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The Story of Astronomy

Page 27

by Peter Aughton


  Extreme Ultraviolet Explorer see EUVE

  Far Ultraviolet Spectroscopic Explorer see FUSE

  Faraday, Michael, 195–6, 226–7

  Fermat, Pierre de, 149

  Fisher, Richard, 342

  Fitzgerald, Edward, 63

  FitzGerald, George, 209

  Flamsteed, John, 125, 152, 166–9, 170–1

  force concept, 332–4

  Fowler, William, 298

  France: maps, 159–60

  Frederick II, king of Denmark, 62, 84–5, 86, 87

  Friedmann, Alexander, 221–2, 326

  FUSE (Far Ultraviolet Spectroscopic Explorer), 322–3

  Gagarin, Yuri, 305–6

  galaxies

  classification, 238–9

  clustering, 351–2

  measuring distance from Earth, 344–5, 351–2

  movements, 239–43

  rotation and structure, 346–53

  see also individual galaxies by name

  Galileo spacecraft, 312, 313–14

  Galileo Galilei, 96, 97–108, 148, 149, 164, 291

  Galle, Johann Gottfried, 193

  gamma rays, 322

  Gamow, George, 326–7

  Ganymede, 314–15

  gas giants, 314, 360

  Gassendi, Pierre, 123, 148

  Geller, Margaret, 352

  Gellibrand, Herbert, 116, 119

  geology, 202–3, 249

  geometry, 57, 62

  George III, king of Great Britain and Ireland, 184

  George, Prince, of Denmark, 169

  Gervaise of Canterbury, 69–70

  Gold, Thomas, 243, 297

  Graham, George, 172

  Grand Unification Epoch see GUE

  gravitational accretion, 359

  gravitational lensing, 222–4, 350–1

  gravity

  and black holes, 269–70, 271–2, 277–8

  Copernican attitude, 75

  and dark energy, 355–7

  escape velocities, 155–6, 270–1

  Galileo’s experiments, 99–100

  importance, 193–5

  measuring specific, 98

  Newton’s theory, 131–3, 134, 135–6, 138–45

  and planetary orbits, 158

  separation from other forces during Big Bang, 334

  and space/time, 216–20

  and unified field theory, 333–4

  “Great Debate,” 233–4

  Great Wall, 352

  Greek astronomy, 22–40, 43–9

  Green, Charles, 177

  Greenwich Observatory, 151, 165–9

  Gregory XIII, Pope, 41

  Grossmann, Marcel, 224

  GUE (Grand Unification Epoch), 335

  Guth, Alan, 335

  H-R diagram, 341–2

  Habicht, Konrad, 212

  Hadron and Lepton Era, 337–8

  Hale, George Ellery, 234–5, 236

  Halley, Edmond, 68–9, 138–43, 169–71

  Harrison, John, 171–6

  Harrison, William, 174

  Harvard, John, 114

  Harvard Observatory, 229

  Harvard University, 114

  Hawking, Jane, 293, 294

  Hawking, Stephen, 278, 290–304

  Heisenberg, Werner, 250

  helium, 338

  Herodotus, 20–1, 22

  Herschel, Caroline, 180–1, 182, 184, 185, 189

  Herschel, John, 126, 184, 186, 188–91

  Herschel, Margaret, 190

  Herschel, Mary, 185, 188

  Herschel, William, 178–89

  Hertzsprung, Ejnar, 341

  Herzog, Albert, 211

  Hesiod, 22

  Hevelius, Elizabeth Margarethe, 127

  Hevelius, Johannes, 126–7

  Hipparchus, 36–40, 44, 46, 47

  Hooke, Robert, 138–40, 153

  Horace, 78

  Horrocks, Jeremiah, 95, 110–26, 168

  Hoyle, Fred, 243, 253, 265–7, 292, 296–8

  Hubble, Edwin, 222, 234, 235, 236–42, 344

  Hubble Space Telescope, 237, 241, 317, 319–22, 345

  Hubble’s constant, 239–42, 344–5

  Hubble’s law, 239–42, 344, 354–5

  Huchra, John, 224, 352

  Huchra Lens, 224

  Humason, Milton, 239, 344

  Huygens, Christiaan, 138, 316

  Hven, 84–6

  hydrogen, 338

  hydrogen line, 342–3, 346–7

  hydrogen spectrum, 199

  hydrostatic balances, 98

  Inflationary Epoch, 335–6

  infrared, 187

  interferometry, 321

