Using a knife on the NASA/ESA/CSA JAmes Webb, astronomers took new high -resolution images of NGC 6072 planet.
Webb/Nircam NGC 6072, a planetary nebula, appears approximately 4,048 light years in the Scorpio Conservative. Credit Image: NASA / EsA / CSA / STCI.
NGC 6072 It is around it 1,241 Persecs (4,048 light years) Far in the Southern Scorpio Consispace.
Also known as ESO 389-15, HEN 2-148 or Iras 16097-3606, Al-Sadim is 10,000 years old.
It was first find out By British astronomer John Hershel on June 7, 1837.
“Since their discovery in the eighteenth century, astronomers have learned that the planetary demolition, or dandruff from the glowing gas that was expelled by the middle -middle mass star late in his life, could come in all shapes and sizes,” said web astronomers.
“Most of the planetary demolitions are circular, oval, or bipolar, but some delusion of the base, as shown in new web pictures of NGC 6072.”
In the new image of Webb’s Nircam (the camera near infrared), it is easily clear that NGC 6072 is multi -poles.
Astronomers said: “This means that there are many different elliptical flows that come out in both cases of the center.”
“These external flows press the gas towards the tropical plane and the creation of a tablet.”
“This is evidence of the presence of at least two stars in the middle of this scene.”
“Specifically, the accompanying star interacts with an aging star that has already begun to get rid of some of his outer layers of gas and dust.”
“The central area of the planets shed from the heart of the hot star, which is seen as a light blue color in the light close to infrared.”
“The dark orange material, which consists of gas and dust, follows pockets or open areas that appear in dark blue.”
“This formation can be created when dense molecules were formed while protecting from hot radiation from the central star.”
“There can also be the time of playing time. For thousands of years, the interior winds can be keen across the aura from the main star when it started losing the mass for the first time.”
Webb / Miri image shows this planetary nugby NGC 6072. Credit image: NASA / ESA / CSA / STSCI.
The longest wavelengths captured by Web’s Miri (Infrared Midr -Radi Tool) highlights dust, and it reveals that stars astronomers suspect can be central in this scene.
The researchers said: “It seems that a small white pink point in this picture,” the researchers said.
“The web look at the wavelength in the middle of the infrared also reveals the united episodes of the center expanding from the central region, which is the most obvious rotation after the edges of the lobes.”
“This may be additional evidence of a secondary star in the middle of the scene hidden from our view.”
“The secondary star could be bent, as it revolves around the original star, episodes of materials in a spiral style where the main star was to expel the mass during a previous stage of her life.”
“The red areas in the light and blue areas of Miri follow both cold molecular gas (hydrogen molecules) while the central areas follow the hot gas.”