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Star V838 Monocerotis 28/10/2004 - V838 Monocerotis 10/2004 - This variable star is located approximately 20,000 years - light from Earth in the constellation Unicorn. In the beginning of 2002, this star illuminated temporarily becoming one of the brightest stars in the sky. Viewed here in October 2004 by the Hubble space telescope, the light echo shows details in the interstellar dust surrounding the star. In January 2002, a variable star in the Monoceros constellation suddenly became 600,000 times more luminous than our Sun, temporarily making it the brightest star in our Milky Way galaxy. The mysterious star, called V838 Monocerotis, has long since faded back to obscurity. Seen here by Nasa's Hubble Space Telescope on October 28, 2004, the light echo around the star has uncovered details in the interstellar dust round the star

Star V838 Monocerotis 28/10/2004 - V838 Monocerotis 10/2004 - This variable star is located approximately 20,000 years - light from Earth in the constellation Unicorn. In the beginning of 2002, this star illuminated temporarily becoming one of the brightest stars in the sky. Viewed here in October 2004 by the Hubble space telescope, the light echo shows details in the interstellar dust surrounding the star. In January 2002, a variable star in the Monoceros constellation suddenly became 600,000 times more luminous than our Sun, temporarily making it the brightest star in our Milky Way galaxy. The mysterious star, called V838 Monocerotis, has long since faded back to obscurity. Seen here by Nasa's Hubble Space Telescope on October 28, 2004, the light echo around the star has uncovered details in the interstellar dust round the star

PIX4572282

The Tower Telescope used at Mt Wilson Observatory

The Tower Telescope used at Mt Wilson Observatory

UIG3740708

Telesope observation from the Pic du Midi observatory (65) - Amateur astronomers at Pic du Midi observatory - Soiree d'observation au Pic du Midi.. Lighting from a first district of Lune Amateur astronomers observing at Pic du Midi observatory

Telesope observation from the Pic du Midi observatory (65) - Amateur astronomers at Pic du Midi observatory - Soiree d'observation au Pic du Midi.. Lighting from a first district of Lune Amateur astronomers observing at Pic du Midi observatory

Patrick Lécureuil

PIX4655597

Crab Nebula seen in different wavelength - The Crab Nebula in multi wavelength: M1, the Crab Nebula, is the rest of a supernova that exploded on July 4, 1054. It is located about 6500 light years from Earth in the constellation Taurus. At the heart of this nebula is a pulsar. To obtain this photo, different observatories and telescopes combined their observations; the VLA provided the radio image (in red), the Spitzer telescope the infrared image (in yellow), the Hubble telescope for the visible part (here in green), XMM-Newton the ultraviolet image (in blue) and the Chandra telescope for X-ray data (purple). The pulsar is the bright spot in the center of the image. The unusual image was produced by combining data from telescopes spanning almost the entire electromagnetic spectrum, from radio waves to X-rays. The Karl G. Jansky Very Large Array (VLA) provided information about the nebula gathered in the radio regime (colored in red). Nasa's Spitzer Space Telescope took images in the in

Crab Nebula seen in different wavelength - The Crab Nebula in multi wavelength: M1, the Crab Nebula, is the rest of a supernova that exploded on July 4, 1054. It is located about 6500 light years from Earth in the constellation Taurus. At the heart of this nebula is a pulsar. To obtain this photo, different observatories and telescopes combined their observations; the VLA provided the radio image (in red), the Spitzer telescope the infrared image (in yellow), the Hubble telescope for the visible part (here in green), XMM-Newton the ultraviolet image (in blue) and the Chandra telescope for X-ray data (purple). The pulsar is the bright spot in the center of the image. The unusual image was produced by combining data from telescopes spanning almost the entire electromagnetic spectrum, from radio waves to X-rays. The Karl G. Jansky Very Large Array (VLA) provided information about the nebula gathered in the radio regime (colored in red). Nasa's Spitzer Space Telescope took images in the in

PIX4626499

Amateur astronomers - Club Lyon Ampere (CALA) Soiree d'observation - CALA amateur observatory. France - 02/05/2005 Observing nigh

Amateur astronomers - Club Lyon Ampere (CALA) Soiree d'observation - CALA amateur observatory. France - 02/05/2005 Observing nigh

Christophe Lebedinsky

PIX4566640

Amateur astronomers - Club Lyon Ampere (CALA) Soiree d'observation - CALA amateur observatory. France - Observing nigh

Amateur astronomers - Club Lyon Ampere (CALA) Soiree d'observation - CALA amateur observatory. France - Observing nigh

Christophe Lebedinsky

PIX4566642

Cloud IC 349 illuminates by the star Merope - Barnard's Merope Nebula (IC 349) - IC 349 is an interstellar cloud illuminated by the star Merope (off-field) of the Pleiades cluster. Image obtained by the Hubble Space Telescope. This ghostly apparition is actually an interstellar cloud caught in the process of destruction by strong radiation from a nearby hot star. This picture, snapped by the Hubble telescope, shows a cloud illuminated by light from the bright star Merope. Located in the Pleiades star cluster, the cloud is called IC 349 or Barnard's Merope Nebul

Cloud IC 349 illuminates by the star Merope - Barnard's Merope Nebula (IC 349) - IC 349 is an interstellar cloud illuminated by the star Merope (off-field) of the Pleiades cluster. Image obtained by the Hubble Space Telescope. This ghostly apparition is actually an interstellar cloud caught in the process of destruction by strong radiation from a nearby hot star. This picture, snapped by the Hubble telescope, shows a cloud illuminated by light from the bright star Merope. Located in the Pleiades star cluster, the cloud is called IC 349 or Barnard's Merope Nebul

PIX4568849

Barree spiral galaxy NGC 4319 and Markarian quasar 205 - Galaxy NGC 4319 and quasar Markarian 205 - The barree spiral galaxy NGC 4319, in the center, is 80 million years - light in the constellation of the Dragon. The Markarian 205 quasar, on the top right, is 14 times further at about 1 billion light years. These two objects are therefore not interacting; on the other hand, the galaxy NGC 4319 is probably interacting with the galaxy NGC 4291, out of field, as the weak arm at the bottom left allows. Quasars are galaxies that create an extremely bright core. Image made by the Hubble Space Telescope in 2002. In this NASA Hubble Space Telescope image, an odd celestial duo, the spiral galaxy NGC 4319 (center) and a quasar called Markarian 205 (upper right), appear to be neighbors. In reality, the two objects don't even live in the same city. NGC 4319 is 80 million light - years from Earth. Markarian 205 (Mrk 205) is more than 14 times farther away, residing 1 billion light - years from Ear

Barree spiral galaxy NGC 4319 and Markarian quasar 205 - Galaxy NGC 4319 and quasar Markarian 205 - The barree spiral galaxy NGC 4319, in the center, is 80 million years - light in the constellation of the Dragon. The Markarian 205 quasar, on the top right, is 14 times further at about 1 billion light years. These two objects are therefore not interacting; on the other hand, the galaxy NGC 4319 is probably interacting with the galaxy NGC 4291, out of field, as the weak arm at the bottom left allows. Quasars are galaxies that create an extremely bright core. Image made by the Hubble Space Telescope in 2002. In this NASA Hubble Space Telescope image, an odd celestial duo, the spiral galaxy NGC 4319 (center) and a quasar called Markarian 205 (upper right), appear to be neighbors. In reality, the two objects don't even live in the same city. NGC 4319 is 80 million light - years from Earth. Markarian 205 (Mrk 205) is more than 14 times farther away, residing 1 billion light - years from Ear

PIX4611257

Pluto - Pluto - The dwarf planet Pluto seen by the Hubble space telescope. These images, recomposed by computer from cliches obtained in 2002 and 2003, are not sufficiently precise to show Pluto's surface in detail but reveal color differences. This is the most detailed view to date of the entire surface of the dwarf planet Pluto, as constructed from multiple NASA Hubble Space Telescope photographs taken from 2002 to 2003. Hubble's view isn't sharp enough to see craters or mountains, if they exist on the surface, but Hubble reveals a complex - looking and variegated world with white, dark - orange, and charcoal - black terrain. The overall color is believed to be a result of ultraviolet radiation from the distant Sun breaking up methane that is present on Pluto's surface, leaving behind a dark, molasse - colored, carbon - rich residue. The center disk (180 degrees) has a mysterious bright spot that is unusually rich in carbon monoxide frost. This region will be photographed in the high

