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Fig. 7 from 'A New Theory of the Earth' by William Whisten, London, 1696 (engraving)

Fig. 7 from 'A New Theory of the Earth' by William Whisten, London, 1696 (engraving)

English School, (17th century)

NCO833817

This panel illustrates the transit of the martian moon Phobos across the Sun.

This panel illustrates the transit of the martian moon Phobos across the Sun.

UIG866431

ISS: modules Unity, Zarya and Zvezda 10/2000 - ISS: modules Unity, Zarya and Zvezda 10/2000 - The international space station shortly before docking with the shuttle Discovery. 12/10/2000. Not long before the link - up of the Space Shuttle Discovery and the International Space Station (ISS), a crew member onboard the shuttle used a handheld 70 mm camera to grab this image of the station. Backdropped against the blackness of space, all the current elements are visible, though this particular angle makes them difficult to delineate. Nearest the camera is the Progress supply ship, attached to the service module or Zvezda, which connects to the functional cargo block (FGB) or Zarya. At the top or far end in this vew is the U.S. - built Unity Node 1. Once the STS - 92 crew completed its work, the addition of the Z1 Truss and a third pressurized mating adapter changed the appearance considerably. Oct 12 2000

ISS: modules Unity, Zarya and Zvezda 10/2000 - ISS: modules Unity, Zarya and Zvezda 10/2000 - The international space station shortly before docking with the shuttle Discovery. 12/10/2000. Not long before the link - up of the Space Shuttle Discovery and the International Space Station (ISS), a crew member onboard the shuttle used a handheld 70 mm camera to grab this image of the station. Backdropped against the blackness of space, all the current elements are visible, though this particular angle makes them difficult to delineate. Nearest the camera is the Progress supply ship, attached to the service module or Zvezda, which connects to the functional cargo block (FGB) or Zarya. At the top or far end in this vew is the U.S. - built Unity Node 1. Once the STS - 92 crew completed its work, the addition of the Z1 Truss and a third pressurized mating adapter changed the appearance considerably. Oct 12 2000

PIX4599996

ISS: Progress ship. 11/2000 - Progress supply ship. 11/2000 - Progress ship, with 2 tons of cargo on board for Expedition 1, approaching the International Space Station (ISS). 11/2000. A Progress supply ship linked up to the orbiting International Space Station (ISS) at 3:48 GMT, November 18, bringing Expedition 1 commander William M. Shepherd, pilot Yuri P. Gidzenko and flight engineer Sergei K. Krikalev two tons of food, clothing, hardware and holiday gifts from their families. The photograph was taken with a 35 mm camera and the film was later handed over to the STS - 97 crew members for return to Earth and subsequent processing. Nov 2000

ISS: Progress ship. 11/2000 - Progress supply ship. 11/2000 - Progress ship, with 2 tons of cargo on board for Expedition 1, approaching the International Space Station (ISS). 11/2000. A Progress supply ship linked up to the orbiting International Space Station (ISS) at 3:48 GMT, November 18, bringing Expedition 1 commander William M. Shepherd, pilot Yuri P. Gidzenko and flight engineer Sergei K. Krikalev two tons of food, clothing, hardware and holiday gifts from their families. The photograph was taken with a 35 mm camera and the film was later handed over to the STS - 97 crew members for return to Earth and subsequent processing. Nov 2000

PIX4600062

Mars Recognition Orbiter and the Comet, Artist view (photo)

Mars Recognition Orbiter and the Comet, Artist view (photo)

Steven Hobbs

PIX6039537

Rosetta probe: the Philae lander poses on the nucleus of the comet: The Rosetta probe was launched on 2 March 2004 to study comet 67P/Churyumov-Gerasimenko. His lander, Philae, landed on the surface of the comet on 12 November 2014 to analyze the composition of the nucleus of the comet - Artist's impression of Rosetta's lander Philae on the surface of comet 67P/Churyumov-Gerasimenko. Philae will be deployed to the comet in November 2014 where it will make in situ observations of the comet surface, including drilling 23 cm into the subsurface to extract material for analysis in its on board laboratory

Rosetta probe: the Philae lander poses on the nucleus of the comet: The Rosetta probe was launched on 2 March 2004 to study comet 67P/Churyumov-Gerasimenko. His lander, Philae, landed on the surface of the comet on 12 November 2014 to analyze the composition of the nucleus of the comet - Artist's impression of Rosetta's lander Philae on the surface of comet 67P/Churyumov-Gerasimenko. Philae will be deployed to the comet in November 2014 where it will make in situ observations of the comet surface, including drilling 23 cm into the subsurface to extract material for analysis in its on board laboratory

Miller, Ron (b.1947)

PIX4643682

Rosetta probe: the Philae lander landed on the nucleus of the comet - The Rosetta lander on a comet nucleus - The Rosetta probe was launched on 2 March 2004 to study comet 67P/Churyumov - Gerasimenko. His lander, Philae, landed on the surface of the comet on November 12, 2014 to analyze the composition of the comet's nucleus. Still image from animation of Philae separating from Rosetta and descending to the surface of comet 67P/Churyumov - Gerasimenko in November 2014

Rosetta probe: the Philae lander landed on the nucleus of the comet - The Rosetta lander on a comet nucleus - The Rosetta probe was launched on 2 March 2004 to study comet 67P/Churyumov - Gerasimenko. His lander, Philae, landed on the surface of the comet on November 12, 2014 to analyze the composition of the comet's nucleus. Still image from animation of Philae separating from Rosetta and descending to the surface of comet 67P/Churyumov - Gerasimenko in November 2014

PIX4607170

Total solar eclipse - 29/03/2006 - Turkey - Total solar eclipse - Turkey - March 29 2006 - Total solar eclipse seen on 29/03/2006 in Turkey. Total solar eclipse - Turkey - March 29, 200

Total solar eclipse - 29/03/2006 - Turkey - Total solar eclipse - Turkey - March 29 2006 - Total solar eclipse seen on 29/03/2006 in Turkey. Total solar eclipse - Turkey - March 29, 200

Sebastian Voltmer

PIX4627990

The Solar Eclipse as seen from the Isle of Dogs on Monday Last (engraving)

The Solar Eclipse as seen from the Isle of Dogs on Monday Last (engraving)

