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The Coronation of The Virgin, The Veil Of Veronique And Saints (Detail) (oil on canvas, 17th century)
The Coronation of The Virgin, The Veil Of Veronique And Saints (Detail) (oil on canvas, 17th century)

LRI4611420: The Coronation of The Virgin, The Veil Of Veronique And Saints (Detail) (oil on canvas, 17th century), Serodine, Giovanni (c.1600-30) / Bridgeman Images

ID: LRI4611420

The Coronation of The Virgin, The Veil Of Veronique And Saints (Detail) (oil on canvas, 17th century)

Serodine, Giovanni (c.1600-30)

Portrait of Catherine de Brunswick Grubenhagen, 16th century (oil on canvas)
Portrait of Catherine de Brunswick Grubenhagen, 16th century (oil on canvas)

JLJ4572768: Portrait of Catherine de Brunswick Grubenhagen, 16th century (oil on canvas), Cranach, Lucas the Elder (1472-1553) / Bridgeman Images

ID: JLJ4572768

Portrait of Catherine de Brunswick Grubenhagen, 16th century (oil on canvas)

Cranach, Lucas the Elder (1472-1553)

Artist's view of a magnetar and its magnetic field - A magnetar with its magnetic field. Artwork - Illustration showing the magnetic field lines of a magnetar. This artist's concept shows a magnetar - - a neutron star with a super - strong magnetic field, represented by the lines in this illustration
Artist's view of a magnetar and its magnetic field - A magnetar with its magnetic field. Artwork - Illustration showing the magnetic field lines of a magnetar. This artist's concept shows a magnetar - - a neutron star with a super - strong magnetic field, represented by the lines in this illustration

PIX4572809: Artist's view of a magnetar and its magnetic field - A magnetar with its magnetic field. Artwork - Illustration showing the magnetic field lines of a magnetar. This artist's concept shows a magnetar - - a neutron star with a super - strong magnetic field, represented by the lines in this illustration / Bridgeman Images

ID: PIX4572809

Artist's view of a magnetar and its magnetic field - A magnetar with its magnetic field. Artwork - Illustration showing the magnetic field lines of a magnetar. This artist's concept shows a magnetar - - a neutron star with a super - strong magnetic field, represented by the lines in this illustration

Madame de Julienne and Madame de Serre doing music by Louis carrogis dit Carmontelle, 18th century (w/c)
Madame de Julienne and Madame de Serre doing music by Louis carrogis dit Carmontelle, 18th century (w/c)

JLJ4572836: Madame de Julienne and Madame de Serre doing music by Louis carrogis dit Carmontelle, 18th century (w/c), Carmontelle, Louis Carrogis (1717-1806) / Bridgeman Images

ID: JLJ4572836

Madame de Julienne and Madame de Serre doing music by Louis carrogis dit Carmontelle, 18th century (w/c)

Carmontelle, Louis Carrogis (1717-1806)

Binary pulsar and gravitational waves - Artist's impression of the pulsar PSR J0348+0432 and its white dwarf companion - Artist's view of a gravitational wave generated by a system of a neutron star associated with a white dwarf, spreading on the fabric of space - time. This artist's impression shows the exotic double object that consists of a tiny, but very heavy neutron star that spins 25 times each second, orbited every two and a half hours by a white dwarf star. The neutron star is a pulsar named PSR J0348+0432 that is giving off radio waves that can be picked up on Earth by radio telescopes. Although this unusual pair is very interesting in its own right it is also a unique laboratory for testing the limits of physical theories. This system is radiating gravitational radiation, ripples in spacetime. Although these waves cannot be detected directly by astronomers on Earth they can be detected indirectly by measuring the change in the orbit of the system as it loses energy. As the pulsar is so small the relative sizes of the two objects are not drawn to scale
Binary pulsar and gravitational waves - Artist's impression of the pulsar PSR J0348+0432 and its white dwarf companion - Artist's view of a gravitational wave generated by a system of a neutron star associated with a white dwarf, spreading on the fabric of space - time. This artist's impression shows the exotic double object that consists of a tiny, but very heavy neutron star that spins 25 times each second, orbited every two and a half hours by a white dwarf star. The neutron star is a pulsar named PSR J0348+0432 that is giving off radio waves that can be picked up on Earth by radio telescopes. Although this unusual pair is very interesting in its own right it is also a unique laboratory for testing the limits of physical theories. This system is radiating gravitational radiation, ripples in spacetime. Although these waves cannot be detected directly by astronomers on Earth they can be detected indirectly by measuring the change in the orbit of the system as it loses energy. As the pulsar is so small the relative sizes of the two objects are not drawn to scale