  Io, 314

  Islamic astronomy see Arabian and Persian astronomy

  Israel, Werner, 303

  James I and VI, king of England and Scotland, 85

  Jansky, Karl, 259–60

  Jeans, Sir James, 243, 297

  Jodrell Bank, 261

  Julius Caesar, 41, 42

  Jupiter

  ancients’ understanding of movements, 11

  and the asteroid belt, 360

  and Copernican cosmology, 78

  exploration, 312–16

  moons, 101, 314–16

  orbit, 158

  rings, 360–1

  use to calculate speed of light, 152–3

  use to determine longitude, 151, 163–4

  Keck Telescopes, 321

  Kelvin, Lord, 202, 246–7

  Kendall, Larcum, 176

  Kennedy, John F., 306

  Kepler, Johannes, 81, 87–95, 116, 258

  Kepler’s Star, 91

  Khwajah Nizami, 64

  Kuiper, Gerard, 319

  Kuiper Belt, 319

  Lagrange, Joseph-Louis, 157, 158, 188

  Laika (dog), 305

  Lansberg, Philip, 116

  Laplace, Pierre Simon, 157, 158, 188

  Large Hadron Collider, 333

  latitude and longitude, 36, 151–2, 159, 161–77

  Le Verrier, Urbain-Jean-Joseph, 193, 219–20

  leap years, 41

  Leavitt, Henrietta, 229–31, 236, 341

  Leibniz, Gottfried, 156

  Lemaître, Georges, 222, 326

  Levy, David, 325

  light

  Herschel’s experiments, 187

  Newton’s experiments, 130–1

  speed of, 152–3, 215–16

  waves or particles?, 153–4, 206–9, 249–50

  see also optics

  light years, 200

  Lippershey, Hans, 100

  Liverpool, 109–11

  longitude see latitude and longitude

  Lorentz, Hendrick, 209

  Lorini, Nicolo, 103

  Louis XIV, king of France, 150–1

  Lowell, Percival, 308

  Lowell Observatory, 231

  lunar parallax, 46, 341

  Lyell, Charles, 202–3

  magnetism, 194–7

  see also electromagnetism

  maps, 159–60

  Mariner missions, 307, 311

  Mars

  ability to support life, 363–4

  ancients’ understanding of movements, 11

  and Copernican cosmology, 77, 78

  exploration, 307–10

  Galileo’s observations, 102

  and Horrocks’ hypothesis, 123

  orbit, 92–3

  use to determine Earth–Sun distance, 152

  Maskelyne, Nevil, 173, 182

  Mather, Richard, 112

  matrix mechanics, 250

  Maxwell, James Clerk, 196–7, 224, 226–7

  Mayans, 14

  Mayer, Tobias, 176

  Mayer, Walter, 225

  Mendeleyev, Dmitry, 199

  Mercury

  ancients’ understanding of movements, 11

  and Copernican cosmology, 77, 78

  death, 253

  exploration, 311–12

  Gassendi’s observations of transit, 123

  orbit, 219


  Mersenne, Marin, 148–9

  Messenger mission, 312

  Messier, Charles, 182

  meteors, 11, 69–70

  Michell, John, 156

  Michelson, Albert, 207–9, 215

  microwaves, 197

  Milky Way

  Herschel’s model, 186–7

  position in universe, 241

  rotation, 347–8

  size, 236

  structure, 235–6, 346–9

  Sun’s position, 186–7, 235–6, 346

  Miller, Stanley, 364

  Miranda, 317

  Mohammed, Prophet, 53

  Moon

  ancients’ understanding of movements, 2, 5–10, 13, 26–9, 44, 46

  craters, 363

  dark side, 306

  distance from Earth and size, 26–9, 37, 46

  Earth’s gravitational force on, 135–6

  first examination by telescope, 101

  formation, 361–3

  landings, 306–7

  libration, 157

  lunar parallax, 46, 341

  maps, 126–7, 181

  meteorites striking, 69–70

  orbit, 124–5

  phases, 9–10

  photographs, 204

  rotation, 159

  and Sumerians, 17

  and tides, 10

  use to determine longitude, 151, 163, 164–5, 167–9, 175–7

  worship, 14

  see also eclipses, lunar

  moons: formation, 360–1

  Morley, Edward, 208, 215

  motion, Newton’s laws, 133–4, 143–5

