levo

Orbits and the Wider Universe

Masses in a double system from radial velocity data

  • 3 things to know
  • Component 2

Overview

Recall questions on obtaining the orbital speeds from the radial velocity curve, the ratio of the masses from the ratio of the speeds, combining that with the period to find each mass, and worked determinations for a spectroscopic binary.

What you need to know

Answer each one before you reveal it.

Your recallNot started
Key term

Why does the same period for both bodies make the speed ratio equal to the radius ratio?

Key term

Why must a double system be viewed edge on for the radial velocity method to give true masses?

Key term

What is obtained instead of the true mass when the tilt of the orbit is unknown?

Questions from this subtopic

Each one with the model answer underneath.

  1. 1

    State the relationship between the orbital speeds and the masses of the two bodies in a double system.

    Model answer

    The relationship is M₁v₁ = M₂v₂, because both bodies circle the centre of mass in the same period and their orbital radii are in inverse proportion to their masses.

  2. 2

    Why does the same period for both bodies make the speed ratio equal to the radius ratio?

    Model answer

    Each body's speed is 2πr/T with the same T, so the speeds are in the same ratio as the orbital radii about the centre of mass.

  3. 3

    Why must a double system be viewed edge on for the radial velocity method to give true masses?

    Model answer

    Only the component of the orbital velocity along the line of sight produces a Doppler shift, so any tilt of the orbital plane makes the measured speed smaller than the true orbital speed.

  4. 4

    What is obtained instead of the true mass when the tilt of the orbit is unknown?

    Model answer

    A lower limit on the mass is obtained, since the measured radial velocity can only be equal to or less than the true orbital speed.

  5. 5

    State the equation relating a body's orbital speed to its orbital radius about the centre of mass and the period.

    Model answer

    The relationship is v = 2πr/T, so the orbital radius is r = vT/2π.

  6. 6

    How is the separation of the two bodies in a double system found from their two orbital speeds and the period?

    Model answer

    Each orbital radius is found from r = vT/2π, and the separation is the sum of the two radii, d = (v₁ + v₂)T/2π.

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.

Basic Physics
Kinematics
Dynamics
Energy Concepts

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.

The wires .
attractrepeltwist

Blank Blitz makes facts automatic

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

AThe equation is pV = NkT.
BThe pressure, p, is in Pa.
CThe volume V is in m³.

Build It gets the exam shape right

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

The joule is a unit of energy.
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 Orbits and the Wider Universe, 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.