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'Orbitant' images et/ou videos résultats page 1 of 2

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The Viking spacecraft imagined orbiting Mars
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Milky Way Galaxy and position of Solar System, Drawing
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Sargasso Sea and Gulf of Mexico photographed from a satellite orbiting the earth
Bohr atomic model
Earths city lights data acquired by the Suomi National Polar-orbiting Partnership (Suomi NPP) satellite 2012
The scale of the sun in comparison to the planets orbiting the sun
Shell atomic model
Diagram of eclipse of sun and moon, Drawing
(photo)
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Diagram of spacecraft artificial satellites orbiting Earth
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Spiral nebula, old incorrect term for spiral galaxy with hazy appearance, Drawing
(photo)
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Kepler-186f (also known by its Kepler Object of Interest designation KOI-571
Lunar Reconnaissance Orbiter
Stronger tide phenomenon during new moon, when gravitational force of Earth and of Sun (aligned) are combined, Drawing
(photo)
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Rutherford atomic model
Artist's imagination of NASA's 2001 Mars Odyssey
International Space Station
International Space Station
Mars Reconnaissance Orbiter
Saturn embraced by the shadows of its stately rings. Cassini.
Andromeda Galaxy (M 31), spiral galaxy with two small satellite galaxies, Drawing
(photo)
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Weak tide phenomenon during first and last moon's quarter phases, when Earth, Moon and Sun are positioned at right angles, Drawing
(photo)
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Diagram of Solar System formation
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Lunar phases diagram
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Moon phases diagram, Drawing
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Determining north celestial pole through constellations, Drawing
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Untitled (Forms Orbiting a Flower), 1947 (pastel & w/c on paper)
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Salyut 1, the First Soviet Orbiting Space Station, Launched in 1971.
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A detailed, global natural color view of Saturn and its rings. Cassini.
View of Saturn's rings as they surround the planet. Cassini.
Orbits of planets of Solar System and, in box, detail of Neptune and Pluto revolution around sun, Drawing
(photo)
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Planet Fomalhaut B viewed by Hubble telescope
Diagram showing Mars' moons, orbits of Phobos and Deimo
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Geocentrism or Aristotelian-Ptolemaic system, Astronomical model that places Earth at center of universe (illustration)
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Beijing, capital city of China viewed from the Landsat 7 satellite, 2000
Colour footage of Laika, the soviet space dog, in Sputnik 2, November 3 1957 (HD)
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The space capsule Columbiad orbiting close to the Moon, 1865 (engraving)
Different phases of sun, illuminated miniature from Kabbalistic treatise, Greek manuscript, 16th century
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Russian Space Program Canine Research, featuring dogs Laika, Albina and Mushka 1950s
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Animation of Project Mercury space expedition
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The Sun and Planets; Le soleil et les planetes, 1941 (oil on canvas)
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Artist's conception of the solar powered GLAST (Gamma Ray Large Area Satellite) satellite orbiting earth in 2008. GLAST studies extreme events that cause high-energy gamma ray bursts, such as flaring of galaxies driven by black holes within their cores
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Project Mercury: members of the Mercury Seven in training
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Abstract Composition, 1972 (oil, gouache and pencil on board)
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Tycho Brahe
United States, 1960s: Space ship orbiting around the Earth
