Chapter 2: Early Astronomy

Chapter 1
How Science Works

  • The Scientific Method
  • Evidence
  • Measurements
  • Units and the Metric System
  • Measurement Errors
  • Estimation
  • Dimensions
  • Mass, Length, and Time
  • Observations and Uncertainty
  • Precision and Significant Figures
  • Errors and Statistics
  • Scientific Notation
  • Ways of Representing Data
  • Logic
  • Mathematics
  • Geometry
  • Algebra
  • Logarithms
  • Testing a Hypothesis
  • Case Study of Life on Mars
  • Theories
  • Systems of Knowledge
  • The Culture of Science
  • Computer Simulations
  • Modern Scientific Research
  • The Scope of Astronomy
  • Astronomy as a Science
  • A Scale Model of Space
  • A Scale Model of Time
  • Questions

Chapter 2
Early Astronomy

  • The Night Sky
  • Motions in the Sky
  • Navigation
  • Constellations and Seasons
  • Cause of the Seasons
  • The Magnitude System
  • Angular Size and Linear Size
  • Phases of the Moon
  • Eclipses
  • Auroras
  • Dividing Time
  • Solar and Lunar Calendars
  • History of Astronomy
  • Stonehenge
  • Ancient Observatories
  • Counting and Measurement
  • Astrology
  • Greek Astronomy
  • Aristotle and Geocentric Cosmology
  • Aristarchus and Heliocentric Cosmology
  • The Dark Ages
  • Arab Astronomy
  • Indian Astronomy
  • Chinese Astronomy
  • Mayan Astronomy
  • Questions

Chapter 3
The Copernican Revolution

  • Ptolemy and the Geocentric Model
  • The Renaissance
  • Copernicus and the Heliocentric Model
  • Tycho Brahe
  • Johannes Kepler
  • Elliptical Orbits
  • Kepler's Laws
  • Galileo Galilei
  • The Trial of Galileo
  • Isaac Newton
  • Newton's Law of Gravity
  • The Plurality of Worlds
  • The Birth of Modern Science
  • Layout of the Solar System
  • Scale of the Solar System
  • The Idea of Space Exploration
  • Orbits
  • History of Space Exploration
  • Moon Landings
  • International Space Station
  • Manned versus Robotic Missions
  • Commercial Space Flight
  • Future of Space Exploration
  • Living in Space
  • Moon, Mars, and Beyond
  • Societies in Space
  • Questions

Chapter 4
Matter and Energy in the Universe

  • Matter and Energy
  • Rutherford and Atomic Structure
  • Early Greek Physics
  • Dalton and Atoms
  • The Periodic Table
  • Structure of the Atom
  • Energy
  • Heat and Temperature
  • Potential and Kinetic Energy
  • Conservation of Energy
  • Velocity of Gas Particles
  • States of Matter
  • Thermodynamics
  • Entropy
  • Laws of Thermodynamics
  • Heat Transfer
  • Thermal Radiation
  • Wien's Law
  • Radiation from Planets and Stars
  • Internal Heat in Planets and Stars
  • Periodic Processes
  • Random Processes
  • Questions

Chapter 5
The Earth-Moon System

  • Earth and Moon
  • Early Estimates of Earth's Age
  • How the Earth Cooled
  • Ages Using Radioactivity
  • Radioactive Half-Life
  • Ages of the Earth and Moon
  • Geological Activity
  • Internal Structure of the Earth and Moon
  • Basic Rock Types
  • Layers of the Earth and Moon
  • Origin of Water on Earth
  • The Evolving Earth
  • Plate Tectonics
  • Volcanoes
  • Geological Processes
  • Impact Craters
  • The Geological Timescale
  • Mass Extinctions
  • Evolution and the Cosmic Environment
  • Earth's Atmosphere and Oceans
  • Weather Circulation
  • Environmental Change on Earth
  • The Earth-Moon System
  • Geological History of the Moon
  • Tidal Forces
  • Effects of Tidal Forces
  • Historical Studies of the Moon
  • Lunar Surface
  • Ice on the Moon
  • Origin of the Moon
  • Humans on the Moon
  • Questions

