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Photometer for the Hubble Telescope, 1980s

Photometer for the Hubble Telescope, 1980s

UIS5073578

Laser shooting at the Paranal Observatory - The VLT Laser Guide Star - View from the LGS (Laser Guide Star), a laser beam launches from the Yepun (UT4) telescope of the VLT. This laser creates an artificial star in the high atmosphere at about 90 km altitude. This repere is analysed and each variation of turbulence in the atmosphere is detected and corrected by the adaptive optics of the telescope. On the left, the two galaxies of the Magellan Cloud, on the right, the dome of the VST (VLT Survey Telescope). A 50 cm wide yellow laser beam is coming out of Yepun, (UT4) of the Very Large Telescope. It is used to create a yellow artificial star at 95 km of altitude which helps the adaptive optics to measure and correct the atmosphere's blurring effect. On the left, the two Magellanic Clouds, on the right, the VST dome

Laser shooting at the Paranal Observatory - The VLT Laser Guide Star - View from the LGS (Laser Guide Star), a laser beam launches from the Yepun (UT4) telescope of the VLT. This laser creates an artificial star in the high atmosphere at about 90 km altitude. This repere is analysed and each variation of turbulence in the atmosphere is detected and corrected by the adaptive optics of the telescope. On the left, the two galaxies of the Magellan Cloud, on the right, the dome of the VST (VLT Survey Telescope). A 50 cm wide yellow laser beam is coming out of Yepun, (UT4) of the Very Large Telescope. It is used to create a yellow artificial star at 95 km of altitude which helps the adaptive optics to measure and correct the atmosphere's blurring effect. On the left, the two Magellanic Clouds, on the right, the VST dome

Stephane Guisard

PIX4656905

Sonde Jupiter Icy Moon Explorer (JUICE) (2023-2030) (illustration)

Sonde Jupiter Icy Moon Explorer (JUICE) (2023-2030) (illustration)

D. Ducros

PIX8702151

The main control room of Dungeness nuclear power station with operators

The main control room of Dungeness nuclear power station with operators

UIS5075350

Jesse Ramsden, English instrument maker, 1791

Jesse Ramsden, English instrument maker, 1791

UIS5062460

Troughton's repeating circle without reflection, 1820

Troughton's repeating circle without reflection, 1820

UIS5096203

Planetary nebula NGC 5189 in the Fly - NGC 5189, a weird planetary nebula - This nebula is located about 3000 years from Earth in the southern constellation of Fly. Image obtained from the 3.9m telescope of Siding Spring The peculiarity of NGC 5189 lies in its astonishingly complex structure, first noted by Sir John Herschel, who discovered it in 1835. Seen through the telescope it seems to have an 'S' shape, reminiscent of a barred spiral galaxy, hence its popular name. This is seen in the colour photograph as the central greenish part. Deep photographs such as this show many filaments, rather more reminiscent of the Crab nebula, a supernova remnant, than a planetary nebula. Unlike the Crab nebula, NGC 5189 is remarkably symmetrical. Distances to planetary nebulae are notoriously difficult to measure, but this one is estimated to be about 3000 light years away

Planetary nebula NGC 5189 in the Fly - NGC 5189, a weird planetary nebula - This nebula is located about 3000 years from Earth in the southern constellation of Fly. Image obtained from the 3.9m telescope of Siding Spring The peculiarity of NGC 5189 lies in its astonishingly complex structure, first noted by Sir John Herschel, who discovered it in 1835. Seen through the telescope it seems to have an 'S' shape, reminiscent of a barred spiral galaxy, hence its popular name. This is seen in the colour photograph as the central greenish part. Deep photographs such as this show many filaments, rather more reminiscent of the Crab nebula, a supernova remnant, than a planetary nebula. Unlike the Crab nebula, NGC 5189 is remarkably symmetrical. Distances to planetary nebulae are notoriously difficult to measure, but this one is estimated to be about 3000 light years away

PIX4623110

Gregorian reflecting telescope, 1763-65

Gregorian reflecting telescope, 1763-65

UIS5089768

Jesse Ramsden, English optician and instrument maker, 1791

Jesse Ramsden, English optician and instrument maker, 1791

UIS5087757

Photometer for the Hubble Telescope, 1980s

Photometer for the Hubble Telescope, 1980s

UIS5073565

Solar disc showing sunspots in false colour, taken from Skylab, 1973

Solar disc showing sunspots in false colour, taken from Skylab, 1973

UIS5070617

Jean-Baptiste Biot, French physicist and astronomer, c 1850-1862

Jean-Baptiste Biot, French physicist and astronomer, c 1850-1862

UIS5064048

Sonde Jupiter Icy Moon Explorer (JUICE) (2023-2030) (illustration)

Sonde Jupiter Icy Moon Explorer (JUICE) (2023-2030) (illustration)

D. Ducros

PIX8702152

Sonde Jupiter Icy Moon Explorer (JUICE) (2023-2030) (illustration)

Sonde Jupiter Icy Moon Explorer (JUICE) (2023-2030) (illustration)

D. Ducros

PIX8702153

Daniell hygrometer made by W

Daniell hygrometer made by W

UIS5102131

Daniell hygrometer made by W

Daniell hygrometer made by W

UIS5102151

Constellation of Sextant - Constellation of Sextans - Constellation of Sextant; below part of the constellation Hydra. At the top of the picture, the bright star is Regulus, of the Lion. Sextans, and part of Hydra. Top of image, the bright star is Regulus in Leo. Sextans, (the Sextant, originally Sextans Uraniae), is small, faint, equatorial constellation south of Leo, framed by the bright stars Regulus to the north and Alphard to the west. It was introduced by Johannes Hevelius in 1687 to commemorate the instrument with which he continued to measure star positions for long after the telescope had been invented. This small and insignificant constellation measures a little more than 17 degrees on a side (about 313 degrees square) and is ranked 45th in area out of the 88 modern constellations. In contrast is the winding collection of stars that make up the head of the Hydra, the Water Snake. This is the largest constellation in the sky, extending over 1300 square degrees, and though the

