears

Saturn in false colours - Saturn in infrared - The planet Saturn seen in visible and infrared by the Cassini probe on November 1, 2008. This false - color composite image, constructed from data obtained by Nasa's Cassini spacecraft, shows Saturn's rings and southern hemisphere. The composite image was made from 65 individual observations by Cassini's visual and infrared mapping spectrometer in the near - infrared portion of the light spectrum on Nov. 1, 2008. The observations were each six minutes long. In this image constructed from data collected in the near - infrared wavelengths of light, scientists designated blue to indicate sunlight reflected at a wavelength of 2 microns, green to indicate sunlight reflected at 3 microns and red to indicate thermal emission at 5 microns. Saturn's rings reflect sunlight at 2 microns, but not at 3 and 5 microns, so they appear deep blue. Saturn's high altitude haze reflects sunlight at both 2 and 3 microns, but not at 5 microns, and so it appears

PIX4625231

Arch Hall, County Meath, Ireland (b/w photo)

Arch Hall, County Meath, Ireland (b/w photo)

Simon Marsden

TMA3263066

Cadaver, St Peter's Churchyard, Drogheda, County Meath, Ireland (b/w photo)

Cadaver, St Peter's Churchyard, Drogheda, County Meath, Ireland (b/w photo)

Simon Marsden

TMA3262914

Andromede Galaxy (M31) infrared view by Herschel - Herschel Infrared view of the Andromeda galaxy - Andromede's spiral galaxy seen in infrared by the Herschel space telescope in December 2010. This is the most detailed image of the Andromeda Galaxy ever taken at far - infrared wavelengths. The Herschel infrared space telescope captured the image during Christmas 2010. The large rings of dust that encircle the centre of the galaxy may be the result of a smaller galaxy having collided with Andromeda some time in the past

Andromede Galaxy (M31) infrared view by Herschel - Herschel Infrared view of the Andromeda galaxy - Andromede's spiral galaxy seen in infrared by the Herschel space telescope in December 2010. This is the most detailed image of the Andromeda Galaxy ever taken at far - infrared wavelengths. The Herschel infrared space telescope captured the image during Christmas 2010. The large rings of dust that encircle the centre of the galaxy may be the result of a smaller galaxy having collided with Andromeda some time in the past

PIX4608974

Pistol star - Massive star in the constellation Sagittarius - The massive star Pistol star in Sagittarius - Pistol star is one of the most massive stars in our galaxy. Located about 25,000 years ago - the light of the Earth in the constellation of Sagittarius, this star shines like 10 million Sun consuming in six seconds as much energy as our star in a year. This star is masked by the numerous interstellar dust present in the Sagittarius near the galactic center and appears only in infrared wavelengths, as in this image obtained with the NICMOS instrument embark on the Hubble space telescope. The nebula that surrounds it (in the shape of a gun), extends over 4 years - light. Image obtained in 1997. Astronomers using Nasa's Hubble Space Telescope have identified what may be the most luminous star known “” a celestial mammoth which releases up to 10 million times the power of the Sun and is big enough to fill the diameter of Earth's orbit. The star unleashes as much energy in six seconds

Pistol star - Massive star in the constellation Sagittarius - The massive star Pistol star in Sagittarius - Pistol star is one of the most massive stars in our galaxy. Located about 25,000 years ago - the light of the Earth in the constellation of Sagittarius, this star shines like 10 million Sun consuming in six seconds as much energy as our star in a year. This star is masked by the numerous interstellar dust present in the Sagittarius near the galactic center and appears only in infrared wavelengths, as in this image obtained with the NICMOS instrument embark on the Hubble space telescope. The nebula that surrounds it (in the shape of a gun), extends over 4 years - light. Image obtained in 1997. Astronomers using Nasa's Hubble Space Telescope have identified what may be the most luminous star known “” a celestial mammoth which releases up to 10 million times the power of the Sun and is big enough to fill the diameter of Earth's orbit. The star unleashes as much energy in six seconds

