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'Hubble Space Telescope' images and/or videos results page 1 of 11

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Image taken by the Hubble Telescope
Hubble Space Telescope
The Hubble space telescope
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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 Launch
Hubble Space Telescope, 1980s
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Hubble Space Telescope, 1980s
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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)
The central region of our Milky Way galaxy. Hubble, Spitzer and Chandra.
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.
Planet Xena
Hubble Space Telescope in orbit, 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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Testing the Hubble Space Telescope, 1980s
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Mirror of the Hubble Space Telescope, 1980s
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Hubble Space Telescope. NASA photograph.
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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Assembly of the 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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Deployment of the Hubble Space Telescope, 1990
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Planet Fomalhaut B viewed by Hubble telescope
The spiral galaxy Messier 101, from composite of views from Spitzer, Hubble, and Chandra.
Hubble Space Telescope above the Earth. NASA photograph.
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
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)
The Hubble Space Telescope (HST), c 1980s
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Hubble Space Telescope and Earth Limb, 1997
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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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Hubble Space Telescope after assembly, 1980s
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Hubble Space Telescope after assembly, 1980s
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Hubble Space Telescope after assembly, 1980s
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This false-color composite image shows the Cartwheel galaxy. Hubble Space Telescope.
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
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
Jupiter
Hubble ultra deep field - In the southern constellation of the furnace, the Hubble space telescope posed 270h to obtain this image of the distant universe. Approximately 10,000 galaxies distant from 5 to 13 billion light years are visible in this image. This view of nearly 10,000 galaxies is the deepest visible - light image of the cosmos. Called the Hubble Ultra Deep Field, this galaxy - studded view represents a “” deep”” core sample of the universe, cutting across billions of light - years. The snapshot includes galaxies of various ages, sizes, shapes, and colors. The smallest, reddest galaxies, about 100, may be among the most distant known, existing when the universe was just 800 million years old. The nearest galaxies - the larger, brighter, well - defined spirals and ellipticals - thrived about 1 billion years ago, when the cosmos was 13 billion years old. In ground - based photographs, the patch of sky in which the galaxies reside (just one - tenth the diameter of the full Moon) is largely empty. Located in the constellation Fornax, the region is so empty that only a handful of stars within the Milky Way galaxy can be seen in the image. In this image, blue and green correspond to colors that can be seen by the human eye, such as hot, young, blue stars and the glow of Sun - like stars in the disks of galaxies. Red represents near - infrared light, which is invisible to the human eye, such as the red glow of dust - enshrouded galaxies.The image required 800 exposures taken over the course of 400 Hubble orbits around Earth. The total amount of exposure time was 11.3 days, taken between Sept. 24, 2003 and Jan. 16, 2004
Saturn Planet - Hubble Space Telescope on June 20, 2019.
Pluto
Barree spiral galaxy NGC 1483 in Dorado - Barred spiral galaxy NGC 1483 in Dorado - NGC 1483 is a barree spiral galaxy located about 60 million years ago - light in the southern constellation of Dorado. Image obtained by the Hubble Space Telescope (HST). NGC 1483 is a barred spiral galaxy located in the southern constellation of Dorado. The nebulous galaxy features a bright central bulge and diffuse arms with distinct star - forming regions. In the background, many other distant galaxies can be seen. The constellation Dorado is home to the Dorado Group of galaxies, a loose group comprising an estimated 70 galaxies and located some 62 million light - years away. The Dorado group is much larger than the Local Group that includes the Milky Way (and which contains around 30 galaxies) and approaches the size of a galaxy cluster. Galaxy clusters are the largest groupings of galaxies (and indeed the largest structures of any type) in the Universe to be held together by their gravity. Barred spiral galaxies are so named because of the prominent bar - shaped structures found in their center. They form about two thirds of all spiral galaxies, including the Milky Way. Recent studies suggest that bars may be a common stage in the formation of spiral galaxies, and may indicate that a galaxy has reached full maturity. Image taken with the Hubble space telescope (HST)