Constellation of Sextant - Constellation of Sextans - Constellation of Sextant; below part of the constellation Hydra. At the top of the picture, the bright star is Regulus, of the Lion. Sextans, and part of Hydra. Top of image, the bright star is Regulus in Leo. Sextans, (the Sextant, originally Sextans Uraniae), is small, faint, equatorial constellation south of Leo, framed by the bright stars Regulus to the north and Alphard to the west. It was introduced by Johannes Hevelius in 1687 to commemorate the instrument with which he continued to measure star positions for long after the telescope had been invented. This small and insignificant constellation measures a little more than 17 degrees on a side (about 313 degrees square) and is ranked 45th in area out of the 88 modern constellations. In contrast is the winding collection of stars that make up the head of the Hydra, the Water Snake. This is the largest constellation in the sky, extending over 1300 square degrees, and though the

PIX4594016

Constellation of Sextant - Constellation of Sextans - Constellation of Sextant; below part of the constellation Hydra. At the top of the picture, the bright star is Regulus, of the Lion. Sextans, and part of Hydra. Top of image, the bright star is Regulus in Leo. Sextans, (the Sextant, originally Sextans Uraniae), is small, faint, equatorial constellation south of Leo, framed by the bright stars Regulus to the north and Alphard to the west. It was introduced by Johannes Hevelius in 1687 to commemorate the instrument with which he continued to measure star positions for long after the telescope had been invented. This small and insignificant constellation measures a little more than 17 degrees on a side (about 313 degrees square) and is ranked 45th in area out of the 88 modern constellations. In contrast is the winding collection of stars that make up the head of the Hydra, the Water Snake. This is the largest constellation in the sky, extending over 1300 square degrees, and though the

Constellation of Sextant - Constellation of Sextans - Constellation of Sextant; below part of the constellation Hydra. At the top of the picture, the bright star is Regulus, of the Lion. Sextans, and part of Hydra. Top of image, the bright star is Regulus in Leo. Sextans, (the Sextant, originally Sextans Uraniae), is small, faint, equatorial constellation south of Leo, framed by the bright stars Regulus to the north and Alphard to the west. It was introduced by Johannes Hevelius in 1687 to commemorate the instrument with which he continued to measure star positions for long after the telescope had been invented. This small and insignificant constellation measures a little more than 17 degrees on a side (about 313 degrees square) and is ranked 45th in area out of the 88 modern constellations. In contrast is the winding collection of stars that make up the head of the Hydra, the Water Snake. This is the largest constellation in the sky, extending over 1300 square degrees, and though the

PIX4594022

Crane control room of the Pile Cap section, Sizewell Nuclear Power Station

Crane control room of the Pile Cap section, Sizewell Nuclear Power Station

UIS5075245

The main control room at Sizewell Nuclear Power station, 1965

The main control room at Sizewell Nuclear Power station, 1965

UIS5076222

Workers inside Sizewell Nuclear Power Station, 1965

Workers inside Sizewell Nuclear Power Station, 1965

UIS5076237

loading fuel elements in to cradle at Hinkley Point nuclear power station

loading fuel elements in to cradle at Hinkley Point nuclear power station

UIS5075196

Cepheides in the galaxy M81 - Cepheids in the galaxy M81 - Cepheides are very bright variable stars that serve as cosmic beacons to measure distance from nearby galaxies. Their pulse period is measured and their absolute luminosite is calculated. By comparing the result to their apparent luminosite in the sky, they can be calculated accurately. Here, the space telescope identified cepheides in the M81 galaxy; astronomers were able to deduce a new distance for this galaxy; it would be 11 million years - light from Earth; previous estimates gave a figure of 18 million light years. Image obtained in 1993. Astronomers have discovered variable stars in the spiral galaxy M81, and measured the distance of the galaxy to be 11 million light - years (3.4 megaparsecs). They quote a 10% uncertainty in this result (plus or minus approximately one million light - years). Previous estimates of the galaxy's distance have ranged from 4.5 to 18 million light - years (1.4 to 5.6 megaparsecs). The astrono

Cepheides in the galaxy M81 - Cepheids in the galaxy M81 - Cepheides are very bright variable stars that serve as cosmic beacons to measure distance from nearby galaxies. Their pulse period is measured and their absolute luminosite is calculated. By comparing the result to their apparent luminosite in the sky, they can be calculated accurately. Here, the space telescope identified cepheides in the M81 galaxy; astronomers were able to deduce a new distance for this galaxy; it would be 11 million years - light from Earth; previous estimates gave a figure of 18 million light years. Image obtained in 1993. Astronomers have discovered variable stars in the spiral galaxy M81, and measured the distance of the galaxy to be 11 million light - years (3.4 megaparsecs). They quote a 10% uncertainty in this result (plus or minus approximately one million light - years). Previous estimates of the galaxy's distance have ranged from 4.5 to 18 million light - years (1.4 to 5.6 megaparsecs). The astrono

PIX4572157

On top of main boilers, Sizewell Nuclear Power station, Suffolk, 1965

On top of main boilers, Sizewell Nuclear Power station, Suffolk, 1965

UIS5075233

Main control room (salle de controle) of Sizewell power station showing consoles, 1965

Main control room (salle de controle) of Sizewell power station showing consoles, 1965

