دانلود والپیپرهای نجومی تلسکوپ هابل در سایز های مختلف

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Credit for Hubble Image: NASA, ESA, N. Smith (University of California, Berkeley), and The Hubble Heritage Team (STScI/AURA)​

Credit for CTIO Image: N. Smith (University of California, Berkeley) and NOAO/AURA/NSF


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About This Image

A portion of the Veil Nebula, left behind with the violent explosion of a massive star, shows delicate wisps of gas and dust.
Credit: NASA, ESA, and the Hubble Heritage (STScI/AURA)-ESA/Hubble Collaboration
Acknowledgment: J. Hester (Arizona State University)

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[h=4]About This Image[/h] Glowing knots of gas from a dying star look like they're streaking through space. The dense knots, which form in the early stages of a planetary nebula, each contain as much mass as three Earths.
Image Credit: NASA and The Hubble Heritage Team (STScI/AURA)



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[h=4]About This Image[/h] Two cones of matter are being ejected from the central star of the Boomerang Nebula. Measurements made in 1995 show the deep interior of the nebula to have a temperature of just one degree Kelvin above absolute zero, making it one of the coldest known places in the universe.

Credit: NASA, ESA and The Hubble Heritage Team (STScI/AURA)



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[h=4]About This Image[/h] As Saturn takes its 29-year journey around the Sun, its tilt allows us to see its rings from different perspectives. Saturn's tilt also gives it seasons. The lowest image on the left shows the northern hemisphere's autumn, while the uppermost right image shows the winter.
Image Credit: NASA and The Hubble Heritage Team (STScI/AURA)




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[h=4]About This Image[/h] Hubble's 20th anniversary image shows a mountain of dust and gas rising in the Carina Nebula. The top of a three-light-year tall pillar of cool hydrogen is being worn away by the radiation of nearby stars, while stars within the pillar unleash jets of gas that stream from the peaks.




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[h=4]About This Image[/h] A brilliant white core is encircled by thick dust lanes in this spiral galaxy, seen edge-on. The galaxy is 50,000 light-years across and 28 million light years from Earth.





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[h=4]About This Image[/h] The Crab Nebula is a supernova remnant, all that remains of a tremendous stellar explosion. Observers in China and Japan recorded the supernova nearly 1,000 years ago, in 1054.



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[h=4]About This Image[/h] Bright knots of glowing gas light up the arms of spiral galaxy M74, indicating a rich environment of star formation. Messier 74, also called NGC 628, is slightly smaller than our Milky Way.


Credit: NASA, ESA, and the Hubble Heritage (STScI/AURA)-ESA/Hubble Collaboration



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[h=4]About This Image[/h] The Cat's Eye Nebula, one of the first planetary nebulae discovered, also has one of the most complex forms known to this kind of nebula. Eleven rings, or shells, of gas make up the Cat's Eye.
Credit: NASA, ESA, HEIC, and The Hubble Heritage Team (STScI/AURA)



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[h=4]About This Image[/h] The gravity of a galaxy cluster called SDSS J1004+4112 warps and magnifies the light from a distant quasar. Light from the quasar, the bright core of a galaxy fed by a black hole, appears in the center of this image and four other locations around it. Other distant galaxies appear as arcs.



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[h=4]About This Image[/h] Thousands of stars are forming in the cloud of gas and dust known as the Orion nebula. More than 3,000 stars of various sizes appear in this image. Some of them have never been seen in visible light.




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[h=4]About This Image[/h] In the Tarantula Nebula lies a bright cluster of brilliant, massive stars, Hodge 301. The cluster, in the lower right-hand corner, is blasting material from supernovae into the surrounding nebula.



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[h=4]About This Image[/h] The large Whirlpool Galaxy (left) is known for its sharply defined spiral arms. Their prominence could be the result of the Whirlpool's gravitational tug-of-war with its smaller companion galaxy (right).



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[h=4]About This Image[/h] M81, a spiral galaxy similar to our own Milky Way, is one of the brightest galaxies that can be seen from Earth. The spiral arms wind all the way down into the nucleus and are made up of young, bluish, hot stars formed in the past few million years, while the central bulge contains older, redder stars.




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