File:Globular Clusters around Milky Way (2019-16-4369).jpg
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DescriptionGlobular Clusters around Milky Way (2019-16-4369).jpg |
English: This illustration shows the fundamental architecture of our island city of stars, the Milky Way galaxy: a spiral disk, central bulge, and diffuse halo of stars and globular star clusters. Not shown is the vast halo of dark matter surrounding our galaxy. A comprehensive survey that combines the observing prowess of both the Hubble Space Telescope and the European Space Agency's Gaia satellite measured the total mass of our galaxy at 1.5 trillion solar masses. Only a few percent of the estimated 200 billion stars in our galaxy contributes to this total. Most of the rest is locked up in invisible dark matter. The precision of Hubble and Gaia each allowed astronomers to measure the movement of the isolated spherical islands called globular star clusters. The more massive a galaxy, the faster its clusters move under the pull of gravity. And, this allows for the mass of our galaxy to be calculated. |
Date | 7 March 2019 (upload date) |
Source | Globular Clusters around Milky Way |
Author | NASA, ESA, and A. Feild (STScI) |
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Licensing[edit]
Public domainPublic domainfalsefalse |
This file is in the public domain because it was created by NASA and ESA. NASA Hubble material (and ESA Hubble material prior to 2009) is copyright-free and may be freely used as in the public domain without fee, on the condition that only NASA, STScI, and/or ESA is credited as the source of the material. This license does not apply if ESA material created after 2008 or source material from other organizations is in use. The material was created for NASA by Space Telescope Science Institute under Contract NAS5-26555, or for ESA by the Hubble European Space Agency Information Centre. Copyright statement at hubblesite.org or 2008 copyright statement at spacetelescope.org. For material created by the European Space Agency on the spacetelescope.org site since 2009, use the {{ESA-Hubble}} tag. |
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Date/Time | Thumbnail | Dimensions | User | Comment | |
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current | 03:01, 20 January 2024 | 3,600 × 2,700 (3.48 MB) | OptimusPrimeBot (talk | contribs) | #Spacemedia - Upload of https://stsci-opo.org/STScI-01EVSWQKMY3GJBHC7CB25A3D60.jpg via Commons:Spacemedia |
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This file contains additional information such as Exif metadata which may have been added by the digital camera, scanner, or software program used to create or digitize it. If the file has been modified from its original state, some details such as the timestamp may not fully reflect those of the original file. The timestamp is only as accurate as the clock in the camera, and it may be completely wrong.
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Credit/Provider | NASA/JPL-Caltech/2MASS/B. Whitney (SSI/University of Wisconsin) |
Headline | A star forming region called BG2107+49 shines from the considerable distance of more than 30,000 light years away in the upper left of this image. |
Source | Spitzer Science Center |
Usage terms |
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Date and time of data generation | 28 July 2010 |
Width | 2,400 px |
Height | 2,400 px |
Bits per component |
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Compression scheme | LZW |
Pixel composition | RGB |
Orientation | Normal |
Number of components | 3 |
Horizontal resolution | 300 dpi |
Vertical resolution | 300 dpi |
Data arrangement | chunky format |
Software used | Adobe Photoshop CC 2017 (Macintosh) |
File change date and time | 12:40, 4 March 2019 |
Exif version | 2.21 |
Color space | sRGB |
Contact information |
http://www.spitzer.caltech.edu MS 220-6, 1200 E. California Blvd. Pasadena, CA, 91125 USA |
Keywords | BG2107+49 |
Date and time of digitizing | 08:50, 21 May 2012 |
Date metadata was last modified | 07:40, 4 March 2019 |
Unique ID of original document | xmp.did:2AA88C1A0E2068118C14FCC293DF2965 |
Copyright status | Copyright status not set |
IIM version | 4 |