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Hubble Views a Galaxy on the ‘Dark Side’


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Hubble Views a Galaxy on the ‘Dark Side’

glowing center and spiral arms, flecked with blue-hued stars, of galaxy NGC 5585 against the black backdrop of space

 

Resting on the tail of the Great Bear in the constellation of Ursa Major lies NGC 5585, a spiral galaxy that is more than it appears.

 

The many stars and clouds of dust and gas that make up NGC 5585, shown here in this Hubble image, contribute only a small fraction

 

of the total mass of the galaxy. As in many galaxies, this discrepancy can be explained by the abundant yet seemingly invisible

 

presence of dark matter, a mysterious material that astronomers can’t directly observe.

 

The stellar disk of the galaxy extends over 35,000 light-years across. When compared with galaxies of a similar shape and size, NGC

 

5585 stands out by having a notably different composition. Contributing to the total mass of the galaxy, it contains a far higher

 

proportion of dark matter.

 

Hot spots of star formation can be seen along the galaxy’s faint spiral arms. These regions shine a brilliant blue, contrasting strikingly

 

against the ever-black background of space.

 

Text credit: ESA (European Space Agency)


Image credit: ESA/Hubble & NASA, R. Tully; acknowledgment: Gagandeep Anand

 

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