File:Stellar sweet shop (50172756827).jpg
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[edit]DescriptionStellar sweet shop (50172756827).jpg |
Looking its best ever is the star cluster NGC 2203, here imaged by the NASA/ESA Hubble Space Telescope. Aside from its dazzling good looks, this cluster of stars contains lots of astronomical treats that have helped astronomers puzzle together the lifetimes of stars. A main sequence star, like our Sun, is the term applied to a star during the longest period of its life, when it burns fuel steadily. Our Sun’s fuel will run out in approximately 6 billion years, and it will then move on to the next stage of its life when it will turn into a red giant. Astronomers studying NGC 2203, which contais stars that are roughly twice as massive as our Sun, found that their rotation might be a factor as to why some of the stars stay longer than usual in this main-sequence phase of their life. This is the best resolution obtained of the star cluster to date. Credits: ESA/Hubble & NASA, L. Girardiñ; CC BY 4.0 |
Date | |
Source | Stellar sweet shop |
Author | European Space Agency |
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This image was originally posted to Flickr by europeanspaceagency at https://flickr.com/photos/37472264@N04/50172756827. It was reviewed on 3 December 2020 by FlickreviewR 2 and was confirmed to be licensed under the terms of the cc-by-2.0. |
3 December 2020
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current | 14:56, 3 December 2020 | ![]() | 3,892 × 4,035 (13.92 MB) | Eyes Roger (talk | contribs) | Transferred from Flickr via #flickr2commons |
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Date and time of data generation | 06:00, 27 July 2020 |
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Short title | Stellar Sweet Shop |
Credit/Provider | ESA/Hubble & NASA, L. Girardi |
Source | ESA/Hubble |
Image title | Looking its best ever is the star cluster NGC 2203, here imaged by the NASA/ESA Hubble Space Telescope. Aside from its dazzling good looks, this cluster of stars contains lots of astronomical treats that have helped astronomers puzzle together the lifetimes of stars. A main sequence star, like our Sun, is the term applied to a star during the longest period of its life, when it burns fuel steadily. Our Sun’s fuel will run out in approximately 6 billion years, and it will then move on to the next stage of its life when it will turn into a red giant. Astronomers studying NGC 2203, which contais stars that are roughly twice as massive as our Sun, found that their rotation might be a factor as to why some of the stars stay longer than usual in this main-sequence phase of their life. This is the best resolution obtained of the star cluster to date. |
Publisher | ESA/Hubble |
Usage terms |
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JPEG file comment | Looking its best ever is the star cluster NGC 2203, here imaged by the NASA/ESA Hubble Space Telescope. Aside from its dazzling good looks, this cluster of stars contains lots of astronomical treats that have helped astronomers puzzle together the lifetimes of stars. A main sequence star, like our Sun, is the term applied to a star during the longest period of its life, when it burns fuel steadily. Our Sun’s fuel will run out in approximately 6 billion years, and it will then move on to the next stage of its life when it will turn into a red giant. Astronomers studying NGC 2203, which contais stars that are roughly twice as massive as our Sun, found that their rotation might be a factor as to why some of the stars stay longer than usual in this main-sequence phase of their life. This is the best resolution obtained of the star cluster to date. |
Orientation | Normal |
Horizontal resolution | 72 dpi |
Vertical resolution | 72 dpi |
Software used | Adobe Photoshop CC 2019 (Windows) |
File change date and time | 15:59, 4 February 2020 |
Y and C positioning | Centered |
Exif version | 2.32 |
Date and time of digitizing | 19:27, 31 October 2012 |
Meaning of each component |
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Supported Flashpix version | 1 |
Color space | Uncalibrated |
IIM version | 4 |
Keywords | NGC 2203 |
Bits per component |
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Height | 4,035 px |
Width | 3,892 px |
Pixel composition | RGB |
Number of components | 3 |
Contact information |
Karl-Schwarzschild-Strasse 2 Garching bei München, None, D-85748 Germany |
Type of media | Observation |
Date metadata was last modified | 16:59, 4 February 2020 |
Unique ID of original document | xmp.did:ABC7783F8023E21187CDFADFB63A653D |