Mean radius explained

The mean radius (or sometimes the volumetric mean radius) in astronomy is a measure for the size of planets and small Solar System bodies. Alternatively, the closely related mean diameter (

D

), which is twice the mean radius, is also used. For a non-spherical object, the mean radius (denoted

R

or

r

) is defined as the radius of the sphere that would enclose the same volume as the object.[1] In the case of a sphere, the mean radius is equal to the radius.

For any irregularly shaped rigid body, there is a unique ellipsoid with the same volume and moments of inertia.[2] The dimensions of the object are the principal axes of that special ellipsoid.[3]

Calculation

2D

The area of a circle of radius R is

\piR2

. Given the area of an non-circular object A, one can calculate its mean radius by setting

A=\pi

2
R
mean
or alternatively

Rmean=\sqrt{

A
\pi
}

For example, a square of side length L has an area of

L2

. Setting that area to be equal that of a circle imply that

Rmean=\sqrt{

1
\pi
} L \approx 0.3183 L

a

and semi-minor axis

b

has mean radius

Rmean=\sqrt{ab}

.

For a circle, where

a=b

, this simplifies to

Rmean=a

.

3D

The volume of a sphere of radius R is

4
3

\piR3

. Given the volume of an non-spherical object V, one can calculate its mean radius by setting

V=

4
3

\pi

3
R
mean
or alternatively

Rmean=\sqrt[3]{

3V
4\pi
}

For example, a cube of side length L has a volume of

L3

. Setting that volume to be equal that of a sphere imply that

Rmean=\sqrt[3]{

3
4\pi
} L \approx 0.6204 L

Similarly, a tri-axial ellipsoid with axes

a

,

b

and

c

has mean radius

Rmean=\sqrt[3]{abc}

.[1] The formula for a rotational ellipsoid is the special case where

a=b

.

Likewise, an oblate spheroid or rotational ellipsoid with axes

a

and

c

has a mean radius of
2
R
mean=\sqrt[3]{a

c}

.

For a sphere, where

a=b=c

, this simplifies to

Rmean=a

.

Examples

R=\sqrt[3]{6378.12 ⋅ 6356.8}=6371.0km

. The equatorial and polar radii of a planet are often denoted

re

and

rp

, respectively.[4]

D=\sqrt[3]{360 ⋅ 294 ⋅ 254}=300km

.[5],

See also

Notes and References

  1. Distorted, nonspherical transiting planets: impact on the transit depth and on the radius determination. J.. Leconte. D.. Lai. G.. Chabrier. Astronomy & Astrophysics. 528. A41. 2011. 9. 10.1051/0004-6361/201015811. 1101.2813 . 2011A&A...528A..41L .
  2. Book: https://perso.math.u-pem.fr/pajor.alain/recherche/docs/Mil-Paj-isot.pdf . V. D.. Milman. A.. Pajor. Geometric Aspects of Functional Analysis . Isotropic position and inertia ellipsoids and zonoids of the unit ball of a normed n-dimensional space . . 65–66 . 1987–88. 1376 . Springer. Berlin, Heidelberg. 10.1007/BFb0090049. 978-3-540-51303-2 .
  3. High precision model of precession and nutation of the asteroids (1) Ceres, (4) Vesta, (433) Eros, (2867) Steins, and (25143) Itokawa. A.. Petit. J.. Souchay. C.. Lhotka. Astronomy & Astrophysics. 565. A79. 2014. 3. 10.1051/0004-6361/201322905. 2014A&A...565A..79P .
  4. Mean radius, mass, and inertia for reference Earth models. F.. Chambat. B.. Valette. Physics of the Earth and Planetary Interiors. 124. 3–4. 2001. 4. 10.1016/S0031-9201(01)00200-X. 2001PEPI..124..237C .
  5. Book: Ridpath, I.. Davida. https://books.google.com/books?id=O31j9UJ3U4oC&q=115. A Dictionary of Astronomy. Oxford University Press. 2012. 115. 978-0-19-960905-5 .
  6. Book: Bello . Ignacio . Britton . Jack Rolf . 1993 . Topics in Contemporary Mathematics . 5th . 512 . Lexington, Mass . D.C. Heath . 9780669289572.
  7. Book: West . P. W. . 2004 . Tree and Forest Measurement . Stem diameter . 13ff . New York . Springer . 9783540403906 .