PIX4572892: Binary pulsar and gravitational waves - Artist's impression of the pulsar PSR J0348+0432 and its white dwarf companion - Artist's view of a gravitational wave generated by a system of a neutron star associated with a white dwarf, spreading on the fabric of space - time. This artist's impression shows the exotic double object that consists of a tiny, but very heavy neutron star that spins 25 times each second, orbited every two and a half hours by a white dwarf star. The neutron star is a pulsar named PSR J0348+0432 that is giving off radio waves that can be picked up on Earth by radio telescopes. Although this unusual pair is very interesting in its own right it is also a unique laboratory for testing the limits of physical theories. This system is radiating gravitational radiation, ripples in spacetime. Although these waves cannot be detected directly by astronomers on Earth they can be detected indirectly by measuring the change in the orbit of the system as it loses energy. As the pulsar is so small the relative sizes of the two objects are not drawn to scale / Bridgeman Images

ID: PIX4572892

Binary pulsar and gravitational waves - Artist's impression of the pulsar PSR J0348+0432 and its white dwarf companion - Artist's view of a gravitational wave generated by a system of a neutron star associated with a white dwarf, spreading on the fabric of space - time. This artist's impression shows the exotic double object that consists of a tiny, but very heavy neutron star that spins 25 times each second, orbited every two and a half hours by a white dwarf star. The neutron star is a pulsar named PSR J0348+0432 that is giving off radio waves that can be picked up on Earth by radio telescopes. Although this unusual pair is very interesting in its own right it is also a unique laboratory for testing the limits of physical theories. This system is radiating gravitational radiation, ripples in spacetime. Although these waves cannot be detected directly by astronomers on Earth they can be detected indirectly by measuring the change in the orbit of the system as it loses energy. As the p

L'apprentice, 1908 (oil on canvas)
L'apprentice, 1908 (oil on canvas)

JLJ4572926: L'apprentice, 1908 (oil on canvas), Raffaelli, Jean Francois (1850-1924) / Bridgeman Images

ID: JLJ4572926

L'apprentice, 1908 (oil on canvas)

Raffaelli, Jean Francois (1850-1924)

