Data Exploration on Exoplanets

Let's discovery Exoplanets together!

Thanks to the data provided by the NASA Exoplanet Archive, we are going to discover information about exoplanets in a dynamical way.


What is considered a planet?

This is a very controversial question but according to the International Astronomical Union, a planet is a celestial body that complies with the 3 following conditions:
  • it must orbit a star,
  • that has enough gravity to force this celestial body into a spherical shape,
  • it must have enough mass that its gravity cleared away any other objects of a similar size near its orbit.
Researchers have found hundreds of extrasolar planets, or "exoplanets", that reside outside of the solar system. There may be billions of exoplanets in the Milky Way galaxy alone, and some may have conditions favorable to life...

Learn more


Stats on our sample*

Total number of exoplanets
Average stellar age (Gyr)
Attribution of exoplanets detections

In Kepler Scope

Not in Kepler Scope

Space

Ground

*Sample dated as of June 10th, 2019

Information related to the discovery of the exoplanet


Discovery location

Discovery facility

Detection Method

Detections Per Year

Cumulative Detections Per Year


Features of the exoplanets


Orbital Period (days)

The Orbital Period is the time (in days) a given exoplanet takes to complete one orbit around its hosting stellar.

Number (known) of planets in planetary system

Distance to the planetary system (parsecs)

The Parsecs(pc) (symbol: pc) is a unit of length used in astronomy. It is about 3.26 light-years, which is equal to just under 31 trillion (3.1×1013) kilometers or just over 19 trillion (1.9×1013) miles.

Stellar age (in Giga Years)


Correlations


Correlation: mass vs. radius of the planet

Correlation: planet mass vs. stellar mass

Correlation: planet radius vs. stellar radius


Information about the selected planets