ASTROPHYSICS Flashcards

(41 cards)

1
Q

Apparent Magnitude

A

brightness of an object as seen from earth

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

Absolute magnitude

A

Brightness seen from 10pc (parsec)

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

light year

A

distance traveled by light in one year

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

parsec

A

distance to an object subtending 1 second of arc to earths orbit

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

State meaning of T in Stefan-Boltzmann law

A

Kelvin temperature of surface

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

Unit of luminosity

A

watts

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

convex/ converging lens

A

focuses incident light

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

concave/ diverging lens

A

spreads out light

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

focal length

A

distance between centre of a lens and principle focus

the shorter the focal length the stronger the lens

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

real image

A

formed when light rays cross before refraction

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

virtual image

A

formed on same side as lens, light rays do not cross

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

lens formula

A

1/u + 1/v = 1/f

u - distance of object to centre of lens
v - distance of image to centre of lens
f - focal length

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

power of a lens

A

shorter focal length, more powerful the lens

measured in D (dioptres)
converging (positive)
diverging (negative)
P = 1/u + 1/v = 1/f

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

normal adjustment

A

sum of focal lengths of objective and eyepiece lens

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

Quantum efficiency equation

A

(#electrons released) divided by
(#incident photons)

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

Quantum efficiency of human eye

A

1%

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
17
Q

CCD advantages

A

store more images
better resolution
wider range of wavelengths detected

18
Q

What is the minimum resolving angle of the human eye

A

3.2 x 10^-4 rad or 0.02 degrees

19
Q

For us to just be able to distinguish between two diffraction patterns…

A

The central maxima of one pattern has to coincide with the other patterns first minimum

20
Q

Astronomical unit

A

1 AU is the mean distance between the Earth and the Sun.

21
Q

number of brightest star in hipparcos scale

22
Q

number of dimmest star in hippacros scale

23
Q

apparent magnitude scale based on…

24
Q

A stars total power output known as its…

25
When regions of a nebula collapse and KE of gas and dust particles increase, how does this affect temperature?
The temperature increases because temperature is proportional to the average kinetic energy of the gas and dust particles.
26
The emitted frequency
the frequency of the sound wave that's emitted by a source
27
Observed frequency
the frequency of the sound wave that reaches your ear.
28
if wave speed is constant, what is the relationship of λ and f
inversely proportional
29
Red shift
When an object is moving away from us (λ increases)
30
Blue shift
When an object is moving towards us (λ decreases)
31
Redshift (using absorption lines)
z = Δλ/λ or -Δf/f
32
Recessional velocity
how fast a star is moving away from us
33
Binary star system
When two objects orbit each other around a common centre of mass
34
Hubble’s constant
v/d = H (kms^-1)(Mpc^-1) = constant
35
Cosmic microwave background radiation
CMBR is radiation left over from the Big Bang, gamma radiation have been stretched out into microwaves (as universe is expanding).
36
Hydrogen and Helium during early universe
75% Hydrogen 25% Helium
37
Element right after big bang
Hydrogen
38
How did helium form after the big bang
The temperature and pressures were so high that pairs of hydrogen nuclei began to fuse into helium
39
After universe expanded the temperature and pressure…
dropped no more fusion of hydrogen into helium
40
evidence for the Big Bang
-Hydrogen and Helium ratio -Red shift, objects moving away from -Cosmic Microwave Background Radiation
41
age of the universe equation
1/H