Stars Flashcards

1
Q

What is the definition of one parsec?

A

The distance at which a star will give a parallax angle of one arc second.

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2
Q

What is the definition of absolute magnitude?

A

The apparent magnitude of a star if it were located 10 parsecs away from Earth.

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3
Q

How does the intensity of light change depending on distance away from it?

A

Intensity is proportional to 1/r^2 (inverse square law)

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4
Q

What is the equation involving distance, apparent magnitude and absolute magnitude?

A

M = m +5 - 5logd

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5
Q

Describe the nature of neutron stars.

A

Electrons forced inside the nucleus and combine with protons to form neutrons. Sea of free nucleons exert a pressure known as neutron degeneracy pressure.

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6
Q

What stages does a star with solar mass go through?

A
  • Protostar
  • Main sequence star
  • Red giant
  • Planetary nebula
  • White dwarf
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7
Q

What stages does a star with extremely large mass go through?

A
  • Protostar
  • Main sequence star
  • Red Super Giant
  • Supernova
  • Either neutron star or black hole
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8
Q

Describe the nature of black holes.

A

Formed when extremely massive stars explode in a supernova - neutron star collapses to zero volume and infinite density. Region around black hole where gravity is so great that light can’t escape is called the Schwarzschild radius.

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9
Q

How did astronomers find evidence for neutron stars and black holes?

A

Neutron stars - Neutron stars rotate very fast producing spiralling electrons
Black holes - X-ray source due to accretion discs from orbiting binary companions

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10
Q

What are the spectral classes and what temperatures and colours are associated with each?

A
O - 50 - 25 thousand K - Blue
B - 25 - 11 thousand K - Blue
A - 11 - 7.5 thousand K - Blue/White
F - 7.5 - 6 thousand K - Green
G - 6 - 5 thousand K - Yellow
K - 5 - 3.5 thousand K - Orange
M - less than 3.5 thousand K - Red
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11
Q

Describe the H-R diagram (including axis scales)

A

Main sequence down middle, red giants in top right and white dwarfs in top left.
Y-axis is Absolute magnitude and X-axis is spectral type (temperature), but is an inverse scale (further along you go, colder star is)

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12
Q

How can elements be found using spectrum?

A

Diffract star light and match absorption lines with corresponding elements absorption lines.

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13
Q

What are emission nebulae, absorption nebulae and open clusters associated with?

A

The birth of stars.

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14
Q

What are planetary nebulae and supernovae associated with?

A

The death of stars.

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