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A First Course in Astronomy & Astrophysics

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Category: Resources
Read Time: 16 mins
2025 · Introductory Course

A First Course in Astronomy and Astrophysics

Astronomy and Astrophysics — Flammarion Engraving

This introductory course covers the foundations of astronomy and astrophysics across six structured modules — from the basic tools and techniques of observational astronomy, through stellar physics and evolution, to the large-scale structure of the Milky Way, galaxies, and the Universe as a whole. The course features hands-on activities alongside video lectures and problem sets, making it suitable for undergraduate students, university teachers, and anyone seeking a rigorous first encounter with modern astrophysics.

Meet the speakers
Course Index ▼
Module 1 — Introduction & Tools of Astronomy
  1. Multiwavelength astronomy & Positional astronomy
  2. Positional astronomy – I
  3. Positional astronomy – II
  4. Photometry
  5. Spectroscopy
  6. Observational tools and techniques – I
  7. Observational tools and techniques – II
Module 2 — Hands-on Activities
  1. Creating Color-Composites – I
  2. Creating Color-Composites – II
  3. Creating Color-Color diagrams
  4. Solar Rotation - I
  5. Solar Rotation - II
  6. Solar Rotation - III
  7. Solar Rotation - IV
Module 3 — Stellar Observations & Structure
  1. Stellar observations – I
  2. Stellar observations – II
  3. Hertzsprung-Russell diagram
  4. Stellar structure – I
  5. Stellar structure – II
Module 4 — Stellar Evolution & End States
  1. Stellar evolution – I
  2. Stellar evolution – II
  3. Stellar evolution – III
  4. Stellar evolution – IV
  5. Stellar evolution – V
  6. Stellar evolution – VI
Module 5 — Milky Way & Galaxies
  1. Galaxy morphology
  2. AGN and galaxy groups
  3. Galaxy groups and clusters
  4. The Milky Way galaxy
Module 6 — Cosmology
  1. Cosmology - I
  2. Cosmology - II
  3. Cosmology - III
  4. Cosmology – Hands-on activity

Video Lectures

01Introduction and Tools of Astronomy▼

Lecture 1.1: Multiwavelength astronomy & Positional astronomy

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An introduction to the night sky — constellations, the celestial sphere, right ascension and declination, the ecliptic, and the apparent motion of stars and planets. Practical guide to reading star charts and using planetarium software.

Lecture 1.2: Positional astronomy – I

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Optical design of refracting and reflecting telescopes, key parameters (aperture, focal length, magnification, resolving power), detector types (CCD, CMOS), and an introduction to radio and space-based observatories.

Lecture 1.3: Positional astronomy – II

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Wave and particle nature of light, the electromagnetic spectrum from radio to gamma rays, blackbody radiation and Planck's law, Wien's displacement law, Stefan-Boltzmann law, and the concept of astronomical magnitude.

Lecture 1.4: Photometry

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The cosmic distance ladder — parallax, spectroscopic parallax, Cepheid variables, Type Ia supernovae as standard candles, and Hubble's law. Discussion of units: AU, parsec, light year, and their physical meaning.

Lecture 1.5: Spectroscopy

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Wave and particle nature of light, the electromagnetic spectrum from radio to gamma rays, blackbody radiation and Planck's law, Wien's displacement law, Stefan-Boltzmann law, and the concept of astronomical magnitude.

Lecture 1.6: Observational tools and techniques - I

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Wave and particle nature of light, the electromagnetic spectrum from radio to gamma rays, blackbody radiation and Planck's law, Wien's displacement law, Stefan-Boltzmann law, and the concept of astronomical magnitude.

Lecture 1.7: Observational tools and techniques - II

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Wave and particle nature of light, the electromagnetic spectrum from radio to gamma rays, blackbody radiation and Planck's law, Wien's displacement law, Stefan-Boltzmann law, and the concept of astronomical magnitude.
02Hands-on Activities▼

Activity 2.1: Creating Color-Composites – I

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Guided naked-eye observation session — identifying prominent constellations, the Milky Way band, and key bright stars. Introduction to binocular astronomy: star clusters, double stars, and the Andromeda galaxy.