English School, (19th century)

LIP1609426

The Phoenix probe on its landing site - Phoenix landing site - Mosaic of polar projection images showing the Phoenix probe placed on Martian soil. The black circle corresponds to the position of the probe camera. The hundreds of clicks needed to make this image were taken between June 5 and July 12, 2008. Phoenix landed on a vast plain north of Mars, in the Vastitas Borealis region. This view is a polar projection that combines more than 500 exposures taken by the Surface Stereo Imager camera on Nasa's Mars Phoenix Lander and projects them as if looking down from above. The black circle on the spacecraft is where the camera itself is mounted on the lander, out of view in images taken by the camera. North is toward the top of the image. The lander's meteorology mast extends above the southwest horzon and is topped by the telltale wind gauge. The ground surface around the lander has polygonal patterning similar to patterns in permafrost areas on Earth. The landing site is at 68.22 degree

The Phoenix probe on its landing site - Phoenix landing site - Mosaic of polar projection images showing the Phoenix probe placed on Martian soil. The black circle corresponds to the position of the probe camera. The hundreds of clicks needed to make this image were taken between June 5 and July 12, 2008. Phoenix landed on a vast plain north of Mars, in the Vastitas Borealis region. This view is a polar projection that combines more than 500 exposures taken by the Surface Stereo Imager camera on Nasa's Mars Phoenix Lander and projects them as if looking down from above. The black circle on the spacecraft is where the camera itself is mounted on the lander, out of view in images taken by the camera. North is toward the top of the image. The lander's meteorology mast extends above the southwest horzon and is topped by the telltale wind gauge. The ground surface around the lander has polygonal patterning similar to patterns in permafrost areas on Earth. The landing site is at 68.22 degree

PIX4616696

The Rosetta spacecraft releases a lander onto a comet nucleus - The Rosetta spacecraft releases a lander onto a comet nucleus - The Rosetta probe was launched on 2 March 2004 to study comet 67P/Churyumov - Gerasimenko. Artist's view of the Philae probe and lander near the nucleus of the comet. The size scales are not respected, the probe measures 32 meters with its panels deployed, the core of the comet about 4 km. Artist's impression of the Rosetta orbiter deploying the Philae lander to comet 67P/Churyumov - Gerasimenko. The image is not to scale; the Rosetta spacecraft measures 32 m across including the solar arrays, while the comet nucleus is thought to be about 4 km wide

The Rosetta spacecraft releases a lander onto a comet nucleus - The Rosetta spacecraft releases a lander onto a comet nucleus - The Rosetta probe was launched on 2 March 2004 to study comet 67P/Churyumov - Gerasimenko. Artist's view of the Philae probe and lander near the nucleus of the comet. The size scales are not respected, the probe measures 32 meters with its panels deployed, the core of the comet about 4 km. Artist's impression of the Rosetta orbiter deploying the Philae lander to comet 67P/Churyumov - Gerasimenko. The image is not to scale; the Rosetta spacecraft measures 32 m across including the solar arrays, while the comet nucleus is thought to be about 4 km wide

PIX4607171

Comparison between Earth, Mercury and the Moon - Earth, Mercury, and Earth's Moon compared - Comparison at the scale of the Earth's size, the planet Mercury and the Moon. The diameter of Mercury is about one third of that of the Earth. Mercury is a little larger than the Earth's Moon and is believed to be composed mostly of iron and rock, making it considerably denser than the Moon. Mercury also has a magnetic field about 1% as strong as the Earth's. Mercury's diameter is only one third that of the Earth's. It has only 6% the mass. If you weigh 180 pounds on the Earth, you would weigh 64 pounds on Mercury. Is only one-third the Earth's distance from the Su

Comparison between Earth, Mercury and the Moon - Earth, Mercury, and Earth's Moon compared - Comparison at the scale of the Earth's size, the planet Mercury and the Moon. The diameter of Mercury is about one third of that of the Earth. Mercury is a little larger than the Earth's Moon and is believed to be composed mostly of iron and rock, making it considerably denser than the Moon. Mercury also has a magnetic field about 1% as strong as the Earth's. Mercury's diameter is only one third that of the Earth's. It has only 6% the mass. If you weigh 180 pounds on the Earth, you would weigh 64 pounds on Mercury. Is only one-third the Earth's distance from the Su

Walter B Myers

PIX4629901

Solar column - Solar pillar - A solar column is created by the reflection of solar light on the horizontal faces of ice crystals. It therefore requires a fairly stable atmosphere to keep these crystals parallel to the horizon. 16 June 2006, Finistere. A solar pillar is created by the reflection a sunlight (when sun is at or low to the horizon) on the horizontal face of ice cristals. So, a quiet atmosphere is needed in order that this cristals stay parallel to the horizon. June 16 2006, Brittany, France

Solar column - Solar pillar - A solar column is created by the reflection of solar light on the horizontal faces of ice crystals. It therefore requires a fairly stable atmosphere to keep these crystals parallel to the horizon. 16 June 2006, Finistere. A solar pillar is created by the reflection a sunlight (when sun is at or low to the horizon) on the horizontal face of ice cristals. So, a quiet atmosphere is needed in order that this cristals stay parallel to the horizon. June 16 2006, Brittany, France

Laurent Laveder

PIX4671499

The International Space Station (ISS) - Anaglyph - The International Space Station (ISS) - Anaglyph - Relief view of the International Space Station (ISS) with the European Columbus module. This image shows the International Space Station with the european laboratory Columbus

The International Space Station (ISS) - Anaglyph - The International Space Station (ISS) - Anaglyph - Relief view of the International Space Station (ISS) with the European Columbus module. This image shows the International Space Station with the european laboratory Columbus

D. Ducros

PIX4603661

Eureca Satellite - The Eureca satellite flies to space after it was deployed by the Atlantis space shuttle on 31 July 1992. The moon is visible. The European Retrievable Carrier 1L (EURECA - 1L) spacecraft, with solar array panels extended, drifts in space after deployment from the payload bay of Atlantis, Orbiter Vehicle (OV) 104, during STS - 46. The moon appears in this image

