Durchmesser der Sonne
About points...
We associate a certain number of points with each exercise.
When you click an exercise into a collection, this number will be taken as points for the exercise, kind of "by default".
But once the exercise is on the collection, you can edit the number of points for the exercise in the collection independently, without any effect on "points by default" as represented by the number here.
That being said... How many "default points" should you associate with an exercise upon creation?
As with difficulty, there is no straight forward and generally accepted way.
But as a guideline, we tend to give as many points by default as there are mathematical steps to do in the exercise.
Again, very vague... But the number should kind of represent the "work" required.
When you click an exercise into a collection, this number will be taken as points for the exercise, kind of "by default".
But once the exercise is on the collection, you can edit the number of points for the exercise in the collection independently, without any effect on "points by default" as represented by the number here.
That being said... How many "default points" should you associate with an exercise upon creation?
As with difficulty, there is no straight forward and generally accepted way.
But as a guideline, we tend to give as many points by default as there are mathematical steps to do in the exercise.
Again, very vague... But the number should kind of represent the "work" required.
About difficulty...
We associate a certain difficulty with each exercise.
When you click an exercise into a collection, this number will be taken as difficulty for the exercise, kind of "by default".
But once the exercise is on the collection, you can edit its difficulty in the collection independently, without any effect on the "difficulty by default" here.
Why we use chess pieces? Well... we like chess, we like playing around with \(\LaTeX\)-fonts, we wanted symbols that need less space than six stars in a table-column... But in your layouts, you are of course free to indicate the difficulty of the exercise the way you want.
That being said... How "difficult" is an exercise? It depends on many factors, like what was being taught etc.
In physics exercises, we try to follow this pattern:
Level 1 - One formula (one you would find in a reference book) is enough to solve the exercise. Example exercise
Level 2 - Two formulas are needed, it's possible to compute an "in-between" solution, i.e. no algebraic equation needed. Example exercise
Level 3 - "Chain-computations" like on level 2, but 3+ calculations. Still, no equations, i.e. you are not forced to solve it in an algebraic manner. Example exercise
Level 4 - Exercise needs to be solved by algebraic equations, not possible to calculate numerical "in-between" results. Example exercise
Level 5 -
Level 6 -
When you click an exercise into a collection, this number will be taken as difficulty for the exercise, kind of "by default".
But once the exercise is on the collection, you can edit its difficulty in the collection independently, without any effect on the "difficulty by default" here.
Why we use chess pieces? Well... we like chess, we like playing around with \(\LaTeX\)-fonts, we wanted symbols that need less space than six stars in a table-column... But in your layouts, you are of course free to indicate the difficulty of the exercise the way you want.
That being said... How "difficult" is an exercise? It depends on many factors, like what was being taught etc.
In physics exercises, we try to follow this pattern:
Level 1 - One formula (one you would find in a reference book) is enough to solve the exercise. Example exercise
Level 2 - Two formulas are needed, it's possible to compute an "in-between" solution, i.e. no algebraic equation needed. Example exercise
Level 3 - "Chain-computations" like on level 2, but 3+ calculations. Still, no equations, i.e. you are not forced to solve it in an algebraic manner. Example exercise
Level 4 - Exercise needs to be solved by algebraic equations, not possible to calculate numerical "in-between" results. Example exercise
Level 5 -
Level 6 -
Question
Solution
Short
Video
\(\LaTeX\)
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Don't forget to subscribe to our channel, like the videos and leave comments!
Exercise:
Wie konnte man erstmals den Durchmesser der Sonne bestimmen?
Solution:
Sonnenfinsternisse haben die Menschen schon immer beeindruckt -- Teil ihrer Faszination beruht gerade darauf dass der Mond die Sonne nahezu perfekt abdeckt. Dieser schon sehr lange bekannte Fakt konnte zu Zeiten von Aristarchos von Samos v.Chr. dazu verwet werden die Grösse der Sonne zu bestimmen nachdem vorher der Abstand ErdMond dMO der Abstand ErdSonne dSO und die Grösse des Mondes rMO Radius bestimmt worden waren. Dann gilt simpler Strahlensatz: fracr_SunIndexr_MoonIndex fracd_SunIndexd_MoonIndex r_SunIndex fracd_SunIndexd_MoonIndex r_MoonIndex fracdSdM rM rS
Wie konnte man erstmals den Durchmesser der Sonne bestimmen?
