The Stardust Revolution

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The Stardust Revolution Page 38

by Jacob Berkowitz


  space research on, 23–25,

  spontaneous generation of, 115–18,

  water and, 168

  See also extraterrestrial life

  light

  elements and, 49–52,

  flames, 48–49,

  interstellar extinction, 140–41, 246

  invisible, 145

  radiation and, 268

  rainbow spectrum, 50

  solar spectrum, 44, 51–55,

  spectrum of, 49–51,

  temperatures of, 144–45,

  wavelengths of, 33, 145–46,

  See also infrared astronomy

  light fingerprints

  discovery of, 50–51,

  dust grains, 198

  elements, 298

  molecules, 186

  stars, 246–47,

  unidentified broad-absorption patterns, 190

  See also spectroscopy

  light-years, distances in, 17–18,

  Limits of Organic Life in Planetary Systems, Committee on the, 288, 294

  Linnaeus, Carl, 277, 284

  lithic astronomy, 199, 215. See also astrogeology

  lithium, 281

  Los Alamos, NM, 196

  Los Angeles, CA, 37–38,

  love and life, 285, 296

  Lovelock, James, 299

  Low, Frank, 147

  LUCA (last universal common ancestor), 12, 291

  Lunar Receiving Laboratory, 201

  Lyttleton, Ray, 34

  MacAlpine Hills 88105 meteorite, 195

  Machu Picchu, 137

  magnesium, 185, 206

  main sequence in stars, 96, 183

  manganese, 143

  Manhattan Project, 81–82, 125

  Marcy, Geoff, 257

  Mars,

  ice on, 178

  images of, 167

  life on, 299

  meteorites from, 195, 207–208,

  missions to, 23–24,

  Martian Chronicles, The (Bradbury), 267

  Martins, Zita, 229

  Marxism, 113

  masers, 169

  idea for, 174

  MASER (microwave amplification by stimulated emission of radiation), 172

  water, 175, 177

  Massachusetts Institute of Technology (MIT), 169, 173

  mass spectrometers, 80, 209, 211

  mathematics, 142, 271

  Matthews, Jaymie, 253–54,

  Mauna Kea, HI, 249–51,

  Mayer, Julius Robert, 77

  Mayor, Michel, 241–44, 255–56, 258, 263, 274, 302

  McDonnell Center for the Space Sciences, 197

  McKay, Chris, 296

  McKellar, Andrew, 166

  “Mémoire sur les corpuscules organisés qui existent dans l’atmosphère” (Pasteur), 118

  Memoirs of the Literary and Philosophical Society of Manchester (Dalton), 73

  Mendeleev, Dmitri, 63, 75

  Mercury, 232, 243, 261

  Merrill, Paul W., 37, 59–65, 95, 104, 190, 304

  Messier object 42 (nebula), 138

  metals, 99

  meteorites, 195–96, 200–12, 214

  National Meteorite Collection, 202

  organic molecules in, 226–31, 236–40,

  origins of, 207–208,

  meteoroids, 198

  methane, 123, 126–27, 147, 185, 187, 191, 225, 299, 301

  methanol, 222, 237–38,

  metric measurements, 18

  M42 (nebula), 138

  Michelson, Albert, 40

  microbes, 115, 118, 131–32,

  microorganisms, 117–18,

  microscopes, 197, 199

  microwave amplification by stimulated emission of radiation (MASER), 172. See also masers

