[DOC] [TLE] Stars Flashcards | Quizlet [PAR] Supernovas occur when a high-mass star can no longer produce enough energy 
to fight the ... What gases/elements do massive supernova-type stars burn up? .... 
Theoretically when a white dwarf no longer emits heat or light it would become a 
black dwarf. ..... -Do not have any particular shape, look irregular and open. [DOC] [TLE] Neutron Stars and Pulsars | Astronomy 801: Planets, Stars, Galaxies ... [PAR] The next logical question to address is: What remnant is left behind (if any) after 
these ... at the beginning of a Type II supernova explosion, a neutron star is 
created. ... The first white dwarf star to be observed was Sirius B when it was 
resolved and ... do not listen to pulsars, some astronomers have taken light 
curves from a... [DOC] [TLE] Lecture notes - NMSU Astronomy [PAR] The distance between the Earth and the Sun is about 8 light minutes. ... e.g. a 
theory, which explains motion of a comet, should be used for ANY comet. ... They 
do not have a solid surface & consist mainly of hydrogen and helium gas. ...... At 
the end of its lifetime in another 5 billion yrs, the Sun will become a white dwarf 
star. [DOC] [TLE] White Dwarfs/Neutron Stars/Pulsars - Introduction to Astronomy [PAR] This causes white dwarfs to have the odd property that if their mass ... Giant 
Branch, or contract still further to become neutron stars or black holes. Once a ... 
The Universe is not yet old enough for stars of less than 1 MSun to have evolved 
to the white dwarf stage. ... When neither is pointed towards us, we don't see any 
light. [DOC] [TLE] Stars [PAR] Of course, if you were to just look at any star and see that it was brighter than the 
stars ... some look rather reddish, some look yellowish, some look white-blue. ... 
Is a star with a magnitude of 4 really "weaker" or not giving off as much light as .... 
of parsecs and light-years - but we have a long ways to go before we get there. [DOC] [TLE] The End of Everything - Universe Today [PAR] Dec 26, 2015 ... That's a long time, but not long enough to appreciate the future the Universe has 
in store for itself. ... of the Universe and it will become a cold black dwarf star  an 
inert chunk of ... At this point, any light emitted by the galaxy will cease to reach 
us. ... become a red giant and then fade away to a white dwarf. [DOC] [TLE] Chandrasekhar limit - Wikipedia [PAR] The Chandrasekhar limit is the maximum mass of a stable white dwarf star. The 
limit was first .... When this is done, the model radius still decreases with mass, 
but becomes zero .... it will eventually shed enough mass to form a white dwarf 
having mass below the ... Most of this energy is carried away by the emitted 
neutrinos. [DOC] [TLE] Cosmologist claims Universe may not be expanding : Nature News ... [PAR] Jul 16, 2013 ... If an atom were to grow in mass, the photons it emits would ... [DOC] [TLE] Living Stars - SAO/NASA Astrophysics Data System [PAR] Their size changes, the quality of the light they emit changes, and the total energy 
... Faint stars such as the white dwarfs produce hardly any energy per unit ... 
region becomes so depleted that hydrogen burning cannot produce enough ... 
When a star can no longer generate energy by nuclear reactions it must cool 
down. [DOC] [TLE] Stellar Evolution  Cosmic Cycles of Formation - Chandra X-ray ... [PAR] years ago. Since the molecules in these clouds do not emit optical light, but do 
release light at radio ... survive the harsh conditions within stellar formation 
regions to become stars. ..... dwarf does not have enough mass; it is heavier than 
a gas giant ... Because a white dwarf is degenerate, gravity cannot compress it 
any more. [DOC] [TLE] Star Images by Jenna Rattan on Prezi [PAR] Star Images Black Holes Ursa Minor Orion Main Sequence Stars

Question: Logically enough, a white dwarf becomes this type of star when it no longer emits any  light
Answer: Black dwarf