231 citations · 521 across the 7 of their papers we have counts for
7 papers
FastChem 2: An improved computer program to determine the gas-phase chemical equilibrium composition for arbitrary element distributions
Joachim W. Stock, Daniel Kitzmann, A. Beate C. Patzer
The computation of complex neutral/ionised chemical equilibrium compositions is invaluable to obtain scientific insights of, for example, the atmospheres of extrasolar planets and…
Presolar Stardust in Highly Pristine CM Chondrites Asuka 12169 and Asuka 12236
Larry R. Nittler, Conel M. O'D. Alexander, Andrea Patzer +1
We report a NanoSIMS search for presolar grains in the CM chondrites Asuka (A) 12169 and A12236. We found 90 presolar O-rich grains and 25 SiC grains in A12169, giving matrix-norma…
A spectral survey of an ultra-hot Jupiter: Detection of metals in the transmission spectrum of KELT-9 b
H. J. Hoeijmakers, D. Ehrenreich, D. Kitzmann +16
Context: KELT-9 b exemplifies a newly emerging class of short-period gaseous exoplanets that tend to orbit hot, early type stars - termed ultra-hot Jupiters. The severe stellar irr…
Assessing the habitability of planets with Earth-like atmospheres with 1D and 3D climate modeling
M. Godolt, J. L. Grenfell, D. Kitzmann +5
The habitable zone (HZ) describes the range of orbital distances around a star where the existence of liquid water on the surface of an Earth-like planet is in principle possible.…
The unstable CO2 feedback cycle on ocean planets
D. Kitzmann, Y. Alibert, M. Godolt +6
Ocean planets are volatile rich planets, not present in our Solar System, which are thought to be dominated by deep, global oceans. This results in the formation of high-pressure w…
3D climate modeling of Earth-like extrasolar planets orbiting different types of host stars
M. Godolt, J. L. Grenfell, A. Hamann-Reinus +7
The potential habitability of a terrestrial planet is usually defined by the possible existence of liquid water on its surface. The potential presence of liquid water depends on ma…