UIS5075243

Desplittering machine with operators at Sizewell Nuclear Power Station, 1965

Desplittering machine with operators at Sizewell Nuclear Power Station, 1965

UIS5076234

Operator with preparation machine, Sizewell Nuclear Power Station, 1965

Operator with preparation machine, Sizewell Nuclear Power Station, 1965

UIS5076246

Pile cap and loading machine at Sizewell Nuclear Power Station, 1965

Pile cap and loading machine at Sizewell Nuclear Power Station, 1965

UIS5076230

Daniell hygrometer made by W

Daniell hygrometer made by W

UIS5102153

Portrait of Jesse Ramsden, The Astronomical Observatory "Giuseppe Piazzi", the Pisana Tower

Portrait of Jesse Ramsden, The Astronomical Observatory "Giuseppe Piazzi", the Pisana Tower

Unknown artist, (18th-19th century)

GRL3900265

Telescope used by General Roy, Hounslow Heath, Middlesex, 1784

Telescope used by General Roy, Hounslow Heath, Middlesex, 1784

UIS5065363

A worker on top of boilers 1A and 1B, Sizewell Nuclear Power Station, 1965

A worker on top of boilers 1A and 1B, Sizewell Nuclear Power Station, 1965

UIS5075277

Worker stands under vast cooling pipes at Sizewell Nuclear Power Station, 1965

Worker stands under vast cooling pipes at Sizewell Nuclear Power Station, 1965

UIS5076227

Earth seen by satellite DSCOVR - Earth seen by satellite DSCOVR - Earth photo obtained by satellite Deep Space Climate Observatory (DSCOVR) on July 6, 2015. This satellite, launched on 11 February 2015, and placed in orbit 1.6 million km, at the point of Lagrange L1 (about 4 times farther than the orbit of the Moon), allows us to obtain views of the Earth as a whole. The journey has been a long one for the Deep Space Climate Observatory (DSCOVR). Once known as Triana, the satellite was conceived in 1998 to provide continuous views of Earth, to monitor the solar wind, and to measure fluctuations in Earth's albedo. The mission was put on hold in 2001, and the partly - built satellite ended up in storage for several years with an uncertain future. In 2008, the National Oceanic and Atmospheric Administration (NOAA), NASA, and the U.S. Air Force decided to refurbish and update the spacecraft for launch

Earth seen by satellite DSCOVR - Earth seen by satellite DSCOVR - Earth photo obtained by satellite Deep Space Climate Observatory (DSCOVR) on July 6, 2015. This satellite, launched on 11 February 2015, and placed in orbit 1.6 million km, at the point of Lagrange L1 (about 4 times farther than the orbit of the Moon), allows us to obtain views of the Earth as a whole. The journey has been a long one for the Deep Space Climate Observatory (DSCOVR). Once known as Triana, the satellite was conceived in 1998 to provide continuous views of Earth, to monitor the solar wind, and to measure fluctuations in Earth's albedo. The mission was put on hold in 2001, and the partly - built satellite ended up in storage for several years with an uncertain future. In 2008, the National Oceanic and Atmospheric Administration (NOAA), NASA, and the U.S. Air Force decided to refurbish and update the spacecraft for launch

PIX4632004

Measuring time

Hardy, Wilf (Wilfred) (20th century)

LAL300748

The research and development makes erosion evaluation on turbine, HInkley

The research and development makes erosion evaluation on turbine, HInkley

UIS5075293

Astronaut Roberta Bondar in the rotating chair 01/1992 - Astronaut Roberta Bondar in rotator chair - Roberta Bondar in the spacelab module, prepares for the experience of the rotating chair in order to experiment with the effects of microgravite on the vestibular system (the main sensory system of perception of motion and orientation in relation to vertical). 01/1992. STS - 42 Payload Specialist Roberta L. Bondar gets into the Microgravity Vestibular Investigations rotator chair to begin an experiment. The chair is mounted in the center aisle of the International Microgravity Laboratory 1 spacelab module. Just above Bondar's head is the helmet assembly which is outfitted with accelerometers to measure head movements and visors that fit over each eye independently to provide visual stimuli. The chair system has three movement patterns: “” sinusoidal”” or traveling predictably back and forth over the same distance at a constant speed; “” pseudorandom””” or moving back and forth over vary

Astronaut Roberta Bondar in the rotating chair 01/1992 - Astronaut Roberta Bondar in rotator chair - Roberta Bondar in the spacelab module, prepares for the experience of the rotating chair in order to experiment with the effects of microgravite on the vestibular system (the main sensory system of perception of motion and orientation in relation to vertical). 01/1992. STS - 42 Payload Specialist Roberta L. Bondar gets into the Microgravity Vestibular Investigations rotator chair to begin an experiment. The chair is mounted in the center aisle of the International Microgravity Laboratory 1 spacelab module. Just above Bondar's head is the helmet assembly which is outfitted with accelerometers to measure head movements and visors that fit over each eye independently to provide visual stimuli. The chair system has three movement patterns: “” sinusoidal”” or traveling predictably back and forth over the same distance at a constant speed; “” pseudorandom””” or moving back and forth over vary

PIX4646902

Main control room at Hinkley Point Nuclear Power Station, Somerset, 1965

Main control room at Hinkley Point Nuclear Power Station, Somerset, 1965

UIS5076241

Operators in main control room (salle de controle) at Hinkley Point nuclear power station

Operators in main control room (salle de controle) at Hinkley Point nuclear power station

