Hubble Space Telescope image showcasing the globular cluster NGC 6540 in the constellation Sagittarius. Credit: ESA/Hubble & NASA, R. Cohen
This scintillating image, which was captured by the NASA/ESA Hubble Space Telescope’s Wide Field Camera 3 and Advanced Camera for Surveys, showcases the globular cluster NGC 6540 in the constellation Sagittarius. These two instruments each have slightly different fields of view — which determines how large an area of sky each instrument captures at one time. 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, which is 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.
Prominent cross-shaped patterns of light known as diffraction spikes adorn the brightest stars in this image. These astronomical embellishments are a type of imaging artifact. This means 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, which causes bright objects to be surrounded by spikes of light.
Hubble peered into the heart of NGC 6540 to assist astronomers in measuring the ages, shapes, and structures of globular clusters towards the center of the Milky Way. The gas and dust shrouding the center of our galaxy block some of the light from these clusters, as well as subtly changing the colors 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.
Hubble Space Telescope image showcasing the globular cluster NGC 6540 in the constellation Sagittarius. Credit: ESA/Hubble & NASA, R. Cohen
This scintillating image, which was captured by the NASA/ESA Hubble Space Telescope’s Wide Field Camera 3 and Advanced Camera for Surveys, showcases the globular cluster NGC 6540 in the constellation Sagittarius. These two instruments each have slightly different fields of view — which determines how large an area of sky each instrument captures at one time. 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, which is 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.
Prominent cross-shaped patterns of light known as diffraction spikes adorn the brightest stars in this image. These astronomical embellishments are a type of imaging artifact. This means 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, which causes bright objects to be surrounded by spikes of light.
Hubble peered into the heart of NGC 6540 to assist astronomers in measuring the ages, shapes, and structures of globular clusters towards the center of the Milky Way. The gas and dust shrouding the center of our galaxy block some of the light from these clusters, as well as subtly changing the colors 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.