astrophysics and cosmology Flashcards

1
Q

What defines a planet?

A

A spherical object with sufficient mass, no nuclear fusion, and a cleared orbit.

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2
Q

What is a dwarf planet?

A

A planet that has not cleared its orbit of other objects.

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3
Q

What is the difference between asteroids and comets?

A

Asteroids are small rocky objects with circular orbits, while comets are irregularly shaped and have eccentric elliptical orbits.

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4
Q

What is a galaxy?

A

A collection of stars, gas, and dust, containing around 100 billion stars.

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5
Q

What is a nebula?

A

A large cloud of gas and dust where stars are born.

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6
Q

What is the main sequence phase of a star?

A

The stable phase where gravitational forces and radiation pressure balance each other.

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7
Q

What happens when a low-mass star (0.5M☉ - 10M☉) runs out of hydrogen?

A

It becomes a red giant, then a white dwarf, and finally cools over time.

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8
Q

What is the Chandrasekhar limit?

A

1.44M☉—the maximum mass a white dwarf can have before collapsing.

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9
Q

How does a massive star (>10M☉) evolve?

A

t becomes a red supergiant, undergoes a supernova, and may become a neutron star or black hole.

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10
Q

How do black holes form?

A

f a collapsing core exceeds 3M☉, gravity overcomes all forces, preventing even light from escaping.

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11
Q

What happens when an electron absorbs energy?

A

It moves to a higher energy level

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12
Q

What is an emission spectrum?

A

Bright spectral lines on a black background, unique to each element.

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13
Q

What is an absorption spectrum?

A

Dark spectral lines on a continuous spectrum where light is absorbed by a cooler gas.

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14
Q

What is Wein’s Law?

A

Peak wavelength of a star’s radiation is inversely proportional to its temperature.

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15
Q

What is Stefan’s Law?

A

A star’s luminosity is proportional to the fourth power of its temperature.

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16
Q

What is an Astronomical Unit (AU)?

A

he average distance from Earth to the Sun (1.5 × 10¹¹ m).

17
Q

What is a parsec (pc)?

A

The distance at which 1 AU subtends an angle of 1 arcsecond (3.1 × 10¹⁶ m).

18
Q

What is stellar parallax?

A

The apparent shift in a star’s position due to Earth’s orbit, used to measure distances up to 100pc.

19
Q

What is the Doppler Effect?

A

The change in wavelength when a source moves relative to an observer.

20
Q

What does redshift indicate?

A

A star or galaxy is moving away from us.

21
Q

What is Hubble’s Law?

A

he farther a galaxy is, the faster it moves away (V = H₀d).

22
Q

hat is the Big Bang Theory?

A

The idea that the universe started as a singularity and has been expanding ever since.

23
Q

What is cosmic microwave background radiation?

A

Remnant radiation from the early universe, supporting the Big Bang theory.

24
Q

What is dark matter?

A

A mysterious substance making up 27% of the universe, detectable only by its gravitational effects.

25
Q

What is dark energy?

A

The unknown force causing the accelerated expansion of the universe.

26
Q

State how an emission line is produced

A

Electron(s) makes a transition to a lower (energy) level /
loses energy and emitting a photon(s) / EM radiation

27
Q

Light from a similar star is viewed in a galaxy further away. The star is part of a pair of stars
which orbit a common centre of mass.
Describe and explain how the equivalent spectrum might appear

A

Less intense
Galaxy is moving faster and therefore greater / longer
wavelength (AW)
Periodic shift in wavelength (if plane of orbit is in line of
sight) (ORA)

28
Q

The Universe evolved from the Big Bang.
Describe the evolution of the Universe up to the formation of the first nuclei.

A

Any three from:
1. At the Big Bang the Universe is a singularity / very
dense / very hot
2. Expansion / inflation / high energy (gamma) photons but
no matter
3. Quarks and leptons form / Quark-Gluon Plasma phase
4. Quarks combine to form neutrons / protons / hadrons
5. Hadrons / neutrons and protons / nucleons combine
to make nucleeus