Exploring the universe Flashcards

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1
Q

Why do astronomers use lightyears to measure the distance of objects in space?

A

Because space is too big to use small measurments like kilometres.

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2
Q

Define nuclear fusion and it’s role when producing energy in the core of a main star.

A

Its when two small nuclei fuse to form a bigger nuclear, and when the energy that stars release forms hydrogen and which further form helium in a core of a main star. In the process the potential energy is converted into mass.

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3
Q

Explain what colour a star would be if the wavelength was approximately 840nm.

A

Because in a diagram of the visble spectrum the wavelength of this specific star would be off to the red side of the wavelengths.

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4
Q

Our galaxy…

A

is called the milky way and is a spiral shape.

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5
Q

What does the mass of a star tell us?

A

It’s absolute brightness.

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6
Q

What is the Big Bang Model

A

It’s the term used to describe the rapid expansion of the very early universe from a hot, dense concentration of matter.

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7
Q

Define Accreation

A

Accretion is defines as the process of growth of a body by gathering or aggregating more matter due to gravitational forces.

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8
Q

What are two peices of evidence that support the Big Bang model?

A

The red shift and cosmic microwaves background radiation.

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9
Q

When does a Protostar form?

A

When the gas of a nebula condenses, losing graviational potential energy and gainign kenetic energy, rasining the temprature of atoms.

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10
Q

What happens when theres fusion in the core of a protostar?

A

If the fusion of hyrdogen is big enough built in the core of a protostar then a main sequence star is formed.

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11
Q

What happens when the hydrogen in the main sequence star runs out?

A

It forms either a red giant or supergiant.

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12
Q

Why do white dwarfs form after red giants

A

Because when the fusion completly stops the gas breaks down, condensing into a small object called a white dwarf.

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13
Q

What is formed after a supergiant?

A

When the fusion stops in a supergiant the remaining energy explodes and creates a supernova.

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14
Q

What are the next steps after a supernova is formed?

A

If the remaining mass is smaller then 3 solar masses a neutron star is formed but if the remaining mass is larger than 3 solar masses then the black hole is created.

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15
Q

Order the suns colour from coldest to hottest.

A

red, yellow, white, blue

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15
Q

Briefly describe the evolution of the universe.

A

The present energy. Electrons, protons and neutrons where formed from the energy that was being converted into mass. Further on when the universe continued to cool and expand, small gaseous atoms like hydrogen and helium where formed. From this dense places squeezed particles of matter together and formed galaxies containing stars. Thus, stars and galaxies formed as a result of accretion.

16
Q

state two advantages of using instruments of board spacecrafts to explore the universe.

A
  1. you can get closer to some astronomical objects
  2. you can avoid the distortain that occure due to the atmosphere.
17
Q

describe a star

A

An astronomical object consisting of a sphere of matter, giving off heat and light, held together by it’s own gravity.

18
Q

What is our solar system

A

It’s made out of a sun, and eight planets and their satellites.

19
Q

Describe the difference between apparent and absolute brightness of a star.

A

The apparent brightness of a star is the brightness that we see from earth, and the absolute is the true brightness of a star.

20
Q

Name the cycle of a star in order.

A
  1. nebula
  2. protostar
  3. main sequence star
  4. red giant
  5. planetary star
  6. white dwarf
  7. supergiant
  8. supernova
  9. neutron star
  10. black hole
21
Q

Define Nebula

A

an enormous cloud of dust and gas occupying the space between stars and acting as a nursery for new stars.

22
Q

How do you find speed?

A

distance/time

23
Q

How do you find the distance?

A

speed x time

24
Q

what is in our solar system?

A

It is made up off a sun, eight planets, and their natural satellites.