Book Read Free

The Stardust Revolution

Page 36

by Jacob Berkowitz


  Sources of Direct Quotations by Page

  (page 241) “The province of the student…” George Ellery Hale, The Study of Stellar Evolution: An Account of Some Recent Methods of Astrophysical Research (Chicago: University of Chicago Press, 1908), p. 4.

  (page 244) “utterly unique…” Peter Ward and Donald Brownlee, Rare Earth: Why Complex Life Is Uncommon in the Universe (New York: Springer-Verlag, 2000) p. xxiv.

  (page 250) “It is quite hard…” Walker, “First High-Precision Radial Velocity Search for Extra-Solar Planets,” p. 2.

  (page 252) “I probably won't…” Marschall and Maran, Pluto Confidential, pp. 170–71.

  CHAPTER 9. DARWIN AND THE COSMOS

  Many years ago, I read and was inspired by a book that led me to thinking about the issues discussed in this chapter: Brian Swimme, The Universe Is a Green Dragon: A Cosmic Creation Story (Santa Fe, NM: Bear, 1985). The history of the concept of cosmic evolution is covered in Steven J. Dick, “Cosmic Evolution: History, Culture, and Human Destiny,” in Cosmos & Culture: Cultural Evolution in a Cosmic Context, ed. Steven J. Dick and Mark Lupisella (Washington, DC: National Aeronautics and Space Administration, Office of External Relations, History Division, 2009). For the reference to Darwin's “gone cycling on,” I’m indebted to Timothy Ferris, who noted Darwin's use of the term in his book The Whole Shebang: A State-of-the-Universe(s) Report (New York: Simon & Schuster, 1997), p. 175.

  Sources by Sections

  The Biological Big Bang

  The section on Alexander Dalgarno is based on my interview with him and on the articles: Alexander Dalgarno, “A Serendipitous Journey,” Annual Review of Astronomy and Astrophysics 46 (2008): 1–20; Alexander Dalgarno, “The Growth of Molecular Complexity in the Universe,” Faraday Discussions 133 (2006): 9–25; and Volker Bromm and Richard B. Larson, “The First Stars,” Annual Review of Astronomy and Astrophysics 42 (2004): 79–118. Current research goals on the eras of cosmic dawn and the cosmic dark ages are outlined in National Research Council of the National Academies, New Worlds, New Horizons in Astronomy and Astrophysics (Washington, DC: National Academies Press, 2010).

  What Is “Life”?

  In writing this section, I drew on Steven Benner, Life, the Universe, and the Scientific Method (Gainesville, FL: Ffame Press, 2009); Steven Benner “Defining Life,” Astrobiology 10 (2010): 1021–30; Stephane Tirard, Michel Morange, and Antonio Lazcano, “The Definition of Life: A Brief History of an Elusive Scientific Endeavor,” Astrobiology 10 (2010): 1003–1009; C. E. Cleland and C. F. Chyba, “Defining ‘Life,'” Origins of Life and Evolution of Biospheres 35 (2002): 333–43; and Antonio Lazcano, “Which Way to Life?” Origins of Life and Evolution of Biospheres 40 (2010): 161–67.

  Alonso Ricardo and Steven Benner, “The Origin of Proteins and Nucleic Acids,” in Planets and Life: The Emerging Science of Astrobiology, ed. Woodruff T. Sullivan III and John Baross (Cambridge: Cambridge University Press, 2007) p. 154.

  For a fascinating look at efforts to trace back our molecular heritage, see Chiaolong Hsiao et al., “Peeling the Onion: Ribosomes Are Ancient Molecular Fossils,” Molecular Biology and Evolution 26 (2009): 2415–45; and the Center for Ribosomal Origins and Evolution, where a large research team is working to rewind the tape of life at the molecular level: http://astrobiology.gatech.edu/home (accessed April 30, 2012).

  For a full discussion of the history of the development of the RNA world theory and the current debate, see Benner, Life, the Universe, and the Scientific Method, chaps. 4 and 5.

  Life as a Cosmic Continuum

  This section draws on George Wald, “The Origins of Life,” Proceedings of the National Academy of Sciences 52, no. 2 (August 1964): 595–611; Chris P. McKay, “What Is Life—and How Do We Search for It in Other Worlds?” PLoS Biology 2 (September 2004): 1260–63; Norman R. Pace, “The Universal Nature of Biochemistry,” Proceedings of the National Academy of Sciences 98 (2001): 805–808; Pascale Ehrenfreund and Mark A. Sephton, “Carbon Molecules in Space: From Astrochemistry to Astrobiology,” Faraday Discussions 133 (2006): 277–88; and National Research Council of the National Academies, The Limits of Organic Life in Planetary Systems (Washington, DC: National Academies Press, 2007).