PIX4572084

Flying Star Zeta Ophiuchi - Runaway Star Zeta Ophiuchi - The blue star near the center of the image is Zeta Ophiuchi, a very massive star moving at 24 km per second. It is a “” fleeing star”, a star ejected by the explosion of his companion star. In this infrared image obtained by the WISE (Wide - field Infrared Survey Explorer) satellite, the interstellar dust traversed by the star appears, as well as an arc-shaped shock wave caused by the powerful stellar winds that the star breaks. The blue star near the center of this image is Zeta Ophiuchi. When seen in visible light it appears as a relatively dim red star surrounded by other dim stars and no dust. However, in this infrared image taken with Nasa's Wide - field Infrared Survey Explorer, or WISE, a completely different view emerges. Zeta Ophiuchi is actually a very massive, hot, bright blue star plowing its way through a large cloud of interstellar dust and gas. Astronomers theorize that this stellar juggernaut was likely once part

Flying Star Zeta Ophiuchi - Runaway Star Zeta Ophiuchi - The blue star near the center of the image is Zeta Ophiuchi, a very massive star moving at 24 km per second. It is a “” fleeing star”, a star ejected by the explosion of his companion star. In this infrared image obtained by the WISE (Wide - field Infrared Survey Explorer) satellite, the interstellar dust traversed by the star appears, as well as an arc-shaped shock wave caused by the powerful stellar winds that the star breaks. The blue star near the center of this image is Zeta Ophiuchi. When seen in visible light it appears as a relatively dim red star surrounded by other dim stars and no dust. However, in this infrared image taken with Nasa's Wide - field Infrared Survey Explorer, or WISE, a completely different view emerges. Zeta Ophiuchi is actually a very massive, hot, bright blue star plowing its way through a large cloud of interstellar dust and gas. Astronomers theorize that this stellar juggernaut was likely once part

PIX4572156

Southern Aurora on the Planet Saturn - Aurora on Saturn - The Planet Saturn accompanied by a Southern Aurora, seen in visible and infrared by the Cassini probe on November 1, 2008. This false - color composite image, constructed from data obtained by Nasa's Cassini spacecraft, shows the glow of auroras streaking out about 1,000 kilometers (600 miles) from the cloud tops of Saturn's south polar region. In this image constructed from data collected in the near - infrared wavelengths of light, the auroral emission is shown in green. Scientists designated blue to indicate sunlight reflected at wavelengths from 2 to 3 microns, green to indicate light from hydrogen ions at wavelengths between 3 and 4 microns and red to indicate thermal emission at 5 microns. Saturn's rings and high altitude haze only reflect sunlight at 3 microns or less, so they appear deep blue. The glow from the aurora can only be seen at the wavelengths in the green channel. The heat emission from the interior of Saturn

Southern Aurora on the Planet Saturn - Aurora on Saturn - The Planet Saturn accompanied by a Southern Aurora, seen in visible and infrared by the Cassini probe on November 1, 2008. This false - color composite image, constructed from data obtained by Nasa's Cassini spacecraft, shows the glow of auroras streaking out about 1,000 kilometers (600 miles) from the cloud tops of Saturn's south polar region. In this image constructed from data collected in the near - infrared wavelengths of light, the auroral emission is shown in green. Scientists designated blue to indicate sunlight reflected at wavelengths from 2 to 3 microns, green to indicate light from hydrogen ions at wavelengths between 3 and 4 microns and red to indicate thermal emission at 5 microns. Saturn's rings and high altitude haze only reflect sunlight at 3 microns or less, so they appear deep blue. The glow from the aurora can only be seen at the wavelengths in the green channel. The heat emission from the interior of Saturn

PIX4625211

Titan, Saturn satellite seen by Cassini - Saturn's moon Titan as seen by Cassini spacecraft: Visible and infrared composite image of Titan taken by the Cassini probe on November 13, 2015. View of the hemisphere oriente towards Saturn - This composite image shows an infrared view of Saturn's moon Titan from Nasa's Cassini spacecraft, acquired during the mission's “” T-114”” flyby on Nov. 13, 2015. The spacecraft's visual and infrared mapping spectrometer (VIMS) instrument made these observations, in which blue represents wavelengths centered at 1.3 microns, green represents 2.0 microns, and red represents 5.0 microns. A view at visible wavelengths (centered around 0.5 microns) would show only Titan's hazy atmosphere (as in PIA14909). The near-infrared wavelengths in this image allow Cassini's vision to penetrate the haze and reveal the moon's surface - During this Titan flyby, the spacecraft's close-approach altitude was 6,200 miles (10,000 kilometers), which is considerably higher than

