Question 1
[Maximum number: 3]
Question (a)
(a)
State the equation that defines the average orbital speed v of a planet. State the meaning of any symbols you use.
[ 2 ]v=2πr/T
r= (average) radius of the orbit AND T= (orbital) period
Question (b)
(b)
Suggest why countries that are a significant distance from the Equator experience significant temperature variation throughout the year.
[ 1 ]rays from Sun strike the country at different angles through the year
OR
rays from Sun strike the country for different number of hours per day through the year
Question 2
[Maximum number: 6]
Question (a)
(a)
Fig. 10.1 represents different positions A-H of the Moon as it rotates around the Earth.
[ 3 ]Question (i)
(i)
State a position of the Moon where an observer on Earth sees:
1. there is a quarter Moon
2. there is a full Moon
[ 2 ]position A and / or E
position G
Question (ii)
(ii)
State the approximate time taken for the Moon to orbit the Earth.
time =..........................................................
[ 1 ]Question (b)
(b)
The average distance of the Earth from the Sun is 1.5×108 km.
[ 3 ]Question (i)
(i)
Calculate the average orbital speed of the Earth in km / h.
average orbital speed = km/h [3]
[ 3 ]110000( km/h)(v=)2πr/TT=365×24 h OR 2π×1.5×108/365×24
Question 3
[Maximum number: 1]
It is summer in the northern hemisphere of the Earth in June.
Which statement explains why?
AThe Earth is closer to the Sun in June.
BThe Earth spins on its axis in the opposite direction to that in which it rotates around the Sun.
CThe Moon is full in June.
DThe north pole of the axis of the Earth's rotation is tilted towards the Sun in June.
Question 4
[Maximum number: 1]
Suggest why countries that are a significant distance from the Equator experience significant temperature variation throughout the year.
rays from Sun strike the country at different angles through the year
OR
rays from Sun strike the country for different number of hours per day through the year
Question 5
[Maximum number: 3]
The average distance of the Earth from the Sun is 1.5×108 km.
Calculate the average orbital speed of the Earth in km / h.
average orbital speed = km/h [3]
110000( km/h)(v=)2πr/TT=365×24 h OR 2π×1.5×108/365×24
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