Exam 3 Flashcards
(74 cards)
The speed of light is about
3x10^5 km/sec
How many layers of the sun are there
There are six
- Corona
- Radiative
- Photosphere
- Convective
- Chromosphere
- Inner core
What is the corona
It is the sun ray part of the sun
“Crown of the sun”
What is the Radiative zone
Bad energy from the sun (Gamma Ray, X Ray)
What is the Photosphere
It is the visible part of the sun
What is the convective part of the sun
It is where the hot and cool gas moves in a cycle in the sun
What is the chromosphere
Color of the sun
What is the inner core
It is where hydrogen turns into helium in fusion
All main sequence stars have this
What spectral type is the sun
G2
What causes the photosphere of our sun to look granulated
Convection to the surface result in a 100k temperature difference b/w light and dark regions
What is the surface temperature of the sun
5800 K
The outer layer of the Suns atmosphere, which can be most easily seen during total solar eclipses, is known as the
Corona
How does the sun produce energy to warm the earth
Fusion of hydrogen to helium in the core of the sun
No fusion no energy
What is solar wind
Charged particles from the sun
Sunspots why are they dark colored
They are cooler temperature from the others parts of the sun
Energy moves through the suns interior —
Convection
What is the main process involved in the sunspot cycle
All due to the magnetic field of the sun
The winding of magnetic field lines due to variations in the suns rotation
The solar cycle from minimum is —
11, 22
Solar cycle from max to max is 11 years
What is process take place in the core of our sun that produces it energy
Nuclear fusion of H to He
Considering parallax angle what do you need to know
D=1/p
Parallax angle is measured in arcseconds
Distance is always in parsecs
What is hydrostatic equilibrium
It is the purpose of why stars are round
Gravity pushes inward
Thermal pressure pushes outward
Until run out of certain element
Parallax is what
Displacement of an object depending how far or close it is
Closer = more displacement Further = less displacement
Considered output vs wavelength graphs
Taller the graph = larger
Smaller the graph =smaller
Peak closer to the left = blue and hot
Peak closer to the right = red and cool
Blue always hotter
Red always bigger
Most of the stars in our galaxies are —
Main sequence stars