Units for Astronomical Distances (OCR A Level Physics): Revision Note

Exam code: H556

Katie M

Written by: Katie M

Reviewed by: Caroline Carroll

Updated on

Units for Astronomical Distances

  • Astronomical distances are very large and as a result, are usually measured using:

    • Astronomical Units (AU)

    • Light–years (ly)

    • Parsecs (pc)

Astronomical Unit (AU)

  • The astronomical unit (AU) is defined as

    The mean distance from the centre of the Earth to the centre of the Sun

  • As the Earth’s orbit around the Sun is elliptical it will be slightly closer to the Sun in January (1.471 × 1011 m) than it is in July (1.521 × 1011 m)

  • Calculating the mean of these two values gives:

(1.471×1011)+(1.521×1011)2 = 1.496 × 1011 m

  • Therefore, 1 astronomical unit = 1.496 × 1011 m ≈ 1.5 × 1011 m

  • The astronomical unit is useful for studying distances on the scale of the solar system

5-12-1-au_ocr-al-physics

Light–year (ly)

  • A light-year is defined as:

    The distance travelled by light in one year

  • This can be calculated using:

Distance = speed × time

  • Where:

    • The speed of light is 3 × 108 m s–1

    • 1 year = 60 × 60 × 24 × 365 = 3.15 × 107 s

  • Hence, the distance travelled by light in one year = (3 × 108) × (3.15 × 107) = 9.46 × 1015 m

    • Therefore, 1 light–year ≈ 9.5 × 1015 m

Parsec (pc)

  • Angles smaller than 1 degree can be measured in arcminutes or arcseconds

    • 1 degree = 60 arcminutes

    • 1 arcminute = 60 arcseconds

    • Therefore, 1 degree = 60 x 60 = 3600 arcseconds

    • 1 arcsecond = 1/3600 degree

  • The parsec is defined as

    A unit of distance that gives a parallax angle of 1 second of an arc (of a degree), using the radius of the Earth’s orbit (1 AU) as the baseline of a right–angled triangle

5-12-1-parsec_ocr-al-physics
  • Given that 1 AU = 1.496 × 1011 m, trigonometry can be used to express 1 parsec in metres:

tanθ = oppadj = 1 AU1 pc

tan(13600) = 1 AU1 pc

1 pc = 1 AUtan(13600) = 1.496 ×1011tan(13600) = 3.09 × 1016 m

  • Therefore, 1 parsec ≈ 3.1 × 1016 m

  • The parsec (1 pc = 3.1 × 1016 m) and the light-year (1 ly = 9.5 × 1015 m) are much greater in size than the astronomical unit (1 AU = 1.496 × 1011 m)

  • This makes them useful when studying interstellar distances

    • For example, on the scale of distances between the Earth and stars, or neighbouring galaxies

Worked Example

The closest star to Earth is a triple–star system called Alpha Centauri, which is approximately 4.35 light-years from Earth. 

Calculate the distance between the Earth and Alpha Centauri in:

a) Astronomical units

b) Parsecs

An astronomical unit is 1.496 × 1011 m

Answer:

Part (a)

Step 1: List the known quantities

  • 1 light-year ≈ 9.5 × 1015 m (from data booklet)

  • 1 AU = 1.496 × 1011 m

  • Distance to Alpha Centauri = 4.35 ly

Step 2: Convert 4.35 light–years into metres

  • 4.35 ly = 4.35 × (9.5 × 1015) = 4.13 × 1016 m

Step 3: Convert from metres into AU

  • 4.13 × 1016 m = 4.13×10161.496×1011 = 2.8 × 105 AU (to 2 s.f)

Part (b)

Step 1: List the known quantities

  • 1 parsec ≈ 3.1 × 1016 m (from data booklet)

  • 4.35 ly = 4.13 × 1016 m (from part a)

Step 2: Convert from metres into parsecs

  • 4.13 × 1016 m = 4.13 × 10163.1 × 1016 = 1.3 pc (to 2 s.f)

Examiner Tips and Tricks

You do not need to learn all of the conversion factors for astronomical distances, you just need to know how to use them! The following are given in the data booklet:

1 light–year ≈ 9.5 × 1015 m

1 parsec ≈ 3.1 × 1016 m

However, the astronomical unit (AU) is not, so this could be useful to learn by heart!

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Katie M

Author: Katie M

Expertise: Curriculum Expert

Katie has always been passionate about the sciences, and completed a degree in Astrophysics at Sheffield University. She decided that she wanted to inspire other young people, so moved to Bristol to complete a PGCE in Secondary Science. She particularly loves creating fun and absorbing materials to help students achieve their exam potential.

Caroline Carroll

Reviewer: Caroline Carroll

Expertise: Head of Content Delivery

Caroline graduated from the University of Nottingham with a degree in Chemistry and Molecular Physics. She spent several years working as an Industrial Chemist in the automotive industry before retraining to teach. Caroline has over 12 years of experience teaching GCSE and A-level chemistry and physics. She is passionate about delivering high-quality resources to help students achieve their full potential.