Planet around the star Fomalhaut - Planet orbiting star Fomalhaut - First visible light photo of an extrasolar planet obtained by the space telescope Hubble. The planet called Fomalhaut b, is a planet with a mass close to Jupiter, orbiting the star Fomalhaut, 25 years - light from Earth in the constellation of Southern Fish. The star Fomalhaut (indicated by a white dot) is hidden here to show the dust disc surrounding it and the position of the planet. Located at a distance of about four times that separating Neptune from the Sun, Fomalhaut b makes a complete orbit around its star in 872 years. November 2008 - This image, taken with the Advanced Camera for Surveys aboard the NASA/ESA Hubble Space Telescope, shows the newly discovered planet, Fomalhaut b, orbiting its parent star, Fomalhaut. The small white box at lower right pinpoints the planet's location. Fomalhaut b has carved a path along the inner edge of a vast, dusty debris ring encircling Fomalhaut that is 34.5 billion kilometers across. Fomalhaut b lies three billion kilometers inside the ring's inner edge and orbits 17 billion kilometers from its star. The inset at bottom right is a composite image showing the planet's position during Hubble observations taken in 2004 and 2006. Astronomers have calculated that Fomalhaut b completes an orbit around its parent star every 872 years. The white dot in the centre of the image marks the star's location. The region around Fomalhaut's location is black because astronomers used the Advanced Camera's coronagraph to block out the star's bright glare so that the dim planet could be seen. Fomalhaut b is 100 million times fainter than its star. The radial streaks are scattered starlight. The red dot at lower left is a background star. The Fomalhaut system is 25 light - years away in the constellation Piscis Austrinus. This false - colour image was taken in October 2004 and July 2006
Planet around the star Fomalhaut - Planet orbiting star Fomalhaut - First visible light photo of an extrasolar planet obtained by the space telescope Hubble. The planet called Fomalhaut b, is a planet with a mass close to Jupiter, orbiting the star Fomalhaut, 25 years - light from Earth in the constellation of Southern Fish. The star Fomalhaut (indicated by a white dot) is hidden here to show the dust disc surrounding it and the position of the planet. Located at a distance of about four times that separating Neptune from the Sun, Fomalhaut b makes a complete orbit around its star in 872 years. November 2008 - This image, taken with the Advanced Camera for Surveys aboard the NASA/ESA Hubble Space Telescope, shows the newly discovered planet, Fomalhaut b, orbiting its parent star, Fomalhaut. The small white box at lower right pinpoints the planet's location. Fomalhaut b has carved a path along the inner edge of a vast, dusty debris ring encircling Fomalhaut that is 34.5 billion kilometers across. Fomalhaut b lies three billion kilometers inside the ring's inner edge and orbits 17 billion kilometers from its star. The inset at bottom right is a composite image showing the planet's position during Hubble observations taken in 2004 and 2006. Astronomers have calculated that Fomalhaut b completes an orbit around its parent star every 872 years. The white dot in the centre of the image marks the star's location. The region around Fomalhaut's location is black because astronomers used the Advanced Camera's coronagraph to block out the star's bright glare so that the dim planet could be seen. Fomalhaut b is 100 million times fainter than its star. The radial streaks are scattered starlight. The red dot at lower left is a background star. The Fomalhaut system is 25 light - years away in the constellation Piscis Austrinus. This false - colour image was taken in October 2004 and July 2006

PIX4573107: Planet around the star Fomalhaut - Planet orbiting star Fomalhaut - First visible light photo of an extrasolar planet obtained by the space telescope Hubble. The planet called Fomalhaut b, is a planet with a mass close to Jupiter, orbiting the star Fomalhaut, 25 years - light from Earth in the constellation of Southern Fish. The star Fomalhaut (indicated by a white dot) is hidden here to show the dust disc surrounding it and the position of the planet. Located at a distance of about four times that separating Neptune from the Sun, Fomalhaut b makes a complete orbit around its star in 872 years. November 2008 - This image, taken with the Advanced Camera for Surveys aboard the NASA/ESA Hubble Space Telescope, shows the newly discovered planet, Fomalhaut b, orbiting its parent star, Fomalhaut. The small white box at lower right pinpoints the planet's location. Fomalhaut b has carved a path along the inner edge of a vast, dusty debris ring encircling Fomalhaut that is 34.5 billion kilometers across. Fomalhaut b lies three billion kilometers inside the ring's inner edge and orbits 17 billion kilometers from its star. The inset at bottom right is a composite image showing the planet's position during Hubble observations taken in 2004 and 2006. Astronomers have calculated that Fomalhaut b completes an orbit around its parent star every 872 years. The white dot in the centre of the image marks the star's location. The region around Fomalhaut's location is black because astronomers used the Advanced Camera's coronagraph to block out the star's bright glare so that the dim planet could be seen. Fomalhaut b is 100 million times fainter than its star. The radial streaks are scattered starlight. The red dot at lower left is a background star. The Fomalhaut system is 25 light - years away in the constellation Piscis Austrinus. This false - colour image was taken in October 2004 and July 2006 / Bridgeman Images

