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The Leibniz Institute for Astrophysics Potsdam (AIP) is dedicated to astrophysical questions ranging from the exploration of our Sun to the evolution of the cosmos. It focuses on the study of stellar, solar and exoplanetary physics, extragalactic astrophysics and the development of research technologies in the fields of spectroscopy, robotic telescopes and E-science.
On 10 December 1999, the European Space Agency's X-ray satellite XMM-Newton began its journey to investigate X-ray sources in the universe. The Leibniz Institute for Astrophysics Potsdam (AIP) has been involved for three decades with software development and data analysis. To mark the anniversary, the AIP is publishing a video with contributions from AIP researchers on science using the satellite's X-ray data.
The STELLA observatory in Tenerife studied a star’s surface for 16 years. Unlike the cyclic spots on our sun, this star exhibited chaotic, non-periodic star spot behavior, revealing a fundamentally different dynamo mechanism. The groundbreaking study has now been published in Nature Communications.
Last November 4th a contract was signed to fund the conceptual study of a new telescope, the Wide Field Spectroscopic Telescope (WST), which could potentially become operational in Chile after 2040. The consortium leading the WST project will receive three million euros to fund a detailed conceptual study over the next three years, from 2025 to 2027.
In honour of Prof. Dr. Johann Wempe (1906 – 1980), the last director of the former Astrophysical Observatory of Potsdam (AOP), the AIP grants the Johann Wempe Award to outstanding scientists. Applications and nominations are accepted until 31st January 2025.
On 10 December 1999, the European Space Agency's X-ray satellite XMM-Newton began its journey to investigate X-ray sources in the universe. The Leibniz Institute for Astrophysics Potsdam (AIP) has been involved for three decades with software development and data analysis.
The STELLA observatory in Tenerife studied a star’s surface for 16 years. Unlike the cyclic spots on our sun, this star exhibited chaotic, non-periodic star spot behavior, revealing a fundamentally different dynamo mechanism. The groundbreaking study has now been published in Nature Communications.
The German MHD Days were initiated in Potsdam in 1997 as a forum for theoretical research problems in magnetohydrodynamics, predominantly in astrophysics and geophysics. Since many of the problems are of fundamental nature, links to liquid metal phenomena, turbulence, convection and rotation of fluids have been in the scope of the meeting since.