  Astrobiology pioneer Lynn Rothschild's “Replaying the Tape” lecture to her astrobiology and space exploration class at Stanford University can be found at https://humbio.stanford.edu/node/2427 (accessed April 30, 2012).

  The study of element-based phylogenetics is the new field of paleoecophylostoichiometrics: paleo: “ancient”; eco: “environment”; phylo: “genetic relationship”; stochiometrics: “measurement of relative quantities”; see Aditya Chopra et al., Palaeoecophylostoichiometrics: Searching for the Elemental Composition of the Last Universal Common Ancestor, in Australian Space Science Conference Series: 9th Conference Proceedings. Full Refereed Proceedings DVD, National Space Society of Australia Ltd., ISBN 13: 978-0-9775740, 2010.

  For thoughts on the cosmic selection process of our genetic code, see Paul G. Higgs and Ralph E. Pudritz, “A Thermodynamic Basis for Prebiotic Amino Acid Synthesis and the Nature of the First Genetic Code,” Astrobiology 9, no. 5 (2009): 483–89; and Gayle K. Philip and Stephen J. Freeland, “Did Evolution Select a Nonrandom ‘Alphabet' of Amino Acids?” Astrobiology 11, no. 3 (2011): 235–40.

  For background on possible abiotic cell membrane precursors, see Sandra Pizzarello, “The Cosmochemical Record of Carbonaceous Meteorites: An Evolutionary Story,” Journal of the Mexican Chemical Society 53, no. 4 (2009): 253–60; George D. Cody et al., “Establishing a Molecular Relationship between Chondritic and Cometary Organic Solids,” Proceedings of the National Academy of Sciences 108 (November 29, 2011): 19171–76; and “Protocells,” Center for Fundamental Living Technology, http://flint.sdu.dk/index.php?page=protocell.

  Bunsen and Kirchhoff's Gift

  For an overview of exoplanet atmospheric science, see Sara Seager and Drake Deming, “Exoplanet Atmospheres,” Annual Review of Astronomy and Astrophysics 48 (2010): 631–72. For proposed missions to study possible living exoplanets, see C. S. Cockell et al., “Darwin—A Mission to Detect and Search for Life on Extrasolar Planets,” Astrobiology 9, no. 1 (January–February 2009): 1–22; and see the entire issue of Astrobiology 10, no. 1 (January–February 2010), especially the article by M. Fridlund et al., “The Search for Worlds Like Our Own,” pp. 5–19.

  An excellent overview of the history and challenging future of direct exoplanet imaging is Paul Kalas, “Planetary Systems Revealed through Direct Imaging,” Hipparchos 2 (September 2011): 23–28.

  For an overview of how NASA discusses its mission in finding an alien Earth, see PlanetQuest on NASA's Jet Propulsion Laboratory's site: http://planetquest.jpl.nasa.gov/.

  The description of the history of searching for living planets based on their atmospheric characteristics is based on J. E. Lovelock, “A Physical Basis for Life Detection Experiments,” Nature 207 (August 7, 1965): 568–70; and Dian R. Hitchcock and James E. Lovelock, “Life Detection by Atmospheric Analysis,” Icarus 7 (1967): 149–59.

  A link between exoplanet geology and atmospherics is found in Nikku Madhusudhan, “A High C/O Ratio and Weak Thermal Inversion in the Atmosphere of Exoplanet WASP-12b,” Nature 469 (January 6, 2011): 64–67. See also Michael F. Sterzik, Stefano Bagnulo, and Enric Palle, “Biosignatures as Revealed by Spectropolarimetry of Earthshine,” Nature 483 (March 1, 2012): 64–66; Shawn D. Domagal-Goldman et al., “Using Biogenic Sulfur Gases as Remotely Detectable Biosignatures of Anoxic Planets,” Astrobiology 11, no. 5 (2011): 419–41; and David J. Des Marais et al., “Biosignatures and Planetary Properties to Be Investigated by the TPF Mission,” NASA-JPL Publication 01-008, Rev. A, October 2001 available online at http://planetquest1.jpl.nasa.gov/TPF/TPF_Biomrkr_REV_3_02.pdf.

  An Ancient View with Stardust Eyes

  I visited Guanajuato, Mexico, from January to June 2012. Presently, the University of Guanajuato offers nightly astronomy viewing from the roof of its main downt
own campus building.

  Sources of Direct Quotations by Page

  (page 227) “We have had a century…” Wald, “Origins of Life,” p. 595.

  (page 284) “a revolution in our…” Dimitar Sasselov, “Two Separate Quests, One to Discover Habitable Worlds, the Other to Synthesize Artificial Organisms, Now Unite to Redefine ‘Life' and Place in the Universe,” SeedMagazine.com, March 14, 2011, pp. 66–67, http://seedmagazine.com/content/article/on_discovering_life/ (accessed February 22, 2012).

