The James Webb Space Telescope (JWST) captured a new image of the star-forming nebula N79. The image was taken by the telescope’s Mid-InfraRed Instrument (MIRI) and shows a massive star-forming complex that spans about 1,630 light-years. N79 is located in the Large Magellanic Cloud, a satellite galaxy.

The JWST’s MIRI has a camera and spectrograph that can see light in the mid-infrared region of the electromagnetic spectrum. This region has wavelengths that are longer than what the human eye can see.

The James Webb Space Telescope took this stunning image of a star-forming nebula called N79, which is a region of ionised interstellar atomic hydrogen. The nebula is in the H II region of the Large Magellanic Cloud, a satellite galaxy of the Milky Way, and was captured by Webb’s Mid-Infrared Instrument (MIRI).

N79 is simply a humongous star-forming celestial region that spans around 1,630 light-years and is in the southwest region of LMC (Large Magellanic Cloud). It is regarded as the younger version of the Tarantula Nebula (officially known as 30 Doradus). However, scientists estimate that N79 has a star formation efficiency that far exceeds the Tarantula Nebula

The six largest “star spikes” that you can see in the image are caused by the hexagonal symmetry of the Webb telescope’s 18 primary mirror segments. These sorts of patterns are usually most visible around very bright and compact objects where a lot of light comes from the same place. Even though most galaxies appear very small to our eyes, they are much more spread out than a single star and thus do not cause this pattern.

The orange, yellow and blue image from the powerful space telescope features the interstellar atomic hydrogen of the 1,630-light-year-wide nebula N79, located in the Large Magellanic Cloud, a satellite galaxy of the Milky Way. This region is actively forming stars and remains virtually unexplored by astronomers

N79 is a star-forming nebula located in the Large Magellanic Cloud (LMC), one of the closest galaxies to our own. It’s a region of ionized atomic hydrogen that’s about 160,000 light-years away from Earth

N79 is a younger, less evolved, and more compact version of the Tarantula Nebula, also known as 30 Doradus. Both nebulae are producing stars at a rate that hasn’t been seen in our galaxy for billions of years. However, N79 is twice as efficient at star formation as 30 Doradus. 

The James Webb Space Telescope (JWST) captured a stunning image of N79 using its Mid-Infrared Instrument (MIRI). The image shows a bright young star and the nebula’s glowing clouds of dust and gas. MIRI can reveal details and structures that are hidden in optical images taken by other telescopes

Nebulae are clouds of gas and dust that provide the raw materials for star formation. Gravity causes the gas and dust to come together, forming a dense core. As the core collapses, it heats up and eventually ignites nuclear fusion, becoming a star

Some nebulae are called “star nurseries” because they are regions where new stars are beginning to form. For example, the Eagle Nebula contains three thick columns of dust and gas known as the Pillars of Creation, where stars are forming. 

Some other types of nebulae are the remnants of supernovae, stars exploding at the end of their regular starry lives

Nebulae are called “stellar nurseries” because the gas and dust in them condense to form new stars. The word “nebula” comes from the Latin word nebula, which means “mist, vapor, fog, smoke, exhalation

Nebulae play a key role in the life cycle of stars, both at their birth and death. They are remnants of dead stars that drift through space. Stars are born in dense clumps of gas, dust, and other material inside diffuse emission nebulae. 

The Orion Nebula is an example of a stellar nursery. It’s an enormous cloud of gas and dust many light-years across. Turbulence from deep within these clouds creates high density regions called knots. These knots contain sufficient mass that the gas and dust can begin to collapse from gravitational attraction

All stars are formed from collapsing clouds of gas and dust, often called nebulae or molecular clouds. Over the course of millions of years, these protostars settle down into a state of equilibrium, becoming what is known as a main-sequence star

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