Chapter 6
The Terrestrial Planets

  • Studying Other Planets
  • The Planets
  • The Terrestrial Planets
  • Mercury
  • Mercury's Orbit
  • Mercury's Surface
  • Venus
  • Volcanism on Venus
  • Venus and the Greenhouse Effect
  • Tectonics on Venus
  • Exploring Venus
  • Mars in Myth and Legend
  • Early Studies of Mars
  • Mars Close-Up
  • Modern Views of Mars
  • Missions to Mars
  • Geology of Mars
  • Water on Mars
  • Polar Caps of Mars
  • Climate Change on Mars
  • Terraforming Mars
  • Life on Mars
  • The Moons of Mars
  • Martian Meteorites
  • Comparative Planetology
  • Incidence of Craters
  • Counting Craters
  • Counting Statistics
  • Internal Heat and Geological Activity
  • Magnetic Fields of the Terrestrial Planets
  • Mountains and Rifts
  • Radar Studies of Planetary Surfaces
  • Laser Ranging and Altimetry
  • Gravity and Atmospheres
  • Normal Atmospheric Composition
  • The Significance of Oxygen
  • Questions

Chapter 7
The Giant Planets and Their Moons

  • The Gas Giant Planets
  • Atmospheres of the Gas Giant Planets
  • Clouds and Weather on Gas Giant Planets
  • Internal Structure of the Gas Giant Planets
  • Thermal Radiation from Gas Giant Planets
  • Life on Gas Giant Planets?
  • Why Giant Planets are Giant
  • Gas Laws
  • Ring Systems of the Giant Planets
  • Structure Within Ring Systems
  • The Origin of Ring Particles
  • The Roche Limit
  • Resonance and Harmonics
  • Tidal Forces in the Solar System
  • Moons of Gas Giant Planets
  • Geology of Large Moons
  • The Voyager Missions
  • Jupiter
  • Jupiter's Galilean Moons
  • Jupiter's Ganymede
  • Jupiter's Europa
  • Jupiter's Callisto
  • Jupiter's Io
  • Volcanoes on Io
  • Saturn
  • Cassini Mission to Saturn
  • Saturn's Titan
  • Saturn's Enceladus
  • Discovery of Uranus and Neptune
  • Uranus
  • Uranus' Miranda
  • Neptune
  • Neptune's Triton
  • Pluto
  • The Discovery of Pluto
  • Pluto as a Dwarf Planet
  • Dwarf Planets
  • Questions

Chapter 8
Interplanetary Bodies

  • Interplanetary Bodies
  • Comets
  • Early Observations of Comets
  • Structure of the Comet Nucleus
  • Comet Chemistry
  • Oort Cloud and Kuiper Belt
  • Kuiper Belt
  • Comet Orbits
  • Life Story of Comets
  • The Largest Kuiper Belt Objects
  • Meteors and Meteor Showers
  • Gravitational Perturbations
  • Asteroids
  • Surveys for Earth Crossing Asteroids
  • Asteroid Shapes
  • Composition of Asteroids
  • Introduction to Meteorites
  • Origin of Meteorites
  • Types of Meteorites
  • The Tunguska Event
  • The Threat from Space
  • Probability and Impacts
  • Impact on Jupiter
  • Interplanetary Opportunity
  • Questions

Chapter 9
Planet Formation and Exoplanets

  • Formation of the Solar System
  • Early History of the Solar System
  • Conservation of Angular Momentum
  • Angular Momentum in a Collapsing Cloud
  • Helmholtz Contraction
  • Safronov and Planet Formation
  • Collapse of the Solar Nebula
  • Why the Solar System Collapsed
  • From Planetesimals to Planets
  • Accretion and Solar System Bodies
  • Differentiation
  • Planetary Magnetic Fields
  • The Origin of Satellites
  • Solar System Debris and Formation
  • Gradual Evolution and a Few Catastrophies
  • Chaos and Determinism
  • Extrasolar Planets
  • Discoveries of Exoplanets
  • Doppler Detection of Exoplanets
  • Transit Detection of Exoplanets
  • The Kepler Mission
  • Direct Detection of Exoplanets
  • Properties of Exoplanets
  • Implications of Exoplanet Surveys
  • Future Detection of Exoplanets
  • Questions

