Файл:Caldwell 104.jpg

АгӀонан чулацам кхечу меттанашкахь тӀекхочуш бац.
ХӀара агӀо Википеди чуьра йу — маьрша энциклопеди

Оригиналан файл(3981 × 4017 пиксель, файлан барам: 17,15 Мб, MIME-тайп: image/jpeg)

ХӀара файл Викиларма чуьра йу и лело йиш йу массо проекташкахь. Цунна хаам гайтина лахахь. Файл Викилармехь

Файлах лаьцна

Цуьнах лаьцна
English: This Hubble image captures what looks like a galactic glitter bomb in the night sky. Caldwell 104, also cataloged as NGC 362, is a globular star cluster located about 27,000 light-years away. Among the earliest homesteaders of the universe, globular clusters are snow-globe-shaped islands of several hundred thousand (or more) ancient stars. Globular clusters like Caldwell 104 typically reside in a spiral galaxy’s halo, which is a relatively sparsely populated, spherical area that surrounds the galaxy like a shell. They are integral to the birth and growth of their host galaxies.

Caldwell 104 is one of about 150 globular clusters in the Milky Way galaxy, but it stands out from the rest. The cluster is unusually young, as indicated by its composition. Following the Big Bang, the universe consisted only of hydrogen and a little helium. The first stars formed from this material and, through the process of nuclear fusion, spent their lives producing heavier elements, which astronomers call “metals.” But the process can only continue for so long before the stars either run out of fuel or grow unstable. Ultimately, massive stars are doomed to explode in violent events called supernovae, which blast their material out into the cosmos. This stellar detritus is recycled into new generations of stars, so stars that form later contain higher proportions of metals than their older relatives.

Astronomers have discovered that Caldwell 104 boasts a surprisingly high metal content, which means that it formed more recently than expected. Most globular clusters are much older than the majority of stars in their host galaxy, but the stars in Caldwell 104 appear to be 2 billion to 3 billion years younger than stars in other Milky Way globulars. Astronomers have used Hubble multiple times to investigate the young cluster’s stellar population. This image was taken in visible light using Hubble's Advanced Camera for Surveys.

Discovered from Australia by Scottish astronomer James Dunlop in 1826, Caldwell 104 cannot be viewed from the Northern Hemisphere except near the equator, but it can be seen year-round from mid-Southern latitudes in the constellation Tucana, near the Small Magellanic Cloud. Binoculars or a modest telescope will provide a somewhat hazy view of the magnitude-6.4 cluster, but a large telescope will reveal individual stars.

For more information about Hubble’s observations of Caldwell 104, see:

https://www.spacetelescope.org/images/potw1643a/

For Hubble's Caldwell catalog site and information on how to find these objects in the night sky, visit:

https://www.nasa.gov/content/goddard/hubble-s-caldwell-catalog
Терахь (released)
Хьост https://www.flickr.com/photos/144614754@N02/49214617111/; see also https://www.flickr.com/photos/europeanspaceagency/30236689120/
Автор ESA/Hubble & NASA

Лицензи

w:ru:Creative Commons
авторш билгалбар
авторш билгалбар
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:
  • The full image or footage credit must be presented in a clear and readable manner to all users, with the wording unaltered (for example: "ESA/Hubble"). Web texts should be credited to ESA/Hubble (except when used by media). The credit should not be hidden or disassociated from the image footage. Links should be active if the credit is online. See the usage rights Q&A section on the ESA copyright page for guidance.
  • ESA/Hubble materials may not be used to state or imply the endorsement by ESA/Hubble or any ESA/Hubble employee of a commercial product or service.
  • ESA/Hubble requests a copy of the product sent to them to be indexed in their archive.
  • If an image shows an identifiable person, using that image for commercial purposes may infringe that person's right of privacy, and separate permission should be obtained from the individual.
  • If images or visuals are changed significantly from the original work (apart from resizing, cropping), we suggest that the changes are mentioned after the credit line. For example "Original image by ESA/Hubble (M. Kornmesser), warping and recolouring by NN".

Notes:

  • Note that this general permission does not extend to the use of ESA/Hubble's logo, which shall remain protected and may not be used or reproduced without prior and individual written consent of ESA/Hubble.
  • Also note that music, scientific papers and code on the esahubble.org site are not released under this license and can not be used for non-ESA/Hubble products.
  • By reproducing ESA/Hubble material, in part or in full, the user acknowledges the terms on which such use is permitted.
w:ru:Creative Commons
авторш билгалбар
ХӀара файл лело йиш йу Creative Commons Attribution 4.0 International лицензица.
Авторан цӀе дӀайазйар: ESA/Hubble
Хьа йиш йу маьрша:
  • произведени йаржо – копи йан, йаржо а, хӀара произведи дӀасайекъа а.
  • арахецарш кхолла – хӀара произведени дӀасайекъа
Лахара хьолаца лело мега:
  • авторш билгалбар – Ахьа авторш билгалбан беза (хьост) кхин авторо йа лицензи хӀотточо билгалйина бакъо (амма авторо ахьа дешдерг кхобалдина санна ма-хилийта).
w:ru:Creative Commons
авторш билгалбар
ХӀара файл лело йиш йу Creative Commons Attribution 2.0 Generic лицензица.
Хьа йиш йу маьрша:
  • произведени йаржо – копи йан, йаржо а, хӀара произведи дӀасайекъа а.
  • арахецарш кхолла – хӀара произведени дӀасайекъа
Лахара хьолаца лело мега:
  • авторш билгалбар – Ахьа авторш билгалбан беза (хьост) кхин авторо йа лицензи хӀотточо билгалйина бакъо (амма авторо ахьа дешдерг кхобалдина санна ма-хилийта).
Это изображение изначально опубликовано на Flickr участником проекта NASA Hubble по ссылке https://flickr.com/photos/144614754@N02/49214617111. Оно было досмотрено 2020 шeран 23 февраль роботом FlickreviewR 2, который подтвердил, что изображение лицензировано в соответствии с условиями cc-by-2.0.

2020 шeран 23 февраль

Куьг

ТӀетоха кху могӀанан тӀе хӀокху файлах лаьцна хаам
Caldwell 104

ХӀокху файл тӀера элементаш

гойту объект

ХӀокху билгалонан цхьадолу маьӀнаш ду элемент йоцуш

MIME-тип оьрсийн

image/jpeg

6613c981461a4c3e2503a616f2527e1006845673

метод определения оьрсийн: SHA-1 оьрсийн

17 981 475 байт

высота/рост оьрсийн

4017 пиксель

ширина оьрсийн

3981 пиксель

Файлан истори

Тlетаlаде терахь/хан, муха хилла хьажарна и файл.

Терахь/ХанЖимаФайлан барамДекъашхоБилгалдаккхар
карара2020, 23 февраль, 20:02Жимо верси 2020, 23 февраль, 20:023981 × 4017 (17,15 Мб)KillarneeUser created page with UploadWizard

ХӀара файл лахарчу 1 агӀонгахь лелош йу:

Глобалан файл лелор

ХӀара файл лелош йу лахахь гайтина йолу википедеш чохь:

Метахаамаш