UIS5076259

Nuclear workers load machine on reactor power cap, Hinkley Point, 1965

Nuclear workers load machine on reactor power cap, Hinkley Point, 1965

UIS5075282

Main control room at Hinkley Point with the instrument reader at control panel

Main control room at Hinkley Point with the instrument reader at control panel

UIS5075298

Deinotherium - Deinotherium appeared in the middle Miocene and the genus fades in the lower Pleistocene. It probably looked like modern elephants, except that its trunk was shorter, its defenses were attached to the lower jaw (not to the skull), and they pointed downwards. Deinotherium is the third largest known terrestrial mammal ever; only Baluchitherium grangeri and Mammuthus sungari were larger. Males were generally 3.5 to 4.5 m tall to the shoulders, although some large specimens were able to measure up to 5m. Their weight was estimated to be between 5 and 10 tonnes and above 14 tonnes for the larger males. Deinotherium crosses the rolling plains of what is today Europe. A prehistoric relative of modern elephants, Deinotherium was larger and had a shorter trunk and downward-curving tusks attached to its lower jaw. Deinotherium is the third largest land mammal known to have existed; only Paraceratherium and some mammoths were larger. Deinotherium likely behaved like modern elephant

Deinotherium - Deinotherium appeared in the middle Miocene and the genus fades in the lower Pleistocene. It probably looked like modern elephants, except that its trunk was shorter, its defenses were attached to the lower jaw (not to the skull), and they pointed downwards. Deinotherium is the third largest known terrestrial mammal ever; only Baluchitherium grangeri and Mammuthus sungari were larger. Males were generally 3.5 to 4.5 m tall to the shoulders, although some large specimens were able to measure up to 5m. Their weight was estimated to be between 5 and 10 tonnes and above 14 tonnes for the larger males. Deinotherium crosses the rolling plains of what is today Europe. A prehistoric relative of modern elephants, Deinotherium was larger and had a shorter trunk and downward-curving tusks attached to its lower jaw. Deinotherium is the third largest land mammal known to have existed; only Paraceratherium and some mammoths were larger. Deinotherium likely behaved like modern elephant

Walter B Myers

PIX4664540

Operator and main control room (salle de contole) at Hinkley Point nuclear power station

Operator and main control room (salle de contole) at Hinkley Point nuclear power station

UIS5076249

Star cluster M46 and planetary nebula NGC 2438 - Open cluster M46 and planetary nebula NGC 2438 - M46 (NGC 2437) is an age cluster located at 5400 years - light. It contains about 500 stars, 150 of which are brilliant. It is about 300 million years old. The planetary nebula NGC 2438 does not appear to belong to this cluster, and must be closer although its distance is unknown. Image obtained by Siding Spring's 3.9m telescope The open cluster NGC 2437 (M46) has an angular diameter of almost half a degree and is quite beautiful in even quite a modest telescope. It has an integrated magnitude of about 6 and so is on the threshold of naked - eye visibility. The cluster is quite old as these things go, about 300 million light years. It is about 5000 light years distant, in the northern part of the constellation of Puppis. Although planetary nebula distances are notoriously difficult to measure, NGC 2438 seems to be in the foreground and is not connected to the cluster. Planetaries are in an

Star cluster M46 and planetary nebula NGC 2438 - Open cluster M46 and planetary nebula NGC 2438 - M46 (NGC 2437) is an age cluster located at 5400 years - light. It contains about 500 stars, 150 of which are brilliant. It is about 300 million years old. The planetary nebula NGC 2438 does not appear to belong to this cluster, and must be closer although its distance is unknown. Image obtained by Siding Spring's 3.9m telescope The open cluster NGC 2437 (M46) has an angular diameter of almost half a degree and is quite beautiful in even quite a modest telescope. It has an integrated magnitude of about 6 and so is on the threshold of naked - eye visibility. The cluster is quite old as these things go, about 300 million light years. It is about 5000 light years distant, in the northern part of the constellation of Puppis. Although planetary nebula distances are notoriously difficult to measure, NGC 2438 seems to be in the foreground and is not connected to the cluster. Planetaries are in an

PIX4568052

Thailand: The karst limestone peaks of Khao Sok National Park, Surat Thani Province

Thailand: The karst limestone peaks of Khao Sok National Park, Surat Thani Province

David Henley

PFH2839118

Thailand: The karst limestone peaks of Khao Sok National Park, Surat Thani Province

Thailand: The karst limestone peaks of Khao Sok National Park, Surat Thani Province

David Henley

PFH2839119

Thailand: The karst limestone peaks of Khao Sok National Park, Surat Thani Province

Thailand: The karst limestone peaks of Khao Sok National Park, Surat Thani Province

David Henley

PFH2839120

Thailand: The karst limestone peaks of Khao Sok National Park, Surat Thani Province

Thailand: The karst limestone peaks of Khao Sok National Park, Surat Thani Province

David Henley

PFH2839122

Thailand: The karst limestone peaks of Khao Sok National Park, Surat Thani Province

Thailand: The karst limestone peaks of Khao Sok National Park, Surat Thani Province

David Henley

PFH2839123

Infrared view of the Andromeda galaxy - Composite of three different wavelengths 24 microns (blue), 70 microns (green), and 160 microns (red). Using these three bands, we can know the temperature differences of the dust: the warmest are the brightest at 24 microns and the coldest shine at 160 microns. The blue/white areas contain the hottest dust. View obtained by Spitzer space telescope on 25 August 2004. The multi - wavelength view of Andromeda combines images taken at 24 microns (blue), 70 microns (green), and 160 microns (red). Using all three bands from the multiband imaging photometer allows astronomers to measure the temperature of the dust by its color. The warmest dust is brightest at 24 microns while the coolest is most evident at 160 microns. The blue/white areas have the hottest dust, as seen in the bulge and in the star - forming areas along the arms. The cooler dust floating further out in the ring and arms are in the redder regions. The data were taken on August 25, 2004