  Mount Wilson Observatory, 234–7

  Much Hoole, 117–18

  mural quadrants, 86

  navigation

  arc of the meridian, 159

  astrolabes, 51–2, 54–5, 60, 70–1, 162

  compasses, 194

  measuring longitude, 151, 161–77

  nautical almanacs, 170–7

  origin of degrees and minutes, 18

  origin of latitude and longitude, 36

  nebulae, 181, 182, 204, 244–5, 346

  planetary, 254

  spiral, 231–4, 237–8

  Neptune, 192–3, 312, 317, 360–1

  neutron stars, 257, 264–5

  neutrons, 337

  New Horizons probe, 318

  Newton, Humphrey, 145–6

  Newton, Isaac

  date of birth, 291

  on Descartes, 150

  and Flamsteed’s research, 169

  on Horrocks, 126

  and light, 153–4

  as Master of the Mint, 191

  and Moon’s motion, 168

  overview, 128–46

  rivalry with Leibniz, 156

  and telescopes, 131, 180

  validity of laws, 226–7

  Nizam ul Mulk, 60–1

  Novara, Domenico Maria de, 72

  nuclear fission, 251

  nuclear force

  strong, 332, 333, 335

  weak, 332, 333

  nuclear fusion, 251

  nuclear physics, 246–58

  numerical systems: zero, 55

  observatories

  Greenwich, 151, 165–9

  Harvard, 229

  Hubble Space Telescope, 237, 241, 317, 319–22, 345

  Lowell, 231

  Mount Wilson, 234–7

  Palomar, 235, 237

  Paris, 150–2

  in space, 322–4

  Uraniborg, 84–6

  Odoacer, 52

  Oenopides, 23

  Olber, Heinrich, 155

  Olber’s paradox, 155

  Omar Khayyam, 60–5

  Oort, Jan, 319

  Oort Cloud, 319

  Opportunity rover, 309

  optics, 58–9

  active and adaptive, 321

  Orion Nebula, 204

  pair production, 335

  Palomar Observatory, 235

  Pandora, 316

  parallax method, 340–1

  lunar parallax, 46, 341

  solar parallax, 123–4

  stellar parallax, 200–1, 204–5, 341

  Parbsjerg, Manderup, 82

  Paris Observatory, 150–2

  parsecs, 200

  Pascal, Blaise, 149

  Pascal’s triangle, 62

  Peacock, George, 188–9

  Penrose, Roger, 278, 299–300, 302–3

  Penzias, Arno, 328

  periodic table, 199

  Perlmutter, Saul, 354

  Persian astronomy see Arabian and Persian astronomy

  PG 2112+059 (quasar), 282

  Phoenix lander, 309

  photoelectric effect, 213–14

  photography see astrophotography

  photons, 208, 248–9, 338–9

  pi, 18–19

  Picard, Jean, 151–2

  Pickering, Edward, 205, 229

  Planck, Max, 330

  Planck Era, 334

  Planck scale, 330–1

  plane of the ecliptic, 48

  planetesimals, 359

  planets

  ancients’ understanding of movements, 10–11, 44–5, 46, 47–9

  and Copernican cosmology, 76–9

  Descartes’ theories on motions, 150

  dwarf planets, 318

  escape velocities, 155–6, 270–1

  formation, 358–61

  gas giants, 314, 360

  gravity’s effect on orbits, 138–45, 158

  Horrocks’ hypothesis, 123

  Kepler’s laws of planetary motion, 93–4

  life on other, 96–7, 261–3, 274–5, 358, 363–4

  measuring distance from Earth, 341

  orbits and positions, 79, 81–95

  see also individual planets by name

  Pluto, 318

  Poseidonius, 33–4

  prime mover, 48

  prisms, 130–1

  probability, binomial, 62

  Prometheus, 316

  protons, 337

  protostars, 245, 339

  Ptolemy

  influence, 67, 72, 75, 83, 91

  and the Moon, 125

  on orbit shape, 93

  overview, 43–9

  pulsars, 261–5

  Pythagoras, 23

  quadrants, mural, 86

  quantum mechanics, 225, 250, 296, 300–2

  quarks, 337

  quasars, 276, 279–83, 298

  quintessence, 356–7

  radio waves, 197

  ratios, 62

  Reber, Grote, 260

  Reconnaissance orbiter, 309

  red giants, 252–8, 266

