1. PHY115 – Sault College – Bazlurslide 1 About Science

2. PHY115 – Sault College – Bazlurslide 2 Physics is the study of the rules of nature

3. PHY115 – Sault College – Bazlurslide 3 Science Science is the body of knowledge that –describes the order within nature and –the causes of that order. Science is an ongoing human activity that represents –the collective efforts, –findings, and –wisdom of the human race, an activity that is dedicated to –gathering knowledge about the world and –organizing and condensing it into testable laws and theories.

4. PHY115 – Sault College – Bazlurslide 4 Advancement of Science Science made great headways in Greece in the third and fourth centuries BC. AD -(anno Domini, Latin for "in the year of the Lord") and BC -(Before Christ). Alternative notations are: CE -Common Era and BCE -Before the Common Era 1 100 200 300 400 500 AD AD 1 - birthdate of JesusJesus 1 CE 1BC 1 BCE 500 BC 400 300 200 100 1

5. PHY115 – Sault College – Bazlurslide 5 Advancement of Science Science advance came to a near halt in Europe when the Roman empire fell in the fifth century AD. Chinese & Polynesians were charting stars and planets. Arabs were developing mathematics and learning chemicals. Greek science was reintroduced to Europe by Islamic influences via Spain in 10 th, 11 th and 12 th centuries. Universities emerged in Europe in 13 th centuries. Polish astronomer Nicolaus Copernicus published book proposing that Earth revolves around the sun. Italian physicist Galileo Galilei was arrested for popularizing Copernican’s theory.

6. PHY115 – Sault College – Bazlurslide 6 Scientific Measurements Measurements are a hallmark of good science. How much you know about something is often related to how well you can measure it. Scientific measurements are not something new but go back to ancient times. In the third century BC, for example, fairly accurate measurements were made of the sizes of the Earth, moon, and sun, and the distances between them.

7. PHY115 – Sault College – Bazlurslide 7 Size of Earth The size of earth was first measured in Egypt by Eratosthenes in 235 BC. Eratosthenes reasoned that on June 22 when the Sun is directly overhead, Sun’s ray would pass directly through the centre if extended. Likewise, a vertical line extended into Earth at Alexandria or anywhere would also pass through the Earth’s centre.

8. PHY115 – Sault College – Bazlurslide 8 Size of Earth At noon on June 22, Eratosthenes measured the shadow cast by a vertical pillar in Alexandria and found it to be 1/8 th the height of the piller. This corrsponds to a 7.2  angle between the Sun’s rays and the vertical piller. Since 7.2  is 7.2  /360 , or 1/50 of a circle, Eratosthenes reasoned that the distance between Alexandria and Syene must be 1/50 the circumference of Earth. Thus the circumference becomes 50 time the distance between these two cities. C = 50 x 800 km = 40,000 km And the radius is r = C/2  = 6370 km

9. PHY115 – Sault College – Bazlurslide 9 Size of Earth without degrees Shadow length / piller height = distance between cities / Earth’s radius 1/8 = 800/r And the radius is r = 800 x 8 = 6,400 km Thus the circumference becomes 2  r. C = 2  r = 2 x 3.14 x 6 400 km = 40,192 km The Earth's equatorial radius, is the distance from its centre to the equator equals 6,378.135 km

10. PHY115 – Sault College – Bazlurslide 10 Size of Earth Using conversion factor: conversion relation is 7.2  = 800 km conversion factors are, Circumference is to 360  x = 50 x 800 km = 40,000 km 7.2  800 km 7.2  800 km 7.2 

11. PHY115 – Sault College – Bazlurslide 11 Size of the Moon Aristarchus correctly measured the Moon’s diameter and its distance from Earth in 240 BC. Moon’s diameter = 1/3.5 of Earth’s Diameter = 3640 km  3,476.2 km + 5%

12. PHY115 – Sault College – Bazlurslide 12 Distance to the Moon View a coin with one eye so it just blocks out the full Moon. This occurs when your eye is about 110coin diameters away. Coin dia/coin distance = Moon dia/Moon distance = 1/110 Moon distance = 3476 km x 110 = 382360 km

13. PHY115 – Sault College – Bazlurslide 13 Distance to the Sun Aristarchus also made a measurement of the Earth-Sun distance. Aristarchus measured 20 times the moon’s distance. In fact it is about 400 times. Sun distance  150,000,000 km In December, 147,000,000 km In June, 152,000,000 km

14. PHY115 – Sault College – Bazlurslide 14 Distance to the Sun sin X = opposite / hypotenuse cos X = base / hypotenuse Hypotenuse = base /cos A = distance between moon and earth / cos 87  = distance between moon and earth / 0.05 = distance between moon and earth x 20 opposite base hypotenuse

15. PHY115 – Sault College – Bazlurslide 15 Size of the Sun Coin dia/coin distance = Sun dia/Sun distance = 1/110 Sun distance = 150,000,000 km Sun diameter = Sun distance x 1/110 Sun diameter = 150,000,000/110 = 1,363,636 km

16. PHY115 – Sault College – Bazlurslide 16 Size of the Sun http://curious.astro.cornell.edu/question.php?number=400 http://www.vt-2004.org/Amateurs/aa-brandys/isc-reports/361,1,http://www.vt-2004.org/Amateurs/aa-brandys/isc-reports/361,1

17. PHY115 – Sault College – Bazlurslide 17 Mathematics – the Language of Science Science and Mathematics integrated 4 centuries ago. When the ideas of science are expressed in mathematical terms, they are unambiguous. The equations of science provide compact expressions of relationships between concepts. The equations are guides to thinking that show the connections between concepts in nature.

18. PHY115 – Sault College – Bazlurslide 18 Scientific Methods There is no one scientific method. But there are common features in the way scientists do their work. –Recognize a question – an unexplained fact –Make an educated guess - a hypothesis –Predict consequences of the hypothesis –Perform experiments or make calculations to test the predictions –Formulate the simple general rule that organizes the three main ingredients: hypothesis, predict effects, and experimental findings.

19. PHY115 – Sault College – Bazlurslide 19 Scientific Methods Although these steps are appealing, much progress in science has come from trial and error, experimentation without hypothesis, or just plain accidental discovery by a well- prepared mind. The success of science rests more on an attitude common to scientists than on a particular method. This attitude is one of inquiry, experimentation, and humility – that is, a willingness to admit error.

20. PHY115 – Sault College – Bazlurslide 20 Physics: The Basic Science Science, once called natural philosophy, encompasses the study of living things and nonliving things: –the life sciences and biology, zoology, and botany –the physical sciences. geology, astronomy, chemistry, and physics

21. PHY115 – Sault College – Bazlurslide 21 Physics: The Basic Science Physics is the basic science. It's about the nature of basic things such as motion, forces, energy, matter, heat, sound, light, and the insides of atoms. Chemistry is about how matter is put together, how atoms combine to form molecules, and how the molecules combine to make up the many kinds of matter around us. Biology is more complex and involves matter that is alive. So underneath biology is chemistry, and underneath chemistry is physics. The concepts of physics reach up to these more complicated sciences. That's why physics is the most basic science. An understanding of science begins with an understanding of physics.