ASTRO 200g – Lecture 2A & 2B Notes: Science, Non-Science & Mātauranga

Learning Outcomes

  • Students should be able to:
    • Reflect on the historical context and current frontiers of astrobiology.
    • Define science, distinguish hypothesis vs theory, and recognise what is not science.
    • Convey a basic understanding of Mātauranga (knowledge of everything visible in the Universe).
    • Explain how Mātauranga relates to Western science.
    • Communicate core ideas of pūrākau (myth/ancient story) and maramataka (lunar calendar; literally “turning of the Moon”).
    • Show a basic grasp of mauri (life-force/essence) in Nature.
  • Required reading: Hikuroa, D. (2017) “Mātauranga Māori—the ūkaipō of knowledge in New Zealand”, JR Soc NZ, 47(1), 5-10.

Key Numerical & Unit References (cheat-sheet)

  • Age of Universe: 13.8Gyr13.8\,\text{Gyr} (billion years).
  • Observable radius: 46Gly46\,\text{Gly} (giga-light-years; 1Gly=109ly1\,\text{Gly}=10^{9}\,\text{ly}).
  • 1 light-year: 9×1012km9\times10^{12}\,\text{km}.
  • Speed of light: 3\times10^{5}\,\text{km\,s^{-1}}.

The Universe & Life – Three Contextual Facts

  • 1️⃣ Vast & Old
    • Universe likely infinite; we see out to 46Gly46\,\text{Gly}; formed 13.8Gyr13.8\,\text{Gyr} ago.
  • 2️⃣ Elements of Life Are Widespread
    • Spectroscopy detects C, H, O, N, P, S, amino acids & complex organics in nebulae, meteorites, comets.
  • 3️⃣ Physical Laws Are Universal
    • Identical physics/chemistry everywhere ⇒ plausible that biology obeys similar constraints.

Biology as a Confluence

  • Biology = Physics + Chemistry set within a planet’s geology.
  • If physical/chemical laws are universal, biology might be universal too.
  • Life on Earth is resilient:
    • Found in virtually every environment (deep-sea vents, Antarctica, acidic hot springs).
    • Ancient fossils prove organisms thrived under very different atmospheric/oceanic conditions.
    • Hence, extraterrestrial life need not resemble modern terrestrial life.

Historical Context of Astrobiology

Early Philosophical Speculations
  • Metrodorus of Chios (4th c. BC): atomic theory; argued multiple worlds are more plausible than a single world—analogy: “one ear of wheat in a vast plain.”
Renaissance & Persecution
  • Giordano Bruno (1548-1600): advocated “plurality of worlds”; envisioned innumerable suns with orbiting Earth-like planets; executed for heresy.
20th-Century Physics & Life Definition
  • Erwin SchrödingerWhat is Life? (1944): described life thermodynamically as creation of order from disorder (“negative entropy”).
    • Tied biology to the 2nd Law of Thermodynamics: living systems export entropy to maintain internal order.
Classical Misconceptions
  • Late 19th-century astronomy: canals on Mars (Schiaparelli → Lowell) & swampy Venus; shown later to be observational artefacts.
  • Carl Sagan (1978) highlighted these as lessons in scientific humility.
Birth of Empirical Astrobiology – Space Age
  • 1965 Mariner 4 fly-by imaged cratered, arid Mars ⇒ shattered assumptions of a thriving Martian civilisation.
  • 1970s Viking Landers: first in-situ life-detection experiments on Mars.
Modern Discoveries & Frontiers
  • Enceladus: Cassini detected south-polar water plumes ⇒ subsurface ocean, hydrothermal energy, potential habitability.
  • Exoplanets:
    • Transit & radial-velocity surveys revealed thousands of planets, including rocky worlds in habitable zones.
    • Goal: statistically assess how common Earth-like planets are and search for atmospheric biosignatures (e.g., O<em>2O<em>2, CH</em>4CH</em>4 disequilibria).

Nature of Scientific Inquiry

  • Science: systematic pursuit of patterns in Nature to make testable, predictive models.
  • Assumes the Universe is consistent & predictable.
  • Data acquired via repeatable observation & measurement (empiricism).
The Scientific Method (core tool)
  1. Observation of a phenomenon.
  2. Formulate a hypothesis (tentative, testable explanation).
  3. Derive predictions that should hold if hypothesis is correct.
  4. Test via further observation/experiment.
  5. If predictions fail ⇒ improve or discard hypothesis.
  6. Iterate; develop broader, simpler models.
Hypothesis vs Theory vs Fact
  • Hypothesis: untested, specific, falsifiable proposition.
  • Theory: broad, simple model explaining diverse data; repeatedly validated, yet always open to refinement (e.g., Gravity, Evolution, Plate Tectonics).
  • Fact: direct observation (e.g., apple falls); theory explains why.

Hallmarks of Science

  1. Seeks explanations via natural causes.
  2. Makes testable predictions.
  3. Permits falsification through observation/experiment.
Pseudoscience
  • Appears scientific but lacks one or more hallmarks; e.g., UFO mythology, Martian “face”, astrology, some cosmetic claims.
Non-Science
  • Realms outside empirical testing: religion, ethics, aesthetics—valuable but use different epistemologies.

Mātauranga Māori – Another Way of Knowing

  • Indigenous knowledge system encompassing astronomy, ecology, medicine, genealogy, ethics.
  • Methodologies include:
    • Pūrākau – narrative encoding ecological & cosmological data.
    • Maramataka – lunar phases guiding planting, fishing, ritual.
    • Observation over generations, calibrated by environmental feedback—empirical within its context, though packaged differently from Western science.
  • Relationship to Science
    • Complementary: Mātauranga provides long-term data sets, ethical frameworks (e.g., kaitiakitanga/guardianship) that can enrich scientific inquiry.
    • Differences: holistic vs reductionist; spiritual aspects (mauri) intertwined with physical observations.

Ethical, Philosophical & Practical Implications

  • Search for life raises questions of planetary protection, contamination, and stewardship of other worlds.
  • Historical missteps (e.g., Bruno’s execution, canal myth) illustrate dangers of dogma & biased interpretation.
  • Integrating Mātauranga promotes inclusivity, decolonises research, and anchors science within cultural responsibility.

Equations, Laws & Key Terms Quick-Find

  • Speed of light: c = 3\times10^{8}\,\text{m\,s^{-1}}.
  • Entropy change: \Delta S > 0 for isolated systems (2nd Law).
  • Negative entropy (life): local \Delta S < 0 by exporting heat/waste.
  • Light-year distance: d=c×t1yeard = c \times t_{1\,\text{year}}.
  • Habitability factors: liquid water, energy source, essential elements, time.

Connections to Previous & Future Lectures

  • Builds on Lecture 1’s cosmic timeline by zooming into life’s requirements.
  • Prepares for upcoming units on extremophiles, planetary missions, and detailed Mātauranga case studies (e.g., Matariki star cluster timing harvests).