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User: NeutronNorman
Name: Norman Anthony Aguero
Currently a student at FIU. My major is chemistry and my minor is physics. My goal is to hopefully earn a Ph.D. in physical organic chemistry.

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Saturday, 15 September 2007

An Expanding Bubble in Space

Bubble Nebula

A star 40 times more massive than our sun is blowing a giant bubble of material into space. In this colorful picture, the Hubble Telescope captured a glimpse of the expanding bubble, dubbed the Bubble Nebula (NGC 7635). The beefy star [lower center] is embedded in the bright blue bubble. The stellar powerhouse is so hot that it is quickly shedding material into space. The dense gas surrounding the star is shaping the castoff material into a bubble. 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 nebula is 6 light-years wide and is expanding at 4 million miles per hour (7 million kilometers per hour). The nebula is 7,100 light-years from Earth in the constellation Cassiopeia.

Image Credit: NASA, Donald Walter (South Carolina State University), Paul Scowen and Brian Moore (Arizona State University)


+ Full Resolution (500 Kb)

Posted by: NeutronNorman at 09:32 | link | comments (2)


Comments:
#1  17 September 2007 - 20:56
 
Wonderful post and picture. I have a quick question. We all know that the sun is a star, but like all other starts will it eventually explode or will it just stay like that forever?
User: mgrhetos2 Contact me View user's mediablog mgrhetos2
#2  18 September 2007 - 04:51
 
The Sun does not have enough mass to explode as a supernova. Instead, in 4–5 billion years, it will enter a red giant phase, its outer layers expanding as the hydrogen fuel in the core is consumed and the core contracts and heats up. Helium fusion will begin when the core temperature reaches around 100 MK, and will produce carbon and oxygen, entering the asymptotic giant branch of a planetary nebula phase in about 7.8 billion years, during which instabilities in interior temperature lead the surface of the sun to shed mass. While it is likely that the expansion of the outer layers of the Sun will reach the current position of Earth's orbit, recent research suggests that mass lost from the Sun earlier in its red giant phase will cause the Earth's orbit to move further out, preventing it from being engulfed. However, Earth's water will be boiled away and most of its atmosphere will escape into space. The increase in solar temperatures over this period is sufficient that by about 500-700 million years into the future, the surface of the Earth will become too hot for the survival of life as we know it.

Following the red giant phase, intense thermal pulsations will cause the Sun to throw off its outer layers, forming a planetary nebula. The only object that will remain after the outer layers are ejected is the extremely hot stellar core, which will slowly cool and fade as a white dwarf over many billions of years. This stellar evolution scenario is typical of low- to medium-mass stars.

Norman
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