RFBE3FRK–The Hubble Space Telescope.

RFRKFX11–Modern Shisha water pipe, overhead shot. Isolated over white background.

'English: Comparison of views of the globular star cluster NGC 6362 from WFI and Hubble This colourful view of the globular cluster NGC 6362 on the left was captured by the Wide Field Imager attached to the MPG/ESO 2.2-metre telescope at ESO’s La Silla Observatory in Chile. This brilliant ball of ancient stars lies in the southern constellation of Ara (The Altar). The close up view of the core of the cluster on the right is from the NASA/ESA Hubble Space Telescope. Credit: ESO About the Image Id:eso1243e Type:Observation Release date:31 October 2012, 12:00 Related releases:eso1243 Size:6

RM2BAMC8T–'English: Comparison of views of the globular star cluster NGC 6362 from WFI and Hubble This colourful view of the globular cluster NGC 6362 on the left was captured by the Wide Field Imager attached to the MPG/ESO 2.2-metre telescope at ESO’s La Silla Observatory in Chile. This brilliant ball of ancient stars lies in the southern constellation of Ara (The Altar). The close up view of the core of the cluster on the right is from the NASA/ESA Hubble Space Telescope. Credit: ESO About the Image Id:eso1243e Type:Observation Release date:31 October 2012, 12:00 Related releases:eso1243 Size:6

NASAÕs Hubble Space Telescope provides a close-up look of Comet ISON (C/2012 S1), on April 10,2013. At the time, the comet was slightly closer than JupiterÕs orbit at a distance of 386 million miles from the sun. The cometÕs dusty coma, or head of the comet, is approximately 3,100 miles across, or 1.2 times the width of Australia. A dust tail extends more than 57,000 miles, far beyond HubbleÕs field of view. ISON stands for International Scientific Optical Network, a group of observatories in ten countries who have organized to detect, monitor, and track objects in space. UPI/NASA/ ESA/ J.Y. L

RMW0MM2Y–NASAÕs Hubble Space Telescope provides a close-up look of Comet ISON (C/2012 S1), on April 10,2013. At the time, the comet was slightly closer than JupiterÕs orbit at a distance of 386 million miles from the sun. The cometÕs dusty coma, or head of the comet, is approximately 3,100 miles across, or 1.2 times the width of Australia. A dust tail extends more than 57,000 miles, far beyond HubbleÕs field of view. ISON stands for International Scientific Optical Network, a group of observatories in ten countries who have organized to detect, monitor, and track objects in space. UPI/NASA/ ESA/ J.Y. L

This image provided by NASA is a Hubble Space Telescope close-up view of Saturn's disk captures the transit of several moons across the face of the gas giant planet. The giant orange moon Titan – larger than the planet Mercury – can be seen at upper right. The white icy moons close to the ring plane are, from left,Enceladus, Dione, and Mimas, at right edge of the plaent. The dark band running across the face of the planet slightly above the rings is the shadow of the rings cast on the planet. The dark dots as the shadows cast by Enceladus and Dione. (AP Photo/NASA)

RM2P8PNN9–This image provided by NASA is a Hubble Space Telescope close-up view of Saturn's disk captures the transit of several moons across the face of the gas giant planet. The giant orange moon Titan – larger than the planet Mercury – can be seen at upper right. The white icy moons close to the ring plane are, from left,Enceladus, Dione, and Mimas, at right edge of the plaent. The dark band running across the face of the planet slightly above the rings is the shadow of the rings cast on the planet. The dark dots as the shadows cast by Enceladus and Dione. (AP Photo/NASA)

This close-up Hubble view of the Meathook Galaxy (NGC 2442), released on May 4, 2011, focuses on the more compact of its two asymmetric spiral arms as well as the central regions. The spiral arm was the location of a supernova that exploded in 1999. These Hubble observations were made in 2006 in order to study the aftermath of this supernova. Ground-based data from MPG/ESO 2.2-metre telescope were used to fill out parts of the edges of this image. .UPI/NASA/ESA

RMW0MHY4–This close-up Hubble view of the Meathook Galaxy (NGC 2442), released on May 4, 2011, focuses on the more compact of its two asymmetric spiral arms as well as the central regions. The spiral arm was the location of a supernova that exploded in 1999. These Hubble observations were made in 2006 in order to study the aftermath of this supernova. Ground-based data from MPG/ESO 2.2-metre telescope were used to fill out parts of the edges of this image. .UPI/NASA/ESA

'English: This image is a “close-up” view from the NASA/ESA Hubble Space Telescope of NGC 4755, or the Jewel Box cluster. Several very bright, pale blue super-giant stars (eg. κ Crucis on the left, HD 111934 on the lower right and HIP 62913 in the middle right), a solitary ruby-red super-giant (HIP 62918 - upper right) and a variety of other brilliantly coloured stars are visible in the image, as well as many much fainter ones, often with intriguing colours. The huge variety in brightness exists because the brighter stars are 15 to 20 times the mass of the Sun, while the dim points are less th

RM2BAMAKC–'English: This image is a “close-up” view from the NASA/ESA Hubble Space Telescope of NGC 4755, or the Jewel Box cluster. Several very bright, pale blue super-giant stars (eg. κ Crucis on the left, HD 111934 on the lower right and HIP 62913 in the middle right), a solitary ruby-red super-giant (HIP 62918 - upper right) and a variety of other brilliantly coloured stars are visible in the image, as well as many much fainter ones, often with intriguing colours. The huge variety in brightness exists because the brighter stars are 15 to 20 times the mass of the Sun, while the dim points are less th

RMAN81CF–Cones pillars and majestic flowing shapes abound in stellar nurseries natal clouds gas dust newborn stars Hubble image