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Bilder zu 'Planetary' gefunden, 2,027

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Tycho Brahe (1546-1601) - celestial globe, 1598

Tycho Brahe (1546-1601) - celestial globe, 1598

XLF3792570

England / UK: Title page of Sir Isaac Newton's Philosophiæ Naturalis Principia Mathematica or 'Mathematical Principles of Natural Philosophy', 3rd edition, London, 1726

England / UK: Title page of Sir Isaac Newton's Philosophiæ Naturalis Principia Mathematica or 'Mathematical Principles of Natural Philosophy', 3rd edition, London, 1726

PFH2561691

Sir William Herschel, German-British astronomer, c 1790s

Sir William Herschel, German-British astronomer, c 1790s

UIS5093286

George Biddell Airy, English astronomer and geophysicist, c 1870

George Biddell Airy, English astronomer and geophysicist, c 1870

UIS5072769

George Biddell Airy, English geophysicist and astronomer, c 1860s

George Biddell Airy, English geophysicist and astronomer, c 1860s

UIS5071524

Manned Space Flight, USA, Apollo 11 Ascent stage of the Apollo 11 Lunar Module, 21st July 1969

Manned Space Flight, USA, Apollo 11 Ascent stage of the Apollo 11 Lunar Module, 21st July 1969

UIS5070191

George Johnstone Stoney, Irish mathematical physicist, c 1900

George Johnstone Stoney, Irish mathematical physicist, c 1900

UIS5082642

Planetary nebula M 27 (NGC 6853) in the little fox - This excellent image of the Dumbbell Nebula (M27, NGC6853), a planetary nebula in the constellation of Vulpecula, was taken at the 3.5 - meter WIYN telescope using the mini - mosaic imager. The nebula was formed when an evolved, red giant star ejected its outer envelope near the end of its lifetime. The expanding cloud of gas becomes visible once the hot core of the star, visible near the center, is exposed and the high - energy, ultraviolet light from the core ionizes the cloud. This makes the nebula emit mostly a strong emission - line spectrum. This color image was obtained by combining three separate pictures, each one taken through a narrow filter centered at the emission wavelengths of Hydrogen (H alpha, red, 656 nm), doubly ionized Oxygen (OII, green, 501 nm), and neutral Oxygen (OI, blue, 630 nm). It is physically very interesting that neutral gas can survive in a region right next to highly ionized gas, and this image shows

Planetary nebula M 27 (NGC 6853) in the little fox - This excellent image of the Dumbbell Nebula (M27, NGC6853), a planetary nebula in the constellation of Vulpecula, was taken at the 3.5 - meter WIYN telescope using the mini - mosaic imager. The nebula was formed when an evolved, red giant star ejected its outer envelope near the end of its lifetime. The expanding cloud of gas becomes visible once the hot core of the star, visible near the center, is exposed and the high - energy, ultraviolet light from the core ionizes the cloud. This makes the nebula emit mostly a strong emission - line spectrum. This color image was obtained by combining three separate pictures, each one taken through a narrow filter centered at the emission wavelengths of Hydrogen (H alpha, red, 656 nm), doubly ionized Oxygen (OII, green, 501 nm), and neutral Oxygen (OI, blue, 630 nm). It is physically very interesting that neutral gas can survive in a region right next to highly ionized gas, and this image shows

PIX4623419

Satellite Herschel - Illustration - Ariane 5 fairing with satellite Herschel. Artwork - Artist's view of the European satellite Herschel during its launch by an Ariane 5 rocket. The Herschel Space Observatory, scheduled to launch in 2009, will study in the infrared the formation of galaxies, stars and planetary systems. This satellite measures nearly 7 metres high by 4.3 metres wide and weighs 3.25 tonnes. Its telescope has a 3.5-meter mirror, making it the largest mirror ever made for a scientific space mission. Herschel will orbit around Lagrange 2, approximately 1.5 million kilometres from Earth. ESA's Herschel Space Observatory (formerly called Far Infrared and Submillimetre Telescope or FIRST) will solve the mystery of how stars and galaxies were born. Objects such as other planetary systems, or processes like the birth of galaxies in the early universe, can best be studied with infrared space telescopes in space. This is the reason for Esa's Herschel. ESA's Herschel Space Observa