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The cloud of Oort - Illustration - The Oort cloud. Artwork - The Oort Cloud is a vast body envelope orbiting well beyond the orbit of the planets of the solar system. Comets would come from that cloud. The Oort Cloud is a huge spherical cloud surrounding our Solar System. Extending about 30 trillion kilometers (18 trillion miles) from the Sun, it was first proposed in 1950 by Dutch astronomer Jan Oort. The vast distance of the Oort cloud is considered to be the outer edge of the Solar System where the Sun's influence ends. It contains billions of icy bodies and seems to be the birth place of comets
Dilemma
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James Ferguson, Scottish astronomer
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Earth-Moon system
Exoplanete Gliese 667 Cc: Gliese 667 Cc is an exoplanet orbiting around the star Gliese 667 C in its habitable area, located about 23 light years from Earth in the constellation of the scorpion. This super Earth was detected using the HARPS program at the La Silla Observatory in Chile in October 2009. The Super-earth Gliese 667 Cc is a 6 Earth-mass exoplanet which circulates around its low-mass host star Gliese 667 C at a distance equal to only 1/20th of the Earth-Sun distance
Project Mercury: Mastery of Space
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Exoplanet WASP-103b - Illustration
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Kepler-452b (sometimes nicknamed Earth 2
Artist's impression of the Exoplanète Proxima Centauri
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In the cloud of Oort - Illustration - Inside the Oort cloud - Illustration - The cloud of Oort is a vast body envelope orbiting well beyond the orbit of the planets of the solar system. Comets would come from that cloud. The Oort Cloud is a huge spherical cloud surrounding our Solar System. Extending about 30 trillion kilometers (18 trillion miles) from the Sun, it was first proposed in 1950 by Dutch astronomer Jan Oort. The vast distance of the Oort cloud is considered to be the outer edge of the Solar System where the Sun's influence ends. It contains billions of icy bodies and seems to be the birth place of comets
The cloud of Oort - Illustration - The Oort cloud. Artwork - The Oort Cloud is a vast body envelope orbiting well beyond the orbit of the planets of the solar system. Comets would come from that cloud. The Oort Cloud is a huge spherical cloud surrounding our Solar System. Extending about 30 trillion kilometers (18 trillion miles) from the Sun, it was first proposed in 1950 by Dutch astronomer Jan Oort. The vast distance of the Oort cloud is considered to be the outer edge of the Solar System where the Sun's influence ends. It contains billions of icy bodies and seems to be the birth place of comets
The cloud of Oort - Illustration - The Oort cloud. Artwork - The Oort Cloud is a vast body envelope orbiting well beyond the orbit of the planets of the solar system. Comets would come from that cloud. The Oort Cloud is a huge spherical cloud surrounding our Solar System. Extending about 30 trillion kilometers (18 trillion miles) from the Sun, it was first proposed in 1950 by Dutch astronomer Jan Oort. The vast distance of the Oort cloud is considered to be the outer edge of the Solar System where the Sun's influence ends. It contains billions of icy bodies and seems to be the birth place of comets
Exoplanets Gliese 876 e and b
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Manned Space Flight, USA, Apollo, General Drawing of Lunar Orbiter, 1966
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The cloud of Oort - Illustration - The Oort cloud. Artwork - The Oort Cloud is a vast body envelope orbiting well beyond the orbit of the planets of the solar system. Comets would come from that cloud. Legendee version. The Oort Cloud is a huge spherical cloud surrounding our Solar System. Extending about 30 trillion kilometers (18 trillion miles) from the Sun, it was first proposed in 1950 by Dutch astronomer Jan Oort. The vast distance of the Oort cloud is considered to be the outer edge of the Solar System where the Sun's influence ends. It contains billions of icy bodies and seems to be the birth place of comets.Annotated image
Exoplanet HD 21749 b
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Super - Land around the star HD 40307 - Super - Earths around HD 40307 - Artist view of three super - Earth orbiting around the star HD 40307, about 42 years ago - light from our Sun. The planets, observed by the HARPS instrument installed on the 3.6m telescope of La Silla, have a mass ranging from 4 to 9 times the mass of the Earth. Artist's impression of the trio of super - Earths discovered by an European team using the HARPS spectrograph on Eso's 3.6 - m telescope at La Silla, Chile, after 5 years of monitoring. The three planets, having 4.2, 6.7, and 9.4 times the mass of the Earth, orbit the star HD 40307 with periods of 4.3, 9.6, and 20.4 days, respectively
Superhabitable Exoplanet
