Astronomy 1P1 - Introduction to Astronomy
Course Introduction
- Instructor: Professor Barak Shashani
- Course: Astronomy 1P1 at Brock University
- Lecture goals:
- Introduction to basic concepts in science and astronomy.
- Overview of fascinating topics to be covered.
- Discussion on scales of the universe.
What is Astronomy?
- Study of celestial objects outside Earth:
- Planets, moons, asteroids, comets, stars, black holes, galaxies, and the universe.
- Astronomy is a science:
- Science is not a body of knowledge, but a method for obtaining and verifying knowledge.
- Involves making observations, experiments, and creating hypotheses.
- Hypotheses lead to predictions tested experimentally.
- Verified hypotheses become theories.
- Theories help understand the universe, predict events, and create new technologies.
- Science is self-correcting; skepticism is key.
The Scientific Method
- Process of creating and testing hypotheses.
- Scientists remain skeptical until sufficient evidence supports a hypothesis.
- No theory is sacred; new evidence may lead to new theories.
Evolution of Astronomical Models
- Ancient geocentric model with Earth at center was replaced by heliocentric model.
- The sun is at the center of the solar system, not the universe.
- Astronomy evolves with new theories and precise instruments.
Unanswered Questions in Astronomy
- Dark matter and dark energy.
- Center of a black hole.
- Existence of life on other planets.
Limitations and Tools in Astronomy
- Astronomers can't do lab experiments, can only observe using telescopes.
- Improvements in technology lead to better, detailed observations.
- Use of instruments for different types of electromagnetic radiation.
Professor's Research: General Relativity
- Provides description of gravity, space, and time.
- Revolutionized astronomy by introducing black holes, gravitational lensing, and waves.
Measuring Distances in Astronomy
- Lightyear: Distance light travels in one year.
- Light travels at 300,000 km/s or 1 billion km/h.
- One lightyear ≈ 9.5 trillion km.
Astronomical Distances
- Distances like the Orion Nebula (1300 lightyears away).
- Observing celestial objects is like looking into the past.
- Time machine analogy for observing distant objects.
Tour of the Universe
- Earth: Diameter ≈ 13,000 km.
- Moon: Diameter ≈ 3,500 km; Distance from Earth ≈ 384,000 km.
- Sun: A star with nuclear reactions generating energy.
- Proxima Centauri: Nearest star (4.2 lightyears away).
- Solar System Planets: Mercury through Neptune.
- Galaxies: Collections of billions of stars.
- Milky Way Galaxy: 100-400 billion stars.
- Andromeda Galaxy: 2.5 million lightyears away.
Large Scale Structures
- Local Group: Includes Milky Way and Andromeda.
- Virgo Supercluster: Part of the Laniakea Supercluster.
- Laniakea Supercluster: Contains over 100,000 galaxies.
The Big Bang and Universe Expansion
- Universe began 13.8 billion years ago from a dense state.
- Expansion started in the Big Bang.
- Observable universe: Sphere with 93 billion light-year diameter.
Misconceptions and Limits
- Expansion is not into anything; distances are increasing.
- Observable universe is limited by light travel time.
- Universe might be infinite or cyclic.
Smallest and Largest Scales in the Universe
- Elementary particles: Electrons, quarks (up, down).
- Protons/neutrons made of quarks.
- Electrons ≈ less than 10^-22 meters.
- Observable universe ≈ 10^24 km.
- Humans located in the middle of these scales.
Potential for Human Space Travel
- Current technology limits human travel to the solar system.
- Andromeda and further galaxies unreachable with current technology.
Time Scales
- Universe: 13.8 billion years.
- Humans evolved 300,000 years ago.
- Recorded history 5,000 years.
- Visual analogy: Universe year; humans appear on December 31st.
Reading and Further Exploration
- Recommended textbook: OpenStax Astronomy.
- Chapter 1 and appendices A-D for further reading.
- Lectures are primary material for exams.
- Further exploration resources are available for deeper understanding.
These notes provide an overview of the key concepts and ideas discussed in the initial lectures on astronomy.