Internet Project
Simultaneously Photographing of the Moon
and Determing its Distance
Solutions
Detailed Problems
-
Consider, for instance, December 9th, 2000, 21.00 UT:
-
In an astronomical almanach for amateurs, you may find:
|
date |
rectascension |
declination |
| Jupiter |
December 5th |
4h14min |
20.3° |
|
December 10th |
4h11min |
20.2° |
|
December 9th (calc.) |
4h11min |
20.2° |
| Saturn |
November 30th |
3h40min |
17.2° |
|
December 15th |
3h35min |
16.9° |
|
December 9th (calc.) |
3h37min |
17.0° |
You can find the calculated values by linear interpolation.
-
With an astronomical computer program you can find the following values:
|
rectascension |
declination |
| Jupiter |
4h11min 4.7s |
62.770° |
20°10'51" |
20.181° |
| Saturn |
3h36min28.7s |
54.120° |
17°00'55" |
17.017° |
-
Determination of angular distances
-
Measurement of the angular distance between Jupiter and Saturn:
-
Calculation of the angular distance between Jupiter and Saturn:
-
For the use of Pythagoras' theorem, you have to take into account the spherical
kind of the coordinates by multiplying the rectascension
alpha
by the cosine of the declination delta.
The angular distance d can therefore be calculated by
d2 = (alpha*cos(delta))2 + delta2.
By this way, you will get the following result:
dJupiter, Saturn = 8.86°
-
Using spherical trigonometry, you have to use the "theorem for the cosines
of sides" ("Seitencosinussatz", in German, I don't know the English terminus!):
| cos(d) |
= |
cos(90°-deltaJ)*cos(90°-deltaS)+ |
|
|
sin(90°-deltaJ)*sin(90°-deltaS)* cos(alphaJ-alphaS) |
|
= |
sin(deltaJ)*sin(deltaS)+ |
|
|
cos(deltaJ)*cos(deltaS)*cos(alphaJ-alphaS) |
Using this formula, you get the following result:
dJupiter, Saturn = 8.79°,
i.e., with an accuracy of about one promille, the same result as above!
-
For instance, we will now evaluate the two pictures taken from Koblenz
and Namibia at 21.00 UT.
k.jpg) |
k.jpg) |
| Koblenz |
Namibia |
With an arbitrary graphic program (PhotoStudio, for instance),
you can determine the pixel coordinates of Jupiter, Saturn and the moon:
| |
|
x
|
y
|
d (J - S)
|
|
Koblenz
|
Jupiter
|
263
|
272
|
342,18
|
| |
Saturn
|
605
|
261
|
| |
moon
|
540
|
166
|
|
Namibia
|
Jupiter
|
507
|
226
|
416,83
|
| |
Saturn
|
92
|
265
|
| |
moon
|
186
|
320
|
Therefore, the scales of the pictures are:
| Koblenz |
0,0257 o/Pixel |
| Namibia |
0,0211 o/Pixel |
-
With the scales known, the angular distances between
the moon and either planets follow immediately from the above pixel coordinates:
| |
d (m - J)
|
d (m - S)
|
| |
pixels
|
degrees
|
pixels
|
degrees
|
|
Koblenz
|
296,59 |
7,62 |
115,11 |
2,96 |
|
Namibia
|
334,48 |
7,06 |
108,91 |
2,30 |
-
Determination of the moon´s parallactic displacement:
-
- With ruler and compasses:
You can draw the either triangles into the same drawing scaled 1o/
cm, for instance.
This construction is in good coincidence with the
combinated picture in
our evaluation document.
By measuring the distance
of the either positions of the moon one gets the following result:
The moon's parallactic displacement due to Koblenz and Namib desert:
1,2°
The distance between the observers:
-
On the large 21.00 UT
picture of the earth Koblenz and Windhoek have the following pixel
coordinates:
|
x |
y |
d |
| Koblenz |
322 |
165 |
459 |
| Windhoek |
351 |
623 |
-
Because of
the earth´s diameter of 768 pixels the distance, therefore, is
-
d (Koblenz, Namibia) = 1.195 RE = 7619 km
-
This value
means the projection of the distance as seen by the moon.
- Our globe has a perimeter of 105.5 cm. For the length of the piece of
string connecting Koblenz and Windhoek we meassured 21.8 cm. The angular
distance between the either locations is, therefore:
-
delta = 360°*21.8/105.5 = 74.4o.
The straight line connecting them, therefore, has the length
-
d = 2 RE sin (delta/ 2) =
1.209RE=7709 km
- The geographical coordinates are
|
latitude |
longitude |
| Koblenz |
50o11´02´´ N |
07o32´16´´ E |
| Namib Desert |
22o28´43´´ S |
14o56´59´´ E |
With the formula given in 2. b. ii. we get the following angular distance:
-
delta = 73.0o .
-
Therefore, the straight distance is
-
d = 1.190 RE = 7588 km.
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last update: January 10th, 2020