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European Space Agency

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by Ruth Titz-Weider (DLR), November 2024

The European Space Agency (ESA) is an international organisation for exploring space and advancing Europe’s scientific and economical interests there. ESA was founded in 1975 and has 22 member countires. By combining finances and know-how of the different countries, it can realize programmes and projects that would be beyond the capabilities of the single countries.

Country flags of ESA members blowing on white masts in front of a blue sky.

Flags of ESA members (2019). Credit: Credit: ESA

Germany’s interests are represented by the German Space Agency as part of the DLR. ESA’s main seat is in Paris, but there are numerous complexes and centers around Europe. For example, Germany hosts the ESA mission control centre ESOC in Darmstadt and the European Astronaut Centre in Cologne.

ESA’s fields of activity are:

  • Earth observation: e.g. Copernicus, the European Earth observation program
  • Navigation: e.g. Galileo, an independent satellite navigation system for Europe
  • Satellite communication/communication systems: e.g. satellite TV, weather forecast, internet access for remote areas
  • Conducting Missions for exploring planets, moons and other celestial objects: e.G. Rosetta, landing a probe on a comet in 2014, and Mars Express, orbiting Mars since 2003.

Artist's impression of a satellite with two solar panels in front of Mars.

Mars Express. Credit: ESA – D. Ducros

Exoplanet exploration

Several of ESA’s missions are explicitly aimed at exploring extrasolar planets. At the moment and in the near future, those are CHEOPS (start: 2019 – end: 2026), PLATO (start: 2026) and ARIEL (start: 2028). Furthermore, the Gaia mission through its highly precise data on the positions and movements of stars, supplies ample indications for exoplanet existence.

Artist's impressions of four satellite telescopes in front of a stylized sarry sky and planet depictions. Texts (left to right): Cheops – First step characterisation of known Earth-to-Neptune size exoplanets; Webb – Detailed characterisation of exoplanet atmospheres through transit studies and direct imaging; Plato – Studying terrestrial planets in orbits up to the habitable zone of Sun-like stars, and characterising these stars; Ariel – Performing a chemical census of a large and diverse sample of exoplanets by analysing their atmospheres.

Current and near future missions on exoplanet research directly conducted by ESA (Cheops, Plato, Ariel) oor with significant ESA collaboration (Webb). Credit: ESA

The search for exoplanets specifically with space-based telescopes started with the CoRoT mission by the French space agency CNES in 2007. For that, CNES collaborated with ESA, In addition, Austria, Belgium, Germany, Spain and the Netherlands were also involved.

The future missions PLATO and ARIEL are scheduled to be carried to space by new launch vehicle Ariane 6, which had its first successfull flight in July 2024. With the European spaceport in Kourou in French Guiana, ESA posesses independent access to space for scientific and commercial missions.

Learn more about ESA and its numerous projects on their web page.

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Oben sieht man, wie das licht eines Sterns durch ein stilisiertes Prisma in seine Farben aufgebrochen wird. Daneben das ungestörte Sternenlichtspektrum in Diagrammform. Unten fällt das Sternenlicht erst durch die Atmosphäre eines Sterns, bevor es durch das Prisma aufgefächert wird. Einige Linien in dem Farbspektrum sind schwarz. Danabene das auf diese Art beeinflusste Sternenpektrum in Diagrammform, mit gut sichtbaren Absorptionslineien.

Observing exo-atmospheres

by | Nov 20, 2024 | All,All about exoplanets,Detection methods | 0 Comments

by Ludwig Scheibe (TU Berlin), November 2024 A planet’s atmosphere, that means the gas layer that envelopes it, provides us with valuable information about the...

Spectroscopy

by | May 8, 2024 | All,All about exoplanets,Detection methods | 0 Comments

The Spectrum of light and what it tells us by Ludwig Scheibe (TU Berlin), July 2024 One fundamental and essential tool in the study of exoplanets is the study of light...

Exoplanet systems

by | Feb 12, 2024 | All,All about exoplanets,Multiple planet systems | 0 Comments

by Ludwig Scheibe & Tanja Schumann (TU Berlin), September 2022Credit: nasa.govDefinition: The planets of our Solar System are ordered a certain way: closest to the...

Astrometry

by | Mar 10, 2023 | All,Astrometry,Detection methods | 0 Comments

How it works: Like the radial velocity method, this technique makes use of the fact that star and planet both orbit a shared center of mass. For systems that we look at...

Direct Imaging

by | Mar 10, 2023 | All,Detection methods,Direct Imaging | 0 Comments

by Ludwig Scheibe (TU Berlin), October 2024 Without a lot of prior knowledge, upon hearing "discovering planets around other stars" most people would probably think...

Gravitational lensing

by | Mar 10, 2023 | All,Detection methods,Gravitational lensing | 0 Comments

How it works: According to Einstein’s general theory of relativity, time and space are merged into one quantity called spacetime. Under this theory, massive objects...

Transit method

by | Mar 10, 2023 | All,Detection methods,Transit method | 0 Comments

by Ludwig Scheibe (TU Berlin), October 2024 Imaging an exoplanet directly is a difficult process that is only doable in a select few cases. Thus, we need indirect...

Radial velocity method

by | Mar 10, 2023 | All,Detection methods,Radial velocity | 0 Comments

by Ludwig Scheibe (TU Berlin), September 2024 Because the direct imaging of planets around other stars is only feasible in select cases, the question arises: How, then,...

Neptune-sized planets

by | Mar 9, 2023 | All,All about exoplanets,Exoplanet types,Neptune-sized | 0 Comments

by Ludwig Scheibe (TU Berlin), October 2024 On the grand size scale between massive gas giants and smaller super-Earths, we find a class of medium-sized planets: Worlds...