Space Physics Flashcards

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1
Q

Why do planets orbit the sun?

A

The sun contains most of the mass in the solar system so it has the strongest gravitational field strength

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2
Q

Why are the inner planets rocky and the others gassy.

A

The heat and radiation from the sun forced the lighter elements(gases) further away.
So the closer planets were formed of heavier and rocky elements. The farther planets were formed mostly of gas.

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3
Q

What is gravitational field strength?

A

Force per unit mass acting on an object in the field.

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4
Q

How does nuclear fusion begin in a star?

A
  • after the formation of a protostar, gravity pulls in mass and gasses. Bringing them closer and heating them up.
  • the gasses become hot and compressed, reaching the temperature and pressure high enough to trigger NUCLEAR FUSION.
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5
Q

How was our solar system formed? [5]

A
  • began as a swirling ball of dust and gas(hydrogen) called a nebula
  • gravity pulls mass to the centre, collapsing the nebula inwards forming a protostar.
  • this becomes a stable star when the inward force of the gravity is equal to the outward force of the heat from the star.
    (The inward force = outward force0
  • the remaining gas and dust(mass) which was not pulled to the centre form a rotating accretion disc.
  • these masses are then slowed by collision and pulled into clumps by gravity to make larger rocks that orbit the sun called proto planets which are then formed into planets.
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6
Q

What is accretion?

A

Gradual growth by the addition of material.

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7
Q

What does gravitational field strength depend on?

A
  1. The mass. Greater mass, greater field strength on the surface of the planet.
  2. Distance. The larger the distance from the planet the weaker the field strength.
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8
Q

What keeps an object in orbit around the sun?

A

The gravitational attraction of the sun.

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9
Q

Why do the outer planets have a longer orbital period?

A

The strength of the sun’s gravitational field decreases with distance.
The further a planet is from the sun, the weaker the gravitational pull(force) of the sun and the slower it’s speed.

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10
Q

Why do objects in elliptical orbits travel faster when closer to the sun?

A

The farther away an object is from the sun, the more gravitational potential energy it will gain and loose kinetic energy.
When close to the sun, it looses it’s gravitational potential energy and gains kinetic energy.

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11
Q

Does gravitational POTENTIAL energy increase with distance?

A

Yes.

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12
Q

Does gravitational FIELD force increase with distance?

A

No.

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13
Q

Which of these have elliptical orbits?
A. The minor planets
B. The major planets
C. Comets

A

A and C

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14
Q

How does orbital distance affect gravitational attraction from the sun?

A

The larger the distance the weaker the gravitational attraction to the sun.

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15
Q

What does the density of a planet imply?

A

The lower the density the larger the size of the planet.
(Gas giants have low density and large volume

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16
Q

What else can affect the surface temperature of a planet?

A
  • the color, black or white. Absorber and emitter.
  • if the planet has an atmosphere. A planet without an atmosphere cannot retain heat so it heats up quickly and looses heat quickly.
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17
Q

Mention 4 properties of the sun

A
  • it is of medium size
  • contains mostly hydrogen and helium
  • it radiates most of its energy in infrared, visible and ultraviolet regions of the electromagnetic spectrum.
  • it is powered by nuclear fusion
18
Q

How are stars powered? And how is it different for stable stars?

A

By nuclear reactions (fusion) that release energy.
In stable stars, the nuclear reactions involve the fusion of hydrogen into helium.

19
Q

What is the closest star to Earth?

A

The sun.

20
Q

When is a star stable?

A

When the inward force of gravity is equal to the outward force of the heat from the fusion reaction.

21
Q

What is the value of a light year?

A

9.5*10^15m
(The speed of light

22
Q

What is the definition of a light year?

A

The distance travelled by light in (the vacuum of) space in one year.

23
Q

Explain the life cycle of a star [8]

A
  1. A star is formed from interstellar clouds of gas and dust that contain hydrogen - nebula.
  2. A protostar is an interstellar cloud collapsing and increasing in temperature as a result of its internal gravitational attraction
  3. A protostar becomes a stable star when the inward force of gravitational attraction is balanced by an outward force due to the high
    temperature in the centre of the star
  4. All stars eventually run out of hydrogen as fuel for the nuclear reaction
  5. Most stars (medium stars) expand to form red giants and more massive stars expand to form red supergiants when most of the hydrogen in the centre of the star has been converted to helium
  6. Red giants shed their outer layers leaving behind a hot and dense core called a white dwarf. (Still considered as a star). This uses helium as its nuclear fusion converting it to carbon. When fusion stops the star cools and fades forever.
  7. A red supergiant explodes as a supernova, forming a nebula containing hydrogen and
    new heavier elements, leaving behind a neutron star or a black hole at its centre
  8. The nebula from a supernova may form new stars with orbiting planets
24
Q

State two properties of our Milky Way galaxy.

A
  • There are 100 billions of stars in a galaxy.
  • the diameter of the milky way is approximately 100 000 light years.
25
Q

What do supernova’s form when they explode?

A

Interstellar nebulas

26
Q
A
27
Q

What do red giants form?

A

Planetary nebula with a white dwarf at the centre.

28
Q

Difference between interstellar nebula’s and planetary nebular’s.

A

Interstellar nebula’s are formed from supernova’s. It is formed away from it’s previous solar system.
Planetary nebular is from a medium sized star.

29
Q

What does red shift prove?

A

It is evidence that the distance between distant galaxies is increasing, thus the universe is expanding.

29
Q

What is redshift?

A

an increase in the observed
wavelength of electromagnetic radiation emitted from receding stars and galaxies

30
Q

How does the red shift support the big bang theory?

A

As the galaxies appear to be moving apart, they may have once been together in the same space.

31
Q

What is CMBR?

A

Cosmic Microwave Background Radiation.

32
Q

Define CMBR.

A

Microwave radiation of a specific frequency is observed at all points in space around us.

33
Q

What is the Doppler Effect?

A

The increase in the wavelength of light waves (electromagnetic radiation) from objects moving away from earth at high speeds.

34
Q

When was CMBR formed?

A

After the universe was formed. The radiation has been expanded into microwave region of the electromagnetic spectrum as the universe expanded

35
Q

What is Hubble’s constant?

A

The ratio of the speed v at which the galaxy is moving away from the earth to its distance from the earth.
v/d

36
Q

What is the value and unit of the Hubble’s constant.

A

2.2 * 10^-18 per second.

37
Q

How do we calculate the speed at which a galaxy is moving away from Earth (receeding).

A

can be found from the change in wavelength of the galaxy’s starlight
due to redshift

38
Q

How do we calculate the distance of a far galaxy?

A

using the brightness of a supernova in the galaxy

39
Q

What does this represent and prove?
D/v = 1/Ho

A

an estimate for the age of the Universe and this is evidence for the idea that all the matter in the Universe was present at
a single point

40
Q
A