Eureca Satellite - The Eureca satellite flies to space after it was deployed by the Atlantis space shuttle on 31 July 1992. The moon is visible. The European Retrievable Carrier 1L (EURECA - 1L) spacecraft, with solar array panels extended, drifts in space after deployment from the payload bay of Atlantis, Orbiter Vehicle (OV) 104, during STS - 46. The moon appears in this image

PIX4646301

Lunar base -Illustration - Lunar base - Illustration - An international lunar base in 2025 - View of artist International lunar base in 2025 - Artist vie

Lunar base -Illustration - Lunar base - Illustration - An international lunar base in 2025 - View of artist International lunar base in 2025 - Artist vie

P. Carril

PIX4638809

Mars Polar Lander - Artist view - Mars Polar Lander spaceprobe - Artist view - The American Mars Polar Lander probe, launched on January 3, 1999, was scheduled to land in December 1999 near the southern polar cap of Mars. Contact with the probe was interrupted on 3 December 1999, when it entered the Martian atmosphere. The Mars Polar Lander is shown on the surface of Mars. The spacecraft was launched in january 1999 to Mars to land near the southern polar cap in December 1999 and carry out a three - month mission to search for traces of subsurface water in this frozen, layered terrain. The contact with the spacecraft was lost on December 9, 1999, shortly after it entered the Martian atmosphere

Mars Polar Lander - Artist view - Mars Polar Lander spaceprobe - Artist view - The American Mars Polar Lander probe, launched on January 3, 1999, was scheduled to land in December 1999 near the southern polar cap of Mars. Contact with the probe was interrupted on 3 December 1999, when it entered the Martian atmosphere. The Mars Polar Lander is shown on the surface of Mars. The spacecraft was launched in january 1999 to Mars to land near the southern polar cap in December 1999 and carry out a three - month mission to search for traces of subsurface water in this frozen, layered terrain. The contact with the spacecraft was lost on December 9, 1999, shortly after it entered the Martian atmosphere

PIX4606673

Sun observation with protective glasses - Sun observation with safe solar glasse

Sun observation with protective glasses - Sun observation with safe solar glasse

Sebastien Beaucourt

PIX4567369

Eclipse de Soleil 20/03/2015 - Svalbard - Solar Eclipse - March 20 2015 - Svalbard - Total Eclipse of Sun 20 March 2015 seen near Longyearbyen on the island of Spitzberg in the Svalbard archipelago. March 20 2015 total solar eclipse seen from Longyearbyen on the island of Spitsbergen in the Svalbard archipelago east of northern Greenland

Eclipse de Soleil 20/03/2015 - Svalbard - Solar Eclipse - March 20 2015 - Svalbard - Total Eclipse of Sun 20 March 2015 seen near Longyearbyen on the island of Spitzberg in the Svalbard archipelago. March 20 2015 total solar eclipse seen from Longyearbyen on the island of Spitsbergen in the Svalbard archipelago east of northern Greenland

PIX4628413

A three-dimensional image of the Sun. STEREO. This image is a composite of left and right eye color image pairs taken by the SECCHI Extreme UltraViolet Imager.

A three-dimensional image of the Sun. STEREO. This image is a composite of left and right eye color image pairs taken by the SECCHI Extreme UltraViolet Imager.

UIG866460

The international space station seen from the space shuttle Discovery - ISS seen from the space shuttle Discovery during undocking - The international space station (ISS) seen during the mooring maneuvers from the space shuttle Discovery. 10/2000. A farewell snapshot of the International Space Station (ISS) was captured with a 35 mm camera through the Space Shuttle Discovery's crew optical alignment system during separation operations. Discoloration of the station is associated with the COAS. This edge - on image reveals the newest additions to the station, with the Z1 Truss structure on top and the third pressurized mating adapter on bottom in this angle

The international space station seen from the space shuttle Discovery - ISS seen from the space shuttle Discovery during undocking - The international space station (ISS) seen during the mooring maneuvers from the space shuttle Discovery. 10/2000. A farewell snapshot of the International Space Station (ISS) was captured with a 35 mm camera through the Space Shuttle Discovery's crew optical alignment system during separation operations. Discoloration of the station is associated with the COAS. This edge - on image reveals the newest additions to the station, with the Z1 Truss structure on top and the third pressurized mating adapter on bottom in this angle

PIX4600002

Mars Polar Lander - Artist view - Mars Polar Lander spaceprobe - Artist view - The American Mars Polar Lander probe, launched on January 3, 1999, was scheduled to land in December 1999 near the southern polar cap of Mars. Contact with the probe was interrupted on 3 December 1999, when it entered the Martian atmosphere. The Mars Polar Lander is shown on the surface of Mars. The spacecraft was launched in january 1999 to Mars to land near the southern polar cap in December 1999 and carry out a three - month mission to search for traces of subsurface water in this frozen, layered terrain. The contact with the spacecraft was lost on December 9, 1999, shortly after it entered the Martian atmosphere

Mars Polar Lander - Artist view - Mars Polar Lander spaceprobe - Artist view - The American Mars Polar Lander probe, launched on January 3, 1999, was scheduled to land in December 1999 near the southern polar cap of Mars. Contact with the probe was interrupted on 3 December 1999, when it entered the Martian atmosphere. The Mars Polar Lander is shown on the surface of Mars. The spacecraft was launched in january 1999 to Mars to land near the southern polar cap in December 1999 and carry out a three - month mission to search for traces of subsurface water in this frozen, layered terrain. The contact with the spacecraft was lost on December 9, 1999, shortly after it entered the Martian atmosphere

PIX4606692

Bepicolombo will be a mission to explore the planet Mercury, carried out jointly by the Japanese Space Agency and the European Space Agency. Its launch is scheduled in October 2018, to reach Mercure in 2025. Two probes form the Bepicolombo mission, the Mercury Planet Orbiter (DFO), which will perform a complete mapping of the surface of Mercury and the Mercury Magnetospheric Orbiter (MMO), which will study the Mercurian magnetosphere.

Bepicolombo will be a mission to explore the planet Mercury, carried out jointly by the Japanese Space Agency and the European Space Agency. Its launch is scheduled in October 2018, to reach Mercure in 2025. Two probes form the Bepicolombo mission, the Mercury Planet Orbiter (DFO), which will perform a complete mapping of the surface of Mercury and the Mercury Magnetospheric Orbiter (MMO), which will study the Mercurian magnetosphere.

