Wednesday , January 27 2021

01/22/2019 – It spreads photos of one star's "last breath"

The Very Large Telescope (VLT) has been captured & # 39; Predictive & # 39; Glow For over 10,000 years, an overview of the eye in astronomical terms, that planet Nebula & # 39; Eso 577-24 & # 39; Arises from

Planetary Nebula & # 39; ESO 577-24 & # 39; It is the result of fossils A dead large star that has erased its outer layersLeaving behind a very hot little star. This fossil will slowly flutter and cool down and its days will be finished just like a ghost as a fairly red vicious star.

The red giants are the stars in the final stages of their lives that have broken hydrogen fuel into their nuclear reactors and They started contracting Under the stupidity of gravity force. As a red giant contract, excessive pressure stimulates the origin of the star, and throws its outer layers into outer form in the form of powerful star winds.

The incandescent part of the dead chunks releases ultraviolet radiation, which is intensified to make these extruded layers ionic and Let them shine. The result is the planet's nebula, or the final final testimony of the old star at the end of his life. His last breath

The Very Large Telescope (VLT) Captures the Globe of Planets' Nebula's EOS 577-24. (AFP)

The Very Large Telescope (VLT) Captures the Globe of Planets' Nebula's EOS 577-24. (AFP)

This brilliant planetary nebula was found in the National Geographic Society-Palomar Observatory Sky Survey in the 1950s, and in 1966 the planetary nebulae's Abel catalog was recorded.

About 1,400 light years from the earth, the haunted glow & # 39; ESA 577-24 & # 39; It is visible only through a powerful telescope. As the dwarf star cools down, the Nebula will continue to expand in space, until it disappears, it will disappear.

& # 39; ESO 577-24 & # 39; This image was created as part of the program EOS Cosmic Jewels, An initiative that uses the ISI telescope to make images of interesting, confusing or visually appealing items with educational and informative purpose, however, the information received is provided to astronomers by the observatory scientific archives.

Source: DPA

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