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NGC 6357

Diffuse nebula
synonym M17 (M17) Generally refers to NGC 6357
NGC six thousand three hundred and fifty-seven ( Provisional Astronomical Number Sh2-11 RCW one hundred and thirty-one Gum 66 )Is a Diffuse nebula this Nebula Contains a Open cluster Pismis 24, It's a few big ones fixed star Home of.
NGC6357 is located near the constellation Scorpius about 8000 light years away from the Earth. Because it looks like a powerful lobster in the visible image, it has earned the nickname of "lobster nebula". NGC6357 is full of gas clouds and tendril black dust. These clouds are breeding stars, including hot stars with dazzling blue and white light. [1]
Chinese name
War and Peace Nebula
Foreign name
NGC 6357
Alias
Sh2-11,GUM 66,RCW 131, Lobster Nebula
Classification
Diffuse nebula
Right ascension
17:26
Declination
-34°12′
Distance from ground
About 8000 light years
Constellations
scorpio
Brightest star
HD 319718

Basic Introduction

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NGC6357
NGC6357 is located near the constellation Scorpius about 8000 light years away from the Earth. It is called the "Lobster Nebula" because it looks like a powerful lobster in the visible light image. In 2013, the VISTA Infrared Survey Telescope of the European Southern Observatory captured the spectacular scene of hot gas clouds and tendril like dust surrounding hot young stars. The infrared image shows the surprising side of NGC6357. [1]

Related Overview

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NGC 6357
Because of the appearance of this nebula, scientists of space relay infrared experiment call it War and Peace Nebula ( War and Peace Nebula )。 They said that in the infrared image, the bright west side looks like a dove, while the east side looks like a skull. This nebula contains many Protostar , including one Open cluster Pismis 24, And young stars surrounded by expanding cocoons.

scientific research

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There is a bright young star named Pismis 24-1 in NGC6357 nebula. Previously, astronomers thought it was the largest known star. Later, astronomers found that this star was actually composed of at least three big stars. Although the mass of each star is less than 100 times the mass of our sun, these stars are still heavyweight. NASA/ESA Hubble Space Telescope and the European Southern Observatory's Very Large Telescope have also captured some images of NGC6357 nebula. But these two telescopes produce visible light images, which are strikingly different from the new infrared images. [1]
Open cluster
Pismis 24
Pismis 24 , an open star cluster. The brightest star in this cluster is Pismis 24-1 , until it was found that each one had a mass of more than 100 solar masses Conjoint star Previously, it was thought that the mass was about 300 solar masses, possibly one of the most massive stars recorded.
Pismis 24-1 (i.e HD 319718 ), Yes Diffuse nebula NGC 6357 Open cluster Part of Pismis 24, 8150 from Earth Light year , the most massive and brightest star in Pismis 24, and also the brightest star known fixed star one of.
G353.2+0.7
Young star cluster G353.2+0.7 , located to the east of Pismis 24, and passing through Chandra X-ray (Chandra X-ray) image was found to have about 800 stars.
G353.1+0.36
Young star cluster G353.1+0.36 , located in the southeast of Pismis 24, through X-ray Tests show that it contains about 800 stars. The area includes several O star , including [BDSB2003] 10

Observation parameters

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NGC 6357 Yes Galaxy One of the most prominent places for the formation of massive stars nearby. Various early O star Located in this nebula Molecular cloud It can be seen that it is surrounded by bubbles cluster
The most obvious star in Pismis 24