PIX4643573

The Hayabusa and Itokawa probe - Hayabusa spacecraft near the asteroid Itokawa: Artist's view of the Hayabusa probe near the asteroid Itokawa. The Japanese probe Hayabusa (MUSES-C) was launched on 9 May 2003 to reach the asteroid 25143 Itokawa in September 2005 and to take samples from it. His return to Earth took place in June 2010

The Hayabusa and Itokawa probe - Hayabusa spacecraft near the asteroid Itokawa: Artist's view of the Hayabusa probe near the asteroid Itokawa. The Japanese probe Hayabusa (MUSES-C) was launched on 9 May 2003 to reach the asteroid 25143 Itokawa in September 2005 and to take samples from it. His return to Earth took place in June 2010

Miller, Ron (b.1947)

PIX4643666

Comparison of Earth Sizes, Venus, Mercure and Mars - Planetary-size comparison: Earth, Venus, Mercury and Mars - Earth diameter: 12 756,28 km Venus diameter: 12 100 km Mercury diameter: 4870 km March diameter: 6790 km Size comparison in diametric values: Earth: 12,756.28 km Venus: 12,100 km Mercury: 4,870 km March: 6,790 k

Comparison of Earth Sizes, Venus, Mercure and Mars - Planetary-size comparison: Earth, Venus, Mercury and Mars - Earth diameter: 12 756,28 km Venus diameter: 12 100 km Mercury diameter: 4870 km March diameter: 6790 km Size comparison in diametric values: Earth: 12,756.28 km Venus: 12,100 km Mercury: 4,870 km March: 6,790 k

PIX4629876

Le Soleil vu by SDO on March 30, 2010 - The Sun seen by SDO. March 30, 2010 - The Sun seen in ultraviolet by SDO (Solar Dynamics Observatory) on March 30, 2010. A full - disk extreme ultraviolet image of the sun taken by SDO (Solar Dynamics Observatory) on March 30, 2010

Le Soleil vu by SDO on March 30, 2010 - The Sun seen by SDO. March 30, 2010 - The Sun seen in ultraviolet by SDO (Solar Dynamics Observatory) on March 30, 2010. A full - disk extreme ultraviolet image of the sun taken by SDO (Solar Dynamics Observatory) on March 30, 2010

PIX4627163

Le Soleil vu par SDO on 16 April 2012 - The Sun seen by SDO - April 2012 - Le Soleil vu en ultraviolet by SDO (Solar Dynamics Observatory) on 16 April 2012 (17:44:21 UT). Image taken on April 16, 2012 (17:44:21 UT) by Solar Dynamics Observatory (SDO)

Le Soleil vu par SDO on 16 April 2012 - The Sun seen by SDO - April 2012 - Le Soleil vu en ultraviolet by SDO (Solar Dynamics Observatory) on 16 April 2012 (17:44:21 UT). Image taken on April 16, 2012 (17:44:21 UT) by Solar Dynamics Observatory (SDO)

PIX4627209

Le Soleil vu by SDO on 27 October 2014 - The Sun seen by SDO - October 27 2014 - Solar eruption (shining spot below right) seen by SDO (Solar Dynamics Observatory) on 27 October 2014. Nasa's Solar Dynamics Observatory captured this image of an X2.0-class solar flare bursting off the lower right side of the sun on Oct. 27, 2014. The image shows a blend of extreme ultraviolet light with wavelengths of 131 and 171 Angstroms.

Le Soleil vu by SDO on 27 October 2014 - The Sun seen by SDO - October 27 2014 - Solar eruption (shining spot below right) seen by SDO (Solar Dynamics Observatory) on 27 October 2014. Nasa's Solar Dynamics Observatory captured this image of an X2.0-class solar flare bursting off the lower right side of the sun on Oct. 27, 2014. The image shows a blend of extreme ultraviolet light with wavelengths of 131 and 171 Angstroms.

PIX4627266

Le Soleil vu par SDO on 12 January 2015 - The Sun seen by SDO - January 12 2015 - Solar eruption (bright spot on the right) seen by SDO (Solar Dynamics Observatory) on 12 January 2015. The sun emitted a mid-level solar flare, peaking at 11:24 p.m. EST on Jan. 12, 2015. Nasa's Solar Dynamics Observatory, which watches the sun constantly, captured an image of the event. Solar flares are powerful bursts of radiation. Harmful radiation from a flare cannot pass through Earth's atmosphere to physically affect humans on the ground, however - when intense enough - they can disturb the atmosphere in the layer where GPS and communications signals travel

Le Soleil vu par SDO on 12 January 2015 - The Sun seen by SDO - January 12 2015 - Solar eruption (bright spot on the right) seen by SDO (Solar Dynamics Observatory) on 12 January 2015. The sun emitted a mid-level solar flare, peaking at 11:24 p.m. EST on Jan. 12, 2015. Nasa's Solar Dynamics Observatory, which watches the sun constantly, captured an image of the event. Solar flares are powerful bursts of radiation. Harmful radiation from a flare cannot pass through Earth's atmosphere to physically affect humans on the ground, however - when intense enough - they can disturb the atmosphere in the layer where GPS and communications signals travel

PIX4627273

Khufu's Solar Boat on Display at the Solar Boat Museum, Giza, Al Jizah, Egypt (photo)

Khufu's Solar Boat on Display at the Solar Boat Museum, Giza, Al Jizah, Egypt (photo)

Peter Langer

UIG1568456

A three-dimensional image of the Sun. STEREO. This image is a composite of left and right eye color image pairs taken by the SECCHI Extreme UltraViolet Imager.

A three-dimensional image of the Sun. STEREO. This image is a composite of left and right eye color image pairs taken by the SECCHI Extreme UltraViolet Imager.

