Sea level – the geographical reference point and indicator of climate change – is a surprisingly variable parameter.
Austria settled on the level in Trieste in 1875, which is 34 centimetres lower.
The Max Planck Society leads internationally, securing 12 ERC Synergy Grants with a 39% success rate, involving 15 researchers out of 57 funded projects.
Gravitational Physics) with Zvi Bern (University of California), Enrico Barausse (SISSA Trieste
The Max Planck Society leads internationally, securing 12 ERC Synergy Grants with a 39% success rate, involving 15 researchers out of 57 funded projects.
Gravitational Physics) with Zvi Bern (University of California), Enrico Barausse (SISSA Trieste
The Max Planck Society leads internationally, securing 12 ERC Synergy Grants with a 39% success rate, involving 15 researchers out of 57 funded projects.
Gravitational Physics) with Zvi Bern (University of California), Enrico Barausse (SISSA Trieste
Die Max-Planck-Gesellschaft sichert sich in der jüngsten Ausschreibung des Europäischen Forschungsrats (ERC) 12 Synergy Grants und führt damit das internationale Ranking der geförderten Institutionen an.
Gravitationsphysik, zusammen mit Zvi Bern, University of California, Enrico Barausse, SISSA Trieste
Die Max-Planck-Gesellschaft sichert sich in der jüngsten Ausschreibung des Europäischen Forschungsrats (ERC) 12 Synergy Grants und führt damit das internationale Ranking der geförderten Institutionen an.
Gravitationsphysik, zusammen mit Zvi Bern, University of California, Enrico Barausse, SISSA Trieste
Die Max-Planck-Gesellschaft sichert sich in der jüngsten Ausschreibung des Europäischen Forschungsrats (ERC) 12 Synergy Grants und führt damit das internationale Ranking der geförderten Institutionen an.
Gravitationsphysik, zusammen mit Zvi Bern, University of California, Enrico Barausse, SISSA Trieste
Diving robots explore the deep sea: a chronology
and Don Walsh reached the ocean floor of the Mariana Trench in the Bathyscaph ‚Trieste
Astronomers led by Maria Bergemann (Max-Planck-Institute for Astronomy) have performed chemical measurements on stars that could markedly change the way cosmologists measure the Hubble constant and determine the amount of so-called dark energy in our universe. Using improved models of how the presence of chemical elements affects a star’s spectrum, the researchers found that so-called supernovae Type Ia have different properties than previously thought. Based on assumption about their brightness, cosmologists have used those supernovae to measure the expansion history of the universe. In light of the new results, it is now likely those assumptions will need to be revised.
University), Mats Carlsson (University of Oslo), Gabriele Cescutti (INAF and IFPU, Trieste