Chapter 10
Detecting Radiation from Space

  • Observing the Universe
  • Radiation and the Universe
  • The Nature of Light
  • The Electromagnetic Spectrum
  • Properties of Waves
  • Waves and Particles
  • How Radiation Travels
  • Properties of Electromagnetic Radiation
  • The Doppler Effect
  • Invisible Radiation
  • Thermal Spectra
  • The Quantum Theory
  • The Uncertainty Principle
  • Spectral Lines
  • Emission Lines and Bands
  • Absorption and Emission Spectra
  • Kirchoff's Laws
  • Astronomical Detection of Radiation
  • The Telescope
  • Optical Telescopes
  • Optical Detectors
  • Adaptive Optics
  • Image Processing
  • Digital Information
  • Radio Telescopes
  • Telescopes in Space
  • Hubble Space Telescope
  • Interferometry
  • Collecting Area and Resolution
  • Frontier Observatories
  • Questions

Chapter 11
Our Sun: The Nearest Star

  • The Sun
  • The Nearest Star
  • Properties of the Sun
  • Kelvin and the Sun's Age
  • The Sun's Composition
  • Energy From Atomic Nuclei
  • Mass-Energy Conversion
  • Examples of Mass-Energy Conversion
  • Energy From Nuclear Fission
  • Energy From Nuclear Fusion
  • Nuclear Reactions in the Sun
  • The Sun's Interior
  • Energy Flow in the Sun
  • Collisions and Opacity
  • Solar Neutrinos
  • Solar Oscillations
  • The Sun's Atmosphere
  • Solar Chromosphere and Corona
  • Sunspots
  • The Solar Cycle
  • The Solar Wind
  • Effects of the Sun on the Earth
  • Cosmic Energy Sources
  • Questions

Chapter 12
Properties of Stars

  • Stars
  • Star Names
  • Star Properties
  • The Distance to Stars
  • Apparent Brightness
  • Absolute Brightness
  • Measuring Star Distances
  • Stellar Parallax
  • Spectra of Stars
  • Spectral Classification
  • Temperature and Spectral Class
  • Stellar Composition
  • Stellar Motion
  • Stellar Luminosity
  • The Size of Stars
  • Stefan-Boltzmann Law
  • Stellar Mass
  • Hydrostatic Equilibrium
  • Stellar Classification
  • The Hertzsprung-Russell Diagram
  • Volume and Brightness Selected Samples
  • Stars of Different Sizes
  • Understanding the Main Sequence
  • Stellar Structure
  • Stellar Evolution
  • Questions

Chapter 13
Star Birth and Death

  • Star Birth and Death
  • Understanding Star Birth and Death
  • Cosmic Abundance of Elements
  • Star Formation
  • Molecular Clouds
  • Young Stars
  • T Tauri Stars
  • Mass Limits for Stars
  • Brown Dwarfs
  • Young Star Clusters
  • Cauldron of the Elements
  • Main Sequence Stars
  • Nuclear Reactions in Main Sequence Stars
  • Main Sequence Lifetimes
  • Evolved Stars
  • Cycles of Star Life and Death
  • The Creation of Heavy Elements
  • Red Giants
  • Horizontal Branch and Asymptotic Giant Branch Stars
  • Variable Stars
  • Magnetic Stars
  • Stellar Mass Loss
  • White Dwarfs
  • Supernovae
  • Seeing the Death of a Star
  • Supernova 1987A
  • Neutron Stars and Pulsars
  • Special Theory of Relativity
  • General Theory of Relativity
  • Black Holes
  • Properties of Black Holes
  • Questions

Chapter 14
The Milky Way

  • The Distribution of Stars in Space
  • Stellar Companions
  • Binary Star Systems
  • Binary and Multiple Stars
  • Mass Transfer in Binaries
  • Binaries and Stellar Mass
  • Nova and Supernova
  • Exotic Binary Systems
  • Gamma Ray Bursts
  • How Multiple Stars Form
  • Environments of Stars
  • The Interstellar Medium
  • Effects of Interstellar Material on Starlight
  • Structure of the Interstellar Medium
  • Dust Extinction and Reddening
  • Groups of Stars
  • Open Star Clusters
  • Globular Star Clusters
  • Distances to Groups of Stars
  • Ages of Groups of Stars
  • Layout of the Milky Way
  • William Herschel
  • Isotropy and Anisotropy
  • Mapping the Milky Way
  • Questions

