Chapter 5 : The formation of stars and planets Flashcards

1
Q

star

A

a dense cloud of gas that produces energy in its core by fusing light atoms into heavier ones

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2
Q

Kelvin temperature scale

A

use this to measure temperature of stars and other objects

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3
Q

interstellar cloud

A

cloud of cool dust and gas in the space between stars, it has self-gravity

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4
Q

self-gravity

A

a gravitational attraction among all parts of the same object

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5
Q

hydrostatic equilibrium of a cloud

A

when the forces on a cloud are balanced

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6
Q

molecular clouds

A
  • the densest, coolest, interstellar clouds

- composed of hydrogen, dust and other gases

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7
Q

Once a molecular-cloud core begins to collapse, what happens?

A

the innermost core becomes a star, the outer parts form planets

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8
Q

protostar

A

innermost part of a collapsing molecular-cloud core

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9
Q

Formation of a protostar

A
  • Molecular cores continue to collapse under their own gravity
  • As cloud collapses, force of gravity increases and the collapse accelerates
  • Center shrinks fastest; outer layers later
  • Produces a dense protostar
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10
Q

Star Formation: Growing Protostar at the Center

A

-Protostar heats up due to the conversion of gravitational energy into thermal energy: Particles collide as they are pulled towards the center, Raises the temperature of the core, Pressures and temperatures are not yet high enough for fusion to occur

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11
Q

Wien’s Law

A

Relationship between temperature of an object and peak wavelength the object emits

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12
Q

Flux

A

Energy emitted by one square meter of the object every second

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13
Q

Luminosity

A

Total energy emitted every second

Depends on temperature and size of the star

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14
Q

nebula

A

interstellar cloud of gas and dust

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15
Q

Protostars emit mainly what type of light? (due to their cool temperatures)

A

infrared

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16
Q

When a protostar is in balance, what is happening?

A

the force from hot gas pushes outward and the force of gravity pulls inward

17
Q

A protostar becomes a star when?

A
  • Core’s temperature and density increase until nuclear fusion is possible
  • Hydrogen begins turning into helium in the core
  • It becomes a star
18
Q

brown dwarf

A
  • Critical temperature for fusion of hydrogen to helium: 10 million Kelvin
  • Protostars less than 0.08 solar masses never start that reaction
  • “failed stars”
19
Q

Collapse is slowed ____ to the rotation axis. (perpendicular or parallel?)

A

Collapse is slowed perpendicular to the rotation axis (toward or away from the axis) but not parallel to it (up or down the axis).

20
Q

accretion disk

A

a disk that forms from the accretion of material around a massive object

21
Q

The accretion disk will have an overall rotation (clockwise or counterclockwise), due to conservation of ____ _____.

A

angular momentum

22
Q

angular momentum

A

conserved quantity of a revolving or rotating system with a value that depends on both the velocity and distribution of the mass

23
Q

Amount of angular momentum depends on 3 things:

A

1) How fast the object is rotating. (faster = more angular momentum)
2) Mass of object (more mass = more angular momentum)
3) Distribution of mass of object (more spread out = more angular momentum)

24
Q

conservation of angular momentum

A

angular momentum must remain the same in the absence of an external force

25
Q

refractory material

A

Does not melt at high temperatures (metals and rock)

26
Q

Volatile material

A

Melts at low temperatures (methane and other hydrocarbons)

27
Q

Inner disk has only _____ materials. Outer disk has _____ and _____ materials.

A

Inner disk has only refractory materials

Outer disk has refractory and volatile materials

28
Q

primary atmosphere

A

the gas (mostly hydrogen and helium) captured by a planet at the time of its formation

29
Q

secondary atmosphere

A

forms later in the life of a planet

30
Q

Four inner planets (terrestrial):

A

Mercury, Venus, Earth Mars

31
Q

Four outer planets (jovian):

A

Jupiter, Saturn, Uranus, Neptune

32
Q

Extrasolar planets

A

planets that orbit stars other than our Sun

33
Q

The Doppler effect

A

Motion of a light source toward or away from us changes the wavelength of the waves reaching us.
Redshift = Motion away
Blueshift = Motion toward

34
Q

Transit method

A

a planet passing in front of a star causes the total brightness of the star to decrease