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Images of '3.6M' found, 20

 
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

PIX4573752

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

PIX4573752

 
La Silla Observatory - Chile - La Silla observatory - La Silla Observatory. From left to right, in the background, the domes of the NTT and the 3.6m (with the CAT), in the foreground, the Schmidt telescope and the 2.2m ESO/MPG (with the silver dome). 2006 The ESO La Silla Observatory at twilight. From left to right, in background, one sees the 3.6m NTT (square) and the double dome of the 3.6m with the tiny 1.4m CAT, in foreground, the Schmidt telescope, and the ESO/MPG 2.2m (silver dome). 200

Stefan Seip

PIX4655953

La Silla Observatory - Chile - La Silla observatory - La Silla Observatory. From left to right, in the background, the domes of the NTT and the 3.6m (with the CAT), in the foreground, the Schmidt telescope and the 2.2m ESO/MPG (with the silver dome). 2006 The ESO La Silla Observatory at twilight. From left to right, in background, one sees the 3.6m NTT (square) and the double dome of the 3.6m with the tiny 1.4m CAT, in foreground, the Schmidt telescope, and the ESO/MPG 2.2m (silver dome). 200

Stefan Seip

PIX4655953

 
Gl 581c: discovery of a habitable planet - Gl 581c: discovery of an habitable planet - Artist's view of the exoplanet Gliese 581c. Gliese 581c, with a radius of 1.5 times that of the Earth, is the first exoplanet gathering the necessary elements to imagine the existence of a possible extra-terrestrial life. From its surface, its star, about 100 times less bright than our Sun, must be large in the sky because of its proximity to the planet. In April 2007 the Geneva Observatory in Switzerland announced the discovery of a “super - earth”” extrasolar planet orbiting the red dwarf star Gliese 581. Dubbed Gliese 581 c, it's been called a super - earth because it is one of the few known extrasolar planets that has a mass near Earth's, and the only one to occupy its sun's “” habitable zone.”” Gliese 581 c is believed to be about five times more massive than the Earth with a diameter about half - again as large as Earth's. Depending upon the planet's composition, whether mostly rock or a combin

Walter B Myers

PIX4573770

Gl 581c: discovery of a habitable planet - Gl 581c: discovery of an habitable planet - Artist's view of the exoplanet Gliese 581c. Gliese 581c, with a radius of 1.5 times that of the Earth, is the first exoplanet gathering the necessary elements to imagine the existence of a possible extra-terrestrial life. From its surface, its star, about 100 times less bright than our Sun, must be large in the sky because of its proximity to the planet. In April 2007 the Geneva Observatory in Switzerland announced the discovery of a “super - earth”” extrasolar planet orbiting the red dwarf star Gliese 581. Dubbed Gliese 581 c, it's been called a super - earth because it is one of the few known extrasolar planets that has a mass near Earth's, and the only one to occupy its sun's “” habitable zone.”” Gliese 581 c is believed to be about five times more massive than the Earth with a diameter about half - again as large as Earth's. Depending upon the planet's composition, whether mostly rock or a combin

Walter B Myers

PIX4573770

 
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

PIX4573193

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

PIX4573193

 
Artist view of the planetary system around Gliese 581 - Planetary system around the red dwarf Gliese 581 - Artist view of the planetary system around the star Gliese 581. In the foreground, the exoplanet Gliese 581st. In the background, Gliese 581d (blueberry), in the center Gliese 581c and near the star, Gliese 581b. Gliese 581e (foreground) is only about twice the mass of our Earth. The Gliese 581 planetary system now has four known planets, with masses of about 1.9 (planet e, left in the foreground), 16 (planet b, nearest to the star), 5 (planet c, centre), and 7 Earth - masses (planet d, with the bluish colour). The planet furthest out, Gliese 581d, orbits its host star in 66.8 days, while Gliese 581 e completes its orbit in 3.15 days

PIX4573711

Artist view of the planetary system around Gliese 581 - Planetary system around the red dwarf Gliese 581 - Artist view of the planetary system around the star Gliese 581. In the foreground, the exoplanet Gliese 581st. In the background, Gliese 581d (blueberry), in the center Gliese 581c and near the star, Gliese 581b. Gliese 581e (foreground) is only about twice the mass of our Earth. The Gliese 581 planetary system now has four known planets, with masses of about 1.9 (planet e, left in the foreground), 16 (planet b, nearest to the star), 5 (planet c, centre), and 7 Earth - masses (planet d, with the bluish colour). The planet furthest out, Gliese 581d, orbits its host star in 66.8 days, while Gliese 581 e completes its orbit in 3.15 days

PIX4573711

 
La Silla Observatory - Chile - La Silla observatory - La Silla Observatory. From left to right, in the background, the domes of the NTT and the 3.6m (with the CAT), in the foreground, the Schmidt telescope and the 2.2m ESO/MPG (with the silver dome). 2006 The ESO La Silla Observatory at twilight. From left to right, in background, one sees the 3.6m NTT (square) and the double dome of the 3.6m with the tiny 1.4m CAT, in foreground, the Schmidt telescope, and the ESO/MPG 2.2m (silver dome). 200

Stefan Seip

PIX4655933

La Silla Observatory - Chile - La Silla observatory - La Silla Observatory. From left to right, in the background, the domes of the NTT and the 3.6m (with the CAT), in the foreground, the Schmidt telescope and the 2.2m ESO/MPG (with the silver dome). 2006 The ESO La Silla Observatory at twilight. From left to right, in background, one sees the 3.6m NTT (square) and the double dome of the 3.6m with the tiny 1.4m CAT, in foreground, the Schmidt telescope, and the ESO/MPG 2.2m (silver dome). 200

Stefan Seip

PIX4655933

 
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

PIX4573201

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

PIX4573201

 
Telescope of 3.60 m from La Silla, Chile - Milky way - La Silla observatory - CAT and 3.6m domes - At 2400 m altitude, the dome of the 3.60 m telescope of the Observatory of La Silla, Chile, is cut off on the Lactee Way. The Jupiter planet rises at the foot of the high tower that houses this telescope, equipped with the HARPS instrument. The 3.6 - m telescope and the attached dome of the CAT are seen under the Milky way. Planet Jupiter is rising between the domes. 3.6 - m telescope is host to the HARPS instrument, perhaps the most successful exoplanet hunter that exists

Serge Brunier

PIX4656053

Telescope of 3.60 m from La Silla, Chile - Milky way - La Silla observatory - CAT and 3.6m domes - At 2400 m altitude, the dome of the 3.60 m telescope of the Observatory of La Silla, Chile, is cut off on the Lactee Way. The Jupiter planet rises at the foot of the high tower that houses this telescope, equipped with the HARPS instrument. The 3.6 - m telescope and the attached dome of the CAT are seen under the Milky way. Planet Jupiter is rising between the domes. 3.6 - m telescope is host to the HARPS instrument, perhaps the most successful exoplanet hunter that exists

Serge Brunier

PIX4656053

 
Milky Way on the Observatory of La Silla -Chile (photo)

Sebastian Voltmer

PIX6333940

Milky Way on the Observatory of La Silla -Chile (photo)

Sebastian Voltmer

PIX6333940

 
Michel Mayor and his colleagues at La Silla - Michel Mayor, Francesco Pepe, and Didier Queloz in front of La Sill's 3.6m telescope

L. Weinstein

PIX4657847

Michel Mayor and his colleagues at La Silla - Michel Mayor, Francesco Pepe, and Didier Queloz in front of La Sill's 3.6m telescope

L. Weinstein

PIX4657847

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