Term
What makes a star a star? It's a . . . |
|
Definition
big bag of gas (plasma), with nuclear fusion reactions in the core
|
|
|
Term
the sun is held up against self-gravity by
|
|
Definition
|
|
Term
The chemical composition of the Sun is most similar to that of
|
|
Definition
|
|
Term
|
Definition
Mass m is a form of energy E |
|
|
Term
What kinds of particles fuse in fusion reactions?
|
|
Definition
protons, as well as other atomic nuclei |
|
|
Term
When hydrogen fusion takes place, some of the ____ of the original ____ gets converted to ____.
|
|
Definition
mass, protons, energy (light) |
|
|
Term
The Sun's energy is derived from... |
|
Definition
fusion of hydrogen to helium in its core |
|
|
Term
|
Definition
Dark, relatively cool patches on the Sun where magnetic fields have suppressed heat flow from the interior |
|
|
Term
Most of the brightest stars we see at night appear bright because
|
|
Definition
they are intrinsically very luminous but much further than the closest stars |
|
|
Term
Measuring stellar parallax is important because |
|
Definition
a parallax allows the direct determination of a stellar
distance |
|
|
Term
A nearby star's parallax _angle_ is accurately measured by Earthlings and Jupiterlings. How do their observed parallax angles compare?
|
|
Definition
the Jupiterlings find a larger parallax angle |
|
|
Term
A nearby star's parallax _angle_ is accurately measured by Earthlings and Venusians. How do their observed parallax angles compare?
|
|
Definition
the Earthlings find a larger parallax angle
|
|
|
Term
Binary stars are essential in determining what stellar property?
|
|
Definition
|
|
Term
Stars with cooler surface temperatures than the Sun but are much more luminous (intrinsically) must be
|
|
Definition
|
|
Term
_____ stars provide most of the total mass in stars;
_____ stars provide most of the light from stars.
|
|
Definition
low mass stars....massive and giant |
|
|
Term
The stellar property that is most important in determining
how quickly a star will evolve is a star's |
|
Definition
|
|
Term
When stars burn hydrogen on the main sequence, the fusion reactions occur
|
|
Definition
|
|
Term
Presently, low mass stars burn Hydrogen via the ____ while high mass stars use the _____.
|
|
Definition
proton-proton chain ... CNO cycle
|
|
|
Term
How did the first generation of high mass stars burn hydrogen?
|
|
Definition
|
|
Term
The Sun is about ____ & is about ____ its life on the main sequence
|
|
Definition
5 billion years old, half way through |
|
|
Term
After the nuclear fuel has been used up in the core of a star, the core then _____ and ____.
|
|
Definition
|
|
Term
What element is produced in helium burning?
|
|
Definition
|
|
Term
Hydrogen fusion in stars occurs at _____ helium fusion
|
|
Definition
a much lower temperature than |
|
|
Term
The stellar remnant (corpse) of a star like the Sun is a
white dwarf |
|
Definition
|
|
Term
Supernovae are particularly important to us because
much of the material that the Earth & we humans are made of was expelled from
|
|
Definition
stellar interiors by supernovae |
|
|
Term
Will our Sun ever undergo a white dwarf supernova?
|
|
Definition
no, our Sun is not in a close binary star system
|
|
|
Term
When a star becomes a black hole, where does the star's mass go?
|
|
Definition
the mass compresses to a singularity at the center
|
|
|
Term
What kind of pressure holds up a black hole?
|
|
Definition
|
|
Term
If the Sun were somehow turned into a black hole of the same mass...
|
|
Definition
our orbit would stay the same, safely distant from the black hole |
|
|
Term
If you were inside the event horizon of a black hole and aimed a flashlight outward, away from the center of the black hole, we on the outside would see your light
|
|
Definition
|
|
Term
If you were inside the event horizon of a black hole, could you see out of it?
|
|
Definition
Yes, photons from outside still pass through the event horizon |
|
|
Term
the solar cycle marked by the appeareneand dissaperanse of sunspots is cause by
|
|
Definition
the growth and decay of magnietic fields |
|
|
Term
stars with biggest luminosity Masses
|
|
Definition
|
|
Term
white dwarfs are not on main line sequence and are at |
|
Definition
the bottom A
Giants at top! C |
|
|
Term
|
Definition
huge balls of burning gas that emit light from far away distance |
|
|
Term
what is defining characteristic of stars |
|
Definition
nuclear fusion in the core of star--FUSION |
|
|
Term
how does the sun hold itself up against self-gravity |
|
Definition
|
|
Term
how is the sun structured? what are its atmospheric layers?
