Star-studded image of the Sextans B dwarf galaxy showcases astronomical curiosities near and far

This image of the dwarf galaxy Sextans B, taken with the Nicholas U. Mayall 4-meter Telescope at Kitt Peak National Observatory, a Program of NSF’s NOIRLab, contains a menagerie of astronomical objects, from bright stars in the foreground to distant galaxies hiding in the background. The galaxy itself contains both the cradles and the graves of stars, hosting star-forming regions as well as stellar death shrouds. Credit: National Science Foundation

This star-studded image shows the irregular dwarf galaxy Sextans B, which lies around 4.5 million light-years from Earth at the outermost edges of the Local Group. With a total mass of around 200 million times the mass of the Sun, Sextans B hosts an intriguing variety of astronomical objects. Some of the most conspicuous are the ruby-red clouds of atomic hydrogen visible near the center of this image. These vast, glowing clouds are giving birth to brilliant new stars. Supernovae and the stellar winds from these young stars will eventually sweep aside the cool clouds of hydrogen, leaving behind clusters of stars with similar ages and properties.


As well as stellar birthplaces, Sextans B harbors sites of stellar death. Sextans B is one of the smallest galaxies known to contain several planetary nebulae (though they are not visible in this image). Planetary nebulae are the outermost layers of aging red giant stars, thrown out into space at the end of a star’s life.

In addition to Sextans B and its contents, this image features both very distant objects and stars much closer to home. Faraway galaxies can be seen littering the background of this image, noticeable by their fuzzy appearance or irregular shapes. Meanwhile, bright stars from our own galaxy shine in the foreground. Several of the bright nearby stars are surrounded by conspicuous diffraction spikes—the prominent crisscross patterns created by light interacting with the structure of a telescope.

Sextans B takes its names from its parent constellation Sextans (the Sextant). The constellation is one of several identified in 1687 by the astronomer Johannes Hevelius, and it is named after an astronomical instrument he and his wife Elisabeth would use in their observations—many of which were conducted without the aid of a telescope.

https://www.youtube.com/watch?v=/j7ZcO2MPxd4

Though the Heveliuses were able to compile painstakingly accurate star charts without telescopes, astronomical technology has progressed since the 17th century. Rather than working with a sextant, astronomers created this image using the Nicholas U. Mayall 4-meter Telescope at Kitt Peak National Observatory (KPNO). Located in the desert of southern Arizona, KPNO is a Program of NSF’s NOIRLab and is home to one of the largest and most diverse arrays of optical and radio telescopes in the world.

However, no matter the telescope or instrument you use, the night sky is filled with interesting objects to observe—as you can see from the collection of intriguing astronomical objects in this image.


Striking new image of the stately galaxy Messier 106 taken with the Nicholas U. Mayall 4-meter Telescope


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Star-studded image of the Sextans B dwarf galaxy showcases astronomical curiosities near and far (2021, April 29)
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