Exam 3 Flashcards
(47 cards)
Photosphere
The surface of a star, where the plasma is thin enough that light can escape freely into space
Corona
A stars upper atmosphere, where thin plasma is heated to millions of Kelvin by the stars magnetic field
Fusion
The process where small nuclei are merged to form a heavier element, which can release energy
Envelope
The interior part of a star where fusion doesn’t occur and where the composition stays the same since the star was formed
Fission
When a heavy unstable nucleus breaks apart to form nuclei of lighter elements, which can release energy
Core
The part of the star where energy is generated
The sun shines because it is
Hot like a stove
Heat is generated in the suns core by
Nuclear fusion of hydrogen into helium
Nuclear ____ involves merging atoms while nuclear ____ involves splitting them
Fusion= merge Fission= split
The sun has been shining for __ years and is..
4.5 billion years; halfway through its life
Sometimes the sun throws a ball of plasma and magnetic field out into the solar system. This is called a
Coronal mass ejection (CME)
What causes sunspots and solar cycles
The suns magnetic field reverses polarity
Fusion powers the core, changes on the surface are c if the magnetic field
There are more sunspots, flares, and CMEs during
The middle of a sunspot cycle
Th corona glows in X-rays while the photosphere only glows in visible light, so we know the corona is ___ than the photosphere
Hotter
The ___ is heated by fusion while the ___ is heated by magnetic fields
Core= fusion Corona= magnetic fields
If you were to dive into the sun, you would hit a solid surface at the..
… actually, the plasma would just get thicker and thicker as you fell in
You can tell the temperature of a star by looking at its
Color
Lost the spectral types from hottest to coolest
OBAFGKM
How would you tell a K type red giant from a K type red dwarf?
The giant is more luminous
True or false: as a star loses mass due to the stellar wind, it goes from being a main sequence O star to being a main sequence G star to finally being a main sequence M star
False; a star lands somewhere on the main sequence depending on its mass, and doesn’t move from there until it leaves the main sequence entirely
On the main sequence compared to low mass stars, high mass stars are hotter
More luminous, and have shorter lifetimes
High mass stars can fuse carbon but the sun cannot because
It’s core is not hot enough
Stars on the main sequence range in luminosity and temperature, but they are all
Fusing hydrogen into helium in their cores
Stars become larger once they leave the main sequence because
They are producing more energy, which makes the surface expand more