Titan, Saturn satellite seen by Cassini - Saturn's moon Titan as seen by Cassini spacecraft: Visible and infrared composite image of Titan taken by the Cassini probe on November 13, 2015. View of the hemisphere oriente towards Saturn - This composite image shows an infrared view of Saturn's moon Titan from Nasa's Cassini spacecraft, acquired during the mission's “” T-114”” flyby on Nov. 13, 2015. The spacecraft's visual and infrared mapping spectrometer (VIMS) instrument made these observations, in which blue represents wavelengths centered at 1.3 microns, green represents 2.0 microns, and red represents 5.0 microns. A view at visible wavelengths (centered around 0.5 microns) would show only Titan's hazy atmosphere (as in PIA14909). The near-infrared wavelengths in this image allow Cassini's vision to penetrate the haze and reveal the moon's surface - During this Titan flyby, the spacecraft's close-approach altitude was 6,200 miles (10,000 kilometers), which is considerably higher than

PIX4625361

Visible Crab Nebula - Infrared and X - The Crab Nebula - M1, the Crab Nebula, is the rest of a supernova that exploded on July 4, 1054. It is located about 7000 light years from Earth in the constellation Taurus. At the heart of this nebula is a pulsar. To obtain this photo, three spatial observatories combined their observations: the Hubble telescope for the visible part (here in red and yellow), the Chandra telescope for the X-ray data (blue) and the Spitzer telescope for the infrared image (purple). The pulsar is the bright spot in the center of the image. The Crab Nebula (M1) is a supernova remnant at about 7,000 light - year from Earth in the constellation Taurus. The star explosion occured on July 04 1054. At the center of this nebula lies a pulsar. This composite image uses data from three of Nasa's Great Observatories. The Chandra X - ray image is shown in blue, the Hubble Space Telescope optical images are in red and yellow, and the Spitzer Space Telescope's infrared image is

Visible Crab Nebula - Infrared and X - The Crab Nebula - M1, the Crab Nebula, is the rest of a supernova that exploded on July 4, 1054. It is located about 7000 light years from Earth in the constellation Taurus. At the heart of this nebula is a pulsar. To obtain this photo, three spatial observatories combined their observations: the Hubble telescope for the visible part (here in red and yellow), the Chandra telescope for the X-ray data (blue) and the Spitzer telescope for the infrared image (purple). The pulsar is the bright spot in the center of the image. The Crab Nebula (M1) is a supernova remnant at about 7,000 light - year from Earth in the constellation Taurus. The star explosion occured on July 04 1054. At the center of this nebula lies a pulsar. This composite image uses data from three of Nasa's Great Observatories. The Chandra X - ray image is shown in blue, the Hubble Space Telescope optical images are in red and yellow, and the Spitzer Space Telescope's infrared image is

PIX4583130

Red Square Nebula

Red Square Nebula

UIG558014

Cadaver, Beaulieu House, County Louth, Ireland (b/w photo)

Cadaver, Beaulieu House, County Louth, Ireland (b/w photo)

Simon Marsden

TMA95879

Bust of Vlad Dracul, Tirgoviste, Romania (b/w photo)

Bust of Vlad Dracul, Tirgoviste, Romania (b/w photo)

Simon Marsden

TMA3263251

Celtic Head, Ballyboy, County Offaly, Ireland (b/w photo)

Celtic Head, Ballyboy, County Offaly, Ireland (b/w photo)

Simon Marsden

TMA3263166

Petrified Lake, Frenchpark, County Roscommon, Ireland (b/w photo)

Petrified Lake, Frenchpark, County Roscommon, Ireland (b/w photo)

