levo

Astrophysics

Principles of the use of stellar spectral classes

  • 6 things to know
  • Paper 3, section B

Overview

The classes O through M, their temperatures and colours, and the absorption lines that identify each.

What you need to know

Answer each one before you reveal it.

Your recallNot started
Numbers

What colour, temperature and lines characterise class O and B stars?

Numbers

What lines and temperature characterise class A stars, and what colour is class F?

Numbers

What temperature and lines characterise class F stars, and what colour is class G?

Numbers

What lines and temperature characterise class K stars, and what class is a star at 4,200 K?

Key term

What is the intrinsic colour of spectral class M stars?

Numbers

From which energy level do electrons start when producing Hydrogen Balmer absorption lines?

Questions from this subtopic

Each one with the model answer underneath.

  1. 1

    What is the intrinsic colour of spectral class O stars?

    Model answer

    Blue

  2. 2

    State the temperature range for spectral class O stars.

    Model answer

    25,000–50,000 K

  3. 3

    Which spectral classes share the same intrinsic colour of blue?

    Model answer

    Spectral classes O and B

  4. 4

    Which prominent absorption lines are observed in the spectra of O-type stars?

    Model answer

    He⁺, He, and H

  5. 5

    A star's spectrum shows strong He⁺ absorption lines. What spectral class is it most likely to be?

    Model answer

    Spectral class O

  6. 6

    What is the intrinsic colour of spectral class B stars?

    Model answer

    Blue

Other ways to work this

The same content, four other ways.

What is inside Levo

Six ways to work the same material.

1Closed book
2Open book
3Closed book

The 3-step method, run for you

Answer cold, learn it, then prove it stuck. Levo tracks the jump between your first attempt and your last.

Measurements and Their Errors
Particles and Radiation
Waves
Mechanics and Materials

Cram a whole paper in one sitting

Sort every topic into what you know and what you do not, then drill only the weak ones.

Q is .
positivenegativezero

Blank Blitz makes facts automatic

Rapid timed gap-fills on the terms and numbers you need to recall without thinking.

AP = 4πr²σT⁴.
BThe surface area of a spherical star is 4πr².
CP₁/P₂ = (r₁²/r₂²) × (T₁⁴/T₂⁴).

Build It gets the exam shape right

Assemble a full-mark answer from its marking points, in the order an examiner wants them.

Speed means rate of change of distance.
TrueFalse

Test It catches misconceptions

Spot the fault in a statement. The traps are the mistakes students actually make.

721941163128510

Brain Breaks between sessions

Short focus games to reset attention, so the next set lands better than the last.

Every question in Astrophysics, on a schedule.

Attempt a question from memory, write the correct version, then attempt it again. Levo records the jump between your first attempt and your last, and brings each question back on the day you are due to forget it.

Or £46 a year, about £3.83 a month. Cancel anytime.