In the animation below, I don't understand why the brightness slightly decreases when the planet is behind the star.

transit method

Where does this effect come from?


Just before the planet goes behind the star, we see the light directly from the star as well as the light reflected from the planet's surface. When the planet is behind the star, we no longer see the reflected light.

Note that the top of the line also curves to reflect how much of the planet's surface is illuminated from the star. The most illumination is when it is almost "full" just before it passes behind the star. The least illumination is when it is "new" just before it passes in front of the star.

Edit (to address Fraxinus's comment below): Here is an example from Zhang et. al: Phase Curves of WASP-33b and HD 149026b and a New Correlation between Phase Curve Offset and Irradiation Temperature.

enter image description here

The above graphic shows processed data from the Spitzer space telescope. From the paper:

Observations were timed to begin before a secondary eclipse and end after the following secondary eclipse,

These light curves help aid in estimates of planetary albedo, day/night temperature, and atmospheric composition.

  • 3
    $\begingroup$ Is the second "dip" really visible for any real star? $\endgroup$ – fraxinus Feb 11 at 10:45
  • 1
    $\begingroup$ @fraxinus Yes, I added an example above. $\endgroup$ – Connor Garcia Feb 11 at 14:58
  • 7
    $\begingroup$ I'm constantly amazed at the precision that we achieve for measurements of distant stars. Intuitively I'd expect this difference to be lost in the noise. $\endgroup$ – Barmar Feb 11 at 15:43
  • 4
    $\begingroup$ @Barmar I definitely cherry-picked an example to show this effect. Wasp-33b is a super-hot Jovian giant with an orbital period of only 1.22 days, so it absorbs and emits tremendous amounts of energy. Most exoplanets' secondary eclipse light signatures would be lost in the stellar noise variations. I don't think aliens from another star system would be able to detect Jupiter's pass behind our Sun! $\endgroup$ – Connor Garcia Feb 11 at 16:03

Your Answer

By clicking “Post Your Answer”, you agree to our terms of service, privacy policy and cookie policy

Not the answer you're looking for? Browse other questions tagged or ask your own question.