Файл:Caldwell 104.jpg

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	Дата/вакыт	Кече рәсем	Үлчәмнәре	Кулланучы	Искәрмә
агымдагы	23 фев 2020, 20:02		3981 × 4017 (17,15 Мб)	wikimediacommons-qic>Killarnee

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Кадр куелышы	Гадәти
Ятма ачыклык	72 точек на дюйм
Асма ачыклык	72 точек на дюйм
Кулланылган программа	Adobe Photoshop CC 2015 (Windows)
Файл үзгәреше датасы һәм вакыты	8 июл 2016, 14:42
Порядок размещения компонент Y и C	Центрированный
Exif чыгарышы	2.31
Чын вакыты	24 окт 2016, 06:00
Санлаштыру вакыты	25 май 2016, 22:11
Төсләр төзелешенең конфигурациясе	Y Cb Cr барлыкта юк
FlashPix ярашлы юрамасы	1
Төсләр киңлеге	Некалиброванное
IIM юрамасы	4
Кыска исем	Youthful NGC 362
Иң мөһиме	NGC 362
Поставщик, кто предоставил изображение	ESA/Hubble & NASA
Чыганак	ESA/Hubble
Сурәт исеме	Globular clusters offer some of the most spectacular sights in the night sky. These ornate spheres contain hundreds of thousands of stars, and reside in the outskirts of galaxies. The Milky Way contains over 150 such clusters — and the one shown in this NASA/ESA Hubble Space Telescope image, named NGC 362, is one of the more unusual ones. As stars make their way through life they fuse elements together in their cores, creating heavier and heavier elements — known in astronomy as metals — in the process. When these stars die, they flood their surroundings with the material they have formed during their lifetimes, enriching the interstellar medium with metals. Stars that form later therefore contain higher proportions of metals than their older relatives. By studying the different elements present within individual stars in NGC 362, astronomers discovered that the cluster boasts a surprisingly high metal content, indicating that it is younger than expected. Although most globular clusters are much older than the majority of stars in their host galaxy, NGC 362 bucks the trend, with an age lying between 10 and 11 billion years old. For reference, the age of the Milky Way is estimated to be above 13 billion years. This image, in which you can view NGC 362’s individual stars, was taken by Hubble’s Advanced Camera for Surveys (ACS).
Төс тирәнлеге	8 8 8
Биеклек	4017 нкт
Киңлек	3981 нкт
Төс моделе	RGB
Төс өлешләре саны	3
Элемтә өчен мәгълүмат	http://www.spacetelescope.org Karl-Schwarzschild-Strasse 2 Garching bei München, None, D-85748 Germany
Нәшир	ESA/Hubble
Медиа төре	Observation
Дата последнего изменения метаданных	8 июл 2016, 16:42
Уникальный идентификатор исходного документа	xmp.did:a0f3c21f-5a21-0f46-9cb8-cae74e192c9d
Куллану шартлары	Creative Commons Attribution 4.0 International License
Примечание JPEG-файла	Globular clusters offer some of the most spectacular sights in the night sky. These ornate spheres contain hundreds of thousands of stars, and reside in the outskirts of galaxies. The Milky Way contains over 150 such clusters — and the one shown in this NASA/ESA Hubble Space Telescope image, named NGC 362, is one of the more unusual ones. As stars make their way through life they fuse elements together in their cores, creating heavier and heavier elements — known in astronomy as metals — in the process. When these stars die, they flood their surroundings with the material they have formed during their lifetimes, enriching the interstellar medium with metals. Stars that form later therefore contain higher proportions of metals than their older relatives. By studying the different elements present within individual stars in NGC 362, astronomers discovered that the cluster boasts a surprisingly high metal content, indicating that it is younger than expected. Although most globular clusters are much older than the majority of stars in their host galaxy, NGC 362 bucks the trend, with an age lying between 10 and 11 billion years old. For reference, the age of the Milky Way is estimated to be above 13 billion years. This image, in which you can view NGC 362’s individual stars, was taken by Hubble’s Advanced Camera for Surveys (ACS).