template<typename units >
units::realT	mx::astro::planetMass2Radius (typename units::realT mass)
	An ad-hoc planetary mass-to-radius relationship (old version) More...

Function Documentation

◆ planetMass2Radius()

template<typename units >

units::realT mx::astro::planetMass2Radius ( typename units::realT mass )

An ad-hoc planetary mass-to-radius relationship (old version)

The goal of this function is to provide a radius given an exoplanet mass, for lightly-irradiated exoplanets. By lightly-irradiated we mean (roughly) planet's at Mercury's separation or further, scaled for stellar luminosity. Here we make use of the transition from rocky to gas-dominated composition at \( 1.6 R_e \) identified by Rogers [22] (see also Marcy et al. (2014) [14]). Below this radius we assume Earth composition and so \( R \propto M^{1/3}\). Above this we scale with a power law matched to the mean radius and mass of Uranus and Neptune, which defines the radius between \( 1.6^3 M_\oplus \) and this Uranus-Neptune mean point. Above this point we use a polynomial fit (in log(M)) to points including the Uranus/Neptune mean, Saturn, Jupiter, and above Jupiter's mass the average points from the 4.5 Gyr 1 AU models from Fortney et al. (2007) [6]. Above 3591.1 \( M_\oplus \) ( \(\sim 11 M_{jup}\)) we scale as \( M^{-1/8} \) based on the curve shown in Fortney et al. (2011) [7].

\( \frac{R}{R_\oplus} = \begin{cases} \left(\frac{M}{M_\oplus}\right)^{1/3}, & M < 4.1 M_\oplus \\ 0.62\left(\frac{M}{M_\oplus}\right)^{0.67}, & 4.1 M_\oplus \le M < 15.84 M_\oplus \\ 14.0211 - 44.8414 \log_{10}\left(\frac{M}{M_\oplus}\right) + 53.6554 \log_{10}^2\left(\frac{M}{M_\oplus}\right) -25.3289\log_{10}^3\left(\frac{M}{M_\oplus}\right) + 5.4920\log_{10}^4\left(\frac{M}{M_\oplus}\right) - 0.4586 \log_{10}^5\left(\frac{M}{M_\oplus}\right), & 15.84 \le M < 3591.1 M_\oplus \\ 32.03 \left(\frac{M}{M_\oplus}\right)^{-1/8}, & 3591.1 M_\oplus \le M \end{cases} \)

The ad-hoc mass-to-radius relationship compared to known planets. Blue circles are the Solar system. Black circles indicate expoplanets with Teq below that of a blackbody at Mercury's separation (413 K).

This function makes use of the units type system (Unit Conversions) so it can be used with Earth masses, Jupiter masses, kg (SI units), etc.

Returns: the estimated radius of the planet.

Template Parameters

units is the units-type specifying the units of mass. See Unit Conversions.

Parameters

mass	The mass of the planet.

Definition at line 57 of file planets.hpp.