Astronomy/Mathematics MSci

University of Glasgow · honours · 5 years · optional year abroad · UCAS 3110course page ↗

AAB – BBB at A level, A-level Mathematics and Physics; graduates earn a median £30,000 three years on.

Typical A level offer
AAB – BBB

A-level Mathematics and Physics · 80% of entrants came with A levels · 80% stay on after year 1 · Glasgow course page, Discover Uni

Year 13 · applying

What do you need to get in?

AAB – BBBtypical A level offer

Typical offer — the grades most applicants are asked for. A contextual offer can be lower for applicants from under-represented backgrounds; none is published for this course.

Glasgow course page, read 19 September 2026 · Discover Uni entry profile

  1. 1A-level Mathematics and Physics
Who actually got in: 80% with A levels, 15% via Access courses. 45% arrived with 208 or more UCAS tariff points — roughly A*A*A or better. Based on 45 entrants.

UCAS tariff points — a points scale for grades: A* = 56, A = 48, so A*A*A = 160. Entrants’ totals include extra subjects.

Other qualifications2
QualificationTypical offerRequired subjects
Scottish HighersAAAAAminimum from S5: BBBBHigher Mathematics and Physics at AA. (AB may be considered).
IB34 (6,5,5)HL Mathematics (Analysis & Approaches) and Physics.
Years 1–5

What do you study?

2compulsory modules in year 1

Compulsory modules this year: mathematics & statistics 48% · natural sciences 39% · transversal skills 9% · language & communication 4%.

Module — one course unit, usually a term or a year long; “core” means everyone takes it. One UK credit is about ten hours of study; a full year is 120 credits.