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Exoplanete HAT-P-32 b - Artist's view: HAT-P-32 b is an exoplanet orbiting around the star HAT-P-32. Discovered on 8 June 2011 by the transit method, it is 0.941 times the mass of Jupiter. Its radius makes it the largest exoplanet known at the end of 2012. Hat-P-32b is a planet in the orbit of the star HAT-P-32, which is approximately 1,044 light years away from Earth in Andromeda constellation. The planet is considered a Hot Jupiter, and although it is slightly less massive than Jupiter, it is bloated to nearly twice Jupiter's size. At the time of its discovery, Hat-p-32b had one of the largest radii known among extrasolar planets
Exoplanets around the pulsar PSR B1257+12: PSR B1257+12, also called Lich since December 2015, is a pulsar located at a distance of 2300 light years from the Sun, in the constellation of the Virgin. In 1992 two planets orbiting the star were discovered. A third planet was discovered later around PSR B1257+12. PSR B1257+12, also named Lich, is a pulsar located 2300 light years from the Sun in the constellation of Virgo. The pulsar has a planetary system with three known extrasolar planets, named “” Draugr”” (PSR B1257+12 A), “” Poltergeist”” (PSR B1257+12 B) and “” Phobetor””” (PSR B1257+12 C), respectively. They were both the first extrasolar planets and the first pulsar planets to be discovered; A and B in 1992 and C in 1994
Exoplanete HD 85512b - The rocky super - Earth HD 85512 b - HD 85512 b is an exoplanet orbiting around the star HD 85512, located about 36 years ago - light from Earth in the constellation of Sails. It is one of the smallest exoplanets in habitable areas discovered to date; this super Earth was detected with the help of the HARPS program at the La Silla Observatory in Chile in August 2011. This artist's impression shows the planet orbiting the Sun - like star HD 85512 in the southern constellation of Vela (The Sail). This planet is one of sixteen super - Earths discovered by the HARPS instrument on the 3.6 - metre telescope at Eso's La Silla Observatory. This planet, HD 85512b, is about 3.6 times as massive as the Earth and lies at the edge of the habitable zone around the star, where liquid water, and perhaps even life, could potentially exist
Exoplanete HD 85512b - The rocky super - Earth HD 85512 b - HD 85512 b is an exoplanet orbiting around the star HD 85512, located about 36 years ago - light from Earth in the constellation of Sails. It is one of the smallest exoplanets in habitable areas discovered to date; this super Earth was detected with the help of the HARPS program at the La Silla Observatory in Chile in August 2011. This artist's impression shows the planet orbiting the Sun - like star HD 85512 in the southern constellation of Vela (The Sail). This planet is one of sixteen super - Earths discovered by the HARPS instrument on the 3.6 - metre telescope at Eso's La Silla Observatory. This planet, HD 85512b, is about 3.6 times as massive as the Earth and lies at the edge of the habitable zone around the star, where liquid water, and perhaps even life, could potentially exist
Exoplanete HD 85512b - The rocky super - Earth HD 85512 b - HD 85512 b is an exoplanet orbiting around the star HD 85512, located about 36 years ago - light from Earth in the constellation of Sails. It is one of the smallest exoplanets in habitable areas discovered to date; this super Earth was detected with the help of the HARPS program at the La Silla Observatory in Chile in August 2011. This artist's impression shows the planet orbiting the Sun - like star HD 85512 in the southern constellation of Vela (The Sail). This planet is one of sixteen super - Earths discovered by the HARPS instrument on the 3.6 - metre telescope at Eso's La Silla Observatory. This planet, HD 85512b, is about 3.6 times as massive as the Earth and lies at the edge of the habitable zone around the star, where liquid water, and perhaps even life, could potentially exist
Exoplanete HD 85512b - The rocky super - Earth HD 85512 b - HD 85512 b is an exoplanet orbiting around the star HD 85512, located about 36 years ago - light from Earth in the constellation of Sails. It is one of the smallest exoplanets in habitable areas discovered to date; this super Earth was detected with the help of the HARPS program at the La Silla Observatory in Chile in August 2011. This artist's impression shows the planet orbiting the Sun - like star HD 85512 in the southern constellation of Vela (The Sail). This planet is one of sixteen super - Earths discovered by the HARPS instrument on the 3.6 - metre telescope at Eso's La Silla Observatory. This planet, HD 85512b, is about 3.6 times as massive as the Earth and lies at the edge of the habitable zone around the star, where liquid water, and perhaps even life, could potentially exist