UIG866455

Earth Moon and the Sun - Earth Moon and Sun - Artist's view

Earth Moon and the Sun - Earth Moon and Sun - Artist's view

PIX4629778

Earth Moon and the Sun - Earth Moon and Sun - Artist's view

Earth Moon and the Sun - Earth Moon and Sun - Artist's view

PIX4629786

Dwarf planets - Dwarf planets Ceres, Pluto, and Eris compared - Comparison at the scale of dwarf planets. From left to right are represented Ceres, Pluto and Eris. Ceres was elevated from asteroid to the status of dwarf planet in 2006 when the International Astronomical Union (IAU) reviewed Pluto's status as the solar system's 9th planet. Pluto was subsequently demoted to dwarf planet. In this image, from left to right are the dwarf planets Ceres, Pluto, and Eris. Eris was discovered in 2003 and is now the largest of the known dwarf planets. It is believed to be slightly more massive than Pluto and follows a highly eccentric orbit that alternately brings it as close as the orbits of Neptune and Pluto and as far as over twice Pluto's furthest distance from the Sun. It was the discovery of Eris that prompted the re-evaluation of Pluto as a planet

Dwarf planets - Dwarf planets Ceres, Pluto, and Eris compared - Comparison at the scale of dwarf planets. From left to right are represented Ceres, Pluto and Eris. Ceres was elevated from asteroid to the status of dwarf planet in 2006 when the International Astronomical Union (IAU) reviewed Pluto's status as the solar system's 9th planet. Pluto was subsequently demoted to dwarf planet. In this image, from left to right are the dwarf planets Ceres, Pluto, and Eris. Eris was discovered in 2003 and is now the largest of the known dwarf planets. It is believed to be slightly more massive than Pluto and follows a highly eccentric orbit that alternately brings it as close as the orbits of Neptune and Pluto and as far as over twice Pluto's furthest distance from the Sun. It was the discovery of Eris that prompted the re-evaluation of Pluto as a planet

Walter B Myers

PIX4630042

Juno Probe - Solar Panels - Juno Solar Panels - View of the solar panels of the Juno probe in operation verification. Launched in 2011, the Juno probe will reach Jupiter in 2016. It will then hold the record for the farthest solar power probe ever sent. Technicians at Astrotech's payload processing facility in Titusville, Fla. stow solar array # 2 against the body of Nasa's Juno spacecraft. Launching from Earth in 2011, the Juno spacecraft will arrive at Jupiter in 2016 to study the giant planet from an elliptical, polar orbit. When Juno arrives at Jupiter in 2016, it will be farther from the sun than any previous solar powered mission. The choice of solar power for Juno necessitates very large solar arrays with dimensions of 2.65 meters wide by 8.9 meters long (about 9 feet wide by 29 feet long). Once in orbit at the giant planet, the three arrays will provide about 450 watts of electricity for Juno

Juno Probe - Solar Panels - Juno Solar Panels - View of the solar panels of the Juno probe in operation verification. Launched in 2011, the Juno probe will reach Jupiter in 2016. It will then hold the record for the farthest solar power probe ever sent. Technicians at Astrotech's payload processing facility in Titusville, Fla. stow solar array # 2 against the body of Nasa's Juno spacecraft. Launching from Earth in 2011, the Juno spacecraft will arrive at Jupiter in 2016 to study the giant planet from an elliptical, polar orbit. When Juno arrives at Jupiter in 2016, it will be farther from the sun than any previous solar powered mission. The choice of solar power for Juno necessitates very large solar arrays with dimensions of 2.65 meters wide by 8.9 meters long (about 9 feet wide by 29 feet long). Once in orbit at the giant planet, the three arrays will provide about 450 watts of electricity for Juno

PIX4605945

A building housing a horizontal solar tower as part of the Cambridge University observatories

A building housing a horizontal solar tower as part of the Cambridge University observatories

UIG3732354

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

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

Alex Conu

PIX4583396

Total Eclipse of Sun - Easter Island 11/07/2010 - Easter Island Total Solar Eclipse - July 11 2010 - Total Eclipse of Sun from 11 July 2010 seen on Easter Island. The total solar eclipse of 11 July 2010 seen in Easter Island

Total Eclipse of Sun - Easter Island 11/07/2010 - Easter Island Total Solar Eclipse - July 11 2010 - Total Eclipse of Sun from 11 July 2010 seen on Easter Island. The total solar eclipse of 11 July 2010 seen in Easter Island

PIX4628267

The Phoenix probe on its landing site - Phoenix landing site, vertical projection - Mosaic of images in vertical projection showing the Phoenix probe on Mars. The probe landed on a vast plain north of the planet in the Vastitas Borealis region. This view combines more than 400 images taken during the first several weeks after Nasa's Phoenix Mars Lander arrived on an arctic plain at 62.22 degrees north latitude, 234.25 degrees east longitude on Mars. The full - circle panorama in approximately true color shows the polygonal patterning of ground in the landing area, similar to patterns in permafrost areas on Earth. North is toward the top. Trenches where Phoenix's robotic arm has been exposing subsurface material are visible just north of the lander. This view includes more than 100 different camera pointings, with images taken through three different filters at each pointing. It is presented here as a vertical projection

The Phoenix probe on its landing site - Phoenix landing site, vertical projection - Mosaic of images in vertical projection showing the Phoenix probe on Mars. The probe landed on a vast plain north of the planet in the Vastitas Borealis region. This view combines more than 400 images taken during the first several weeks after Nasa's Phoenix Mars Lander arrived on an arctic plain at 62.22 degrees north latitude, 234.25 degrees east longitude on Mars. The full - circle panorama in approximately true color shows the polygonal patterning of ground in the landing area, similar to patterns in permafrost areas on Earth. North is toward the top. Trenches where Phoenix's robotic arm has been exposing subsurface material are visible just north of the lander. This view includes more than 100 different camera pointings, with images taken through three different filters at each pointing. It is presented here as a vertical projection

PIX4616646

Kepler's Law - Illustration - The segment that connects the planet to the Sun sweeps equal areas in equal times. In other words, the speed of a planet becomes greater when the planet approaches the Sun. It is maximum in the vicinity of the shortest radius (perihelie), and minimal in the vicinity of the largest radius (aphelie). Second Kepler's law, the line joining a planet and the Sun sweeps out equal areas during equal intervals of time. The planet moves faster near the Sun, so the same area is swept out in a given time as at larger distances, where the planet moves more slowl

Kepler's Law - Illustration - The segment that connects the planet to the Sun sweeps equal areas in equal times. In other words, the speed of a planet becomes greater when the planet approaches the Sun. It is maximum in the vicinity of the shortest radius (perihelie), and minimal in the vicinity of the largest radius (aphelie). Second Kepler's law, the line joining a planet and the Sun sweeps out equal areas during equal intervals of time. The planet moves faster near the Sun, so the same area is swept out in a given time as at larger distances, where the planet moves more slowl

Sebastien Beaucourt

PIX4629399

Solar panel, electrical motor and weight hanging by string

Solar panel, electrical motor and weight hanging by string

UDK844869

This composite image combines Extreme Ultravoilet Imaging Telescope (EIT) images from three wavelengths into one that reveals solar features of the Sun unique to each wavelength.