Activity 2.2: Creating Color-Composites – II

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Hands-on session with equatorial and alt-azimuth mounted telescopes. Polar alignment, star-hopping techniques, eyepiece selection, and focused observation of the Moon, planets, and deep-sky objects.

Activity 2.3: Creating Color-Color diagrams

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Introduction to astronomical image reduction — bias, dark and flat-field corrections, image stacking, and basic photometry using free tools (AstroImageJ / FITS Liberator). Participants process real observational data.

Activity 2.4: Solar Rotation - I

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Introduction to astronomical image reduction — bias, dark and flat-field corrections, image stacking, and basic photometry using free tools (AstroImageJ / FITS Liberator). Participants process real observational data.

Activity 2.5: Solar Rotation - II

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Introduction to astronomical image reduction — bias, dark and flat-field corrections, image stacking, and basic photometry using free tools (AstroImageJ / FITS Liberator). Participants process real observational data.

Activity 2.6: Solar Rotation - III

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Introduction to astronomical image reduction — bias, dark and flat-field corrections, image stacking, and basic photometry using free tools (AstroImageJ / FITS Liberator). Participants process real observational data.

Activity 2.7: Solar Rotation - IV

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Introduction to astronomical image reduction — bias, dark and flat-field corrections, image stacking, and basic photometry using free tools (AstroImageJ / FITS Liberator). Participants process real observational data.
03Stellar Observations and Stellar Structure▼

Lecture 3.1: Stellar observations – I

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Absorption and emission spectra, the Harvard spectral classification (OBAFGKM), luminosity classes, and the Morgan-Keenan system. Spectroscopic determination of stellar temperatures, composition, radial velocities, and binary systems.

Lecture 3.2: Stellar observations – II

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Constructing and interpreting the H-R diagram — the main sequence, giant branch, supergiant and white dwarf regions. Colour-magnitude diagrams of star clusters as probes of stellar age and distance.

Lecture 3.3: Hertzsprung-Russell diagram

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Equations of stellar structure — hydrostatic equilibrium, energy transport (radiation, convection), and nuclear energy generation. The proton-proton chain and CNO cycle. Introduction to stellar models and the mass-luminosity relation.

Lecture 3.4: Stellar structure – I

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Radiative transfer in stellar atmospheres, opacity sources, the photosphere, chromosphere and corona. Solar activity — sunspots, flares, coronal mass ejections — and their relationship to stellar magnetic fields.

Lecture 3.5: Stellar structure – II

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Radiative transfer in stellar atmospheres, opacity sources, the photosphere, chromosphere and corona. Solar activity — sunspots, flares, coronal mass ejections — and their relationship to stellar magnetic fields.
04Stellar Evolution & End State of Stars▼

Lecture 4.1: Stellar evolution – I

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Interstellar medium, molecular clouds, and the Jeans criterion for gravitational collapse. Pre-main sequence contraction, Hayashi tracks, and T Tauri stars. Formation of protoplanetary discs and the initial mass function.

Lecture 4.2: Stellar evolution – II

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Stellar lifetimes on the main sequence as a function of mass, changes in chemical composition, and the evolution of the zero-age main sequence. The Sun as a case study — past, present and future.

Lecture 4.3: Stellar evolution – III

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Subgiant and red giant branch evolution, helium flash, horizontal branch, asymptotic giant branch stars, thermal pulses and mass loss. Planetary nebulae formation and the s-process nucleosynthesis.

Lecture 4.4: Stellar evolution – IV

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Stellar end states — white dwarfs and the Chandrasekhar limit, core-collapse supernovae and neutron stars, pulsars and magnetars, stellar-mass black holes. A brief introduction to gravitational wave sources from compact binary mergers.

Lecture 4.5: Stellar evolution – V

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Stellar end states — white dwarfs and the Chandrasekhar limit, core-collapse supernovae and neutron stars, pulsars and magnetars, stellar-mass black holes. A brief introduction to gravitational wave sources from compact binary mergers.

