12 to 18 years old

Complete this investigation to discover how to analyse satellite data to uncover the size and orbital period of exoplanets and become a real exoplanet detective.

Question 1

Exoplanets are planets orbiting stars other than our Sun. We have discovered over 5000 exoplanets, but they are difficult to detect, as the signal received from them is small in comparison to the much larger signal coming from their bigger, brighter host stars.

How are exoplanets detected?

Choose one or multiple options.

The correct options are:
  • By spotting the exoplanets directly
  • By measuring variations in the host star movement
  • By measuring variations in the light that we receive from the star

Exoplanets are very far away from planet Earth, making it impossible for us to travel to them.

Satellites, such as Cheops study exoplanets by measuring the dip of stellar light caused by the planets’ transit of their host stars.

Question 2

One of the methods to detect exoplanets is transit photometry. The exoplanet is detected by measuring a dimming in the light coming from the star when the exoplanet passes in between the star and the telescope. This is called an exoplanet transit.

A light curve is the measurement of the light of the host star over a period of time. The size of the dip in a light curve of a star during an exoplanet transit is called transit depth.

What is the transit depth in the light curve representation in Figure 1?

Figure 1: Simulated light curve, including one transit

Choose one option.

The correct option is 8%.

Question 3

Let’s now analyse a real light curve from the KELT-3 star. The data were acquired by ESA’s Cheops satellite in January 2023.
Analyse the light curve. Measure the transit depth of the exoplanet KELT-3b and estimate its radius using the equation below.

\text{radius of the planet} \approx  \sqrt{\text{radius of the star}^2 × \frac{\text{transit depth}}{100\%}}

The radius of the star KELT-3 is 1.7 times the radius of the Sun.

What is the radius of the exoplanet KELT-3b?

Figure 2: KELT-3b data from Cheops with the transit light curve best fit model from allesfitter

Choose one option.

The correct answer is 0.16 times de radius of the Sun. 

Let’s go through the calculation in detail:

Data KELT-3b z Cheopsu s nejlepším modelem tranzitní světelné křivky z allesfitteru.

Figure 2a: KELT-3b data from Cheops with the transit light curve best fit model from allesfitter with transit depth estimation.

The radius of the star KELT-3 is known and provided:

\thickspace \thickspace \text{radius of the star} = 1.7 × \text{radius of the Sun}

Analýzou Cheopsových dat můžeme změřit hloubku tranzitu přibližně na hodnotu 0.9\% (Figure 2a).

Pomocí rovnice:

\thickspace \thickspace \text{radius of the planet} \approx \sqrt{\text{radius of the star}^2 × \frac{\text{transit depth}}{100\%}}

\thickspace \thickspace \text{radius of the planet} \approx \sqrt{{(1.7 × \text{radius of  the Sun} )}^2 × \frac{0.9\%}{100\%}}

\thickspace \thickspace \text{radius of the planet} \approx 0.16 × {\text{radius of  the Sun}}

You can also compare this value with Earth by converting to Earth radii units. 

\thickspace \thickspace \text{radius of the Sun} \approx  109 × \text{radius of the Earth}

\thickspace \thickspace \text{radius of the planet} \approx 0.16 ×  109 \approx  17.44 × \text{radius of the Earth}

Question 4

Figure 3 shows a simulated light curve representing measurements of the light from an exoplanet host star over a period of 1 week. During this time the simulated exoplanet transited three times. You can estimate the period of this fake exoplanet by measuring the distance between the dips in the light curve.

What is the orbital period of this exoplanet?

Figure 3: Simulated light curve, including multiple transits.

Choose one option.

The correct option is 2 days.

Question 5

You are now ready to interpret the measured light curve of K2-141. The data were acquired by ESA’s Cheops satellite in September 2023.

Analyse the light curve in Figure 4. Describe what information you can retrieve from this data set.

Figure 4: Light curve of the star K2-141, the blue circles represent data taken with Cheops, and the red line is the best fit model from allesfitter


Extra information: K2-141 star radius is 0.7 times the radius of the Sun.


Do you see anything unusual in the plot?

Explain your observations. 


Question 6

Exoplanets are very diverse, they can have different sizes, masses, and temperatures. We can group them into different types by relating their properties to the planets in our Solar System.



Analyse the characteristics of all the planets and exoplanets below. Connect each exoplanet’s type with its name.

  • Horký Jupiter
  • Mini-Neptune
  • Super-Earth
  • K2-141b
  • KELT-3b
  • TOI-560c


\footnotesize \text{radius} = 1 × \text{radius of the Earth}
\footnotesize \text{mass} = 1 × \text{mass of the Earth}
\footnotesize \text{temperature} = 15 \degree C


\footnotesize \text{radius} = 11.21 × \text{radius of the Earth}
\footnotesize \text{mass} = 317.8 × \text{mass of the Earth}
\footnotesize \text{temperature} = -110\degree C


\footnotesize \text{radius} = 3.88 × \text{radius of the Earth}
\footnotesize \text{mass} = 17.1 × \text{mass of the Earth}
\footnotesize \text{temperature} = -200\degree C


\footnotesize \text{radius} = 17.5 × \text{radius of the Earth}
\footnotesize \text{mass} = 617 × \text{mass of the Earth}
\footnotesize \text{temperature} = 1543 \degree C


\footnotesize \text{radius} = 2.4 × \text{radius of the Earth}
\footnotesize \text{mass} = 10 × \text{mass of the Earth}
\footnotesize \text{temperature} = 225 \degree C


\footnotesize \text{radius} = 1.5 × \text{radius of the Earth}
\footnotesize \text{mass} = 5 × \text{mass of the Earth}
\footnotesize \text{temperature} = 1830 \degree C

Temperature refers to average temperature on the surface of the planet.
Size of the planets and exoplanets not to scale. 

The correct solution is:

  • Hot Jupiter — KELT-3b 
  • Mini-Neptune — TOI-560c
  • Super-Earth — K2-141b

Question 7

As of today, Earth is the only location in the Universe that we know of with life. The oldest dated fossils on planet Earth are 3.7 billion years old. When life first formed in our planet conditions were very different. 

Do you think life could exist in any of the three exoplanets listed before? 



Explain why.



None of these three exoplanets have habitability conditions. They all orbit very close to their host star, they are exposed to high doses of radiation and very high temperatures making it impossible for life to develop.

To learn more about habitability conditions watch our expert Laetitia Delrez analysing KELT-3b conditions.


Průběh vyšetřování


Certificate Hack an Exoplanet 2024

Continue your investigation work by analysing in detail the Cheops data from KELT-3b, TOI-560c or K2-141 planetary system.