Infrared view of the Andromeda galaxy - Composite of three different wavelengths 24 microns (blue), 70 microns (green), and 160 microns (red). Using these three bands, we can know the temperature differences of the dust: the warmest are the brightest at 24 microns and the coldest shine at 160 microns. The blue/white areas contain the hottest dust. View obtained by Spitzer space telescope on 25 August 2004. The multi - wavelength view of Andromeda combines images taken at 24 microns (blue), 70 microns (green), and 160 microns (red). Using all three bands from the multiband imaging photometer allows astronomers to measure the temperature of the dust by its color. The warmest dust is brightest at 24 microns while the coolest is most evident at 160 microns. The blue/white areas have the hottest dust, as seen in the bulge and in the star - forming areas along the arms. The cooler dust floating further out in the ring and arms are in the redder regions. The data were taken on August 25, 2004

PIX4608941

Atlantis moored the space station 07/2011 - Atlantis docked to the International Space station 07/2011 - The International Space Station (ISS) seen on 12 July 2011 by astronaut Ron Garan during his release into space. Two ships are moored at the station, the shuttle Atlantis visible on the right, and a Soyuz ship on the left. At the center of the AMS (Alpha Magnetic Spectrometer) experiment for the study of cosmic rays. Mission STS-135, the last United States space shuttle mission. This picture, photographed by NASA astronaut Ron Garan during the spacewalk conducted on July 12, 2011, shows the International Space Station with space shuttle Atlantis docked at right and a Russian Soyuz docked to Pirs, below the sun at far left. In the center foreground is the Alpha Magnetic Spectrometer (AMS) experiment installed during the STS - 134 mission. AMS is a state - of - the - art particle physics detector designed to use the unique environment of space to advance knowledge of the universe and

Atlantis moored the space station 07/2011 - Atlantis docked to the International Space station 07/2011 - The International Space Station (ISS) seen on 12 July 2011 by astronaut Ron Garan during his release into space. Two ships are moored at the station, the shuttle Atlantis visible on the right, and a Soyuz ship on the left. At the center of the AMS (Alpha Magnetic Spectrometer) experiment for the study of cosmic rays. Mission STS-135, the last United States space shuttle mission. This picture, photographed by NASA astronaut Ron Garan during the spacewalk conducted on July 12, 2011, shows the International Space Station with space shuttle Atlantis docked at right and a Russian Soyuz docked to Pirs, below the sun at far left. In the center foreground is the Alpha Magnetic Spectrometer (AMS) experiment installed during the STS - 134 mission. AMS is a state - of - the - art particle physics detector designed to use the unique environment of space to advance knowledge of the universe and

PIX4649824

Thailand: The karst limestone peaks of Khao Sok National Park, Surat Thani Province

Thailand: The karst limestone peaks of Khao Sok National Park, Surat Thani Province

David Henley

PFH2839121

Thailand: The karst limestone peaks of Khao Sok National Park, Surat Thani Province

Thailand: The karst limestone peaks of Khao Sok National Park, Surat Thani Province

David Henley

PFH2839124

Thailand: The karst limestone peaks of Khao Sok National Park, Surat Thani Province

Thailand: The karst limestone peaks of Khao Sok National Park, Surat Thani Province

David Henley

PFH2839125

Satellite Sentinel - 2 - Artist's view - Artist's view of the European satellite Sentinel - 2 in orbit around the Earth. This Earth observation satellite of the European programme Copernicus observes vegetation with a resolution of 10 m to 60 m, in thirteen spectral bands ranging from visible to infrared. Sentinel - 2A was launched on June 23, 2015 and Sentinel - 2B will be launched in 2016. Sentinel - 2 carries a high - resolution multispectral optical imager to monitor changes in vegetation for Europe's environmental monitoring Copernicus programme. This mission offers key information to optimise crop yield, thus helping to improve food security. Data can be used to measure leaf area index, leaf chlorophyll and leaf water content to monitor plant growth, which is particularly important during the growing season. It will be used to generate land - cover maps, to track changes in the way land is being used and to monitor the world's forests. In addition, Sentinel-2 provides information

Satellite Sentinel - 2 - Artist's view - Artist's view of the European satellite Sentinel - 2 in orbit around the Earth. This Earth observation satellite of the European programme Copernicus observes vegetation with a resolution of 10 m to 60 m, in thirteen spectral bands ranging from visible to infrared. Sentinel - 2A was launched on June 23, 2015 and Sentinel - 2B will be launched in 2016. Sentinel - 2 carries a high - resolution multispectral optical imager to monitor changes in vegetation for Europe's environmental monitoring Copernicus programme. This mission offers key information to optimise crop yield, thus helping to improve food security. Data can be used to measure leaf area index, leaf chlorophyll and leaf water content to monitor plant growth, which is particularly important during the growing season. It will be used to generate land - cover maps, to track changes in the way land is being used and to monitor the world's forests. In addition, Sentinel-2 provides information

PIX4644343

Satellite Sentinel - 2 - Artist's view - Artist's view of the European satellite Sentinel - 2 in orbit around the Earth. This Earth observation satellite of the European programme Copernicus observes vegetation with a resolution of 10 m to 60 m, in thirteen spectral bands ranging from visible to infrared. Sentinel - 2A was launched on June 23, 2015 and Sentinel - 2B will be launched in 2016. Sentinel - 2 carries a high - resolution multispectral optical imager to monitor changes in vegetation for Europe's environmental monitoring Copernicus programme. This mission offers key information to optimise crop yield, thus helping to improve food security. Data can be used to measure leaf area index, leaf chlorophyll and leaf water content to monitor plant growth, which is particularly important during the growing season. It will be used to generate land - cover maps, to track changes in the way land is being used and to monitor the world's forests. In addition, Sentinel-2 provides information