Pluto - Pluto - The dwarf planet Pluto seen by the Hubble space telescope. These images, recomposed by computer from cliches obtained in 2002 and 2003, are not sufficiently precise to show Pluto's surface in detail but reveal color differences. This is the most detailed view to date of the entire surface of the dwarf planet Pluto, as constructed from multiple NASA Hubble Space Telescope photographs taken from 2002 to 2003. Hubble's view isn't sharp enough to see craters or mountains, if they exist on the surface, but Hubble reveals a complex - looking and variegated world with white, dark - orange, and charcoal - black terrain. The overall color is believed to be a result of ultraviolet radiation from the distant Sun breaking up methane that is present on Pluto's surface, leaving behind a dark, molasse - colored, carbon - rich residue. The center disk (180 degrees) has a mysterious bright spot that is unusually rich in carbon monoxide frost. This region will be photographed in the high

PIX4624317

The planet Saturn observed with the Hubble space telescope in October 1996. Saturn measures 120,000 km in diameter -: Saturn by Hubble- natural colors-10-1996

The planet Saturn observed with the Hubble space telescope in October 1996. Saturn measures 120,000 km in diameter -: Saturn by Hubble- natural colors-10-1996

PIX4624800

Barree spiral galaxy NGC 7479 in Pegase - Barred spiral galaxy NGC 7479 in Pegasus - Image obtained by the Hubble space telescope (HST). Its distance is estimated to be about 105 million light years away. Image taken with the Hubble space telescope (HST)

Barree spiral galaxy NGC 7479 in Pegase - Barred spiral galaxy NGC 7479 in Pegasus - Image obtained by the Hubble space telescope (HST). Its distance is estimated to be about 105 million light years away. Image taken with the Hubble space telescope (HST)

PIX4613187

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

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

PIX4572084

Supernova Remnants SNR B0509 - 67.5 - Supernova Remnant SNR B0509 - 67.5 - SNR B0509 - 67.5 (or SNR 0509) is the rest of a star explosion in the galaxy of the Great Magellan Cloud. This 23-year bubble - light of diameter extends at a speed of 18 million km/h. Composite of images obtained by the Hubble Space Telescope (HST) in 2006 and 2010. This delicate shell, photographed by the NASA/ESA Hubble Space Telescope, appears to float serenely in the depths of space, but this apparent calm hides an inner turmoil. The gaseous envelope formed as the expanding blast wave and ejected material from a supernova tore through the nearby interstellar medium. Called SNR B0509 - 67.5 (or SNR 0509 for short), the bubble is the visible remnant of a powerful stellar explosion in the Large Magellanic Cloud (LMC), a small galaxy about 160,000 light - years from Earth. Ripples in the shell's surface may be caused either by subtle variations in the density of the ambient interstellar gas, or possibly be driv

Supernova Remnants SNR B0509 - 67.5 - Supernova Remnant SNR B0509 - 67.5 - SNR B0509 - 67.5 (or SNR 0509) is the rest of a star explosion in the galaxy of the Great Magellan Cloud. This 23-year bubble - light of diameter extends at a speed of 18 million km/h. Composite of images obtained by the Hubble Space Telescope (HST) in 2006 and 2010. This delicate shell, photographed by the NASA/ESA Hubble Space Telescope, appears to float serenely in the depths of space, but this apparent calm hides an inner turmoil. The gaseous envelope formed as the expanding blast wave and ejected material from a supernova tore through the nearby interstellar medium. Called SNR B0509 - 67.5 (or SNR 0509 for short), the bubble is the visible remnant of a powerful stellar explosion in the Large Magellanic Cloud (LMC), a small galaxy about 160,000 light - years from Earth. Ripples in the shell's surface may be caused either by subtle variations in the density of the ambient interstellar gas, or possibly be driv

PIX4583175

Pic du Midi de Bigorre/Astronomy Observatory/Pyrenees National Park/Hautes Pyrenees/Midi Pyrenees/France

Pic du Midi de Bigorre/Astronomy Observatory/Pyrenees National Park/Hautes Pyrenees/Midi Pyrenees/France

Petit J.P

HFE4455865

Telescope/Mirror 60 cm/at the disposal of amateur astronomers/Pic du Midi de Bigorre/National Park of Pyrenees/Hautes Pyrenees/Midi Pyrenees/France

Telescope/Mirror 60 cm/at the disposal of amateur astronomers/Pic du Midi de Bigorre/National Park of Pyrenees/Hautes Pyrenees/Midi Pyrenees/France

Petit J.P

HFE4455874

Pic du Midi de Bigorre/Meteorological Station/Pyrenees National Park/Hautes Pyrenees/Midi Pyrenees/France

Pic du Midi de Bigorre/Meteorological Station/Pyrenees National Park/Hautes Pyrenees/Midi Pyrenees/France

Petit J.P

HFE4455877

Astronomy, The James Lick Telescope at the University of California's Lick Observatory, engtaving c. 1889

Astronomy, The James Lick Telescope at the University of California's Lick Observatory, engtaving c. 1889

EVB2929504

Sun Unit Telescope 1, Moon Unit Telescope 2, Southern Cross Unit Telescope 3 & Venus Unit Telescope 4 (photo)

Sun Unit Telescope 1, Moon Unit Telescope 2, Southern Cross Unit Telescope 3 & Venus Unit Telescope 4 (photo)

UIG2915909

Views in Rodriguez Relating to the Transit of Venus (engraving)

Views in Rodriguez Relating to the Transit of Venus (engraving)

English School, (19th century)

LIP1589406

A recent Hubble Space Telescope (HST) view reveals Uranus surrounded by its 4 major rings and 10 of its 17 known satellites

A recent Hubble Space Telescope (HST) view reveals Uranus surrounded by its 4 major rings and 10 of its 17 known satellites

UIG529096

Switzerland Bern University Observatory, 1956 (b/w photo)

Switzerland Bern University Observatory, 1956 (b/w photo)

KES6247784

Hypertelescope Carlina - Carlina Hypertelescope concept - This hypertelescope concept is the optical analogue of Arecibo's radiotelescope, but it uses a balloon to carry focal optics. On the ground, several mirrors in a crater or a natural bowl form a virtual giant mirror. Principle of the Carlina hypertelescope. Many small mirrors are distributed on a spherical surface. A helium balloon carries a gondola that contains focal optics

Hypertelescope Carlina - Carlina Hypertelescope concept - This hypertelescope concept is the optical analogue of Arecibo's radiotelescope, but it uses a balloon to carry focal optics. On the ground, several mirrors in a crater or a natural bowl form a virtual giant mirror. Principle of the Carlina hypertelescope. Many small mirrors are distributed on a spherical surface. A helium balloon carries a gondola that contains focal optics

Gregoire Cirade

PIX4655341

Observatory of the Pic du Midi - Pic du Midi observatory - In the foreground, the dome of the T60, a 60 cm telescope made available to amateurs. Foreground is the 60 cm telescope dome welcoming amateur astronomers via the Association T60

Observatory of the Pic du Midi - Pic du Midi observatory - In the foreground, the dome of the T60, a 60 cm telescope made available to amateurs. Foreground is the 60 cm telescope dome welcoming amateur astronomers via the Association T60

L. Ades

PIX4655548

Spiral galaxy NGC 7331 in Pegase - Spiral galaxy NGC 7331 in Pegasus: The galaxy NGC 7331 is located about 45 million light years away from Earth. Image obtained with the Hubble Space Telescope. NGC 7331 is located about 45 million light-years away in the constellation of Pegasus (The Winged Horse). Facing us partially edge-on, the galaxy showcases it's beautiful arms which swirl like a whirlpool around its bright central region. Astronomers took this image using Hubble's Wide Field Camera 3 (WFC3), as they were observing an extraordinary exploding star - a supernova - which can still be faintly seen as a tiny red dot near the galaxy's central yellow core. Named SN2014C, it rapidly evolved from a supernova containing very little Hydrogen to one that is Hydrogen-rich - in just one year. This rarely observed metamorphosis was luminous at high energies and provides unique insight into the poorly understood final phases of massive stars. NGC 7331 is similar in size, shape, and mass to the

Spiral galaxy NGC 7331 in Pegase - Spiral galaxy NGC 7331 in Pegasus: The galaxy NGC 7331 is located about 45 million light years away from Earth. Image obtained with the Hubble Space Telescope. NGC 7331 is located about 45 million light-years away in the constellation of Pegasus (The Winged Horse). Facing us partially edge-on, the galaxy showcases it's beautiful arms which swirl like a whirlpool around its bright central region. Astronomers took this image using Hubble's Wide Field Camera 3 (WFC3), as they were observing an extraordinary exploding star - a supernova - which can still be faintly seen as a tiny red dot near the galaxy's central yellow core. Named SN2014C, it rapidly evolved from a supernova containing very little Hydrogen to one that is Hydrogen-rich - in just one year. This rarely observed metamorphosis was luminous at high energies and provides unique insight into the poorly understood final phases of massive stars. NGC 7331 is similar in size, shape, and mass to the

PIX4613167

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

Astronomical bezel - 130 mm refractor - 130 mm aperture f/8 refractor, 80 mm guidescope, German Equatorial mounting. Astrophotography Setup

Astronomical bezel - 130 mm refractor - 130 mm aperture f/8 refractor, 80 mm guidescope, German Equatorial mounting. Astrophotography Setup

Jerry Lodriguss

PIX4567088

The Eagle nebula, an industrious star-making factory located 7,000 light-years away in the Serpens constellation. The image shows the region's entire network of turbulent clouds and newborn stars in infrared light. Hubble Space Telescope (HST),Spitzer Space Telescope.