  (pages 288–89) “This is no accident,” Benner, Life, the Universe, and the Scientific Method, p. 23.

  (page 290) “Life is a self-sustaining chemical system…” Ibid., p. 24.

  (page 292) “If the origin of life…” Lazcano, “Which Way to Life?” p. 166.

  (pages 292–93) “Though no evidence…” J. Peretó, J. Bada, and A. Lazcano, “Charles Darwin and the Origin of Life,” Origins of Life and Evolution of the Biosphere 39 (2009): 404.

  (page 293) “The human genome…” Ricardo and Benner, “Origin of Proteins and Nucleic Acids,” p. 154.

  (page 296) “Different life forms…” McKay, “What Is Life?” p. 1262.

  (page 297) “What drives us…” Jacob Berkowitz, “The New Age in Astronomy: Ottawa Native Spots Jupiter-Sized Exoplanet, a Mere 500 Light-Years Away,” Ottawa Citizen, September 10, 2006.

  (page 304) “the contrast between the apparent…” Paul W. Merrill, “Stars as They Look and as They Are,” Publications of the Astronomical Society of the Pacific 38, no. 221 (1926): 14.

  (page 306) “To the ancient Aztecs…” Octavio Paz, The Labyrinth of Solitude: Life and Thought in Mexico, trans. Lysander Kemp (New York: Grove, 1961), p. 56.

  abundances of elements, 84–85, 87, 91–92, 97, 99–100, 143, 293–94

  “Abundances of the Elements” (Suess and Urey), 99–100,

  accretion disk, 220

  acetic acid, 187, 227

  acetone, 187

  Adams, Walter, 67

  adenosine triphosphate (ATP), 230

  AGB-type stars, 155

  alanine, 223

  alchemy, 71–73, 79

  alcohol, 186

  Aldrin, Buzz, 167

  Alien (film), 294, 295

  aliens, 15, 161–62, 164, 294

  search for, 160, 177, 244, 249, 256

  See also exoplanets

  Allamandola, Lou, 221

  Allan Hills 84001 meteorite, 195

  Allende meteorite, 200–202, 204–207, 209–12,

  alpha particles, 78, 86, 93–94,

  alpha process, 101

  Alpher, Ralph, 88

  aluminum, 185, 186, 204–206,

  Alvarez, Luis, 233

  American Astronomical Society, 98, 251

  American Imperial measurement system, 18

  amino acids, 127–28, 223, 227–29, 295–96,

  ammonia

  in carbonaceous chondrites, 225

  in Earth's primordial atmosphere, 123, 126–27,

  experiments with, 212, 222

  in interstellar space, 172–75, 180, 187, 191

  on planets, 261, 301

  anaerobic bacteria, 302

  ancestors

  cosmic, 284

  in family history, 12

  molecular, 291

  remains of, 216

  stars as, 11, 15, 183, 293, 306

  ancient cultures, 13–14,

  Anders, Edward, 207–14, 218

  Annual Reviews in Astronomy and Astrophysics, 105

  Antarctica, 195

  Apollo missions, 133, 166–69, 231, 268, 285

  Apollo 8 mission, 166

  Apollo 11 mission, 167, 201

  Apollo 17 mission, 14

  arachidic acid, 227

  Arecibo radio telescope, 161

  Arizona Radio Observatory, 160, 181

  Armstrong, Neil, 167, 169, 201

  Arrhenius, Svante, 119

  asteroids

  asteroid belt, 198, 207

  Ceres, 220

  impacts on Earth, 232–33,

  meteorites from, 203, 204, 207–208,

  molecules formed in, 239

  origins of, 225

  samples from, 196

  Vesta, 220

  Aston, Francis William, 80

  astrobiology, 27, 121, 224, 285–86,

  Astrobiology Roadmap, NASA, 27

  astrochemistry, 22, 30–31, 180–91, 224, 235

  astrogeology, 199, 205–206, 214–16, 235

  astrometry, 246

  astromineralogy, 156–57,

  Astronomer Royal, 98

  astronomer's periodic table, 102, 105, 205, 280

  astronomy

  and biology, 277, 297

  history of, 28

  popularizers, 31, 79, 89

  positional, 139

  Astrophysical Context of Life (Committee on the Origins and Evolution of Life), 24