ID: PIX4573107

Planet around the star Fomalhaut - Planet orbiting star Fomalhaut - First visible light photo of an extrasolar planet obtained by the space telescope Hubble. The planet called Fomalhaut b, is a planet with a mass close to Jupiter, orbiting the star Fomalhaut, 25 years - light from Earth in the constellation of Southern Fish. The star Fomalhaut (indicated by a white dot) is hidden here to show the dust disc surrounding it and the position of the planet. Located at a distance of about four times that separating Neptune from the Sun, Fomalhaut b makes a complete orbit around its star in 872 years. November 2008 - This image, taken with the Advanced Camera for Surveys aboard the NASA/ESA Hubble Space Telescope, shows the newly discovered planet, Fomalhaut b, orbiting its parent star, Fomalhaut. The small white box at lower right pinpoints the planet's location. Fomalhaut b has carved a path along the inner edge of a vast, dusty debris ring encircling Fomalhaut that is 34.5 billion kilomete

Portrait of Woman, 16th century (oil on canvas)
Portrait of Woman, 16th century (oil on canvas)

JLJ4573119: Portrait of Woman, 16th century (oil on canvas), Zacchia, Paolo (fl.1519-61) / Bridgeman Images

ID: JLJ4573119

Portrait of Woman, 16th century (oil on canvas)

Zacchia, Paolo (fl.1519-61)

Diane and nymph Callisto Diane surprises the pregnant callisto nymph of Zeus, The Nymph hides her pregnancy, 17th century (oil on canvas)
Diane and nymph Callisto Diane surprises the pregnant callisto nymph of Zeus, The Nymph hides her pregnancy, 17th century (oil on canvas)

JLJ4573212: Diane and nymph Callisto Diane surprises the pregnant callisto nymph of Zeus, The Nymph hides her pregnancy, 17th century (oil on canvas), Rubens, Peter Paul (1577-1640) / Bridgeman Images

ID: JLJ4573212

Diane and nymph Callisto Diane surprises the pregnant callisto nymph of Zeus, The Nymph hides her pregnancy, 17th century (oil on canvas)

Rubens, Peter Paul (1577-1640)

Exoplanets around 70 Virginis - A jovian planet orbiting 70 Virginis - Artist's view of the extrasolar planet 70 Vir B, a giant gas planet orbiting around a solar star, about 78 years old - light from the Sun. This exoplanet has about 6 times the mass of Jupiter and its distance from its star 70 Virginis is almost the same as that of Mercury from the Sun. A ringed 70 Vir B presides over the hot and airless terrain of a hypothetical moon. While it is not known if 70 Vir B has rings, it is certainly possible. 70 Vir B's rings would have no ice in them due to is proximity to its sun. Such rings would likely be less than 100 million years old and could have been formed from the shattered remnants of an asteroid that wondered too close to this giant planet. 70 Vir B's eccentric orbit would increase the likelihood of its encountering other objects in orbit around 70 Virginis. About 78 light years from the Earth astronomers believe that there is a large planet orbiting 70 Virginis, a type G5V star (similar to our own sun). Designated 70 Vir B, this planet is believed to have over six times the mass of the planet Jupiter and orbits around its sun in an eccentric orbit once every 116 days. 70 Vir B's average distance from its sun is about the same as that of the planet Mercury from our own sun
Exoplanets around 70 Virginis - A jovian planet orbiting 70 Virginis - Artist's view of the extrasolar planet 70 Vir B, a giant gas planet orbiting around a solar star, about 78 years old - light from the Sun. This exoplanet has about 6 times the mass of Jupiter and its distance from its star 70 Virginis is almost the same as that of Mercury from the Sun. A ringed 70 Vir B presides over the hot and airless terrain of a hypothetical moon. While it is not known if 70 Vir B has rings, it is certainly possible. 70 Vir B's rings would have no ice in them due to is proximity to its sun. Such rings would likely be less than 100 million years old and could have been formed from the shattered remnants of an asteroid that wondered too close to this giant planet. 70 Vir B's eccentric orbit would increase the likelihood of its encountering other objects in orbit around 70 Virginis. About 78 light years from the Earth astronomers believe that there is a large planet orbiting 70 Virginis, a type G5V star (similar to our own sun). Designated 70 Vir B, this planet is believed to have over six times the mass of the planet Jupiter and orbits around its sun in an eccentric orbit once every 116 days. 70 Vir B's average distance from its sun is about the same as that of the planet Mercury from our own sun

