Space Physics Flashcards

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1
Q

Galaxies

A

Collections of billions of stars orbiting around a galactic centre (black hole)

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2
Q

Star

A

Ball of gas (hydrogen and helium) which radiate energy in the form of electromagnetic wave

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3
Q

The sun

A

An average star in the Milky Way, halfway through its lifespan, which emits infrared, ultraviolet and visible light

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4
Q

Nuclear fusion in a stable star

A

Hydrogen atoms join together with enough force to fuse into helium atoms. This reaction produces a lot of energy which is released in the form of electromagnetic waves

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5
Q

Nuclear fusion in older stars

A

Old stars run out of hydrogen, so start fusing other things together and becomes unstable

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6
Q

From where a star is born

A

Interstellar clouds of gas and dust of which hydrogen must b present in

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7
Q

When is a star considered a protostar

A

When, due to gravity, the interstellar clouds start to collapse upon themselves causing all the elements to clump together. Hydrogen nuclei start fusing together and gravity pulls in more materials causing the temperature to increase

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8
Q

How can astronomical distances be measured

A

In light years where one light year is the distance travelled in the vacuum of space by light in one year.

9.5 x 10^5

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9
Q

Life cycle of a star (8)b

A

-Star formed from interstellar clouds of gas and dust containing hydrogen
-protostar forms due to the cloud collapsing and increasing in temperature due to its internal gravitational attraction
-Stable star forms when the inward force of gravity is balanced by an outward force due to the high temperatures
-

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10
Q

Describe what the solar system contains (5)

A

One star, the sun
8 planets mvemjsun
Minor planets, dwarf planets (Pluto) and asteroids in the asteroid belt
Moons that orbit the planets
Smaller solar system bodies (comets + natural satellites)

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11
Q

What are seasons caused by

A

Solar rays are more concentrated over a smaller area in the summer than in the winter

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12
Q

Comets

A

Clumps of loosely bound rock and ice moving in highly elliptical orbits around the sun

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13
Q

Orbits of the planets and comets etc.

A

They have elliptical orbits, of which the sun is not the centre unless when the orbit is approximately circular. When an object is closer to the sun it is faster as gravitational potential energy is converted to kinetic

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14
Q

What does the gravitational field strength of a planet depend on

A

It’s mass

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15
Q

Compare the first 4 planets to the last 4, why are they different

A

First 4 are rocky and small, last 4 are gaseous and large

The accretion model for solar system formation

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16
Q

Accretion model

A

4.5 billion years ago:
-Interstellar clouds of gas pulled together by gravity
-Planets formed in the accretion disk formed, through the rotation of material in the cloud, as the dust and gas comprised of many elements came together
When there was enough mass in the sun:
- Huge amount of energy produced that blew lighter particles from the planets to the outer parts of the solar system, resulting in the inner planets having a higher density than the outer

17
Q

Why planets orbit the sun

A

As the sun contains most of the mass in the solar system. This means that the sun has a very strong gravitational attraction which keeps the planets in orbit

18
Q

Describe the sun referring to size, composition and energy radiation

A

Star in the galaxy called the milky way
Medium size
Hydrogen and helium
Infrared, visible and ultraviolet regions of the electromagnetic spectrum

19
Q

What are stars powered by

A

Nuclear reactions that release energy

20
Q

What Nuclear reactions in stable stars involve

A

The fusion of hydrogen into helium

21
Q

Galaxies

A

Consist of billions of stars

22
Q

Describe the distance between the earth and the sun and other stars in the Milky Way

A

The earth is closer to the sun than the other stars

23
Q

How can astronomical distances be measured

A

In light years (distance traveled in the vacuum of space by light in one year)
9.5x10*15

24
Q

Light year

A

Distance travelled in the vacuum of space by light in one year
9.5x10*15

25
Q

Redshift

A

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

26
Q

Diameter of the Milky Way

A

100 000 light years

27
Q

The universe

A

Made up of billions of galaxies

28
Q

Describe Light emitted from distance galaxies

A

Appears redshift in comparison to light on earth, is evidence of the universe expanding and supports the Big Bang theory

29
Q

CMBR

A

Cosmic Microwave Background Radiation
Microwave radiation of a specific frequency observed at all points in space, produced shortly after the universe was formed and expanded into the microwave region of the electromagnetic spectrum as the universe expanded

30
Q

How can the speed at which a galaxy is moving away from the earth be found

A

The change in wavelength of the galaxy’s starlight due to red shift

31
Q

How can the distance of a galaxy be determined

A

From the brightness of a supernova in that galaxy

32
Q

How can the distance of a galaxy be found

A

Using the brightness of a supernova in that galaxy

33
Q

Hubble constant

A

Ratio of the speed at which the galaxy is moving away from the earth due to its distance from the earth
H0=v/d

34
Q

Current estimate for bubbles constant

A

2.2x10*-18 per second

35
Q

What does
d/v=1/H
Represent

A

An estimate for the age of the universe
Evidence for the idea that all matter in the universe was present at a single point