Glasgow course page · optional modules vary by year

Year 1 · 2 core · 80 credits ≈ 800 hours
  • Astronomy 1
    What you learn (31)
    • describe the origin and structure of the solar system
    • state the law of blackbody radiation
    • state the laws of gravitation
    • state the gas laws
    • apply physical laws to explain properties of solar system bodies
    • explain the formation and evolution of the solar system using physical laws
    • state formulae of spherical trigonometry
    • apply spherical trigonometry to planetary motion and navigation
    • describe different astronomical coordinate systems
    • convert between different astronomical coordinate systems
    • solve problems on the apparent motion of stars
    • state basic concepts of newtonian gravitation
    • calculate surface gravity and escape velocity using gravitational concepts
    • determine properties of planetary orbits using gravitational theory
    • describe the electromagnetic spectrum and its units
    • describe sky properties across different spectral regions
    • explain the operation and properties of telescopes
    • evaluate quantitative properties of telescopes and instrumentation
    • describe the main types of stars and their spectral classification
    • describe the hertzsprung-russell diagram
    • state physical principles underlying main sequence star models
    • relate stellar evolution to the hertzsprung-russell diagram
    • describe the process of gravitational collapse
    • list observational evidence for stellar end states
    • describe properties of the main galaxy types
    • describe large scale structures and their relative scales in the universe
    • explain the big bang model
    • evaluate the big bang model against cosmological observations
    • conduct practical investigations in astronomy
    • analyse observational data from astronomical investigations
    • report findings of astronomical investigations in writing
    ASTRO1001 40 cr
  • Mathematics 1
    What you learn (18)
    • communicate mathematical ideas using sets, functions, relations and groups
    • identify the components of a mathematical statement such as hypotheses and conclusions
    • construct valid proofs using direct argument, induction, contradiction or counterexample
    • solve equations and inequalities across number systems and geometric settings
    • solve differential equations using algebraic and calculus techniques
    • define groups and subgroups and recognise their properties
    • perform group operations using cycle notation for permutation groups
    • calculate the order of groups and elements using Lagrange's theorem
    • derive derivatives and integrals from first principles using limits
    • relate differentiation and integration through the fundamental theorem of calculus
    • compute derivatives of scalar and vector functions using standard rules
    • compute integrals using substitution, parts and other standard methods
    • apply calculus techniques to solve optimisation and geometric measurement problems
    • perform matrix and vector operations in three-dimensional space
    • model real-world problems using mathematical tools and interpret the solutions
    • extract key concepts and methods from independent reading of mathematical texts
    • present mathematical arguments in writing with precise notation and clear conclusions
    • collaborate with peers to discuss and solve mathematical problems
    MATHS1017 40 cr
Year 2 · 4 core · 60 credits ≈ 600 hours
  • Astronomy 2
    What you learn (8)
    • describe modern astronomical observation methods
    • perform astronomical observations using laboratory instruments
    • collect and process astronomical data
    • explain stellar classification schemes
    • identify spectral features of stars
    • apply theoretical and statistical concepts to interpret astrophysical radiation
    • solve astrophysical problems using statistical and theoretical models
    • describe underlying principles of general relativity
    ASTRO2001 30 cr
  • Mathematics 2A: Multivariable Calculus
    What you learn (14)
    • sketch three-dimensional surfaces using cross-sections and contour lines
    • apply the chain rule to differentiate partial derivatives
    • determine stationary points of multivariable functions
    • apply Lagrange multipliers to solve constrained optimisation problems
    • state the definitions of divergence, gradient and curl operators
    • apply vector differential operators to solve problems
    • compute signed volume under a surface via double integration
    • determine integration limits for a given domain
    • change the order of integration and apply jacobian-based variable substitution
    • compute line integrals along curves
    • parametrise surfaces and compute surface integrals
    • apply Green's theorem to evaluate closed line integrals
    • state key mathematical definitions, results and formulae from lectures
    • apply lecture results and formulae to solve new problems
    MATHS2001 10 cr
  • Mathematics 2B: Linear Algebra
    What you learn (18)
    • state fundamental properties of matrices and their operations
    • apply matrix operations and symbolic manipulation to solve problems
    • determine whether a given set forms a vector subspace
    • determine whether a set of vectors is linearly independent
    • describe the span of a set of vectors
    • determine whether a map between vector spaces is linear
    • derive the matrix representation of a linear map for given bases
    • calculate a matrix determinant using cofactor expansion
    • prove properties of determinants under row or column operations
    • derive the characteristic polynomial of a square matrix
    • compute eigenvalues and eigenvectors of a matrix
    • apply eigenvalues and eigenvectors to solve problems
    • derive the quadratic form associated with a symmetric matrix
    • determine the rank and signature of a symmetric matrix
    • diagonalise a symmetric matrix
    • apply the Gram-Schmidt process to construct an orthonormal basis
    • state key definitions and theorems covered in the module
    • apply covered theorems and definitions to solve problems
    MATHS2004 10 cr
  • Mathematics 2D: Mathematical Methods and Modelling
    What you learn (7)
    • analyse dynamical systems with one dependent variable using ODE models
    • construct phase portraits for single-variable dynamical systems
    • solve linear autonomous ODE systems using matrix exponentials
    • compute Fourier series and Fourier and Laplace transforms
    • apply transform properties to simplify and solve differential equations
    • state key definitions, results and formulae taught in the module
    • apply taught formulae and methods to solve new problems
    MATHS2033 10 cr
Year 3 · 9 core · 135 credits ≈ 1,350 hours
  • Astronomy Skills 1
    What you learn (6)
    • write code or use astronomical software to solve astrophysics problems
    • design and carry out experiments with laboratory and astronomical equipment
    • assess the uncertainty associated with experimental measurements
    • search library and online databases to compile a scientific literature review
    • deliver a multimedia presentation on a researched topic
    • apply logical reasoning to solve scientific problems
    ASTRO4003P 15 cr
  • Heliophysics and Stellar Atmospheres
    What you learn (3)
    • describe key processes and relationships in heliophysics and stellar atmospheres
    • analyse quantitatively astrophysical processes using relevant techniques
    • apply astrophysical laws and techniques to solve unfamiliar problems
    ASTRO4005 15 cr
  • Cosmology
    What you learn (3)
    • describe key processes and relationships in cosmology
    • analyse cosmological phenomena using quantitative methods
    • apply cosmological techniques to solve problems including unfamiliar cases
    ASTRO4006 15 cr
  • Exploring Planetary Systems
    What you learn (3)
    • describe key processes and relationships in planetary systems
    • analyse planetary phenomena using quantitative methods
    • apply astrophysical techniques to solve unfamiliar problems
    ASTRO4007 15 cr
  • Galaxies
    What you learn (3)
    • describe key physical processes and relationships governing galaxies
    • analyse quantitatively astrophysical processes and techniques related to galaxies
    • apply galactic astrophysics concepts to solve unfamiliar problems
    ASTRO4008 15 cr
  • High Energy Astrophysics
    What you learn (3)
    • describe key processes and relationships in high energy astrophysics
    • analyse astrophysical processes quantitatively using relevant techniques
    • apply astrophysical concepts to solve unfamiliar problems
    ASTRO4009 15 cr
  • Instruments for Optical and Radio Astronomy
    What you learn (3)
    • describe key instrumentation concepts for optical and radio astronomy
    • analyse quantitatively processes and techniques relevant to astronomical instruments
    • apply relevant techniques to solve unfamiliar problems in astronomical instrumentation
    ASTRO4010 15 cr
  • Stellar Structure and Evolution
    What you learn (3)
    • describe key processes and relationships in stellar structure and evolution
    • analyse stellar astrophysical processes using quantitative methods
    • apply astrophysical techniques to solve unfamiliar stellar problems
    ASTRO4011 15 cr
  • Astronomical Data Analysis
    What you learn (2)
    • describe key processes and techniques in astronomical data analysis
    • apply quantitative techniques to solve astronomical data problems
    ASTRO4013 15 cr
Year 4 · 6 core · 95 credits ≈ 950 hours
  • Astronomy Skills 2
    What you learn (5)
    • design and carry out experiments using laboratory and astronomical instruments
    • assess uncertainties in experimental measurements
    • search library and web databases to review scientific literature
    • produce a written report presenting a researched scientific topic
    • apply logical reasoning to solve scientific problems
    ASTRO4004P 15 cr
  • Astronomy Project for 4M Students
    What you learn (6)
    • write code or use astronomical software to analyse data and solve problems
    • plan and carry out experimental investigations using laboratory or astronomical equipment
    • evaluate measurement uncertainties and computational errors in experiments
    • prepare a written project report situating findings within wider research context
    • design and deliver an oral presentation on project work
    • apply logical reasoning to solve scientific problems
    ASTRO4020P 20 cr
  • General Relativity and Gravitation
    What you learn (3)
    • explain key concepts and principles of general relativity and gravitation
    • relate topics in general relativity to concepts from other physics courses
    • analyse quantitatively physical processes and relationships using relativistic techniques
    ASTRO5001 15 cr
  • Pulsars and Supernovae
    What you learn (2)
    • describe key physical processes underlying pulsars and supernovae
    • analyse quantitatively relationships and techniques relevant to pulsars and supernovae
    ASTRO5002 15 cr
  • Statistical Astronomy
    What you learn (2)
    • describe core concepts and methods in statistical astronomy
    • relate statistical astronomy topics to concepts from other astrophysics courses
    ASTRO5003 15 cr
  • Plasma Theory and Diagnostics
    What you learn (3)
    • describe core concepts of plasma theory and diagnostic techniques
    • analyse quantitatively plasma processes and relationships using relevant techniques
    • apply plasma theory concepts to solve advanced or unfamiliar problems
    ASTRO5004 15 cr
Year 5 · 4 core · 60 credits ≈ 600 hours
  • General Relativity and Gravitation
    What you learn (3)
    • explain key concepts and principles of general relativity and gravitation
    • relate topics in general relativity to concepts from other physics courses
    • analyse quantitatively physical processes and relationships using relativistic techniques
    ASTRO5001 15 cr
  • Pulsars and Supernovae
    What you learn (2)
    • describe key physical processes underlying pulsars and supernovae
    • analyse quantitatively relationships and techniques relevant to pulsars and supernovae
    ASTRO5002 15 cr
  • Statistical Astronomy
    What you learn (2)
    • describe core concepts and methods in statistical astronomy
    • relate statistical astronomy topics to concepts from other astrophysics courses
    ASTRO5003 15 cr
  • Plasma Theory and Diagnostics
    What you learn (3)
    • describe core concepts of plasma theory and diagnostic techniques
    • analyse quantitatively plasma processes and relationships using relevant techniques
    • apply plasma theory concepts to solve advanced or unfamiliar problems
    ASTRO5004 15 cr