Chapter 15
Galaxies

  • The Milky Way Galaxy
  • Mapping the Galaxy Disk
  • Spiral Structure in Galaxies
  • Mass of the Milky Way
  • Dark Matter in the Milky Way
  • Galaxy Mass
  • The Galactic Center
  • Black Hole in the Galactic Center
  • Stellar Populations
  • Formation of the Milky Way
  • Galaxies
  • The Shapley-Curtis Debate
  • Edwin Hubble
  • Distances to Galaxies
  • Classifying Galaxies
  • Spiral Galaxies
  • Elliptical Galaxies
  • Lenticular Galaxies
  • Dwarf and Irregular Galaxies
  • Overview of Galaxy Structures
  • The Local Group
  • Light Travel Time
  • Galaxy Size and Luminosity
  • Mass to Light Ratios
  • Dark Matter in Galaxies
  • Gravity of Many Bodies
  • Galaxy Evolution
  • Galaxy Interactions
  • Galaxy Formation
  • Questions

Chapter 16
The Expanding Universe

  • Galaxy Redshifts
  • The Expanding Universe
  • Cosmological Redshifts
  • The Hubble Relation
  • Relating Redshift and Distance
  • Galaxy Distance Indicators
  • Size and Age of the Universe
  • The Hubble Constant
  • Large Scale Structure
  • Galaxy Clustering
  • Clusters of Galaxies
  • Overview of Large Scale Structure
  • Dark Matter on the Largest Scales
  • The Most Distant Galaxies
  • Black Holes in Nearby Galaxies
  • Active Galaxies
  • Radio Galaxies
  • The Discovery of Quasars
  • Quasars
  • Types of Gravitational Lensing
  • Properties of Quasars
  • The Quasar Power Source
  • Quasars as Probes of the Universe
  • Star Formation History of the Universe
  • Expansion History of the Universe
  • Questions

Chapter 17
Cosmology

  • Cosmology
  • Early Cosmologies
  • Relativity and Cosmology
  • The Big Bang Model
  • The Cosmological Principle
  • Universal Expansion
  • Cosmic Nucleosynthesis
  • Cosmic Microwave Background Radiation
  • Discovery of the Microwave Background Radiation
  • Measuring Space Curvature
  • Cosmic Evolution
  • Evolution of Structure
  • Mean Cosmic Density
  • Critical Density
  • Dark Matter and Dark Energy
  • Age of the Universe
  • Precision Cosmology
  • The Future of the Contents of the Universe
  • Fate of the Universe
  • Alternatives to the Big Bang Model
  • Space-Time
  • Particles and Radiation
  • The Very Early Universe
  • Mass and Energy in the Early Universe
  • Matter and Antimatter
  • The Forces of Nature
  • Fine-Tuning in Cosmology
  • The Anthropic Principle in Cosmology
  • String Theory and Cosmology
  • The Multiverse
  • The Limits of Knowledge
  • Questions

Chapter 18
Life On Earth

  • Nature of Life
  • Chemistry of Life
  • Molecules of Life
  • The Origin of Life on Earth
  • Origin of Complex Molecules
  • Miller-Urey Experiment
  • Pre-RNA World
  • RNA World
  • From Molecules to Cells
  • Metabolism
  • Anaerobes
  • Extremophiles
  • Thermophiles
  • Psychrophiles
  • Xerophiles
  • Halophiles
  • Barophiles
  • Acidophiles
  • Alkaliphiles
  • Radiation Resistant Biology
  • Importance of Water for Life
  • Hydrothermal Systems
  • Silicon Versus Carbon
  • DNA and Heredity
  • Life as Digital Information
  • Synthetic Biology
  • Life in a Computer
  • Natural Selection
  • Tree Of Life
  • Evolution and Intelligence
  • Culture and Technology
  • The Gaia Hypothesis
  • Life and the Cosmic Environment

Chapter 19
Life in the Universe

  • Life in the Universe
  • Astrobiology
  • Life Beyond Earth
  • Sites for Life
  • Complex Molecules in Space
  • Life in the Solar System
  • Lowell and Canals on Mars
  • Implications of Life on Mars
  • Extreme Environments in the Solar System
  • Rare Earth Hypothesis
  • Are We Alone?
  • Unidentified Flying Objects or UFOs
  • The Search for Extraterrestrial Intelligence
  • The Drake Equation
  • The History of SETI
  • Recent SETI Projects
  • Recognizing a Message
  • The Best Way to Communicate
  • The Fermi Question
  • The Anthropic Principle
  • Where Are They?

