File:NGC 2906 galaxy.jpg
Original file (1,280 × 832 pixels, file size: 133 KB, MIME type: image/jpeg)
This is a file from the Wikimedia Commons. Information from its description page there is shown below. Commons is a freely licensed media file repository. You can help. |
Summary
DescriptionNGC 2906 galaxy.jpg |
English: This image depicts a swirling spiral galaxy named NGC 2906.
The blue speckles seen scattered across this galaxy are massive young stars, which emit hot, blue-tinged radiation as they burn through their fuel at an immense rate. The swathes of orange are a mix of older stars that have swollen and cooled, and low-mass stars that were never especially hot to begin with. Owing to their lower temperatures, these stars emit a cooler, reddish, radiation. This image of NGC 2906 was captured by the NASA/ESA Hubble Space Telescope’s Wide Field Camera 3, an instrument installed on Hubble in 2009 during the telescope’s fourth servicing mission. Hubble observed this galaxy on the hunt for fading light from recent, nearby occurrences of objects known as supernovae. Credit: ESA/Hubble & NASA, A Filippenko |
Date | |
Source | https://www.spacetelescope.org/images/potw2015a/ |
Author | ESA/Hubble & NASA, A Filippenko |
Licensing
ESA/Hubble images, videos and web texts are released by the ESA under the Creative Commons Attribution 4.0 International license and may on a non-exclusive basis be reproduced without fee provided they are clearly and visibly credited. Detailed conditions are below; see the ESA copyright statement for full information. For images created by NASA or on the hubblesite.org website, or for ESA/Hubble images on the esahubble.org site before 2009, use the {{PD-Hubble}} tag.
Conditions:
Notes:
|
- You are free:
- to share – to copy, distribute and transmit the work
- to remix – to adapt the work
- Under the following conditions:
- attribution – You must give appropriate credit, provide a link to the license, and indicate if changes were made. You may do so in any reasonable manner, but not in any way that suggests the licensor endorses you or your use.
Items portrayed in this file
depicts
13 April 2020
File history
Click on a date/time to view the file as it appeared at that time.
Date/Time | Thumbnail | Dimensions | User | Comment | |
---|---|---|---|---|---|
current | 10:23, 19 May 2020 | 1,280 × 832 (133 KB) | Garamora | Uploaded a work by ESA/Hubble & NASA, A Filippenko from https://www.spacetelescope.org/images/potw2015a/ with UploadWizard |
File usage
The following page uses this file:
Metadata
This file contains additional information, probably added from the digital camera or scanner used to create or digitize it.
If the file has been modified from its original state, some details may not fully reflect the modified file.
Credit/Provider | ESA/Hubble & NASA, A Filippenko |
---|---|
Source | ESA/Hubble |
Short title |
|
Image title |
|
Usage terms |
|
Date and time of data generation | 06:00, 13 April 2020 |
JPEG file comment | The NASA/ESA Hubble Space Telescope peers deeply into a site of star formation in this image. Numerous young stars appear veiled here by smoke, as if freshly forged in a foundry. This smoky haze is actually the gas and dust permeating this stellar factory, which is being illuminated by hot new stars. This star forge is found within an object known as NGC 1333, located about 1000 light-years away in the constellation of Perseus (The Hero). NGC 1333 is a reflection nebula — a vast cloud of gas that, as the name suggests, reflects and scatters the light from nearby stars out into space. In fact, the star forge in this image could just as easily be called a planet forge, or a Solar System forge — but how so? Well, stars form as cool gas pools into a cloud and begins to collapse under the force of gravity. The core of this cloud compresses and heats up, eventually shining forth and springing to life as a fully-fledged star. Some of the remaining material is blasted away, but often some remains in a disc around the forming star. It is from this disc that planets develop, as grains gather together into larger and larger rocky entities to form individual planets and, over time, full planetary systems. |
Software used | Adobe Photoshop CC 2019 (Windows) |
File change date and time | 14:16, 29 November 2019 |
Date and time of digitizing | 18:57, 27 November 2019 |
Date metadata was last modified | 15:16, 29 November 2019 |
Unique ID of original document | xmp.did:1175e424-5ae7-f441-9489-d4fb12a5a4d3 |
Keywords | NGC 2906 |
Contact information |
Karl-Schwarzschild-Strasse 2 Garching bei München, None, D-85748 Germany |
IIM version | 4 |