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Hubble photographed a random group of galaxies

Universe Today

A collection of galaxies photographed by Hubble

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Like a photographer, who takes random pictures of a crowd of people, NASA's Hubble Space Telescope took a picture of a collection of galaxies. Hubble's advanced camera wasn't looking for a specific target when it took this image. The camera simply photographed a typical region of the sky, while Hubble's infrared camera looked at a target in a nearby galaxy-rich region.

The night of the galaxies in the image, taken in September 2003, includes a yellow spiral galaxy whose arms have been stretched, possibly as a result of a collision (bottom right of the image); A young blue galaxy full of newborn stars (top of image) and several smaller red galaxies.

The strangest looking galaxy of the bunch, with the blue arc in the center of the image, is actually an optical illusion. The blue rainbow is actually the image of a distant galaxy, smeared into a strange shape by a phenomenon called gravitational lensing. This "hall of mirrors" effect occurs when light from a distant object is bent and stretched by a mass that is between us and the object. In the present case, the gravitational lens, or the mass that causes the distortion, is a red elliptical galaxy about 6 billion light-years from Earth. The red color of the galaxy indicates the formation of older, colder stars.

The distant object, whose image is smeared next to the long blue arc, is about 10 billion years away from us. This ancient galaxy existed just a few million years after the Big Bang, when the universe was about a quarter of its current age. Its blue color indicates the inventions of young and hot stars in the galaxy.

Gravitational lenses can be seen in many places in the sky, as the universe is littered with galaxies. Hence, a pine of distant galaxies cannot move through space without encountering another galaxy along the way. It's like walking through a crowded airport. In space, light from a distant galaxy will pass through a galaxy on the way, but if the galaxy is massive enough, its gravity will bend and distort the light from the distant galaxy.

Long arcs like the one seen here are a common sight in large clusters of galaxies due to the huge concentration of mass. However, the arcs are not so common in the case of single galaxies such as the one in the picture. For the gravitational collapse to occur, the galaxies must be almost perfectly aligned.

Gravitational lensing provides important information about galaxies. They are a unique and particularly efficient way to directly determine the mass of the galaxy, including the mass of the dark matter in it. Galaxies are not made up of stars, gas and dust only. Most of the mass of the galaxy is an invisible type of matter, called dark matter. A study of this galaxy system, discovered not long ago and named J033238-275653, was published in the Astrophysical Journal Letters. This study, along with other observations, may help astronomers directly measure the masses of bright, nearby galaxies for the first time.

Translation: Dikla Oren

The article in Universe Today
Knowledge of astrophysics - stars and galaxies

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