Satellite Sentinel - 2 - Artist's view - Artist's view of the European satellite Sentinel - 2 in orbit around the Earth. This Earth observation satellite of the European programme Copernicus observes vegetation with a resolution of 10 m to 60 m, in thirteen spectral bands ranging from visible to infrared. Sentinel - 2A was launched on June 23, 2015 and Sentinel - 2B will be launched in 2016. Sentinel - 2 carries a high - resolution multispectral optical imager to monitor changes in vegetation for Europe's environmental monitoring Copernicus programme. This mission offers key information to optimise crop yield, thus helping to improve food security. Data can be used to measure leaf area index, leaf chlorophyll and leaf water content to monitor plant growth, which is particularly important during the growing season. It will be used to generate land - cover maps, to track changes in the way land is being used and to monitor the world's forests. In addition, Sentinel-2 provides information

PIX4644423

IWorker with Ion horizontal loading machine in the reactor, HInkley Point

IWorker with Ion horizontal loading machine in the reactor, HInkley Point

UIS5075292

Desplittering machine in the reactor (reacteur nucleaire) showing handling of nuclear rods

Desplittering machine in the reactor (reacteur nucleaire) showing handling of nuclear rods

UIS5075284

Satellite Sentinel-2 - Artist's view: Artist's view of the European Sentinel-2 satellite orbiting the Earth. This Earth observation satellite of the European programme Copernicus observes vegetation with a resolution of 10 m to 60 m, in thirteen spectral bands ranging from visible to infrared. Sentinel-2A was launched on 23 June 2015 and Sentinel-2B will be launched in 2016 - Sentinel-2 carries a high-resolution multispectral optical imager to monitor changes in vegetation for Europe's environmental monitoring Copernicus programme. This mission offers key information to optimise crop yield, thus helping to improve food security. Data can be used to measure leaf area index, leaf chlorophyll and leaf water content to monitor plant growth, which is particularly important during the growing season. It will be used to generate land-cover maps, to track changes in the way land is being used and to monitor the world's forests. In addition, Sentinel-2 provides information on pollution in lakes

Satellite Sentinel-2 - Artist's view: Artist's view of the European Sentinel-2 satellite orbiting the Earth. This Earth observation satellite of the European programme Copernicus observes vegetation with a resolution of 10 m to 60 m, in thirteen spectral bands ranging from visible to infrared. Sentinel-2A was launched on 23 June 2015 and Sentinel-2B will be launched in 2016 - Sentinel-2 carries a high-resolution multispectral optical imager to monitor changes in vegetation for Europe's environmental monitoring Copernicus programme. This mission offers key information to optimise crop yield, thus helping to improve food security. Data can be used to measure leaf area index, leaf chlorophyll and leaf water content to monitor plant growth, which is particularly important during the growing season. It will be used to generate land-cover maps, to track changes in the way land is being used and to monitor the world's forests. In addition, Sentinel-2 provides information on pollution in lakes

PIX4644364

Thailand: Cheow Lan Lake (Rajjaprabha Dam Reservoir), Khao Sok National Park, Surat Thani Province

Thailand: Cheow Lan Lake (Rajjaprabha Dam Reservoir), Khao Sok National Park, Surat Thani Province

David Henley

PFH2839100

Thailand: Cheow Lan Lake (Rajjaprabha Dam Reservoir), Khao Sok National Park, Surat Thani Province

Thailand: Cheow Lan Lake (Rajjaprabha Dam Reservoir), Khao Sok National Park, Surat Thani Province

David Henley

PFH2839104

Thailand: Cheow Lan Lake (Rajjaprabha Dam Reservoir), Khao Sok National Park, Surat Thani Province

Thailand: Cheow Lan Lake (Rajjaprabha Dam Reservoir), Khao Sok National Park, Surat Thani Province

David Henley

PFH2839106

Thailand: Cheow Lan Lake (Rajjaprabha Dam Reservoir), Khao Sok National Park, Surat Thani Province

Thailand: Cheow Lan Lake (Rajjaprabha Dam Reservoir), Khao Sok National Park, Surat Thani Province

David Henley

PFH2839107

Thailand: Boats on Cheow Lan Lake (Rajjaprabha Dam Reservoir), Khao Sok National Park, Surat Thani Province

Thailand: Boats on Cheow Lan Lake (Rajjaprabha Dam Reservoir), Khao Sok National Park, Surat Thani Province

David Henley

PFH2839117

Thailand: Cheow Lan Lake (Rajjaprabha Dam Reservoir), Khao Sok National Park, Surat Thani Province

Thailand: Cheow Lan Lake (Rajjaprabha Dam Reservoir), Khao Sok National Park, Surat Thani Province

David Henley

PFH2839105

Thailand: Cheow Lan Lake (Rajjaprabha Dam Reservoir), Khao Sok National Park, Surat Thani Province

Thailand: Cheow Lan Lake (Rajjaprabha Dam Reservoir), Khao Sok National Park, Surat Thani Province

David Henley

PFH2839101

Thailand: Cheow Lan Lake (Rajjaprabha Dam Reservoir), Khao Sok National Park, Surat Thani Province

Thailand: Cheow Lan Lake (Rajjaprabha Dam Reservoir), Khao Sok National Park, Surat Thani Province

