Stampa:Globular Star Cluster NGC 1466 (2019-42-4567).png
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Fajl oriġinali (3,191 × 3,161 pixel, dimensjoni: 18.96 MB, tip ta' MIME: image/png)
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Taqsira
DeskrizzjoniGlobular Star Cluster NGC 1466 (2019-42-4567).png |
English: This image from NASA's Hubble Space Telescope reveals an ancient, glimmering ball of stars called NGC 1466. It is a globular cluster — a gathering of stars all held together by gravity — that is slowly moving through space on the outskirts of the Large Magellanic Cloud, one of our closest galactic neighbors.
Blue straggler stars are blue, bright stars, with a higher mass than the average for a cluster, and they are expected to sink towards the center of a star cluster over time. Those closest to the cluster core are the first to migrate inwards, with more distant blue stragglers progressively moving inwards over time. |
Data | 9 Settembru 2019 (upload date) |
Sors | Globular Star Cluster NGC 1466 |
Awtur | ESA and NASA |
Verżjonijiet oħra |
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Liċenzja
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. |
copyright status Ingliż
media type Ingliż
image/png
height Ingliż
3,161 pixel
width Ingliż
3,191 pixel
data size Ingliż
19,881,000 byte
checksum Ingliż
338620e7b35102f5890954bbee27cec745fbb7d2
9 Settembru 2019
pHash checksum Ingliż
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Kronoloġija tal-fajl
Agħfas fuq il-grupp data/ħin biex tara l-fajl biex tara kif jidher dak il-ħin.
Data/Ħin | Minjatura | Qisien | Utent | Kumment | |
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kurrenti | 19:22, 26 Awwissu 2023 | 3,191 × 3,161 (18.96 MB) | OptimusPrimeBot | #Spacemedia - Upload of https://stsci-opo.org/STScI-01EVSV7X5X0V7VZ302DCTZF9EY.png via Commons:Spacemedia |
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Dan il-fajl fih aktar informazzjoni, aktarx ġie miżjud minn kamera diġitali jew skanner li ġew użati sabiex joħolquh jew biex jagħmluh diġitali.
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Awtur | Space Telescope Science Institute Office of Public Outreach |
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Titlu tal-istampa |
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Titlu qasir |
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Fornitur | Image: NASA and ESAScience: NASA, ESA, and F. Ferraro (University of Bologna, Italy) |
Titlu | Different structures of star clusters are due to different levels of dynamical aging. |
Sors | STScI |
Termini ta' użu | |
Data u ħin tal-ħolqien tad-data | 9 Settembru 2019 |
Kumment tal-fajl PNG |
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Informazzjoni dwar il-kuntatt | outreach@stsci.edu
3700 San Martin Drive Baltimore, MD, 21218 USA |
Kliem importanti | NGC 1466 |
Data meta l-metadati ġew modifikati l-aħħar | 05:48, 5 Settembru 2019 |
ID unika tad-dokument oriġinali | xmp.did:6b464c15-a3a8-4ef6-aab4-76c56a844ba1 |
Riżoluzzjoni orizzontali | 28.34 dpc |
Riżoluzzjoni vertikali | 28.34 dpc |
Data jew ħin ta' modifiki tal-fajl | 05:31, 5 Settembru 2019 |