The Eagle nebula, an industrious star-making factory located 7,000 light-years away in the Serpens constellation. The image shows the region's entire network of turbulent clouds and newborn stars in infrared light. Hubble Space Telescope (HST),Spitzer Space Telescope.

UIG867081

Telescope Yepun - Paranal Observatory, Chile - Yepun and the Magellanic clouds - Paranal Observatory, Chile: The 8,2m diameter telescope Yepun and an auxiliary telescope seen on August 8, 2014. In the sky the clouds of Magellan. The four 8m telescopes telescopes, named Antu (Sun), Kueyen (Moon), Melipal (Southern Cross), and Yepun (Venus) form a very versatile observatory. They can be used as a single large telescope that adds (incoherently) the light from all four, in order to achieve the light gathering ability of a single 16m telescope. Also, their light can be combined in a coherent manner in order to achieve a solving power equivalent to the one of a telescope with a diameter as large as the baseline between the units. Of course, all the telescopes can be used individually, which is usually the default mode of operation

Telescope Yepun - Paranal Observatory, Chile - Yepun and the Magellanic clouds - Paranal Observatory, Chile: The 8,2m diameter telescope Yepun and an auxiliary telescope seen on August 8, 2014. In the sky the clouds of Magellan. The four 8m telescopes telescopes, named Antu (Sun), Kueyen (Moon), Melipal (Southern Cross), and Yepun (Venus) form a very versatile observatory. They can be used as a single large telescope that adds (incoherently) the light from all four, in order to achieve the light gathering ability of a single 16m telescope. Also, their light can be combined in a coherent manner in order to achieve a solving power equivalent to the one of a telescope with a diameter as large as the baseline between the units. Of course, all the telescopes can be used individually, which is usually the default mode of operation

Alex Tudorica

PIX4657504

Observation Night - Star Party - Meeting of Amateur Astronomers in the United States. The summer Milky Way in Sagittarius sets behind a group of amateur astronomers at the Black Forest Star Party in Cherry Springs Pennsylvania, USA on September 3, 2005

Observation Night - Star Party - Meeting of Amateur Astronomers in the United States. The summer Milky Way in Sagittarius sets behind a group of amateur astronomers at the Black Forest Star Party in Cherry Springs Pennsylvania, USA on September 3, 2005

Jerry Lodriguss

PIX4565862

Gazing at the stars - Observation of the sky with a bezel

Gazing at the stars - Observation of the sky with a bezel

Alex Conu

PIX4565920

La Silla Observatory - Danish Telescope of 1.54m - La Silla observatory - Danish 1.54m telescope - La Silla Observatory, Danish telescope of 1.54m in diameter. 2006. Danish 1.54m telescope in La Silla observatory, Chile. 2006

La Silla Observatory - Danish Telescope of 1.54m - La Silla observatory - Danish 1.54m telescope - La Silla Observatory, Danish telescope of 1.54m in diameter. 2006. Danish 1.54m telescope in La Silla observatory, Chile. 2006

Stefan Seip

PIX4656322

Star field in the constellation Sagittarius - Starfield in Sagittarius - Stars in Sagittarius towards the galactic center seen by the Hubble space telescope in February 2004. This field contains approximately 150,000 stars, down to 30th magnitude. The stars in the Galactic disk and bulge have a mixture of colors and masses. Image taken with the Hubble space telescope in february 2004

Star field in the constellation Sagittarius - Starfield in Sagittarius - Stars in Sagittarius towards the galactic center seen by the Hubble space telescope in February 2004. This field contains approximately 150,000 stars, down to 30th magnitude. The stars in the Galactic disk and bulge have a mixture of colors and masses. Image taken with the Hubble space telescope in february 2004

PIX4572231

Star V838 Monocerotis. 11/2005 - Star V838 Monocerotis seen by the Hubble space telescope. 11/2005 - This variable star is located about 20,000 years ago - light from Earth in the constellation Unicorn. Beginning in 2002, this star illuminated temporarily becoming one of the brightest stars in the sky. Viewed here in November 2005 by the Hubble space telescope, the light echo reveals details in the interstellar dust surrounding the star. Light from a star that erupted almost five years ago continues propagating outward through a cloud of dust surrounding the star. The light reflects or “” echoes”” off the dust and then travels to Earth. Because of the extra distance the scattered light travels, it reaches the Earth long after the light from the stellar outburst itself. Therefore, a light echo is an analog of a sound echo produced, for example, when sound from an Alpine yodeler echoes off of the surrounding mountainsides. The echo comes from the unusual variable star V838 Monocerotis (V

Star V838 Monocerotis. 11/2005 - Star V838 Monocerotis seen by the Hubble space telescope. 11/2005 - This variable star is located about 20,000 years ago - light from Earth in the constellation Unicorn. Beginning in 2002, this star illuminated temporarily becoming one of the brightest stars in the sky. Viewed here in November 2005 by the Hubble space telescope, the light echo reveals details in the interstellar dust surrounding the star. Light from a star that erupted almost five years ago continues propagating outward through a cloud of dust surrounding the star. The light reflects or “” echoes”” off the dust and then travels to Earth. Because of the extra distance the scattered light travels, it reaches the Earth long after the light from the stellar outburst itself. Therefore, a light echo is an analog of a sound echo produced, for example, when sound from an Alpine yodeler echoes off of the surrounding mountainsides. The echo comes from the unusual variable star V838 Monocerotis (V

PIX4572295

Star V838 Monocerotis. 09/2006 - V838 Monocerotis seen by the Hubble space telescope. 09/2006 - This variable star is located about 20,000 years ago - light from Earth in the constellation of Unicorn. Beginning in 2002, this star illuminated temporarily becoming one of the brightest stars in the sky. Viewed here in September 2006 by the Hubble space telescope, the light echo reveals details in the interstellar dust surrounding the star. Light from a star that erupted almost five years ago continues propagating outward through a cloud of dust surrounding the star. The light reflects or “” echoes”” off the dust and then travels to Earth. Because of the extra distance the scattered light travels, it reaches the Earth long after the light from the stellar outburst itself. Therefore, a light echo is an analog of a sound echo produced, for example, when sound from an Alpine yodeler echoes off of the surrounding mountainsides. The echo comes from the unusual variable star V838 Monocerotis (V8

Star V838 Monocerotis. 09/2006 - V838 Monocerotis seen by the Hubble space telescope. 09/2006 - This variable star is located about 20,000 years ago - light from Earth in the constellation of Unicorn. Beginning in 2002, this star illuminated temporarily becoming one of the brightest stars in the sky. Viewed here in September 2006 by the Hubble space telescope, the light echo reveals details in the interstellar dust surrounding the star. Light from a star that erupted almost five years ago continues propagating outward through a cloud of dust surrounding the star. The light reflects or “” echoes”” off the dust and then travels to Earth. Because of the extra distance the scattered light travels, it reaches the Earth long after the light from the stellar outburst itself. Therefore, a light echo is an analog of a sound echo produced, for example, when sound from an Alpine yodeler echoes off of the surrounding mountainsides. The echo comes from the unusual variable star V838 Monocerotis (V8

