Last Unit Flashcards

All the other stuff

1
Q

What nuclear reactions happen to a star while it is on the main sequence?

A

Hydrogen fusion to helium

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2
Q

What triggers a star to leave the main sequence?

A

No more hydrogen in the core

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3
Q

What happens to the internal events of a star when it leaves the main sequence?

A

The core collapses, increasing it’s temperature.
The envelope swells, decreasing it’s temperature.
A shell is created where hydrogen is fused.

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4
Q

What happens during the helium flash?

A

The core is now hot enough to fuse helium.

The core becomes larger, shortening the envelope.

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5
Q

In a star like our sun what happens when it runs out of helium?

A

There is not enough mass to fuse carbon, so it will explode into a planetary nebula, ejecting a fraction of the envelope. A white dwarf will remain.

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6
Q

What are the properties of a white dwarf?

A

Very small, very hot star where no more nuclear reactions occur. Little luminosity.

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7
Q

What fate awaits stars with less than 5 solar masses?

A

A white dwarf

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8
Q

If a white dwarf gains enough mass and exceeds the Chandrasekhar limit (1.4 solar masses), what will happen to the star?

A

It will collapse into a neutron star giving rise to a supernova of type Ia.

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9
Q

What is the fate of a star with a mass greater than 5 but less than 15 solar masses?

A

It will become a neutron star.

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10
Q

What are the characteristics of a neutron star?

A

It is very small (~10km) but has a mass between 1.4 and 3 solar masses so it is very dense. It rotates really fast because of the conservation of angular momentum during it’s collapse. It also has a huge magnetic field.

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11
Q

How can a neutron star be observed?

A

As the companion of a star

As a pulsar (similar to a lighthouse)

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12
Q

What fate awaits a star should it have a mass greater than 15 times that of our sun?

A

Collapse into a black hole

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13
Q

If the mass of a star is less than 0.08 solar masses, what happens?

A

Nuclear reactions never start and is therefore called a brown dwarf.

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14
Q

What are the building blocks of the universe and how are they organized?

A

Galaxies, organized in Groups, Clusters and Superclusters.

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15
Q

What are the three main types of galaxies?

A
Spiral galaxies (~60%)
Elliptical galaxies (~35%)
Irregular galaxies (~5%)
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16
Q

How do we know we aren’t in the center of the galaxy?

A

The galactic halo is not centered around the Sun

17
Q

The disk or the halo of a galaxy mostly consists of pop II stars

A

Halo

18
Q

How many major arms does our galaxy have?

A

2

19
Q

What is the rotation curve of a galaxy?

A

He rotation differential (not as a rigid body) the variation of vrot with distance.

20
Q

On what order of years does it take the sun to revolve once around the galaxy?

A

200 million years

21
Q

What is 90% of the mass of our galaxy?

A

Dark matter

22
Q

What are some possible candidates for dark matter?

A

MACHOS (faint stars, failed stars, planets, etc.)

WIMPS (neutrinos? exotic particles?)

23
Q

What is the cosmological principle?

A

The idea that we are not a special case in the universe.

24
Q

What supports the cosmological principle?

A
  • The homogeneity of matter distribution (same density everywhere)
  • The isotropy of the Hubble flow (same in every direction)
  • The isotropy of the cosmic microwave background