- #1
piareround
- 79
- 0
Recently I been reading about exoplanets on wikipedia when I came across a line that caught my idea:
So I started wondering exactly what did Wikipedia mean by "based on the intensity of light" and later on by "temperature measure by observing the variation in infrared radiation". I mean really how do astronomers and astrophysics find the temperatures of nearby exoplanets even though they are hundreds of parsecs away. Specifically, I really wanted to know the following two things:
1. Where kind I find more through information about theory and concepts behind the transit method of observing exoplanets? Specifically I was curious about the formulas/theory they used.
2. How does one estimate, say to the nearest hundred degrees, a exoplanet's effective temperature when the exoplanet's albedo is unknown?
It is possible to estimate the temperature of an exoplanet based on the intensity of the light it receives from its parent star. However, such estimates may be substantially in error because they depend on the planet's usually unknown albedo, and because factors such as the greenhouse effect may introduce unknown complications. A few planets have had their temperature measured by observing the variation in infrared radiation as the planet moves around in its orbit and is eclipsed by its parent star
So I started wondering exactly what did Wikipedia mean by "based on the intensity of light" and later on by "temperature measure by observing the variation in infrared radiation". I mean really how do astronomers and astrophysics find the temperatures of nearby exoplanets even though they are hundreds of parsecs away. Specifically, I really wanted to know the following two things:
1. Where kind I find more through information about theory and concepts behind the transit method of observing exoplanets? Specifically I was curious about the formulas/theory they used.
2. How does one estimate, say to the nearest hundred degrees, a exoplanet's effective temperature when the exoplanet's albedo is unknown?