  Astrophysical Journal Letters, 279

  astrophysics

  atoms and, 68

  celestial mechanics, 266

  geology and, 214

  history of, 28–30, 57

  molecular, 180, 280

  scientific establishment and, 33–35,

  Asunsolo, Guillermo, 200

  atmospheres

  Earth, 123, 126–30,

  exoplanets, 298–302,

  habitability of, 271

  oxidative, 123, 129

  reducing, 123, 129

  Sun, 54

  water in, 147

  atomic bombs, 81–83, 125

  atomic energy, 80

  Atomic Energy Commission Space Nuclear Systems Office, 181–82,

  atomic physics, 69, 88, 90

  atomic weight, 74, 88

  atoms

  creation of, 281–82,

  electrons, 67, 76, 171, 209, 268, 281–82,

  Greek idea of, 73

  laboratory analysis of, 67–68,

  splitting of, 78–79,

  transmutation of, 78–82,

  ATP (adenosine triphosphate), 230

  Australia, 226

  Aztecs, 306

  B2FH, 100–102,

  Baade, Walter, 91

  Baboquivari Peak, 160

  bacteria

  anaerobic, 302

  fossil and biochemical evidence of, 235

  reproduction, 130

  Bada, Jeffrey, 127–28,

  Bakh, Alexei N., 114

  barium (element), 54, 99

  Barnard, E. E., 138

  Barnard's Star, 248

  Barrett, Alan, 173

  baryonic matter, 281

  bases.See nucleobases

  Batalha, Natalie, 272–74,

  Bell, Jocelyn, 104

  Bell Telephone Company, 162–64, 170, 171

  Benner, Steve, 286–90, 293, 294

  benzene, 188

  Bernstein, Max, 221

  beryllium (element), 84, 93, 94, 102, 281

  Berzelius, Jöns Jacob, 116

  beta decay, 98–99, 101

  Betelgeuse, 155, 304, 305

  Bethe, Hans, 81–84, 100–101,

  big bang

  biological, 283

  cosmic microwaves, 165

  nucleosynthesis, 281

  theory, 14, 60, 82, 86–89, 92, 103

  Biochemical Institute (USSR), 114

  biochemistry, 113–14, 121, 125

  cellular biochemistry, 296

  experiments in, 126

  universal nature of, 295

  biology

  and astronomy, 24, 277, 297

  evolution and, 244

  exoplanets and, 267

  molecular, 128

  in space age, 131–32,

  as subdivision of chemistry, 290

  bismuth (element), 101

  Black Cloud, The (Hoyle), 141

  black holes, 177

  Bohr, Niels, 90, 125, 174

  Bok, Bart, 151–53,

  Bok globules, 151–53,

  border patrol, United
States, 159–60,

  Borucki, William “Bill,” 266–72, 274–75, 307

  Boss, Alan, 256

  Bowen, Ira, 62, 98, 174

  Bradbury, Ray, 267

  Brief History of Time, A (Hawking), 29, 297

  British Association for the Advancement of Science's Royal Institution, 73

  Brownlee, Donald, 197–98,

  B2FH, 100–102,

  Bunsen, Robert, 29, 46–51, 55, 61, 298, 300

  Bunsen burner, 47, 166

  Burbidge, Geoffrey and Margaret, 96–102, 104–105, 183

  Bush, George W., 23, 24

  butadiynyl radical, 186

  cacodyls, 47–48,

  caffeine, 230

  calcium-aluminum-rich inclusions, 204–205,

  calcium-44, 218

  Calcutta, India, 129–30,

  California Institute of Technology (Caltech), 41, 67–69, 83, 92–94, 99, 100, 148, 152, 170, 174

  Caltech.See California Institute of Technology (Caltech)

  Cambridge University, 72, 76, 78–80, 90–91, 147, 289

  Cameron, Alastair, 104

  Campbell, Bruce, 245–53, 255, 257, 269

  Canada

  astronomy funding in, 252

  Grasslands National Park, 135–37,

  National Meteorite Collection, 202

  Canada-France-Hawaii Telescope, 249–50,

  Cannon, Annie Jump, 58, 278

  Cape Canaveral Air Force Station, 272

  caprylic acid, 227

  carbon

  carbon-based molecules, 158, 162, 185

  abundance of, 295

  cosmic origin of, 235–40,

  carbon dioxide, 147, 191, 238, 300

  carbon hydride, interstellar, 166

  carbon monoxide, 173, 179, 187, 283, 301

  in cosmic dust, 142–43, 234

  as element of life, 119–20, 293

  formation of, 101

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

  in stars, 69, 93–95, 178, 282

  carbonaceous chondrites, 203–204, 225–31, 233, 235–39, 291

  carboxylic acid, 226–27,

  Carnegie, Andrew, 41

  Carnegie Fellows, 98

  Carnegie Observatories, 42

  Cassiopeia (constellation), 151, 164

  Cassiopeia A, 155

  Cat's Eye nebula, 185

  Cavendish Laboratory, 76, 80

  Celsius temperature scale, 17

  Ceres (asteroid), 220

  cesium (element), 51

  CfA (Harvard-Smithsonian Center for Astrophysics), 254, 277, 279, 284, 297

 

‹ Prev