PIX4572319

Barree spiral galaxy NGC 4394 in Berenice's Hair - Barred spiral galaxy NGC 4394 in Coma Berenices: NGC 4394 is a barree spiral galaxy located in the Virgin's cluster about 55 million light years from Earth. Image obtained by the Hubble Space Telescope (HST) - Discovered in 1784 by the German-British astronomer William Herschel, NGC 4394 is a barred spiral galaxy situated about 55 million light-years from Earth. The galaxy lies in the constellation of Coma Berenices (Berenice's Hair), and is considered to be a member of the Virgo Cluster. NGC 4394 is the archetypal barred spiral galaxy, with bright spiral arms emerging from the ends of a bar that cuts through the galaxy's central bulge. These arms are peppered with young blue stars, dark filaments of cosmic dust, and bright, fuzzy regions of active star formation. At the centre of NGC 4394 lies a region of ionised gas known as a LINER. Liners are active regions that display a characteristic set of emission lines in their spectra- mostl

Barree spiral galaxy NGC 4394 in Berenice's Hair - Barred spiral galaxy NGC 4394 in Coma Berenices: NGC 4394 is a barree spiral galaxy located in the Virgin's cluster about 55 million light years from Earth. Image obtained by the Hubble Space Telescope (HST) - Discovered in 1784 by the German-British astronomer William Herschel, NGC 4394 is a barred spiral galaxy situated about 55 million light-years from Earth. The galaxy lies in the constellation of Coma Berenices (Berenice's Hair), and is considered to be a member of the Virgo Cluster. NGC 4394 is the archetypal barred spiral galaxy, with bright spiral arms emerging from the ends of a bar that cuts through the galaxy's central bulge. These arms are peppered with young blue stars, dark filaments of cosmic dust, and bright, fuzzy regions of active star formation. At the centre of NGC 4394 lies a region of ionised gas known as a LINER. Liners are active regions that display a characteristic set of emission lines in their spectra- mostl

PIX4611351

The Earl of Rosse's Great Telescope at Parsonstown (engraving)

The Earl of Rosse's Great Telescope at Parsonstown (engraving)

English School, (19th century)

LIP1100738

Sir Martin Ryle

Sir Martin Ryle

UIG3585593

The Hubble space telescope

The Hubble space telescope

UDK844647

Galaxy NGC 6384 in Ophiuchus - Galaxy NGC 6384 in Ophiuchus - The spiral galaxy NGC 6384, is located about 80 million years ago - light from Earth in the constellation Ophiuchus. Image obtained by the Hubble Space Telescope (HST). The NASA/ESA Hubble Space Telescope has produced this finely detailed image of the beautiful spiral galaxy NGC 6384. This galaxy lies 80 million light years away in the constellation of Ophiuchus (The Serpent Bearer), not far from the centre of the Milky Way on the sky. The positioning of NGC 6384 means that we have to peer at it past many dazzling foreground Milky Way stars that are scattered across this image

Galaxy NGC 6384 in Ophiuchus - Galaxy NGC 6384 in Ophiuchus - The spiral galaxy NGC 6384, is located about 80 million years ago - light from Earth in the constellation Ophiuchus. Image obtained by the Hubble Space Telescope (HST). The NASA/ESA Hubble Space Telescope has produced this finely detailed image of the beautiful spiral galaxy NGC 6384. This galaxy lies 80 million light years away in the constellation of Ophiuchus (The Serpent Bearer), not far from the centre of the Milky Way on the sky. The positioning of NGC 6384 means that we have to peer at it past many dazzling foreground Milky Way stars that are scattered across this image

PIX4612914

The elliptical galaxy NGC 4458 - The elliptical galaxy NGC 4458 - The galaxy NGC 4458 is 53 million years away - light from Earth, in the Virgin's cluster. Image obtained by the Hubble Space Telescope. The elliptical galaxy NGC 4458 lies at a distance of 53 million light - years from the Sun in the spring constellation Virgo. This image was made from data taken with Hubble space telescope

The elliptical galaxy NGC 4458 - The elliptical galaxy NGC 4458 - The galaxy NGC 4458 is 53 million years away - light from Earth, in the Virgin's cluster. Image obtained by the Hubble Space Telescope. The elliptical galaxy NGC 4458 lies at a distance of 53 million light - years from the Sun in the spring constellation Virgo. This image was made from data taken with Hubble space telescope

PIX4611377

Pluto - Hubble's Full Photomap of Pluto - The dwarf planet Pluto seen by the Hubble space telescope. These images, recomposed by computer from cliches obtained in 2002 and 2003, are not sufficiently precise to show Pluto's surface in detail but reveal color differences. This is the most detailed view to date of the entire surface of the dwarf planet Pluto, as constructed from multiple NASA Hubble Space Telescope photographs taken from 2002 to 2003. Hubble's view isn't sharp enough to see craters or mountains, if they exist on the surface, but Hubble reveals a complex - looking and variegated world with white, dark - orange, and charcoal - black terrain. The overall color is believed to be a result of ultraviolet radiation from the distant Sun breaking up methane that is present on Pluto's surface, leaving behind a dark, molasse - colored, carbon - rich residue. The center disk (180 degrees) has a mysterious bright spot that is unusually rich in carbon monoxide frost. This region will b

Pluto - Hubble's Full Photomap of Pluto - The dwarf planet Pluto seen by the Hubble space telescope. These images, recomposed by computer from cliches obtained in 2002 and 2003, are not sufficiently precise to show Pluto's surface in detail but reveal color differences. This is the most detailed view to date of the entire surface of the dwarf planet Pluto, as constructed from multiple NASA Hubble Space Telescope photographs taken from 2002 to 2003. Hubble's view isn't sharp enough to see craters or mountains, if they exist on the surface, but Hubble reveals a complex - looking and variegated world with white, dark - orange, and charcoal - black terrain. The overall color is believed to be a result of ultraviolet radiation from the distant Sun breaking up methane that is present on Pluto's surface, leaving behind a dark, molasse - colored, carbon - rich residue. The center disk (180 degrees) has a mysterious bright spot that is unusually rich in carbon monoxide frost. This region will b

PIX4624313

The VISTA telescope - Chile - The VISTA telecope - Chile: The dome of the 4.1m VISTA telescope seen from the VLT, in the Atacama desert in Chile. The Vista, 4.1 meter wide-field telescope for Infrared survey seen from VLT in Atacama Desert.

The VISTA telescope - Chile - The VISTA telecope - Chile: The dome of the 4.1m VISTA telescope seen from the VLT, in the Atacama desert in Chile. The Vista, 4.1 meter wide-field telescope for Infrared survey seen from VLT in Atacama Desert.

Alex Tudorica

PIX4657630

The planet Saturn observed with the Hubble space telescope in October 1998. Saturn is 120,000 km in diameter: The Planet Saturn seen by the Hubble Space Telescope in 1998 - Saturn seen from the Hubble Space Telescope in october 1998.

The planet Saturn observed with the Hubble space telescope in October 1998. Saturn is 120,000 km in diameter: The Planet Saturn seen by the Hubble Space Telescope in 1998 - Saturn seen from the Hubble Space Telescope in october 1998.

PIX4624799

Paranal Observatory, Chile 03/2008 - Paranal Observatory, Chile 03/2008 - Panorama of the Paranal Observatory at dusk. March 2008. Paranal Observatory is an astronomical observatory located on the top of Cerro Paranal in the Atacama Desert in the northern part of Chile. March 2008

Paranal Observatory, Chile 03/2008 - Paranal Observatory, Chile 03/2008 - Panorama of the Paranal Observatory at dusk. March 2008. Paranal Observatory is an astronomical observatory located on the top of Cerro Paranal in the Atacama Desert in the northern part of Chile. March 2008

Stephane Guisard

PIX4657141

Saturn by the Hubble Space Telecope - natural colors - 11/1999 - Saturn seen from the Hubble Space Telescope in november 1999 - The Saturn Planet observed with the Hubble Space Telescope in November 1999. Saturn is 120,000 km in diameter

Saturn by the Hubble Space Telecope - natural colors - 11/1999 - Saturn seen from the Hubble Space Telescope in november 1999 - The Saturn Planet observed with the Hubble Space Telescope in November 1999. Saturn is 120,000 km in diameter

PIX4624826

Constellation of the Altar - Constellations of Ara, Norma and Telescopium - The Altar is a constellation of the southern hemisphere located between the Centaur and the Wolf. Also visible are the constellations of the Rule and the Telescope. Ara (the Altar) is an inconspicuous constellation in the southern sky. It was once considered part of Centaurus and Lupus but became separated when the 'modern' constellation Norma was created by Lacaille in the 1750s. It was recognised by the Greeks and Romans and was visualised as the altar on which the Centaur, Centaurus, was to sacrifice Lupus, the Wolf. This is reflected in its Latin name, Ara Centauri. The constellation is the 63rd largest in the sky and covers about 237 square degrees. The best - known objects in this field are some diffuse dusty nebulae and star clusters. The only named star in Ara is Karnot Mizbeach (ss Ara). Best seen in the early evening in July