Simon Marsden

TMA3263208

Greenhouse effect on Earth

Greenhouse effect on Earth

UIG558115

Titan, Saturn satellite seen by Cassini: Visible and infrared composite image of Titan taken by the Cassini probe on September 12, 2013. View of methane and ethane lakes. - This false-color mosaic, made from infrared data collected by Nasa's Cassini spacecraft, reveals the differences in the composition of surface materials around hydrocarbon lakes at Titan, Saturn's largest moon. Titan is the only other place in the solar system that we know has stable liquid on its surface, though its lakes are made of liquid ethane and methane rather than liquid water. While there is one large lake and a few smaller ones near Titan's south pole, almost all of Titan's lakes appear near the moon's north pole - Scientists mapped near-infrared colors onto the visible color spectrum. Red in this image was assigned a wavelength of 5 microns (10 times longer than visible light), green 2.0 microns (four times longer than visible light), and blue 1.3 microns (2.6 times longer than visible light) - The orange

Titan, Saturn satellite seen by Cassini: Visible and infrared composite image of Titan taken by the Cassini probe on September 12, 2013. View of methane and ethane lakes. - This false-color mosaic, made from infrared data collected by Nasa's Cassini spacecraft, reveals the differences in the composition of surface materials around hydrocarbon lakes at Titan, Saturn's largest moon. Titan is the only other place in the solar system that we know has stable liquid on its surface, though its lakes are made of liquid ethane and methane rather than liquid water. While there is one large lake and a few smaller ones near Titan's south pole, almost all of Titan's lakes appear near the moon's north pole - Scientists mapped near-infrared colors onto the visible color spectrum. Red in this image was assigned a wavelength of 5 microns (10 times longer than visible light), green 2.0 microns (four times longer than visible light), and blue 1.3 microns (2.6 times longer than visible light) - The orange

PIX4625336

Woods, County Meath, Ireland (b/w photo)

Woods, County Meath, Ireland (b/w photo)

Simon Marsden

TMA3263219

The star Fomalhaut and its dust disc - Star Fomalhaut dust ring - The star Fomalhaut is located 25 years - light from Earth in the constellation of the Southern Fish. A dust disc surrounds it, seen here by the Hubble telescopes (left), Herschel (far infrared, centre) and Alma (right). This disc of interplanetary dust revolves around the young star at a distance of about 20 billion kilometers from it. The image taken at 850 microns wavelength by Alma seems to confirm that the planet discovered in 2008 in the Fomalhaut disc by Hubble does not exist. This image shows Fomalhaut and its dust ring. Images taken by the Hubble space telescope (HST, at left), Herschel telescope (middle) and Alma telescope (at right). Fomalhaut is much hotter than our Sun, 15 times as bright, and lies 25 light - years from Earth. An exoplanet was discovered in its dust ring but Alma observations seem to prove this planet doesn't exist

The star Fomalhaut and its dust disc - Star Fomalhaut dust ring - The star Fomalhaut is located 25 years - light from Earth in the constellation of the Southern Fish. A dust disc surrounds it, seen here by the Hubble telescopes (left), Herschel (far infrared, centre) and Alma (right). This disc of interplanetary dust revolves around the young star at a distance of about 20 billion kilometers from it. The image taken at 850 microns wavelength by Alma seems to confirm that the planet discovered in 2008 in the Fomalhaut disc by Hubble does not exist. This image shows Fomalhaut and its dust ring. Images taken by the Hubble space telescope (HST, at left), Herschel telescope (middle) and Alma telescope (at right). Fomalhaut is much hotter than our Sun, 15 times as bright, and lies 25 light - years from Earth. An exoplanet was discovered in its dust ring but Alma observations seem to prove this planet doesn't exist

PIX4571988

The Horsehead Nebula in infrared - The Horsehead Nebula in infrared - The horse head nebula seen in infrared by the Hubble space telescope. This Hubble space telescope image shows the Horsehead Nebula (Barnard 33) in infrared

The Horsehead Nebula in infrared - The Horsehead Nebula in infrared - The horse head nebula seen in infrared by the Hubble space telescope. This Hubble space telescope image shows the Horsehead Nebula (Barnard 33) in infrared

PIX4622126

Tree Roots, Wakehurst Place, Sussex, England (b/w photo)

