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Hubble Captures Galactic Tug-of-War

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This six-panel illustration of a tidal disruption event around a supermassive black hole shows the following: 1) A supermassive black hole is adrift inside a galaxy, its presence only detectable by gravitational lensing; 2) A wayward star gets swept up in the black hole's intense gravitational pull; 3) The star is stretched or "spaghettified" by gravitational tidal effects; 4) The star's remnants form a disk around the black hole; 5) There is a period of black hole accretion, pouring out radiation across the electromagnetic spectrum, from X-rays to radio wavelengths; and 6) The host galaxy, seen from afar, contains a bright flash of energy that is offset from the galaxy's nucleus, where an even more massive black hole dwells. Credit: NASA, ESA, STScI, Ralf Crawford (STScI)

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Ram Pressure Shapes Star Birth: Hubble Captures Galactic Tug-of-War

by nasaspacenews
March 16, 2024
in News, Others
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Hubble Captures Galactic Tug-of-War
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A captivating image captured by the Hubble Space Telescope reveals LEDA 42160, a dwarf galaxy locked in a cosmic tug-of-war. Located roughly 52 million light-years away within the Virgo galaxy cluster, LEDA 42160 is battling the immense pressure exerted by the surrounding gas. This phenomenon, known as ram pressure, has a dramatic impact on the galaxy’s ability to form stars.

The Stranglehold of Ram Pressure

As LEDA 42160 plows through the dense gas and dust that permeate the Virgo cluster, it encounters immense resistance. This ram pressure can act like a cosmic stranglehold, stripping the galaxy of the raw materials necessary for star formation – gas and dust. Imagine a snowball hurtling through a thick cloud of snow; the faster the snowball moves, the more resistance it encounters. In the case of LEDA 42160, the interstellar medium acts like that dense cloud, and the galaxy is the snowball. This ram pressure can be so intense that it can completely halt the creation of new stars, essentially shutting down the galaxy’s stellar nursery.

However, ram pressure can also have a counterintuitive effect. The immense pressure exerted by the surrounding gas can compress the gas and dust within the galaxy itself. Imagine squeezing a ball of dough; the internal pressure increases as you compress it. In the case of LEDA 42160, this compression can trigger a burst of star formation. The dens gas clouds become more prone to collapse, leading to the birth of new stars. The bright patches observed on the lower-right side of LEDA 42160 might be a testament to this phenomenon, acting as stellar nurseries brimming with newborn stars.

Unveiling the Secrets of Star Formation

This Hubble observation is part of a larger project investigating the impact of ram pressure on dwarf galaxies residing in massive clusters like Virgo. While previous studies suggest ram pressure can trigger star formation in larger galaxies, scientists are now investigating its effect on smaller galaxies like LEDA 42160. Understanding how these forces play out in different galactic environments is crucial for creating a comprehensive picture of star formation across the cosmos.

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By studying LEDA 42160 in detail, astronomers hope to gain a deeper understanding of the complex interplay between ram pressure and star formation. This knowledge will shed light on the processes that govern the birth of stars in galaxies throughout the universe. Imagine a cosmic recipe for star formation; ram pressure adds another crucial ingredient to this recipe, influencing the rate and location of star birth within galaxies.

Hubble’s observations of LEDA 42160 offer a glimpse into the dynamic forces shaping galaxies within dense clusters. The findings will not only improve our understanding of star formation in these extreme environments but also provide valuable insights into the evolution of galaxies within the vast cosmic web. Galaxies like LEDA 42160, locked in a cosmic tug-of-war with the surrounding gas, offer a unique window into the delicate balance between star formation and galactic evolution.

Tags: space discoveryspace exploration

FEATURED POST

Image NASA’s Solar Dynamics Observatory captured this image of the Sun on May 7, 2024

There’s a Violent Solar Storm That Could Have Been Worse—Here’s the Scary Truth

May 11, 2025
This six-panel illustration of a tidal disruption event around a supermassive black hole shows the following: 1) A supermassive black hole is adrift inside a galaxy, its presence only detectable by gravitational lensing; 2) A wayward star gets swept up in the black hole's intense gravitational pull; 3) The star is stretched or "spaghettified" by gravitational tidal effects; 4) The star's remnants form a disk around the black hole; 5) There is a period of black hole accretion, pouring out radiation across the electromagnetic spectrum, from X-rays to radio wavelengths; and 6) The host galaxy, seen from afar, contains a bright flash of energy that is offset from the galaxy's nucleus, where an even more massive black hole dwells. Credit: NASA, ESA, STScI, Ralf Crawford (STScI)

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Image NASA’s Solar Dynamics Observatory captured this image of the Sun on May 7, 2024

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This six-panel illustration of a tidal disruption event around a supermassive black hole shows the following: 1) A supermassive black hole is adrift inside a galaxy, its presence only detectable by gravitational lensing; 2) A wayward star gets swept up in the black hole's intense gravitational pull; 3) The star is stretched or "spaghettified" by gravitational tidal effects; 4) The star's remnants form a disk around the black hole; 5) There is a period of black hole accretion, pouring out radiation across the electromagnetic spectrum, from X-rays to radio wavelengths; and 6) The host galaxy, seen from afar, contains a bright flash of energy that is offset from the galaxy's nucleus, where an even more massive black hole dwells. Credit: NASA, ESA, STScI, Ralf Crawford (STScI)

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