VLT Survey Telescope Observes Messier 18
News Staff, Science News | Aug, 10, 2016
ESO’s VLT Survey Telescope at Paranal Observatory, Chile, has captured a new image of the star cluster Messier 18, also known as NGC 6613 and M18.
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Messier 18 (upper left) and its surroundings. This image was captured by the OmegaCAM, a camera installed on the VLT Survey Telescope. Image credit: ESO.[/TD]
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Messier 18 is an open star cluster located in the constellation Sagittarius.News Staff, Science News | Aug, 10, 2016
ESO’s VLT Survey Telescope at Paranal Observatory, Chile, has captured a new image of the star cluster Messier 18, also known as NGC 6613 and M18.
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It spans about 18 light-years across and is at a distance of 4,230 light-years from Earth.
It was discovered in 1764 by the French astronomer Charles Messier during his search for comet-like objects.
There are over 1,000 known open clusters within our Milky Way Galaxy, with a wide range of properties, such as size and age, that provide astronomers with clues to how stars form, evolve and die.
The main appeal of these clusters is that all of their stars are born together out of the same material.
In Messier 18 the blue and white colors of the stellar population indicate that the cluster’s stars are very young, probably around 30 million years old.
Being siblings means that any differences between the stars will only be due to their masses, and not their distance from Earth or the composition of the material they formed from. This makes clusters very useful in refining theories of star formation and evolution.
Scientists now know that most stars do form in groups, forged from the same cloud of gas that collapsed in on itself due to the attractive force of gravity.
The cloud of leftover gas and dust that envelops the new stars is often blown away by their strong stellar winds, weakening the gravitational shackles that bind them.
Over time, loosely bound stellar siblings like those pictured here will often go their separate ways as interactions with other neighboring stars or massive gas clouds nudge, or pull, the stars apart.
Our Sun was most likely once part of a cluster very much like Messier 18 until its companions were gradually distributed across the Milky Way.
The dark lanes that snake through this image are murky filaments of cosmic dust, blocking out the light from distant stars.
The contrasting faint reddish clouds that seem to weave between the stars are composed of ionized hydrogen gas.
The gas glows because young, extremely hot stars like these are emitting intense UV light which strips the surrounding gas of its electrons and causes it to emit the faint glow seen in this image.
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Globular clusters are different. The stars in globular clusters are held together by gravity and do not wander away as do stars in open clusters. - Ilan
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