Modern Astronomy

0.0(0)
Studied by 0 people
call kaiCall Kai
learnLearn
examPractice Test
spaced repetitionSpaced Repetition
heart puzzleMatch
flashcardsFlashcards
GameKnowt Play
Card Sorting

1/64

encourage image

There's no tags or description

Looks like no tags are added yet.

65 Terms

1
New cards

What is the distance ladder?

A series of methods used to measure distances in space.

2
New cards

What is parallax?

Measuring nearby star distances using their apparent shift in position.

3
New cards

What is the period-luminosity relationship?

A Cepheid variable star's period reveals its luminosity, helping measure distance.

4
New cards

What is spectroscopic parallax?

Estimating a star's distance using its properties and the H-R diagram.

5
New cards

What does the H-R diagram show?

Stars arranged by luminosity and temperature.

6
New cards

What is the interstellar medium (ISM)?

Gas and dust found between stars.

7
New cards

What are molecular clouds?

Cold, shielded clouds made mostly of molecular hydrogen where stars form.

8
New cards

What radiation does hot ionized gas emit?

Ultraviolet radiation.

9
New cards

How can molecular clouds be observed?

Through infrared and radio emission and absorption.

10
New cards

Why are there dark patches in the Milky Way?

Interstellar dust blocks starlight.

11
New cards

What is a reflection nebula?

A dust cloud reflecting light from nearby stars.

12
New cards

What causes reddening?

Dust scatters blue light more strongly than red light.

13
New cards

What radiation does interstellar dust emit?

Infrared radiation.

14
New cards

What causes a molecular cloud to collapse?

Gravity overcomes gas pressure.

15
New cards

What happens as a molecular cloud contracts?

It spins faster and can break into smaller regions.

16
New cards

Why do stars form in clusters?

Star formation often happens in waves within large clouds.

17
New cards

What is a protostar?

A young star still forming from collapsing gas.

18
New cards

Which is larger and denser: a cloud or a protostar?

The cloud is larger, but the protostar is denser.

19
New cards

What powers a pre-main-sequence star?

Gravitational contraction instead of nuclear fusion.

20
New cards

What clears gas away from a young star?

Stellar winds.

21
New cards

Why do planets form around stars?

Leftover gas and dust form a spinning disk where planets develop.

22
New cards

What is the skater effect?

A contracting spinning object rotates faster.

23
New cards

What is the Doppler method for detecting planets?

Detecting a star's wobble through changes in its spectrum.

24
New cards

What is the transit method for detecting planets?

Detecting a planet when it passes in front of its star and dims its light.

25
New cards

What are selection effects in planet detection?

Some planets are easier to detect than others.

26
New cards

What is a rogue planet?

A planet that does not orbit a star.

27
New cards

What is the Drake Equation?

An equation estimating the number of communicating civilizations in our galaxy.

28
New cards

What does N represent in the Drake Equation?

The number of communicating civilizations.

29
New cards

What does R* represent in the Drake Equation?

The rate of star formation.

30
New cards

What does fp represent in the Drake Equation?

The fraction of stars with planets.

31
New cards

What does ne represent in the Drake Equation?

The average number of potentially habitable planets per planetary system.

32
New cards

What does fl represent in the Drake Equation?

The fraction of habitable planets where life develops.

33
New cards

What does fi represent in the Drake Equation?

The fraction of life-bearing planets where intelligent life develops.

34
New cards

What does fc represent in the Drake Equation?

The fraction of intelligent civilizations that communicate.

35
New cards

What does L represent in the Drake Equation?

How long civilizations remain detectable.

36
New cards

What is the main sequence?

The stage when stars fuse hydrogen into helium in their cores.

37
New cards

Why do stars leave the main sequence?

They run out of hydrogen in their cores.

38
New cards

Why do massive stars have shorter lifetimes?

They burn through their nuclear fuel faster.

39
New cards

What happens when a star becomes a giant?

Its size and luminosity increase greatly.

40
New cards

What does cluster evolution reveal?

Massive stars evolve faster than low-mass stars.

41
New cards

What determines how a star dies?

Its mass.

42
New cards

What happens during helium burning?

Helium fuses into carbon.

43
New cards

What is double-shell burning?

Hydrogen and helium fuse in separate shells around a star's core.

44
New cards

Which stars form planetary nebulae?

Low-mass stars, like the Sun, eject their outer layers.

45
New cards

What happens to the Sun at the end of its life?

It becomes a white dwarf, not a neutron star.

46
New cards

What are the sizes of white dwarfs and neutron stars?

White dwarfs are Earth-sized; neutron stars are city-sized.

47
New cards

What is a white dwarf made of?

Mostly carbon and oxygen, supported by electron pressure.

48
New cards

What is the Chandrasekhar mass limit?

About 1.4 solar masses, the maximum mass for a typical white dwarf.

49
New cards

How does a neutron star form?

A massive star's core collapses, combining protons and electrons into neutrons.

50
New cards

What is a neutron star made of?

Mostly neutrons packed extremely tightly together.

51
New cards

Why is neutron star material denser than white dwarf material?

Neutron stars compress more mass into much less space.

52
New cards

What is a pulsar?

A rotating neutron star whose radiation beams sweep past Earth like a lighthouse.

53
New cards

What is a Type II supernova?

A massive star's iron core collapses, causing an explosion.

54
New cards

What role do neutrinos play in a supernova?

They carry energy away and help power the explosion.

55
New cards

What triggers a Type Ia supernova?

Runaway nuclear burning in a white dwarf.

56
New cards

How does a solar-mass star eject its outer layers?

Late-stage instability and double-shell burning lead to mass loss.

57
New cards

What is an accretion disk?

A spinning disk of matter falling toward a compact object.

58
New cards

What is an event horizon?

The boundary beyond which nothing, including light, can escape.

59
New cards

What is a black hole singularity?

A theoretical point of infinite density at a black hole's center.

60
New cards

What are two ways a black hole can form?

A massive star's core collapses, or a neutron star gains enough mass to collapse.

61
New cards

What is gravitational lensing?

Gravity bending light from distant objects.

62
New cards

What are three pieces of evidence for black holes?

Orbiting stars, X-rays from accretion disks, and gravitational lensing.

63
New cards

What is a quasar?

An extremely bright active galactic nucleus powered by a feeding supermassive black hole.

64
New cards

Why is the sky blue?

Air molecules scatter blue light more strongly than red light.

65
New cards

Why are sunsets red?

Sunlight travels through more atmosphere, scattering away much of the blue light.