Tree Roots, Wakehurst Place, Sussex, England (b/w photo)

Simon Marsden

TMA3263190

Infrared view of the Andromeda galaxy - The Spitzer space telescope observed the Andromede spiral galaxy for over 18 hours on August 25, 2004, obtaining 11,000 different poses. Assembled in mosaic the result shows details never seen before. The brightest ring appears to be hole at the bottom right of the image; these are traces of the passage of a satellite galaxy. Nasa's Spitzer Space Telescope has captured stunning infrared views of the famous Andromeda galaxy to reveal insights that were only hinted at in visible light. Spitzer's 24 - micron mosaic is the sharpest image ever taken of the dust in another spiral galaxy. This is possible because Andromeda is a close neighbor to the Milky Way at a mere 2.5 million light - years away. The Spitzer multiband imaging photometer's 24 - micron detector recorded 11,000 separate snapshots to create this new comprehensive picture. Asymmetrical features are seen in the prominent ring of star formation. The ring appears to be split into two pieces

Infrared view of the Andromeda galaxy - The Spitzer space telescope observed the Andromede spiral galaxy for over 18 hours on August 25, 2004, obtaining 11,000 different poses. Assembled in mosaic the result shows details never seen before. The brightest ring appears to be hole at the bottom right of the image; these are traces of the passage of a satellite galaxy. Nasa's Spitzer Space Telescope has captured stunning infrared views of the famous Andromeda galaxy to reveal insights that were only hinted at in visible light. Spitzer's 24 - micron mosaic is the sharpest image ever taken of the dust in another spiral galaxy. This is possible because Andromeda is a close neighbor to the Milky Way at a mere 2.5 million light - years away. The Spitzer multiband imaging photometer's 24 - micron detector recorded 11,000 separate snapshots to create this new comprehensive picture. Asymmetrical features are seen in the prominent ring of star formation. The ring appears to be split into two pieces

PIX4608959

Trench Mausoleum, Woodlawn, County Galway, Ireland (b/w photo)

Trench Mausoleum, Woodlawn, County Galway, Ireland (b/w photo)

Simon Marsden

TMA3263567

Sombrero M104 Spiral Galaxy - Visible Composite - Infrared - The Sombrero galaxy. Composite of visible and infrared views - Composite image of the spiral galaxy M104 (Sombrero galaxy), located about 28 million years ago - light. Infrared image obtained with the Spitzer space telescope in 2004 and January 2005 superimposed on the image made by the Hubble space telescope visible in May and June 2003. The dark band of girders in this galaxy is visible throughout the circumference. Composite image of a visible image and an infrared image of the galaxy M104. The visible image was obtained by the Hubble space telescope in 2003, the infrared view by Spitzer telescope in 2004 and 2005. This spiral galaxy is located some 28 million light - years away. The infrared image obtained by Spitzer space telescope pierces through the obscuring dust, along with the bulge of stars. It shows that the disk is warped, which is often the result of a gravitational encounter with another galaxy; clumpy areas sp

Sombrero M104 Spiral Galaxy - Visible Composite - Infrared - The Sombrero galaxy. Composite of visible and infrared views - Composite image of the spiral galaxy M104 (Sombrero galaxy), located about 28 million years ago - light. Infrared image obtained with the Spitzer space telescope in 2004 and January 2005 superimposed on the image made by the Hubble space telescope visible in May and June 2003. The dark band of girders in this galaxy is visible throughout the circumference. Composite image of a visible image and an infrared image of the galaxy M104. The visible image was obtained by the Hubble space telescope in 2003, the infrared view by Spitzer telescope in 2004 and 2005. This spiral galaxy is located some 28 million light - years away. The infrared image obtained by Spitzer space telescope pierces through the obscuring dust, along with the bulge of stars. It shows that the disk is warped, which is often the result of a gravitational encounter with another galaxy; clumpy areas sp

PIX4611601

Roadside Shrine, County Roscommon, Ireland (b/w photo)

Roadside Shrine, County Roscommon, Ireland (b/w photo)

