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.

JUICE: Preparing for a Double Flyby

JUICE: Preparing for a Double Flyby

After almost one and a half years of traveling through space, ESA’s space probe JUICE is due to pay a visit home at the beginning of next week: In order to adjust its speed and course on its way to Jupiter, the space probe will first fly close to the Moon and then to Earth on Monday and Tuesday, August 19 and 20, 2024. This is the first time that a space probe has attempted a maneuver of this kind. The scientific and technical teams at the MPS have been preparing for this event for months.

 

Tiny Meteorites Create Lunar Atmosphere

Tiny Meteorites Create Lunar Atmosphere

The extremely thin atmosphere that surrounds the moon is primarily created by the constant bombardment of the lunar surface by dust-sized mini-meteorites. Other processes, such as the interaction with particles and radiation from the Sun, play a subordinate role, as researchers from the University of Chicago, the Massachusetts Institute of Technology, the MPS and the NASA Goddard Space Flight Center report in the journal Science Advances.

 

Key to Rapid Planet Formation

Key to Rapid Planet Formation

Ring-shaped perturbations in disks of gas and dust orbiting young stars can trigger the formation of several gas giants, as researchers from the ORIGINS Cluster of Excellence, Ludwig-Maximilians-Universität in Munich and the MPS report in the current issue of Astronomy and Astrophysics. The team has developed a model that for the first time combines all the necessary physical processes that play a role in planet formation. According to this model, giant planets can form more efficiently and faster than previously assumed.

 

Otto Haxel Award for Yuto Bekki

Otto Haxel Award for Yuto Bekki

Dr. Yuto Bekki has been honored with the Otto Haxel Award for Physics for his doctoral dissertation. In collaboration with the German Physical Society, the Society for the Promotion of the Karlsruhe Institute of Technology (KIT) annually bestows this award upon the three best dissertations in physics from the Universities of Göttingen, Heidelberg, and KIT. During his doctorate, Yuto Bekki studied the Sun’s long-period oscillations, which had recently been discovered by researchers at the MPS.
 

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 Department
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: Cross-scale characteristics of decayless waves in the solar corona. (Arpit Kumar Shrivastav)

Aug 26, 2024 11:00 AM - 12:00 PM (Local Time Germany)
MPS, Room: Lecture Hall

IMPRS Defense: Structuring of the quiet solar corona (Nikolina Milanovic)

Aug 30, 2024 01:15 PM - 02:45 PM (Local Time Germany)
TU Braunschweig, Physikzentrum, Mendelssohnstraße 3, MS 3.3, Room: MS 3.3

IMPRS Defense: Solar spectropolarimetry in orbit: from raw data to physical parameters (Kinga Albert)

Aug 30, 2024 03:30 PM - 05:00 PM (Local Time Germany)
TU Braunschweig, Physikzentrum, Mendelssohnstraße 3, MS 3.3, Room: MS 3.3

IMPRS Defense: Towards a new view of the photospheric magnetic field with the Polarimetric and Helioseismic Imager on Solar Orbiter (Jonas Sinjan)

Sep 5, 2024 10:00 AM - 11:30 AM (Local Time Germany)
Max-Plack-Institut für Sonnensystemforschung, Room: Aquila + Bootes

IMPRS Defense: Modeling spectral and total solar irradiance variability from any vantage point in the Solar System (Isabela de Oliveira)

Sep 25, 2024 02:00 PM - 03:30 PM (Local Time Germany)
Max-Plack-Institut für Sonnensystemforschung, Room: Auditorium

News

After almost one and a half years of traveling through space, ESA’s space probe JUICE is due to pay a visit home at the beginning of next week: In order to adjust its speed and course on its way to Jupiter, the space probe will first fly close to the ...

The extremely thin atmosphere that surrounds the moon is primarily created by the constant bombardment of the lunar surface by dust-sized mini-meteorites. Other processes, such as the interaction with particles and radiation from the Sun, play a ...

Ring-shaped perturbations in disks of gas and dust orbiting young stars can trigger the formation of several gas giants, as researchers from the ORIGINS Cluster of Excellence, Ludwig-Maximilians-Universität in Munich (Germany) and the Max Planck ...

Dr. Yuto Bekki of the Max Planck Institute for Solar System Research (MPS) has been honored with the Otto Haxel Award for Physics for his doctoral dissertation. In collaboration with the German Physical Society (DPG), the Society for the Promotion of ...

Please also have a look at the job offers at the web pages in German.

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