Satellite Herschel - Illustration - Ariane 5 fairing with satellite Herschel. Artwork - Artist's view of the European satellite Herschel during its launch by an Ariane 5 rocket. The Herschel Space Observatory, scheduled to launch in 2009, will study in the infrared the formation of galaxies, stars and planetary systems. This satellite measures nearly 7 metres high by 4.3 metres wide and weighs 3.25 tonnes. Its telescope has a 3.5-meter mirror, making it the largest mirror ever made for a scientific space mission. Herschel will orbit around Lagrange 2, approximately 1.5 million kilometres from Earth. ESA's Herschel Space Observatory (formerly called Far Infrared and Submillimetre Telescope or FIRST) will solve the mystery of how stars and galaxies were born. Objects such as other planetary systems, or processes like the birth of galaxies in the early universe, can best be studied with infrared space telescopes in space. This is the reason for Esa's Herschel. ESA's Herschel Space Observa

D. Ducros

PIX4646125

Satellite Herschel - Illustration - Ariane 5 stage with satellite Herschel. Artwork - Artist's view of the European satellite Herschel during its launch by an Ariane 5 rocket. The Herschel Space Observatory, launched on 14 May 2009, is studying in the infrared the formation of galaxies, stars and planetary systems. This satellite measures nearly 7 metres high by 4.3 metres wide and weighs 3.25 tonnes. Its telescope has a 3.5-meter mirror, making it the largest mirror ever made for a scientific space mission. Herschel is in orbit around Lagrange 2, approximately 1.5 million kilometres from Earth. ESA's Herschel Space Observatory (formerly called Far Infrared and Submillimetre Telescope or FIRST) will solve the mystery of how stars and galaxies were born. Objects such as other planetary systems, or processes like the birth of galaxies in the early universe, can best be studied with infrared space telescopes in space. This is the reason for Esa's Herschel. ESA's Herschel Space Observatory

Satellite Herschel - Illustration - Ariane 5 stage with satellite Herschel. Artwork - Artist's view of the European satellite Herschel during its launch by an Ariane 5 rocket. The Herschel Space Observatory, launched on 14 May 2009, is studying in the infrared the formation of galaxies, stars and planetary systems. This satellite measures nearly 7 metres high by 4.3 metres wide and weighs 3.25 tonnes. Its telescope has a 3.5-meter mirror, making it the largest mirror ever made for a scientific space mission. Herschel is in orbit around Lagrange 2, approximately 1.5 million kilometres from Earth. ESA's Herschel Space Observatory (formerly called Far Infrared and Submillimetre Telescope or FIRST) will solve the mystery of how stars and galaxies were born. Objects such as other planetary systems, or processes like the birth of galaxies in the early universe, can best be studied with infrared space telescopes in space. This is the reason for Esa's Herschel. ESA's Herschel Space Observatory

D. Ducros

PIX4646153

Satellite Herschel - Illustration - Ariane 5 fairing with satellite Herschel. Artwork - Artist's view of the European satellite Herschel during its launch by an Ariane 5 rocket. The Herschel Space Observatory, launched on 14 May 2009, is studying in the infrared the formation of galaxies, stars and planetary systems. This satellite measures nearly 7 metres high by 4.3 metres wide and weighs 3.25 tonnes. Its telescope has a 3.5-meter mirror, making it the largest mirror ever made for a scientific space mission. Herschel is in orbit around Lagrange 2, approximately 1.5 million kilometres from Earth. ESA's Herschel Space Observatory (formerly called Far Infrared and Submillimetre Telescope or FIRST) will solve the mystery of how stars and galaxies were born. Objects such as other planetary systems, or processes like the birth of galaxies in the early universe, can best be studied with infrared space telescopes in space. This is the reason for Esa's Herschel. ESA's Herschel Space Observato