Simon Marsden

TMA3263526

Broken Frieze, Ducketts Grove, County Carlow, Ireland (b/w photo)

Broken Frieze, Ducketts Grove, County Carlow, Ireland (b/w photo)

Simon Marsden

TMA3263496

The Horsehead Nebula in infrared - The Horsehead Nebula in infrared - This infrared image shows the nebula of the horse's head (right) accompanied by the small nebula NGC 2023. Image obtained by the 4 meter telescope VISTA. This VISTA (infrared ESO 4 meter telescope) view shows the ghostly outline of the Horsehead Nebula (Barnard 33), at right, and the reflection nebula NGC 2023

The Horsehead Nebula in infrared - The Horsehead Nebula in infrared - This infrared image shows the nebula of the horse's head (right) accompanied by the small nebula NGC 2023. Image obtained by the 4 meter telescope VISTA. This VISTA (infrared ESO 4 meter telescope) view shows the ghostly outline of the Horsehead Nebula (Barnard 33), at right, and the reflection nebula NGC 2023

PIX4622111

Spiral galaxy of the Sombrero M104 infrared view - Sombrero galaxy seen in infrared - Infrared image of the spiral galaxy M104 (Sombrero galaxy), located about 28 million years ago - light, obtained with the Spitzer space telescope in 2004 and January 2005. Infrared radiation shows the dust of the disc visible throughout the circumference. A high emission also comes from the center of the galaxy where a supermassive black hole is thought to reside there. This spiral galaxy is located some 28 million light - years away. The infrared image obtained by Spitzer space telescope in 2004 and 2005 pierces through the obscuring dust, along with the bulge of stars. It shows that the disk is warped, which is often the result of a gravitational encounter with another galaxy; clumpy areas spotted in the far edges of the ring indicate young star - forming regions. Spitzer detected infrared emission not only from the ring, but from the center of the galaxy too, where there is a huge black hole, belie

Spiral galaxy of the Sombrero M104 infrared view - Sombrero galaxy seen in infrared - Infrared image of the spiral galaxy M104 (Sombrero galaxy), located about 28 million years ago - light, obtained with the Spitzer space telescope in 2004 and January 2005. Infrared radiation shows the dust of the disc visible throughout the circumference. A high emission also comes from the center of the galaxy where a supermassive black hole is thought to reside there. This spiral galaxy is located some 28 million light - years away. The infrared image obtained by Spitzer space telescope in 2004 and 2005 pierces through the obscuring dust, along with the bulge of stars. It shows that the disk is warped, which is often the result of a gravitational encounter with another galaxy; clumpy areas spotted in the far edges of the ring indicate young star - forming regions. Spitzer detected infrared emission not only from the ring, but from the center of the galaxy too, where there is a huge black hole, belie

PIX4611595

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

Star clusters IC 348 in Persee seen in infrared - Star clusters IC 348 in Perseus - IC 348 is a cluster of 300 stars associated with a relatively bright nebula. The infrared image of the Spitzer telescope shows young stars (red and pink) that appeared about 3 million years ago and still surrounded by their gas cocoon. The nebula is located 1043 years of light from Earth. The IC 348 is a cluster which contains more than 300 young stars. Baby stars are forming near the eastern rim of the cosmic cloud Perseus, in this infrared image from Nasa's Spitzer Space Telescope. The baby stars are approximately three million years old and are shown as reddish - pink dots to the right of the image. The pinkish color indicates that these infant stars are still shrouded by the cosmic dust and gas that collapsed to form them. The Perseus Nebula is located about 1,043 light - years away in the Perseus constellation

Star clusters IC 348 in Persee seen in infrared - Star clusters IC 348 in Perseus - IC 348 is a cluster of 300 stars associated with a relatively bright nebula. The infrared image of the Spitzer telescope shows young stars (red and pink) that appeared about 3 million years ago and still surrounded by their gas cocoon. The nebula is located 1043 years of light from Earth. The IC 348 is a cluster which contains more than 300 young stars. Baby stars are forming near the eastern rim of the cosmic cloud Perseus, in this infrared image from Nasa's Spitzer Space Telescope. The baby stars are approximately three million years old and are shown as reddish - pink dots to the right of the image. The pinkish color indicates that these infant stars are still shrouded by the cosmic dust and gas that collapsed to form them. The Perseus Nebula is located about 1,043 light - years away in the Perseus constellation

