Найти тему
Хайтек

Посмотрите на новый снимок «Хаббла»: он поможет раскрыть раннюю историю Млечного Пути

   This scintillating image showcases the globular cluster NGC 6540 in the constellation Sagittarius, which was captured by the NASA/ESA Hubble Space Telescope’s Wide Field Camera 3 and Advanced Camera for Surveys. These two instruments have slightly different fields of view — which determines how large an area of sky each instrument captures. This composite image shows the star-studded area of sky that was captured in both instruments’ field of view.  NGC 6540 is a globular cluster, a stable, tightly bound multitude of stars. The populations of these clusters can range from tens of thousands to millions of stars, all of which are trapped in a closely-packed group by their mutual gravitational attraction. The brightest stars in this image are adorned with prominent cross-shaped patterns of light known as diffraction spikes. These astronomical embellishments are a type of imaging artefact, meaning that they are caused by the structure of Hubble rather than the stars themselves. The path taken by the starlight as it enters the telescope is slightly disturbed by its internal structure, causing bright objects to be surrounded by spikes of light. Hubble peered into the heart of NGC 6540 to help astronomers measure the ages, shapes, and structures of globular clusters towards the centre of the Milky Way. The gas and dust shrouding the centre of our galaxy block some of the light from these clusters, as well as subtly changing the colours of their stars. Globular clusters contain insights into the earliest history of the Milky Way, and so studying them can help astronomers understand how our galaxy has evolved. Анастасия Никифорова
This scintillating image showcases the globular cluster NGC 6540 in the constellation Sagittarius, which was captured by the NASA/ESA Hubble Space Telescope’s Wide Field Camera 3 and Advanced Camera for Surveys. These two instruments have slightly different fields of view — which determines how large an area of sky each instrument captures. This composite image shows the star-studded area of sky that was captured in both instruments’ field of view. NGC 6540 is a globular cluster, a stable, tightly bound multitude of stars. The populations of these clusters can range from tens of thousands to millions of stars, all of which are trapped in a closely-packed group by their mutual gravitational attraction. The brightest stars in this image are adorned with prominent cross-shaped patterns of light known as diffraction spikes. These astronomical embellishments are a type of imaging artefact, meaning that they are caused by the structure of Hubble rather than the stars themselves. The path taken by the starlight as it enters the telescope is slightly disturbed by its internal structure, causing bright objects to be surrounded by spikes of light. Hubble peered into the heart of NGC 6540 to help astronomers measure the ages, shapes, and structures of globular clusters towards the centre of the Milky Way. The gas and dust shrouding the centre of our galaxy block some of the light from these clusters, as well as subtly changing the colours of their stars. Globular clusters contain insights into the earliest history of the Milky Way, and so studying them can help astronomers understand how our galaxy has evolved. Анастасия Никифорова

Шаровое скопление NGC 6540 находится в созвездии Стрельца. Астрономы сделали изображение с помощью широкоугольной камеры НАСА/ЕКА 3 и усовершенствованной камеры для обзоров.

Инструменты различаются полем зрения: это влияет на то, насколько большую область неба захватывает каждый из них. На новом составном изображении показана усеянная звездами область неба, которую засняли оба инструмента.

NGC 6540 — стабильное шаровое скопление, тесно связанное множество звезд. Население этих скоплений варьируется от десятков тысяч до миллионов звезд. Все они заключены в плотную группу из-за взаимного гравитационного притяжения.

Самые яркие звезды на изображении украшены заметными крестообразными световыми узорами, известными как дифракционные всплески. Эти артефакты изображения вызваны структурой «Хаббла», а не самими звездами. Путь, по которому проходит звездный свет, когда он попадает телескоп, слегка нарушен его внутренней структурой, в результате чего яркие объекты окружены вспышками света.

«Хаббл» изучил сердце NGC 6540, чтобы астрономы измерили возраст, форму и структуру шаровых скоплений в центре Млечного Пути. Газ и пыль, покрывающие центр галактики, блокируют часть света от скоплений, а также слегка меняют цвета их звезд. Шаровые скопления содержат информацию о самой ранней истории Млечного Пути.

Читать далее:

«Джеймс Уэбб» прислал фото столкновения двух огромных галактик

«Бесполезная» бактерия на Земле обеспечит жизнь колонизаторам Марса

На пирамиде в Китае нашли портрет «царя предков». Он правил более 4 000 лет назад