David Henley

PFH2839103

Apollo 17: experience LEAM - The Lunar Ejecta and Meteorite (LEAM) experiment - Apollo 17 - LEAM (white box in the foreground) is the acronym for Lunar Ejecta And Meteorites; this instrument was installed by astronauts of the Apollo 17 mission to study dust ejected by meteorite impacts on the surface of the Moon. The Lunar Ejecta and Meteorite (LEAM) instrument as deployed at the Apollo 17 ALSEP site. The central station is directly behind it, the RTG to the right of that, and the Lunar Surface Gravimeter (LSG) to the left of the central station. Discarded pallets and trash are also visible. The North Massif dominates the right side of the picture. The objectives of the LEAM experiment were to detect secondary particles that had been ejected by meteorite impacts on the lunar surface and to detect primary micrometeorites themselves. The 3 classes of particles encountered by the LEAM included lunar ejecta, interstellar grains, and cometary debris, all of which can be considered under the

Apollo 17: experience LEAM - The Lunar Ejecta and Meteorite (LEAM) experiment - Apollo 17 - LEAM (white box in the foreground) is the acronym for Lunar Ejecta And Meteorites; this instrument was installed by astronauts of the Apollo 17 mission to study dust ejected by meteorite impacts on the surface of the Moon. The Lunar Ejecta and Meteorite (LEAM) instrument as deployed at the Apollo 17 ALSEP site. The central station is directly behind it, the RTG to the right of that, and the Lunar Surface Gravimeter (LSG) to the left of the central station. Discarded pallets and trash are also visible. The North Massif dominates the right side of the picture. The objectives of the LEAM experiment were to detect secondary particles that had been ejected by meteorite impacts on the lunar surface and to detect primary micrometeorites themselves. The 3 classes of particles encountered by the LEAM included lunar ejecta, interstellar grains, and cometary debris, all of which can be considered under the

PIX4597805

Thailand: Cheow Lan Lake (Rajjaprabha Dam Reservoir), Khao Sok National Park, Surat Thani Province

Thailand: Cheow Lan Lake (Rajjaprabha Dam Reservoir), Khao Sok National Park, Surat Thani Province

David Henley

PFH2839102

Thailand: Cheow Lan Lake (Rajjaprabha Dam Reservoir), Khao Sok National Park, Surat Thani Province

Thailand: Cheow Lan Lake (Rajjaprabha Dam Reservoir), Khao Sok National Park, Surat Thani Province

David Henley

PFH2839108

Galaxies clusters Abell 370 - Abell 370 cluster of galaxies with gravitational arcs - This cluster of galaxies is located about 5 billion years away from Earth. This image obtained by the Hubble Space Telescope on July 16, 2009 shows gravitational arcs among galaxies. These mirages are deformed images of farther galaxies located behind the cluster. The NASA/ESA Hubble Space Telescope's newly repaired Advanced Camera for Surveys (ACS) has peered across almost five billion light - years to resolve intricate details in the galaxy cluster Abell 370. Abell 370 is one of the very first galaxy clusters where astronomers observed the phenomenon of gravitational lensing, the warping of space - time by the cluster's gravitational field that distorts the light from galaxies lying far behind it. This is manifested as arcs and streaks in the picture, which are the stretched images of background galaxies. Gravitational lensing is a vital tool for astronomers when measuring the dark matter distributi

Galaxies clusters Abell 370 - Abell 370 cluster of galaxies with gravitational arcs - This cluster of galaxies is located about 5 billion years away from Earth. This image obtained by the Hubble Space Telescope on July 16, 2009 shows gravitational arcs among galaxies. These mirages are deformed images of farther galaxies located behind the cluster. The NASA/ESA Hubble Space Telescope's newly repaired Advanced Camera for Surveys (ACS) has peered across almost five billion light - years to resolve intricate details in the galaxy cluster Abell 370. Abell 370 is one of the very first galaxy clusters where astronomers observed the phenomenon of gravitational lensing, the warping of space - time by the cluster's gravitational field that distorts the light from galaxies lying far behind it. This is manifested as arcs and streaks in the picture, which are the stretched images of background galaxies. Gravitational lensing is a vital tool for astronomers when measuring the dark matter distributi

PIX4565651

Barree spiral galaxy NGC 4639 in Virgo - Barred galaxy NGC 4639 in Virgo - The barree spiral galaxy NGC 4639 is located 78 million years - light in the Virgin's galaxy cluster. The blue dots visible on this image obtained by the Hubble Space Telescope are young stars. Other stars, cepheides have also been observed in this galaxy, allowing us to measure their distance with precision. This Hubble Space Telescope image shows NGC 4639, a spiral galaxy located 78 million light - years away in the Virgo cluster of galaxies. The blue dots in the galaxy's outlying regions indicate the presence of young stars. Among them are older, bright stars called Cepheids, which are used as reliable milepost markers to obtain accurate distances to nearby galaxies. Astronomers measure the brightness of Cepheids to calculate the distance to a galaxy. After using Cepheids to calculate the distance to NGC 4639, the team compared the results to the peak brightness measurements of SN 1990N, a type Ia supernova l

Barree spiral galaxy NGC 4639 in Virgo - Barred galaxy NGC 4639 in Virgo - The barree spiral galaxy NGC 4639 is located 78 million years - light in the Virgin's galaxy cluster. The blue dots visible on this image obtained by the Hubble Space Telescope are young stars. Other stars, cepheides have also been observed in this galaxy, allowing us to measure their distance with precision. This Hubble Space Telescope image shows NGC 4639, a spiral galaxy located 78 million light - years away in the Virgo cluster of galaxies. The blue dots in the galaxy's outlying regions indicate the presence of young stars. Among them are older, bright stars called Cepheids, which are used as reliable milepost markers to obtain accurate distances to nearby galaxies. Astronomers measure the brightness of Cepheids to calculate the distance to a galaxy. After using Cepheids to calculate the distance to NGC 4639, the team compared the results to the peak brightness measurements of SN 1990N, a type Ia supernova l