PIX4573224: Exoplanets around 70 Virginis - A jovian planet orbiting 70 Virginis - Artist's view of the extrasolar planet 70 Vir B, a giant gas planet orbiting around a solar star, about 78 years old - light from the Sun. This exoplanet has about 6 times the mass of Jupiter and its distance from its star 70 Virginis is almost the same as that of Mercury from the Sun. A ringed 70 Vir B presides over the hot and airless terrain of a hypothetical moon. While it is not known if 70 Vir B has rings, it is certainly possible. 70 Vir B's rings would have no ice in them due to is proximity to its sun. Such rings would likely be less than 100 million years old and could have been formed from the shattered remnants of an asteroid that wondered too close to this giant planet. 70 Vir B's eccentric orbit would increase the likelihood of its encountering other objects in orbit around 70 Virginis. About 78 light years from the Earth astronomers believe that there is a large planet orbiting 70 Virginis, a type G5V star (similar to our own sun). Designated 70 Vir B, this planet is believed to have over six times the mass of the planet Jupiter and orbits around its sun in an eccentric orbit once every 116 days. 70 Vir B's average distance from its sun is about the same as that of the planet Mercury from our own sun / Bridgeman Images

ID: PIX4573224

Exoplanets around 70 Virginis - A jovian planet orbiting 70 Virginis - Artist's view of the extrasolar planet 70 Vir B, a giant gas planet orbiting around a solar star, about 78 years old - light from the Sun. This exoplanet has about 6 times the mass of Jupiter and its distance from its star 70 Virginis is almost the same as that of Mercury from the Sun. A ringed 70 Vir B presides over the hot and airless terrain of a hypothetical moon. While it is not known if 70 Vir B has rings, it is certainly possible. 70 Vir B's rings would have no ice in them due to is proximity to its sun. Such rings would likely be less than 100 million years old and could have been formed from the shattered remnants of an asteroid that wondered too close to this giant planet. 70 Vir B's eccentric orbit would increase the likelihood of its encountering other objects in orbit around 70 Virginis. About 78 light years from the Earth astronomers believe that there is a large planet orbiting 70 Virginis, a type G5V

Colors of Plants on Alien Worlds - An artist's view of extrasolar planets where plant life could be very different from what we know on Earth. Artwork showing different colors of vegetal life on exoplanets
Colors of Plants on Alien Worlds - An artist's view of extrasolar planets where plant life could be very different from what we know on Earth. Artwork showing different colors of vegetal life on exoplanets

PIX4573296: Colors of Plants on Alien Worlds - An artist's view of extrasolar planets where plant life could be very different from what we know on Earth. Artwork showing different colors of vegetal life on exoplanets / Bridgeman Images

ID: PIX4573296

Colors of Plants on Alien Worlds - An artist's view of extrasolar planets where plant life could be very different from what we know on Earth. Artwork showing different colors of vegetal life on exoplanets

Life of John the Baptist: st John the baptist in prison, detail, 1435 (fresco)
Life of John the Baptist: st John the baptist in prison, detail, 1435 (fresco)

LRI4573342: Life of John the Baptist: st John the baptist in prison, detail, 1435 (fresco), Masolino da Panicale, Tommaso (1383-c.1447) / Bridgeman Images

ID: LRI4573342

Life of John the Baptist: st John the baptist in prison, detail, 1435 (fresco)

Masolino da Panicale, Tommaso (1383-c.1447)

