Max Planck Institute for Solar System Research

Max Planck Institute for Solar System Research

The research focus of the Max Planck Institute for Solar System Research is our cosmic neighborhood: the solar system with its planets and moons, comets and asteroids as well as the sun. The aim of the scientists is to describe the processes in the solar system in models and to simulate them on the computer. In addition, instruments are being developed and built to study these bodies from space. The Institute is involved in numerous space missions.

Season’s Greetings

Season’s Greetings

This year, the Sun put on quite a show. In both May and October, powerful eruptions led to strong solar storms. Auroras were visible even over Göttingen (and the MPS) and made the night sky glow in beautiful colors.
The year also offered further reasons to celebrate. Read more...

We would like to thank you very much for your
support and cooperation during this past year.
We wish you happy holidays and a healthy and
successful New Year 2025.
 

Old Moon with a Young Crust

Old Moon with a Young Crust

A few hundred million years after its formation, the Moon may have been the scene of such immense volcanic activity that its entire crust melted several times and was completely churned through. The new considerations presented in the journal Nature by an international team of researchers from the University of California Santa Cruz, the MPS and the Collège de France resolve previous contradictions and inconsistencies regarding the age of the Moon. According to the researchers, the Moon was formed between 4.43 and 4.51 billion years ago. Its crust, however, appears at least 80 million years younger.

 

First Solar Images from Sunrise III

First Solar Images from Sunrise III

The balloon-borne solar observatory Sunrise III captured images of the Sun with highest resolution in July of this year during its six-and-a-half-day stratospheric flight. The team has now published the first, carefully processed images. They show smallest structures on the Sun’s visible surface, only 50 kilometers in size. The Sunrise III data make it possible to follow processes on the solar surface and in its lower atmosphere at an unprecedented height resolution for several hours without interruption.

Superflares once per Century

Superflares once per Century

Stars similar to the Sun produce a gigantic outburst of radiation on average about once every hundred years per star. Such superflares release more energy than a trillion hydrogen bombs and make all previously recorded solar flares pale in comparison. This estimate is based on an inventory of 56450 sun-like stars, which an international team of researchers led by the MPS presents in the journal Science. It shows that previous studies have significantly underestimated the eruptive potential of these stars.

 

Research Departments

Sun and Heliosphere
The focus of this department is the solar interior, the solar atmosphere, the solar magnetic field, the heliosphere, and the interplanetary medium, as well as solar radiation and solar energetic particles. The balloon-mission Sunrise, a balloon-borne solar observatory, is managed by this department. The mission investigates our central star from a height of about 35 km. In addition to several other participations in space missions, the department significantly contributes to the ESA's Solar Orbiter.
Planetary Science
This department investigates the interior, the surfaces, atmospheres, ionospheres, and magnetospheres of planets and their moons, as well as comets and asteroids. The department currently contributes or has contributed to important space missions such as the ESA's missions JUICE to the Jovian system, BepiColombo to Mercury and Rosetta to comet Churyumov-Gerasimenko as well as NASA's missions InSight to Mars and Dawn to the asteroid belt.
Solar and Stellar Interiors
Helioseismology and asteroseismology are tools that use the oscillations of the Sun and stars to probe their interior structure and dynamics. This allows us to test and refine the theory of stellar structure and evolution, thereby bringing us closer to understanding solar and stellar magnetism. The department hosts the German Data Center for NASA's Solar Dynamics Observatory, and is preparing to host the data center of ESA's exoplanet hunting mission, PLATO.

At a Glance

International Office
On the pages of the International Office, new employees and guests will find information for their stay in Göttingen and at the institute.
IMPRS
PhD programme: International Max Planck Research School for Solar System Science at the University of Göttingen.
Staff at the MPS
Staff directory
Restaurant at the End of the Universe
Canteen at the MPS
Mon - Fri 9 - 13
This week's menu

News

Seminars

MPS Seminar: The Sun’s global magnetic field: Understanding the sources of the slow solar wind. (David Pontin)

Jan 14, 2025 11:00 AM - 12:00 PM (Local Time Germany)
MPS, Room: Lecture Hall

S3 Seminar: Tools talks

Jan 15, 2025 02:00 PM - 03:00 PM (Local Time Germany)
Max-Plack-Institut für Sonnensystemforschung, Room: Hörsaal

S3 Seminar: Tools talks

Jan 22, 2025 02:00 PM - 03:00 PM (Local Time Germany)
Max-Plack-Institut für Sonnensystemforschung, Room: Hörsaal

S3 Seminar: Tools talks

Jan 22, 2025 02:00 PM - 03:00 PM (Local Time Germany)
Max-Plack-Institut für Sonnensystemforschung, Room: Hörsaal

S3 Seminar: Angular momentum transport in radially heated Keplerian flow (Abhiroop Bhadra)

Feb 5, 2025 02:30 PM - 03:00 PM (Local Time Germany)
Max-Plack-Institut für Sonnensystemforschung, Room: Hörsaal

S3 Seminar: In situ Rb-Sr using fs-LA-MS/MS-MC-ICP-MS (Miles Lindner)

Feb 5, 2025 03:00 PM - 03:30 PM (Local Time Germany)
Max-Plack-Institut für Sonnensystemforschung, Room: Hörsaal

News

Old Moon with a Young Crust

December 18, 2024

A few hundred million years after its formation, the Moon may have been the scene of such immense volcanic activity that its entire crust melted several times and was completely churned through. At that time, the Moon orbited significantly closer to ...

The balloon-borne solar observatory Sunrise III captured images of the Sun with highest resolution in July of this year during its six-and-a-half-day stratospheric flight. The team has published the first, carefully processed images today. They show ...

Stars similar to the Sun produce a gigantic outburst of radiation on average about once every hundred years per star. Such superflares release more energy than a trillion hydrogen bombs and make all previously recorded solar flares pale in ...

During its flyby of Uranus 38 years ago, NASA's space probe Voyager 2 witnessed the ice giant’s magnetosphere in a truly exceptional state: an unusually strong solar wind likely dramatically compressed the planet's magnetic shield at the time. This ...

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