Файл:Caldwell 104.jpg
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Файлан истори
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| Терахь/Хан | Жима | Файлан барам | Декъашхо | Билгалдаккхар | |
|---|---|---|---|---|---|
| карара | 2020, 23 февраль, 20:02 | | 3981 × 4017 (17,15 Мб) | wikimediacommons-qic>Killarnee |
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Метахаамаш
ХӀокху файлаца кхин тӀе хаам бу, гуттара чуйоккхуш йолу терахьца чоьнашца йа тӀейоккхучуьнца. Нагахь файлан тӀаьхьа хийцам бинехь, тӀаккха цхьаболу барам цхьаьна ца ба мега хӀинцалера суьртаца.
| Оригиналан терахь а, хан а | 2016, 24 октябрь, 06:00 |
|---|---|
| Йоцца цӀе | Youthful NGC 362 |
| Кхоьхьург, хьа делла сурт | ESA/Hubble & NASA |
| Хьост | ESA/Hubble |
| Суьртан цӀе | 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). |
| Арахецархо | ESA/Hubble |
| Лелоран биллам |
|
| JPEG-файлан билгалдаккхар | 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). |
| Кадран ориентаци | Лартӏахь |
| Шоралла | 72 тӏадамаш дюйман |
| Локхалла | 72 тӏадамаш дюйман |
| Лелина программа | Adobe Photoshop CC 2015 (Windows) |
| Файлан хийцам бина терахь а, хан а | 2016, 8 июль, 14:42 |
| Y а, C а компонентин листаран кеп | Йукъйина |
| Верси Exif | 2.31 |
| Оцифровк йина терахь а, хан а | 2016, 25 май, 22:11 |
| Бесара компонентин конфигураци |
|
| Ловш йолу верси FlashPix | 1 |
| Беснийн меттиг | Калибраци ца йина |
| Верси IIM | 4 |
| Коьрта дешнаш | NGC 362 |
| Бесан кIоргалла |
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| Локхалла | 4017 пкс |
| Шоралла | 3981 пкс |
| Беснин модель | RGB |
| Беснийн компонентийн дукхалла | 3 |
| Контактан хаам |
Karl-Schwarzschild-Strasse 2 Garching bei München, None, D-85748 Germany |
| Медиан тайп | Observation |
| ТӀаьххьара метахаамаш хийцина терахь | 2016, 8 июль, 16:42 |
| Йуьхьанцара документан ша тайпа ID | xmp.did:a0f3c21f-5a21-0f46-9cb8-cae74e192c9d |
