Measuring the Diameters of the Moon at Perigee and Apogee

In summary, the conversation discusses measuring the diameters of the Moon at perigee and apogee, and using this information to determine the ratio between the two distances and the eccentricity of the Moon's orbit. The formula e = (1-b^2/a^2)^0.5 is mentioned, but there is confusion about how it relates to the problem. The speaker also suggests double checking the measurements.
  • #1
crystalplane
11
0

Homework Statement



the image below shows the Moonat perigee and apogee. Measure the diameters for the two, and determine the ratio between perigee and apogee idstance.Based on your result, what is the eccentricity of the Moon'orbit? Compare your value with the Moon' s mean orbital eccentricity(e= 0.0549)

Homework Equations


i have already measured diameters of apogee and perigee, 6.00cm and 13.00 cm(i am not sure about these two numbers.)


The Attempt at a Solution


based on the formula e= (1-b^2/a^2)^0.5,where b is the sei-minor axis...i am very confused about this question.
any help is appreciated.
 
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  • #2
You need to find a formula that relates eccentricity to apogee and perigee rather than to the semi-major and semiminor axi. (Or find a formula that relates the apogee and perigee to the semi-major and semi minor axi.)

I'd also double check your measurements. (they seem a bit off to me.)
 
  • #3


I would first clarify the measurements provided in the problem statement. Are the measurements in centimeters or another unit? Are the measurements accurate and precise? It is important to have accurate and precise measurements in order to calculate the eccentricity of the Moon's orbit.

Assuming the measurements are in centimeters, the ratio between the diameters at perigee and apogee would be 13.00cm/6.00cm, or approximately 2.17. However, this ratio alone does not provide enough information to determine the eccentricity of the Moon's orbit.

To calculate the eccentricity, we need to know the semi-major axis (a) and semi-minor axis (b) of the Moon's orbit. These values can be calculated using the measured diameters and the formula for the eccentricity of an ellipse (e= c/a, where c is the distance from the center of the ellipse to one of its foci).

Without knowing the values for a and b, it is not possible to accurately determine the eccentricity of the Moon's orbit. However, we can compare the calculated eccentricity with the Moon's mean orbital eccentricity (e= 0.0549). If the calculated eccentricity is significantly different from the mean value, it could indicate that the measurements were not precise or that there are other factors affecting the Moon's orbit. Further analysis and data collection would be needed to accurately determine the eccentricity of the Moon's orbit.
 

1. How do you measure the diameter of the Moon at perigee and apogee?

The diameter of the Moon at perigee and apogee is measured using a technique called lunar laser ranging. This involves sending a laser beam from Earth to reflect off of retroreflectors placed on the Moon's surface by previous Apollo missions. The time it takes for the laser beam to travel back to Earth is measured and used to calculate the distance between the two objects. By measuring the distance at different points in the Moon's orbit, scientists can determine the diameter of the Moon at perigee and apogee.

2. Why is it important to measure the diameter of the Moon at perigee and apogee?

Measuring the diameter of the Moon at perigee and apogee allows scientists to better understand the Moon's orbit and its relationship with Earth. This information can also be used to refine lunar and Earth-based navigation systems, as well as improve our understanding of lunar tides and the Moon's influence on Earth's rotation.

3. How often do the Moon's diameter measurements change at perigee and apogee?

The distance between the Moon and Earth changes constantly due to the Moon's elliptical orbit, so the diameter measurements at perigee and apogee also change. However, the difference in diameter between perigee and apogee is relatively small, with a maximum difference of about 14%.

4. Can other methods be used to measure the diameter of the Moon at perigee and apogee?

Yes, there are other methods that can be used to estimate the diameter of the Moon at perigee and apogee. These include using telescopes and cameras to measure the apparent size of the Moon in the sky, or using radar measurements to determine the distance between Earth and the Moon. However, lunar laser ranging is considered the most accurate method.

5. How does measuring the diameter of the Moon at perigee and apogee help in studying other celestial objects?

Measuring the diameter of the Moon at perigee and apogee can provide valuable information for understanding the orbits and sizes of other celestial objects. By comparing the Moon's orbit and diameter to other objects, scientists can gain insights into the formation and evolution of our solar system and the universe as a whole.

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