Satellite Herschel - Illustration - Ariane 5 fairing with satellite Herschel. Artwork - Artist's view of the European satellite Herschel during its launch by an Ariane 5 rocket. The Herschel Space Observatory, launched on 14 May 2009, is studying in the infrared the formation of galaxies, stars and planetary systems. This satellite measures nearly 7 metres high by 4.3 metres wide and weighs 3.25 tonnes. Its telescope has a 3.5-meter mirror, making it the largest mirror ever made for a scientific space mission. Herschel is in orbit around Lagrange 2, approximately 1.5 million kilometres from Earth. ESA's Herschel Space Observatory (formerly called Far Infrared and Submillimetre Telescope or FIRST) will solve the mystery of how stars and galaxies were born. Objects such as other planetary systems, or processes like the birth of galaxies in the early universe, can best be studied with infrared space telescopes in space. This is the reason for Esa's Herschel. ESA's Herschel Space Observato

D. Ducros

PIX4646169

Exoplanets around Kepler-11: Kepler-11 is a star similar to the Sun, located about 2,000 light years from the Solar System in the constellation Swan. It has a planetary system consisting of at least six exoplanets detected by the Kepler space telescope in 2011. Kepler-11 is a Sun-like star in the constellation Cygnus, located some 2,000 light years from Earth. Announced on February 2, 2011, the star system is among the most compact and flattest systems yet discovered. It is the first discovered case of a star system with six transiting planets. All discovered planets are larger than Earth, with the larger ones being about Neptune's size

Exoplanets around Kepler-11: Kepler-11 is a star similar to the Sun, located about 2,000 light years from the Solar System in the constellation Swan. It has a planetary system consisting of at least six exoplanets detected by the Kepler space telescope in 2011. Kepler-11 is a Sun-like star in the constellation Cygnus, located some 2,000 light years from Earth. Announced on February 2, 2011, the star system is among the most compact and flattest systems yet discovered. It is the first discovered case of a star system with six transiting planets. All discovered planets are larger than Earth, with the larger ones being about Neptune's size

Miller, Ron (b.1947)

PIX4608132

George Biddell Airy, English astronomer and geophysicist, mid 19th century

George Biddell Airy, English astronomer and geophysicist, mid 19th century

UIS5072776

Orrery, 1910-1920

Orrery, 1910-1920

UIS5084501

George Biddell Airy, English geophysicist and astronomer, c 1860s

George Biddell Airy, English geophysicist and astronomer, c 1860s

UIS5071519

England / UK: Title page of Sir Isaac Newton's Philosophiæ Naturalis Principia Mathematica or 'Mathematical Principles of Natural Philosophy', 1st edition, London, 1687

England / UK: Title page of Sir Isaac Newton's Philosophiæ Naturalis Principia Mathematica or 'Mathematical Principles of Natural Philosophy', 1st edition, London, 1687

PFH2561690

The capture of the Moon - Moon capture theory - Infographic showing the different processes of capturing a satellite by a planet. At the top, the developing planetary halo of gas slows down and captures a passing Celestial body. In the middle, the sphere of gravitational influence of the planet develops and attracts a celestial body. At the bottom, interactions between passing asteroids can cause one to remain in orbit around a planet. Infographic shows processes for planet to aquire a satellite. A developing planet's halo of gas expands to capture a passing body (top). Its gravitational sphere of influence expands as well (middle). Interactions between passing asteroids may cause one to fall into orbit (bottom)

The capture of the Moon - Moon capture theory - Infographic showing the different processes of capturing a satellite by a planet. At the top, the developing planetary halo of gas slows down and captures a passing Celestial body. In the middle, the sphere of gravitational influence of the planet develops and attracts a celestial body. At the bottom, interactions between passing asteroids can cause one to remain in orbit around a planet. Infographic shows processes for planet to aquire a satellite. A developing planet's halo of gas expands to capture a passing body (top). Its gravitational sphere of influence expands as well (middle). Interactions between passing asteroids may cause one to fall into orbit (bottom)

Dixon, Don (b.1951)

