



Study with the several resources on Docsity
Earn points by helping other students or get them with a premium plan
Prepare for your exams
Study with the several resources on Docsity
Earn points to download
Earn points by helping other students or get them with a premium plan
Community
Ask the community for help and clear up your study doubts
Discover the best universities in your country according to Docsity users
Free resources
Download our free guides on studying techniques, anxiety management strategies, and thesis advice from Docsity tutors
Instructions on how to estimate the size and distance of the Earth and the Moon using ancient mathematical techniques. It includes examples of how Eratosthenes and Thales estimated the Earth's diameter and the distance to the Moon, respectively. It also explains Aristarchus' method for estimating the Earth-Moon distance and the Earth-Sun distance.
What you will learn
Typology: Exams
1 / 7
This page cannot be seen from the preview
Don't miss anything!
CSUN Math How big? How far?
¶ 1. What is the diameter of the Earth? What is the radius of the Earth? Of course, you can Google this numbers in no time. But you can arrive at a rather precise estimate using readily available information and some elementary mathematics. For example:
CSUN Math How big? How far?
¶ 2. The first estimate of the diameter of the Earth of which we have records today was done by Eratosthenes of Cyrene (276-194 B.C.). He knew that at certain time of the year (midday of June 21 by our current calenders) in the ancient town of Syene the light rays of the sun felt straight down on the Earth, the sun made no shadow. However, at that say time, in Alexandria, which is straight north from Syene, the shadow at noon made an angle of about 1/50 of a full circle.
S
A
Eratosthenes Of Cyrene
CSUN Math How big? How far?
¶ 4. It may now seen obvious that to estimate the distance from the earth to the Moon we should estimate the angle difference between to points on the surface of the Earth, like two cities a few miles apart. Unfortunately, the angles are so small that the resulting errors in measurement are too big to have any value. However, Aristarchus of Samos (310-230 B.C.) came up with a novel idea for estimating the distance from the Earth to the Moon. By observing lunar eclipses and carefully measuring how long it took for the Moon to travel under the shadow of the Earth, he was able to determine that the diameter of the Earth was about three and a half times the diameter of the Moon.
Aristarchus of Samos
You may produce a “lunar eclipse” by holding a coin in front of you so as to cover the Moon exactly. A little experimentation will show you that You can exactly cover the whole Moon with a quarter held about 9 feet in front of you.