Tauragės „Versmės“ gymnasium Moon’s diameter calculation Justinas Jorudas IIIe 2012 Introduction The moon is Earth's closest celestial neighbor. It has a huge influence upon our lives, governs the tides and is responsible for eclipses. The moon lies, on average, 384,400 km (238,900 miles) away and takes 27.3 days to orbit the Earth. Strange as it may seem, its rotation period is exactly the same as its orbital period, something that scientists call tidally locked. Therefore, one half is always facing the Earth while the other half is always facing away. Objective To calculate moon diameter using DIY tools and simple math. Tools DYI cross-staff, tripod. Cross-staff Cross-staff is a simple device, used centuries before the invention of the telescope to determine the angular separation between two objects, or the angular size of a single object. If you are measuring single object, cross-staff can be use to determine its linear size or distance. The cross staff consists of meter stick and a crosspiece attached at a right angle. All you have to do is sight an abject along the stick and slide the crosspiece back and forth until the apparent or angular size of the crosspiece matches the apparent or angular size of the distant object. Since we are only going to measure the diameter of the moon, we can make a very simple device. Take a small empty rectangular box. Then cut a slot at the bottom of the middle of each of the longer sides. Make these slots the same size as the height and width of a meter stick that you happen to have (If done right, you will have something that slides smoothly up and down meter stick.) Take a thin piece of a cardboard and make a nice, neat hole in the center of it. (5-7mm) Tape this to the box bottom that slides up and down meter stick. In my case, I manufactured everything from wood. My slider: Meter stick: My cross-staff: To do Make a Moon measuring device, as described above. Using a millimeter ruler, as accurately as you can measure the diameter (d’) of your hole that will be used for sighting. Now go outside on a reasonably clear night, when the Moon is up and match moon size with your sighting holes size, while cross-staff is up against your cheekbone. Make sure you write down the distance from meter stick’s end (from that end which you were looking) to sighting hole. This distance will be D’. Calculation Using properties of similar triangles, we can measure distance to the moon if we know diameter or vice versa. 𝒅′ 𝑫′ 𝒅 =𝑫 In this formula d’ is diameter of your sighting hole, D’ is distance you wrote down earlier from your sightings, d - is diameter of Moon, D – distance to Moon. I know that distance to Moon is 385304 km. (according to Wofram|Apha data). So: 𝒅= 𝒅′ × 𝑫 𝑫′ 𝒅= 𝟖𝒎𝒎 × 𝟑𝟖𝟓𝟑𝟎𝟒𝟎𝟎𝟎𝟎𝟎𝟎 𝒎𝒎 𝟖𝟗𝟎 𝒎𝒎 𝒅 = 𝟑𝟒𝟔𝟑, 𝟒𝟎𝟔 𝒌𝒎