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'Hubble Space Telescope' Bilder und Clips Suchergebnisse page 1 of 11

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Image taken by the Hubble Telescope
The Hubble space telescope
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Hubble Space Telescope
The Hubble space telescope
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The central region of our Milky Way galaxy. Hubble, Spitzer and Chandra.
Jupiter seen by the Hubble Space Telescope
Hubble Space Telescope Repair
Hubble Space Telescope, 1980s
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Hubble Space Telescope Launch
JWST mirror compares to the Hubble space telescope mirror - Size comparison between the JWST's mirror and HST's mirror - The 6.5-metre primary mirror of the James Webb Space Telescope (JWST), composed of 18 mirrors, compares to the primary mirror of the Hubble space telescope. The large JWST 6.5 meters (21.3 feet) mirror compared to the Hubble Space Telescope primary mirror (at left). The James Webb Space Telescope (JWST) is a large, infrared - optimized space telescope scheduled for launch in 2014
Hubble Space Telescope above the Earth (launched April 24, 1990)
Hubble Space Telescope, 1980s
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Completed Hubble Space Telescope, 1980s
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Deployment of the Hubble Space Telescope, 1990
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Deployment of the Hubble Space Telescope, 1990
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Assembly of the Hubble Space Telescope, 1980s
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Image of Mars from Hubble Space Telescope
The central region of our Milky Way galaxy. Hubble, Spitzer and Chandra.
The central region of our Milky Way galaxy. Hubble, Spitzer and Chandra.
The central region of our Milky Way galaxy. Hubble, Spitzer and Chandra.
Deployment of the Hubble Space Telescope, 1990
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Deployment of the Hubble Space Telescope, 1990
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Deployment of the Hubble Space Telescope, 1990
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Assembly of the Hubble Space Telescope, 1980s
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Planet Xena
The central region of our Milky Way galaxy. Hubble, Spitzer and Chandra.
Deployment of the Hubble Space Telescope, 1990
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Hubble Space Telescope in orbit, 1980s
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Testing the Hubble Space Telescope, 1980s
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Deployment of the Hubble Space Telescope, 1990
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Hubble Space Telescope. NASA photograph.
Mirror of the Hubble Space Telescope, 1980s
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Hubble Space Telescope and Earth Limb, 1997
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Planet Fomalhaut B viewed by Hubble telescope
Hubble Space Telescope after assembly, 1980s
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The spiral galaxy Messier 101, from composite of views from Spitzer, Hubble, and Chandra.
Crab Pulsar in Nebula M1 - The Crab pulsar: This false-colored image obtained by 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.. In 1054 AD, during the Song dynasty, Chinese astronomers spotted a bright new star in the night sky. This newcomer turned out to be a violent explosion within the Milky Way, caused by the spectacular death of a star some 1600 light-years away. This explosion created one of the most well-studied and beautiful objects in the night sky - the Crab Nebula. The beautiful result of this cataclysmic Type II supernova is shown here, imaged by the NASA/ESA Hubble Space Telescope's Advanced Camera for Surveys. Unlike more commonly seen views of this remnant, which show incredibly intricate branches and spires laced throughout the region, this image uses just a single filter, giving rise to a smoother and far simpler view of the famous nebula. The unstoppable collapse of the Crab's progenitor star led to the formation of a rapidly rotating neutron star named the Crab Pulsar, which lurks at the heart of the nebula. This object is roughly the same size as Mars' small moon Phobos, but contains almost one and a half times the mass of the Sun, and whirls around thirty times every second. This causes jets of high-energy radiation to periodically sweep in the direction of Earth, like the spinning beams of a lighthouse, causing the Crab Nebula to appear to pulse at specific wavelengths. The Crab Nebula is also known as NGC 1952 and Messier 1. The second of these names was assigned by Charles Messier. He initially misclassified the neb
Hubble Space Telescope above the Earth. NASA photograph.
The Hubble Space Telescope (HST), c 1980s
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The Hubble Space Telescope (HST), c 1980s
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NASA launched observatory Hubble Space Telescope (HST)
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Cepheide RS Puppis - Cepheides are very bright variable stars that serve as cosmic beacons to measure the distance of 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 photographed one of the brightest cepheids, RS Puppis (in the center of the image), located 6500 years - light in the southern constellation of the Puppi. The bright southern hemisphere star RS Puppis, at the center of the image, is swaddled in a gossamer cocoon of reflective dust illuminated by the glittering star. The super star is ten times more massive than our Sun and 200 times larger. RS Puppis rhythmically brightens and dims over a six - week cycle. It is one of the most luminous in the class of so - called Cepheid variable stars. Its average intrinsic brightness is 15,000 times greater than our Sun's luminosity. The nebula flickers in brightness as pulses of light from the Cepheid propagate outwards. By observing the fluctuation of light in RS Puppis itself, as well as recording the faint reflections of light pulses moving across the nebula, astronomers are able to measure these light echoes and pin down a very accurate distance. The distance to RS Puppis has been narrowed down to 6,500 light - years (with a margin of error of only one percent)
Visible Crab Nebula - Infrared and X - The Crab Nebula - M1, the Crab Nebula, is the rest of a supernova that exploded on July 4, 1054. It is located about 7000 light years from Earth in the constellation Taurus. At the heart of this nebula is a pulsar. To obtain this photo, three spatial observatories combined their observations: the Hubble telescope for the visible part (here in red and yellow), the Chandra telescope for the X-ray data (blue) and the Spitzer telescope for the infrared image (purple). The pulsar is the bright spot in the center of the image. The Crab Nebula (M1) is a supernova remnant at about 7,000 light - year from Earth in the constellation Taurus. The star explosion occured on July 04 1054. At the center of this nebula lies a pulsar. This composite image uses data from three of Nasa's Great Observatories. The Chandra X - ray image is shown in blue, the Hubble Space Telescope optical images are in red and yellow, and the Spitzer Space Telescope's infrared image is in purple
This false-color composite image shows the Cartwheel galaxy. Hubble Space Telescope.
Hubble Space Telescope after assembly, 1980s
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Hubble Space Telescope after assembly, 1980s
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Saturn by Hubble Space Telescope - from 1994 to 200
Hubble space telescope - Artist's view - Hubble space telescope - Artwork - Artist's view of the space shuttle with the Hubble space telescope in its hold. The Hubble Space Telescope is a telescope orbiting the Earth at about 600 km altitude. It is 13 metres long, its main mirror has a diameter of 2.4 metres. He is equipped with spectrometer and several cameras observing the Universe in visible and infrared. Illustration showing the space shuttle with the Hubble space telescope in its payload bay during a servicing mission
Jupiter
Saturn Planet - Hubble Space Telescope on June 20, 2019.
Summary image: NASA and European Space Agency Hubble Space Telescope
Summary image: NASA and European Space Agency Hubble Space Telescope