Space Flashcards

1
Q

For projectile motion, what is the only equation you should use for the vertical part of the motion?

A

For the vertical part of the motion, the only equation which should be used is

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2
Q

What is the difference between mass and weight?

A

Mass is a measure of the amount of ‘stuff’ that makes up an object.

Weight is the force due to gravity acting on an object.

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3
Q

By referring to the horizontal and vertical parts of its motion, explain the curved path of a projectile.

A

A projectile has

constant horizontal velocity and

constant vertical acceleration.

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4
Q

What is meant by terminal velocity?

A

When a falling object (e.g. a skydiver) accelerates, the air resistance acting against the object increases, until it is balanced with the object’s weight. When the forces are balanced, it will travel at a constant speed (called ‘terminal velocity’).

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5
Q

What does the prefix M stand for?

A

M stands for mega

mega = x 106

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6
Q

What is a star?

A

A star is a sphere of plasma that emits heat and light.

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7
Q

What is the relationship between the altitude of a satellite (height above the Earth) and its period (time taken to complete one orbit of the Earth)?

A

The higher the altitude, the longer the period of the satellite.

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8
Q

What are the different types of wave detected by space telescopes?

A

As well as visible light, space telescopes detect infrared (IR), ultraviolet (UV), X-rays and gamma rays.

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9
Q

What is a moon?

A

A moon is a natural satellite of a planet.

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10
Q

What does the prefix G stand for?

A

G stands for giga

giga = x 109

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11
Q

What is a dwarf planet?

A

A dwarf planet is an object which orbits the Sun but, due its small mass, whose orbit is not uniform enough to be classed as a planet.

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12
Q

What is the unit for weight?

A

The unit for weight is

newtons (N)

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13
Q

What is a galaxy?

A

A galaxy is a group of stars, gases and dust held together by gravity.

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14
Q

Is the mass of an object constant at all points in the universe?

A

Yes. The mass of an object does not change, regardless of the force of gravity.

1kg on Earth would be 1kg on the Moon, 1kg in outer space, and so on.

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15
Q

Describe to calculate one light-year in metres.

A

Use the formula d = v x t :

  • v = 3 x 108 ms-1 (speed of light)
  • t = 1 year (convert into seconds: 365.25 x 24 x 60 x 60)
  • Calculate d
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16
Q

Explain the orbit of a satellite in terms of projectile motion.

A

A satellite is like a projectile: it is travelling ‘forwards’ (horizontally) with a constant velocity, but also accelerating ‘downwards’ (vertically).

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17
Q

Is the weight of an object constant at all points in the universe?

A

No - the weight of an object depends on its mass and the gravitational field strength. Therefore, the weight of an object can vary at different points in the universe.

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18
Q

What is the Sun?

A

The Sun is the star at the centre of our solar system.

19
Q

Use Newton’s 3rd Law to explain how a rocket accelerates.

A

Newton’s 3rd Law is about action and reaction forces.

In a rocket, the rocket pushes the combustion gases downwards, and the gases push back up against the rocket (causing it to accelerate).

20
Q

What does the prefix m stand for?

A

m stands for milli

milli = x 10-3

21
Q

What is a solar system?

A

A solar system is a collection of objects orbiting a star.

22
Q

What is a projectile?

A

A projectile is an object which is moving only under the influence of gravity.

(assume that air resistance is negligible)

23
Q

What name is given to this pattern, produced when a source of white light is viewed through a spectroscope?

A

When white light is viewed through a spectroscope, a continuous spectrum is produced.

24
Q

Describe some of the risks of space exploration.

A
  • Astronauts can be exposed to a high level of radiation, without the Earth’s atmosphere to absorb some of the cosmic rays
  •  Space is a vacuum, and so there is a large difference in pressure between the inside of a spacecraft (or spacesuit) and outside
  • Astronauts’ bodies can suffer loss of muscle mass and weakening of bones due to weightlessness whilst in orbit
  •  Re-entry to a planet’s atmosphere creates a large amount of heat due to air resistance. Thermal protection systems must be used to ensure the spacecraft is protected on re-entry.
  •  The angle of re-entry must be precisely calculated so the spacecraft doesn’t ‘bounce off’ the atmosphere.
25
What is meant by the '**observable universe**'?
The furthest point in space that we can see is the distance light must have travelled for the whole age of the universe. This distance is called the 'observable universe'.
26
Name the three quantities shown in this formula.
F = unbalanced force m = mass a = acceleration
27
Describe some of the **benefits** of **space exploration**.
Space exploration has helped to develop ## Footnote *  The accuracy of weather forecasting *  Telecommunications via satellites *  Analysis of our environment *  National security *  Sat-Nav systems *  Robotics
28
Why are **distances in space** measured in **light-years**?
Distances in space are **vast**. They are too big to be easily understood using metres. A **light-year** is **large enough** to be suitable for describing the distance between objects in space.
29
What name is given to this pattern, produced when certain elements are viewed through a spectroscope?
When elements (in a star, or produced by a discharge lamp) are viewed through a spectroscope, a **line spectrum** is produced.
30
For projectile motion, what is the **only** equation you should use for the **horizontal** part of the motion?
For the **horizontal** part of the motion, the only equation which should be used is
31
What is a **planet**?
A **planet** is an object in orbit around a star.
32
What is an **exo-planet**?
An **exo-planet** is a planet outwith our solar system.
33
What is **Newton's 2nd Law**?
If the **forces** on an object are **unbalanced**, the object will **accelerate** in the direction of the unbalanced force. ## Footnote **F = m x a**
34
What **impact** has **space exploration** had on our **understanding of the universe**?
* Hubble’s deep field lens allows us to capture images across many wavelengths of EM radiation from deep space. * Voyager has performed ‘fly-pasts’ of many objects in our solar system giving up-close, detailed images never seen before. * Spirit analysed the terrain on Mars to help determine if life had ever existed there.
35
What does the prefix **µ** stand for?
**µ** stands for **micro** **micro** = **x 10-6**
36
What is meant by **balanced forces**?
Balanced forces means forces which are the **same size** but in **opposite directions**.
37
What is **Newton's 3rd Law**?
**Newton's 3rd Law** states that **for every 'action' force** there is an **equal but opposite 'reaction' force**.
38
What is an **asteroid**?
An **asteroid** is a small rocky body orbiting the Sun.
39
What does the prefix **k** stand for?
**k** stands for **kilo** **kilo** = **x 103**
40
What is required for a planet to be able to sustain life?
To sustain life, a planet must be within the right temperature range - it must be capable of having liquid water and an oxygen-rich atmosphere.
41
What is the **universe**?
The **universe** is all existing matter and space.
42
What does the prefix **n** stand for?
**n** stands for **nano** **nano** = **x 10-9**
43
In space physics, how do scientists use **line spectra**?
Scientists use **line spectra** to identify the different **elements** present in **stars** and **galaxies**.