Constellation of the Altar - Constellations of Ara, Norma and Telescopium - The Altar is a constellation of the southern hemisphere located between the Centaur and the Wolf. Also visible are the constellations of the Rule and the Telescope. Ara (the Altar) is an inconspicuous constellation in the southern sky. It was once considered part of Centaurus and Lupus but became separated when the 'modern' constellation Norma was created by Lacaille in the 1750s. It was recognised by the Greeks and Romans and was visualised as the altar on which the Centaur, Centaurus, was to sacrifice Lupus, the Wolf. This is reflected in its Latin name, Ara Centauri. The constellation is the 63rd largest in the sky and covers about 237 square degrees. The best - known objects in this field are some diffuse dusty nebulae and star clusters. The only named star in Ara is Karnot Mizbeach (ss Ara). Best seen in the early evening in July

PIX4589021

Spiral galaxy NGC 3147 in the constellation Dragon

Spiral galaxy NGC 3147 in the constellation Dragon

PIX5940204

Sun Unit Telescope 1 & Moon Unit Telescope 2 (photo)

Sun Unit Telescope 1 & Moon Unit Telescope 2 (photo)

UIG2915903

Shooting star on the Tenerife Observatory - Fireball above Teide observatory: A lightning speed -8.5 passes over the solar laboratory (SolarLab) of the Teide Observatory, Tenerife, Canary Islands. In the sky, the brightest point at the top of the image is the planet Jupiter, in the constellation of Taurus. November 11, 2012. A -8.5m fireball photographed at the Observatorio del Teide, in Tenerife, Canary Islands. The pyramidal building is a solar telescope (SolarLab) and the red light is produced by someone walking around to his camera

Shooting star on the Tenerife Observatory - Fireball above Teide observatory: A lightning speed -8.5 passes over the solar laboratory (SolarLab) of the Teide Observatory, Tenerife, Canary Islands. In the sky, the brightest point at the top of the image is the planet Jupiter, in the constellation of Taurus. November 11, 2012. A -8.5m fireball photographed at the Observatorio del Teide, in Tenerife, Canary Islands. The pyramidal building is a solar telescope (SolarLab) and the red light is produced by someone walking around to his camera

Alex Tudorica

PIX4656579

Spiral Galaxy M81 viewed from the Hubble Space Telescope. Credit NASA. Science Astronomy Stellar

Spiral Galaxy M81 viewed from the Hubble Space Telescope. Credit NASA. Science Astronomy Stellar

UIG528807

Astronomy. Observing a solar eclipse on January 1, 1907, near the Cherniaevo Station in the Tian-Shan mountains, Golodnaia Steppe, Kazakhstan, Jan 1, 1907

Astronomy. Observing a solar eclipse on January 1, 1907, near the Cherniaevo Station in the Tian-Shan mountains, Golodnaia Steppe, Kazakhstan, Jan 1, 1907

EVB2929505

Spiral galaxy IC 391 in the Giraffe - Spiral galaxy IC 391 in Camelopardalis - Spiral galaxy IC 391 located about 80 million years ago - light in the constellation Giraffe. Image obtained with the Hubble Space Telescope (HST). IC 391 lies about 80 million light - years away in the constellation of Camelopardalis (the Giraffe) in the far northern part of the sky. The British amateur observer William Denning discovered it in the late nineteenth century, and described it as faint, small and round. Image taken with the Hubble space Telescope (HST)

Spiral galaxy IC 391 in the Giraffe - Spiral galaxy IC 391 in Camelopardalis - Spiral galaxy IC 391 located about 80 million years ago - light in the constellation Giraffe. Image obtained with the Hubble Space Telescope (HST). IC 391 lies about 80 million light - years away in the constellation of Camelopardalis (the Giraffe) in the far northern part of the sky. The British amateur observer William Denning discovered it in the late nineteenth century, and described it as faint, small and round. Image taken with the Hubble space Telescope (HST)

PIX4613272

The elliptical galaxy NGC 4660 - The elliptical galaxy NGC 4660 - The galaxy NGC 4660 is located 49 million years ago - light from Earth, in the Virgin's cluster. Image obtained by the Hubble Space Telescope. The elliptical galaxy NGC 4660 lies at a distance of 49 million light - years from the Sun in the spring constellation Virgo. This image was made from data taken with Hubble space telescope

The elliptical galaxy NGC 4660 - The elliptical galaxy NGC 4660 - The galaxy NGC 4660 is located 49 million years ago - light from Earth, in the Virgin's cluster. Image obtained by the Hubble Space Telescope. The elliptical galaxy NGC 4660 lies at a distance of 49 million light - years from the Sun in the spring constellation Virgo. This image was made from data taken with Hubble space telescope

PIX4611798

Bright Spiral Galaxy M81 viewed from the Hubble telescope. Credit NASA. Science Astronomy Stellar Space

Bright Spiral Galaxy M81 viewed from the Hubble telescope. Credit NASA. Science Astronomy Stellar Space

UIG528801

Supernova 19i87A observed with Huble Space Telescope, wide field planetary telescope 2. NASA photograph.

Supernova 19i87A observed with Huble Space Telescope, wide field planetary telescope 2. NASA photograph.

UIG538947

Mobile refracting telescope with achromatic lens, brass, by Giuseppe Megele (1740-1816) Detail

Mobile refracting telescope with achromatic lens, brass, by Giuseppe Megele (1740-1816) Detail

DGA2581694

Gazing at the stars - Observation of the sky with a bezel

Gazing at the stars - Observation of the sky with a bezel

Alex Conu

PIX4565936

Galaxy NGC 891 in Andromede - Edge-on spiral galaxy NGC 891 in Andromeda: Spiral galaxy seen by the slice located at a distance of 10 million light-years. Composite image. Located about 10 million light years from Earth, NGC 891 is one of the most photographed edge-on spiral galaxies in the northern skies. Composite Image made from multiple data sources.

Galaxy NGC 891 in Andromede - Edge-on spiral galaxy NGC 891 in Andromeda: Spiral galaxy seen by the slice located at a distance of 10 million light-years. Composite image. Located about 10 million light years from Earth, NGC 891 is one of the most photographed edge-on spiral galaxies in the northern skies. Composite Image made from multiple data sources.

PIX4574271

Spiral Galaxy NGC 4522 - Galaxy Spiral NGC 4522 - Moving at a speed of 10 million km/h in the Virgin's galaxy cluster, this spiral galaxy loses some of its gas. NGC 4522 is located about 60 million light years away from Earth. Image obtained by the Hubble Space Telescope. NGC 4522 is a spectacular example of a spiral galaxy that is currently being stripped of its gas content. The galaxy is part of the Virgo galaxy cluster and its rapid motion within the cluster results in strong winds across the galaxy as the gas within is left behind. Scientists estimate that the galaxy is moving at more than 10 million kilometers per hour. A number of newly formed star clusters that developed in the stripped gas can be seen in the Hubble image. The stripped spiral galaxy is located some 60 million light - years away from Earth

Spiral Galaxy NGC 4522 - Galaxy Spiral NGC 4522 - Moving at a speed of 10 million km/h in the Virgin's galaxy cluster, this spiral galaxy loses some of its gas. NGC 4522 is located about 60 million light years away from Earth. Image obtained by the Hubble Space Telescope. NGC 4522 is a spectacular example of a spiral galaxy that is currently being stripped of its gas content. The galaxy is part of the Virgo galaxy cluster and its rapid motion within the cluster results in strong winds across the galaxy as the gas within is left behind. Scientists estimate that the galaxy is moving at more than 10 million kilometers per hour. A number of newly formed star clusters that developed in the stripped gas can be seen in the Hubble image. The stripped spiral galaxy is located some 60 million light - years away from Earth

PIX4611473

Jupiter seen by Hubble Space Telescope - Jupiter seen by HST - Image obtained on April 3, 2017 by Hubble Space Telescope. On April 3, 2017, as Jupiter made its nearest approach to Earth in a year, Nasa's Hubble Space Telescope viewed the solar system's largest planet in all of its up-close glory. At a distance of 415 million miles (668 million kilometers) from Earth, Jupiter offered spectacular views of its colorful, roiling atmosphere, the legendary Great Red Spot, and its smaller companion at farther southern latitudes dubbed “” Red Spot Jr.””