Exoplanete HD 209458b - Artist's view - This exoplanet located in the constellation Pegase, about 150 years ago - light from Earth, seems to be a gas giant whose hydrogene evaporates. An international team of astronomers led by Alfred Vidal - Madjar (Institut d'Astrophysique de Paris, CNRS, France) observed the first signs of oxygen and carbon in the atmosphere of a planet beyond our Solar System for the first time using the NASA/ESA Hubble Space Telescope. The atoms of carbon and oxygen are swept up from the lower atmosphere with the flow of escaping atmospheric atomic hydrogen - like dust in a supersonic whirlwind - in a process called atmospheric 'blow off'. Credit: European Space Agency and Alfred Vidal - Majar (Institut d'Astrophysique de Paris, CNRS, France
Exoplanete HD 209458b - Artist's view - This exoplanet located in the constellation Pegase, about 150 years ago - light from Earth, seems to be a gas giant whose hydrogene evaporates. An international team of astronomers led by Alfred Vidal - Madjar (Institut d'Astrophysique de Paris, CNRS, France) observed the first signs of oxygen and carbon in the atmosphere of a planet beyond our Solar System for the first time using the NASA/ESA Hubble Space Telescope. The atoms of carbon and oxygen are swept up from the lower atmosphere with the flow of escaping atmospheric atomic hydrogen - like dust in a supersonic whirlwind - in a process called atmospheric 'blow off'. Credit: European Space Agency and Alfred Vidal - Majar (Institut d'Astrophysique de Paris, CNRS, France

PIX4573375: Exoplanete HD 209458b - Artist's view - This exoplanet located in the constellation Pegase, about 150 years ago - light from Earth, seems to be a gas giant whose hydrogene evaporates. An international team of astronomers led by Alfred Vidal - Madjar (Institut d'Astrophysique de Paris, CNRS, France) observed the first signs of oxygen and carbon in the atmosphere of a planet beyond our Solar System for the first time using the NASA/ESA Hubble Space Telescope. The atoms of carbon and oxygen are swept up from the lower atmosphere with the flow of escaping atmospheric atomic hydrogen - like dust in a supersonic whirlwind - in a process called atmospheric 'blow off'. Credit: European Space Agency and Alfred Vidal - Majar (Institut d'Astrophysique de Paris, CNRS, France / Bridgeman Images

ID: PIX4573375

Exoplanete HD 209458b - Artist's view - This exoplanet located in the constellation Pegase, about 150 years ago - light from Earth, seems to be a gas giant whose hydrogene evaporates. An international team of astronomers led by Alfred Vidal - Madjar (Institut d'Astrophysique de Paris, CNRS, France) observed the first signs of oxygen and carbon in the atmosphere of a planet beyond our Solar System for the first time using the NASA/ESA Hubble Space Telescope. The atoms of carbon and oxygen are swept up from the lower atmosphere with the flow of escaping atmospheric atomic hydrogen - like dust in a supersonic whirlwind - in a process called atmospheric 'blow off'. Credit: European Space Agency and Alfred Vidal - Majar (Institut d'Astrophysique de Paris, CNRS, France

Artist's view of a hot Jupiter - Artist's view of the transit of a hot Jupiter (gas-like planet very close to its star) in front of its star
Artist's view of a hot Jupiter - Artist's view of the transit of a hot Jupiter (gas-like planet very close to its star) in front of its star

PIX4573405: Artist's view of a hot Jupiter - Artist's view of the transit of a hot Jupiter (gas-like planet very close to its star) in front of its star / Bridgeman Images

ID: PIX4573405

Artist's view of a hot Jupiter - Artist's view of the transit of a hot Jupiter (gas-like planet very close to its star) in front of its star

