Chapter 20 Cosmology Flashcards
Why are the three astronomical units of distance in increasing orders
Define the AU and the light year
1) the AU
- this is the average distance from centre of earth to centre of sun
2) Light year
- distance light can travel in one year (in a vacuum)
3) parsec
Before defining the parsec must define small units of angle
What is the arc minute and ar second
SO HOW MANY ARCSECONDS IN A DEGREE
There are 60 arc minute in 1° and 60 arc seconds in 1 arc minute
Therefore in 1 ° = 3600 arc seconds
1 arc second = 1°/3600
So what is a parsec definition
The distance made when a radius of 1 Au subtended an angle 1 arc second
So basically triangle with AU opposite, 1 parsec adjacent and theta being 1 arc second
The parsec forms 90° with the sun and the earth au
How ti find exact distance of parsec
If angle is 1 arc second, tan arc sec = 1AU/ 1 Parsec
Rearrange to find distance
What can we say about the angle subtended if the distance away from the sun increases in parsecs
As tan theta = theta when theta is SMALL
A distance of 1 parsec gives the formula tan (1 arcsecond) = 1AU/ 1 parsec
- thus 1 arcsecond = 1 au / 1 parsec using small angle
So if we increase 1 parsec to 2, the equation corrects when the angle is now 1/2 arcsecond etc
So the relationship is theta is inversely propritnsk to distance in parsecs
So in summary, What is relationship using small angle approx again for angle subtended and distance In parsecs
!!!
Theta in arcsecond = 1/d in parsec
What is the technique stellar parallax used for ( short answer)
Used to determine the DISTANCE of stars relatively close to the earth
What does the parallax part in the stellar parallax mean?
Why do the background stars not apparently shift ?
Parallax is the APPARENT shift in the position of a star when compared to BACKGROUND STARS, as the earth ORBITS THE Sun
This is because the background stars further back are through to be constant
So explain how we can use stellar parallax to work distance
Well, when earth at summer, looking at nearby star agsisnt backdrop will postion it somewhere
- 6 month later when earth is in anti part of the orbit in winter, looking at same star against backdrop will place it somewhere else against the fixed backdrop
(This is just an illusion)
- using clear measurements, the PARALLAX ANGLE can be determined . Once we have this, we use precious formula of angle =1/d to d = 1/angle to find distance in parsecs star is from the SUN
What is parallax angle then?
This is the angle that the planet subtends 1 AU from the sun , with a specific distance away from the sun which is in PARSECS
Finally summarise the equations for parallax, what’s all we need to find the distance it is away from sun
Just parallax angle, then do d = 1/p for distance in parsecs it is from the sun
Why can’t parallax be used for far stars?
Apparent shift isn’t so apparent anymore as the further away you look the less it shifts
What is the basic idea of the Doppler effect with sound waves and an ambulance AMBULANCE COMING TOWARDS YOU
Basically, when someone in an ambulance and moves, hears constsnt frequency
But when the ambulance moves TOWARDS a stationary observer, as the source emits waves, it CATCHES UP TO THESE WAVES BASED ON ITS SPEED, and so by the time these waves reach observer, he’s hearing MORE waves per second than he should, and so waves are MORE COMPRESSED, and more waves per second = frequency INCREASES.
- thus as observed comes close to you, frequency appears to shift HIGHER, and so neeeee pitch is heard
What about Doppler effect when ambulance passes you and moves AWAY?
As it moves away, it moves AWAY from waves produced, so the distance between waves coming to you INCREASED, wavelength increases, and as less waves reaching you per second, frequency decreases
So lower pitch heard as it moves away from you
What’s a good summary definition of the Doppler effec then
The apparent shift in OBSERVED frequency/ wavelength CAUSED BY the relative motion between a source and an observer
Is Doppler effect only for sound?
No, all wave related
Okay so how does Doppler effect work for LIGHT COMING FROM STARS?
If we look at the ABSORBTION SPECTRA of an element found in earth, and in a star, then if the position of the absorption lines are different, then it MUST BE DUE TO THE RELATIVE MOTION BETWEEN STAR AND EARTH
So if all the lines have moved towards one end of spectrum or other, we can tell if the star is thus moving closer or AWAY FROM US
Okay so what way are all the spectrum lines shifted if it’s moving away or towards us?
The star moving away from us, (assuming we are stationary) that means light we see will be of longer wavelength DUE to Doppler effect and the relative motion between the star and the earth , and so towards red spectrum thus RED SHIFT,
If light we see is towards blue spectrum, then IT MEANS MOVING TOWARDS US, light we see is of higher frequencies due to Doppler effect, and so star is moving towards us = BLUE SHIFT
What is the DOPPLER SHIFT FULL EQUATION
change in f/ f = change in wl/ WL = V/C
Where change in F and WL is the mod of actual wavelength and observer wavelength
And V is the RELATIVE VELOCITY between the star and the earth or whatever
c is the speed of light
Why does the shifted frequency and wavelength of a galaxy still give speed of light
Thus if you found the shifted f, how can easily find shifted wavelength without using Doppler equation
As shifting f up shifts wl down, the ratio is the same
So if you found one, YOU CAN USE THE SPEED OF LIGHT TO FIND SHIFTED OTHER