  redshift, 231–2, 280–1, 344–5, 352

  relativity

  and black holes, 277

  general theory of, 216–21, 222–4

  and quantum mechanics, 296, 300–2

  special theory of, 208–9, 210, 213–16

  Rhaeticus, 80

  Rhodes, Colossus of, 35–6

  ring systems, 360–1

  Roman empire, fall of, 52

  Rømer, Ole, 152–3

  Romulus Augustus, Western Roman emperor, 52

  rotation curve, 348

  Royal Astronomical Society, 188

  Royal Society, 131, 138, 147, 149–50

  RR Lyrae variables, 236

  Rubin, Vera, 348

  Rudolf II, Holy Roman Emperor, 87, 90, 94–5

  Rudolphine Tables, 90–1, 94–5, 116

  Russell, Henry Norris, 341

  Rutherford, Ernest, 247–8

  Sagredo, Giovanni Francesco, 105

  Salviati, Fillipo, 104

  Sandage, Allan, 279

  satellites, manmade, 305, 306

  Saturn

  ancients’ understanding of movements, 11

  and Copernican cosmology, 78

  exploration, 312, 316–17

  moons, 159, 185–6, 316–17

  orbit, 158

  rings, 101–2, 158–9, 316, 360

  Schiaparel
li, Giovanni, 308

  Schmidt, Brian, 354

  Schmidt, Maarten, 280

  Schrödinger, Erwin, 250

  Schwarzchild radius, 272, 287

  Scout missions, 309–10

  Secchi, Angelo, 205–6

  SETI (Search for Extraterrestrial Intelligence), 274–5

  Seven Wonders of the Ancient World, 35–6

  Shapley, Harlow, 233–4, 235–6

  Shoemaker-Levy 9 (comet), 313, 325

  singularity theory, 299–300, 302

  Sirius, 11, 254

  Slipher, Vesto, 231–2, 239, 344

  SNC meteorite, 363–4

  SOHO (Solar and Heliospheric Observatory) spacecraft, 323

  solar parallax, 123–4

  Solovine, Maurice, 212

  solstices, precession of, 42

  Sosigenes, 41

  South, James, 189–90

  space exploration, 305–25

  spectrographs, 205

  spectroscopy, 205–6, 231–3

  spiral nebulae, 231–4, 237–8

  Spirit rover, 309

  Spitzer Space Telescope, 322–3

  Sputnik I, 305

  stars

  ancients’ understanding of movements, 47, 48

  binary, 181–2, 189–91, 273

  birth, 245–6, 339, 346

  death, 252–8

  distribution in sky, 186–7, 189–91

  and element formation, 253, 254, 256–7, 265–9, 297–8

  escape velocities, 271

  globular star clusters, 235–6

  Helvelius’ maps, 127

  magnitudes and positions, 36–7, 57, 86–7, 200–1, 204–5, 229–31, 341–4

  neutron stars, 257, 264–5

  photographs, 204

  spectral features, 205–6, 231–3

  stellar parallax, 200–1, 204–5, 341

  supernovae, 83–4, 91, 257–8, 261–9, 325

  telescopes lead to discovery of many more, 102–3

  variable stars, 230–1, 236, 237–8, 342

  why they shine, 245–7, 251–2

  see also individual stars by name

  steady-state theory, 243, 297, 327–9

  stellar parallax, 200–1, 204–5, 341

  Strabo, 33

  Stukeley, William, 132

  Sumerians, 16–18

  Sun

  age, 202, 246–7

  ancients’ understanding of movements, 2, 5–10, 13, 23, 26, 44, 48

  and Babylonians, 19

  classification as star, 154

  and Copernican cosmology, 71–80, 104–8

  death, 252–4

  distance from Earth and size, 29–30, 38–40, 46, 152, 177

  distance from planets, 94

  gravitational effect on planets’ orbits, 138–45

  position in Milky Way, 186–7, 235–6, 346

  solar parallax, 123–4

  solar wind, 323

  space observation of, 323

  why it shines, 251–2

  worship, 14

  see also eclipses, solar; stars

  supernovae, 83–4, 91, 257–8, 261–9, 325

  Type 1a, 343–4, 354

  super-sphere, 285–6

  Tariq ibn Ziyad, 66

  telescopes

  Allen Telescope Array, 274–5

  Chandra, 322

 

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