Hosted by SolarSystem.video · EN · 20 episodes
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Rocky Worlds Discussions bring together planetary scientists, astronomers, and earth scientists to foster interactions across the communities and build the collaborations that will pave the way for the next decade of rocky exoplanet discovery and characterisation. Creating a globally connected community, Rocky Worlds Discussions aim to achieve continuous exchange and face-to-face discussions on a monthly basis. The setup for each meeting consists of a talk by a speaker highlighting challenging and creative questions surrounding the nature of rocky worlds plus extended plenary discussion. The essential goal of the meetings is to stimulate a lively debate on major interdisciplinary questions across the communities of exoplanet astronomy, planetary science, and astrobiology. All meetings are conducted virtually via Zoom. Generously supported by: The Royal Astronomical Society - https://ras.ac.uk The Meteoritical Society - https://meteoritical.org
SolarSystem.video hosts Rocky Worlds Discussions, a technology show with 20 episodes published.
Eleonora Alei (NASA Goddard Space Flight Center) One of the primary goals of the astronomical community in the next few decades is to characterize temperate terrestrial exoplanets to search for life. To address this chal
Shang-Min (Shami) Tsai (ASIAA) Sub-Neptune exoplanets are the most common class of planets detected to date. They occupy the transitional regime between rocky planets and gas giants, yet degeneracies in their internal st
Ana-Catalina Plesa (DLR) Understanding the interior of rocky planets such as Mercury, the Moon, Mars, and Venus helps us to put the Earth in a global planetary context. The surfaces of terrestrial planets that we observe
Miki Nakajima (University of Rochester) Planets experience numerous large impacts at the end of the planetary accretion stage. Such large impacts can produce deep magma oceans (MOs) within planets. During magma ocean cry
Lisa Dang (Université de Montréal) Lava planets are ultra-short-period planets with bulk densities consistent with terrestrial composition, but dayside temperatures hot enough to melt—and vaporize—rock. Of these planets,
Moa Persson (Swedish Institute of Space Physics) Venus has no magnetic shield, yet its atmosphere remains astonishingly thick. How does a planet withstand the solar wind without a protective magnetosphere? The answer lie
Day 1 of the fourth edition of the biennial Rocky Worlds conference The planets that are best understood are the four terrestrial planets of our own solar system. Applying the detailed understanding gleaned from these bo
Annelies Mortier (University of Birmingham) In just 30 years, we went from no known exoplanets to more than 6000 known exoplanets. This growing sample of exoplanetary systems allows us to study their mass-radius relation
Diogo Lourenco (ETH Zurich) Venus’ mass and radius are similar to those of Earth, yet its internal structure, chemical composition, and overral evolution and dynamics remain poorly constrained. A striking difference is V
Remo Burn (MPIA) Owing to observational advances, exoplanets are no longer treated as simple point masses in planet formation theory - their masses, radii, and thus densities are now measurable. Combined with atmospheric
Kazumasa Ohno (NAOJ) GJ 1214b is the archetype low-density sub-Neptune orbiting around a M-dwarf. The bulk composition of GJ 1214b remained elusive, as its mass-radius relation can be explained either by a rocky core wit
Michael L. Wong & Anirudh Prabhu (Carnegie Earth & Planets Laboratory) Humanity is embarking on a potential golden age of astrobiology, with numerous current and future space missions being tasked with the explicit goal
Sebastiaan Krijt (University of Exeter) The properties of planetary systems depend sensitively on the physical and chemical structure of the protoplanetary discs in which they form. At the same time, the processes associ
Katherine de Kleer (Caltech) Tides are a key internal energy source for numerous Solar System moons as well as exoplanets, driving their chemical evolution, geological activity, and even habitability. At Jupiter’s moon I
Michael Way (NASA/GISS, Uppsala University) In recent years a great deal of work has appeared related to better quantifying Venus' evolutionary path from Magma Ocean to present day Hell House world. We will present the l
Joshua Krissansen-Totton (University of Washington) Early JWST observations of hot rocky exoplanets have revealed that many of these objects may be airless rocks. For example, JWST observations of TRAPPIST-1b [1] and c [
Jayne Birkby (University of Oxford) High resolution cross-correlation spectroscopy (HRCCS) has proven a powerful and highly versatile tool in the characterization of exoplanet atmospheres. Its sensitivity to the position
Renyu Hu (JPL Caltech) JWST enables the measurements of the thermal emission spectra of small exoplanets to characterize their atmospheres and surfaces. Such measurements open up a new way to test models of atmospheric e
Anna Mittelholz (ETH Zurich) Planetary missions to Mars have enabled us to study its magnetic field environment - an important component of Mars’ history that is intertwined with virtually any other aspect of planetary e
Day 3 of the fourth edition of the biennial Rocky Worlds conference The planets that are best understood are the four terrestrial planets of our own solar system. Applying the detailed understanding gleaned from these bo
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Rocky Worlds Discussions is hosted by SolarSystem.video. The show is categorised under technology and has published 20 episodes.
Rocky Worlds Discussions has published 20 episodes.
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