Astronomy

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40 Terms

1
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Most of the iron on Earth came from:

supernova explosions

2
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Older clusters have main sequence turn-off points at what color?

Redder colors (cooler stars)

3
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What happens when a massive star’s core becomes iron?

The core collapses rapidly

4
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Which of the following describes main sequence stars?

They are fusing hydrogen in their cores

5
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Open clusters are:

Young and loosely bound group of stars

6
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How do open clusters differ from globular clusters?

Open clusters are younger and contain fewer stars

7
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The vertical axis of the H-R diagram typically represents:

Luminosity

8
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A star’s position on the main sequence is primarily determined by its:

Mass

9
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After a supernova, a core greater than 3 solar masses likely becomes:

A black hole

10
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A nova is:

A sudden brightening of a white dwarf in a binary system

11
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What happens in a close binary system when one star becomes a white dwarf?

Material can transfer to the white dwarf, leading to novae or supernovae

12
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The primary energy source for stars on the main sequence is:

Hydrogen fusion into helium

13
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What happens in the core of a low-mass star when hydrogen runs out?

The core contracts and heats up, beginning helium fusion

14
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We determine the age of a cluster using:

Main sequence turn-off point

15
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What is the likely fate of a star with a mass greater than 25 solar masses?

It collapses into a black hole

16
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The key factor that determines a star's evolutionary path is its:

Mass

17
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What allows a nova to repeat over time?

Ongoing mass transfer in a binary system

18
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In a neutron star, collapse is prevented by:

Neutron degeneracy pressure

19
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What are the axes of the Hertzsprung-Russell (H-R) diagram?

Luminosity and temperature

20
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An accretion disk forms when:

Material spirals into a compact object like a white dwarf or black hole

21
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What does the B-V color index represent?

The stars temperature and color

22
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What marks the turn-off point on a cluster's HR diagram?

The point where stars leave the main sequence

23
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Which observational quantity is directly plotted on the Y-axis of an HR diagram made from B and V data?

Apparent or absolute V magnitude

24
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What causes a star to leave the main sequence and enter the giant phase?

It exhausts hydrogen in its core

25
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What is the approximate age range of most globular clusters based on HR diagrams?

Over 12 billion years

26
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Why is B-V color index useful in plotting an HR diagram?

It estimates temperature using observable photometric data

27
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Where are main sequence stars found on the HR diagram?

Along a diagonal from upper-left to lower-right

28
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What distinguishes a star cluster HR diagram from a general stellar population?

All stars are at the same distance and age

29
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What does a star’s position on the main sequence primarily depend on?

It’s mass

30
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What is the shape of the main sequence on a B-V vs. V magnitude diagram?

Downward slope from left to right

31
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Why are most stars in a globular cluster located near the lower-right of the HR diagram?

They are cooler and less luminous main sequence stars

32
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Why must we filter out stars with inconsistent radial velocities in HR diagram studies of clusters?


They are likely non-cluster members

33
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A lower B-V value indicates a star is:

Hotter and bluer

34
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What physical properties are plotted on a Hertzsprung-Russell (HR) diagram?

Temperature vs. luminosity

35
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If a star has a high V magnitude but low B magnitude, its B-V index will be:

Negative, indicating a blue star

36
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How does the turn-off point help astronomers determine the age of a star cluster?

It reveals the lifespan of stars that have just left the main sequence

37
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Compared to open clusters, globular clusters are generally:

Older and more densely packed

38
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What is typically found above the main sequence on an HR diagram of an old cluster?


Red giants and horizontal branch stars

39
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Which type of stars evolve off the main sequence first in a cluster?


High-mass blue stars

40
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What is the primary fuel used by stars on the main sequence?

Hydrogen