How do I calculate the transit depth?
Transit depth is calculated by squaring the ratio of the planetβs radius to the starβs radius (Rβ/Rβ)Β².
What does transit depth tell us about exoplanets?
Transit depth provides information on the size of an exoplanet relative to its host star, helping determine if it’s a gas giant or terrestrial planet.
Why is the area ratio squared in the transit depth formula?
Because the area blocked by a planet is proportional to the square of its radius when viewed from the star.
Can transit depth be used to detect exoplanets?
Yes, significant dimming during transit indicates an exoplanet passing in front of its host star.
How accurate does the measurement need to be for transit depth calculations?
High precision is required, typically measured in parts per thousand (ppt) or parts per million (ppm), depending on the star’s brightness and the planet’s size.
What other factors can affect the observed transit depth?
Atmospheric effects, stellar spots, and orbital inclination can all influence the observed transit depth.
Is there a limit to how small an exoplanet can be detected using transit depth?
Yes, smaller planets require longer observation times and more precise measurements to detect their transits reliably.