Exoplanete HD 85512b - The rocky super - Earth HD 85512 b - HD 85512 b is an exoplanet orbiting around the star HD 85512, located about 36 years ago - light from Earth in the constellation of Sails. It is one of the smallest exoplanets in habitable areas discovered to date; this super Earth was detected with the help of the HARPS program at the La Silla Observatory in Chile in August 2011. This artist's impression shows the planet orbiting the Sun - like star HD 85512 in the southern constellation of Vela (The Sail). This planet is one of sixteen super - Earths discovered by the HARPS instrument on the 3.6 - metre telescope at Eso's La Silla Observatory. This planet, HD 85512b, is about 3.6 times as massive as the Earth and lies at the edge of the habitable zone around the star, where liquid water, and perhaps even life, could potentially exist
Artist's view of the asteroid 2060 Chiron: (2060) Chiron, also designed as 95P/Chiron, is a centaur type cometary asteroid, an ice body of 166 kilometres of diameter orbiting around the Sun between Saturn and Uranus. 2060 Chiron, also known as 95P/Chiron, is a minor planet in the outer Solar System, orbiting the Sun between Saturn and Uranus. Discovered in 1977 it was the first-identified member of a new class of objects now known as centaurs - bodies orbiting between the asteroid belt and the Kuiper belt. Besides the four giant planets, Chiron and 10199 Chariklo, also a centaur, are the only other bodies in the Solar System known to have rings. Although it was initially called an asteroid and classified only as a minor planet with the designation “” 2060 Chiron””, it was later found to exhibit behavior typical of a comet. Today it is classified as both a minor planet and a comet, and is accordingly also known by the cometary designation “” 95P/Chiron””
Planetary system around the star HD 69830 - Planetary System Around HD 69830 - Artist's view of three planets orbiting around the star HD 69830. This planetary system is the first detects around a star similar to the Sun that contains several planets whose mass is less than that of Jupiter. It seems that this system also has an asteroid belt. Using the ultra - precise HARPS spectrograph on Eso's 3.6 - m telescope at La Silla (Chile), a team of European astronomers have discovered that a nearby star is host to three Neptune - mass planets. The innermost planet is most likely rocky, while the outermost is the first known Neptune - mass planet to reside in the habitable zone. This unique system is likely further enriched by an asteroid belt. This view portaits a point of view inside the asteroid belt, which is assumed here to lie between the two outermost planets
Full Moon from space, 2004-2005
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Planetary system around the star HD 69830 - Planetary System Around HD 69830 - Artist's view of three planets orbiting around the star HD 69830. This planetary system is the first detects around a star similar to the Sun that contains several planets whose mass is less than that of Jupiter. It seems that this system also has an asteroid belt. Using the ultra - precise HARPS spectrograph on Eso's 3.6 - m telescope at La Silla (Chile), a team of European astronomers have discovered that a nearby star is host to three Neptune - mass planets. The innermost planet is most likely rocky, while the outermost is the first known Neptune - mass planet to reside in the habitable zone. This unique system is likely further enriched by an asteroid belt. This view portaits a point of view inside the asteroid belt, which is assumed here to lie between the two outermost planets
Exoplanete Gliese 667 Cb - The system Gliese 667 (Artist's impression) - Gliese 667 Cb is an exoplanet orbiting the star Gliese 667 C, located about 23 years ago - light from Earth in the constellation of the scorpion. This super Earth was detected using the HARPS program at the La Silla Observatory in Chile in October 2009. On 19 October 2009, the team who built the High Accuracy Radial Velocity Planet Searcher, better known as HARPS, the spectrograph for ESO's 3.6 - metre telescope, reported on the incredible discovery of some 32 new exoplanets, cementing Harps's position as the world's foremost exoplanet hunter. One of these is surrounding the star Gliese 667 C, which belongs to a triple system. The 6 Earth - mass exoplanet circulates around its low - mass host star at a distance equal to only 1/20th of the Earth - Sun distance. The host star is a companion to two other low - mass stars, which are seen here in the distance
NASA's Kepler mission confirmed the discovery of its first rocky planet, named Kepler-10b, 2000
Atoms, Elements & Molecules, Models Sodium atom model, c 1912-1926
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