Hubble Images Milky Way's Big Sister 31 July 2018

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Hubble images Milky Way's big sister 31 July 2018 adding to the argument of this galaxy's liveliness. SN 2005at is a Type Ic supernova, formed when a massive star collapses on itself and loses its hydrogen envelope. Provided by NASA Credit: ESA/Hubble & NASA; acknowledgment: Judy Schmidt This image taken by the NASA/ESA Hubble Space Telescope's Wide Field Camera 3 (WFC3) shows a beautiful spiral galaxy called NGC 6744. At first glance, it resembles our Milky Way albeit larger, measuring more than 200,000 light-years across compared to a 100,000-light-year diameter for our home galaxy. NGC 6744 is similar to our home galaxy in more ways than one. Like the Milky Way, NGC 6744 has a prominent central region packed with old yellow stars. Moving away from the galactic core, one can see parts of the dusty spiral arms painted in shades of pink and blue; while the blue sites are full of young star clusters, the pink ones are regions of active star formation, indicating that the galaxy is still very lively. In 2005, a supernova named 2005at (not visible in this image) was discovered within NGC 6744, 1 / 2 APA citation: Hubble images Milky Way's big sister (2018, July 31) retrieved 29 September 2021 from https://phys.org/news/2018-07-hubble-images-milky-big-sister.html This document is subject to copyright. Apart from any fair dealing for the purpose of private study or research, no part may be reproduced without the written permission. The content is provided for information purposes only. 2 / 2 Powered by TCPDF (www.tcpdf.org).

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