PIX4633504

Callisto, one of the moons of Jupiter, 1979

Callisto, one of the moons of Jupiter, 1979

UIS5071209

The Ring Nebula, 1998

The Ring Nebula, 1998

UIS5093533

Manned Space Flight, USA, Apollo 11 Astronauts Armstrong and Aldrin unfurling the US flag on the Moon, 1969

Manned Space Flight, USA, Apollo 11 Astronauts Armstrong and Aldrin unfurling the US flag on the Moon, 1969

UIS5071502

Hubble Reopens Eye on the Universe, 2000

Hubble Reopens Eye on the Universe, 2000

UIS5093510

Exoplanete WASP-12b: WASP-12b is a hot Jupiter-type exoplanet orbiting in 1.09 days around the star WASP-12, located about 870 light-years from the Sun, in the constellation of Coach. This planet is so close to its star that it is stretched by the maree forces of the latter so that it presents an ovoid shape and its atmosphere is little by little torn away by the star. WASP-12b is an extrasolar planet orbiting the star WASP-12, discovered by the SuperWasp planetary transit survey. Due to its extremely close orbit to its star, the star's tidal forces are distorting it into an egg shape and pulling away its atmosphere. The planet takes only a little over a day to orbit the star

Exoplanete WASP-12b: WASP-12b is a hot Jupiter-type exoplanet orbiting in 1.09 days around the star WASP-12, located about 870 light-years from the Sun, in the constellation of Coach. This planet is so close to its star that it is stretched by the maree forces of the latter so that it presents an ovoid shape and its atmosphere is little by little torn away by the star. WASP-12b is an extrasolar planet orbiting the star WASP-12, discovered by the SuperWasp planetary transit survey. Due to its extremely close orbit to its star, the star's tidal forces are distorting it into an egg shape and pulling away its atmosphere. The planet takes only a little over a day to orbit the star

Miller, Ron (b.1947)

PIX4608333

Dumb-bell nebula (M27), 3 October 1888

Dumb-bell nebula (M27), 3 October 1888

UIS5095876

'Telescopic Appearance of the Moon', c 1851

'Telescopic Appearance of the Moon', c 1851

UIS5096359

Orrery with wooden case, 1718-1747

Orrery with wooden case, 1718-1747

UIS5085345

Portrait of a gentleman in his study with scientific instruments, c 1750

Portrait of a gentleman in his study with scientific instruments, c 1750

UIS5063980

The Cat's Eye Nebula, 1994

The Cat's Eye Nebula, 1994

UIS5093411

Herschel Satellite - Illustration - Herschel Satellite. Artwork - Artist's view of the European satellite Herschel. The Herschel Space Observatory, scheduled to launch in 2009, will study in the infrared the formation of galaxies, stars and planetary systems. This satellite measures nearly 7 metres high by 4.3 metres wide and weighs 3.25 tonnes. Its telescope has a 3.5-meter mirror, making it the largest mirror ever made for a scientific space mission. Herschel will orbit around Lagrange 2, approximately 1.5 million kilometres from Earth. ESA's Herschel Space Observatory (formerly called Far Infrared and Submillimetre Telescope or FIRST) will solve the mystery of how stars and galaxies were born. Infrared astronomy is as young as it is fruitful. In less than three decades infrared astronomers have unveiled tens of thousands of new galaxies, and have made discoveries as surprising as the huge amounts of water vapour that fill the galaxy. Yet scientists know there is still much more to d

Herschel Satellite - Illustration - Herschel Satellite. Artwork - Artist's view of the European satellite Herschel. The Herschel Space Observatory, scheduled to launch in 2009, will study in the infrared the formation of galaxies, stars and planetary systems. This satellite measures nearly 7 metres high by 4.3 metres wide and weighs 3.25 tonnes. Its telescope has a 3.5-meter mirror, making it the largest mirror ever made for a scientific space mission. Herschel will orbit around Lagrange 2, approximately 1.5 million kilometres from Earth. ESA's Herschel Space Observatory (formerly called Far Infrared and Submillimetre Telescope or FIRST) will solve the mystery of how stars and galaxies were born. Infrared astronomy is as young as it is fruitful. In less than three decades infrared astronomers have unveiled tens of thousands of new galaxies, and have made discoveries as surprising as the huge amounts of water vapour that fill the galaxy. Yet scientists know there is still much more to d

