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File:Rotation of the Large Magellanic Cloud ESA393163.png

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Summary

Description
English: The Large Magellanic Cloud (LMC), one of the nearest galaxies to our Milky Way, as viewed by ESA’s Gaia satellite using information from the mission’s second data release.

This image combines the total amount of radiation detected by Gaia in each pixel with measurements of the radiation taken through different filters on the spacecraft to generate colour information. Information about the proper motion of stars – their velocity across the sky – is represented as the texture of the image. Measuring the proper motion of several million stars in the LMC, astronomers were able to see an imprint of the stars rotating clockwise around the centre of the galaxy. The image processing technique used to create this image is called Line Integral Convolution.

Acknowledgement: Gaia Data Processing and Analysis Consortium (DPAC); A. Moitinho / A. F. Silva / M. Barros / C. Barata, University of Lisbon, Portugal; H. Savietto, Fork Research, Portugal; P. McMillan, Lund Observatory, Sweden
Date
Source http://www.esa.int/spaceinimages/Images/2018/04/Rotation_of_the_Large_Magellanic_Cloud
Author European Space Agency
Permission
(Reusing this file)
ESA/Gaia/DPAC,CC BY-SA 3.0 IGO
Title
InfoField
Rotation of the Large Magellanic Cloud
Mission
InfoField
Gaia
Activity
InfoField
Space Science

Licensing

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This file is licensed under the Creative Commons Attribution-ShareAlike 3.0 IGO license.
Attribution: ESA/Gaia/DPAC, CC BY-SA IGO 3.0
You are free:
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25 April 2018

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Date/TimeThumbnailDimensionsUserComment
current14:06, 3 April 2019Thumbnail for version as of 14:06, 3 April 20191,000 × 1,000 (2.83 MB)European Space Agency, Id 393163, http://www.esa.int/spaceinimages/Images/2018/04/Rotation_of_the_Large_Magellanic_Cloud, User:Fæ/Project_list/ESA

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