Jupiter seen by Hubble Space Telescope - Jupiter seen by HST - Image obtained on April 3, 2017 by Hubble Space Telescope. On April 3, 2017, as Jupiter made its nearest approach to Earth in a year, Nasa's Hubble Space Telescope viewed the solar system's largest planet in all of its up-close glory. At a distance of 415 million miles (668 million kilometers) from Earth, Jupiter offered spectacular views of its colorful, roiling atmosphere, the legendary Great Red Spot, and its smaller companion at farther southern latitudes dubbed “” Red Spot Jr.””

PIX4614034

Barree spiral galaxy NGC 2146 in the Giraffe - Barred spiral galaxy NGC 2146 in Camelopardalis - NGC 2146 is a barree spiral galaxy located about 70 million years ago - light from Earth in the constellation Giraffe (Camelopardalis). Image obtained by the Hubble Space Telescope (HST). NGC 2146 is classified as a barred spiral due to its shape, but the most distinctive feature is the dusty spiral arm that has looped in front of the galaxy's core as seen from our perspective. The forces required to pull this structure out of its natural shape and twist it up to 45 degrees are colossal. The most likely explanation is that a neighbouring galaxy is gravitationally perturbing it and distorting the orbits of many of NGC 2146's stars. It is probable that we are currently witnessing the end stages of a process which has been occurring for tens of millions of years. NCG 2146 is undergoing intense bouts of star formation, to such an extent that it is referred to as a starburst galaxy. This is a co

Barree spiral galaxy NGC 2146 in the Giraffe - Barred spiral galaxy NGC 2146 in Camelopardalis - NGC 2146 is a barree spiral galaxy located about 70 million years ago - light from Earth in the constellation Giraffe (Camelopardalis). Image obtained by the Hubble Space Telescope (HST). NGC 2146 is classified as a barred spiral due to its shape, but the most distinctive feature is the dusty spiral arm that has looped in front of the galaxy's core as seen from our perspective. The forces required to pull this structure out of its natural shape and twist it up to 45 degrees are colossal. The most likely explanation is that a neighbouring galaxy is gravitationally perturbing it and distorting the orbits of many of NGC 2146's stars. It is probable that we are currently witnessing the end stages of a process which has been occurring for tens of millions of years. NCG 2146 is undergoing intense bouts of star formation, to such an extent that it is referred to as a starburst galaxy. This is a co

PIX4609999

Sun Unit Telescope 1, Moon Unit Telescope 2, Southern Cross Unit Telescope 3, Venus Unit Telescope 4 (photo)

Sun Unit Telescope 1, Moon Unit Telescope 2, Southern Cross Unit Telescope 3, Venus Unit Telescope 4 (photo)

UIG2915896

This painterly portrait of a star-forming cloud, called NGC 346, is a combination of multiwavelength light from NASA's Spitzer Space Telescope (infrared), the European Southern Observatory's New Technology Telescope (visible), and the European Space Agency's XMM-Newton space telescope (X-ray).

This painterly portrait of a star-forming cloud, called NGC 346, is a combination of multiwavelength light from NASA's Spitzer Space Telescope (infrared), the European Southern Observatory's New Technology Telescope (visible), and the European Space Agency's XMM-Newton space telescope (X-ray).

UIG867119

Barree spiral galaxy UGC 12158 - Galaxy UGC 12158 - The galaxy UGC 12158, is about 400 million light years away from Earth in the constellation Pegase. In this image obtained by the Hubble space telescope, a blue star is visible near the center of the galaxy (lower left), it is a supernova, SN 2004ef. The galaxy captured in this image, called UGC 12158, certainly isn't camera - shy: this spiral stunner is posing face - on to the NASA/ESA Hubble Space Telescope's Advanced Camera for Surveys, revealing its structure in fine detail. UGC 12158 is an excellent example of a barred spiral galaxy in the Hubble sequence - - a scheme used to categorise galaxies based on their shapes. Barred spirals, as the name suggest, feature spectacular swirling arms of stars that emanate from a bar - shaped centre. Such bar structures are common, being found in about two thirds of spiral galaxies, and are thought to act as funnels, guiding gas to their galactic centres where it accumulates to form newborn st

Barree spiral galaxy UGC 12158 - Galaxy UGC 12158 - The galaxy UGC 12158, is about 400 million light years away from Earth in the constellation Pegase. In this image obtained by the Hubble space telescope, a blue star is visible near the center of the galaxy (lower left), it is a supernova, SN 2004ef. The galaxy captured in this image, called UGC 12158, certainly isn't camera - shy: this spiral stunner is posing face - on to the NASA/ESA Hubble Space Telescope's Advanced Camera for Surveys, revealing its structure in fine detail. UGC 12158 is an excellent example of a barred spiral galaxy in the Hubble sequence - - a scheme used to categorise galaxies based on their shapes. Barred spirals, as the name suggest, feature spectacular swirling arms of stars that emanate from a bar - shaped centre. Such bar structures are common, being found in about two thirds of spiral galaxies, and are thought to act as funnels, guiding gas to their galactic centres where it accumulates to form newborn st

PIX4613612

Spiral galaxy NGC 7331 in Pegase - Spiral galaxy NGC 7331 in Pegasus - The galaxy NGC 7331 is located about 50 million years away - light from Earth. The small galaxies around her form a cluster much farther away. Image obtained with the Hubble Space Telescope and Subaru Telescope. NGC 7331 is located 49 million light years away. The smaller galaxies visible are much farer

Spiral galaxy NGC 7331 in Pegase - Spiral galaxy NGC 7331 in Pegasus - The galaxy NGC 7331 is located about 50 million years away - light from Earth. The small galaxies around her form a cluster much farther away. Image obtained with the Hubble Space Telescope and Subaru Telescope. NGC 7331 is located 49 million light years away. The smaller galaxies visible are much farer

PIX4613142

Observatory of La Silla - Telescope LET - La Silla observatory. Chile. Leonard Euler Telescope - 1.2m Swiss Telescope Leonard Euler Telescope. La Silla Observatory, Chile. 11/05/2007. Swiss 1.2 meter Leonard Euler Telescope (LET). La Silla observatory, Chile

Observatory of La Silla - Telescope LET - La Silla observatory. Chile. Leonard Euler Telescope - 1.2m Swiss Telescope Leonard Euler Telescope. La Silla Observatory, Chile. 11/05/2007. Swiss 1.2 meter Leonard Euler Telescope (LET). La Silla observatory, Chile

Guillaume Blanchard

PIX4656309

Spiral galaxy NGC 2683 in Lynx - Spiral galaxy NGC 2683 in Lynx - Spiral galaxy NGC 2683 distant about 16 million years - light in the constellation Lynx. Image obtained by the Hubble Space Telescope (HST). NGC 2683 is a spiral galaxy seen almost edge - on, giving it the shape of a classic science fiction spaceship. The delicate dusty lanes of the spiral arms are silhouetted against the golden haze of the galaxy's core. In addition, brilliant clusters of young blue stars shine scattered throughout the disc, mapping the galaxy's star - forming regions. Perhaps surprisingly, side - on views of galaxies like this one do not prevent astronomers from deducing their structures. Studies of the properties of the light coming from NGC 2683 suggest that this is a barred spiral galaxy, even though the angle we see it at does not let us see this directly. NGC 2683, discovered on 5 February 1788 by the famous astronomer William Herschel, lies in the Northern constellation of Lynx. A constellation n

Spiral galaxy NGC 2683 in Lynx - Spiral galaxy NGC 2683 in Lynx - Spiral galaxy NGC 2683 distant about 16 million years - light in the constellation Lynx. Image obtained by the Hubble Space Telescope (HST). NGC 2683 is a spiral galaxy seen almost edge - on, giving it the shape of a classic science fiction spaceship. The delicate dusty lanes of the spiral arms are silhouetted against the golden haze of the galaxy's core. In addition, brilliant clusters of young blue stars shine scattered throughout the disc, mapping the galaxy's star - forming regions. Perhaps surprisingly, side - on views of galaxies like this one do not prevent astronomers from deducing their structures. Studies of the properties of the light coming from NGC 2683 suggest that this is a barred spiral galaxy, even though the angle we see it at does not let us see this directly. NGC 2683, discovered on 5 February 1788 by the famous astronomer William Herschel, lies in the Northern constellation of Lynx. A constellation n