This composite image combines Extreme Ultravoilet Imaging Telescope (EIT) images from three wavelengths into one that reveals solar features of the Sun unique to each wavelength.

UIG866430

ATV Jules Verne - The Jules Verne ATV - View of the first European automatic cargo ship ATV christens Jules Verne, leaving the international space station on 5 September 2008. Designed to supply the station with various equipment, the ATV, with several tons of fuel on board, is used to bring the station back into its orbit. Jules Verne moored at the station on April 3, 2008. 5 Sept. 2008 - Backdropped by the blackness of space, European Space Agency's (ESA) “” Jules Verne”” Automated Transfer Vehicle (ATV) begins its relative separation from the International Space Station. The ATV undocked from the aft port of the Zvezda Service Module at 4:29 p.m. (CDT) on Sept. 5, 2008 and was placed in a parking orbit for three weeks, scheduled to be deorbited on Sept. 29 when lighting conditions are correct for an ESA imagery experiment of reentry

ATV Jules Verne - The Jules Verne ATV - View of the first European automatic cargo ship ATV christens Jules Verne, leaving the international space station on 5 September 2008. Designed to supply the station with various equipment, the ATV, with several tons of fuel on board, is used to bring the station back into its orbit. Jules Verne moored at the station on April 3, 2008. 5 Sept. 2008 - Backdropped by the blackness of space, European Space Agency's (ESA) “” Jules Verne”” Automated Transfer Vehicle (ATV) begins its relative separation from the International Space Station. The ATV undocked from the aft port of the Zvezda Service Module at 4:29 p.m. (CDT) on Sept. 5, 2008 and was placed in a parking orbit for three weeks, scheduled to be deorbited on Sept. 29 when lighting conditions are correct for an ESA imagery experiment of reentry

PIX4602164

Rosetta probe: the Philae lander poses on the nucleus of the comet: The Rosetta probe was launched on 2 March 2004 to study comet 67P/Churyumov-Gerasimenko. His lander, Philae, landed on the surface of the comet on 12 November 2014 to analyze the composition of the nucleus of the comet - Artist's impression of Rosetta's lander Philae on the surface of comet 67P/Churyumov-Gerasimenko. Philae will be deployed to the comet in November 2014 where it will make in situ observations of the comet surface, including drilling 23 cm into the subsurface to extract material for analysis in its on board laboratory

Rosetta probe: the Philae lander poses on the nucleus of the comet: The Rosetta probe was launched on 2 March 2004 to study comet 67P/Churyumov-Gerasimenko. His lander, Philae, landed on the surface of the comet on 12 November 2014 to analyze the composition of the nucleus of the comet - Artist's impression of Rosetta's lander Philae on the surface of comet 67P/Churyumov-Gerasimenko. Philae will be deployed to the comet in November 2014 where it will make in situ observations of the comet surface, including drilling 23 cm into the subsurface to extract material for analysis in its on board laboratory

Miller, Ron (b.1947)

PIX4974341

The Rosetta lander on a comet nucleus - The Rosetta lander on a comet nucleus - The Rosetta probe was launched on 2 March 2004 to study comet 67P/Churyumov - Gerasimenko. His lander, Philae, landed on the surface of the comet on November 12, 2014 to analyze the composition of the comet's nucleus. Artist's impression of Rosetta's lander Philae (front view) on the surface of comet 67P/Churyumov - Gerasimenko. Philae will be deployed to the comet in November 2014 where it will make in situ observations of the comet surface, including drilling 23 cm into the subsurface to extract material for analysis in its on board laboratory

The Rosetta lander on a comet nucleus - The Rosetta lander on a comet nucleus - The Rosetta probe was launched on 2 March 2004 to study comet 67P/Churyumov - Gerasimenko. His lander, Philae, landed on the surface of the comet on November 12, 2014 to analyze the composition of the comet's nucleus. Artist's impression of Rosetta's lander Philae (front view) on the surface of comet 67P/Churyumov - Gerasimenko. Philae will be deployed to the comet in November 2014 where it will make in situ observations of the comet surface, including drilling 23 cm into the subsurface to extract material for analysis in its on board laboratory

PIX4607164

Comparison between Earth and Venus - Earth and Venus compared - Comparison at the scale of the sizes of Earth and Venus, seen here without their atmosphere. The size of the Venus planet is roughly the same as that of the Earth. This to-scale image suggests how the Earth and Venus might appear without their atmospheres. Venus' diameter is 86% that of the Earth's. It has 82% the mass. If you weigh 180 pounds on the Earth, you would weigh 163 pounds on Venus. Venus is about three-quarters the Earth's distance from the Sun. While Venus is roughly the same size and density as the Earth, it is otherwise a very different world. Earth's surface is a varied one, with liquid water covering three quarters of its surface. Those areas not under water have been highly modified by plate tectonics, weather, and life itself. Venus on the other hand is far too hot to host liquid water. Volcanoes, massive lava flows and the occasional impact crater characterize its surface. Latest observations suggest th

Comparison between Earth and Venus - Earth and Venus compared - Comparison at the scale of the sizes of Earth and Venus, seen here without their atmosphere. The size of the Venus planet is roughly the same as that of the Earth. This to-scale image suggests how the Earth and Venus might appear without their atmospheres. Venus' diameter is 86% that of the Earth's. It has 82% the mass. If you weigh 180 pounds on the Earth, you would weigh 163 pounds on Venus. Venus is about three-quarters the Earth's distance from the Sun. While Venus is roughly the same size and density as the Earth, it is otherwise a very different world. Earth's surface is a varied one, with liquid water covering three quarters of its surface. Those areas not under water have been highly modified by plate tectonics, weather, and life itself. Venus on the other hand is far too hot to host liquid water. Volcanoes, massive lava flows and the occasional impact crater characterize its surface. Latest observations suggest th

