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THE SOLAR SYSTEM
A scale model. The scale
Fran J. García Gil
Our objective: To make a scale model of the solar system using one of the wall of our
class. In order to work in this way, we have to work in two phases:
PHASE I: Calculate distances between the sun and the planets (orbit radius)
PHASE II: Represent a scale model of sun and the planets (the scale we will use here will be
different).
PHASE I: Distances between sun and the planets.
We have a wall of 8.9 m in the class, and the largest distance we want to represent is
30.06 AU (Astronomical Units).
Question 1: How many meters do we need to represent one AU
8.9m÷30.06 AU =0.30m every AU
Question 2: Investigate (Internet) the distance from the sun to the rest of the planets.
Question 3: Try to complete the following table:
Planet Real distance (AU) Class distance
Mercury 0.39
Venus 0.72
Earth 1
Mars 1,52
Jupiter 5,2
Saturn 9,54
Uranus 19,22
Neptune 30,06
PHASE II: Planet sizes
If we used the same scale we used for the distances between planets, we had a radium
for sun of 0.00459 AU. So, it will be better for us to chose another scale.
For example, Sun Radius could be 1.25 m. The problem now is, what will be the radius of
every planet?
Let's think. Sun real radius is 695,000 km. So, if we are going to make a sun wtih a radius of
1.25 m = 125 cm, every km is transformed into:
Question 1: How many real km are in 1 cm of the representation?
695,000km÷125cm=5560 km/cm
Question 2: How many cm do we need to represent a real km
125cm/695,000km=0.000180cm/ km
Question 3: Investigate (Internet) the radius of every planet.
Question 4: Try to complete the following table:
Planet Real diameter (km) Real radius (km) Class radius (cm)
Sun 695
Mercury 4878
Venus 12104
Earth 12576
Mars 6787
Jupiter 142800
Saturn 120000
Uranus 51118
Neptune 49528
To be continued... with the mathematical use of scales

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101113 build solarsystem

  • 1. THE SOLAR SYSTEM A scale model. The scale Fran J. García Gil Our objective: To make a scale model of the solar system using one of the wall of our class. In order to work in this way, we have to work in two phases: PHASE I: Calculate distances between the sun and the planets (orbit radius) PHASE II: Represent a scale model of sun and the planets (the scale we will use here will be different). PHASE I: Distances between sun and the planets. We have a wall of 8.9 m in the class, and the largest distance we want to represent is 30.06 AU (Astronomical Units). Question 1: How many meters do we need to represent one AU 8.9m÷30.06 AU =0.30m every AU Question 2: Investigate (Internet) the distance from the sun to the rest of the planets. Question 3: Try to complete the following table: Planet Real distance (AU) Class distance Mercury 0.39 Venus 0.72 Earth 1 Mars 1,52 Jupiter 5,2 Saturn 9,54 Uranus 19,22 Neptune 30,06 PHASE II: Planet sizes If we used the same scale we used for the distances between planets, we had a radium for sun of 0.00459 AU. So, it will be better for us to chose another scale. For example, Sun Radius could be 1.25 m. The problem now is, what will be the radius of every planet? Let's think. Sun real radius is 695,000 km. So, if we are going to make a sun wtih a radius of 1.25 m = 125 cm, every km is transformed into: Question 1: How many real km are in 1 cm of the representation? 695,000km÷125cm=5560 km/cm
  • 2. Question 2: How many cm do we need to represent a real km 125cm/695,000km=0.000180cm/ km Question 3: Investigate (Internet) the radius of every planet. Question 4: Try to complete the following table: Planet Real diameter (km) Real radius (km) Class radius (cm) Sun 695 Mercury 4878 Venus 12104 Earth 12576 Mars 6787 Jupiter 142800 Saturn 120000 Uranus 51118 Neptune 49528 To be continued... with the mathematical use of scales