You should read Can You See
Your Moon before
you read this page.
When you see a moon in the sky, what
you see is affected by
- the actual size of the moon
- how far away the moon is
Just as on earth, a big object very
far away looks small. A small, distant moon may look like a dot
of light, like a star.
Here is a table that Dr Viau has made
for you to help you to understand what we are getting at here.
We see that when the Tangent of Theta
has more than 3 zeros right after the decimal, we get a dot of
light in the sky. You may see the dot moving, like a planet,
but you will not get exciting moon effects with this satellite.
| Earth to |
Distance
from Sun km |
Distance from Earth km |
Diameter km |
Diameter
Distance |
Tangent of Theta |
Viewing
Angle |
We
see |
| Moon |
|
384,400 |
3476 |
3476
384,400 |
0.009 |
0.5 |
Disk |
| Mercury |
57,910,000 |
91,690,000 |
4880 |
4880
91,690,000 |
0.00005 |
0.003 |
dot |
| Venus |
108,200,000 |
41,400,000 |
12,104 |
12,104
41,400,000 |
0.00029 |
approx.
0.02 |
bright
dot |
| Mars |
227,940,000 |
78,340,000 |
6794 |
6794
78,340,000 |
0.0001 |
|
dot |
| Jupiter |
778,330,000 |
628,730,000 |
142,984 |
142,984
628,730,000 |
0.00023 |
approx 0.02 |
bright
dot |
| Saturn |
1,429,400,000 |
1,279,800,000 |
120,536 |
120,536
1,279,800,000 |
0.00009 |
|
dot |
| Uranus |
2,870,990,000 |
2,721,390,000 |
51,118 |
51,118
2,721,390,000 |
0.00002 |
|
dot |
| The Sun |
|
149,600,000 |
1,390,000 |
1,390,000
149,600,000 |
.00929 |
approx. 0.5 |
Disk |
Click here for the Tangent Table

We see that on earth the moon and the sun appear to be about
the same size even though the sun is actually much, much bigger.
However, the sun in also much farther away. During a solar
eclipse, the moon just about covers the sun, as in this picture.
How
can you get the biggest possible moon in your sky?
You will need to study orbits
and The Roche Limit to find out!
Then check out this page about Big
Moons!
Here is something else to think about.
This is a diagram of our moon, which is 0.5 degrees of viewing
angle across.
What happens if we make a moon that has a viewing angle
only half the size of our moon?
This moon would look as if it had half the diameter
of our moon.
You can see that half the diameter is not the
same as half the moon!
Actually, you only get a quarter of the area (disk
surface).
Your moon is going to look quite a bit
smaller in
the sky.
It will not give as much light.

Here I cut the viewing angle into fifths!
Look at the tiny little moons I got!
Each one has only one 25th the area of our moon.
Would these little moons look any different from bright stars?
What About
the Albedo?
The albedo measures how much light an object
reflects.
Example: a mirror
reflects nearly all the light that falls on it: the albedo of
a mirror is perhaps 0.96, which is nearly one.
Example:
a black sweater, which is dark and
rough, reflects very little light. Its albedo might be 0.05.
The numbers that describe albedo go
from 0 (no light reflected)to 1 (all light reflected).
Remember that planets and moons shine
by reflected light. A planet or moon with high albedo
will shine brightly, but it will not look any larger than it
would if its albedo were low.
|
These two moons are the same size
and the same distance from a star.
They both receive the same amount of light. |
|
This is a high albedo moon. |
This is a low albedo moon. |
 |

|
|
A moon or planet with high
albedo:
- shines brightly
- can be seen for a long distance
|
A moon or planet with low albedo
- does not reflect much light
- can be seen close up but soon gets dim
|
Example: Venus
has an albedo of 0.7 (This means it sends back about 70% of the
light that falls on it.) It is the brightest planet, and easily
seen in the sky. However, its viewing angle is small, and it
looks like a bright dot in the sky.
Example: Our moon
has an albedo of only 0.02, which is about 2% of all the light
that it receives from the sun. The moon seems bright to us because
we are close to it.
©
2000, 2003. Elizabeth Anne Viau.
All rights reserved. This material may be used by individuals
for instructional purposes but not sold. Please inform the author
if you use it at eviau@earthlink.net. |