Dividing Time


In mid-northern latitudes, such as in the United States, Canada, or Europe, the Sun rides much higher above the horizon in the summer than in the winter. In the summer, it rises in the northeast, crosses the meridian nearly overhead, and sets in the northwest. But in the winter, it rises in the southeast, crosses the meridian low in the south, and then sets in the southwest. You can mark the passage of the seasons by tracking the position of sunrise or sunset on the horizon. A distant feature, like a rugged mountain range, makes a simple but effective measuring device.

A calendar is a means of counting the days in a year. Ancient people did this by counting the days until the sunrise (or sunset) position moved back to its extreme northerly (or southerly) position after a cycle of the seasons — called a solar year. The earliest records we have, show a count of 360 days in the year. The Egyptians had revised the count to 365 days and they added a leap year — a year of 366 days inserted every fourth year — for an average calendar 365¼ days long. By 2700 B.C., the Babylonians had refined this to a calendar of 365.26 days which was accurate to about 30 minutes in a year. This is an impressive calendar. Nearly 5,000 years ago, the length of the year was known to an accuracy of better than one part in ten thousand!


Illustration of the position of the Earth relative to the Sun during specific times of the year, indicating seasons.

Ancient observers divided the year into seasons using four special dates that we still recognize. Winter solstice is the first day of winter, around December 22nd. On this day the Sun rises and sets farthest to the south. This day has the shortest period of daylight of any day in the year in the northern hemisphere. The pre-Christian pagan cultures of England and France began the year on this date, to celebrate the return of the Sun toward the northern sky. Since the seasons vary smoothly throughout the year, it is quite arbitrary when we choose to begin the calendar. Spring equinox is the first day of spring, around March 21st. On this day the Sun rises due east and sets due west. Day and night are equal in length on this day (in the word equinox, equi- means equal and -nox means night). Other pagan cultures, such as those that worshipped the goddess Maia, began the year on this date because it marked the beginning of the cycle of new growth. Summer solstice is the first day of summer, around June 22nd. On this day the Sun rises and sets farthest to the north. It has the longest daylight period of the year. In many ancient calendars, it marked a day of celebration, when the days were long and the weather pleasant. Autumn equinox is the first day of fall, around September 22nd. On this day the Sun rises due east and sets due west and day and night are again equal.

Primitive cultures also marked the midpoints of the calendar between the solstices and the equinoxes. These dates are February 1st, May 1st, August 1st, and November 1st. In Ireland, these festivals are all still celebrated and are known by their Gaelic names: Imbolc, Beltane, Lughnasa, and Samhain. May Day was originally a fertility festival in the pagan world, and it is still a folk festival in England. And of course, the eve of November 1st is celebrated in many parts of the world, as All Saints' Day in England, as the Day of the Dead in Mexico, and as Halloween in the United States.

You might think that knowledge of solstices and sunrise positions is useless knowledge from the ancient past. However, it has applications in the present, especially in an environmentally conscious age. Consider the layout of windows in your home or apartment. Windows facing northeast or northwest allow sunlight to enter on summer mornings or afternoons when you are likely not to want extra heat in the house. Draperies or shades on these windows in the summer will block sunlight and save on energy bills. Windows facing southeast or southwest, on the other hand, will let in the low-angled light of the winter Sun, giving a free input of extra heat. In a house specifically designed to take advantage of these ideas, windows are placed to take advantage of the midwinter morning and afternoon Sun on the southeast and southwest side. Trees might be planted to shade the northeast, east, west, and northwest sides of the house during the summer mornings and afternoons. Roof overhangs shade southern exposures from the high summer midday Sun while letting the low winter midday Sun warm the interior and exterior of the home.