  microwave molecular spectroscopy, 171–73,

  microwaves, 145, 163–64,

  Microwave Spectroscopy (Schawlow and Townes), 172

  military rockets, telescopes on, 147

  Milky Way

  dark patches, 136–38, 140

  Earth-like planets in, 307

  electrical static, 163

  hydrogen clouds, 165

  search for planets in, 270

  solar systems in, 275

  Miller, Stanley, 124–29, 191, 223–24, 233, 288, 289

  Miller, William, 56–57,

  Millikan, Robert, 67

  minerals

  mineralogists, 286

  oldest discovered, 213–14,

  in stardust, 156–57,

  Ming, Tang, 212

  mini-Neptunes, 261–62, 275

  Mira (star), 184

  Mira variable stars, 61–62,

  MIT (Massachusetts Institute of Technology), 169, 173

  moissanite (mineral), 156

  molecules

  chiral structure of, 228

  cold molecular clouds, 222–23,

  cosmic

  discovery of, 30, 166

  diversity of, 186–87,

  detection of

  by microwave signals, 171–75,

  by radio telescopes, 161–62,

  evolution of, 121–24,

  extragalactic, 22

  organic, 131

  radio frequencies of, 165

  stellar molecular synthesis, 183

  molybdenum (element 42), 64

  Moon

  craters on, 305

  Earthshine on, 301

  eclipse of, 129

  ice on, 177–78,

  Late Heavy Bombardment, 231–35,

  meteorites from, 195, 207–208,

  missions to, 23–24, 167–70,

  molecules on, 133

  protection of, 131–32,

  rocks from, 201, 231

  voyages to, 35

  See also Apollo missions

  “Moondust” (Lederberg), 133

  Mount Lassen, 174

  Mount Palomar, 41, 62

  Mount Wilson Observatory

  Adams, Walter, 67

  Bowen, Ira, 174

  history and significance of, 39–43,

  Hoyle, Fred, 91–92,

  living quarters, women in, 98

  Merrill, Paul, 59–61, 95, 304

  150-Foot Solar Tower, 37–40, 43

  spectrograph, 166

  Murchison meteorite, 226–30, 240

  amino acids in, 238

  photograph of, 217

  nano-diamonds, stellar, 157, 212–13, 218, 239

  nanoSIMS (nano Secondary Ion Mass Spectrometer), 216

  NASA (National Aeronautics and Space Administration)

  Ames Research Center, 195, 221, 223–24, 238, 271

  Apollo Science and Technology Advisory Committee, 168–69,

  Astrobiology Science Conference, 284–86,

  creation of, 35, 132, 181

  Great Observatories, 272

  Hubble Space Telescope, 148, 260, 272, 300, 302

  International Space Station, 272

  Jet Propulsion Lab, 299

  Johnson Space Center, 182, 285

  Kepler Space Telescope, 262–63, 266–67, 271–76, 302, 307

  life, working definition of, 290

  Lincoln Lab, 173

  Mariner Mars orbiter, 167

  Office of Space Science, 23

  Origins Program, 23–24, 272

  Planetary Protection Program, 110, 132

  search for extraterrestrial intelligence (SETI) program, 24

  Shuttle Infrared Telescope Facility (SIRTF), 148

  Space Shuttle, 272

  Spitzer Space Telescope, 33, 146, 148–49, 151, 157, 260, 302

  Stardust mission, 26, 195–96, 198

  Terrestrial Planet Finder, 298, 302

  See also Apollo missions

  National Aeronautics and Space Act, 132

  National Aeronautics and Space Administration (NASA). See NASA (National Aeronautics and Space Administration)

