The latest image of “Ratil Nebula” was released

According to RCO News Agency, The Hubble Space Telescope is still working for more than five years, observing the universe and sending different images to us to surprise us.

NASA and the European Space Agency have now released an image taken by Hubble from Tarantula Nebula, the official name “Doradus” in a large Magellani cloud, displaying a spectacular cosmic view.

According to NASA, the “Ratil Nebula” is the largest and most radical area of ​​the star around us, with stars in the center of which have a mass mass of the sun.

“The Retill Nebula” is a famous nebula in the constellation of “Golden Fish” in the Great Magellani Galaxy. Initially, it was thought to be a star, until it was discovered by Nicolas-Lawi in the year 2.

This nebula is the brightest non -starring mass ever discovered, and it is so brilliant that if the Nebula was in the Milky Way, it could have shadowed on earth. In fact, the Ratil Nebula is the most active area of ​​the birth of stars in our local galactic group.

This Hubble view gives us a look at the suburbs of this nebula and reveals layers of colorful gases and stars.

The Retill Nebula is located in a large Magellani cloud next to a dwarf galaxy. This nebula is known for its sophisticated structure and network that resembles spider web.

While in the final photo we see that the image is full of brilliant colors, Hubble images are initially captured and received in the gray spectrum. As NASA explains, scientists can create a combined color image using different color filters on the telescope, with the wavelength of the filter, along with a combination of images.

The new image of the Retill Nebula not only shows visible light, but also shows the ultraviolet and infrared spectrum. In such a case, colors are related to the wavelengths that we usually can’t see.

Astronomers describe this image: Stars that are in the background or between the dusty clouds of this image, because of the exposure properties, appear to be reduced than stars without dust cover. This discoloration occurs because cosmic dust absorbs and disperses blue light. So more red light reaches the telescopes. This makes the stars look red than their actual state.

The study of nebulae such as the “Ratil Nebula” in a large Magellani cloud or other galaxies allows scientists to better understand the role of cosmic dust in the formation of new stars and planets. Hubble data is a valuable tool for these studies and helps researchers to better understand these particles and examine their consequences on cosmic processes.

This is not the first time the Hubble Space Telescope has been photographing the Retill Nebula. In the past, Hubble has also recorded attractive images of the area. The latest images previously taken by Hubble are from year 1 and 2, but what made the Nebula a reputation was an image released by the James Webm Space Telescope in Year 2. This image was one of the first goals of the space telescope and was able to showcase important information on the “Ratil Nebula”.

The formation of stars is a complex and energetic process. When dust and gas is compressed in an area of ​​space, gravity gradually pulls these materials and forms masses. These masses, known as Protostars, are the cores of newborn stars. These young stars release a lot of energy and, because of their high radiation, look much brighter than older stars like the sun.

Researchers still disagree on the rate of stars in the Milky Way, but what is generally accepted is that the Milky Way produces more stars than the Andromeda Galaxy. However, the large Magellanon cloud has a high star formation rate despite being smaller than both galaxies. This feature, in addition to its proximity to our galaxy, has made the galaxy a wonderful natural laboratory to study starring processes.

Hubble and James Web telescopes have powerful tools to study this small but energetic galaxy. These telescopes provide more detailed details of the process of stars formation, interactions between cosmic dust, the light of stars, as well as the role of gases in creating these cosmic structures. With this information, scientists can create better simulated models to understand how stars and planetary poems are formed around the world.

Retill Nebula is recognized as one of the key areas for studying these processes. Not only because of its beautiful and complex structure, but also because of its valuable scientific information, it attracted a lot of astronomers. Careful shooting of space telescopes from the area helps scientists to better understand not only the “Retail Nebula” but also other similar areas in other galaxies.

So further studies on this nebula and other similar areas can help us to have a deeper understanding of the formation of stars and the evolution of galaxies and better understand our place in this great world.

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