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    Home»Space»Hubble Views Galaxy 2MASX J05210136-2521450
    Space

    Hubble Views Galaxy 2MASX J05210136-2521450

    By European Space Agency/NASA Hubble; NASAMay 13, 20132 Comments1 Min Read
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    Hubble Views Galaxy 2MASX J05210136 2521450
    Hubble Space Telescope image of a galaxy cataloged as 2MASX J05210136-2521450. Credit: ESA/Hubble & NASA, Acknowledgment: Luca Limatola

    This new image from the Hubble Space Telescope shows galaxy 2MASX J05210136-2521450.

    When we look into the distant cosmos, the great majority of the objects we see are galaxies: immense gatherings of stars, planets, gas, dust, and dark matter, showing up in all kinds of shapes. This Hubble picture registers several, but the galaxy cataloged as 2MASX J05210136-2521450 stands out at a glance due to its interesting shape.

    This object is an ultraluminous infrared galaxy that emits a tremendous amount of light at infrared wavelengths. Scientists connect this to intense star formation activity, triggered by a collision between two interacting galaxies.

    The merging process has left its signs: 2MASX J05210136-2521450 presents a single, bright nucleus and a spectacular outer structure that consists of a one-sided extension of the inner arms, with a tidal tail heading in the opposite direction, formed from material ripped out from the merging galaxies by gravitational forces.

    The image is a combination of exposures taken by Hubble’s Advanced Camera for Surveys, using near-infrared and visible light.

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    Astronomy European Space Agency Hubble Space Telescope NASA
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    2 Comments

    1. Peter Jackson FRAS on May 14, 2013 3:06 am

      According to a good-fit theoretical analysis this is simply a single galaxy with helically precessing outflows oriented towards and away the HSC.

      Reply
    2. Shivam pyasi on June 17, 2013 7:37 pm

      Last night i saw a planet ( star or other things) which speed is very fast like a light,
      His motion started to one star to universe,
      what is this please tell me,

      Reply
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