Walter B Myers

PIX4629857

Solar Spectrum and Typical Colors (colour litho)

Solar Spectrum and Typical Colors (colour litho)

English School, (20th century)

LLM3624604

The Phoenix probe on its landing site - Phoenix landing site - Mosaic of images in vertical projection showing the Phoenix probe placed on Martian soil. The black circle corresponds to the position of the probe camera. The hundreds of clicks needed to make this image were taken between June 5 and July 12, 2008. Phoenix landed on a vast plain north of Mars, in the Vastitas Borealis region. This view is a vertical projection that combines hundreds exposures taken by the Surface Stereo Imager camera on Nasa's Mars Phoenix Lander and projects them as if looking down from above. The black circle on the spacecraft is where the camera itself is mounted on the lander, out of view in images taken by the camera. North is toward the top of the image. The height of the lander's meteorology mast, extending towards the southwest, appears exaggerated because that mast is taller than the camera mast. This view is in approximately true color. The landing site is at 68.22 degrees north latitude, 234.25

The Phoenix probe on its landing site - Phoenix landing site - Mosaic of images in vertical projection showing the Phoenix probe placed on Martian soil. The black circle corresponds to the position of the probe camera. The hundreds of clicks needed to make this image were taken between June 5 and July 12, 2008. Phoenix landed on a vast plain north of Mars, in the Vastitas Borealis region. This view is a vertical projection that combines hundreds exposures taken by the Surface Stereo Imager camera on Nasa's Mars Phoenix Lander and projects them as if looking down from above. The black circle on the spacecraft is where the camera itself is mounted on the lander, out of view in images taken by the camera. North is toward the top of the image. The height of the lander's meteorology mast, extending towards the southwest, appears exaggerated because that mast is taller than the camera mast. This view is in approximately true color. The landing site is at 68.22 degrees north latitude, 234.25

PIX4616671

The Rosetta spacecraft releases a lander onto a comet nucleus - The Rosetta spacecraft releases a lander onto a comet nucleus - The Rosetta probe was launched on 2 March 2004 to study comet 67P/Churyumov - Gerasimenko. Artist's view of the Philae probe and lander near the nucleus of the comet. The size scales are not respected; the probe measures 32 meters with its deployed panels; the core of the comet about 4 km.; Artist's impression of the Rosetta orbiter deploying the Philae lander to comet 67P/Churyumov - Gerasimenko.; The image is not to scale; the Rosetta spacecraft measures 32 m across including the solar arrays; while the comet nucleus is thought to be about 4 km wide

The Rosetta spacecraft releases a lander onto a comet nucleus - The Rosetta spacecraft releases a lander onto a comet nucleus - The Rosetta probe was launched on 2 March 2004 to study comet 67P/Churyumov - Gerasimenko. Artist's view of the Philae probe and lander near the nucleus of the comet. The size scales are not respected; the probe measures 32 meters with its deployed panels; the core of the comet about 4 km.; Artist's impression of the Rosetta orbiter deploying the Philae lander to comet 67P/Churyumov - Gerasimenko.; The image is not to scale; the Rosetta spacecraft measures 32 m across including the solar arrays; while the comet nucleus is thought to be about 4 km wide

PIX4607178

Communication satellite - Satellite communication - Artist's view showing a telecommunication satellite around the Earth. Illustration of a satellite communication around the Earth

Communication satellite - Satellite communication - Artist's view showing a telecommunication satellite around the Earth. Illustration of a satellite communication around the Earth

D. Ducros

PIX4643252

Size Comparison: Earth, Titan satellite and Moon - Earth, Titan, and Earth's Moon compared - Saturn's largest satellite, Titan compares to Earth and Moon. Titan may be larger than the planet Mercury - and (the dwarf planet) Pluto- but it is still considerably smaller than the Earth. Despite Titan's diminutive size, its atmosphere is dense enough that the barometric pressure at Titan's surface is one and-a-half times greater than that of the Earth's at sea level

Size Comparison: Earth, Titan satellite and Moon - Earth, Titan, and Earth's Moon compared - Saturn's largest satellite, Titan compares to Earth and Moon. Titan may be larger than the planet Mercury - and (the dwarf planet) Pluto- but it is still considerably smaller than the Earth. Despite Titan's diminutive size, its atmosphere is dense enough that the barometric pressure at Titan's surface is one and-a-half times greater than that of the Earth's at sea level

Walter B Myers

PIX4629987

This panel illustrates the transit of the martian moon Phobos across the Sun.

This panel illustrates the transit of the martian moon Phobos across the Sun.

UIG866432

The Mars Express and Beagle 2 probe - Artist view - Mars Express and Beagle 2 - Separation of the Beagle 2 module. The Beagle 2 landing gear that was supposed to perform analysis on the surface of Mars did not work. The European Mars Express probe was launched on 2 June 2003 and began its observations in early 2004. Illustration showing the separation of Beagle 2 from Mars Express. Beagle 2 was lost but the european spaceprobe Mars Express began its March observations in 2004

The Mars Express and Beagle 2 probe - Artist view - Mars Express and Beagle 2 - Separation of the Beagle 2 module. The Beagle 2 landing gear that was supposed to perform analysis on the surface of Mars did not work. The European Mars Express probe was launched on 2 June 2003 and began its observations in early 2004. Illustration showing the separation of Beagle 2 from Mars Express. Beagle 2 was lost but the european spaceprobe Mars Express began its March observations in 2004

D. Ducros

PIX4606646

Comparison between Earth and Mars - Earth and Mars compared - Comparison at the scale of Earth and Mars sizes. The diameter of the planet Mars is half the diameter of the Earth. Mars' diameter is half that of the Earth's It has ten percent the mass If you weigh 180 pounds on Earth, you would weigh only 68 pounds on Mars. Mars is half again further from the Sun than the Earth The vast deserts of North Africa are no match for the planet-wide desert that is Mars. While the Earth is host to oceans of liquid water and has a relatively dense water-rich atmosphere, Mars is exceedingly dry, cold, and so far as we know, sterile. It is believed that Mars lost most of its water to space a long time ago, and any water that remains is frozen at the poles and locked deep in the ground as permafrost. It is an interesting coincidence that the total surface area of Mars is about the same as the surface area of dry land on the Earth

