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Peruse Hubble images of beautiful astronomical objects visible in the night sky

This year, the beloved Hubble Space Telescope turned 30. Launched in 1990, it has been instrumental in helping us understand the expansion of the universe and has allowed us to peer out at objects far beyond our solar system.

Now, NASA has updated its Hubble Caldwell catalog, a collection of some of the most beautiful images Hubble has captured throughout the years. The Caldwell catalog project, which began in 1995, was a list originally compiled by astronomer Sir Patrick Caldwell-Moore as an addition to the traditional Messier catalog which lists astronomical objects that can be seen in the sky. The Caldwell catalog contains 109 objects including galaxies, nebulae, and star clusters which are visible to amateur astronomers.

For astronomers who want to refer to highly detailed images of the objects they’re observing, or simply for those who love to enjoy stunning images of space, the Hubble Caldwell catalog shows all of these objects in exquisite detail, as well as a map of where in the night sky each is located.

We’ve shared some of our favorite additions to the catalog below, which include dusty nebulae, distant galaxies, and bright star clusters:

This stunning image captures a small region on the edge of the inky Coalsack Nebula, or Caldwell 99.
This stunning image captures a small region on the edge of the inky Coalsack Nebula, or Caldwell 99. NASA, ESA, and R. Sahai (Jet Propulsion Laboratory); Processing: Gladys Kober (NASA/Catholic University of America)
Caldwell 72, also known as NGC 55, is a galaxy located 6.5 million light-years from Earth in the constellation Sculptor.
Caldwell 72, also known as NGC 55, is a galaxy located 6.5 million light-years from Earth in the constellation Sculptor. NASA, ESA, R. de Jong (Leibniz-Institut fur Astrophysik Potsdam [AIP]), and G. Illingworth (University of California – Santa Cruz); Processing: Gladys Kober (NASA/Catholic University of America)
Caldwell 29, also known as NGC 5005, is a spiral galaxy that likely harbors a supermassive black hole at its heart.
Caldwell 29, also known as NGC 5005, is a spiral galaxy that likely harbors a supermassive black hole at its heart. NASA, ESA, and L. Ho (Peking University); Processing: Gladys Kober (NASA/Catholic University of America)
This beautiful Hubble image captures the core and some of the spiral arms of the galaxy Caldwell 36. Also known as NGC 4559, this spiral galaxy is located roughly 30 million light-years from Earth in the constellation Coma Berenices.
This beautiful Hubble image captures the core and some of the spiral arms of the galaxy Caldwell 36. Also known as NGC 4559, this spiral galaxy is located roughly 30 million light-years from Earth in the constellation Coma Berenices. NASA, ESA, and S. Smartt (The Queen's University of Belfast); Processing: Gladys Kober (NASA/Catholic University of America)
Galaxies consist of a number of different structures, and the particulars of these structures drive the evolution of a given galaxy. One such structure in spiral galaxies like Caldwell 40 (or NGC 3626) is the galactic bulge. This structure is a densely packed region of stars that encompasses the heart of a spiral galaxy.
Galaxies consist of a number of different structures, and the particulars of these structures drive the evolution of a given galaxy. One such structure in spiral galaxies like Caldwell 40 (or NGC 3626) is the galactic bulge. This structure is a densely packed region of stars that encompasses the heart of a spiral galaxy. NASA, ESA, and P. Erwin (Max Planck Institute for Extraterrestrial Physics); Processing: Gladys Kober (NASA/Catholic University of America)
Caldwell 45, or NGC 5248, is a spiral galaxy located in the constellation Boötes, and it is notable for the ring structure around its nucleus.
Caldwell 45, or NGC 5248, is a spiral galaxy located in the constellation Boötes, and it is notable for the ring structure around its nucleus. NASA, ESA, J. Lee (California Institute of Technology), and A. Filippenko (University of California – Berkeley); Processing: Gladys Kober (NASA/Catholic University of America)
This Hubble image captures Caldwell 78 (or NGC 6541), a globular star cluster roughly 22,000 light-years from Earth. The cluster is bright enough that backyard stargazers in the Southern Hemisphere can easily spot it with binoculars.
This Hubble image captures Caldwell 78 (or NGC 6541), a globular star cluster roughly 22,000 light-years from Earth. The cluster is bright enough that backyard stargazers in the Southern Hemisphere can easily spot it with binoculars. NASA, ESA, and G. Piotto (Università degli Studi di Padova); Processing: Gladys Kober (NASA/Catholic University of America)

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Georgina Torbet
Georgina is the Digital Trends space writer, covering human space exploration, planetary science, and cosmology. She…
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This image from the NASA/ESA Hubble Space Telescope is a relatively close star-forming region known as IRAS 16562-3959.

A stunning new image from the Hubble Space Telescope shows the birth of a new, massive star at around 30 times the mass of our sun. Nestled with a nearby star-forming region called IRAS 16562-3959, the baby star is located within our galaxy and around 5,900 light-years from Earth.

You can see the sparkle of bright stars throughout the image, with the star-forming region visible as the orange-colored clouds of dust and gas stretching diagonally across the frame. These clouds are where dust and gas clump together to form knots, gradually attracting more dust and gas, growing over time to become protostars.

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When two galaxies collide, the results can be destructive, with one of the galaxies ending up ripped apart, but it can also be constructive too. In the swirling masses of gas and dust pulled around by the gravitational forces of interacting galaxies, there can be bursts of star formation, creating new generations of stars. The Hubble Space Telescope recently captured one such hotbed of star formation in galaxy AM 1054-325, which has been distorted into an unusual shape due to the gravitational tugging of a nearby galaxy.

Galaxy AM 1054-325 has been distorted into an S-shape from a normal pancake-like spiral shape by the gravitational pull of a neighboring galaxy, as seen in this Hubble Space Telescope image. A consequence of this is that newborn clusters of stars form along a stretched-out tidal tail for thousands of light-years, resembling a string of pearls. NASA, ESA, STScI, Jayanne English (University of Manitoba)

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“This would be the first time that we can directly show through an atmospheric detection that these planets with water-rich atmospheres can actually exist around other stars,” said researcher Björn Benneke of the Université de Montréal in a statement. “This is an important step toward determining the prevalence and diversity of atmospheres on rocky planets."

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