Frost on reedmace, Italy
Frost on reedmace, Italy

CUB4516705: Frost on reedmace, Italy / Bridgeman Images

ID: CUB4516705

Frost on reedmace, Italy

Frost on spindle tree leaf, Italy
Frost on spindle tree leaf, Italy

CUB4516725: Frost on spindle tree leaf, Italy / Bridgeman Images

ID: CUB4516725

Frost on spindle tree leaf, Italy

Frost on butterbur leaves, Italy
Frost on butterbur leaves, Italy

CUB4516743: Frost on butterbur leaves, Italy / Bridgeman Images

ID: CUB4516743

Frost on butterbur leaves, Italy

Frost on rose, Italy
Frost on rose, Italy

CUB4516749: Frost on rose, Italy / Bridgeman Images

ID: CUB4516749

Frost on rose, Italy

Marrows, Italy
Marrows, Italy

CUB4516788: Marrows, Italy / Bridgeman Images

ID: CUB4516788

Marrows, Italy

Snow on straws, Italy
Snow on straws, Italy

CUB4516844: Snow on straws, Italy / Bridgeman Images

ID: CUB4516844

Snow on straws, Italy

Ice and stalks, Italy
Ice and stalks, Italy

CUB4516872: Ice and stalks, Italy / Bridgeman Images

ID: CUB4516872

Ice and stalks, Italy

Snow on winter cherry, Italy
Snow on winter cherry, Italy

CUB4516878: Snow on winter cherry, Italy / Bridgeman Images

ID: CUB4516878

Snow on winter cherry, Italy

Snow on aucuba, Italy
Snow on aucuba, Italy

CUB4516902: Snow on aucuba, Italy / Bridgeman Images

ID: CUB4516902

Snow on aucuba, Italy

Snow on winter cherry, Italy
Snow on winter cherry, Italy

CUB4516917: Snow on winter cherry, Italy / Bridgeman Images

ID: CUB4516917

Snow on winter cherry, Italy

Snow on pineto, Italy
Snow on pineto, Italy

CUB4516931: Snow on pineto, Italy / Bridgeman Images

ID: CUB4516931

Snow on pineto, Italy

Frost on hazel amentum, Italy
Frost on hazel amentum, Italy

CUB4516950: Frost on hazel amentum, Italy / Bridgeman Images

ID: CUB4516950

Frost on hazel amentum, Italy

Snow on dry shrubs, Italy
Snow on dry shrubs, Italy

CUB4516980: Snow on dry shrubs, Italy / Bridgeman Images

ID: CUB4516980

Snow on dry shrubs, Italy

Snow on little house and beeches, Valsassina, Lombardy, Italy
Snow on little house and beeches, Valsassina, Lombardy, Italy

CUB4517004: Snow on little house and beeches, Valsassina, Lombardy, Italy / Bridgeman Images

ID: CUB4517004

Snow on little house and beeches, Valsassina, Lombardy, Italy

Spluga passage, Italy
Spluga passage, Italy

CUB4517036: Spluga passage, Italy / Bridgeman Images

ID: CUB4517036

Spluga passage, Italy

Drops on eschscholtzia, Italy
Drops on eschscholtzia, Italy

CUB4517061: Drops on eschscholtzia, Italy / Bridgeman Images

ID: CUB4517061

Drops on eschscholtzia, Italy

Drops on sword-lily, Italy
Drops on sword-lily, Italy

CUB4517071: Drops on sword-lily, Italy / Bridgeman Images

ID: CUB4517071

Drops on sword-lily, Italy

Hypogymnia physodes lichen on trunk, Italy
Hypogymnia physodes lichen on trunk, Italy

CUB4517107: Hypogymnia physodes lichen on trunk, Italy / Bridgeman Images

ID: CUB4517107

Hypogymnia physodes lichen on trunk, Italy

Madesimo, Lombardy, Italy
Madesimo, Lombardy, Italy

CUB4517114: Madesimo, Lombardy, Italy / Bridgeman Images

ID: CUB4517114

Madesimo, Lombardy, Italy

Juniper, Italy
Juniper, Italy

CUB4517132: Juniper, Italy / Bridgeman Images

ID: CUB4517132

Juniper, Italy

Red elder, Italy
Red elder, Italy

CUB4517180: Red elder, Italy / Bridgeman Images

ID: CUB4517180

Red elder, Italy

Snow and farmstead, Piani di Nava, Lombardy, Italy
Snow and farmstead, Piani di Nava, Lombardy, Italy

CUB4517204: Snow and farmstead, Piani di Nava, Lombardy, Italy / Bridgeman Images

ID: CUB4517204

Snow and farmstead, Piani di Nava, Lombardy, Italy


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