I've just seen this Forbes article.
Why do gas giants appear to have clearly delineated surfaces, whereas the Earth's atmosphere fades into space?
Is it just a matter of scale? Or is there some form of "surface-tension" for the hydrogen gas?
I've just seen this Forbes article.
Why do gas giants appear to have clearly delineated surfaces, whereas the Earth's atmosphere fades into space?
Is it just a matter of scale? Or is there some form of "surface-tension" for the hydrogen gas?
In an isothermal atmosphere, the exponential scale height of the atmosphere is $$ h \sim \frac{k_\mathrm B T}{\mu g},$$ where $g$ is the gravitational field, $\mu$ is the mean mass of a particle and $T$ is the temperature (in kelvin).
i.e. The pressure/density of the atmosphere falls exponentially, with an e-folding height given by the above expression.
I suppose what matters when you look at a photo, is how this height compares with the radius of the planet. $$ \frac{h}{R} \sim \frac{k_\mathrm B T}{\mu g R}$$
Jupiter is half the temperature, 11 times the radius and with 3 times the gravity of Earth. However $\mu$ is about ten times smaller (hydrogen vs nitrogen/oxygen). Overall that means $h/R$ for Jupiter is of order 5–10 times smaller than for Earth and so it will appear "sharper".
EDIT: If you put some reasonable numbers in for Jupiter ($T \sim 130$ K, $\mu=2$, $R=7\times 10^7$ m), then $h/R \sim 3 \times 10^{-4}$. This means even if Jupiter fills a photo that is 3000 pixels across, the atmosphere will be about 1 pixel high.