PIX4610165

Spiral galaxy NGC 2683 in Lynx - Spiral galaxy NGC 2683 in Lynx - Spiral galaxy NGC 2683 distant about 16 million years - light in the constellation Lynx. Composite image obtained from the Hubble Space Telescope (HST) and the Subaru Telescope. Spiral galaxy NGC 2683 located 16 million years away in the constellation of Lynx. Composite image taken by the Hubble space telescope (HST) and Subaru

Spiral galaxy NGC 2683 in Lynx - Spiral galaxy NGC 2683 in Lynx - Spiral galaxy NGC 2683 distant about 16 million years - light in the constellation Lynx. Composite image obtained from the Hubble Space Telescope (HST) and the Subaru Telescope. Spiral galaxy NGC 2683 located 16 million years away in the constellation of Lynx. Composite image taken by the Hubble space telescope (HST) and Subaru

PIX4610150

Gamma ray telescope HESS - Gamma rays telescope HESS - High Energy Stereoscopic System (HESS) telescope located in Namibia near Gamsberg. This network of telescopes is dedicated to the study of high energy gamma rays. High Energy Stereoscopic System or HESS is a system of Imaging Atmospheric Cherenkov Telescopes (IACT) for the investigation of cosmic gamma rays. It is located in Namibia, near Gamsberg

Gamma ray telescope HESS - Gamma rays telescope HESS - High Energy Stereoscopic System (HESS) telescope located in Namibia near Gamsberg. This network of telescopes is dedicated to the study of high energy gamma rays. High Energy Stereoscopic System or HESS is a system of Imaging Atmospheric Cherenkov Telescopes (IACT) for the investigation of cosmic gamma rays. It is located in Namibia, near Gamsberg

Sebastian Voltmer

PIX4653334

Image of Mars from Hubble Space Telescope

Image of Mars from Hubble Space Telescope

UIG531595

Illustration of Astronomy, c.1771 (engraving)

Illustration of Astronomy, c.1771 (engraving)

European School, (18th century)

XJF745420

Sun Unit Telescope 1 & Moon Unit Telescope 2 (photo)

Sun Unit Telescope 1 & Moon Unit Telescope 2 (photo)

UIG2915905

Moon and planets above the Paranal Observatory - Paranal Observatory, Venus - Mercury - Mars - Moon conjunction - The Moon with the Venus planets (the brightest at the bottom right of the Moon), Mercury (to the right of the Moon) and Mars (to the top right of the Moon), seen on 1 September 2008 at the Paranal Observatory in Chile. Moon - Venus - Mercury - Mars conjunction in twilight. Paranal Observatory, Chile. Sep 1st 2008

Moon and planets above the Paranal Observatory - Paranal Observatory, Venus - Mercury - Mars - Moon conjunction - The Moon with the Venus planets (the brightest at the bottom right of the Moon), Mercury (to the right of the Moon) and Mars (to the top right of the Moon), seen on 1 September 2008 at the Paranal Observatory in Chile. Moon - Venus - Mercury - Mars conjunction in twilight. Paranal Observatory, Chile. Sep 1st 2008

Stephane Guisard

PIX4657158

Ancient astronomers.

Ancient astronomers.

UIG5307479

Switzerland Federal Observatory Zurich, 1970 (b/w photo)

Switzerland Federal Observatory Zurich, 1970 (b/w photo)

Stringer (STR)

KES6247782

Crab pulsar in nebula M1 - The Crab pulsar: This image from the Hubble space telescope shows the central region of the Crab nebula or resides its pulsar. The pulsar is visible in the center of the image. It is a very dense neutron star from the explosion of a massive supernova star. This star quickly rotates on itself developing a powerful magnetic field, emitting beams of light and radio waves. M1 is located about 6000 light-years in the constellation Taurus.. While many other images of the famous Crab Nebula have focused on the filaments in the outer part of the nebula, this image shows the very heart of the Crab Nebula including the central neutron star - it is the rightmost of the two bright stars near the centre of this image. The rapid motion of the material nearest to the central star is revealed by the subtle rainbow of colours in this time-lapse image, the rainbow effect being due to the movement of material over the time between one image and another

Crab pulsar in nebula M1 - The Crab pulsar: This image from the Hubble space telescope shows the central region of the Crab nebula or resides its pulsar. The pulsar is visible in the center of the image. It is a very dense neutron star from the explosion of a massive supernova star. This star quickly rotates on itself developing a powerful magnetic field, emitting beams of light and radio waves. M1 is located about 6000 light-years in the constellation Taurus.. While many other images of the famous Crab Nebula have focused on the filaments in the outer part of the nebula, this image shows the very heart of the Crab Nebula including the central neutron star - it is the rightmost of the two bright stars near the centre of this image. The rapid motion of the material nearest to the central star is revealed by the subtle rainbow of colours in this time-lapse image, the rainbow effect being due to the movement of material over the time between one image and another

PIX4583135

Constellations of the Telescopium and Sagittarius - The Telescope is a small constellation of the southern hemisphere located just above Sagittarius

Constellations of the Telescopium and Sagittarius - The Telescope is a small constellation of the southern hemisphere located just above Sagittarius

Christopher Picking

PIX4594195

Gamma ray telescope HESS - Gamma rays telescope HESS - High Energy Stereoscopic System (HESS) telescope located in Namibia near Gamsberg. This network of telescopes is dedicated to the study of high energy gamma rays. High Energy Stereoscopic System or HESS is a system of Imaging Atmospheric Cherenkov Telescopes (IACT) for the investigation of cosmic gamma rays. It is located in Namibia, near Gamsberg

Gamma ray telescope HESS - Gamma rays telescope HESS - High Energy Stereoscopic System (HESS) telescope located in Namibia near Gamsberg. This network of telescopes is dedicated to the study of high energy gamma rays. High Energy Stereoscopic System or HESS is a system of Imaging Atmospheric Cherenkov Telescopes (IACT) for the investigation of cosmic gamma rays. It is located in Namibia, near Gamsberg

Sebastian Voltmer

PIX4653270

Saturn seen from the Hubble space telescope in november 2000 - Saturn seen from the Hubble space telescope in november 2000 - Saturn planet observed with the Hubble space telescope in November 2000. Saturn is 120,000 km in diameter

Saturn seen from the Hubble space telescope in november 2000 - Saturn seen from the Hubble space telescope in november 2000 - Saturn planet observed with the Hubble space telescope in November 2000. Saturn is 120,000 km in diameter

PIX4624813

Spiral galaxy NGC 2683 in Lynx - Spiral galaxy NGC 2683 in Lynx - Spiral galaxy NGC 2683 distant about 16 million years - light in the constellation Lynx. Image obtained by the Hubble Space Telescope (HST). Spiral galaxy NGC 2683 located 16 million years away in the constellation of Lynx. Image taken by the Hubble space telescope (HST)

Spiral galaxy NGC 2683 in Lynx - Spiral galaxy NGC 2683 in Lynx - Spiral galaxy NGC 2683 distant about 16 million years - light in the constellation Lynx. Image obtained by the Hubble Space Telescope (HST). Spiral galaxy NGC 2683 located 16 million years away in the constellation of Lynx. Image taken by the Hubble space telescope (HST)

R. Gendler

PIX4610141

Spiral Galaxy NGC 634 - NGC 634 is a spiral galaxy located about 250 million light years away from Earth in the constellation Andromede. Image obtained by the Hubble Space Telescope (HST). NGC 634 is located 250 million light years away in the constellation of Andromeda. This spiral galaxy was discovered back in the nineteenth century by English astronomer Edouard Jean - Marie Stephan, but in 2008 it became a prime target for observations thanks to the violent demise of a white dwarf star. The type Ia supernova known as SN2008A was spotted in the galaxy and briefly rivalled the brilliance of its entire host galaxy but, despite the energy of the explosion, it can no longer be seen this Hubble image, which was taken around a year and a half later

Spiral Galaxy NGC 634 - NGC 634 is a spiral galaxy located about 250 million light years away from Earth in the constellation Andromede. Image obtained by the Hubble Space Telescope (HST). NGC 634 is located 250 million light years away in the constellation of Andromeda. This spiral galaxy was discovered back in the nineteenth century by English astronomer Edouard Jean - Marie Stephan, but in 2008 it became a prime target for observations thanks to the violent demise of a white dwarf star. The type Ia supernova known as SN2008A was spotted in the galaxy and briefly rivalled the brilliance of its entire host galaxy but, despite the energy of the explosion, it can no longer be seen this Hubble image, which was taken around a year and a half later

PIX4609410

In this processed Spitzer Space Telescope image, baby star HH 46/47 can be seen blowing two massive "bubbles." The star is 1,140 light-years away from Earth.