PIX4646040

Sundials, Altitude Chalice sundial, 1596

Sundials, Altitude Chalice sundial, 1596

UIS5061585

Glass prism, used by Sir William Herschel, c 1770-1822

Glass prism, used by Sir William Herschel, c 1770-1822

UIS5067845

Callisto, one of the moons of Jupiter, 1979

Callisto, one of the moons of Jupiter, 1979

UIS5071076

Herschel Satellite - Illustration - Herschel Satellite. Artwork - Artist's view of the European satellite Herschel. The Herschel Space Observatory, scheduled to launch in 2009, will study in the infrared the formation of galaxies, stars and planetary systems. This satellite measures nearly 7 metres high by 4.3 metres wide and weighs 3.25 tonnes. Its telescope has a 3.5-meter mirror, making it the largest mirror ever made for a scientific space mission. Herschel will orbit around Lagrange 2, approximately 1.5 million kilometres from Earth. ESA's Herschel Space Observatory (formerly called Far Infrared and Submillimetre Telescope or FIRST) will solve the mystery of how stars and galaxies were born. Infrared astronomy is as young as it is fruitful. In less than three decades infrared astronomers have unveiled tens of thousands of new galaxies, and have made discoveries as surprising as the huge amounts of water vapour that fill the galaxy. Yet scientists know there is still much more to d

Herschel Satellite - Illustration - Herschel Satellite. Artwork - Artist's view of the European satellite Herschel. The Herschel Space Observatory, scheduled to launch in 2009, will study in the infrared the formation of galaxies, stars and planetary systems. This satellite measures nearly 7 metres high by 4.3 metres wide and weighs 3.25 tonnes. Its telescope has a 3.5-meter mirror, making it the largest mirror ever made for a scientific space mission. Herschel will orbit around Lagrange 2, approximately 1.5 million kilometres from Earth. ESA's Herschel Space Observatory (formerly called Far Infrared and Submillimetre Telescope or FIRST) will solve the mystery of how stars and galaxies were born. Infrared astronomy is as young as it is fruitful. In less than three decades infrared astronomers have unveiled tens of thousands of new galaxies, and have made discoveries as surprising as the huge amounts of water vapour that fill the galaxy. Yet scientists know there is still much more to d

PIX4646048

The lily and Saturn, 13th century. Saturn rules both Capricorn and Aquarius in classical astrology, hence the goat and water carrier depicted with him. Saturn also governs old age and infirmity. Therefore he is depicted as an old man leaning on a crutch. He also holds a sickle, which is perhaps a reference to death and the grim reaper. From a printed edition of "Naturalia" by Albertus Magnus, showing plants which embodied planetary influences

The lily and Saturn, 13th century. Saturn rules both Capricorn and Aquarius in classical astrology, hence the goat and water carrier depicted with him. Saturn also governs old age and infirmity. Therefore he is depicted as an old man leaning on a crutch. He also holds a sickle, which is perhaps a reference to death and the grim reaper. From a printed edition of "Naturalia" by Albertus Magnus, showing plants which embodied planetary influences

