Extreme Star Birth in Merging Galaxies

The newest image released from the Hubble Space Telescope shows the turbulent region where two galaxies are merging together. The galactic collision is known as Arp 220, and it’s one of the nearest, brightest examples of this in the sky. Hubble’s keen vision has located more than 200 massive star clusters, the largest of which is twice as big as anything we have in the Milky Way. Arp 220 should continue producing new start clusters until it runs out of gas in about 40 million years.

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An international team of astronomers have discovered a massive gas ball hurtling through a distant galaxy cluster. This ball of gas is traveling more than 750 km/second (466 miles/second) through galaxy cluster Abell 3266. The enormous speed and pressure has heated the gas up to the point that it blazes in the X-ray spectrum. The discovery was made using ESA’s XMM-Newton X-ray satellite.

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Globular Cluster 47 Tucanae



One of the biggest brightest clusters of stars in the sky is 47 Tucanae, located in the southern constellation of the Toucan. Located about 16,000 light years away, this globular cluster contains a million times the mass of our Sun, and measures 120 light years across. The stars in the cluster are so dense, they average only 1/10th a light year apart; approximately the size of the Solar System. This photograph was taken using the European Southern Observatory’s Very Large Telescope

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Highway of Stars in the Sky



A pair of astronomers from the US and Italy have discovered a stream of stars moving through the sky at 230 km/second (500,000 mph). The stream has been found to extend 30,000 light years across the sky, but it could extend even further. The discoverers believe the stream is all the remains of a gigantic star cluster that was torn apart by the Milky Way’s gravity. If correct, there could be hundreds more of these streams circling our galaxy.

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Supernovae Generated the Universe’s Early Dust



As early as 700 million years after the Big Bang, galaxies were already filled with cosmic dust. But where did it come from? There are two known sources of dust: old stars and supernovae. Astronomers studied nearby supernovae SN 2003gd using the Spitzer space telescope, and found that it had produced tremendous amounts of dust. Since there were many supernovae in the early Universe, they could be the source of all this dust

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The Hubble Space Telescope captured this magnificent view of disk galaxy NGC 5866, seen nearly edge on from our vantage point. The galaxy’s dark dust lane is clearly visible, and it appears to be slightly warped, compared to the disk of starlight. This indicates that it probably brushed past another galaxy in the distant past. NGC 5866 is located in the constellation Draco, approximately 44 million light-years away; it’s similar in mass to the Milky Way, but only two-thirds the diameter.

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Large Amounts of Carbon Around a Distant Star



Astronomers have discovered a solar system with an unusually high amount of carbon; it could be at the stage where the rocky planets are forming. The system, called Beta Pictoris, is located 63 light-years from Earth and has a central star with twice the mass of our Sun. NASA’s FUSE (Far Ultraviolet Spectroscopic Explorer) and Hubble observed that gas around the star matches the composition of our own Solar System quite well. The stars intense radiation should be driving this gas away, but ionized carbon atoms are acting as a brake to keep it contained.

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Colliding Galaxies Simulated



Just like many businesses, galaxies grow through mergers and acquisitions. As galaxies are made up of countless individual stars, simulating these mergers is tremendously challenging, even for the most powerful supercomputers. A international team of researchers have produced a new simulation that shows how colliding galaxies are connected by a “bridge” of material, and spew out enormous tails of dust and debris. New programming and hardware upgrades have made this kind of simulation possible to do.

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Amazing Images Spiral,
Cheers

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