PIX4568939

Steps up to Queribus Castle, Languedoc, France (b/w photo)

Steps up to Queribus Castle, Languedoc, France (b/w photo)

Simon Marsden

TMA3262886

Loch Fynne, Argyll, Scotland (b/w photo)

Loch Fynne, Argyll, Scotland (b/w photo)

Simon Marsden

TMA3263196

Connor Pass, County Kerry, Ireland (b/w photo)

Connor Pass, County Kerry, Ireland (b/w photo)

Simon Marsden

TMA3263216

Menhir of Guihalon, Brittany, France (b/w photo)

Menhir of Guihalon, Brittany, France (b/w photo)

Simon Marsden

TMA3262986

Star Formation in Cassiopee - Star Formation in Cassiopeia - This star-forming region, called W5, is located approximately 6500 light years ago in the constellation Cassiopee. Several generations of stars appear on this cliche; the older ones are the blue stars in the centre of the two cavities; the younger stars are grouped at the edges of these cavities and at the ends of the gas pillars or they appear like pink dots; the white areas are home to the very young stars in formation. In this infrared image, heated dust appears in red, dense gas clouds appear in green. Composite image obtained by the Spitzer space telescope in 2006 and 2007. Generations of stars can be seen in this infrared portrait from Nasa's Spitzer Space Telescope. In this wispy star - forming region, called W5, the oldest stars can be seen as blue dots in the centers of the two hollow cavities (other blue dots are background and foreground stars not associated with the region). Younger stars line the rims of the cavi

Star Formation in Cassiopee - Star Formation in Cassiopeia - This star-forming region, called W5, is located approximately 6500 light years ago in the constellation Cassiopee. Several generations of stars appear on this cliche; the older ones are the blue stars in the centre of the two cavities; the younger stars are grouped at the edges of these cavities and at the ends of the gas pillars or they appear like pink dots; the white areas are home to the very young stars in formation. In this infrared image, heated dust appears in red, dense gas clouds appear in green. Composite image obtained by the Spitzer space telescope in 2006 and 2007. Generations of stars can be seen in this infrared portrait from Nasa's Spitzer Space Telescope. In this wispy star - forming region, called W5, the oldest stars can be seen as blue dots in the centers of the two hollow cavities (other blue dots are background and foreground stars not associated with the region). Younger stars line the rims of the cavi

PIX4621160

Star Formation in Cassiopee - Star Formation in Cassiopeia - This star-forming region, called W5, is located approximately 6500 light years ago in the constellation Cassiopee. Several generations of stars appear on this cliche; the older ones are the blue stars in the centre of the two cavities; the younger stars are grouped at the edges of these cavities and at the ends of the gas pillars or they appear like pink dots; the white areas are home to the very young stars in formation. In this infrared image, heated dust appears in red, dense gas clouds appear in green. Composite image obtained by the Spitzer space telescope in 2006 and 2007. Generations of stars can be seen in this infrared portrait from Nasa's Spitzer Space Telescope. In this wispy star - forming region, called W5, the oldest stars can be seen as blue dots in the centers of the two hollow cavities (other blue dots are background and foreground stars not associated with the region). Younger stars line the rims of the cavi

Star Formation in Cassiopee - Star Formation in Cassiopeia - This star-forming region, called W5, is located approximately 6500 light years ago in the constellation Cassiopee. Several generations of stars appear on this cliche; the older ones are the blue stars in the centre of the two cavities; the younger stars are grouped at the edges of these cavities and at the ends of the gas pillars or they appear like pink dots; the white areas are home to the very young stars in formation. In this infrared image, heated dust appears in red, dense gas clouds appear in green. Composite image obtained by the Spitzer space telescope in 2006 and 2007. Generations of stars can be seen in this infrared portrait from Nasa's Spitzer Space Telescope. In this wispy star - forming region, called W5, the oldest stars can be seen as blue dots in the centers of the two hollow cavities (other blue dots are background and foreground stars not associated with the region). Younger stars line the rims of the cavi

