Web Results

Planetary nebula - Wikipedia


A planetary nebula, often abbreviated as PN or plural PNe, is a kind of emission nebula ... After most of the red giant's atmosphere is dissipated, the ultraviolet radiation of .... This led to ...

What is a planetary nebula What happens to the core - Course Hero


What is a planetary nebula What happens to the core of a star after a ... Be sure to explain both the changes that occur in the Sun's core with each stage and the ...

Essential Cosmic Perspective Chapter 12 Flashcards | Quizlet


Explain why degeneracy pressure can support a stellar core against gravity even when the ... What happens to the core of a star after a planetary nebula occurs?

Stellar Evolution


What happens to the Earth when the Sun starts to "die"? What is .... When the core temperature reaches 100 million K, it is hot enough for helium fusion to occur. ..... All that is left of the star after the Planetary Nebula stage is the hot little core.

Late stages of evolution for low-mass stars


... for low-mass stars. This movie summarizes the evolution of a star like our Sun after it has reached the main sequence. ... But what happens when they finally use up all the hydrogen in their cores? ... After it occurs, the star settles down to a new phase of helium burning. ... Evolution of the outer envelope: planetary nebulae.

Stage 8: Planetary Nebula or Supernova - Astronomy Notes


Feb 17, 2015 ... Planetary nebulae can be distinguished from H II regions by their compact shape ... When a massive star's iron core implodes, the protons and electrons fuse ... This happens in about the first 15 minutes of the supernova. ... What remains after the outer layers are thrown off depends on the mass of the core.

Life Cycles of Stars - UWGB Home


Mar 26, 1998 ... In addition, astronomers can calculate what would happen to stars .... look disk- like in a telescope, they are called planetary nebulae. Some giants are massive enough to start other cycles of nuclear reactions after their helium runs out; ... When helium begins to fuse in the sun's core, the outer gases of the ...

Page 1 @ Helium-burning supergiant: Helium fusion begins when ...


What happens to a low-mass star after it exhausts its core helium? ... after a planetary nebula occurs? because one day the Sun will blow up as a supernova. 9.

Red Giants and White Dwarfs - The Star Garden


After this, the core will become a white dwarf, while the outer layers will form a planetary nebula. ... oxygen fusion to begin, and so this only occurs in stars over about 10 times the mass of the Sun. ... Planetary Nebula: Cat's Eye Nebula. ... This is what's happened to PSR J1719-1438 b, which is known as a diamond planet.



This process occurs soon after star birth and remains active possibly for a million years. ... In stars larger than our sun, the dominant fusion process in the core is called ... layers of the star's atmosphere into space creating a "Planetary Nebula". .... time in the universe for this to happen if the theory of the big b...

More Info

Background: Life Cycles of Stars - Imagine the Universe! - NASA


May 7, 2015 ... As the main sequence star glows, hydrogen in its core is converted into helium by nuclear fusion. ... A planetary nebula is formed by the outer layers. ... However, their life cycles start to differ after the red giant phase. ... What happens between the red giant phase and the supernova explosion is described ...

Stellar Death - University of Oregon


... this mass limit. An example of this is the Cat's Eye Nebula shown below: ... Even higher mass stars will burn neon after carbon is used up. ... Iron can fuse, but it absorbs energy in the process and the core temperature drops. ... This entire process happens so fast that we can only follow it using supercomputer simulations.

The Evolution of Massive Stars and Type II Supernovae | Astronomy ...


Planets, Stars, Galaxies, and the Universe ... The lifecycle of high mass stars diverges from that of low mass stars after the ... At some point, the fusion reactions will create iron in the core of the star, and when this occurs, the star has only minutes to live. ... Figure 6.9: The Tarantula Nebula and supernova 1987a in the LMC.