Exoplanets

Atmospheric Science · Part 10

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Table of Contents

  1. 1.Transit (Transmission) Spectroscopy
  2. 2.Secondary Eclipse & Phase Curves
  3. 3.Hot Jupiters: Tidally Locked Worlds
  4. 4.Super-Earths & Mini-Neptunes
  5. 5.Habitable Zone: Inner & Outer Edges
  6. 6.Biosignatures & False Positives
  7. 7.JWST Capabilities & TRAPPIST-1
  8. 8.Atmospheric Escape & the Radius Valley
  9. 9.1D Atmospheric Models & Opacity Sources
  10. 10.Fortran: 1D Radiative Equilibrium for Irradiated Planet

Key Equations

$$R_{\text{eff}}(\lambda) = R_p + nH\ln\left(\frac{\sigma(\lambda) P_0}{mg}\sqrt{\frac{2\pi R_p}{H}}\right)$$
$$\frac{F_p(\lambda)}{F_\star(\lambda)} = \left(\frac{R_p}{R_\star}\right)^2 \frac{B_\lambda(T_{\text{day}})}{B_\lambda(T_\star)}$$
$$T_{\text{sub}} = T_\star\sqrt{\frac{R_\star}{a}} \left(\frac{1-A_B}{f}\right)^{1/4}$$
$$S_{\text{eff}} = S_{\text{eff},\odot} + aT_\star + bT_\star^2 + cT_\star^3 + dT_\star^4$$

Equations are rendered with MathJax in the PDF with professional LaTeX typesetting.

Course Context

This PDF is part of the Atmospheric Science course on CoursesHub.World. Study the physics of weather and climate from atmospheric thermodynamics to planetary atmospheres. Covers atmospheric dynamics, synoptic meteorology, clouds and precipitation, radiation budgets, clima...

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