Astronomers Discover an Extremely Unusual Galaxy

Sitting in the arms of Cassiopeia (The Seated Queen) 

This image, taken by the NASA/ESA Hubble Space Telescope’s Wide Field Planetary Camera 2, shows a spiral galaxy named NGC 278. This cosmic beauty lies some 38 million light-years away in the northern constellation of Cassiopeia (The Seated Queen). Credits: NASA/Hubble/ESA

Space news (galaxy evolution: unusual galaxies; spiral galaxy NGC 278) – 38 million light-years away, sitting in the arms of northern constellation Cassiopeia (The Seated Queen) – 

The image above shows spiral galaxy NGC 278, a very unusual island universe astronomers are currently studying looking for clues to its unique nature. This unusual galaxy looks quiet and serene from here, but there’s unusual starburst activity taking place astronomers are currently trying to explain.  

Each of the unmistakable blue knots seen strewn across NGC 278’s spiral arms is a clump of hot, newly born stars. These blue knots of young stars doesn’t extend to the outer edges of the galaxy but only reside within an inner ring some 6,500 light-years across. The two-tiered structure astronomers have identified within NGC 278 shows a bright galactic center, with much darker outer regions. 

Astrophysicists studying this unusual spiral galaxy think this weird two-tiered structure and current starburst activity is due to a recent merger with a smaller, gas-rich galaxy. A merger that has ignited starburst within the center of this island universe, while the leftovers of the galactic snack dispersed into its outer regions. This activity created the ring of blue knots of newly formed stars seen here, which astronomers have dubbed a nuclear ring. A very unusual structure not often observed in galaxies with a bar across their center region. Making NGC 278 an unusual, intriguing galactic specimen they plan on studying closer for clues to its unusual nature. 

Learn more about why simple elliptical galaxy UGC 1382 astonishes astronomers?

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Learn about the things NASA has discovered during the human journey to the beginning of space and time here.  

Read and learn more about galaxies. 

Discover everything they know about spiral galaxy NGC 278 here. 

Learn more about the northern constellation Cassiopeia (The Seated Queen). 

Read, learn and discover more about starburst galaxies here. 

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Barred Spiral Galaxy NGC 4394

One of the most common types of island universes viewed during our journey

Space news (The Hubble Tuning Fork: barred spiral galaxies) – 55 million light-years from Earth toward the constellation of Coma Berenices (Berenice’s Hair) –

These arms are peppered with young blue stars, dark filaments of cosmic dust, and bright, fuzzy regions of active star formation. At the centre of NGC 4394 lies a region of ionised gas known as a LINER. LINERs are active regions that display a characteristic set of emission lines in their spectra

First documented in the western world by German-British astronomer William Herschel, barred spiral galaxy NGC 4394 is a member of the most common type of galaxy viewed in the Galaxy Zoo. Estimated by astronomers to be 55 million light-years from Sol, toward the constellation of Coma Berenices, this island universe is considered a member of the Virgo Cluster. 

The prototypical barred spiral galaxy, NGC 4394 has bright spiral arms sprouting from the ends of a bar cutting through its middle bulge. Sprinkled with blue, young stars its spiral arms contain fuzzy regions where stars are being formed and dark filaments of cosmic dust. Near the center of this island universe lies a region of ionized gas known as a low-ionization nuclear emission-line region (LINER). An active region displaying a specific set of emission lines in its spectra, a LINER contains mainly weakly ionized atoms of oxygen, nitrogen, and sulfur.

LINERS have been viewed relatively often during the human journey to the beginning of space and time and they’re starting to piece together their puzzle. Astronomers still need to figure out where the energy comes from to ionize the gas. Presently astronomers believe it could be due to the influence of the supermassive black hole or extreme levels of star formation. In the case of NGC 4394, gas from a nearby galaxy has likely flowed into its central region, providing a new source to fuel the process, either way.

You can learn more about galaxies with a LINER here.

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Learn more about the Hubble Tuning Fork here.

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Read more about barred spiral galaxies here.

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