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The 17th-anniversary celebration featured a panorama of part of the Carina Nebula, and a collection of images selected from that area. [4]In its 17 years of exploring the heavens, NASA's Hubble Space Telescope has made nearly 800,000 observations and snapped nearly 500,000 images of more than 25,000 celestial objects.
NGC 6826 (also known as Caldwell 15) is a planetary nebula located in the constellation Cygnus. It is commonly referred to as the "Blinking Planetary", although many other nebulae exhibit such "blinking". When viewed through a small telescope, the brightness of the central star overwhelms the eye when viewed directly, obscuring the surrounding ...
NASA News Release; Discovery of the star; ESA/Hubble News Release; SIMBAD Query Result; NGC 6302 on WikiSky: DSS2, SDSS, GALEX, IRAS, Hydrogen α, X-Ray, Astrophoto, Sky Map, Articles and images; Butterfly Nebula at Constellation Guide; NASA Astronomy Picture of the Day: The Butterfly Nebula from Hubble (1 October 2014)
A Hubble Space Telescope (HST) image of Pismis 24-1, the "core" of NGC 6357. Dark Energy Camera captures the star-forming nebula NGC 6357. This nebula includes the open cluster Pismis 24, which is home to several massive stars.
Cat's Eye Nebula images at ESA/Hubble; Chandra X-Ray Observatory Photo Album: NGC 6543; Astronomy Picture of the Day. The Cat's Eye Nebula October 31, 1999; Halo of the Cat's Eye 2010 May 9; The Cat's Eye Nebula 2016 July 3; Hubble Probes the Complex History of a Dying Star—HubbleSite article about the Cat's Eye Nebula. NGC6543 The Cats Eye ...
This video clip shows a visualization of the three-dimensional structure of the Pillars of Creation. Closer view of one pillar. Pillars of Creation is a photograph taken by the Hubble Space Telescope of elephant trunks of interstellar gas and dust in the Eagle Nebula, in the Serpens constellation, some 6,500–7,000 light-years (2,000–2,100 pc; 61–66 Em) from Earth. [1]
It is the brightest of the far southern planetary nebulae. This nebula was discovered by Sir John Herschel in March 1834 and is easily visible through small telescopes. The round or even slightly oval diameter is telescopically between 8 and 10 arcsec , though deep images extends this to about 19 or 20 arcsec.
It spins at a rate of 30 times per second, spewing energy beams and taking on a decidedly pulsating appearance.
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