Inventory of "From Stargazers to Starships"
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Sect. Concepts
1 Celestial sphere and its pole.
Equatorial and altazimuth mounting, coordinates.
2 The ecliptic and the zodiac.
Planets in the sky (also in #1)
2a Sundial construction
3 Seasons of the year and inclination of the Earth's axis.
4 Seasonal changes in the position of the Sun
4a The period of the Moon's orbit and the lunar monthwhy different.
How the moon revolves once a month.
The gravitygradient force on the Moon.
4b Craters of the Moonwhy round, why middle higher.
Loss of atmosphere by the Moon.
5 Latitude and Longitude.
Local and universal time
The International date line
Declination and right ascension, first point in Aries
6 Calendar: solar and sidereal day
Julian and Gregorian calendar
Lunar calendarMetonic and Moslem.
7 Precession of the Earth, shift of pole star
Milankovich theory of ice ages.
8 Longitude and latitude
8a Why existence of horizon suggests the Earth curves.
8b Parallax, and its use estimating distancesto Moon, Stars, outdoors.
9a, 9b Aristarchus and his estimate of the size and distance of the Sun
9c Retrograde motion of inner and outer planets.
Ptolemy's theory of epicycles.
Copernicus modelplanets overtaking or being overtaken.
10 Conic sections
11 Graphs, incl. circle and ellipse in (x,y) coords.
Exampledrawing a specified ellipse.
Ellipse as collection of points with R1+R2 = const.
11a. Ellipse in polar coords. Orbital elements:
Semimajor axis, eccentricity.
Center of motion is not Sun but mutual center of gravity.
12. Intuitive concept of 2nd lawplanet or satellite slows down when further away, relation to conservation of energy and analogy to motion of thrown stone.
12a Example of nonalgebraic equation (Kepler's)
Concept of solving an equation by iteration [see M2 for "Algorithm"]
Idea of orbital inclination, and that 2 more angles are needed to specify the orbit in 3 dimensions.
13 Acceleration, in particular acceleration g of free fall.
14 Concept of vector
vector addition and resolution into components.
15 Energy, kinetic, potential and other kinds. Conversion of energy from one kind to another, special role of heat [in 27, heat engines].
16 Newton's 1st and 3rd laws: steady motion in a straight line, reaction
17 Concept of massgravitational vs. inertial.
18 Concept of equilibrium, and reaction forces in equilibria.
18a. Momentum and its conservation.
19 Centripetal acceleration and force.
20 The force of gravitation and its inversesquares variation.
21 Escape velocity from Earth.
22 Concept of frame of reference: constant motion makes no difference.
22a. The aberration of starlight, comet tails etc.
22b Elementary notions about aerodynamics.
23 Accelerating frames of reference and inertial forces.
Motion in a circle as sensed in rotating frame: the centrifugal force.
24 "Weightlessness" in orbiting spacecraft: gravity is still present.
Coriolis force and inertia, on a rotating space station.
25 Concept of center of gravity
Principle of rocket motion.
26 Ballistic pendulum
DeLaval nozzle as a heat engine, rocket design.
27 Staging of rockets, its reasons. Proportion of fuel in a rocket's weight.
28 Problems of atmospheric reentry, shock wave.
29 (ae) 5 classes of unmanned spacecraft.
30 About using cannon for space launches, need for onboard rocket
32 Solar sails.
33 Solar ion propulsion. Need to neutralize spacecraft.
34 Sun synchronous orbits
Lagrangian points
Escape velocity from the Sun
35 Elastic collisions with moving body can lose or gain energy
Rocket propulsion gains leverage if applied near planet or star.
Sect. Calculations and formulas
2a (formulas for sundialoptional)
2a+ (reason why sundial must point at pole of the heavensoptional)
5a Finding one's lattitude using the pole star
Finding latitude using the noontime Sun
5b Cartesian and polar coordinates, in 2 and 3 dimensions (sine & cosine)
8 Calculation by Erastothenes of the Earth's size.
8a Distance to the horizon (use the theorem of Pythagoras)
8b Derivation of the parsec.
8c Calculation of the distance to the Moon by Aristarchus, using a total lunar eclipse
8d Calculation of the distance to the Moon by Hipparchus, using a total solar eclipse
9a Estimate of the distance and size of the Sun by Aristarchus, and how this might relate to his heliocentric theory.
9b The shadowcone of the Earth.
10 Kepler's laws, formula for the 3rd law and examples from solar system.
11 Graphs of functions in rectangular coordinates. Graph of circle, ellipse.
11a Graphs in polar coordinates. Graph of cosine and
of ellipse, properties of ellipse.
12 Energy, and its conservation in free fall and in planetary motion.
(Mean anomaly, describing motion of a planet).
12a Orbital elements, Kepler's equation.(optional extension)
Mean anomaly.
13 Motion of falling or thrown object.
14 Vector addition and resolution into components
Acceleration down an inclined plane.
15 Equation of energy for falling object and pendulum
Units of energy.
16 Newton's laws.
18 Argument why "F=ma" is by itself meaningless.
Newton's 2nd lawits consistent formulation by Mach.
19 Derivation of centripetal acceler. (using the theorem of Pythagoras).
20 How Newton tied the acceleration g due to gravity to the Moon's period.
21 Orbital and escape velocities.
Kepler's 3rd law for Earth satellites.
21a A practical equation for circular orbits around Earth, applied in 34.