PIX4611731

Spiral galaxy NGC 3370 in the Lion - Spiral galaxy NGC 3370 in Leo - The spiral galaxy NGC 3370 is located about 100 million years away - light from Earth. In November 1994, light emitting from a supernova type Ia, SN 1994ae, part of this galaxy, reached Earth. In this image taken by the Hubble space telescope in May 2003, this supernova is no longer detectable. On the other hand, the telescope was able to observe in this galaxy cepheides, variable stars used to accurately measure distances in the universe and calculate the rate of expansion of the universe. Many galaxies are visible in the background. The majestic dusty spiral, NGC 3370, looms in the foreground in this NASA Hubble Space Telescope image. Recent observations taken with the Advanced Camera for Surveys show intricate spiral arm structure spotted with hot areas of new star formation. In November 1994, the light of a supernova in nearby NGC 3370 reached Earth. This stellar outburst briefly outshone all of the tens of billio

Spiral galaxy NGC 3370 in the Lion - Spiral galaxy NGC 3370 in Leo - The spiral galaxy NGC 3370 is located about 100 million years away - light from Earth. In November 1994, light emitting from a supernova type Ia, SN 1994ae, part of this galaxy, reached Earth. In this image taken by the Hubble space telescope in May 2003, this supernova is no longer detectable. On the other hand, the telescope was able to observe in this galaxy cepheides, variable stars used to accurately measure distances in the universe and calculate the rate of expansion of the universe. Many galaxies are visible in the background. The majestic dusty spiral, NGC 3370, looms in the foreground in this NASA Hubble Space Telescope image. Recent observations taken with the Advanced Camera for Surveys show intricate spiral arm structure spotted with hot areas of new star formation. In November 1994, the light of a supernova in nearby NGC 3370 reached Earth. This stellar outburst briefly outshone all of the tens of billio

PIX4610684

Spiral galaxy NGC 3370 in the Lion - Spiral galaxy NGC 3370 in Leo - The spiral galaxy NGC 3370 is located about 100 million years away - light from Earth. In November 1994, light emitting from a supernova type Ia, SN 1994ae, part of this galaxy, reached Earth. In this image taken by the Hubble space telescope in May 2003, this supernova is no longer detectable. On the other hand, the telescope was able to observe in this galaxy cepheides, variable stars used to accurately measure distances in the universe and calculate the rate of expansion of the universe. Many galaxies are visible in the background. The majestic dusty spiral, NGC 3370, looms in the foreground in this NASA Hubble Space Telescope image. Recent observations taken with the Advanced Camera for Surveys show intricate spiral arm structure spotted with hot areas of new star formation. In November 1994, the light of a supernova in nearby NGC 3370 reached Earth. This stellar outburst briefly outshone all of the tens of billio

Spiral galaxy NGC 3370 in the Lion - Spiral galaxy NGC 3370 in Leo - The spiral galaxy NGC 3370 is located about 100 million years away - light from Earth. In November 1994, light emitting from a supernova type Ia, SN 1994ae, part of this galaxy, reached Earth. In this image taken by the Hubble space telescope in May 2003, this supernova is no longer detectable. On the other hand, the telescope was able to observe in this galaxy cepheides, variable stars used to accurately measure distances in the universe and calculate the rate of expansion of the universe. Many galaxies are visible in the background. The majestic dusty spiral, NGC 3370, looms in the foreground in this NASA Hubble Space Telescope image. Recent observations taken with the Advanced Camera for Surveys show intricate spiral arm structure spotted with hot areas of new star formation. In November 1994, the light of a supernova in nearby NGC 3370 reached Earth. This stellar outburst briefly outshone all of the tens of billio

PIX4610713

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

Supernovae distant - These Hubble Space Telescope images pinpoint three distant supernovae, which exploded and died billions of years ago. Scientists are using these faraway light sources to estimate if the universe was expanding at a faster rate long ago and is now slowing down. Images of SN 1997cj are in the left hand column; SN 1997ce, in the middle; and SN 1997ck, on the right. All images were taken by the Hubble telescope's Wide Field and Planetary Camera 2. The top row of images are wider views of the supernovae. The supernovae were discovered in April 1997 in a ground - based survey at the Canada - France - Hawaii Telescope on Mauna Kea, Hawaii. Once the supernovae were discovered, the Hubble telescope was used to distinguish the supernovae from the light of their host galaxies. A series of Hubble telescope images were taken in May and June 1997 as the supernovae faded. Six Hubble telescope observations spanning five weeks were taken for each supernova. This time series enabled

Supernovae distant - These Hubble Space Telescope images pinpoint three distant supernovae, which exploded and died billions of years ago. Scientists are using these faraway light sources to estimate if the universe was expanding at a faster rate long ago and is now slowing down. Images of SN 1997cj are in the left hand column; SN 1997ce, in the middle; and SN 1997ck, on the right. All images were taken by the Hubble telescope's Wide Field and Planetary Camera 2. The top row of images are wider views of the supernovae. The supernovae were discovered in April 1997 in a ground - based survey at the Canada - France - Hawaii Telescope on Mauna Kea, Hawaii. Once the supernovae were discovered, the Hubble telescope was used to distinguish the supernovae from the light of their host galaxies. A series of Hubble telescope images were taken in May and June 1997 as the supernovae faded. Six Hubble telescope observations spanning five weeks were taken for each supernova. This time series enabled

PIX4583191

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