70 million years ago it would have had the same angular diameter of … Your answer should be between 30 and 35 arcminutes in diameter. The Moon takes 2 minutes to sink below the horizon at the equator when observed at night (about the same time as the Sun takes to set). As we saw in example 1, the Moon's angular size is 30 minutes of arc which is about the same size that a tennis ball appears at 24 feet. Take a penny and place it in front of your eye, so that it blocks out the moon. The Moons angular size can be converted from radians to arcseconds by multiplying by 206,264. Do you think that the angular size of the Sun is greater or smaller than the angular size of the Moon Now, move the penny away from your eye, until the apparent angular size of the penny is that of the moon. Arcminutes can be found by dividing by 60. It derives the equations necessary. This states that the perceived angular size of the moon is proportional to the perceived angular size of objects around it. This demo shows how to calculate the size of the Moon and the Sun, given angular size and distance. The Moon's elongation is its angular distance east of the Sun at any time. From trigonometry we can derive a simple formula that works for small angles only. Part III: Putting Together Geometry and Observation to Measure the Size of the Moon Aristarchus' observations showed angular size of Earth's shadow at the distance to the Moon ----- = 2.7 angular size of the Moon which meant that R em /R m = 2.7 but since R em = R e - R m. then (R e - R m)/R m = 2.7 and Divide that number into 1.9 cm, which is the diameter of the penny. Angular Size of the Sun. The Moon's angular extent viewed from Earth is small enough that this approximation is adequate for this calculation, so we can simply use the ratio of viewing distances as a proxy for the Moon's angular size. Dividing the apogee distance by that of the perigee gives 405948/359861 = 1.1281, in close agreement with the ratio of image sizes. Angular size has two measurements, the angular distance and the angular diameter. At new moon, it is zero and the Moon is said to be in conjunction.At full moon, the elongation is 180° and it is said to be in opposition.In both cases, the Moon is in syzygy, that is, the Sun, Moon and Earth are nearly aligned.When elongation is either 90° or 270°, the Moon is said to be in quadrature. Elongation. pick a night when the moon is moderately near the horizon. Taking measurements of the angular size of the moon is also determining the angular distance of the two objects. For an observer on the Earth, the angular diameter of the Moon and the Sun are quite similar ( ~ 0.5 o = 30 arcmin).In reality, the Sun’s physical diameter is 400 times bigger than the Moon, while the Moon is ~ 400 times closer to the Earth. So let us add the Sun to the picture. If the radius of th Measure the distance between your eye and the penny in centimeters. At any rate, the Moon would only have been 0.4% closer and look 0.8% bigger. Usually, the mean Moon has the same angular size as an American cent at a distance of 2.051 meters. The angular size can be measured in units of radians, units of degrees, arc minutes (1degree= 60 arc minutes) and arc seconds (one second= 60 arc seconds). And, because the angular sizes of the Moon and the Sun are equal, it is quite reasonable to try finding this equation on the opposite side of the earth’s orbit.

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