Solution:
Sonnenfinsternisse haben die Menschen schon immer beeindruckt -- Teil ihrer Faszination beruht gerade darauf dass der Mond die Sonne nahezu perfekt abdeckt. Dieser schon sehr lange bekannte Fakt konnte zu Zeiten von Aristarchos von Samos v.Chr. dazu verwet werden die Grösse der Sonne zu bestimmen nachdem vorher der Abstand ErdMond dMO der Abstand ErdSonne dSO und die Grösse des Mondes rMO Radius bestimmt worden waren. Dann gilt simpler Strahlensatz: fracr_SunIndexr_MoonIndex fracd_SunIndexd_MoonIndex r_SunIndex fracd_SunIndexd_MoonIndex r_MoonIndex fracdSdM rM rS
Meta Information
Exercise:
Wie konnte man erstmals den Durchmesser der Sonne bestimmen?
Solution:
Sonnenfinsternisse haben die Menschen schon immer beeindruckt -- Teil ihrer Faszination beruht gerade darauf dass der Mond die Sonne nahezu perfekt abdeckt. Dieser schon sehr lange bekannte Fakt konnte zu Zeiten von Aristarchos von Samos v.Chr. dazu verwet werden die Grösse der Sonne zu bestimmen nachdem vorher der Abstand ErdMond dMO der Abstand ErdSonne dSO und die Grösse des Mondes rMO Radius bestimmt worden waren. Dann gilt simpler Strahlensatz: fracr_SunIndexr_MoonIndex fracd_SunIndexd_MoonIndex r_SunIndex fracd_SunIndexd_MoonIndex r_MoonIndex fracdSdM rM rS
Wie konnte man erstmals den Durchmesser der Sonne bestimmen?
Solution:
Sonnenfinsternisse haben die Menschen schon immer beeindruckt -- Teil ihrer Faszination beruht gerade darauf dass der Mond die Sonne nahezu perfekt abdeckt. Dieser schon sehr lange bekannte Fakt konnte zu Zeiten von Aristarchos von Samos v.Chr. dazu verwet werden die Grösse der Sonne zu bestimmen nachdem vorher der Abstand ErdMond dMO der Abstand ErdSonne dSO und die Grösse des Mondes rMO Radius bestimmt worden waren. Dann gilt simpler Strahlensatz: fracr_SunIndexr_MoonIndex fracd_SunIndexd_MoonIndex r_SunIndex fracd_SunIndexd_MoonIndex r_MoonIndex fracdSdM rM rS
Contained in these collections
| Title | Creator | Matched on |
|---|---|---|
| Masse der Erde | uz | tags |
| Entfernung der Sonne | uz | tags |
| Durchmesser des Mondes | uz | tagstitle |
| Entfernung des Mondes | uz | tags |
| MC Mondphase | uz | tags |
Similar exercises (22)
| Title | Creator | Matched on |
|---|---|---|
| Masse der Erde | uz | tags |
| Entfernung der Sonne | uz | tags |
| Durchmesser des Mondes | uz | tagstitle |
| Entfernung des Mondes | uz | tags |
| MC Mondphase | uz | tags |
| MC Abnehmender Mond | uz | tags |
| MC Zunehmender Mond | uz | tags |
| MC Mondphase | uz | tags |
| MC Ebbe und Flut | uz | tags |
| MC Jahreszeit | uz | tags |
| MC Ebbe und Flut Zeitverschiebung | uz | tags |
| MC Jahreszeit | uz | tags |
| MC Ebbe und Flut Zeitdauer | uz | tags |
| MC Ebbe und Flut | uz | tags |
| MC Satellit | uz | tags |
| MC Ebbe und Flut | uz | tags |
| MC Jahreszeit | uz | tags |
| Umlaufzeit | uz | tags |
| Irdisches Wasser, Sonne und Mond | uz | tags |
| Ebbe und Flut | uz | tags |
| Mond und Erde | uz | tags |
| Mondgesicht | uz | tags |

