Astro - Star Classification Flashcards

1
Q

Define apparent magnitude. What is the scale?

A

A measure of the brightness of the star as measured from Earth. Hipparcos scale, 1-6, brightest to dimmest.

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
2
Q

What is the equation for I1 / I2 ?

A

= 2.51^m1-m2

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
3
Q

What is an astronomical unit in words?

A

The average distance from the Sun to the Earth.

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
4
Q

What is a lightyear in words?

A

The distance travelled by moving at the speed of light for one year.

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
5
Q

What is a parsec in words?

A

The distance at which one AU subtends a parallax angle of one arcsecond.

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
6
Q

What is one arcsecond?

A

1/3600 degrees.

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
7
Q

Define absolute magnitude.

A

The apparent magnitude that an object would have if it were observed from a distance 10 parsecs away.

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
8
Q

What is the equation for absolute magnitude?

A

m - M = 5log(d / 10)
m = apparent magnitude
M = absolute magnitude
d = distance in PARSECS

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
9
Q

Between which numbers for magnitude of a star would be visible.

A

1-6.

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
10
Q

On a spectral irradiance over wavelength graph what is the peak value of a curve?

A

Predominant wavelength, wavelength MAX.

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
11
Q

What is Wein’s law?

A

λMAX T = 2.9x10^-3

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
12
Q

What is Stephan’s law?

A

P = 𝜎AT^4
P = luminosity

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
13
Q

What is the intensity law?

A

I = P / 4πd^2
d = distance from star to observer

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
14
Q

What are Balmer absorption lines?

A

A set of visible lines in the spectrum corresponding from n>3 to n=2.

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
15
Q

What are the spectral classes?

A

O - oh
B - bollocks
A - am
F - fucking
G - gonna
K - kill
M - myself

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
16
Q

What are the colours of spectral class in order from O to M?

A

Blue
Blue
Blue/White
White
Yellow/White
Orange
Red

17
Q

What are the temperatures of spectral class in order from O to M?

A

25000 - 30000
11000 - 25000
7500 - 11000
6000 - 7500
5000 - 6000
3500 - 5000
< 3500

18
Q

What are the absorption lines of spectral class in order from O to M?

A

He+, He, H
He, H
H
ionised metals
ionised metals, neutral metals
neutral metals
neutral atoms

19
Q

What are the axis of a H-R diagram? What do you need to remember?

A

Absolute magnitude over temperature. Temperature goes down from 50000 to 2500. M goes up from +15 to -10.

20
Q

What are the blobs on a H-R diagram and where are they?

A

White dwarf - round blob, bottom left
Main sequence - long thin diagonal blob, top of y to right of x
- colour classed from hot to cold (O-M)
Blue super giants - round blob between white dwarfs and red super giants
Red super giants - round blob on top right

21
Q

What are the 4 steps in star formation?

A

1) interstellar dust cloud collapses under gravity
2) GPE decreases, KE increases, temperature increases
3) When temperature reaches 10 million K H nuclei fuse into He
4) Radiation and gas pressure outward forces = gravity inwards forces

22
Q

What will happen in the evolution of a star similar to our Sun?

A

Main sequence - red giant - white dwarf and planetary nebula

23
Q

What will happen in the evolution of a massive star?

A

Main sequence - super red giant - supernova - black hole OR neutron star (dependant on mass)

24
Q

What are the features of a neutron star?

A

Very dense, 4x10^17 kg/m^3
Small, around 10 km

25
What are the features of a black hole?
Extremely dense (like you) Escape velocity > speed of light
26
How do you derive the equation for the Schwarzschild radius?
0.5 m ve^2 = G M m / rs rs = 2 G M m / c^2
27
What are type 1a supernovae? What can they be used for?
Happens with stars about the same mass and same brightness curve, they can be sued as standard candles to determine the distance of objects.
28
Where are SUPERMASSIVE BLACK HOLES found?
In the centre of galaxies.