Most of the major divisions of time have astronomical origins. The illumination cycle of the Moon gives rise to the month. Every 29½ days there is a Full Moon or a New Moon, and this cycle divides approximately 12 times into the solar year. We have found carved animal bones and other artifacts dating back 20,000 to 30,000 years in France and other parts of Europe. Some of these objects have numbers of notches that indicate that the cave dwellers were using them to count months. These portable calendar sticks are among the oldest human relics.

There is a difference between time kept using the Sun and Moon, and time kept using the stars. The time taken for the Sun to pass through the meridian on successive days is a solar day. The time taken for a star to pass through the meridian on successive nights is a sidereal day. Since every star rises and sets a little bit earlier every day, a solar day is about 4 minutes longer than a sidereal day.

Similarly, the time taken for the same phase of the moon to recur is the Moon's synodic period — 29.5 days. This is longer than the time taken for the Moon to pass the same place among the stars — the Moon's sidereal period is 27.3 days. These differences occur because the stars that would be seen in the direction of the Sun shift gradually as the Earth spins and as the Moon orbits the Earth.

Once ancient people recognized the fixed pattern of the constellations, they discovered that five bright "stars" were different from all the others. These "stars" moved from week to week relative to the pattern of the fixed stars. They became known as planets, from the Greek word for wanderer. The planets had unusual attributes. For example, they were not found any place in the sky but always in the strip of sky occupied by the Sun and Moon. Some planets were only seen close to the Sun, others were seen far from the Sun. Some planets would even reverse their direction in the sky when viewed from week to week. Our names for the planets come from the Roman gods Mercury, Venus, Mars, Jupiter, and Saturn. (The other planets — Uranus, Neptune, and Pluto — were not discovered until the invention of the telescope, and the Earth was not yet recognized as one of the planets.)

Every culture has felt the need to create a chunk of time like a week. Ancient Egyptians used 10 days, the Babylonians used 7 days, the Assyrians used 5 days, and some West African tribes have used 4 days in the week. Our calendar is based on Roman tradition, which named the seven days of the week after the seven "moving" objects in the sky — the Sun, the Moon, and five planets. Some of these names are obvious: Saturn-day, Sun-day, Moon-day. The connections to other planets are clearer in languages that are derived from Latin such as Spanish, Italian, and French. Tuesday is Mars-day for example (Mardi in French, and Martes in Spanish). Wednesday is Mercury-day (Mercredi in French, and Miercoles in Spanish), Thursday is Jupiter-day (Jeudi in French, and Jueves in Spanish), and Friday is Venus-day (Vendredi in French, and Viernes in Spanish). So what happened to the names of these four days in English? They were named after gods from the Anglo-Saxon culture of a thousand years ago. Tuesday comes from Tiw, the Norse god of war. Wednesday comes from Woden, the supreme deity. Thursday comes from Thor, the god of thunder. And Friday comes from Frigg, the wife of Woden and goddess of love and beauty.

Even the division of the day into hours has an astronomical origin. Egyptian astronomers used a sequence of bright stars across the sky for timekeeping at night. Twelve timekeeping stars were visible during the critical midsummer period when the Nile would flood so the night (and later the day) was divided into twelve hours. Timekeeping was very primitive until the last 250 years. The Greeks used sundials and the Romans perfected the water clock, where water could drip at a regulated rate through a small hole in a hard stone or jewel. The sand hourglass dates from 8th century Europe. Nobody could divide hours into minutes and seconds until the pendulum clock was invented in the 17th century. We can thank the Babylonians of 5000 years ago for the division of the hour into 60 minutes and the minute into 60 seconds.

Many other features of our calendar and timekeeping spring from the pagan cult of Sun worship. Stonehenge and other great prehistoric structures were built to measure and celebrate the motions of the Sun. Many pagan traditions were borrowed by the early Christian calendar that we still follow. The year starts on January 1st. This copies the pagan cultures which began their calendar when they could detect the Sun beginning to move further north in its rising and setting position. Our rest day of Sunday follows the pagan day of worship of the Sun. Why do clocks move clockwise? In northern Europe, clocks were designed to mimic the arcing motion of the Sun from left to right across the southern sky. Our habits of timekeeping are a rich brew of astronomical ideas taken from earlier cultures.


Author: Chris Impey