In this processed Spitzer Space Telescope image, baby star HH 46/47 can be seen blowing two massive "bubbles." The star is 1,140 light-years away from Earth.

UIG867108

Globular cluster NGC 288 - The Globular Cluster NGC 288 - NGC 288 is a cluster of stars located about 30,000 years - light from Earth in the constellation Sculptor. This image made by the Hubble space telescope highlights the different types of stars that coexist in the center of the cluster

Globular cluster NGC 288 - The Globular Cluster NGC 288 - NGC 288 is a cluster of stars located about 30,000 years - light from Earth in the constellation Sculptor. This image made by the Hubble space telescope highlights the different types of stars that coexist in the center of the cluster

PIX4564321

Globular cluster M71 in the Fleche - Globular cluster M71 in Sagitta - M71 is located about 12,000 light years away from Earth. Image of the central region of the cluster obtained by the Hubble space telescope. This NASA/ESA Hubble Space Telescope image shows a bright scattering of stars in the small constellation of Sagitta (the Arrow). This is the centre of the globular cluster Messier 71, a great ball of ancient stars on the edge of our galaxy around 13,000 light - years from Earth. M71 is around 27 light - years across. Globular clusters are like galactic suburbs, pockets of stars that exist on the edge of major galaxies. These clusters are tightly bound together by their gravitational attraction, hence their spherical shape and their name: globulus means little sphere”” in Latin. Around 150 such globular clusters are known to exist around our Milky Way, each one of them containing several hundred thousand stars. Despite being a familiar object, Messier 71's precise nature was disp

Globular cluster M71 in the Fleche - Globular cluster M71 in Sagitta - M71 is located about 12,000 light years away from Earth. Image of the central region of the cluster obtained by the Hubble space telescope. This NASA/ESA Hubble Space Telescope image shows a bright scattering of stars in the small constellation of Sagitta (the Arrow). This is the centre of the globular cluster Messier 71, a great ball of ancient stars on the edge of our galaxy around 13,000 light - years from Earth. M71 is around 27 light - years across. Globular clusters are like galactic suburbs, pockets of stars that exist on the edge of major galaxies. These clusters are tightly bound together by their gravitational attraction, hence their spherical shape and their name: globulus means little sphere”” in Latin. Around 150 such globular clusters are known to exist around our Milky Way, each one of them containing several hundred thousand stars. Despite being a familiar object, Messier 71's precise nature was disp

PIX4565068

Globular cluster NGC 6401 in Ophiuchus - Globular cluster NGC 6401 in Ophiuchus - The NASA/ESA Hubble Space Telescope has used its powerful optics to separate the globular cluster NGC 6401 into its constituent stars. What was once only visible as a ghostly mist in the eyepieces of astronomical instruments has been transformed into a stunning stellar landscape. NGC 6401 can be found within the constellation of Ophiuchus (The Serpent Bearer). The globular cluster itself is relatively faint, so a telescope and some observational experience are required to see it. Globular clusters are very rich, and generally spherical, collections of stars, hence the name. They orbit the cores of galaxies, with the force of gravity also keeping the stars bound as a group. There are around 160 globular clusters associated with our Milky Way, of which NGC 6401 is one. These objects are very old, containing some of the most ancient stars known. However, there are many mysteries surrounding them, with the or

Globular cluster NGC 6401 in Ophiuchus - Globular cluster NGC 6401 in Ophiuchus - The NASA/ESA Hubble Space Telescope has used its powerful optics to separate the globular cluster NGC 6401 into its constituent stars. What was once only visible as a ghostly mist in the eyepieces of astronomical instruments has been transformed into a stunning stellar landscape. NGC 6401 can be found within the constellation of Ophiuchus (The Serpent Bearer). The globular cluster itself is relatively faint, so a telescope and some observational experience are required to see it. Globular clusters are very rich, and generally spherical, collections of stars, hence the name. They orbit the cores of galaxies, with the force of gravity also keeping the stars bound as a group. There are around 160 globular clusters associated with our Milky Way, of which NGC 6401 is one. These objects are very old, containing some of the most ancient stars known. However, there are many mysteries surrounding them, with the or

PIX4564826

Paranal Observatory, Chile - Paranal Observatory, Chile - Yepun, one of the four 8.2m telescopes of the VLT (Very Large Telescope), and two of the four 1.8m auxiliary telescopes. On the horizon, the shadow of the Earth projected on the atmosphere, the belt of Venus (or anticrepuscular arch). January 2008. Paranal Observatory is an astronomical observatory located on the top of Cerro Paranal in the Atacama Desert in the northern part of Chile. This picture shows at left Yepun, one of the four 8,2m telescopes of the Very Large Telescope (VLT), with two auxiliary telescopes. Visible too, the anticrepuscular arch (or belt of Venus, the shadow of earth projected in the atmosphere) January 2008

Paranal Observatory, Chile - Paranal Observatory, Chile - Yepun, one of the four 8.2m telescopes of the VLT (Very Large Telescope), and two of the four 1.8m auxiliary telescopes. On the horizon, the shadow of the Earth projected on the atmosphere, the belt of Venus (or anticrepuscular arch). January 2008. Paranal Observatory is an astronomical observatory located on the top of Cerro Paranal in the Atacama Desert in the northern part of Chile. This picture shows at left Yepun, one of the four 8,2m telescopes of the Very Large Telescope (VLT), with two auxiliary telescopes. Visible too, the anticrepuscular arch (or belt of Venus, the shadow of earth projected in the atmosphere) January 2008

Guillaume Blanchard

PIX4657124

Amateur astronomer - Amateur astronomer - Amateur astronomer at the Paranal Observatory in Chile. FS128 bezel. Amateur astronomer at Paranal observatory in Chile. Takahashi FS128 refractor

Amateur astronomer - Amateur astronomer - Amateur astronomer at the Paranal Observatory in Chile. FS128 bezel. Amateur astronomer at Paranal observatory in Chile. Takahashi FS128 refractor

Stephane Guisard

PIX4566132

Amateur astronomer at La Silla Observatory in Chile - Amateur astronomer - Amateur astronomer at La Silla Observatory in Chile. Amateur astronomer at La Silla Observatory in Chile

Amateur astronomer at La Silla Observatory in Chile - Amateur astronomer - Amateur astronomer at La Silla Observatory in Chile. Amateur astronomer at La Silla Observatory in Chile

Stefan Seip

PIX4566001

Colliding galaxies NGC 2623 in Cancer - Colliding galaxies NGC 2623 - The galaxy NGC 2623 (Arp 243) is located about 250 million years ago - light from Earth in the constellation of Cancer. It is a system of two spiral galaxies colliding and eventually forming only one galaxy. This image was obtained by the Hubble Space Telescope in 2007. Located 250 million light - years away in the constellation of Cancer, these colliding galaxies are in the late stages of the merging process with the centres of the original galaxy pair now merged into one nucleus. Image obtained by the Hubble space telescope in 2007

Colliding galaxies NGC 2623 in Cancer - Colliding galaxies NGC 2623 - The galaxy NGC 2623 (Arp 243) is located about 250 million years ago - light from Earth in the constellation of Cancer. It is a system of two spiral galaxies colliding and eventually forming only one galaxy. This image was obtained by the Hubble Space Telescope in 2007. Located 250 million light - years away in the constellation of Cancer, these colliding galaxies are in the late stages of the merging process with the centres of the original galaxy pair now merged into one nucleus. Image obtained by the Hubble space telescope in 2007

PIX4610122

Spiral galaxy NGC 1313 in the Reticule - The starburst galaxy NGC 1313 - NGC 1313 is a galaxy located about 15 million years ago - light. Intense star formations are observed. Image made with one of the 8.2m telescopes of the VLT in Chile. NGC 1313 is a galaxy hardly affected by starburst activity. It lies at a distance of about 15 million light years. Image taken by the Very Large Telescope

Spiral galaxy NGC 1313 in the Reticule - The starburst galaxy NGC 1313 - NGC 1313 is a galaxy located about 15 million years ago - light. Intense star formations are observed. Image made with one of the 8.2m telescopes of the VLT in Chile. NGC 1313 is a galaxy hardly affected by starburst activity. It lies at a distance of about 15 million light years. Image taken by the Very Large Telescope

PIX4609756

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