  Nazi Germany, 88, 165–66, 187, 211, 247. See also World War II

  nebulae

  Bok globules, 151–53,
r />   Cat's Eye nebula, 185

  discovery of, 137–38,

  gravitational collapse, 155

  Helix Nebula, 185

  Orion Nebula, 138, 175, 177, 206, 260, 305, 306

  planetary nebulae, 185

  solar, 205, 206

  spiral, 138–39,

  Neptune, 220, 257

  mini-Neptunes, 261–62, 275

  Neptune-sized exoplanets, 261

  NERVA (Nuclear Engine for Rocket Vehicle Application), 181

  Neugebauer, Gerry, 152

  neutrons, 87–88,

  discovery of, 90

  neutron capture, 99, 101

  New Mexico Institute of Mining and Technology, 196–97,

  Newton, Isaac, 29, 49, 53, 71–72, 121

  night-vision combat technology, 147

  Nimitz, Chester, 169

  nitrogen, 119–20, 293, 295

  Nobel Prizes, 68, 81, 102–104, 125, 130, 132, 165, 169, 175

  noble gases, 209

  nuclear alchemy, 64

  Nuclear Engine for Rocket Vehicle Application (NERVA), 181

  nuclear fusion, 182

  nuclear physics, 83, 87

  nuclear reactions, 78–79, 82

  nuclear research, 181–82,

  nuclear weapons, 81–83, 125, 131

  nucleobases, 189, 229–31, 238

  nucleosynthesis in stars, 103

  nucleotides, 229, 291, 296

  O, B, A, F, G, K, and M system, 59, 278

  observatories, 41–43,

  Oh Be A Fine Girl/Guy, Kiss Me! system, 59, 278

  Old Faithful, 242

  olivine (mineral), 156

  150-Foot Solar Tower, 37–40, 43

  Oparin, Alexander Ivanovich, 112–15, 119, 120–27, 130

  open-star clusters, 139–40,

  Oppenheimer, Robert, 170

  organic chemistry, 162, 183–85, 228. See also chemistry

  organic molecules, 223, 233–35,

  Orgueil carbonaceous chondrite, 219

  “Origin, Age, and Composition of Meteorites” (Anders), 207

  Origin of Life, The (Oparin), 112, 114–15, 119, 130

  Origin of Species, On the (Darwin), 42, 49, 110, 113, 117, 278

  origins, 12, 25, 29–30,

  Origins and Evolution of Life, Committee on the, 23–24, 109–12, 132

  Origins of Life Initiative, Harvard University, 284, 297

  Origins Program, 23–24, 272

  Orion (constellation), 155, 304

  Orion Nebula, 138, 175, 177, 206, 260, 305, 306

  orphan planets, 264

  oxidative atmospheres, 123, 129

  oxygen

  in atmosphere, 299, 301

  as element of life, 119–20, 178–79, 293–95,

  molecular, 123

  nucleosynthesis, 101

  in water, 74

  ozone, 301

  Padilla, Steve, 37–40,

  PAHs (polycyclic aromatic hydrocarbons), 187–88, 224, 230

  paleogenetics, 287

  paleontology, molecular, 288

  Palomar, Mount, 41, 62

  panspermia, 119

  paradigm shifts, 33–34,

  Pasteur, Louis, 29, 117–18,

  Paz, Octavio, 306

  Peiresc, Nicolas-Claude Fabri de, 138

  Penzias, Arno, 29, 164–65,

  Perceptron (computer), 269

  periodic table of elements, 59, 63, 75

  Perrier, Carlo, 63

  Philosopher's Stone, 71, 86

  philosophy, 45–46, 115

  phosphorus, 293

  photography, 57–59,

  photometers, 269–70, 272

  “Physical Basis of Life, On the” (Huxley), 119

  physics, 49, 286, 293

  research, 68

  unified theory, 29

  use of math, 142

  See also astrophysics

  Pickering, Edward C., 58

  Pillars of Creation, 150

  Pius XII (pope), 87

  planetary chemistry, 296

  planetary embryos, 220

  planetary nebulae, 185

  planetesimals, 203, 221

  planets

  in double-star systems, 264–65,

  51 Peg b (51 Pegasi b), 243, 255, 261, 272

  gap in knowledge about, 243–44,

  living planets, 297–302,

  orphan planets, 264

  types of, 261

  See also exoplanets

  plasmas, 76, 268–69,

  platinum, 101

  Pluto, dwarf-planet status, 265

  pollution, 189

  polysaccharides, 296

  potassium chloride, 187

  Pouchet, Félix Archimède, 117–18,

  prairies, North American, 135–36,

  pre-solar stardust grains, 215–19, 239

  primordial soup, 126–27, 130, 223–24, 289

  prisms, 49–51, 144–45,

  Profitable Disposal of Sewage, The (Crookes), 72

  proplyds, 260. See also protoplanetary disks

  proteins, 223, 226, 227, 229, 295, 296

  protobiologists, 115

  protocosmologists, 86

  protons, 281

  protoplanetary disks, 204, 221, 260, 263

  Prout, William, 74–76,

  Puerto Rico, 161

  quantum atom, 90

  quantum mechanics, 69, 86

  quantum physics, 91, 125

  quarks, 281

  quartz, 143

  Queloz, Didier, 243–44, 255–56,

  “Quest for the Origin of the Elements, The” (Fowler), 102

  radar, 91, 163–64, 170–71,

  radial velocity method, 246–47,

  radioactive alpha decay, 86

  radioactive elements, 63

  radioactivity, 78

  radio astronomy, 22, 33, 160–67, 174, 177, 235

  radio waves, 145–46, 163

  radium (element), 78

  rainbows, 50, 144–45,

  Rank, David, 174–75,

  Reber, Grote, 163

  Recombination Era, 282

  red giant stars

  carbon production in, 143, 183–85, 237

  circumstellar envelope, 185

  diamonds formed in, 213

  dust created in, 155, 157

  energy from, 80

  nucleosynthesis, 101

  silicon carbide stardust grains, 218

  spectroscopic fingerprints of, 239

  water formed by, 178–79,

  red shift, 61, 140, 246–47,

  reducing atmospheres, 123, 129

  regolith, 168, 170

  Reilly, Edith, 151–52,

  R Geminorum (star), 62

  ribonucleic acid (RNA). See RNA (ribonucleic acid)

