Introduction to the Solar System


APAS 1110 Summer 1996

Lecture 2 -- Deep Distance

Tuesday June 4



  • What did the ancients see in the sky?

    Most of the stars rotate about in the sky, rising in E, setting in W
    Stars trace circles in the sky E to W
    N stars circle, S stars dip below the horizon
    Celestial equator
    N, S celestial poles
    Meridian
    Zenith

    Path of the sun -- in winter--ecliptic
    Path of the sun -- in summer
    Path of the sun -- in spring and fall
    Each night, the same stars come up, but 4 minutes earlier. After one
    year, all the little 4 minutes add up, and we see the same sky
    Constellations are groupings of stars that they associated with the seasons

    Planets --go roughly along the line with the sun, the ecliptic.
    The Moon also goes roughly along the ecliptic
    Planets -- 2 wanderers stayed close to the sun, tracing back and forth
    The other 5 wanderers seem to go all the way around the sky, but took
    a strange loop in the sky. This confused the ancients, and probably
    was responsible for the concept of epicycles, or circles within circles,
    to explain celestial motions
    W of the sun -- planets rise as morning stars
    E of the sun -- we see planets in the evening

    Spring Equinox -- March 21 (Vernal Equinox) 'Hope'
    Sun crosses the equator and goes N
    Summer Solstice -- June 21, 'Celebration'
    Sun reaches farthest N, and is highest in the sky
    Important to ancient cultures -- max daylight, brightness, sense
    of long, lazy summers
    Autumn Equinox -- Sept 22, 'Preparation'
    Sun crosses the celestial equator, going S
    Winter Solstice -- Dec 21, 'Hibernation'
    Sun furthest S of celestial equator, lowest in the sky

    Moon: races through the sky and goes through phases (interactive animation)
    Moon close to the sun -- New Moon, a crescent
    1 week later, Moon at right angle to Sun, a half circle Quarter Moon
    Overhead at sunset, sets at midnight
    Waxing -- increasing in size
    Terminator -- line between light and dark
    1 week later Moon opposite sun, Full Moon
    Rising at sunset, all through the night, sets at sunrise
    1 week later Moon at right angle to Sun, half circle Three Quarter Moon
    Rises at midnight, we see it in the morning sky, sets at midnight
    Waning -- decreasing in size


  • How did the ancients interpret this motion?

    What was their cosmology? The beginnings of trying to explain the Universe

    Aristotle -- 350 BC
    With Plato, developed rational thought and rudiments of scientific method
    But they thought very highly of absolute symmetry, simplicity, and an
    abstract idea of perfection
    Earth at the center of the Universe
    Universe was spherical and finite
    Planets and stars moved on spherical shells
    Spherical Moon -- Curvature of Moon's terminator
    Model-Experiment-Test-Refine
    Sun farther than Moon, because the Moon passes between the Sun and Earth -- a recognition of the meaning of lunar phases (interactive animation).
    Spherical Earth: Moon was a sphere, and, as you go N, stars sink below the horizon
    But Earth is at the center of the Universe, because the stars didn't move
    Error: Problem with distance scales, inability to abstract

    Hipparchus -- 130 BC -- Considered the first real astronomer
    Observed the positions of stars and planets, and recorded them
    Could PREDICT position of sun and moon
    Discovered wandering of the northern focus of sky motion - Precession
    But Chinese were recording positions as early as 1000 BC

    Ptolomy -- 150 AD
    Circular orbits around the Earth: Moon, Mercury, Venus, the Sun, Mars, Jupiter and Saturn
    Because planets don't move at constant rates, he said the circles were offset from each other, and that planets moved in epicycles
    Could explain all the motions in the sky to pretty good precision
    Wrote the Almagest, the Bible of ancient astronomy for 1000 years
    His work remained at the Great Library of Alexandria in Egypt, until it was plundered by Arabs.
    The Arabs took the knowledge and named the stars. Most names are arabic. Constellations are in Latin. Planets are in Latin

    Copernicus -- 1500
    Applied Occam's Razor: Among competing theories, the best is the simplest theory, the one with the fewest assumptions
    Aesthetic problems with so many little epicycles
    Correctly concluded from the inaccuracies in Ptolemaic model that the sun was at the center of the solar system
    Inferior planets and superior planets
    Copernicus died before his revolution, but Giordano Bruno died because of his revolution

    Tycho Brahe -- 1600
    With funds from King of Denmark, built Uraniborg (Sky Castle) on his own private island
    Measured stars very accurately
    Detected shift in stars over seasons -- parallax
    Remained a Ptolemaist, but pounded the nail in the coffin of Brahe

    Johannes Kepler -- 1600
    Inherited the detailed records
    Addressed the question of Mars' motion, because of its pronounced retrograde cycle (interactive animation).
    Came up with Kepler's Laws
    1. Each planet moves in an ellipse, with Sun at one focus
    2. Line between sun and planet sweeps equal areas in equal time
    3. ratio of cube of the semimajor axis to square of period is the same for each planet

    Galileo Galilei -- 1610
    Saw phases of Venus and moons around Jupiter
    Sun was at center -- some things revolved around something other than Earth
    Saw the planets as WORLDS

    Isaac Newton -- 1700
    'Saw futher because he stood on the shoulders of Giants"
    Deduced that white light was made up of colors (split with prism)
    Looked for the laws that made the Universe tick, not just mechanics
    Newton's Universal Law of Gravitation
    Every particle in the Universe attracts every other particle
    with a force proportional to their masses and inversely
    proportional to the square of the distance between them
    Newton's Laws of Motion
    1. A body at rest stays at rest, and a body in motion moves at constant speed in a straight line unless a force acts upon it
    2. A force acting on a body causes it to accelerate in the direction of the force and inversely proportional to the mass of the body
    3. For every force on a body, there is an equal and opposite force acting on another body



  • The Solar System as We See it Today

    The solar system, slightly elliptical orbits, stars very far away. Santa Fe in our model solar system -- Alpha Centauri
    Moon: Demo of New, First Quarter, Full and Last Quarter
    Same face is always facing us
    Seasons: Due to the tilt of the Earth's axis as it goes around the Sun
    Northern Summer: N pole is tilted towards the sun
    at the same time, it is Southern Winter
    Northern Winter: N pole is tilted away from the sun
    Parallax -- Apparent seasonal shift of nearby stars due to the Earth's motion around the sun
    Constellations change with the seasons, because the background stars change as the direction we look out into changes with our orbit around the sun


  • Light: Colors of the spectrum and dark lines in the spectrum

    White light is actually composed of all the colors mixed together
    Colors can be spread out with a prism -- Isaac Newton
    Specific colors can be removed from a beam of light by intervening atoms
    Caused by the absorption of light at specific colors, due to electrons around the atoms
    Each type of atom has a unique fingerprint, or pattern of dark lines that it can remove from the spectrum

    VIDEO: THE FILMS OF CHARLES AND RAY EAMES: VOLUME1 - POWERS OF TEN

    6/4/96