PIX4621152

Titan, Saturn satellite seen by Cassini - Saturn's moon Titan as seen by Cassini spacecraft: Visible and infrared composite image of Titan taken by the Cassini probe on August 21, 2014. View of methane and ethane lakes lit by the Sun. - This near-infrared, color mosaic from Nasa's Cassini spacecraft shows the sun glinting off of Titan's north polar seas. - The sunglint, also called a specular reflection, is the bright area near the 11 o'clock position at upper left. This mirror-like reflection, known as the specular point, is in the south of Titan's largest sea, Kraken Mare, just north of an island archipelago separating two separate parts of the sea - This particular sunglint was so bright as to saturate the detector of Cassini's Visual and Infrared Mapping Spectrometer (VIMS) instrument, which captures the view. - The southern portion of Kraken Mare (the area surrounding the specular feature toward upper left) displays a “” bathtub ring”” - a bright margin of evaporate deposits - whi

Titan, Saturn satellite seen by Cassini - Saturn's moon Titan as seen by Cassini spacecraft: Visible and infrared composite image of Titan taken by the Cassini probe on August 21, 2014. View of methane and ethane lakes lit by the Sun. - This near-infrared, color mosaic from Nasa's Cassini spacecraft shows the sun glinting off of Titan's north polar seas. - The sunglint, also called a specular reflection, is the bright area near the 11 o'clock position at upper left. This mirror-like reflection, known as the specular point, is in the south of Titan's largest sea, Kraken Mare, just north of an island archipelago separating two separate parts of the sea - This particular sunglint was so bright as to saturate the detector of Cassini's Visual and Infrared Mapping Spectrometer (VIMS) instrument, which captures the view. - The southern portion of Kraken Mare (the area surrounding the specular feature toward upper left) displays a “” bathtub ring”” - a bright margin of evaporate deposits - whi

PIX4625340

Statues, Chantilly Chateau, Picardy, France (b/w photo)

Statues, Chantilly Chateau, Picardy, France (b/w photo)

Simon Marsden

TMA3263010

Mazan Cemetery, Provence, France (b/w photo)

Mazan Cemetery, Provence, France (b/w photo)

Simon Marsden

TMA3263028

Field of distant galaxies - Hubble eXtreme Deep Field (XDF) - Distant galaxies - Hubble eXtreme Deep Field (XDF) - Image of distant galaxies obtained in infrared by the Hubble space telescope in the constellation of the Furnace. The farthest galaxies visible in this image are 13.2 billion light years away. Called the Extreme Deep Field, or XDF, the photo was assembled by combining 10 years of NASA Hubble Space Telescope photographs taken of a patch of sky at the center of the original Hubble Ultra Deep Field. The XDF is a small fraction of the angular diameter of the full Moon. The Hubble Ultra Deep Field is an image of a small area of space in the constellation Fornax, created using Hubble Space Telescope data from 2003 and 2004. By collecting faint light over many hours of observation, it revealed thousands of galaxies, both nearby and very distant, making it the deepest image of the universe ever taken at that time. The new full - color XDF image reaches much fainter galaxies, and i

Field of distant galaxies - Hubble eXtreme Deep Field (XDF) - Distant galaxies - Hubble eXtreme Deep Field (XDF) - Image of distant galaxies obtained in infrared by the Hubble space telescope in the constellation of the Furnace. The farthest galaxies visible in this image are 13.2 billion light years away. Called the Extreme Deep Field, or XDF, the photo was assembled by combining 10 years of NASA Hubble Space Telescope photographs taken of a patch of sky at the center of the original Hubble Ultra Deep Field. The XDF is a small fraction of the angular diameter of the full Moon. The Hubble Ultra Deep Field is an image of a small area of space in the constellation Fornax, created using Hubble Space Telescope data from 2003 and 2004. By collecting faint light over many hours of observation, it revealed thousands of galaxies, both nearby and very distant, making it the deepest image of the universe ever taken at that time. The new full - color XDF image reaches much fainter galaxies, and i

PIX4613831

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