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Earth Moon And Our Eyes

Earth Earth is where we stand and is home to living creatures. Of course, living creatures that we know such as humans, animals, plants, fungi, microorganisms and so on. It is from this earth that humans try to study the celestial objects they see. So finally we know that Earth is one of the planets that surrounds the solar system.

Earth is the third planet from the sun, as well as the densest and fifth largest planet of the eight planets that revolve around the sun in the solar system.

The Earth is considered to be a solid sphere with a mean radius of 6.37×1066.37\times 10^6 m. The mass of the earth is expressed by M=r2gGM=\frac{r^2g}{G} where rr represents the radius of the earth, gg is the gravitational acceleration at the earth’s surface, and GG is the general constant of gravity. The mass of the earth if g=9.8g=9.8 and G=6.67×1011NM2kg2G=6.67\times 10^{-11}NM^2kg^2 is:m=r2gG=(6.37×106)2(9.8)6.67×1011=(6.372×1012)(9.8)6.67×1011=(6.372×9.8)×10126.67×1011=397,65362×10126.67×101159,618×10235,96×1024\begin{aligned} m&=\frac{r^2g}{G}\\ &=\frac{(6.37\times 10^6)^2 (9.8)}{6.67\times 10^{-11}}\\ &=\frac{(6.37^2\times 10^{12}) (9.8)}{6.67\times 10^{-11}}\\ &=\frac{(6.37^2\times 9.8)\times 10^{12}}{6.67\times 10^{-11}}\\ &=\frac{397, 65362\times 10^{12}}{6.67\times 10^{-11}}\\ &\approx 59, 618\times 10^{23}\\ &\approx 5, 96\times 10^{24} \end{aligned}So, the mass of the earth is about 5.96×10245.96\times 10^{24} kg.## Calculating the Moon’s Orbital Speed

Month The moon is the earth’s satellite. The moon always rotates around the earth and around the sun.

The orbital speed of the moon is expressed by v=2πrTv=\frac{2\pi r}{T}, where rr represents the average radius and TT represents the time (in seconds) required in one round. The orbital speed of the moon around the Earth with an average radius of 3.84×1083.84\times 10^8 m and taking 2.36×1062.36\times 10^6 seconds to complete one revolution (π=3.14)(\pi=3.14) is:v=2πrT=2(3.14)(3.84×108)2.36×106=6.28(3.84×108)2.36×106=24.1152×1082.36×10610,218×1021.02×103\begin{aligned} v&=\frac{2\pi r}{T}\\ &=\frac{2(3.14) (3.84\times 10^8)}{2.36\times 10^6}\\ &=\frac{6.28 (3.84\times 10^8)}{2.36\times 10^6}\\ &=\frac{24.1152\times 10^8}{2.36\times 10^6}\\ &\approx 10,218\times 10^2\\ &\approx 1.02\times 10^3 \end{aligned}So, the orbital speed of the moon around the Earth is 1.02×1031.02\times 10^3 m/s.## Calculating the Pupil’s Area

Eye Pupils The pupil is in the center of the iris (the part that gives color to the eyes). The function of the pupil is to allow light to enter the eye so that it can be focused on the retina to begin the vision process. In general, the pupils will look perfectly round, the same size and black. The black color occurs because light passing through the pupil is absorbed by the retina and is not reflected back.

When the light is dim, the pupil radius becomes 6×1036\times 10^{-3} m. Using the circle area formula L=πr2L=\pi r^2, the area of ​​the pupil in dim light with a value of π=3.14\pi = 3.14 is: L=πr2=3.14×(6×103)2=3.14×62×106=113.04×106=1,130×104\begin{aligned} L&=\pi r^2\\ &=3.14\times (6\times 10^{-3})^2\\ &=3.14\times 6^2\times 10^{-6}\\ &=113.04\times 10^{-6}\\ &=1,130\times 10^{-4}\\ \end{aligned}So, the area of ​​the pupil in dim light is 1,130×1041,130\times 10^{-4} m. So, I hope this article is useful. If you have criticism, suggestions or improvements, please leave them in the comments. Thank you.😊🙏

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