Comparison between Earth and Mars - Earth and Mars compared - Comparison at the scale of Earth and Mars sizes. The diameter of the planet Mars is half the diameter of the Earth. Mars' diameter is half that of the Earth's It has ten percent the mass If you weigh 180 pounds on Earth, you would weigh only 68 pounds on Mars. Mars is half again further from the Sun than the Earth The vast deserts of North Africa are no match for the planet-wide desert that is Mars. While the Earth is host to oceans of liquid water and has a relatively dense water-rich atmosphere, Mars is exceedingly dry, cold, and so far as we know, sterile. It is believed that Mars lost most of its water to space a long time ago, and any water that remains is frozen at the poles and locked deep in the ground as permafrost. It is an interesting coincidence that the total surface area of Mars is about the same as the surface area of dry land on the Earth

Walter B Myers

PIX4629809

Solar panels and telescope on the Moon-Illustration - Solar arrays and telescope on Moon's surface - Illustratio

Solar panels and telescope on the Moon-Illustration - Solar arrays and telescope on Moon's surface - Illustratio

S. Numazawa

PIX4638799

Exploration of Mars-Illustration - Mars rover rendezvous - The exploration of Mars by men will require vehicles that can take a crew long distances and will have to provide them with all the necessary protection against this hostile environment. A pair of manned Mars rovers rendezvous on the martian surface. Humans may one day explore the martian surface with the help of pressurized rovers that would provide a shirt sleeve environment while protecting them from the deadly extremes of the martian environment. In this image each rover provides transportation and life support for two crew members. By traveling in pairs each rover can provide backup for the other, and if necessary a single rover could serve as refuge and transportation for all four explorers

Exploration of Mars-Illustration - Mars rover rendezvous - The exploration of Mars by men will require vehicles that can take a crew long distances and will have to provide them with all the necessary protection against this hostile environment. A pair of manned Mars rovers rendezvous on the martian surface. Humans may one day explore the martian surface with the help of pressurized rovers that would provide a shirt sleeve environment while protecting them from the deadly extremes of the martian environment. In this image each rover provides transportation and life support for two crew members. By traveling in pairs each rover can provide backup for the other, and if necessary a single rover could serve as refuge and transportation for all four explorers

Walter B Myers

PIX4639944

Meudon Observatory - Solar Tower - Meudon observatory: the solar tower

Meudon Observatory - Solar Tower - Meudon observatory: the solar tower

E. Graeff

PIX4654754

Mars Polar Lander - Artist view - Mars Polar Lander spaceprobe - Artist view - The American Mars Polar Lander probe, launched on January 3, 1999, was scheduled to land in December 1999 near the southern polar cap of Mars. Contact with the probe was interrupted on 3 December 1999, when it entered the Martian atmosphere. The Mars Polar Lander is shown on the surface of Mars. The spacecraft was launched in january 1999 to Mars to land near the southern polar cap in December 1999 and carry out a three - month mission to search for traces of subsurface water in this frozen, layered terrain. The contact with the spacecraft was lost on December 9, 1999, shortly after it entered the Martian atmosphere

Mars Polar Lander - Artist view - Mars Polar Lander spaceprobe - Artist view - The American Mars Polar Lander probe, launched on January 3, 1999, was scheduled to land in December 1999 near the southern polar cap of Mars. Contact with the probe was interrupted on 3 December 1999, when it entered the Martian atmosphere. The Mars Polar Lander is shown on the surface of Mars. The spacecraft was launched in january 1999 to Mars to land near the southern polar cap in December 1999 and carry out a three - month mission to search for traces of subsurface water in this frozen, layered terrain. The contact with the spacecraft was lost on December 9, 1999, shortly after it entered the Martian atmosphere

PIX4606678

Mars Polar Lander - Artist view - Mars Polar Lander spaceprobe - Artist view - The American Mars Polar Lander probe, launched on January 3, 1999, was scheduled to land in December 1999 near the southern polar cap of Mars. Contact with the probe was interrupted on 3 December 1999, when it entered the Martian atmosphere. The Mars Polar Lander is shown on the surface of Mars. The spacecraft was launched in january 1999 to Mars to land near the southern polar cap in December 1999 and carry out a three - month mission to search for traces of subsurface water in this frozen, layered terrain. The contact with the spacecraft was lost on December 9, 1999, shortly after it entered the Martian atmosphere

Mars Polar Lander - Artist view - Mars Polar Lander spaceprobe - Artist view - The American Mars Polar Lander probe, launched on January 3, 1999, was scheduled to land in December 1999 near the southern polar cap of Mars. Contact with the probe was interrupted on 3 December 1999, when it entered the Martian atmosphere. The Mars Polar Lander is shown on the surface of Mars. The spacecraft was launched in january 1999 to Mars to land near the southern polar cap in December 1999 and carry out a three - month mission to search for traces of subsurface water in this frozen, layered terrain. The contact with the spacecraft was lost on December 9, 1999, shortly after it entered the Martian atmosphere

PIX4606690

Le Soleil vu by SDO on May 23, 2010 - The Sun seen by SDO. May 23, 2010 - Le Soleil vu en ultraviolet by SDO (Solar Dynamics Observatory) on May 23, 2010. This image taken by SDO (Solar Dynamics Observatory) is a composite of three extreme ultraviolet wavelengths: 211 A (false - color yellow) 193 A (green) and 171 A (blue), each tracing a different gas temperature ranging from 1 to 2 million degrees K

Le Soleil vu by SDO on May 23, 2010 - The Sun seen by SDO. May 23, 2010 - Le Soleil vu en ultraviolet by SDO (Solar Dynamics Observatory) on May 23, 2010. This image taken by SDO (Solar Dynamics Observatory) is a composite of three extreme ultraviolet wavelengths: 211 A (false - color yellow) 193 A (green) and 171 A (blue), each tracing a different gas temperature ranging from 1 to 2 million degrees K

PIX4627172

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