
Index
The Sun S3.The Magnetic Sun S3A. Interplanetary Magnetic Fields S4. Colors of Sunlight S4A.Color Expts. Optional: Doppler Effect S4A1 Speed of Light S4A2. Frequency Shift S4A3 Rotating Galaxies and Dark Matter  S5.Waves & Photons Optional: Quantum Physics Q1.Quantum Physics Q2. Atoms Q3. Energy Levels Q4. Radiation from Hot Objects Q5.The Atomic Nucleus and Bohr's Model Q6. Expansion of Bohr's Model Q7.Wave Mechanics Q8. Tunneling  S6.The Xray Sun S7.The Sun's Energy 
IntroductionThis part of "Stargazers" assumes the reader is already familiar with sections
(S4) The Many Colors of Sunlight From here one can continue with sections on the Sun, its energy and related sections on nuclear energy. All these provide a reasonably comprehensive, nonmathematical introduction to solarrelated physics, at the level of high school or beginning college. However... whereas rest of "From Stargazers to Starships" revolves around Newton's laws of motion and their applications, Sunrelated physics is frequently concerned with the physics of the atom and nucleus, where those laws are greatly modified. Like Newtonian mechanics, "quantum mechanics" is a mathematical field, but even its basic applications demand much more mathematics. Its coverage here is therefore very much simplified. Do not expect "Stargazers" to teach you quantum physics: the most these web pages can do is give a quick survey of its origins, and sketch out some basic ideas. You will learn what the main components are, and a bit about the way they evolved, but to do more, you will have to fill those empty boxes with solid, mathematical knowledge. This is optional material: if you skip it and continue, you may still get a fairly coherent picture. Planck's ConstantEinstein's 1905 formula (see here)
was an early indication that on the atomic scale the laws of physics were quite different. Furthermore, it suggested that the new laws were intimately connected with a new physical constant, now known (for reasons discussed below) as "Planck's constant" h. To an accuracy of 6 decimals

Much of the physics of the 20th century involves atomic phenomena, an area rarely covered in high school or beginning college, where studies stress "classical physics" based on the laws of Newton and Maxwell; indeed, with the limited time available in physics classes, even that part of physics is only partially covered. Classical physics is indeed more relevant to most engineering applications. Furthermore, the mathematical tools involved in the "new physics," the mathematics of wave functions, are only taught in classes on advanced calculus (while these sites try to be calculusfree). Thus a gap is almost inevitable. This overview will not close that gap: at most, it can present some of the framework of the physics of the atomic level. As in other parts of "From Stargazers to Starships," here too the pattern is outlined by a history of its discoveries. 
Next Stop: Q2 The Atomic Structure of Matter Or else, return to section #6 on physics related to the Sun: (S6) Seeing the Sun in a New Light Timeline Glossary Back to the Master List
Author and Curator: Dr. David P. Stern 