BL5346417

Orrery with armillary bands, 1740-1747

Orrery with armillary bands, 1740-1747

UIS5061960

Geological map of the moon, 1967

Geological map of the moon, 1967

UIS5071972

Orrery, 1851-1856

Orrery, 1851-1856

UIS5061649

George Biddell Airy, English astronomer and geophysicist, 1852

George Biddell Airy, English astronomer and geophysicist, 1852

UIS5062600

Wooden pulley orrery, 1755-1756

Wooden pulley orrery, 1755-1756

UIS5061954

Orrery with wooden case, 1718-1747

Orrery with wooden case, 1718-1747

UIS5085358

Kepler's trigon diagram, 1606

Kepler's trigon diagram, 1606

UIS5086387

Sir Isaac Newton, English mathematician and physicist, 1702

Sir Isaac Newton, English mathematician and physicist, 1702

UIS5072541

Orrery, 1738-1777

Orrery, 1738-1777

UIS5084355

Ganymede, one of the moons of Jupiter, 1979

Ganymede, one of the moons of Jupiter, 1979

UIS5071198

Surface of the planet Mars, 1976

Surface of the planet Mars, 1976

UIS5071756

View of the Moon', c 1850

View of the Moon', c 1850

UIS5090300

View of the Moon', c 1850

View of the Moon', c 1850

UIS5096221

Delta II rocket decolling - DAWN probe - 09 - 2007 - Dawn spacecraft launch - 09 - 2007 - Delta II rocket decolving on 27 September 2007 carrying the DAWN probe destined for the study of the asteroid Vesta and the dwarf planet Ceres. September 27, 2007. The Delta II rocket carrying Nasa's Dawn spacecraft begin its 1.7 - billion - mile journey through the inner solar system to study a pair of asteroids. Liftoff was at 7:34 a.m. EDT from Pad 17 - B at Cape Canaveral Air Force Station. The spacecraft will be the first to orbit two planetary bodies, asteroid Vesta and dwarf planet Ceres, during a single mission. It is also NASA's first purely scientific mission powered by three solar electric ion propulsion engine

Delta II rocket decolling - DAWN probe - 09 - 2007 - Dawn spacecraft launch - 09 - 2007 - Delta II rocket decolving on 27 September 2007 carrying the DAWN probe destined for the study of the asteroid Vesta and the dwarf planet Ceres. September 27, 2007. The Delta II rocket carrying Nasa's Dawn spacecraft begin its 1.7 - billion - mile journey through the inner solar system to study a pair of asteroids. Liftoff was at 7:34 a.m. EDT from Pad 17 - B at Cape Canaveral Air Force Station. The spacecraft will be the first to orbit two planetary bodies, asteroid Vesta and dwarf planet Ceres, during a single mission. It is also NASA's first purely scientific mission powered by three solar electric ion propulsion engine

PIX4605150

Drum model brass orrery (planetaire), 1781-1795

Drum model brass orrery (planetaire), 1781-1795

UIS5060550

Orrery, 1738-1777

Orrery, 1738-1777

UIS5085581

Sir Isaac Newton, English mathematician and physicist, 1666

Sir Isaac Newton, English mathematician and physicist, 1666

UIS5084494

Close up of the surface of Ganymede, one of the moons of Jupiter, 1979 This photograph taken by one of the two Voyager spacecraft shows impact craters and ejecta on the surface of Ganymede

Close up of the surface of Ganymede, one of the moons of Jupiter, 1979 This photograph taken by one of the two Voyager spacecraft shows impact craters and ejecta on the surface of Ganymede

UIS5071653

Asteroid collapsed by tidal force - Artist view - Artist view - Artist view - Artist view - Artist view of an asteroid breaks by the gravitational attraction of a star at the end of life, a white dwarf. This artist's concept illustrates a dead star, or “” white dwarf,””” surrounded by the bits and pieces of a disintegrating asteroid. Asteroids are leftover scraps of planetary material. They form early on in a star's history when planets are forming out of collisions between rocky bodies. When a star like our sun dies, shrinking down to a skeleton of its former self called a white dwarf, its asteroids get jostled about. If one of these asteroids gets too close to the white dwarf, the white dwarf's gravity will chew the asteroid up, leaving a cloud of dust

Asteroid collapsed by tidal force - Artist view - Artist view - Artist view - Artist view - Artist view of an asteroid breaks by the gravitational attraction of a star at the end of life, a white dwarf. This artist's concept illustrates a dead star, or “” white dwarf,””” surrounded by the bits and pieces of a disintegrating asteroid. Asteroids are leftover scraps of planetary material. They form early on in a star's history when planets are forming out of collisions between rocky bodies. When a star like our sun dies, shrinking down to a skeleton of its former self called a white dwarf, its asteroids get jostled about. If one of these asteroids gets too close to the white dwarf, the white dwarf's gravity will chew the asteroid up, leaving a cloud of dust