  Rice University, 182

  ring-shaped hydrocarbons, 188–89,

  RNA (ribonucleic acid), 189, 229, 290–91,

  Rockefeller, John D., Sr., 41

  rocks, 84, 156, 197, 199–205, 208, 215, 221, 230–31,

  Rosenblatt, Frank, 269–70, 272

  r-process (rapid), 101–102,

  Russell, Henry Norris, 91

  Russian Revolution, 114, 131

  Rutherford, Ernest, 78–79, 81, 90

  Safronov, Viktor, 208

  Sagan, Carl, 132, 159, 161, 269

  cosmic delivery of organic material, 233

  on extraterrestrial life, 31–32, 223–24,

  life, definition of, 290

  support for planet hunting, 252

  Sagittarius B, 174–75,

  Salpeter, Edwin, 93, 269

  salt, 54, 120, 185, 187, 300

  Sandford, Scott, 195–99, 221–24, 234, 238, 240

  Sanford, Roscoe Frank, 138–39,

  Saskatchewan, Canada, 135–36,

  Sasselov, Dimitar, 284

  Saturn, 176, 220, 257

  Schawlow, Arthur, 172

  Schmidt, Otto, 208

  science fiction, 180, 243, 267, 287, 294


  books, 89, 141

  films, 23, 25, 161

  scientific establishment, 33–35,

  scientific methods, 46

  scientific revolutions, 28

  Sea of Tranquility, 167

  search for extraterrestrial intelligence (SETI) program, 24, 161, 164, 271

  sedimentary rocks, 203

  seeing, 32–33, 38, 43, 144, 160

  Segrè, Emilio, 63

  SETI (search for extraterrestrial intelligence) program, 24, 161, 164, 271

  Shapley, Harlow, 40

  silicate dust, 143, 156–57,

  silicon-based life, 294–95,

  silicon carbide, 218, 239

  silicon dioxide, 283

  silver (element), 85, 101, 303, 304

  SIRTF (Shuttle Infrared Telescope Facility), 148

  Smithsonian Institution, 201

  sodium, light fingerprint of, 53, 300

  sodium chloride, 185, 187

  solar observation, 37–44,

  solar spectrum, 44, 51–55,

  Solar System

  birth of, 219–23,

  changing perspectives on, 265

  formation of, 206, 231–32,

  as model, 257–58, 260–61,

  origin of, 196, 208

  solid phase of, 205

  water, discovery of, 176–78,

  solar systems

  behaviors of, 263–64,

  diversity of, 258–59,

  in Milky Way, 275

  search for, 243–44,

  See also Extreme Solar Systems II conference (Jackson Hole, WY)

  Solution of the Sewage Question, A (Crookes), 72

  Sonora Desert, AZ, 159

  Soviet Union

  Biochemical Institute, 114

  scientific research, 208

  Soviet Academy of Sciences, 124, 126

  Sputnik I (satellite), 34–35, 131, 181

  space age, modern, 35–36, 131, 181

  space and time, beginning of, 280–81,

  Space Sciences Board, 132

  Space Studies Board. See United States Space Studies Board

  spectroscopy

  Doppler spectroscopy, 246, 249, 257, 259

  gases, identification of, 298

  mysteries in, 190

  spectral fingerprints of elements, 76

  spectrograms, 57–59, 166

  spectrography, 258

  spectroscopes, 44, 50–51, 268

  stellar, 55–63, 123, 245

  See also light fingerprints

  spiral nebulae, 138–39,

  Spitzer, Lyman, 148, 151

  Spitzer Space Telescope, 33, 146, 148–49, 151, 157, 260, 302

  spontaneous generation, 114–18,

  s-process (slow), 101

  Sputnik I (satellite), 34–35, 131, 181

  spy equipment, 147, 197, 268

  Stalin, Joseph, 208

  Standard Model of Cosmology, 29

  stardust

  defined, 25

  diamonds in, 213

  emergence of Earth from, 208

  first created, 153–54,

  grains, 215–20,

  infrared images of, 150–51,

  organic, 239

  stardust geology, 214–16,

  stardust science, 25–35,

  See also cosmic dust

  Stardust mission, 224–25,

 

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