Space Physics Flashcards

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1
Q

What are some features of the sun?

A

•Produces its own light
•A star
•6000°C temperature
•halfway through its lifetime of 10,000million years

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2
Q

What are the main features of the rocky planets?

A

•Mercury, Venus Earth and Mars
•Small
•Solid and rocky
•Layered structure

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3
Q

What are the main features of the gas planets?

A

•Jupiter, Saturn, Neptune, Uranus
•Made of gases
•Much larger
•Colder

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4
Q

What are the main features of moons?

A

•Solid rocky surface
•Orbits planets
•Has craters from meteors etc

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5
Q

What are the main features of asteroids?

A

•Consist of pieces of rock
•Various sizes
•Orbits between mars and Jupiter

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6
Q

What are the main features of comets?

A

•Consist of dust embedded in ice from water and methane
•Density similar to the 4 outer planets
•Large elliptical orbits

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7
Q

What is the order of the planets from the sun outwards?

A

Mercury, Venus, Earth, Mars, Jupiter
Saturn, Uranus, Neptune, Pluto
(MVEMJSUNP)

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8
Q

What does gravity provide that’s needed in space?

A

The force for initial motion of planets, comets, moons and satellites

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9
Q

How do stars form?

A

When enough dust and gas from space is pulled together by gravitational attraction.

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10
Q

What happens when smaller masses that form are attracted to larger mass?

A

Becomes planets

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11
Q

What do the studies of light from stars show?

A

They’re are compressed from mainly hydrogen and helium and their energy is supplied by the fusion of hydrogen into helium

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12
Q

What is formed by nuclear fusion in stars?

A

Naturally occurring elements apart from hydrogen

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13
Q

What is the life cycle of stars of a small mass?

A

-Yellow dwarf
-Red giant
-White dwarf
-Red dwarf
-Black dwarf

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14
Q

What is the life cycle of a star of a large mass?

A

-Blue star
-Blue supergiant
-Red supergiant
-Supernova
-Neutron star or black hole

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15
Q

Why is a star stable during the ‘main sequence’ period of its life cycle?

A

The outward force of thermal expansion is balanced by the inward force of gravity

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16
Q

What is the “main sequence” part of the stars life cycle?

A

Where a star spends most of its existence.

17
Q

Why do massive stars have a different life cycle after the ‘main sequence’ period?

A

They become red supergiants followed by a explosion which is called a supernova, this will then collapse and become neutron stars or black holes

18
Q

How did the universe begin and when?

A

As a big bang 14 billion years ago

19
Q

Why can nothing escape from a black hole?

A

Due to such a large gravitational field, with electromagnetic radiation such as light

20
Q

What is the evidence that the universe is expanding?

A

The observation that light from other galaxies is shifted to the red end of the spectrum. This shows all the galaxies are moving away from us.

21
Q

How were neutrons and protons formed?

A

After the Big Bang all the matter in the form of elementary subatomic particles moved in all directions

22
Q

How was nuclei formed?

A

With continued expansion and cooling

23
Q

How were hydrogen atoms formed?

A

After hydrogen nuclei was formed, Electrons were combined with hydrogen nuclei which formed hydrogen atoms.

24
Q

What is the further existence of the Big Bang?

A

Existence of cosmic microwave background radiation (CMBR)

25
Q

What is the evidence for planets outside our solar system? And methods used for this?

A

•The Hubble telescope
•The SETI project which involves using radio telescopes to search for meaningful radio signals

26
Q

How can the composition of the atmosphere of planets outside our solar system be determined?

A

Examination of light passing through their atmospheres, in search for oxygen.

27
Q

Why are distances to stars and galaxies measured in light years?

A

The distances are very large

28
Q

What is a light year?

A

The distance light travels in one year

29
Q

What are the possibilities of space exploration in terms of distance and speed of travel?

A

•Manned space craft
•Unmanned probes and use of robots to transmit photographs or collect specimens
•Chemical analysis of gases in atmosphere to reveal presence of life
•the SETI project to detect radio signals in other galaxies

30
Q

What are the limitations of space exploration in terms of distance and speed of light?

A

•Space radiation,
•Isolation and confinement
•Distance from Earth,
•Gravity (and lack of it)
•Closed or hostile environments.

31
Q

How can you calculate speed of recession of a galaxy?

A

V (directly proportional to) S
or
V=H° x S

32
Q

How can you calculate age of galaxy or universe?

A

Age= Distance Apart S
——————— = —
Speed of recession V

33
Q

What is ‘H°’? (Space speed and distance calculations)

A

Hubble constant

34
Q

What is ‘V’? (Space speed and distance calculations)

A

Speed of recession

35
Q

What is ‘S’? (Space speed and distance calculations)

A

Distance