NASA’s Hubble Traces ‘String of Pearls’ Star Clusters in Galaxy Collisions

3 min read NASA’s Hubble Traces ‘String of Pearls’ Star Clusters in Galaxy Collisions 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, seen in this NASA 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. They form when knots of gas gravitationally collapse to create about 1 million newborn stars per cluster. NASA, ESA, STScI,…

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What is Dark Energy? Inside our accelerating, expanding Universe

11 min read What is Dark Energy? Inside our accelerating, expanding Universe Some 13.8 billion years ago, the universe began with a rapid expansion we call the big bang. After this initial expansion, which lasted a fraction of a second, gravity started to slow the universe down. But the cosmos wouldn’t stay this way. Nine billion years after the universe began, its expansion started to speed up, driven by an unknown force that scientists have named dark energy. But what exactly is dark energy? The short answer is: We don’t…

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Hubble Views a Dim but Distinct Galaxy

2 min read Hubble Views a Dim but Distinct Galaxy Both visible and ultraviolet wavelengths of light comprise this Hubble Space Telescope image of the spiral galaxy UGC 11105. ESA/Hubble & NASA, R. J. Foley (UC Santa Cruz) This image of the softly luminous spiral galaxy UGC 11105 is from the NASA/ESA Hubble Space Telescope. It lies about 110 million light-years from Earth in the constellation Hercules. Astronomers have different ways of quantifying how bright celestial objects are. Apparent magnitude is one of those methods. It describes how bright an…

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How do galaxies grow while ensnared in the universe’s cosmic web?

Just like being trapped within a spider’s web drastically changes a fly’s life, galaxies ensnared in the vast cosmic web are dramatically and irreversibly altered. Now, scientists from the University of Kansas are aiming to better understand the mechanisms at play in shaping clusters of galaxies as they travel through a cosmic web of different environments. KU professor of physics and astronomy Gregory Rudnick is leading the effort, which involves recreating the cosmic web in a computer simulation, then studying gas content and star-formation properties of galaxies as they move…

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Hubble Observes a Galactic Distortion

1 min read Hubble Observes a Galactic Distortion The galaxy NGC 5427 shines in this new NASA Hubble Space Telescope image. NASA, ESA, and R. Foley (University of California – Santa Cruz); Processing: Gladys Kober (NASA/Catholic University of America) The galaxy NGC 5427 shines in this new NASA Hubble Space Telescope image. It’s part of the galaxy pair Arp 271, and its companion NGC 5426 is located below this galaxy and outside of this image’s frame. However, the effects of the pair’s gravitational attraction is visible in the galactic distortion…

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Hubble Spies a Spinning Spiral

2 min read Hubble Spies a Spinning Spiral This new NASA Hubble Space Telescope image features the face-on spiral and Seyfert galaxy, ESO 420-G013. NASA/ESA/A. Evans (University of Virginia)/Processing: Gladys Kober (NASA/Catholic University of America) Looking like a baseball lobbed into the depths of the universe, ESO 420-G013 is a face-on spiral galaxy and a Seyfert galaxy. Dark lanes of dust are visible against the background glow of the galaxy’s many stars.  About 10 percent of all the galaxies in the universe are thought to be Seyfert galaxies. They are…

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NASA’s Webb Depicts Staggering Structure in 19 Nearby Spiral Galaxies

6 Min Read NASA’s Webb Depicts Staggering Structure in 19 Nearby Spiral Galaxies Webb’s set of 19 PHANGS images of face-on spiral galaxies. Credits: NASA, ESA, CSA, STScI, Janice Lee (STScI), Thomas Williams (Oxford), and the PHANGS team It’s oh-so-easy to be absolutely mesmerized by these spiral galaxies. Follow their clearly defined arms, which are brimming with stars, to their centers, where there may be old star clusters and – sometimes – active supermassive black holes. Only NASA’s James Webb Space Telescope can deliver highly detailed scenes of nearby galaxies…

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Hubble Studies a Sparkling Galaxy Pair

1 min read Hubble Studies a Sparkling Galaxy Pair This new NASA Hubble Space Telescope image features a pair of interacting galaxies called, NGC 5410 and UGC 8932/PGC 49896. NASA/ESA/D. Bowen (Princeton University)/Processing: Gladys Kober (NASA/Catholic University of America) A pair of small, interacting galaxies shine in this new NASA Hubble Space Telescope image. The larger of the two galaxies is named NGC 5410 and was discovered in 1787 by British astronomer William Herschel. It spans 80,000 light-years across and has a bright white bar of stars at its center.…

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Hubble Glimpses a Bright Galaxy Group

2 min read Hubble Glimpses a Bright Galaxy Group This new NASA Hubble Space Telescope image shows a tangled group of interacting galaxies called LEDA 60847. NASA/ESA/A. Barth (University of California – Irvine)/M. Koss (Eureka Scientific Inc.)/A. Robinson (Rochester Institute of Technology)/Processing: Gladys Kober (NASA/Catholic University of America) This new NASA Hubble Space Telescope image shows a group of interacting galaxies known as LEDA 60847. LEDA 60847 is classified as an active galactic nuclei, or AGN. An AGN has a supermassive black hole in the galaxy’s central region that is…

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Hubble Observes an Askew Galaxy Coaxing Star Formation from its Partner 

2 min read Hubble Observes an Askew Galaxy Coaxing Star Formation from its Partner  This new NASA Hubble Space Telescope image features two interacting spiral galaxies collectively called Arp 300. NASA, ESA, J. Dalcanton (University of Washington), and R. Windhorst (Arizona State University); Processing: Gladys Kober (NASA/Catholic University of America) Arp 300 consists of two interacting galaxies, UGC 05028 (the smaller face-on spiral galaxy) and UGC 05029 (the larger face-on spiral). Likely due to its gravitational dance with its larger partner, UGC 05028 has an asymmetric, irregular structure, which is…

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