|
|
Definition
photoshpere, chromosphere, cornoa |
|
|
Term
what is the chemical composition of the sun and how does it compare to those of the planets? |
|
Definition
hy he +gases - like jovian planets |
|
|
Term
what fusion reaction is teh sun using primarily and where |
|
Definition
nuclear fusion , dense core |
|
|
Term
what was teh solar neutrino "problem" |
|
Definition
a lot on earch seen 1/3 expected- turned into 2 other kinds . we found 3 |
|
|
Term
what are sunspots and why are they relatively dark |
|
Definition
dark spots in photosphere, darker becuase they are cooler. very magnetic |
|
|
Term
what drives teh solar activty cycle |
|
Definition
|
|
Term
how do we determine basic stellar properties such as surface temperature, chemacal composition, luminosity, mass , siz and velocity? |
|
Definition
|
|
Term
how do we measure distances to stars |
|
Definition
|
|
Term
|
Definition
direct determination of steller distance- shift |
|
|
Term
are the britest stars in the night sky just closer to us or far away and unusually luminous |
|
Definition
closer- brigher ( size, distance, luminosity)
farther away- could mean more luminous
Depends? |
|
|
Term
how does suns luminosity compare to other stars |
|
Definition
average star compared to others |
|
|
Term
what does e=mc^2 mean and how is it relevant to the fusion process |
|
Definition
Mass m is form of energy E.
stars create their own energy through fusion |
|
|
Term
why does fusion requre extremely high temperatures and densities |
|
Definition
very small go fast - high temps |
|
|
Term
what kinds of particles fuse in fusion reactions? |
|
Definition
protons, as well as other atomic nuclei hy he carbon |
|
|
Term
how do fusion reactions produce engergy |
|
Definition
join 2 nuclei to single nuclei - release energy |
|
|
Term
where do fusion reactions occur in a star? |
|
Definition
|
|
Term
how do stars fuse hydrogen, helium, carbon, etc? |
|
Definition
hy: proton-proton chain CNO cycle
He: trople alpha (2 step)
cabon: alpaha (capture) |
|
|
Term
|
Definition
cold dense clouds, gravitationally contracting and fragmenting |
|
|
Term
which stars are most numerous, which provide the most mass, which generate the most light |
|
Definition
numerous- more low mass stars than high mass stars
most massive most mass from low mass stars
most lifht most light from high mass and giant stars |
|
|
Term
how old is the sun and when will it start to die |
|
Definition
5 billion and die at 10 billion |
|
|
Term
what stellar property determines how quickley a star evolves and dies? |
|
Definition
|
|
Term
how does the temperature for helium fusion compare to that for hydrogen fusion |
|
Definition
he required more energy bc fusing only 2 He = unstable beryllium |
|
|
Term
where are heavy elements like oxygen, calcium and iron made? |
|
Definition
|
|
Term
how do stars die? what are the threee kinds of stellar corpes?
|
|
Definition
from same way its born , it dies, as nuclear fusion process takes place each atom slams into each other not only producing that energy but the 2 atoms that smah turn into one atom/ heavier/ it turns from Hy to a heavy element. the heavier the more heat is produced to fuse them (elements). depending on the mass of the star it can continue the neculear process all the way to the element that absorbs energy so the nuclear process ends there for majority of the stars. the stars core wil try to fuse iron but fail and stars expand and BOOM = supernovae
luminosity dermines how star dies
1. white dwarf+planetary nebula: many buring stages but short of core Fe - buring
2. neturon star + supernova II : many burning stages, ending with core Fe- buring implosion
3. Black hole: same as 2^. but outer star smothers SN and Fe core grows too massive for NS |
|
|
Term
what happens to a star if it tries to fuse iron in its core? |
|
Definition
iron coreimplosion- neutron state |
|
|
Term
what will the Sun become when it dies? what will most stars end up as? |
|
Definition
white dwarf--> black holes (red giant) |
|
|
Term
how do lifetimes of stars compare to the current age of the universe? |
|
Definition
I DONT KNOW. age of universe ?? |
|
|
Term
how can stars evolution be affected by being in close stellar binary system |
|
Definition
transfer mass to each other
type II single Masses star iron core
collapse---> leaves NS remnant youn stellar pops |
|
|
Term
what kinds of stars blow up in supernovae? what do these explosions leave behind? |
|
Definition
type 1
accrcting WD in binary star system explodes old stellar population
?? idk |
|
|
Term
how does the structure of a star change when it dies? |
|
Definition
|
|
Term
what is a planetary nebula? |
|
Definition
gas cloud puffed out off unstable star
cor shrinks and becomes white dwarf |
|
|
Term
what do Hertzprung-Russell diagrams plot? why are they useful? |
|
Definition
