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View Images Library Photos and Pictures. These Mini Hot Pink Rags in a Bag can be used for: Make-up Removal Lens Cleaning (Eyeglasses, Sunglasses, Camcorder Lenses, Camera Lenses, Telescope Lenses, Binoculars, Watch Faces, etc.) Electronic "Gizmo and Gadget" Cleaning (Smartphones, Tablets, Computer Screens, Computer Key Boards, Remotes, Calculators, etc.) Mini and Small Picture Frames and Glass Inserts Matterport Pro 3D Camera uses an array of 2D and 3D sensors to quickly capture… Stargazing tips and more Pricing Calculator for Photographers

. Description - StarSense Hand Control is compatible with the StarSense AutoAlign accessory for use with Celestron computerized telescopes - Flash upgradeable via the Internet; latest updates can be found at Celestron.com - 40,000-object database. - Dual line, 16-character LCD screen with adjustable backlighting. - Now connects to your PC directly with a mini-USB cable (cable not included) for software updates or optional telescope control with third party software Business Line Design Icons Bundle The Exposure Triangle: Making Sense of Aperture, Shutter Speed, and ISO

A NASA/ESA Hubble Space Telescope image of the galaxy UGC 9391, one of the galaxies in the new survey. UGC 9391 contains the two types of stars — Cepheid variables and a Type 1a supernova — that astronomers used to calculate a more precise Hubble Constant. The red circles that mark the locations of Cepheids. The blue "X" denotes the location of supernova 2003du, a Type Ia supernova. The observations for this composite image were taken between 2012 and 2013 by Hubble's Wide Field Camera 3. Im...

A NASA/ESA Hubble Space Telescope image of the galaxy UGC 9391, one of the galaxies in the new survey. UGC 9391 contains the two types of stars — Cepheid variables and a Type 1a supernova — that astronomers used to calculate a more precise Hubble Constant. The red circles that mark the locations of Cepheids. The blue "X" denotes the location of supernova 2003du, a Type Ia supernova. The observations for this composite image were taken between 2012 and 2013 by Hubble's Wide Field Camera 3. Im...

The Exposure Triangle: Making Sense of Aperture, Shutter Speed, and ISO

The Kepler Mission passes the torch on the search for exoplanets to TESS, the Transitory Exoplanet Survey Sattelite. SETI is alive and well.

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Johann Christoph Schuster, calculating machine, 1789. Germany. Deutsches Museum

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Description - StarSense Hand Control is compatible with the StarSense AutoAlign accessory for use with Celestron computerized telescopes - Flash upgradeable via the Internet; latest updates can be found at Celestron.com - 40,000-object database. - Dual line, 16-character LCD screen with adjustable backlighting. - Now connects to your PC directly with a mini-USB cable (cable not included) for software updates or optional telescope control with third party software

These Mini Hot Pink Rags in a Bag can be used for: Make-up Removal Lens Cleaning (Eyeglasses, Sunglasses, Camcorder Lenses, Camera Lenses, Telescope Lenses, Binoculars, Watch Faces, etc.) Electronic "Gizmo and Gadget" Cleaning (Smartphones, Tablets, Computer Screens, Computer Key Boards, Remotes, Calculators, etc.) Mini and Small Picture Frames and Glass Inserts

Celestron - StarSense Explorer 114mm Newtonian Reflector Telescope - Silver/Black

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This NASA/ESA Hubble Space Telescope image reveals the iridescent interior of one of the most active galaxies in our local neighborhood '" NGC 1569, aandnbsp;small galaxyandnbsp;located about eleven million light-years away in theandnbsp;constellation of Camelopardalisandnbsp;(The Giraffe). This galaxy is currently a hotbed of vigorous star formation. NGC 1569 is aandnbsp;starburst galaxy, meaning that '" as the name suggests '" it is bursting at the seams with stars, and is currently producing them at a rate far higher than that observed in most other galaxies. For almost 100 million years, NGC 1569 has pumped out stars more than 100 times faster than theandnbsp;Milky Way! As a result, this glittering galaxy is home toandnbsp;super star clusters, three of which are visible in this image '" one of the two bright clusters is actuallyandnbsp;the superposition of two massive clusters. Each containing more than a million stars, these brilliant blue clusters reside within a large cavity of gas carved out by multipleandnbsp;supernovae, the energetic remnants of massive stars. In 2008, Hubble observed the galaxy's cluttered core and sparsely populated outer fringes. By pinpointing individualandnbsp;red giant stars, Hubble'sandnbsp;Advanced Camera for Surveysandnbsp;enabled astronomers to calculate a new '" and much more precise '" estimate for NGC 1569's distance. This revealed that the galaxy is actually one and a half times farther away than previously thought, and a member of the IC 342 galaxy group. Astronomers suspect that the IC 342 cosmic congregation is responsible for the star-forming frenzy observed in NGC 1569. Gravitational interactions between this galactic group are believed to be compressing the gas within NGC 1569. As it is compressed, the gas collapses, heats up and forms new stars. Image credit: ESA/Hubble andamp; NASA, Aloisi, Ford; Acknowledgement: Judy Schmidt Text credit: European Space Agency Hubble Space Telescope

This remarkable picture from the Advanced Camera for Surveys on the NASA/ESA Hubble Space Telescope shows one of the most perfect geometrical forms created in space. It captures the formation of an unusual pre-planetary nebula, known as IRAS 23166+1655, around the star LL Pegasi (also known as AFGL 3068) in the constellation of Pegasus (the Winged Horse). The striking picture shows what appears to be a thin spiral pattern of astonishingly regularity winding around the star, which is itself ...

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Ripples found in the Milky Way Galaxy's disk reveal our galaxy survived an ancient hit-and-run. Now, astronomers might have caught the culprit.

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Galaxy cluster RCS2 J2327 is an extremely massive cluster of galaxies located approximately 6 billion light-years away towards the constellation Pisces. The mass of the cluster causes both strong and weak gravitational lensing, which can be used to calculate the mass of the cluster. This image is a composite of observations from the HAWK-I instrument on ESO's Very Large Telescope and the NASA/ESA Hubble Space Telescope's Advanced Camera for Surveys. (Credit: ESO & ESA/Hubble & NASA)