Lecture 4.6: Stellar evolution – VI

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Stellar end states — white dwarfs and the Chandrasekhar limit, core-collapse supernovae and neutron stars, pulsars and magnetars, stellar-mass black holes. A brief introduction to gravitational wave sources from compact binary mergers.
05Milky Way and Galaxies▼

Lecture 5.1: Galaxy morphology

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Components of the Milky Way — disc, bulge, halo and dark matter halo. Spiral arm structure, star-forming regions, and open and globular cluster distributions. Evidence for a central supermassive black hole (Sgr A*).

Lecture 5.2: AGN and galaxy groups

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The Hubble tuning-fork classification — elliptical, lenticular, spiral and irregular galaxies. Galaxy scaling relations (Tully-Fisher, Faber-Jackson), galaxy clusters and groups, and large-scale structure of the Universe.

Lecture 5.3: Galaxy groups and clusters

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Seyfert galaxies, quasars, blazars and radio galaxies as manifestations of AGN activity. The unified AGN model, accretion disc physics, relativistic jets, and the role of supermassive black holes in galaxy evolution.

Lecture 5.4: The Milky Way galaxy

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Seyfert galaxies, quasars, blazars and radio galaxies as manifestations of AGN activity. The unified AGN model, accretion disc physics, relativistic jets, and the role of supermassive black holes in galaxy evolution.
06Cosmology▼

Lecture 6.1: Cosmology - I

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Observational evidence for an expanding Universe — galaxy redshifts and Hubble's law. The cosmological principle, co-moving coordinates, the scale factor, and Friedmann equations from Newtonian and relativistic perspectives.

Lecture 6.2: Cosmology - II

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Thermal history of the Universe — inflation, baryogenesis, Big Bang nucleosynthesis, recombination and the surface of last scattering, the epoch of reionisation, and structure formation. Successes of the standard hot Big Bang model.

Lecture 6.3: Cosmology - III

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Observational evidence for dark matter — galaxy rotation curves, gravitational lensing, and the Bullet Cluster. Evidence for dark energy from Type Ia supernovae, the cosmic energy budget, and the Lambda-CDM concordance model.

Lecture 6.4: Cosmology – Hands-on activity

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Discovery and properties of the CMB, its near-perfect blackbody spectrum, and temperature anisotropies. The angular power spectrum and what it reveals about cosmological parameters — from the COBE, WMAP, and Planck satellite missions.

Problem Sets

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Problem Set 1: Units, magnitudes, and the electromagnetic spectrum

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Problems on astronomical units and distance scales, the magnitude system, blackbody radiation, and applications of Wien's law and the Stefan-Boltzmann law.

Problem Set 2: Celestial coordinates and telescope optics

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Coordinate conversions between equatorial, ecliptic and galactic systems, resolving power calculations, telescope design problems, and atmospheric seeing.

Problem Set 3: Stellar spectra and the H-R diagram

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Spectral classification problems, use of the H-R diagram to determine stellar properties, and colour-magnitude diagram analysis of star clusters.

Problem Set 4: Stellar structure and energy generation

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Hydrostatic equilibrium, nuclear timescales, energy generation rate calculations, and simple models of stellar interiors including the mass-luminosity relation.

Problem Set 5: Stellar evolution and end states

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Main sequence lifetimes, post-main sequence tracks on the H-R diagram, the Chandrasekhar limit, and problems on neutron star and black hole properties.

Problem Set 6: Galaxies and large-scale structure

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Galaxy rotation curves and evidence for dark matter, the Tully-Fisher relation, galaxy cluster dynamics, and problems on the distance ladder.

Problem Set 7: Cosmology

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Friedmann equation solutions, Hubble time calculations, Big Bang nucleosynthesis, CMB temperature and anisotropies, and the cosmic energy budget in the Lambda-CDM model.

Additional Resources

Supplementary reading lists, software guides, and data sets for the hands-on activities.

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