plot steller temp v luminosity
know things about star by knowing temperature |
|
|
Term
what is the physical signifiance of the "main sequence" of a hertzprung-Russell diagram? |
|
Definition
age luminousity distance clolor
"spetroscopiz parallax" |
|
|
Term
what other stellar properties apart from those expliity plotted can be deduced from the diagrams? |
|
Definition
color age distance
spectroscopiz |
|
|
Term
how are the mass and luminosity of main swquence stars related ? |
|
Definition
|
|
Term
what is the relative size of a star which is cooler than the sun but it more luminous? |
|
Definition
|
|
Term
what is the physical signifiance of the "main swquence turnoff" |
|
Definition
tells the age of the most massive star on sequence
*orion - lower left is sirus B |
|
|
Term
what is a white dwarf? how does a white dwarf form |
|
Definition
the stellar remnant of a star like the sun
(corpse)
stopped contracting, stopped fusion reactions- expand to red giant and shrink and die
so small not much light |
|
|
Term
how big in size is white dwarf? whats its maximum mass |
|
Definition
diameter= 1 earth diam
mass <1.4 M sun |
|
|
Term
what is the ultimate fate of an isolatedd white dwarf
|
|
Definition
will cool forever -> black dwarf (none old enough yet) |
|
|
Term
what happens to a WD if its mass is pushed ober its mass limit? |
|
Definition
will explode - core collaspe
neutron stars |
|
|
Term
will our sun ever undergo a white dwarf supernova? |
|
Definition
no our sun is not in a close binary star system
|
|
|
Term
what is a neutron star? how do they form |
|
Definition
remnant of core collapse supernova
most gigantic "atomic nuclei" |
|
|
Term
what kind of pressure holds up a nuetron star? |
|
Definition
Neutron degerency pressure
-not strong force |
|
|
Term
what is the mazimum mass of a neutron star? |
|
Definition
3-3.25 masses 1.472.3 M
??
AHH |
|
|
Term
what happens if you add mass t oa neutron star near its mass limit? |
|
Definition
expands and then blows up into supernova |
|
|
Term
how big in size is a neutron star? |
|
Definition
small city 10 km in diam
very compact |
|
|
Term
how do we detect netron stars?
|
|
Definition
|
|
Term
|
Definition
A celestial object, thought to be a rapidly rotating neutron star, that emits regular pulses of radio waves and other electromagnetic radiation at rates of up to one thousand pulses per second.
--says google |
|
|
Term
what are black holes? what are their basic properties? |
|
Definition
surrounded by even horizon
nothing can escape not even light= black
-collapse star with strong gravity- pull fields that even light cannot escape^. massive gravity |
|
|
Term
|
Definition
dying of giant stars - gravatiy forces matter to crush until singularity(core of bh) is created |
|
|
Term
what holds up a black hole against self gravity |
|
Definition
|
|
Term
what is the even horizon of a black hole? how does its size related to the mass of a black hole? |
|
Definition
"the point of no return" i.e. the point at which the gravitational pull becomes so great as to make escape impossible. Light emitted from beyond the horizon can never reach the observer. any object approaching the horizon from the observer's side appears to slow down and never quite pass through the horizon, with its image becoming more and more redshifted as time elapses.
When people talk about the size of a black hole, they are referring to the size of the event horizon. The more mass the singularity has, the larger the event horizon. |
|
|
Term
when a star becomes a black holewhere doesthe star's mass go? |
|
Definition
mass compresses to a singularity at center core |
|
|
Term
how do we detect black holes? |
|
Definition
how they influence gavity and light
1 star orbiting something invisible
|
|
|
Term
what is the maximum mass of a black hole? |
|
Definition
|
|
Term
what happens to to the appearence of an object as it falls into a black hole? |
|
Definition
blueshifted.. events happen faster bc sense of time is faster |
|
|
Term
can you see out of a black hole |
|
Definition
yes photons from outside pass through event horizon |
|
|
Term
if sun turns into black hole, same mass |
|
Definition
our orbit would stay the same, safely distant from the black hole |
|
|
Term
where are stars with larger diameteres |
|
Definition
|
|
Term
where are stars with shortest life time on main sequence? |
|
Definition
|
|
Term
where do stars have shortest life? |
|
Definition
|
|
Term
|
Definition
|
|
Term
|
Definition
|
|
Term
high maginitude =
low maginitdue = |
|
Definition
|
|
Term
the bigger stars are born the faster they die.
|
|
Definition
|
|
Term
if main sequence is yellow it is older than a blue cluster |
|
Definition
|
|
Term
Neutron stars and black holes have____. (element) |
|
Definition
|
|
Term
orion is in lower left
sirius b white
closest dwarf |
|
Definition
|
|
Term
|
Definition
|
|