“What you learn” restates each module’s published learning outcomes in our own words, as short skill statements in the same form as the GCSE and A level curriculum, with the help of an AI model; fields of knowledge follow the twelve fields of the knowledge sphere. The university’s module page, linked from each title, is the authoritative description.

After graduating

Where does it lead?

£30,000median pay three years after graduating
Lower quarter£25k
Median£30k
Upper quarter£34k

Median — the middle earner: half earned more, half less. Pay is for graduates of this subject at this university who finished in 2016-18, not adjusted for inflation; based on 90 graduates.

Discover Uni dataset (HESA and Office for Students, CC BY 4.0, contains HESA data); earnings from the Longitudinal Education Outcomes data (Department for Education) · aggregation level 23, 13, 22

Half of graduates earned between £24,500 and £33,500. Five years on, the median is £37,000. 85% were in work or further study 15 months after finishing; 65% of those in work were in professional or managerial jobs.

All outcome figures7
MeasureValueBased on
Continue after year 120% left80%30
In work or study, 15 months on15% studying85%20
Professional or managerial job65%10
Pay 15 months on, median£30,00030
Pay 3 years on, median£30,00090
Pay 5 years on, median£37,000100
Money

What does it cost?

Fees not on file; see the university’s fees page.

Glasgow fees page

National Student Survey 2025-26

What do students say?

62%agreed the course was good overall (question 26)

NSS — a yearly survey of final-year students at every UK university; 65% of this course’s final year answered. Small groups can swing a lot year to year.

National Student Survey, via Discover Uni · 45 students answered

Highest: 100% agreed on question 21; lowest: 42% on question 14.

All questions26
QuestionAgree
Question 193%
Question 269%
Question 395%
Question 488%
Question 580%
Question 683%
Question 772%
Question 873%
Question 972%
Question 1058%
Question 1176%
Question 1262%
Question 1369%
Question 1442%
Question 1595%
Question 1692%
Question 1770%
Question 1879%
Question 1986%
Question 2092%
Question 21100%
Question 2285%
Question 2387%
Question 2469%
Question 2588%
Question 2662%

Question texts are published by the Office for Students; the dataset carries only the question numbers.

Modules, entry requirements and fees are facts read from University of Glasgow’s course page on 2026-09-19 and may change; the university’s page is authoritative. Descriptions are not reproduced. Outcome figures are from the Discover Uni dataset. University of Glasgow is a trade mark of the university; sch.today is independent of it.