22a Sweepback of airplane wings
Operation of variablepitch propeller on an airplane.
(this item & next illustrate frames of reference and resolution of vectors).
23 Variation of gravity observed from poles to equator. "Loop the loop"
on a roller coaster. Analysis in rotating and static frame.
24 Coriolis force due to Earth's rotation. Estimate effect in bathroom sink.
25 In 2body interaction, center of gravity does not move.
26 Ballistic pendulum, used in determining the speed of a bullet.
27 Kinetic energy which needs to be dissipated in rocket reentry.
30 Acceleration in a cannon for space launches.
Molecular veloc. inside cannon, reason for using hydrogen [also in 31]
34 Lagrangian points L1 and L2 (qualitatively)
34a Calculating distance to L1, circular orbits.(optional)
34b Calculating position of L5, circular orbits.(optional)
35 Elastic collisions between oppositely moving objects (by frames of ref.)
35a Estimate transfer of energy in elastic collision greatest loss when
overtaking object moving at half the speed.
M1 Basic ideas of algebra: (1) unknown numbers can be handled as numbers. (2) Equal operations on both sides of equality create new equality.
M3 Formulasequations can be given only in symbols.
M4 Identities: distributive law and its consequences.
M5 Approximations with small quantities; Newton's binomial theorem.
M6 Theorem of Pythagoras, proof by identities for the square of sum and difference.
M7 Trigonometry: basic application, concept of baseline
M8 Sines and cosines, sums of squares. (tan. & cotan., definition only)
M9 Calculations: sines and cosines of complementary angles, derivation for angles of (30, 60), 45, (0, 90) and (15, 75) degrees.
M10 Sines and cosines past 90 degrees, generalized using polar coordinates. Graph.
M11 Sine and cosine of sum of angles.
Sect. Stories, extensions and illustrating examples
1 Psalm 19
4 Orientation of solar panels
Design of house windows, taking advantage of the Sun's motion.
4a Poem by Vachel Lindsay.
4b The story of exploration of the Moon using space vehicles.
5 Poem by John Masefield
5a Story of search for method to find longitude.
Story of Nansen getting lost, by losing the accurate time.
5b Rene Descartes
6 Lengthening of the day due to tides
Switch from Julian to Gregorian Washington's birthday, October Revolution.
7 Use of eclipses by Hipparchus to discover precession of equinoxes.
The evidence for ice ages on Earth.
The song "Dawning of the age of Aquarius" and its background.
8 Size of Earth as estimated by the ancients and by Columbus.
8a The story of Pike's Peak.
9a Story of Aristarchus, estimating the Sun's distance
and proposing the Earth went around the Sun.
9b Story of Copernicus.
Galileo and his firstever astronomical telescope.
10 Story of Tycho and Kepler
11 Story of focusing of sound in old senate chamber.
11b Search for distant planets by wobble of star's position.
12 Jefferson's clock in Charlottesville.
13 Stories of Galileo and tower of Pisa,
Galileo using slanted board to study ball rolling under gravity
Cartoon depiction of gravity suddenly taking over is incorrect.
The way a gunsight works
Air resistance, and story of astronaut demonstrating free fall on Moon
15 Analogy of energy and money.
Calories in food.
16 Isaac Newton.
Examples of 3rd law: jumping from a boat, balancing a bicycle
17 Why mass explains the reason all bodies fall at the same rate.
Mass in the horizontal motion of a heavy wagon.
Measuring mass on the space station "Skylab," in "zerog." Analogy to the balance spring on a wristwatch.
17a The complete story of mass measurement aboard "Skylab".
18 Roland Eötvös and the equality of gravitational and inertial mass.
(in 27, Eötvös and the high schools of Budapest)
20 Story of Newton's apple.
22a The aberration of starlight and how Bradley solved it.
Aberration of the solar wind, comet tails.
22b Problems of flight near the speed of sound.
24. NASA's simulation of weightlessness on an airplane.
26 History of rocket: Ft. McHenry, Tsiolkovsky, Goddard
Detailed story of Goddard: vision as teen ager. His use of a ballistic pendulum
Introduction of DeLaval nozzle, liquid fueled rocket.
27 History of rocketryin Germany (V2) US. Von Braun, Oberth, Karman.
28 Stories of Sputnik and of Explorers 1 and 3.
29 Manned space flightJohn Glenn, etc.
29a Spacecraft for astronomyHubble, etc. Links to sites.
29b Earthmonitoring spacecraft. Links to sites.
29c Spacecraft observing the Earth's outer environment. Links to sites.
29d Commercial use of spacecomsats, GPS. Links to sites.
29e Planetary and lunar exploration by spacecraft. Links to sites.
30 The SHARP cannon at Livermore National Lab.
30a The HARP cannon and the story of Gerald Bull.
31 The NERV and Rover nuclear rocket projects.
"Project Orion"spaceship propulsion by nuclear bombs.
32 Solar sail projects.
Robert Forward's visionary laserdrive space sail.
32a Using light pressure for stationkeeping beyond L1 Lagrangian pt.
33 Solar ion enginesDS1 mission, XIPS engine.
34 Energy gain of "Voyager", ISEE3 etc. from close encounters.
35a Story of Lester Pelton and his turbinerelate to Calif. gold rush.
NASA's solar probe mission.
M2 History of algebra: AlKhorezmi.
M6 Story of how the height of Mt. Everest was first measured.
M7 Origin of word "sine."
