Numerical simulations of lava planets interior dynamics with no rotation. The dimensionless temperature scale is the maximum super-adiabatic temperature contrast: temperature is 1 at the base of the magma ocean,
Numerical simulations of lava planets interior dynamics with no rotation. The dimensionless temperature scale is the maximum super-adiabatic temperature contrast: temperature is 1 at the base of the magma ocean,
External components on the TISR return vehicle. — NASA NTRS Titan is unique in the outer solar system in that it is the only moon with a thick atmosphere, and
The magnification excess maps for planet-satellite configurations with log q = −1.5 and | log s| = 0.3. The color coding indicates fractional magnification differences between the 2L1S and 1L1S
Graphical Abstract — Earth, Planets and Space via X-mol The formation and alteration of organic molecules within the Solar System and beyond is closely related to the life cycle of
Normalised to peak flux spectra of our sample of millimetre-compact disks. The red line indicates the estimated continuum. The indicated types and their meaning are discussed in Section 5.1. In
Schematic overview of CO2 ice segregation in protostellar envelopes. The temperature and density zones are separated by the gray dashed lines and each grain represents a different stage of ice
Liquid brine veins, where RNA molecules can replicate, surround solid ice crystals in water ice, as seen with an electron microscope. Credit Philipp Holliger, MRC LMB Chemists at UCL and
Astrobiology and Space Biology On Another World – Grok via Astrobiology.com Executive Summary: Distinct lines of scientific inquiry drives the separation of NASA’s fundamental life science research into Space Biology
Four team members are managing the instrument control laptop. — Earth and Space Science Planetary caves are desirable environments for the search for biosignatures corresponding to extant or extinct extraterrestrial
Plot of the various HZ limits (solid red and blue lines) and the evolution of instellation and effective temperature at the orbiting distance of each of the outer planets from