PIX4584086

Print from original 1794 plate of Herschel's reflecting telescope, 1976

Print from original 1794 plate of Herschel's reflecting telescope, 1976

UIS5096329

Ring Nebula in the constellation of Lyra (M57), 14 July 1887

Ring Nebula in the constellation of Lyra (M57), 14 July 1887

UIS5095894

Planetary nebula NGC 7027 in the Swan/HST - This NASA Hubble Space Telescope image of planetary nebula NGC 7027 shows remarkable new details of the process by which a star like the Sun dies. New features include: faint, blue, concentric shells surrounding the nebula; an extensive network of red dust clouds throughout the bright inner region; and the hot central white dwarf, visible as a white dot at the center. The nebula is a record of the star's final death throes. Initially the ejection of the star's outer layers, when it was at its red giant stage of evolution, occurred at a low rate and was spherical. The Hubble photo reveals that the initial ejections occurred episodically to produce the concentric shells. This culminated in a vigorous ejection of all of the remaining outer layers, which produced the bright inner regions. At this later stage the ejection was non - spherical, and dense clouds of dust condensed from the ejected material. NGC 7027 is located about 3,000 light - year

Planetary nebula NGC 7027 in the Swan/HST - This NASA Hubble Space Telescope image of planetary nebula NGC 7027 shows remarkable new details of the process by which a star like the Sun dies. New features include: faint, blue, concentric shells surrounding the nebula; an extensive network of red dust clouds throughout the bright inner region; and the hot central white dwarf, visible as a white dot at the center. The nebula is a record of the star's final death throes. Initially the ejection of the star's outer layers, when it was at its red giant stage of evolution, occurred at a low rate and was spherical. The Hubble photo reveals that the initial ejections occurred episodically to produce the concentric shells. This culminated in a vigorous ejection of all of the remaining outer layers, which produced the bright inner regions. At this later stage the ejection was non - spherical, and dense clouds of dust condensed from the ejected material. NGC 7027 is located about 3,000 light - year

PIX4623552

Orrery, 1738-1777

Orrery, 1738-1777

UIS5087759

Orrery, 1738-1777

Orrery, 1738-1777

UIS5088526

Exoplanets around the pulsar PSR B1257+12: PSR B1257+12, also called Lich since December 2015, is a pulsar located at a distance of 2300 light years from the Sun, in the constellation of the Virgin. In 1992 two planets orbiting the star were discovered. A third planet was discovered later around PSR B1257+12. PSR B1257+12, also named Lich, is a pulsar located 2300 light years from the Sun in the constellation of Virgo. The pulsar has a planetary system with three known extrasolar planets, named “” Draugr”” (PSR B1257+12 A), “” Poltergeist”” (PSR B1257+12 B) and “” Phobetor””” (PSR B1257+12 C), respectively. They were both the first extrasolar planets and the first pulsar planets to be discovered; A and B in 1992 and C in 1994

Exoplanets around the pulsar PSR B1257+12: PSR B1257+12, also called Lich since December 2015, is a pulsar located at a distance of 2300 light years from the Sun, in the constellation of the Virgin. In 1992 two planets orbiting the star were discovered. A third planet was discovered later around PSR B1257+12. PSR B1257+12, also named Lich, is a pulsar located 2300 light years from the Sun in the constellation of Virgo. The pulsar has a planetary system with three known extrasolar planets, named “” Draugr”” (PSR B1257+12 A), “” Poltergeist”” (PSR B1257+12 B) and “” Phobetor””” (PSR B1257+12 C), respectively. They were both the first extrasolar planets and the first pulsar planets to be discovered; A and B in 1992 and C in 1994

Miller, Ron (b.1947)

PIX4608544

Jupiter's four 'Galilean' moons, 1979

Jupiter's four 'Galilean' moons, 1979

UIS5072263

Photomontage of a large crater on the Moon, 1971-1972

Photomontage of a large crater on the Moon, 1971-1972

UIS5071867

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