Topic 10 - Space Flashcards

1
Q

What is an Astronomical Unit(AU)?

A
  • Mean distannce between the Earth and Sun
How well did you know this?
1
Not at all
2
3
4
5
Perfectly
2
Q

What is a light year?

A
  • Distance travelled by an EM wave through space in one year
  • Equal to 63000AU
How well did you know this?
1
Not at all
2
3
4
5
Perfectly
3
Q

What is parallax?

A
  • The apparent in position of an object depending on the vewing angle
  • Change in position is measured as the parallax angle
How well did you know this?
1
Not at all
2
3
4
5
Perfectly
4
Q

How can you use parallax measurements to calculate the distance of an object from the Earth?

A
  • The object is viewed from two positions whilst the Earth is on opposite ends of its orbit diameter around the Sun.
  • The change in angular position against the background of fixed stars in measured
  • Trigonometry is used to calculate distance to star
How well did you know this?
1
Not at all
2
3
4
5
Perfectly
5
Q

What is the limitation of using parallax measurements?

A
  • If stars are too far away the angular displacement is too small to measure
How well did you know this?
1
Not at all
2
3
4
5
Perfectly
6
Q

What is a parsec?

A
  • Distance to a star whose parallax angle is 1 arcsecond
  • 3.09x10^16
How well did you know this?
1
Not at all
2
3
4
5
Perfectly
7
Q

What is luminosity?

A
  • Total energy a star emits in one second
How well did you know this?
1
Not at all
2
3
4
5
Perfectly
8
Q

How can you calculate luminosity?

A
  • Stefan-boltzmann law: L=4πr^2σT^4
  • Where σ is the steffan boltzmann-constant
  • Where T is the surface temperature of the star (in Kelvin)
  • Where r is the radius of the star
How well did you know this?
1
Not at all
2
3
4
5
Perfectly
9
Q

What is intensity?

A
  • Power of radiation incident on Earth from star per square meter.
How well did you know this?
1
Not at all
2
3
4
5
Perfectly
10
Q

How can you calculate intensity?

A
  • Inverse square law: I = L/(4πd^2)
  • Where d is the distance from the object to Earth
How well did you know this?
1
Not at all
2
3
4
5
Perfectly
11
Q

What is a standard candle?

A
  • A stellar object of known luminosity
How well did you know this?
1
Not at all
2
3
4
5
Perfectly
12
Q

How can standard candles be used to calculate distances?

A
  • Standard candle has known luminosity
  • Standard candle’s flux on Earth is measured
  • Use inverse square law
  • Distance to standard candle is calculated and used as a reference to find out other distances
How well did you know this?
1
Not at all
2
3
4
5
Perfectly
13
Q

What is Wein’s Law?

A
  • λ(max)T= 2.9x10^-3
How well did you know this?
1
Not at all
2
3
4
5
Perfectly
14
Q

What is a Hertzsprung-Russel (H-R) diagram?

A
  • Visual represntation of lifecycle of a star
  • A plot of luminosity against surface temperature
How well did you know this?
1
Not at all
2
3
4
5
Perfectly
15
Q

What is the lifecycle of a star with similar mass to the sun?

A
  • Stellar nebula
  • Protostar
  • Main Sequence
  • Red Giant
  • White dwarf
  • Black dwarf
How well did you know this?
1
Not at all
2
3
4
5
Perfectly
16
Q

What is the lifecycle for a star with mass between 1.4 and 3 times solar masses?

A
  • Stellar nebula
  • Protostar
  • Main Sequence
  • Red Supergiant
  • Supernova
  • Neutron Star
17
Q

What is the lifecycle for a star with mass greater than 3 times solar masses?

A
  • Stellar nebula
  • Protostar
  • Main Sequence
  • Red Supergiant
  • Supernova
  • Black Hole
18
Q

How is a protostar formed?

A
  • Clouds of gas and dust (nebulae) clump together under gravity
  • Clumps form a denser centre
  • Temperature increases as star gets denser
19
Q

How is a main sequnce star formed?

A
  • Once temperature of protostar is high enough fusion of hydrogen nuclei begins
  • Outwards force due to fusion and gravity are in equilibrium
  • Greater the mass of the star the shorter its main sequnce stage
20
Q

How is a Red Giant formed?

A
  • Once hydrogen fuel in main sequnce star runs out temperature of core increases under weight of star
  • Fusion of helium begins
  • Outer layers expand and cool
21
Q

How are white dwarfs formed?

A
  • Once helium fuel in a Red Giant runs out, star collapses under its own weight again
  • Core shrinks and ejects its outer layers leaving behind a white dwarf
22
Q

How are Supernova formed?

A
  • When all fuel runs out core collapses inwards and becomes rigid as it cant be compressed further
  • Outer layers fall inwards and rebound off the core into space in a shockwave
23
Q

How are neutron stars formed?

A
  • When core of a larger star collapses gravity is so strong it forces electrons and protons together to form neutrons
24
Q

How are black holes formed?

A
  • When core of a giant star collapses neutrons are unable to withstand the force of gravity forcing them together
25
Q
A