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Monster Star Hidden In The Bubble Nebula

11 April, 2012

MessageToEagle.com - A hot, powerful 0-type star 45 times more massive and several 100,000 times more luminous than the Sun is located near the center of this impressive bubble known as "Bubble Nebula".

The stellar powerhouse is so hot that it is quickly shedding material into space.

Despite its apparently spherical shape, it seems not to have the characteristics of either a planetary nebula or a supernova remnant.

This remarkable giant "Bubble" is expanding. The Bubble Nebula (also known as NGC 7635), is a mere 10 light-years wide.

It marks the boundary between an intense wind of particles from the star and the more quiescent interior of the nebula.

The central star of the nebula is responsible for a stellar wind moving at 2,000 kilometers per second (4 million miles per hour or 7 million kilometers per hour) which propels particles off the surface of the star.

The bubble surface actually marks the leading edge of this wind's gust front, which is slowing as it plows into the denser surrounding material.

The surface of the bubble is not uniform because as the shell expands outward it encounters regions of the cold gas, which are of different density and therefore arrest the expansion by differing amounts, resulting in the rippled appearance.



Click on image to enlarge

NGC 7635: The Bubble Nebula

Blown by the wind from a massive star, this interstellar apparition has a surprisingly familiar shape. Cataloged as NGC 7635, it is also known simply as The Bubble Nebula. This colorful telescopic image includes a long exposure through a hydrogen alpha filter to reveal details of the cosmic bubble and its environment. Although it looks delicate, the 10 light-year diameter bubble offers evidence of violent processes at work. A fierce stellar wind and intense radiation from that star has blasted out the structure of glowing gas against denser material in a surrounding molecular cloud. The intriguing Bubble Nebula lies a mere 11,000 light-years away toward the boastful constellation Cassiopeia. Credit & Copyright: Kent Wood


It is this gradient of background material that the wind is encountering that places the central star off center in the bubble.

There is more material to the northeast of the nebula than to the southwest, so that the wind progresses less in that direction, offsetting the central star from the geometric center of the bubble.

At a distance of 7,100 light-years from Earth, the Bubble Nebula is located in the constellation Cassiopeia and has a diameter of 6 light-years.



Click on image to enlarge

NGC 7635: The Bubble Nebula

It's the bubble versus the cloud. NGC 7635, the Bubble Nebula, is being pushed out by the stellar wind of massive central star BD+602522. Next door, though, lives a giant molecular cloud, visible to the right. At this place in space, an irresistible force meets an immovable object in an interesting way. The cloud is able to contain the expansion of the bubble gas, but gets blasted by the hot radiation from the bubble's central star. The radiation heats up dense regions of the molecular cloud causing it to glow. The Bubble Nebula, pictured above in scientifically mapped colors to bring up contrast, is about 10 light-years across and part of a much larger complex of stars and shells. Image Credit & Copyright: Larry Van Vleet


The "clouds" are a ridge of much denser gas. The lower left portion of this ridge is the brightest because it is closest to the star.

But the star's intense ultraviolet light and its strong "wind" of material is heating and eroding this area the fastest. The region between the star and the ridge reveals several loops and arcs that have never been seen before.

Astronomers are uncertain about the origin of this "bubble-within-a-bubble." It may be due to a collision of two distinct winds of material. The star's intense wind may be colliding with material streaming off the ridge of gas, which the star's intense radiation is heating and eroding.

The bubble's surface is not smooth like a soap bubble's. Its rippled appearance is due to encounters with gases of different thickness.
The Bubble Nebula can be seen with a small telescope towards the constellation of the Queen of Aethiopia (Cassiopeia).

MessageToEagle.com via NASA

See also:
Intimate Connection Between Black Holes And New-Born Stars

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